Talks

14329 - 14340 of 14970 Results

Supersymmetry and the LHC Inverse Problem

Jesse Thaler Massachusetts Institute of Technology (MIT)

March 21, 2006 PIRSA:06030017

Quantum Fields and Strings

Particle Physics
LHC Olympics at CERN

Jesse Thaler Massachusetts Institute of Technology (MIT)

March 21, 2006 PIRSA:06030016

Quantum Fields and Strings

Particle Physics

Cosmology
Introduction to quantum gravity - Part 16

Lee Smolin Perimeter Institute for Theoretical Physics

March 15, 2006 PIRSA:06030015
Introduction to quantum gravity - Part 15

Lee Smolin Perimeter Institute for Theoretical Physics

March 15, 2006 PIRSA:06030014
Limits on efficient computation in the physics world

Scott Aaronson The University of Texas at Austin

March 15, 2006 PIRSA:06030013

Quantum Information

Quantum Foundations
Chaos from the Big Bang to Black Holes

Janna Levin Columbia University

March 15, 2006 PIRSA:06030012
String Loops vs. AdS/CFT

Gordon Semenoff University of British Columbia

March 14, 2006 PIRSA:06030011

Quantum Fields and Strings
The chaotic evolution of Newton's universe

March 09, 2006 PIRSA:06030010
Introduction to quantum gravity - Part 14

Lee Smolin Perimeter Institute for Theoretical Physics

March 08, 2006 PIRSA:06030009
Introduction to quantum gravity - Part 13

Lee Smolin Perimeter Institute for Theoretical Physics

March 08, 2006 PIRSA:06030008
GHZ correlations are just a bit nonlocal

Carlton Caves University of New Mexico

March 08, 2006 PIRSA:06030007

Quantum Information
Newton-Hooke algebras, non-relativistic branes and generalized pp-wave metrics

Joaquim Gomis Universitat de Barcelona

March 07, 2006 PIRSA:06030006

Quantum Fields and Strings

Supersymmetry and the LHC Inverse Problem

Jesse Thaler Massachusetts Institute of Technology (MIT)

March 21, 2006 PIRSA:06030017

Quantum Fields and Strings

Particle Physics
LHC Olympics at CERN

Jesse Thaler Massachusetts Institute of Technology (MIT)

March 21, 2006 PIRSA:06030016

Quantum Fields and Strings

Particle Physics

Cosmology
Introduction to quantum gravity - Part 16

Lee Smolin Perimeter Institute for Theoretical Physics

March 15, 2006 PIRSA:06030015

This is an introduction to background independent quantum theories of gravity, with a focus on loop quantum gravity and related approaches. Basic texts: -Quantum Gravity, by Carlo Rovelli, Cambridge University Press 2005 -Quantum gravityy with a positive cosmological constant, Lee Smolin, hep-th/0209079 -Invitation to loop quantum gravity, Lee Smolin, hep-th/0408048 -Gauge fields, knots and gravity, JC Baez, JP Muniain Prerequisites: -undergraduate quantum mechanics -basics of classical gauge field theories -basic general relativity -hamiltonian and lagrangian mechanics -basics of lie algebras
Introduction to quantum gravity - Part 15

Lee Smolin Perimeter Institute for Theoretical Physics

March 15, 2006 PIRSA:06030014

This is an introduction to background independent quantum theories of gravity, with a focus on loop quantum gravity and related approaches. Basic texts: -Quantum Gravity, by Carlo Rovelli, Cambridge University Press 2005 -Quantum gravityy with a positive cosmological constant, Lee Smolin, hep-th/0209079 -Invitation to loop quantum gravity, Lee Smolin, hep-th/0408048 -Gauge fields, knots and gravity, JC Baez, JP Muniain Prerequisites: -undergraduate quantum mechanics -basics of classical gauge field theories -basic general relativity -hamiltonian and lagrangian mechanics -basics of lie algebras
Limits on efficient computation in the physics world

