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Gravity, Astrophysics and Cosmology Daniel Grumiller * Institute for Theoretical Physics Vienna University of Technology Seminar Doktorandenkolleg Fundamental Interactions, April 2011 *supported by START prize

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Page 1: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity, Astrophysics and Cosmology

Daniel Grumiller∗

Institute for Theoretical PhysicsVienna University of Technology

Seminar Doktorandenkolleg Fundamental Interactions, April 2011

∗supported by START prize

Page 2: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Outline

IntroductionCosmologyAstrophysicsGravity

Black holesHow can we observe black holes?Why are black holes interesting for quantum gravity?Holography: An Introduction

3D gravityMotivationTopologically massive gravityResearch directions

D. Grumiller — Gravity 2/36

Page 3: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Outline

IntroductionCosmologyAstrophysicsGravity

Black holesHow can we observe black holes?Why are black holes interesting for quantum gravity?Holography: An Introduction

3D gravityMotivationTopologically massive gravityResearch directions

D. Grumiller — Gravity Introduction 3/36

Page 4: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

The Standard Models

D. Grumiller — Gravity Introduction 4/36

Page 5: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

D. Grumiller — Gravity Introduction 5/36

Page 6: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

I 370000 years: 3000K ≈ 0.3eV

I ...that means no ions any more!

I Universe became transparent

I Fluctuations: “echo” of Big Bang

I COBE (1989-1993), WMAP(since 2001), Planck (since 2009)

D. Grumiller — Gravity Introduction 5/36

Page 7: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

I 370000 years: 3000K ≈ 0.3eV

I ...that means no ions any more!

I Universe became transparent

I Fluctuations: “echo” of Big Bang

I COBE (1989-1993), WMAP(since 2001), Planck (since 2009)

D. Grumiller — Gravity Introduction 5/36

Page 8: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

I 370000 years: 3000K ≈ 0.3eV

I ...that means no ions any more!

I Universe became transparent

I Fluctuations: “echo” of Big Bang

I COBE (1989-1993), WMAP(since 2001), Planck (since 2009)

D. Grumiller — Gravity Introduction 5/36

Page 9: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

I 370000 years: 3000K ≈ 0.3eV

I ...that means no ions any more!

I Universe became transparent

I Fluctuations: “echo” of Big Bang

I COBE (1989-1993), WMAP(since 2001), Planck (since 2009)

D. Grumiller — Gravity Introduction 5/36

Page 10: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

I 370000 years: 3000K ≈ 0.3eV

I ...that means no ions any more!

I Universe became transparent

I Fluctuations: “echo” of Big Bang

I COBE (1989-1993), WMAP(since 2001), Planck (since 2009)

D. Grumiller — Gravity Introduction 5/36

Page 11: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Brief history of the UniverseCMB:

Above: COBE satellite (900km)Below: WMAP satellite at Lagrangepoint L2 (1.5 ∗ 106km)

D. Grumiller — Gravity Introduction 5/36

Page 12: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

D. Grumiller — Gravity Introduction 6/36

Page 13: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand (see talks

by Andre Hoang, Beatrix Hiesmayr,Claudia Wulz, Helmut Neufeld,Walter Grimus, Eberhard Widmann,Manfried Faber, Anton Rebhan,Helmut Leeb, Johann Marton,Johann Zmeskal) less than 5% of theUniverse!

I Dark Matter: many indications,many candidates

I Plausible candidate: LSP

I Might be discovered at LHC (seetalk by Robert Schofbeck)

I Less plausible, but logically possible:dark matter is gravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 14: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand (see talks

by Andre Hoang, Beatrix Hiesmayr,Claudia Wulz, Helmut Neufeld,Walter Grimus, Eberhard Widmann,Manfried Faber, Anton Rebhan,Helmut Leeb, Johann Marton,Johann Zmeskal) less than 5% of theUniverse!

I Dark Matter: many indications,many candidates

I Plausible candidate: LSP

I Might be discovered at LHC (seetalk by Robert Schofbeck)

I Less plausible, but logically possible:dark matter is gravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 15: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand (see talks

by Andre Hoang, Beatrix Hiesmayr,Claudia Wulz, Helmut Neufeld,Walter Grimus, Eberhard Widmann,Manfried Faber, Anton Rebhan,Helmut Leeb, Johann Marton,Johann Zmeskal) less than 5% of theUniverse!

I Dark Matter: many indications,many candidates

I Plausible candidate: LSP

I Might be discovered at LHC (seetalk by Robert Schofbeck)

I Less plausible, but logically possible:dark matter is gravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 16: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand (see talks

by Andre Hoang, Beatrix Hiesmayr,Claudia Wulz, Helmut Neufeld,Walter Grimus, Eberhard Widmann,Manfried Faber, Anton Rebhan,Helmut Leeb, Johann Marton,Johann Zmeskal) less than 5% of theUniverse!

I Dark Matter: many indications,many candidates

I Plausible candidate: LSP

I Might be discovered at LHC (seetalk by Robert Schofbeck)

I Less plausible, but logically possible:dark matter is gravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 17: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

I More than 70% “Dark Energy”

I Simplest correct explanation:cosmological constant

I BUT: why so small??? 10−123

I Logical possibility: acceleration isgravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 18: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

I More than 70% “Dark Energy”

I Simplest correct explanation:cosmological constant

I BUT: why so small??? 10−123

I Logical possibility: acceleration isgravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 19: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

I More than 70% “Dark Energy”

I Simplest correct explanation:cosmological constant

I BUT: why so small??? 10−123

I Logical possibility: acceleration isgravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 20: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

I More than 70% “Dark Energy”

I Simplest correct explanation:cosmological constant

I BUT: why so small??? 10−123

I Logical possibility: acceleration isgravitational effect

D. Grumiller — Gravity Introduction 6/36

Page 21: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is the Universe made of?

Building blocks of our Universe:I Progress: we understand less

than 5% of the Universe!

I More than 70% “Dark Energy”

I Simplest correct explanation:cosmological constant

I BUT: why so small??? 10−123

I Logical possibility: acceleration isgravitational effect

To address these issues we need tounderstand GRAVITY!

D. Grumiller — Gravity Introduction 6/36

Page 22: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 23: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 24: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 25: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 26: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 27: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: Early success...

Neptune:I 1821: Alexis Bouvard published tables of orbit of

Uranus

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1845: John Couch Adams and especially Urbain LeVerrier predict new planet and calculate its position

I 1846: Observational confirmation by Johann GottfriedGalle and Heinrich Louis d’Arrest

Discovery of Neptune was first success of theDark Matter concept!

D. Grumiller — Gravity Introduction 7/36

Page 28: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 29: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 30: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 31: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 32: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 33: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 34: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AstrophysicsDark Matter hypothesis: ...and early failure

Vulcan:I 1840: Francois Arago suggests problem of Mercury

orbit to Urbain Le Verrier

I Observations deviate from tables: gravitationalanomalies!

