Search Talks

Search results from PIRSA

9829 - 9840 of 16958 Results

Sequestering the Standard Model Vacuum Energy

Nemanja Kaloper University of California, Davis
February 21, 2014

PIRSA:14020109
High Energy Physics
13/14 PSI - Quantum Information Review - Lecture 4

Andrew Childs University of Waterloo

February 21, 2014

PIRSA:14020075
13/14 PSI - Quantum Gravity Review - Lecture 4

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 21, 2014

PIRSA:14020064
13/14 PSI - Beyond the Standard Model - Lecture 3

Robert Mann University of Waterloo

February 21, 2014

PIRSA:14020053
Quantum Raychaudhuri equation

Saurya Das University of Lethbridge
February 20, 2014

PIRSA:14020130
General Relativity & Quantum Cosmology
The Sherrington-Kirkpatrick model and its diluted version

Dmitry Panchenko Texas A&M University
February 20, 2014

PIRSA:14020151
Mathematical Physics
Causality, holography, and entanglement entropy
February 20, 2014

PIRSA:14020146
General Relativity & Quantum Cosmology

High Energy Physics

Condensed Matter

General Relativity & Quantum Cosmology
13/14 PSI - Quantum Information Review - Lecture 3

Andrew Childs University of Waterloo

February 20, 2014

PIRSA:14020074
The emergent of the chiral spin liquid in kagome Heisenberg model

Dong-Ning Sheng California State University, Northridge
February 20, 2014

PIRSA:14020149
Condensed Matter
13/14 PSI - Quantum Gravity Review - Lecture 3

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 20, 2014

PIRSA:14020063
13/14 PSI - Beyond the Standard Model - Lecture 2

Robert Mann University of Waterloo

February 20, 2014

PIRSA:14020052
Non equilibrium thermodynamic of gravitational screens

Laurent Freidel Perimeter Institute for Theoretical Physics
February 19, 2014

PIRSA:14020144
General Relativity & Quantum Cosmology

Mathematical Physics

Sequestering the Standard Model Vacuum Energy

Nemanja Kaloper University of California, Davis
February 21, 2014

PIRSA:14020109
High Energy Physics
We propose a very simple reformulation of General Relativity, which completely sequesters from gravity {\it all} of the vacuum energy from a matter sector, including all loop corrections and renders all contributions from phase transitions automatically small. The idea is to make the dimensional parameters in the matter sector functionals of the 4-volume element of the universe. For them to be nonzero, the universe should be finite in spacetime. If this matter is the Standard Model of particle physics, our mechanism prevents any of its vacuum energy, classical or quantum, from sourcing the curvature of the universe. The mechanism is consistent with the large hierarchy between the Planck scale, electroweak scale and curvature scale, and early universe cosmology, including inflation. Consequences of our proposal are that the vacuum curvature of an old and large universe is not zero, but very small, that wDE≃−1 is a transient, and that the universe will collapse in the future.
13/14 PSI - Quantum Information Review - Lecture 4

Andrew Childs University of Waterloo

February 21, 2014

PIRSA:14020075
13/14 PSI - Quantum Gravity Review - Lecture 4

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 21, 2014

PIRSA:14020064
13/14 PSI - Beyond the Standard Model - Lecture 3

Robert Mann University of Waterloo

February 21, 2014

PIRSA:14020053
Quantum Raychaudhuri equation

Saurya Das University of Lethbridge
February 20, 2014

PIRSA:14020130
General Relativity & Quantum Cosmology
We compute quantum corrections to the Raychaudhuri equation, by replacing classical geodesics with quantal (Bohmian) trajectories, and show that they prevent focusing of geodesics, and the formation of conjugate points. We discuss implications for the Hawking-Penrose singularity theorems, and for curvature singularities. Reference: arXiv: 1311.6539
The Sherrington-Kirkpatrick model and its diluted version

Dmitry Panchenko Texas A&M University
February 20, 2014

PIRSA:14020151
Mathematical Physics
I will talk about two types of random processes -- the classical Sherrington-Kirkpatrick (SK) model of spin glasses and its diluted version. One of the main motivations in these models is to find a formula for the maximum of the process, or the free energy, in the limit when the size of the system is getting large. The answer depends on understanding the structure of the Gibbs measure in a certain sense, and this structure is expected to be described by the so called Parisi solution in the SK model and Mézard-Parisi solution in the diluted SK model. I will explain what these are and mention some results in this direction.
Causality, holography, and entanglement entropy
February 20, 2014

PIRSA:14020146
General Relativity & Quantum Cosmology

High Energy Physics

Condensed Matter

General Relativity & Quantum Cosmology
After giving a brief overview of holographic entanglement entropy formulas, I will explore a curious feature they imply: when the bulk spacetime includes a black hole, the entanglement entropies often appear to depend on the spacetime geometry inside the horizon. I will ask whether this implies any loss of causality in the field theory. To answer this question, I will present a new general-relativity theorem concerning the causal structure of asymptotically AdS spacetimes, which implies an interesting relationship between bulk and boundary causal domains.
13/14 PSI - Quantum Information Review - Lecture 3

