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A workshop in honour of Bill Unruh on occasion of his 70th birthday.
Registration for this event is now closed.
- Valeri Frolov, University of Alberta
- Stephen Fulling, Texas A&M University
- Masahiro Hotta, Tohoku University
- Ted Jacobsen, University of Maryland
- Raymond Laflamme, Institute for Quantum Computing
- George Matsas, Instituto de Física Teórica, Universidade Estadual Paulista
- Jonathan Oppenheim, University College London
- Marek Radzikowski, American University of Afghanistan
- Benni Reznik, Tel Aviv University
- Ralf Schuetzhold, Universitat Duisburg-Essen
- Robert Wald, University of Chicago
- Silke Weinfurtner, University of Nottingham
- Bruno Arderuci, University of British Columbia
- Kaca Bradonjic, Wellesley College
- Bianca Dittrich, Perimeter Institute
- Valeri Frolov, University of Alberta
- Stephen Fulling, Texas A&M University
- Henrique Gomes, Perimeter Institute
- Stephen Green, Perimeter Institute
- Masahiro Hotta, Tohoku University
- Ted Jacobsen, University of Maryland
- Farbod Kamiab, Perimeter Institute
- Achim Kempf, Perimeter Institute & University of Waterloo
- Raymond Laflamme, Institute for Quantum Computing
- Morgan Lynch, University of Wisconsin-Milwaukee
- Eduardo Martin-Martinez, Perimeter Institute & University of Waterloo
- George Matsas, Instituto de Física Teórica, Universidade Estadual Paulista
- Robert Myers, Perimeter Institute
- Jonathan Oppenheim, University College London
- Eric Poisson, University of Guelph
- Marek Radzikowski, American University of Afghanistan
- Benni Reznik, Tel Aviv University
- Ralf Schuetzhold, Universitat Duisburg-Essen
- Barak Shoshany, Perimeter Institute
- Vasudev Shyam, Perimeter Institute
- Lee Smolin, Perimeter Institute
- Rafael Sorkin, Perimeter Institute
- Fumika Suzuki, University of British Columbia
- Bill Unruh, University of British Columbia
- Robert Wald, University of Chicago
- Silke Weinfurtner, University of Nottingham
- Steven Weinstein, Perimeter Institute * University of Waterloo
- Yasaman Yazdi, Perimeter Institute
- Nosiphiwo Zwane, Perimeter Institute
Thursday, August 13, 2015
Time |
Event |
Location |
8:30 – 9:00am |
Registration |
Reception |
9:00 – 9:05am |
Silke Weinfurtner, University of Nottingham |
Bob Room |
9:05 – 10:00am |
Robert Wald, University of Chicago |
Bob Room |
10:00 – 10:30am |
Coffee Break |
Bistro – 1^{st} Floor |
10:30 – 11:30am |
Jonathan Oppenheim, University College London |
Bob Room |
11:30 – 12:30pm |
Marek Radzikowski, American University of Afghanistan |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 3:00pm |
Stephen Fulling, Texas A&M University |
Bob Room |
3:00 – 4:00pm |
Raymond Laflamme, Institute for Quantum Computing |
Bob Room |
4:00 – 4:10pm |
Conference Photo |
TBA |
4:10 – 4:30pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:30 – 5:30pm |
Silke Weinfurtner, University of Nottingham |
Bob Room |
5:30 – 6:00pm |
Wilhelm E. Nassau |
Bob Room |
7:00 – 9:00pm |
Banquet |
Bistro – 2^{nd} Floor |
Friday, August 14, 2015
Time |
Event |
Location |
9:00 – 10:00am |
Valeri Frolov, University of Alberta |
Bob Room |
10:00 – 10:30am |
Coffee Break |
Bistro – 1^{st} Floor |
10:30 – 11:30am |
Masahiro Hotta, Tohoku University |
Bob Room |
11:30 – 12:30pm |
George Matsas, |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 3:00pm |
Ted Jacobson, University of Maryland |
Bob Room |
3:00 – 4:00pm |
Benni Reznik, Tel Aviv University |
Bob Room |
4:00 – 4:30pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:30 – 5:30pm |
Ralf Schuetzhold, Universitat Duisburg-Essen |
Bob Room |
5:30 – 6:00pm |
Discussion |
Bob Room |
Valerie Frolov, University of Alberta
Mass gap for black hole formation in higher derivative and ghost-free gravity
The problem of the gravitational collapse of small mass in the higher derivative and ghost free theories of gravity is discussed. It will be demonstrated how higher derivative and non-local modifications of gravity equations regularizes static and dynamical solutions. Boosting a static solution of the linearized equations for the gravitational potential of a point mass we obtain a solution for the field of the ultra-relativistic source (gyraton). Using the latter we construct solutions for the collapsing spherical (thin and thick) null shell. By analysing the obtained solutions we demonstrate that for small enough value of the mass M an apparent horizon is not formed for the gravitational collapse of small mass in the higher-derivative and ghost free theories of gravity. We demonstrate that this “mass gap” property is connected with the presence of the UV cut-off in such theories.