I Different explanations: change law of gravitation orpredict Dark Matter to account for anomalies

I 1859: Urbain Le Verrier predicts new planet andcalculates its position

I 1860: Observational ‘confirmation’ by Lescarbault

I 1915: Einstein explains perihelion shift of Mercurywith General Relativity

Non-discovery of Vulcan was first failure ofthe Dark Matter concept!

D. Grumiller — Gravity Introduction 8/36

Page 35: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:

I Fact 1: Vulcan scenario is unlikely for Dark Matter

I Reason 1: experimental data!

I Reason 2: modified gravity usually does not work

I Fact 2: Nevertheless crucial to understand gravity well in the deep IR

I Reason 1: important for precision experiments

I Reason 2: relevant to test theories

I Fact 3: Even more challenging is to understand gravity in the deep UV

I Reason 1: experimentally difficult to access

I Reason 2: need quantum gravity theory

I Summary: we understand gravity above micro-meter scale and up tosolar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 36: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!

Not only galactic rotations curves (see pictures), but also: galaxyclusters, gravitational lensing, velocity dispersion of galaxies, CMBdata, structure formation, bullet cluster, sky surveys, Lyman α forest,indirect confirmations like type Ia supernovae and theoretical motivations like inflationary models, string theory, etc.

I Reason 2: modified gravity usually does not workI Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experimentsI Reason 2: relevant to test theoriesI Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to accessI Reason 2: need quantum gravity theoryI Summary: we understand gravity above micro-meter scale and up to

solar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 37: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!I Reason 2: modified gravity usually does not work

Constraints from solar system tests, astrophysical observations,Cosmology, Earth based precision experiments (see talk by HartmutAbele)

I Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experimentsI Reason 2: relevant to test theoriesI Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to accessI Reason 2: need quantum gravity theoryI Summary: we understand gravity above micro-meter scale and up to

solar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 38: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:

I Fact 1: Vulcan scenario is unlikely for Dark Matter

I Reason 1: experimental data!

I Reason 2: modified gravity usually does not work

I Fact 2: Nevertheless crucial to understand gravity well in the deep IR

I Reason 1: important for precision experiments

I Reason 2: relevant to test theories

I Fact 3: Even more challenging is to understand gravity in the deep UV

I Reason 1: experimentally difficult to access

I Reason 2: need quantum gravity theory

I Summary: we understand gravity above micro-meter scale and up tosolar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 39: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!I Reason 2: modified gravity usually does not workI Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experiments

Note: there are couple of tentative experimental anomalies in thedeep IR besides Dark Matter and Dark Energy: Pioneer anomaly,fly-by anomaly, increase of astronomical units, ...

I Reason 2: relevant to test theoriesI Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to accessI Reason 2: need quantum gravity theoryI Summary: we understand gravity above micro-meter scale and up to

solar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 40: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!I Reason 2: modified gravity usually does not workI Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experimentsI Reason 2: relevant to test theories

Some quantum theories of gravity predict modifications of GR in thedeep IR, others do not — deep IR physics might be a useful (andunexpected) experimental window for quantum gravity

I Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to accessI Reason 2: need quantum gravity theoryI Summary: we understand gravity above micro-meter scale and up to

solar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 41: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:

I Fact 1: Vulcan scenario is unlikely for Dark Matter

I Reason 1: experimental data!

I Reason 2: modified gravity usually does not work

I Fact 2: Nevertheless crucial to understand gravity well in the deep IR

I Reason 1: important for precision experiments

I Reason 2: relevant to test theories

I Fact 3: Even more challenging is to understand gravity in the deep UV

I Reason 1: experimentally difficult to access

I Reason 2: need quantum gravity theory

I Summary: we understand gravity above micro-meter scale and up tosolar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 42: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!I Reason 2: modified gravity usually does not workI Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experimentsI Reason 2: relevant to test theoriesI Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to access

EPlanck ∼ 1019GeV� 10TeV

See Manfred Krammers talk for state of the art of particle detectorsin high energy physics

I Reason 2: need quantum gravity theoryI Summary: we understand gravity above micro-meter scale and up to

solar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 43: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:I Fact 1: Vulcan scenario is unlikely for Dark MatterI Reason 1: experimental data!I Reason 2: modified gravity usually does not workI Fact 2: Nevertheless crucial to understand gravity well in the deep IRI Reason 1: important for precision experimentsI Reason 2: relevant to test theoriesI Fact 3: Even more challenging is to understand gravity in the deep UVI Reason 1: experimentally difficult to accessI Reason 2: need quantum gravity theory

See also talk by Harald Skarke on string theory (currently the onlyquantum theory of gravity consistent with all experiments)

I Summary: we understand gravity above micro-meter scale and up tosolar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 44: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is Dark Matter?Are we in a Neptune or a Vulcan scenario?

Some crucial facts about the Dark Side of life:

I Fact 1: Vulcan scenario is unlikely for Dark Matter

I Reason 1: experimental data!

I Reason 2: modified gravity usually does not work

I Fact 2: Nevertheless crucial to understand gravity well in the deep IR

I Reason 1: important for precision experiments

I Reason 2: relevant to test theories

I Fact 3: Even more challenging is to understand gravity in the deep UV

I Reason 1: experimentally difficult to access

I Reason 2: need quantum gravity theory

I Summary: we understand gravity above micro-meter scale and up tosolar system scale. GR migth be correct at arbitrarily big length scales,but it is a logical possibility that there are IR modifications of GR.

D. Grumiller — Gravity Introduction 9/36

Page 45: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Blackboard IModel for gravity at large distances

D. Grumiller — Gravity Introduction 10/36

Page 46: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physics

I We know that the deep UV must contain new physics!I Therefore, we need a UV completion of gravity (General Relativity)!I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 47: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physicsI We know that the deep UV must contain new physics!

I Therefore, we need a UV completion of gravity (General Relativity)!I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 48: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physicsI We know that the deep UV must contain new physics!

I Fact 1: QED has Landau poleI Fact 2: Standard Model cannot be valid at arbitrary high energiesI Indication 1: Singularities in GR are signal of new physicsI Indication 2: Dimensional analysis: expect new physics at Planck

energy 1019 GeV (or below)I Indication 3: General Relativity unlikely correct at Planck scale —

non-renormalizable = typical sign of low-energy effective theoriesI Indication 4: Unification of forces below Planck scale (around

1016 GeV) likely from experimental data

I Therefore, we need a UV completion of gravity (General Relativity)!I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 49: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physicsI We know that the deep UV must contain new physics!I Therefore, we need a UV completion of gravity (General Relativity)!

