emergent inflationigpg.gravity.psu.edu/igc/talks/alexander.pdf · 2007. 9. 5. · stephon alexander...
TRANSCRIPT
![Page 1: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/1.jpg)
Stephon AlexanderTirtho BiswasDeepak Vaid (Grad Student)Penn State University
Emergent Inflation
![Page 2: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/2.jpg)
Outline
Overview of Inflation Main Idea: The Instability of the Perturtbative
Vacuum Review of the microscopic BCS theory Calculation and Realization Conclusion Outlook
![Page 3: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/3.jpg)
Why is Inflation NeededA. Horizon Problem
Here and Now
![Page 4: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/4.jpg)
Inflation is an epoch whereinThe scale factor has positive acceleration
(Guth, Linde, Mukhanov.Starobinsky early 80s)
![Page 5: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/5.jpg)
Inflation is an epoch whereinThe scale factor has near exponential growth.
![Page 6: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/6.jpg)
-The biggest problem with inflation boils down to its reliance on scalar fields.
-Borde, Guth, Vilenkin (PRL 2003) proved that scalar field driven inflation suffers geodesic incompleteness and from a big bang singularity. (modulo rare null-energy violating fluctuations)
-Scalar fields are the culprit behind the infamous fine tuning problems in inflation (and the standard model).
-How does inflation end?
-Cosmological Constant Problem.
![Page 7: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/7.jpg)
Don’t Throw out the BabyUniverse with the Bathwater!
1) Can we obtain inflation naturally withoutfundamental scalar fields?
2) If this is possible will we resolve the problemsthat currently afflict inflation
Answer: (1) Yes (2) Very likely
![Page 8: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/8.jpg)
A New Outlook:Condensates in Cosmology
(Parker, Brout, Brandenberger, Zhitnitsky, S.A, Moffat, Mbonye)
Condensates are attractive because they can vanish in the UV and IR (superfluidity).
They can be purely long range (macroscopic) quantum phenomena.
They are very common across a wide range of physical phenomena. In the context of inflation they could drive inflation and dissapear at the end (IR) leading to a natural graceful exit. But what exactly is this magical condensate?
![Page 9: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/9.jpg)
The Cooper Instability
-In a conducting medium the Fermi sea is always unstable if there exist a small attractive interaction.
-Phonons screening of the electric charge giving an effective attractive interaction.
-A new ground state is found whose fundamental excitations are spin zero paired electrons (Cooper Pairs).
![Page 10: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/10.jpg)
BCS Theory: Fundamentals
Key: Correlations of fermions across Fermi surface
![Page 11: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/11.jpg)
SUPERCONDUCTIVITY
Fermi Surface
True Ground State
The perturbative vacuum (Fermi surface) is unstable, due to strongly correlated electron pairs. There is a non-perturbative ground state with lower energy,separated by an energy gap.
=density of states
![Page 12: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/12.jpg)
WHAT IF THE PETURBATIVEINTERACTIONS OFFERMIONS WITH RESPECT TOGRAVITY IS UNSTABLEIN THE SAME WAY?
ANSWER: THIS IS PLAUSIBLE IF THERE IS1) A FOUR FERMION INTERACTION
2) A FERMI SURFACE (CHEMICAL POTENTIAL)
3) SCREENING OF REPULSIVE INTERACTION (NEUTRAL FERMIONS WOULD ALSO SUFFICE)
![Page 13: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/13.jpg)
Perturbative Vacuum
True Ground State
The perturbative vacuum is unstable. There is a non-perturbative ground state.
E
Space-time Superconductivity
![Page 14: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/14.jpg)
![Page 15: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/15.jpg)
A key insight in BCS theory is that the true groundstate wavefunction (BCS State) is constructed by a phase coherent superposition of paired states
g is the weight of each of the paired states
![Page 16: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/16.jpg)
BCS HAMILTONIAN
This Hamiltonian has a non perturbative ground state which corresponds to pairs of fermions with opposite spin and momenta.
The Schrodinger eq. yields an exact ground state energy with an energy gap separating the condensate from the ‘free state’
Bardeen, Cooper and Schrieffer considered the Hamiltonian describing the superconducting state.
-fermion creation operator
-Two body interaction potential of correlated fermions.
k & s denote momenta and spin of fermion in fermi sea
![Page 17: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/17.jpg)
The |BCS> state is an eigenstate of the transformed HamiltonianThe Amplitude (gap) needs to be determined.
This new state is the true ground state, separated from false ground state by this gap.
u and v -> probability of creating and destroying a Cooper Pair
The BCS state is a coherent state of Cooper Pairs:
![Page 18: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/18.jpg)
After transforming the Hamiltonian
To get ground state, set occupation numbersto zero and anticommutation of b’s gives a self consistent eq for the gap:
![Page 19: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/19.jpg)
There will now be a transformed Hamiltonian that acts on |BCS> which is a coherent state of fermion pairs.