Andrew Childs University of Waterloo

February 20, 2014

PIRSA:14020074
The emergent of the chiral spin liquid in kagome Heisenberg model

Dong-Ning Sheng California State University, Northridge
February 20, 2014

PIRSA:14020149
Condensed Matter
The quantum spin liquid is an emergent new state of matter, which has attracted a lot of recent attention. In particular, the time reversal symmetry broken spin liquid (Kalmeyer et. al. and Wen et. al.), characterized by the chiral ordering and fractionalized quasi-particle as a realization of the fractional quantum Hall state had been proposed for more than 20 years, but never identified as the true ground state in any more generic (e.g. Heisenberg spin exchange) models with time reversal symmetry. Here I will report two concrete examples where chiral spin liquid (CSL) emerge for a range of parameter space for kagome J1-J2-J3 (three nearest neighbors) model based on accurate density matrix renormalization group (DMRG) simulations. We identify long-range chiral ordering, ground state degeneracy, characteristic entanglement spectra, and the fractionalized topological Chern number to establish the topological state in such a system as the long-sought CSL. We further explicitly extract the modular matrix, which captures all the information of the fractional statistics of the quasi-particles in the system. I will also discuss the close relation of our model to some frustrated kagome antiferromagnets, and make a conjecture that J1 kagome model is near an unconventional critical point. I will conclude the talk with some discussions of the open directions.
13/14 PSI - Quantum Gravity Review - Lecture 3

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 20, 2014

PIRSA:14020063
13/14 PSI - Beyond the Standard Model - Lecture 2

Robert Mann University of Waterloo

February 20, 2014

PIRSA:14020052
Non equilibrium thermodynamic of gravitational screens

Laurent Freidel Perimeter Institute for Theoretical Physics
February 19, 2014

PIRSA:14020144
General Relativity & Quantum Cosmology

Mathematical Physics
In this talk I will review the evidence for a mysterious and deep relationship between gravitational dynamics and thermodynamics. I will show how we can extend this connection to non equilibrium thermodynamics. Using the fact that the gravitational equations are fundamentally holographic, we express them in a way that shows a deep connection between gravity and the dynamics of viscous bubbles. We will explore some aspects of this surprising correspondence.

Title	Date	Collection	Type	Info
Sequestering the Standard Model Vacuum Energy	2014‑02‑21	Particle Physics	Scientific Series	View details
13/14 PSI - Quantum Information Review - Lecture 4	2014‑02‑21	13/14 PSI - Quantum Information Review	Course	View details
13/14 PSI - Quantum Gravity Review - Lecture 4	2014‑02‑21	13/14 PSI - Quantum Gravity Review	Course	View details
13/14 PSI - Beyond the Standard Model - Lecture 3	2014‑02‑21	13/14 PSI - Beyond the Standard Model	Course	View details
Quantum Raychaudhuri equation	2014‑02‑20	Quantum Gravity	Scientific Series	View details
The Sherrington-Kirkpatrick model and its diluted version	2014‑02‑20	Colloquium	Scientific Series	View details
Causality, holography, and entanglement entropy	2014‑02‑20	Quantum Fields and Strings	Scientific Series	View details
13/14 PSI - Quantum Information Review - Lecture 3	2014‑02‑20	13/14 PSI - Quantum Information Review	Course	View details
The emergent of the chiral spin liquid in kagome Heisenberg model	2014‑02‑20	Quantum Matter	Scientific Series	View details
13/14 PSI - Quantum Gravity Review - Lecture 3	2014‑02‑20	13/14 PSI - Quantum Gravity Review	Course	View details
13/14 PSI - Beyond the Standard Model - Lecture 2	2014‑02‑20	13/14 PSI - Beyond the Standard Model	Course	View details
Non equilibrium thermodynamic of gravitational screens	2014‑02‑19	Colloquium	Scientific Series	View details

Supported by

Format results

Sequestering the Standard Model Vacuum Energy

13/14 PSI - Quantum Information Review - Lecture 4

13/14 PSI - Quantum Gravity Review - Lecture 4

13/14 PSI - Beyond the Standard Model - Lecture 3

Quantum Raychaudhuri equation

The Sherrington-Kirkpatrick model and its diluted version

Causality, holography, and entanglement entropy

13/14 PSI - Quantum Information Review - Lecture 3

The emergent of the chiral spin liquid in kagome Heisenberg model

13/14 PSI - Quantum Gravity Review - Lecture 3

13/14 PSI - Beyond the Standard Model - Lecture 2

Non equilibrium thermodynamic of gravitational screens

Sequestering the Standard Model Vacuum Energy

13/14 PSI - Quantum Information Review - Lecture 4

13/14 PSI - Quantum Gravity Review - Lecture 4

13/14 PSI - Beyond the Standard Model - Lecture 3

Quantum Raychaudhuri equation

The Sherrington-Kirkpatrick model and its diluted version

Causality, holography, and entanglement entropy

13/14 PSI - Quantum Information Review - Lecture 3

The emergent of the chiral spin liquid in kagome Heisenberg model

13/14 PSI - Quantum Gravity Review - Lecture 3

13/14 PSI - Beyond the Standard Model - Lecture 2

Non equilibrium thermodynamic of gravitational screens