I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 50: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physicsI We know that the deep UV must contain new physics!I Therefore, we need a UV completion of gravity (General Relativity)!I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 51: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity in the deep UVaka quantum gravity

I We saw that the deep IR might contain new physicsI We know that the deep UV must contain new physics!I Therefore, we need a UV completion of gravity (General Relativity)!I Energy scale EQG where quantum gravity effects kick in:

1 TeV < EQG < a few 1019 GeV

The Holy Grail of Theoretical Physics

Construct UV completion of gravityaka Quantum Gravity

.

D. Grumiller — Gravity Introduction 11/36

Page 52: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity

Within the landscape of Physics:

Theoretical Physics

Fundamental interactions

Gravitational interactions

BLACK HOLES

I Primordial BHs

I Stellar&supermassive BHs

I Dual BHs

I BHs as “hydrogen atom”

I BHs as litmus test

I Condensed matter physics

I Fundamental interactions

D. Grumiller — Gravity Introduction 12/36

Page 53: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity

Within the landscape of Physics:

Theoretical Physics

Fundamental interactions

Gravitational interactions

BLACK HOLES

I Primordial BHs

I Stellar&supermassive BHs

I Dual BHs

I BHs as “hydrogen atom”

I BHs as litmus test

I Condensed matter physics

I Fundamental interactions

I Strong interactions

I Weak interactions

I Electromagnetic interactions

I Gravitational interactions

D. Grumiller — Gravity Introduction 12/36

Page 54: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity

Within the landscape of Physics:

Theoretical Physics

Fundamental interactions

Gravitational interactions

BLACK HOLES

I Primordial BHs

I Stellar&supermassive BHs

I Dual BHs

I BHs as “hydrogen atom”

I BHs as litmus test

I Condensed matter physics

I Fundamental interactions

I Strong interactions

I Weak interactions

I Electromagnetic interactions

I Gravitational interactions

I Cosmology

I Astrophysics

I Gauge/gravity correspondence

I Quantum gravity

I Model building

D. Grumiller — Gravity Introduction 12/36

Page 55: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Gravity

Within the landscape of Physics:

Theoretical Physics

Fundamental interactions

Gravitational interactions

BLACK HOLES

I Primordial BHs

I Stellar&supermassive BHs

I Dual BHs

I BHs as “hydrogen atom”

I BHs as litmus test

I Condensed matter physics

I Fundamental interactions

I Strong interactions

I Weak interactions

I Electromagnetic interactions

I Gravitational interactions

I Cosmology

I Astrophysics

I Gauge/gravity correspondence

I Quantum gravity

I Model building

D. Grumiller — Gravity Introduction 12/36

Page 56: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Outline

IntroductionCosmologyAstrophysicsGravity

Black holesHow can we observe black holes?Why are black holes interesting for quantum gravity?Holography: An Introduction

3D gravityMotivationTopologically massive gravityResearch directions

D. Grumiller — Gravity Black holes 13/36

Page 57: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is a black hole?

Fishy analogy (Bill Unruh ’81): The real stuff:

Above: black hole(NASA picture)Left: Waterfall

Analogy:Infinity↔ Lake

Horizon↔ Point of no return

Singularity↔ Waterfall

D. Grumiller — Gravity Black holes 14/36

Page 58: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

What is a black hole?Example: causal structure of Schwarzschild black hole

Schwarzschild line-element:

ds2 = −(

1− 2M

r

)dt2 +

dr2

1− 2Mr

+ r2 dθ2 + r2 sin2θ dφ2

D. Grumiller — Gravity Black holes 15/36

Page 59: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why Study Black Holes?

Depending whom you ask you’ll hear:I General Relativist: because they are unavoidableI Mathematician: because they are interestingI Science Fiction Writer: because they are coolI Astrophysicist: because they explain the dataI String Theoretician: because they hold the key to quantum gravityI Particle Physicist: because they might be produced at LHCI Cosmologist: because they existI Numerical Relativist: because they present challenge for coding skillsI Nuclear Physicist: because they are dual to a strongly coupled plasmaI Condensed Matter Physicist: because we can produce them in the labI Gravitational Wave Experimentalist: because we need to understand

black holes to provide templates for gravitational wave detection

Many reasons to study black holes in physics!

D. Grumiller — Gravity Black holes 16/36

Page 60: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Have to understand the physics of this...

D. Grumiller — Gravity Black holes 17/36

Page 61: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Black hole observationsConfirmed stellar black holes in X-ray binaries

Objects whose mass is clearly beyond TOV limit M > 3M�:

System Porb f(M) Donor Classification Mx†

[days] [M�] Spect. Type [M�]GRS 1915+105a 33.5 9.5 ± 3.0 K/M III LMXB/Transient 14 ± 4V404 Cyg 6.471 6.09 ± 0.04 K0 IV ,, 12 ± 2Cyg X-1 5.600 0.244 ± 0.005 09.7 Iab HMXB/Persistent 10 ± 3LMC X-1 4.229 0.14 ± 0.05 07 III ,, > 4XTE J1819-254 2.816 3.13 ± 0.13 B9 III IMXB/Transient 7.1 ± 0.3GRO J1655-40 2.620 2.73 ± 0.09 F3/5 IV ,, 6.3 ± 0.3

BW Cirb 2.545 5.74 ± 0.29 G5 IV LMXB/Transient > 7.8GX 339-4 1.754 5.8 ± 0.5 – ,,LMC X-3 1.704 2.3 ± 0.3 B3 V HMXB/Persistent 7.6 ± 1.3XTE J1550-564 1.542 6.86 ± 0.71 G8/K8 IV LMXB/Transient 9.6 ± 1.24U 1543-475 1.125 0.25 ± 0.01 A2 V IMXB/Transient 9.4 ± 1.0H1705-250 0.520 4.86 ± 0.13 K3/7 V LMXB/Transient 6 ± 2GS 1124-684 0.433 3.01 ± 0.15 K3/5 V ,, 7.0 ± 0.6XTE J1859+226c 0.382 7.4 ± 1.1 – ,,GS2000+250 0.345 5.01 ± 0.12 K3/7 V ,, 7.5 ± 0.3A0620-003 0.325 2.72 ± 0.06 K4 V ,, 11 ± 2XTE J1650-500 0.321 2.73 ± 0.56 K4 V ,,GRS 1009-45 0.283 3.17 ± 0.12 K7/M0 V ,, 5.2 ± 0.6GRO J0422+32 0.212 1.19 ± 0.02 M2 V ,, 4 ± 1XTE J1118+480 0.171 6.3 ± 0.2 K5/M0 V ,, 6.8 ± 0.4

Source: J. Casares, astro-ph/0612312

Black holes in X-ray binaries particularly “simple” to detect

D. Grumiller — Gravity Black holes 18/36

Page 62: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Recent milestones

I S. Dimopoulos and G.L. Landsberg; S.B. Giddings and S. Thomas (2001): Blackholes at the LHC?

