Talks

12025 - 12036 of 19958 Results

13/14 PSI - Quantum Field Theory II - Lecture 12

Francois David CEA Saclay

November 26, 2013

PIRSA:13110023
13/14 PSI - Condensed Matter - Lecture 11

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 25, 2013

PIRSA:13110041
13/14 PSI - Quantum Field Theory II - Lecture 11

Francois David CEA Saclay

November 25, 2013

PIRSA:13110022
13/14 PSI - Condensed Matter - Lecture 10

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 22, 2013

PIRSA:13110038
13/14 PSI - Quantum Field Theory II - Lecture 10

Francois David CEA Saclay

November 22, 2013

PIRSA:13110019
General Relativity for Cosmology - Lecture 20

Achim Kempf University of Waterloo

November 21, 2013

PIRSA:13110006
General Relativity for Cosmology - Lecture 19

Achim Kempf University of Waterloo

November 21, 2013

PIRSA:13110002
Dimensional reduction in the sky

November 21, 2013

PIRSA:13110059

General Relativity & Quantum Cosmology
Charged particle motion in magnetized black holes

Valeri Frolov University of Alberta

November 21, 2013

PIRSA:13110066

General Relativity & Quantum Cosmology
13/14 PSI - Condensed Matter - Lecture 9

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 21, 2013

PIRSA:13110037
13/14 PSI - Quantum Field Theory II - Lecture 9

Francois David CEA Saclay

November 21, 2013

PIRSA:13110018
Quantum Adversary (Upper) Bound

Shelby Kimmel Massachusetts Institute of Technology (MIT)

November 20, 2013

PIRSA:13110090

Quantum Physics

13/14 PSI - Quantum Field Theory II - Lecture 12

Francois David CEA Saclay

November 26, 2013

PIRSA:13110023
13/14 PSI - Condensed Matter - Lecture 11

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 25, 2013

PIRSA:13110041
13/14 PSI - Quantum Field Theory II - Lecture 11

Francois David CEA Saclay

November 25, 2013

PIRSA:13110022
13/14 PSI - Condensed Matter - Lecture 10

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 22, 2013

PIRSA:13110038
13/14 PSI - Quantum Field Theory II - Lecture 10

Francois David CEA Saclay

November 22, 2013

PIRSA:13110019
General Relativity for Cosmology - Lecture 20

Achim Kempf University of Waterloo

November 21, 2013

PIRSA:13110006
General Relativity for Cosmology - Lecture 19

Achim Kempf University of Waterloo

November 21, 2013

PIRSA:13110002
Dimensional reduction in the sky

November 21, 2013

PIRSA:13110059

General Relativity & Quantum Cosmology

In several approaches to quantum-gravity, the spectral dimension of spacetime runs from the standard value of 4 in the infrared (IR) to a smaller value in the ultraviolet (UV). Describing this running in terms of deformed dispersion relations, I show that a striking cosmological implication is that that UV behavior leading to 2 spectral dimensions results in an exactly scale-invariant spectrum of vacuum scalar and tensor fluctuations. I discuss scenarios that break exact scale-invariance and show that the tensor to scalar ratio is fixed by the UV ratio between the speed of gravity and the speed of light. Cosmological perturbations in this framework display a wavelength-dependent speed of light, but by transforming to a suitable "rainbow frame" this feature can be removed, at the expense of modifying gravity. In particular it turns out that the following concepts are closely connected: scale-invariance of vacuum fluctuations, conformal invariance of the gravitational coupling, UV reduction to spectral dimension 2 in position space and UV reduction to Hausdorff dimension 2 in energy-momentum space.
Charged particle motion in magnetized black holes