This new state is the true ground state, separated from false ground state by an energy gap.
Where u,v are determined by the BCS wavefunctionThese new operators corresponding to breaking
![Page 20: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/20.jpg)
In terms of the new Hamiltonian the gap represents an exitation of quasiparticle’s energy spectrum
![Page 21: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/21.jpg)
Which has both weak and strong coupling solution.
We’ll get back to this later.
EXACT NON-PERTURBATIVE SOLUTION
D = Density of states (number of states per unit frequency)V= interaction coupling
![Page 22: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/22.jpg)
The Lesson
Superconducivity is an example of a macroscopic non-perturbative phenomena which is purely quantum mechanical.
Cannot be seen by perturbation theory.
The Cooper pairs behave effectively like a scalar field but is not fundamental.
QUESTION: Can this give us inflation?
![Page 23: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/23.jpg)
We now demonstrate that General Relativity coupled to freefermions have the necessary four fermion interactions necessary for a BCS condensate.
The Mechanism:1) A time dependent space-time background self consistently generates a non-perturbative condensation of fermions. 2) The energy gap yields a repulsive effect which generates inflation.3) As the universe inflates the gap contribution becomes irrelevant and inflation naturally ends.
![Page 24: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/24.jpg)
![Page 25: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/25.jpg)
General Relativity Covariantly Coupled to Free-Fermions
![Page 26: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/26.jpg)
We now vary the action w.r.t the connection:
We find the following solution:
First term is pure gravitational part (symmetric)Second term is fermion current.
![Page 27: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/27.jpg)
We reinsert the solutions:
And get the much sought after universal four-fermionInteraction!
![Page 28: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/28.jpg)
HamiltonianAfter a lot of simple algebra and using the ADM 3+1Decomposition we arrive at the following Hamiltonian
K is the extrinsic curvature
![Page 29: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/29.jpg)
We will restrict this system to a cosmology, ie non-vanishing Lambda
The Hamiltonian simplifies significantly.
Question: What is the self consistent solution the fermion many body wavefunction in a time dependent background?
![Page 30: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/30.jpg)
Our Hamiltonian is very similar to the BCS one.
We can try to find the gap using the same methods.
Setting the occupation numbers equal to zero and diagonalizing H
![Page 31: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/31.jpg)
We obtain the equation for the gap
![Page 32: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/32.jpg)
Realization of Emergent Inflation
This mess beautifully simplifies to:
![Page 33: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/33.jpg)
EMERGENT INFLATION
a(t)
We get exponential growth which ends.
![Page 34: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/34.jpg)
Cosmological Gap
![Page 35: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/35.jpg)
Hubble Parameter
![Page 36: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/36.jpg)
What is going on physically?
-The instability of the perturbative vacuumyields an emergent phenomena.
-This emergent phenomena is a large scale Phase coherence which amplifies the scalefactor.
-Macroscopic phase coherence = Inflation.
-Similar to the emergent (collective)phenomena known as superconductivity.
![Page 37: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/37.jpg)
No Multiverse!
Scale factor is not sufficient to describe correlations inHubble radius.
Phase coherence of condensate wavefunction is tiedInto the amplification of scale factor.
Therefore eternally inflating bubbles can not satisfy thisInitial conditon since it is geodesically complete in past.
![Page 38: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/38.jpg)
The number of e-foldings are only sensitive to the initial fermi energy (density of states)
The generation of perturbations on superhorizonScales will correspond to fluctuations in condensate-> supressed on superhorizon scales.
Geodesically complete since scalar field is not fundamentalAnd initial state is Minkowski.
Do We resolve problems of scalarField inflation?
![Page 39: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/39.jpg)
Conclusion and Outlook
-We have begun the first steps toward an emergent inflationary model which requires no scalar fields.
-Inflation is equivalent to a superconducting phase space-time
-The Graceful exit problem is self-consistently solved.
-We may actually have a synergy between bouncing Singularity free cosmology followed by inflation
-What are the predictions? Could it be the Higgs?
![Page 40: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/40.jpg)
COULD THIS HAPPEN IN THE CONTEXT OF ADS/CFT?
IS INFLATION A BOUNCINGCOSMOLOGY IN DISGIUSE?
![Page 41: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/41.jpg)
![Page 42: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/42.jpg)
![Page 43: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/43.jpg)
![Page 44: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/44.jpg)
![Page 45: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/45.jpg)
![Page 46: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/46.jpg)
![Page 47: Emergent Inflationigpg.gravity.psu.edu/igc/talks/Alexander.pdf · 2007. 9. 5. · Stephon Alexander Tirtho Biswas Deepak Vaid (Grad Student) Penn State University Emergent Inflation](https://reader035.vdocuments.net/reader035/viewer/2022081601/610d9585a552a71e65636348/html5/thumbnails/47.jpg)