I Saggitarius A∗ (2002): Supermassive black hole in center of Milky WayI R. Emparan and H. Reall (2002): Black rings in five dimensionsI S. Hawking (2004): concedes bet on information paradox — end of “black hole

wars”I P. Kovtun, D. Son and A. Starinets (2004): Viscosity in strongly interacting

Quantum Field Theories from black hole physicsI F. Pretorius (2005): Breakthrough in numerical treatment of binary problemI C. Barcelo, S. Liberati, and M. Visser (2005): “Analogue gravity”I J.E. McClintock et al. (2006): Measuring of spin of GRS1915+105 — nearly

extremal Kerr black hole!I E. Witten (2007), W. Li, W. Song and A. Strominger (2008) and D. Grumiller,

N. Johansson (2008): Quantum gravity in three dimensions?I S. Gubser; S. Hartnoll, C. Herzog and G. Horowitz (2008): “Holographic

superconductors”I D. Son; K. Balasubramanian and J. McGreevy (2008): Black hole duals for cold

atoms proposedI O. Lahav, A. Itah, A. Blumkin, C. Gordon, and J. Steinhauer (2009): Sonic black

hole in Bose-Einstein condensate

D. Grumiller — Gravity Black holes 19/36

Page 63: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why are black holes interesting for quantum gravity?Black holes as the hydrogen atom of quantum gravity

Some properties of black holes (BHs):I BHs are simple, much like elementary particlesI BHs are characterized by mass, spin and charges

I Classically BHs do not radiateI Semi-classically BHs emit Hawking radiationI Thermodynamically BHs have entropy proportional to horizon area:

SBH =1

4Ah

I Quantum-mechanically BH evaporation entails “information paradox”I BHs are the simplest systems that allow to address conceptual

problems of quantum gravity, for instance:unitarity of quantum gravity, microscopic understanding of BHentropy, holographic principle, modelling of BH evaporation, ...

Understanding quantum black holes and holographyis milestone on road to quantum gravity!

D. Grumiller — Gravity Black holes 20/36

Page 64: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why are black holes interesting for quantum gravity?Black holes as the hydrogen atom of quantum gravity

Some properties of black holes (BHs):I BHs are simple, much like elementary particlesI BHs are characterized by mass, spin and chargesI Classically BHs do not radiate

I Semi-classically BHs emit Hawking radiationI Thermodynamically BHs have entropy proportional to horizon area:

SBH =1

4Ah

I Quantum-mechanically BH evaporation entails “information paradox”I BHs are the simplest systems that allow to address conceptual

problems of quantum gravity, for instance:unitarity of quantum gravity, microscopic understanding of BHentropy, holographic principle, modelling of BH evaporation, ...

Understanding quantum black holes and holographyis milestone on road to quantum gravity!

D. Grumiller — Gravity Black holes 20/36

Page 65: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why are black holes interesting for quantum gravity?Black holes as the hydrogen atom of quantum gravity

Some properties of black holes (BHs):I BHs are simple, much like elementary particlesI BHs are characterized by mass, spin and chargesI Classically BHs do not radiateI Semi-classically BHs emit Hawking radiationI Thermodynamically BHs have entropy proportional to horizon area:

SBH =1

4Ah

I Quantum-mechanically BH evaporation entails “information paradox”I BHs are the simplest systems that allow to address conceptual

problems of quantum gravity, for instance:unitarity of quantum gravity, microscopic understanding of BHentropy, holographic principle, modelling of BH evaporation, ...

Understanding quantum black holes and holographyis milestone on road to quantum gravity!

D. Grumiller — Gravity Black holes 20/36

Page 66: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why are black holes interesting for quantum gravity?Black holes as the hydrogen atom of quantum gravity

Some properties of black holes (BHs):I BHs are simple, much like elementary particlesI BHs are characterized by mass, spin and chargesI Classically BHs do not radiateI Semi-classically BHs emit Hawking radiationI Thermodynamically BHs have entropy proportional to horizon area:

SBH =1

4Ah

I Quantum-mechanically BH evaporation entails “information paradox”I BHs are the simplest systems that allow to address conceptual

problems of quantum gravity, for instance:unitarity of quantum gravity, microscopic understanding of BHentropy, holographic principle, modelling of BH evaporation, ...

Understanding quantum black holes and holographyis milestone on road to quantum gravity!

D. Grumiller — Gravity Black holes 20/36

Page 67: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Holography — Main ideaaka gauge/gravity duality, aka AdS/CFT correspondence

One of the most fruitful ideas in contemporary theoretical physics:I The number of dimensions is a matter of perspective

I We can choose to describe the same physical situation using twodifferent formulations in two different dimensions

I The formulation in higher dimensions is a theory with gravityI The formulation in lower dimensions is a theory without gravity

D. Grumiller — Gravity Black holes 21/36

Page 68: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Holography — Main ideaaka gauge/gravity duality, aka AdS/CFT correspondence

One of the most fruitful ideas in contemporary theoretical physics:I The number of dimensions is a matter of perspectiveI We can choose to describe the same physical situation using two

different formulations in two different dimensions

I The formulation in higher dimensions is a theory with gravityI The formulation in lower dimensions is a theory without gravity

D. Grumiller — Gravity Black holes 21/36

Page 69: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Holography — Main ideaaka gauge/gravity duality, aka AdS/CFT correspondence

One of the most fruitful ideas in contemporary theoretical physics:I The number of dimensions is a matter of perspectiveI We can choose to describe the same physical situation using two

different formulations in two different dimensionsI The formulation in higher dimensions is a theory with gravityI The formulation in lower dimensions is a theory without gravity

D. Grumiller — Gravity Black holes 21/36

Page 70: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity?The holographic principle in black hole physics

Boltzmann/Planck: entropy of photon gas in d spatial dimensions

Sgauge ∝ volume ∝ Ld

Bekenstein/Hawking: entropy of black hole in d spatial dimensions

Sgravity ∝ area ∝ Ld−1

Daring idea by ’t Hooft/Susskind (1990ies):

Any consistent quantum theory of gravity could/should have a holo-graphic formulation in terms of a field theory in one dimension lower

Ground-breaking discovery by Maldacena (1997):

Holographic principle is realized in string theory in specific way

e.g. 〈Tµν〉gauge = TBYµν δ(gravity action) =

∫ddx√|h|TBYµν δhµν

D. Grumiller — Gravity Black holes 22/36

Page 71: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity?The holographic principle in black hole physics

Boltzmann/Planck: entropy of photon gas in d spatial dimensions

Sgauge ∝ volume ∝ Ld

Bekenstein/Hawking: entropy of black hole in d spatial dimensions

Sgravity ∝ area ∝ Ld−1

Daring idea by ’t Hooft/Susskind (1990ies):

Any consistent quantum theory of gravity could/should have a holo-graphic formulation in terms of a field theory in one dimension lower