Scott Aaronson The University of Texas at Austin

March 15, 2006 PIRSA:06030013

Quantum Information

Quantum Foundations
Chaos from the Big Bang to Black Holes

Janna Levin Columbia University

March 15, 2006 PIRSA:06030012
String Loops vs. AdS/CFT

Gordon Semenoff University of British Columbia

March 14, 2006 PIRSA:06030011

Quantum Fields and Strings
The chaotic evolution of Newton's universe

March 09, 2006 PIRSA:06030010

In this expository talk, I describe how "chaotic behavior" not only was discovered in the study of the Newtonian N-body problem, but also is responsible for several strange appearing motions. Then, a mathematical outline of the general evolution of the universe, under Newton's laws, is provided. No prior background in dynamics or the mathematics of the N-body problem is needed to follow this lecture
Introduction to quantum gravity - Part 14

Lee Smolin Perimeter Institute for Theoretical Physics

March 08, 2006 PIRSA:06030009

This is an introduction to background independent quantum theories of gravity, with a focus on loop quantum gravity and related approaches. Basic texts: -Quantum Gravity, by Carlo Rovelli, Cambridge University Press 2005 -Quantum gravityy with a positive cosmological constant, Lee Smolin, hep-th/0209079 -Invitation to loop quantum gravity, Lee Smolin, hep-th/0408048 -Gauge fields, knots and gravity, JC Baez, JP Muniain Prerequisites: -undergraduate quantum mechanics -basics of classical gauge field theories -basic general relativity -hamiltonian and lagrangian mechanics -basics of lie algebras
Introduction to quantum gravity - Part 13

Lee Smolin Perimeter Institute for Theoretical Physics

March 08, 2006 PIRSA:06030008

This is an introduction to background independent quantum theories of gravity, with a focus on loop quantum gravity and related approaches. Basic texts: -Quantum Gravity, by Carlo Rovelli, Cambridge University Press 2005 -Quantum gravityy with a positive cosmological constant, Lee Smolin, hep-th/0209079 -Invitation to loop quantum gravity, Lee Smolin, hep-th/0408048 -Gauge fields, knots and gravity, JC Baez, JP Muniain Prerequisites: -undergraduate quantum mechanics -basics of classical gauge field theories -basic general relativity -hamiltonian and lagrangian mechanics -basics of lie algebras
GHZ correlations are just a bit nonlocal

Carlton Caves University of New Mexico

March 08, 2006 PIRSA:06030007

Quantum Information

The amount of nonlocality in the GHZ state can be quantified by determining how much classical communication is required to bring a local-hidden-variable model into agreement with the predictions of quantum mechanics. It turns out that one bit suffices, and, of course, nothing less will do. I will discuss generalizations of this result to graph states and its relation to the stabilizer formalism.
Newton-Hooke algebras, non-relativistic branes and generalized pp-wave metrics

Joaquim Gomis Universitat de Barcelona

March 07, 2006 PIRSA:06030006

Quantum Fields and Strings

Title	Speaker(s)	Date	Collection	Type	Info
Supersymmetry and the LHC Inverse Problem	Jesse Thaler	2006‑03‑21	Quantum Fields and Strings	Scientific Series	View details
LHC Olympics at CERN	Jesse Thaler	2006‑03‑21	Quantum Fields and Strings	Scientific Series	View details
Introduction to quantum gravity - Part 16	Lee Smolin	2006‑03‑15	Introduction to Quantum Gravity - 2006	Conference	View details
Introduction to quantum gravity - Part 15	Lee Smolin	2006‑03‑15	Introduction to Quantum Gravity - 2006	Conference	View details
Limits on efficient computation in the physics world	Scott Aaronson	2006‑03‑15	Perimeter Institute Quantum Discussions	Scientific Series	View details
Chaos from the Big Bang to Black Holes	Janna Levin	2006‑03‑15	Colloquium	Scientific Series	View details
String Loops vs. AdS/CFT	Gordon Semenoff	2006‑03‑14	Quantum Fields and Strings	Scientific Series	View details
The chaotic evolution of Newton's universe		2006‑03‑09	Colloquium	Scientific Series	View details
Introduction to quantum gravity - Part 14	Lee Smolin	2006‑03‑08	Introduction to Quantum Gravity - 2006	Conference	View details
Introduction to quantum gravity - Part 13	Lee Smolin	2006‑03‑08	Introduction to Quantum Gravity - 2006	Conference	View details
GHZ correlations are just a bit nonlocal	Carlton Caves	2006‑03‑08	Perimeter Institute Quantum Discussions	Scientific Series	View details
Newton-Hooke algebras, non-relativistic branes and generalized pp-wave metrics	Joaquim Gomis	2006‑03‑07	Quantum Fields and Strings	Scientific Series	View details

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