jim brau univ. of oregon quarknet july 9, 2008 modern particle physics how we got here, and where...

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Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

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Page 1: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

MODERN PARTICLE PHYSICS

How we got here, and where we’re going

Page 2: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Mysteries of the Universe

• Quarks• Leptons• Higgs Bosons• Supersymmetric

Particles• SuperString

Theory

• Dark Matter• Dark Energy

and the cosmological constant

• Accelerating Universe

• Gravity Waves• Extra Dimensions

Page 3: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The End of Physics

"The more important fundamental laws and facts of physical science have all been discovered,

and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.”

Page 4: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894

The End of Physics

Page 5: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Miracle Year - 1905

RelativityQuantum PhysicsAtoms

1915 - General Theory of Relativity, the theory of gravity, based on warped space

Page 6: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Relativity

• When a man sits with a pretty girl for an hour, it seems like a minute.

• But let him sit on a hot stove for a minute—and it’s longer than any hour.

• That’s relativity.

Page 7: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Missing from understanding of the Universe in 1905?

Physics in 1905

Quantum MechanicsNuclear Physics

Elementary Particles

Page 8: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Missing from understanding of the Universe in 1905?

Physics in 1905

Edwin Powell Hubble (1889-1953)

Page 9: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Einstein’s Theoretical Discoveries

– Light comes in small packets - photons

– The speed of light is a constant• Independent of observer’s motion

Page 10: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Einstein’s Theoretical Discoveries

– Light comes in small packets - photons

– The speed of light is a constant• Independent of observer’s motion

– E=mc2

– Space is warped by massive objects

– “Cosmological constant”

– Many others

Page 11: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

– Light comes in small packets - photons

– The speed of light is a constant• Independent of observer’s motion

– E=mc2

– Space is warped by massive objects

– “Cosmological constant”

– Many others

• Remain central to our exploration of the universe

•xx

Einstein’s Theoretical Discoveries

•xx•xx

•xx•xx

Page 12: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Einstein and Quantum Mechanics

Page 13: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Quantum Mechanics and Gravity

Inconsistent?

Page 14: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Einstein’s Dream

• To understand the underlying simplicity behind the vast complexities of Nature

Suspected gravity was a key

Page 15: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Unification

Understand how nature’s forces are relatedelectricity, magnetism, and gravityelectromagnetis

m

Page 16: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Einstein’s Dream Today

• Today, STRING THEORY – Unifies all forces– Overcomes inconsistencies between

gravity and quantum mechanics

• Ultimate Explanation?– from the tiniest quanta to the cosmos

• The Dream Lives On

• There are encouraging signs that success is near

Page 17: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Universe is Mysterious, but Comprehensible

Willamette HallNo doubt about it

Al – we’ve mathematically expressed the purpose of the

universe. God, how I love

the thrill of scientific discovery

Page 18: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Next RevolutionToday on the threshold of a revolution in understanding of the Universe

Recent discoveries

and powerful set of tools:

Page 19: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

• What is the universe made of?– Ordinary matter and the known forces? Or more?

• How does it work?– From the sub-atomic to the cosmic scale

• How many spatial dimensions are there?– Just 3, or more (hidden dimensions)

• Why does matter have mass?• What was the Big Bang?

The Frontier The Frontier NowNow

Page 20: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Convergence of the Large and the Small

Page 21: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Modern scientific instruments

Fermilab, near ChicagoFermilab, near Chicago

Stanford Linear AcceleratorStanford Linear Accelerator

LIGO Laboratory, HanfordLIGO Laboratory, Hanford

Hubble Space TelescopeHubble Space Telescope

Cerro Tololo, ChileCerro Tololo, Chile

Page 22: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

• probe laws of the cosmos in 2 ways

1. Super-microscope

2. Creation of massive matter (E=mc2) Heavy ordinary matter

Dark Matter

Particle Accelerators

ANTI-PROTONPROTON

Page 23: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

What is matter?

• All matter we are familiar with is composed of atoms, or parts of atoms– Living things – butterflys, elephants, people …– Inanimate things – rocks, watches, cannonballs …– Astrophysical objects – planets, moon, stars, asteroids …

Even cosmic rays!

Page 24: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

What is matter?Experiments with particle colliders have

advanced our detailed understanding of matter and how it behaves

Page 25: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

What is matter?• Quarks

– combine to make protons and neutrons

• Leptons– eg. electron, neutrino

• Force Carriers– defines behavior of matter

We have a precise understanding of matter and its behavior

Page 26: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Structure of Matter

?

?

Page 27: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Are atoms alone a sufficient basis for explaining the

Universe?

No – not even close

Page 28: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Halo of Dark Matter

Page 29: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

How do we know that galaxies are surrounded by dark halo?

Galaxies are spinning too fast to be held together by gravity of the stars

Vera Rubin1950s

Page 30: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

• 1930s motions of clusters of galaxies cannot be understood – Fritz Zwicky

• 1990-2000s Refined studies show dark matter dominance

Dark Matter Evidence

Page 31: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Dark Matter Evidence

• 1930s motions of clusters of galaxies cannot be understood – Fritz Zwicky

• 1990-2000s Refined studies show dark matter dominance

Page 32: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Imaging Dark Matter

Page 33: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Imaging Dark Matter

Hubble Data analyzed by Yale astrophysicists

Page 34: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Observing Galaxies• There must be a dominant presence of

a dark form of matter

– It is invisible!– We “see” it through gravitational effects

– this is the only way we know it exists

– What is it?– Is it just faint, ordinary matter?