Ground-breaking discovery by Maldacena (1997):

Holographic principle is realized in string theory in specific way

e.g. 〈Tµν〉gauge = TBYµν δ(gravity action) =

∫ddx√|h|TBYµν δhµν

D. Grumiller — Gravity Black holes 22/36

Page 72: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity?The holographic principle in black hole physics

Boltzmann/Planck: entropy of photon gas in d spatial dimensions

Sgauge ∝ volume ∝ Ld

Bekenstein/Hawking: entropy of black hole in d spatial dimensions

Sgravity ∝ area ∝ Ld−1

Daring idea by ’t Hooft/Susskind (1990ies):

Any consistent quantum theory of gravity could/should have a holo-graphic formulation in terms of a field theory in one dimension lower

Ground-breaking discovery by Maldacena (1997):

Holographic principle is realized in string theory in specific way

e.g. 〈Tµν〉gauge = TBYµν δ(gravity action) =

∫ddx√|h|TBYµν δhµν

D. Grumiller — Gravity Black holes 22/36

Page 73: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity?The holographic principle in black hole physics

Boltzmann/Planck: entropy of photon gas in d spatial dimensions

Sgauge ∝ volume ∝ Ld

Bekenstein/Hawking: entropy of black hole in d spatial dimensions

Sgravity ∝ area ∝ Ld−1

Daring idea by ’t Hooft/Susskind (1990ies):

Any consistent quantum theory of gravity could/should have a holo-graphic formulation in terms of a field theory in one dimension lower

Ground-breaking discovery by Maldacena (1997):

Holographic principle is realized in string theory in specific way

e.g. 〈Tµν〉gauge = TBYµν δ(gravity action) =

∫ddx√|h|TBYµν δhµν

D. Grumiller — Gravity Black holes 22/36

Page 74: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Blackboard IIBrown–York stress energy tensor and intro to holographic renormalization

D. Grumiller — Gravity Black holes 23/36

Page 75: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 76: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 77: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 78: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 79: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 80: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 81: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 82: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why should I care?...and why were there > 7000 papers on holography in the past 13 years?

I Many applications!

I Tool for calculations

I Strongly coupled gauge theories (difficult) mapped to semi-cassicalgravity (simple)

I Quantum gravity (difficult) mapped to weakly coupled gauge theories(simple)

I Examples of first type: heavy ion collisions at RHIC and LHC (seetalk by Toni Rebhan), superfluidity, type II superconductors (?), coldatoms (?), ...

I Examples of the second type: microscopic understanding of blackholes, information paradox, Kerr/CFT (?), 3D quantum gravity (?), ...

We can expect many new applications in the next decade!

D. Grumiller — Gravity Black holes 24/36

Page 83: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Outline

IntroductionCosmologyAstrophysicsGravity

Black holesHow can we observe black holes?Why are black holes interesting for quantum gravity?Holography: An Introduction

3D gravityMotivationTopologically massive gravityResearch directions

D. Grumiller — Gravity 3D gravity 25/36

Page 84: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

2D gravity: black holes!

Applications:I Solve conceptual problems of (quantum) gravity

I Approximate geometry of cosmic strings/particles confined in plane

I Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 85: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

3D gravity: black holes and gravitons!

Applications:I Solve conceptual problems of (quantum) gravity

I Approximate geometry of cosmic strings/particles confined in plane

I Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 86: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

3D gravity: black holes and gravitons!

Applications:I Solve conceptual problems of (quantum) gravity

Black hole evaporation, information loss problem, gravity as emergentphenomenon, ...

I Approximate geometry of cosmic strings/particles confined in planeI Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 87: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

3D gravity: black holes and gravitons!

Applications:I Solve conceptual problems of (quantum) gravity

I Approximate geometry of cosmic strings/particles confined in plane

I Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 88: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

3D gravity: black holes and gravitons!

Applications:I Solve conceptual problems of (quantum) gravity

I Approximate geometry of cosmic strings/particles confined in plane

I Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 89: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Why gravity in three dimensions?“As simple as possible, but not simpler”

Gravity simpler in lower dimensions

11D: 1144 Weyl, 66 Ricci, 5D: 35 Weyl, 15 Ricci, 4D: 10 Weyl, 10 Ricci3D: no Weyl, 6 Ricci, 2D: no Weyl, 1 Ricci

3D gravity: black holes and gravitons!

Applications:I Solve conceptual problems of (quantum) gravity

I Approximate geometry of cosmic strings/particles confined in plane

I Holographic tool for 2D condensed matter systems

pioneering work by Deser, Jackiw and Templeton in 1980ies2007 Witten rekindled interest in 3D gravity

D. Grumiller — Gravity 3D gravity 26/36

Page 90: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Cosmological topologically massive gravity (CTMG)

Action!

ICTMG =1

16πG

∫d3x√−g[R+

2

`2+

1

2µελµν Γρλσ

(∂µΓσνρ +

2

3ΓσµτΓτ νρ

)]Equations of motion:

Gµν +1

µCµν = 0

I Gravitons (topologically massive spin 2 excitations)

I Black holes (BTZ)

I Asymptotically anti-deSitter solutions (AdS/CFT!?)

I Higher derivative terms (third derivatives in EOM)

I Parity violating Chern–Simons term

I Related: new massive gravity (Bergshoeff, Hohm, Townsend 2009)

Properties of CTMG

D. Grumiller — Gravity 3D gravity 27/36

Page 91: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Cosmological topologically massive gravity (CTMG)

Action!

ICTMG =1

16πG

∫d3x√−g[R+

2

`2+

1

2µελµν Γρλσ

(∂µΓσνρ +

2

3ΓσµτΓτ νρ

)]Equations of motion:

Gµν +1

µCµν = 0

I Gravitons (topologically massive spin 2 excitations)

I Black holes (BTZ)

I Asymptotically anti-deSitter solutions (AdS/CFT!?)

I Higher derivative terms (third derivatives in EOM)

I Parity violating Chern–Simons term

I Related: new massive gravity (Bergshoeff, Hohm, Townsend 2009)

Properties of CTMG

D. Grumiller — Gravity 3D gravity 27/36

Page 92: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Linearized equations of motion

Linearization around AdS background

gµν = gµν + hµν

leads to linearized EOM that are third order PDE

G(1)µν +

1

µC(1)µν = (DRDLDMh)µν = 0 (1)

with three mutually commuting first order operators

(DL/R)µν = δνµ ± ` εµαν∇α , (DM )µ

ν = δνµ +1

µεµαν∇α

Three linearly independent solutions to (1):(DLhL

)µν

= 0 ,(DRhR

)µν

= 0 ,(DMhM

)µν

= 0

Li, Song and Strominger (2008):

At chiral point left (L) and massive (M) branches coincide!