Stephen Fulling, Texas A&M University
Acceleration Radiation: The Prophet and the Heretics
I review the contentious question, "Does a uniformly accelerated detector radiate?" As Audretsch and Muller pointed out long ago, this is partly a semantic dispute. The
talk draws on recent discussions with Alex Calogeracos and George Matsas.
Masahiro Hotta, Tohoku University
Consciousness Does Not Cause Quantum Zeno Effect
Discussion
On the partner particles for black hole evaporation
Due to the linearity of the field equations and the resulting bilinear structure of the Hamiltonian, quantum radiation effects such as black hole evaporation or particle creation in an expanding universe are typically described as (squeezing) processes where particles are created in pairs.
Here, we address the following question: given a mode (e.g., wave-packet) corresponding to a created particle (e.g., as part of Hawking radiation), what is its partner, i.e., the other particle of the pair?
Lattice gauge theories with cold atoms
Can high energy physics can be simulated by low-energy, nonrelativistic, many-body systems, such as ultracold atoms? Ultracold atomic systems lack the type of symmetries and dynamical properties of high energy physics models: in particular, they do not manifest local gauge invariance nor Lorentz invariance, which are crucial properties of the quantum field theories which are the building blocks of the standard model of elementary particles.
Fun with ideal plasmas
I will sketch a few interesting phenomena involving ideal plasmas, including helicity conservation, frozen flux, the Blandford-Znajek mechanism, and self-confined Poynting jets, using the language of differential forms.
On the Observability of the Unruh Effect
This year marks the 40’th anniversary of the Unruh effect as described at the first Marcel Grossmann meeting in 1975. We revisit it with emphasis on the observability issue which might be a concern at first sight, since the linear acceleration needed to reach a temperature 1 K is of order 10^20 m/s^2 . We close the talk by emphasizing that the Unruh effect does not require any verification beyond that of relativistic free field theory itself. The Unruh effect lives among us.
Consciousness Does Not Cause Quantum Zeno Effect
The quantum Zeno effect is often very controversial in the context of consciousness problems.
Frequent direct measurements of a quantum system freeze its time evolution.
Then what happes if an observer continuously watches a Schrodinger's cat from the start of the experiment?
Naively this looks like a yes-no measurement of a unstable atom decay, which emits a gamma ray as a trigger of the cat execution.
Mass gap for black hole formation in higher derivative and ghost-free gravity
The problem of the gravitational collapse of small mass in the higher derivative and ghost free theories of gravity is discussed. It will be demonstrated how higher derivative and non-local modifications of gravity equations regularizes static and dynamical solutions. Boosting a static solution of the linearized equations for the gravitational potential of a point mass we obtain a solution for the field of the ultra-relativistic source (gyraton). Using the latter we construct solutions for the collapsing spherical (thin and thick) null shell.
The Third Man, Exciting Events in Post War Vienna
Hydrodynamic simulations of rotating and non-rotating black holes
In 1981 Bill discovered an analogy between the propagation of fields in the vicinity of
astrophysical black holes and the that of small excitations in fluids. He postulated that this
analogy allows one to test, challenge and verify, in tabletop experiments, the elusive
processes of black hole mass and angular momentum loss. Indeed, 34 years later
analogue gravity experiments are carried out all over the world to implement his idea.
Experimental Quantum Error Correction
The last decade has seen the impressive development of quantum information science, both in theory and in experiment. There are many measures that can be used to assess the achievements in the field: new algorithms, new applications and larger quantum processors, to name a few. The discovery of quantum algorithms has demonstrated the potential power of quantum information.
As pointed out by Bill some years ago, to realize this potential requires the ability to overcome the imprecision and imperfection inherent in physical systems.
Pages
Scientific Organizers:
Matt Choptuik, University of British Columbia
Ralf Schuetzhold, Duisburg-Essen University
Silke Weinfurtner, University of Nottingham