• Most likely not - Promising candidate - exotic type of fundamental particle which is anticipated by particle theory

• Supersymmetric particle (Neutralino)

Page 35: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Symmetries of particles

• 1928, Paul A.M. Dirac – Theory of the electron– Combining relativity and quantum mechanics

• He needed to assume there were partner particles for every known particle

• ANTI-MATTER • DOUBLED THE NUMBER OF PARTICLES

Page 36: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Discovery of Anti-Matter

• 1932 -Carl Anderson – The anti-electron,

or positron

All known particles have anti-particles

ELEMENTARYANTI-PARTICLES

Ant

i-Q

uark

sA

nti-

Lep

tons

Page 37: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

SuperString Theory

• Unifies all particles and all forces– gravity with quantum mechanics

• Fundamental particles are represented as vibrations on string

– String is miniscule • Atom is 10,000,000,000,000,000,000,000,000 x bigger

– Space is ten-dimensional (not 3D!)– A matching set of particles appear

• the super-partners of ordinary particles

Page 38: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Structure of Matter

?

hypothesis

?

Page 39: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

ELEMENTARYANTI-PARTICLES

Ant

i-Q

uark

sA

nti-

Lep

tons

Supersymmetry and Strings

• History repeats?• Just as for anti-matter,

– New particles are required tomake successful theory

• The supersymmetric particles have just the properties expected of Dark Matter

Page 40: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Universe

Another puzzle What gives matter mass?

• An ocean of Higgs Bosons - “Higgs Field”

Page 41: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Large Hadron Collider (LHC)Geneva, Switzerland

Nearing Nearing CompletionCompletion

Begins Begins operation this operation this

yearyear

Page 42: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

International Linear Collider (ILC)

30 Miles

Under development

Page 43: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Big Bang

• Fundamental Physics needed to understand Big Bang

Page 44: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Cosmic Fireball

• Visible remnant of the Big Bang – microwaves in the sky– traveling through space for 14 billion years

Microwaves in the sky

Page 45: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Probing the Big Bang

• Studied since 1965 discovery

• Series of increasingly more sensitive experiments

• Lastest - WMAP

Page 46: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Probing the Big Bang

• Analysis of the WMAP data is equivalent to “weighing” the universe

Page 47: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Probing the Big Bang

• The stars are a very small fraction

Energy ofOur

Universe

•Additional ordinary matter, Still a small fraction

•Anti- matter miniscule

Page 48: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Probing the Big Bang

• The dominant “weight” of the universe is dark matter and dark energy

•Dark Energy Surprise•Related to Einstein’s Cosmological Constant

Page 49: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

The Dark Side Controls the Universe

Dark Matter HOLDS IT TOGETHER

Dark Energy DETERMINES ITS DESTINY

Dark Matter is strange!Dark Matter is strange!

What about Dark Energy?What about Dark Energy?

Page 50: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Measuring the Universe’ Expansion

Acceleration

Driven by Dark

Energy

After Supernova After Supernova After Supernova

Page 51: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

• The closest realization of “nothing” is the vacuum – “empty space”

• Quantum physics -> no truly empty space• “Empty space” filled with temporary

particles

The Dark Energy Something from Nothing Dark

Energy

Dark Matter

Page 52: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Empty Space

The Dark Energy Something from Nothing

Dark Energy

Dark Matter

Page 53: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Quantum Fluctuations Create a “Dark Energy”

– Cosmological constant

The Dark Energy Something from Nothing

Dark Energy

Dark Matter

Page 54: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Something from Nothing

• We can calculate the effect of these virtual particles on Dark Energy– This theoretical result is too big

– This is a BIG-time mystery • we know how the universe might make

Dark Energy, but we don’t know how to make so little

– By a factor of 1,000,000,000,000,000,000,000,000,000,000,000,000,000,000,

000,000,000,000,000,000,000,000,000,000,000,000,000, 000,000,000,000,000,000,000,000,000,000,000,000,000

Page 55: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Seeking the Primordial Gravity Waves

• The fabric of the universe is still rattling from the violent Big Bang

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

Page 56: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Primordial Gravity Waves

• LIGO looks for evidence of gravity waves

Hanford LIGO

Page 57: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Gravity Waves Probe the Extremely Early Universe

14 billion

Page 58: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Extra Dimensions

• String Theory– 10-dimensional space

• Particle Collider Experiments are looking for these hidden dimensions

Page 59: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Our Mysterious Universe

Page 60: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

Realizing Einstein’s Dream

• We are on the eve of a revolution in physics– Many mysteries – Solutions appear near – Deeper understanding of the universe itself

• Gravity waves may image earliest moments of Big Bang

• Dark Matter particles – may appear soon in particle collider experiments at accelerators

• Why is there mass? – Higgs Boson• Dark Energy – this is the biggest mystery of all

Page 61: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008

RESEARCH SUPPORTED BY

Department of Energy OFFICE OF SCIENCE

NATIONAL SCIENCE FOUNDATION

Philip H. Knight

Acknowledgements

Page 62: Jim Brau Univ. of Oregon QuarkNet July 9, 2008 MODERN PARTICLE PHYSICS How we got here, and where we’re going

Jim Brau Univ. of Oregon QuarkNet July 9, 2008