With Sachs: recently found and classified all soutions to linearized EOM

D. Grumiller — Gravity 3D gravity 28/36

Page 93: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Linearized equations of motion

Linearization around AdS background

gµν = gµν + hµν

leads to linearized EOM that are third order PDE

G(1)µν +

1

µC(1)µν = (DRDLDMh)µν = 0 (1)

with three mutually commuting first order operators

(DL/R)µν = δνµ ± ` εµαν∇α , (DM )µ

ν = δνµ +1

µεµαν∇α

Three linearly independent solutions to (1):(DLhL

)µν

= 0 ,(DRhR

)µν

= 0 ,(DMhM

)µν

= 0

Li, Song and Strominger (2008):

At chiral point left (L) and massive (M) branches coincide!

With Sachs: recently found and classified all soutions to linearized EOM

D. Grumiller — Gravity 3D gravity 28/36

Page 94: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Linearized equations of motion

Linearization around AdS background

gµν = gµν + hµν

leads to linearized EOM that are third order PDE

G(1)µν +

1

µC(1)µν = (DRDLDMh)µν = 0 (1)

with three mutually commuting first order operators

(DL/R)µν = δνµ ± ` εµαν∇α , (DM )µ

ν = δνµ +1

µεµαν∇α

Three linearly independent solutions to (1):(DLhL

)µν

= 0 ,(DRhR

)µν

= 0 ,(DMhM

)µν

= 0

Li, Song and Strominger (2008):

At chiral point left (L) and massive (M) branches coincide!

With Sachs: recently found and classified all soutions to linearized EOM

D. Grumiller — Gravity 3D gravity 28/36

Page 95: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Linearized equations of motion

Linearization around AdS background

gµν = gµν + hµν

leads to linearized EOM that are third order PDE

G(1)µν +

1

µC(1)µν = (DRDLDMh)µν = 0 (1)

with three mutually commuting first order operators

(DL/R)µν = δνµ ± ` εµαν∇α , (DM )µ

ν = δνµ +1

µεµαν∇α

Three linearly independent solutions to (1):(DLhL

)µν

= 0 ,(DRhR

)µν

= 0 ,(DMhM

)µν

= 0

Li, Song and Strominger (2008):

At chiral point left (L) and massive (M) branches coincide!

With Sachs: recently found and classified all soutions to linearized EOMD. Grumiller — Gravity 3D gravity 28/36

Page 96: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AdS/CFT – but which CFT?Chiral versus logarithmic

Pre-cursor of AdS/CFT: Brown–Henneaux 1986

3D quantum gravity on AdS dual to 2D CFT with cL = cR = 3`/2GN

Constant time slice of EAdS3

I Boundary of AdS3: cylinder

I Dual CFT on cylinder

I Characterized by central charges

I cL = cR in Einstein gravity

I cL 6= cR in CTMG

I cL = (1− 1/µ`) 3`/2GNI Chiral point: µ` = 1

I At chiral point cL = 0

D. Grumiller — Gravity 3D gravity 29/36

Page 97: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AdS/CFT – but which CFT?Chiral versus logarithmic

Pre-cursor of AdS/CFT: Brown–Henneaux 1986

3D quantum gravity on AdS dual to 2D CFT with cL = cR = 3`/2GN

Constant time slice of EAdS3

I Boundary of AdS3: cylinder

I Dual CFT on cylinder

I Characterized by central charges

I cL = cR in Einstein gravity

I cL 6= cR in CTMG

I cL = (1− 1/µ`) 3`/2GNI Chiral point: µ` = 1

I At chiral point cL = 0

D. Grumiller — Gravity 3D gravity 29/36

Page 98: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AdS/CFT – but which CFT?Chiral versus logarithmic

Pre-cursor of AdS/CFT: Brown–Henneaux 1986

3D quantum gravity on AdS dual to 2D CFT with cL = cR = 3`/2GN

Constant time slice of EAdS3

I Boundary of AdS3: cylinder

I Dual CFT on cylinder

I Characterized by central charges

I cL = cR in Einstein gravity

I cL 6= cR in CTMG

I cL = (1− 1/µ`) 3`/2GNI Chiral point: µ` = 1

I At chiral point cL = 0

D. Grumiller — Gravity 3D gravity 29/36

Page 99: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

AdS/CFT – but which CFT?Chiral versus logarithmic

Pre-cursor of AdS/CFT: Brown–Henneaux 1986

3D quantum gravity on AdS dual to 2D CFT with cL = cR = 3`/2GN

Constant time slice of EAdS3

I Boundary of AdS3: cylinder

I Dual CFT on cylinder

I Characterized by central charges

I cL = cR in Einstein gravity

I cL 6= cR in CTMG

I cL = (1− 1/µ`) 3`/2GNI Chiral point: µ` = 1

I At chiral point cL = 0

D. Grumiller — Gravity 3D gravity 29/36

Page 100: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 101: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 102: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 103: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 104: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZR

I Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 105: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 106: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

A tempting conjecture

Observation:

At chiral point cL = 0

Chiral gravity conjecture (Li, Song, Strominger 2008):

CFT dual to CTMG exists and is chiral

Why would that be useful?

I Nice toy model for quantum gravity without strings

I Entropy of BTZ black hole: microstate counting

I Partition function factorizes holomorphically: Z = ZRZL = ZRI Partition function calculated already!

However...

D. Grumiller — Gravity 3D gravity 30/36

Page 107: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Another tempting conjecture

Observation (E: energy, J : angular momentum):

(E + J)

(logleft

)=

(2 1

20 2

)(logleft

),

(E − J)

(logleft

)=

(0 1

20 0

)(logleft

).

Such a Jordan form of E ± J is defining property of a logarithmic CFT!Logarithmic gravity conjecture (Grumiller, Johansson 2008):

CFT dual to CTMG exists and is logarithmic

I Logarithmic CFT: not unitary and not chiral!

I Either logarithmic or chiral CFT dual (or none)

I Until recently unknown which of these alternatives is realized!

D. Grumiller — Gravity 3D gravity 31/36

Page 108: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Another tempting conjecture

Observation (E: energy, J : angular momentum):

(E + J)

(logleft

)=

(2 1

20 2

)(logleft

),

(E − J)

(logleft

)=

(0 1

20 0

)(logleft

).

Such a Jordan form of E ± J is defining property of a logarithmic CFT!Logarithmic gravity conjecture (Grumiller, Johansson 2008):

CFT dual to CTMG exists and is logarithmic

I Logarithmic CFT: not unitary and not chiral!

I Either logarithmic or chiral CFT dual (or none)

I Until recently unknown which of these alternatives is realized!

D. Grumiller — Gravity 3D gravity 31/36

Page 109: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Another tempting conjecture

Observation (E: energy, J : angular momentum):

(E + J)

(logleft

)=

(2 1

20 2

)(logleft

),

(E − J)

(logleft

)=

(0 1

20 0

)(logleft

).