Valeri Frolov University of Alberta

November 21, 2013

PIRSA:13110066

General Relativity & Quantum Cosmology

There exist evidences that magnetic field in the vicinity of astrophysical black holes plays an important role. In particular it is required for explanation of such phenomenon as jet formation. Study of such problems in all their complexity requires 3D numerical simulations of the magnetohydrodynamics in a strong gravitational field. Quite often when dealing with such a complicated problem it is instructive to consider first its simplifications, which can be treated either analytically, or by integrating ordinary differential equations. Motion of a charged particle in a weakly magnetized black hole is an important example. We consider a non-rotating black hole in the weak magnetic field which is homogeneous at infinity. In the talk I discuss the following problems: How does such a magnetic field affect charged particle motion in the equatorial plane? How does it change the radius of the innermost stable circular orbits (ISCO) and period of rotation? I shall demonstratethat the magnetic field increases the efficiency of the energy extraction from the black hole and that magnetized black holes can be used as "particle accelerators". Finally, I shall discuss out-of-equatorial-plane motion and demonstrate that it is chaotic. Possible applications of these results to astrophysics are briefly discussed.
13/14 PSI - Condensed Matter - Lecture 9

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 21, 2013

PIRSA:13110037
13/14 PSI - Quantum Field Theory II - Lecture 9

Francois David CEA Saclay

November 21, 2013

PIRSA:13110018
Quantum Adversary (Upper) Bound

Shelby Kimmel Massachusetts Institute of Technology (MIT)

November 20, 2013

PIRSA:13110090

Quantum Physics

I discuss a technique - the quantum adversary upper bound - that uses the structure of quantum algorithms to gain insight into the quantum query complexity of Boolean functions. Using this bound, I show that there must exist an algorithm for a certain Boolean formula that uses a constant number of queries. Since the method is non-constructive, it does not give information about the form of the algorithm. After describing the technique and applying it to a class of functions, I will outline quantum algorithms that match the non-constructive bound.

Title	Date	Collection	Type	Info
13/14 PSI - Quantum Field Theory II - Lecture 12	2013‑11‑26	13/14 PSI - Quantum Field Theory II	Course	View details
13/14 PSI - Condensed Matter - Lecture 11	2013‑11‑25	13/14 PSI - Condensed Matter	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 11	2013‑11‑25	13/14 PSI - Quantum Field Theory II	Course	View details
13/14 PSI - Condensed Matter - Lecture 10	2013‑11‑22	13/14 PSI - Condensed Matter	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 10	2013‑11‑22	13/14 PSI - Quantum Field Theory II	Course	View details
General Relativity for Cosmology - Lecture 20	2013‑11‑21	General Relativity for Cosmology - 2013	Course	View details
General Relativity for Cosmology - Lecture 19	2013‑11‑21	General Relativity for Cosmology - 2013	Course	View details
Dimensional reduction in the sky	2013‑11‑21	Quantum Gravity	Scientific Series	View details
Charged particle motion in magnetized black holes	2013‑11‑21	Strong Gravity	Scientific Series	View details
13/14 PSI - Condensed Matter - Lecture 9	2013‑11‑21	13/14 PSI - Condensed Matter	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 9	2013‑11‑21	13/14 PSI - Quantum Field Theory II	Course	View details
Quantum Adversary (Upper) Bound	2013‑11‑20	Perimeter Institute Quantum Discussions	Scientific Series	View details

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Format results

13/14 PSI - Quantum Field Theory II - Lecture 12

13/14 PSI - Condensed Matter - Lecture 11

13/14 PSI - Quantum Field Theory II - Lecture 11

13/14 PSI - Condensed Matter - Lecture 10

13/14 PSI - Quantum Field Theory II - Lecture 10

General Relativity for Cosmology - Lecture 20

General Relativity for Cosmology - Lecture 19

Dimensional reduction in the sky

Charged particle motion in magnetized black holes

13/14 PSI - Condensed Matter - Lecture 9

13/14 PSI - Quantum Field Theory II - Lecture 9

Quantum Adversary (Upper) Bound

13/14 PSI - Quantum Field Theory II - Lecture 12

13/14 PSI - Condensed Matter - Lecture 11

13/14 PSI - Quantum Field Theory II - Lecture 11

13/14 PSI - Condensed Matter - Lecture 10

13/14 PSI - Quantum Field Theory II - Lecture 10

General Relativity for Cosmology - Lecture 20

General Relativity for Cosmology - Lecture 19

Dimensional reduction in the sky

Charged particle motion in magnetized black holes

13/14 PSI - Condensed Matter - Lecture 9

13/14 PSI - Quantum Field Theory II - Lecture 9

Quantum Adversary (Upper) Bound