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Quantum Liquids and Turbulent Black Holes

Allan Adams Massachusetts Institute of Technology (MIT) - Department of Physics
February 24, 2014

PIRSA:14020141
High Energy Physics
13/14 PSI - Quantum Information Review - Lecture 6

Andrew Childs University of Waterloo

February 24, 2014

PIRSA:14020078
Quantum Many-body Dynamics with Matrix Product States

Martin Ganahl Sandbox AQ
February 24, 2014

PIRSA:14020156
Astrophysics

Condensed Matter
13/14 PSI - Quantum Gravity Review - Lecture 5

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 24, 2014

PIRSA:14020067
13/14 PSI - Beyond the Standard Model - Lecture 4

Robert Mann University of Waterloo

February 24, 2014

PIRSA:14020056
13/14 PSI - Quantum Information Review - Lecture 5

Andrew Childs University of Waterloo

February 21, 2014

PIRSA:14020153
Sequestering the Standard Model Vacuum Energy

Nemanja Kaloper University of California System
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

Quantum Liquids and Turbulent Black Holes

Allan Adams Massachusetts Institute of Technology (MIT) - Department of Physics
February 24, 2014

PIRSA:14020141
High Energy Physics
The physics of black hole horizons is intimately connected to the physics of quantum liquids. In this talk I will review the connection and draw lessons about quantum turbulence from black hole dynamics and vice versa. For example, gravitational dynamics reveal that quantum turbulence can behave very differently from normal fluid turbulence in 2d, with long-wavelength excitations rapidly dissolving into small fluctuations and dissipating as in a 3d normal liquid. Meanwhile, familiar facts about turbulent flows in normal fluids imply that the horizons of certain accreting black holes evolve in time as if they have a non-trivial fractal dimension.
13/14 PSI - Quantum Information Review - Lecture 6

Andrew Childs University of Waterloo

February 24, 2014

PIRSA:14020078
Quantum Many-body Dynamics with Matrix Product States

Martin Ganahl Sandbox AQ
February 24, 2014

PIRSA:14020156
Astrophysics

Condensed Matter
The talk is divided into two parts: in the first, I will talk about dynamics of far-from equilibrium initial states in different lattice models. I will present results of quench dynamics of the XXZ-Heisenberg magnet, where interesting physics emerges after quenching the system. Then I will present results for scattering of solitonic objects in different integrable and non-integrable lattice models. In the second part, I will talk about dynamics of impurity systems. There I will talk about how impurity spectral functions can be calculated using the Chebyshev technique, and how MPS can serve as a high resolution impurity solver for Dynamical Mean-Field Theory. Finally, I will show some results for steady-state currents through a quantum dot device.
13/14 PSI - Quantum Gravity Review - Lecture 5

Bianca Dittrich Perimeter Institute for Theoretical Physics

February 24, 2014

PIRSA:14020067
13/14 PSI - Beyond the Standard Model - Lecture 4

Robert Mann University of Waterloo

February 24, 2014

PIRSA:14020056
13/14 PSI - Quantum Information Review - Lecture 5

Andrew Childs University of Waterloo

February 21, 2014

PIRSA:14020153
Sequestering the Standard Model Vacuum Energy

Nemanja Kaloper University of California System
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.

Title	Date	Collection	Type	Info
Quantum Liquids and Turbulent Black Holes	2014‑02‑24	Quantum Fields and Strings	Scientific Series	View details
13/14 PSI - Quantum Information Review - Lecture 6	2014‑02‑24	13/14 PSI - Quantum Information Review	Course	View details
Quantum Many-body Dynamics with Matrix Product States	2014‑02‑24	Quantum Matter	Scientific Series	View details
13/14 PSI - Quantum Gravity Review - Lecture 5	2014‑02‑24	13/14 PSI - Quantum Gravity Review	Course	View details
13/14 PSI - Beyond the Standard Model - Lecture 4	2014‑02‑24	13/14 PSI - Beyond the Standard Model	Course	View details
13/14 PSI - Quantum Information Review - Lecture 5	2014‑02‑21	13/14 PSI - Quantum Information Review	Course	View details
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

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Format results

Quantum Liquids and Turbulent Black Holes

13/14 PSI - Quantum Information Review - Lecture 6

Quantum Many-body Dynamics with Matrix Product States

13/14 PSI - Quantum Gravity Review - Lecture 5

13/14 PSI - Beyond the Standard Model - Lecture 4

13/14 PSI - Quantum Information Review - Lecture 5

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

Quantum Liquids and Turbulent Black Holes

13/14 PSI - Quantum Information Review - Lecture 6

Quantum Many-body Dynamics with Matrix Product States

13/14 PSI - Quantum Gravity Review - Lecture 5

13/14 PSI - Beyond the Standard Model - Lecture 4

13/14 PSI - Quantum Information Review - Lecture 5

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