Such a Jordan form of E ± J is defining property of a logarithmic CFT!Logarithmic gravity conjecture (Grumiller, Johansson 2008):

CFT dual to CTMG exists and is logarithmic

I Logarithmic CFT: not unitary and not chiral!

I Either logarithmic or chiral CFT dual (or none)

I Until recently unknown which of these alternatives is realized!

D. Grumiller — Gravity 3D gravity 31/36

Page 110: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Another tempting conjecture

Observation (E: energy, J : angular momentum):

(E + J)

(logleft

)=

(2 1

20 2

)(logleft

),

(E − J)

(logleft

)=

(0 1

20 0

)(logleft

).

Such a Jordan form of E ± J is defining property of a logarithmic CFT!Logarithmic gravity conjecture (Grumiller, Johansson 2008):

CFT dual to CTMG exists and is logarithmic

I Logarithmic CFT: not unitary and not chiral!

I Either logarithmic or chiral CFT dual (or none)

I Until recently unknown which of these alternatives is realized!

D. Grumiller — Gravity 3D gravity 31/36

Page 111: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Another tempting conjecture

Observation (E: energy, J : angular momentum):

(E + J)

(logleft

)=

(2 1

20 2

)(logleft

),

(E − J)

(logleft

)=

(0 1

20 0

)(logleft

).

Such a Jordan form of E ± J is defining property of a logarithmic CFT!Logarithmic gravity conjecture (Grumiller, Johansson 2008):

CFT dual to CTMG exists and is logarithmic

I Logarithmic CFT: not unitary and not chiral!

I Either logarithmic or chiral CFT dual (or none)

I Until recently unknown which of these alternatives is realized!

D. Grumiller — Gravity 3D gravity 31/36

Page 112: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Consistency checks

I Performed various consistency checks with Niklas Johansson

I All of them pointed towards validity of logarithmic conjecture

I Recently: Skenderis, Taylor, van Rees calculated 2-point correlators

I Calculation of 2- and 3-point correlators with Ivo Sachs

Results:

〈right(z, z) right(0)〉 =cR2z4

(2)

〈left(z, z) log(0)〉 = − b

2z4(3)

〈log(z, z) log(0)〉 =2b ln (m2|z|2)

z4(4)

These are precisely the 2-point correlators of a logarithmic CFT!

3-point correlators also consistent with logarithmic CFT conjecture

D. Grumiller — Gravity 3D gravity 32/36

Page 113: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Consistency checks

I Performed various consistency checks with Niklas Johansson

I All of them pointed towards validity of logarithmic conjecture

I Recently: Skenderis, Taylor, van Rees calculated 2-point correlators

I Calculation of 2- and 3-point correlators with Ivo Sachs

Results:

〈right(z, z) right(0)〉 =cR2z4

(2)

〈left(z, z) log(0)〉 = − b

2z4(3)

〈log(z, z) log(0)〉 =2b ln (m2|z|2)

z4(4)

These are precisely the 2-point correlators of a logarithmic CFT!

3-point correlators also consistent with logarithmic CFT conjecture

D. Grumiller — Gravity 3D gravity 32/36

Page 114: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Consistency checks

I Performed various consistency checks with Niklas Johansson

I All of them pointed towards validity of logarithmic conjecture

I Recently: Skenderis, Taylor, van Rees calculated 2-point correlators

I Calculation of 2- and 3-point correlators with Ivo Sachs

Results:

〈right(z, z) right(0)〉 =cR2z4

(2)

〈left(z, z) log(0)〉 = − b

2z4(3)

〈log(z, z) log(0)〉 =2b ln (m2|z|2)

z4(4)

These are precisely the 2-point correlators of a logarithmic CFT!

3-point correlators also consistent with logarithmic CFT conjecture

D. Grumiller — Gravity 3D gravity 32/36

Page 115: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Consistency checks

I Performed various consistency checks with Niklas Johansson

I All of them pointed towards validity of logarithmic conjecture

I Recently: Skenderis, Taylor, van Rees calculated 2-point correlators

I Calculation of 2- and 3-point correlators with Ivo Sachs

Results:

〈right(z, z) right(0)〉 =cR2z4

(2)

〈left(z, z) log(0)〉 = − b

2z4(3)

〈log(z, z) log(0)〉 =2b ln (m2|z|2)

z4(4)

These are precisely the 2-point correlators of a logarithmic CFT!

3-point correlators also consistent with logarithmic CFT conjecture

D. Grumiller — Gravity 3D gravity 32/36

Page 116: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Consistency checks

I Performed various consistency checks with Niklas Johansson

I All of them pointed towards validity of logarithmic conjecture

I Recently: Skenderis, Taylor, van Rees calculated 2-point correlators

I Calculation of 2- and 3-point correlators with Ivo Sachs

Results:

〈right(z, z) right(0)〉 =cR2z4

(2)

〈left(z, z) log(0)〉 = − b

2z4(3)

〈log(z, z) log(0)〉 =2b ln (m2|z|2)

z4(4)

These are precisely the 2-point correlators of a logarithmic CFT!

3-point correlators also consistent with logarithmic CFT conjecture

D. Grumiller — Gravity 3D gravity 32/36

Page 117: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

3D gravity summary

I Cosmological topologically massive gravity at the chiral point is anintersting gravitational theory in three dimensions

I Its dual CFT was conjectured to be logarithmic in work with NiklasJohansson 2008

I Conjecture confirmed by calculations of correlators (Skenderis, Taylorand van Rees 2009, and Grumiller and Sachs 2009)

I CTMG probably not good toy model for quantum gravityNeeds unitary completion or truncationExciting possibility: gravity duals to strongly coupledlogarithmic CFTs in condensed matter physicsExamples: turbulence, critical polymers, percolation, disorderedsystems, sandpile model, quantum Hall effect, ...

It seems we have uncovered yet-another interesting chapter in the epicAdS/CFT saga...

D. Grumiller — Gravity 3D gravity 33/36

Page 118: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

3D gravity summary

I I II Cosmological topologically massive gravity at the chiral point is anintersting gravitational theory in three dimensions

I Its dual CFT was conjectured to be logarithmic in work with NiklasJohansson 2008

I Conjecture confirmed by calculations of correlators (Skenderis, Taylorand van Rees 2009, and Grumiller and Sachs 2009)

I CTMG probably not good toy model for quantum gravity

Needs unitary completion or truncationExciting possibility: gravity duals to strongly coupledlogarithmic CFTs in condensed matter physicsExamples: turbulence, critical polymers, percolation, disorderedsystems, sandpile model, quantum Hall effect, ...

It seems we have uncovered yet-another interesting chapter in the epicAdS/CFT saga...

D. Grumiller — Gravity 3D gravity 33/36

Page 119: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

3D gravity summary

I I II Cosmological topologically massive gravity at the chiral point is anintersting gravitational theory in three dimensions

I Its dual CFT was conjectured to be logarithmic in work with NiklasJohansson 2008

I Conjecture confirmed by calculations of correlators (Skenderis, Taylorand van Rees 2009, and Grumiller and Sachs 2009)

I CTMG probably not good toy model for quantum gravityNeeds unitary completion or truncation

Exciting possibility: gravity duals to strongly coupledlogarithmic CFTs in condensed matter physicsExamples: turbulence, critical polymers, percolation, disorderedsystems, sandpile model, quantum Hall effect, ...

It seems we have uncovered yet-another interesting chapter in the epicAdS/CFT saga...

D. Grumiller — Gravity 3D gravity 33/36

Page 120: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

3D gravity summary

I I II Cosmological topologically massive gravity at the chiral point is anintersting gravitational theory in three dimensions

I Its dual CFT was conjectured to be logarithmic in work with NiklasJohansson 2008

I Conjecture confirmed by calculations of correlators (Skenderis, Taylorand van Rees 2009, and Grumiller and Sachs 2009)

I CTMG probably not good toy model for quantum gravityNeeds unitary completion or truncationExciting possibility: gravity duals to strongly coupledlogarithmic CFTs in condensed matter physics

Examples: turbulence, critical polymers, percolation, disorderedsystems, sandpile model, quantum Hall effect, ...

It seems we have uncovered yet-another interesting chapter in the epicAdS/CFT saga...

D. Grumiller — Gravity 3D gravity 33/36

Page 121: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

3D gravity summary

I I II Cosmological topologically massive gravity at the chiral point is anintersting gravitational theory in three dimensions

I Its dual CFT was conjectured to be logarithmic in work with NiklasJohansson 2008

I Conjecture confirmed by calculations of correlators (Skenderis, Taylorand van Rees 2009, and Grumiller and Sachs 2009)

I CTMG probably not good toy model for quantum gravityNeeds unitary completion or truncationExciting possibility: gravity duals to strongly coupledlogarithmic CFTs in condensed matter physicsExamples: turbulence, critical polymers, percolation, disorderedsystems, sandpile model, quantum Hall effect, ...

It seems we have uncovered yet-another interesting chapter in the epicAdS/CFT saga...

D. Grumiller — Gravity 3D gravity 33/36

Page 122: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Current projects

Collaborations with local postdocs, PhD students and undergraduates:

I I II Warped AdS holography: with Niklas Johansson, Sabine Ertl andFrederic Brunner

I New anomalies in logarithmic CFT dual to generalized massivegravity: with Niklas Johansson and Thomas Zojer

I Exact solutions in 3D gravity: with Niklas Johansson and Sabine Ertl

Supplemented by collaborations withMIT (Olaf Hohm, Roman Jackiw),LMU Munich/AEI (Ivo Sachs),Chicago U. (Robert McNees),Perimeter Institute (Robert Mann),McGill U. (Alejandra Castro),Princeton U. (Nicolas Yunes),Michigan U. (Finn Larsen),YITP Stony Brook (Peter van Nieuwenhuizen),etc.

D. Grumiller — Gravity 3D gravity 34/36

Page 123: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Current projects

Collaborations with local postdocs, PhD students and undergraduates:

I Warped AdS holography: with Niklas Johansson, Sabine Ertl andFrederic Brunner

I New anomalies in logarithmic CFT dual to generalized massivegravity: with Niklas Johansson and Thomas Zojer

I Exact solutions in 3D gravity: with Niklas Johansson and Sabine Ertl

Supplemented by collaborations withMIT (Olaf Hohm, Roman Jackiw),LMU Munich/AEI (Ivo Sachs),Chicago U. (Robert McNees),Perimeter Institute (Robert Mann),McGill U. (Alejandra Castro),Princeton U. (Nicolas Yunes),Michigan U. (Finn Larsen),YITP Stony Brook (Peter van Nieuwenhuizen),etc.

D. Grumiller — Gravity 3D gravity 34/36

Page 124: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Current projects

Collaborations with local postdocs, PhD students and undergraduates:

I Warped AdS holography: with Niklas Johansson, Sabine Ertl andFrederic Brunner

I New anomalies in logarithmic CFT dual to generalized massivegravity: with Niklas Johansson and Thomas Zojer

I Exact solutions in 3D gravity: with Niklas Johansson and Sabine Ertl

Supplemented by collaborations withMIT (Olaf Hohm, Roman Jackiw),LMU Munich/AEI (Ivo Sachs),Chicago U. (Robert McNees),Perimeter Institute (Robert Mann),McGill U. (Alejandra Castro),Princeton U. (Nicolas Yunes),Michigan U. (Finn Larsen),YITP Stony Brook (Peter van Nieuwenhuizen),etc.

D. Grumiller — Gravity 3D gravity 34/36

Page 125: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Current projects

Collaborations with local postdocs, PhD students and undergraduates:

I Warped AdS holography: with Niklas Johansson, Sabine Ertl andFrederic Brunner

I New anomalies in logarithmic CFT dual to generalized massivegravity: with Niklas Johansson and Thomas Zojer

I Exact solutions in 3D gravity: with Niklas Johansson and Sabine Ertl

Supplemented by collaborations withMIT (Olaf Hohm, Roman Jackiw),LMU Munich/AEI (Ivo Sachs),Chicago U. (Robert McNees),Perimeter Institute (Robert Mann),McGill U. (Alejandra Castro),Princeton U. (Nicolas Yunes),Michigan U. (Finn Larsen),YITP Stony Brook (Peter van Nieuwenhuizen),etc.D. Grumiller — Gravity 3D gravity 34/36

Page 126: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 127: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 128: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 129: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 130: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 131: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 132: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 133: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 134: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Future directions

Directions implied by topics addressed in this talk:

I Holography in 2D?

I AdS3/(L)CFT2: better understanding of holography

I 3D quantum gravity?

I Condensed matter applications of AdS3/LCFT2?

Directions related to topics addressed in this talk:

I Numerical relativity (black hole collapse, numerical AdS/CFT)

I Black hole analogs in condensed matter systems

I Applications to astrophysical black holes (near extremal Kerr)

I Gravity aspects of the dark side of the Universe

Many interesting topics for PhDs!

D. Grumiller — Gravity 3D gravity 35/36

Page 135: Gravity, Astrophysics and Cosmologyquark.itp.tuwien.ac.at/~grumil/pdf/ring2011.pdf · Gravity, Astrophysics and Cosmology Daniel Grumiller Institute for Theoretical Physics Vienna

Thank you for your attention!Black hole curves spacetime Simple black hole analog

Thank you for your attention!

Thanks to Bob McNees for providing the LATEX beamerclass!

D. Grumiller — Gravity 3D gravity 36/36