Wednesday, March 14, 2018
Sunday, December 10, 2017
Skype Seminar by
Klaus Liegner
"Hamiltonian Renormalisation"
We study the question whether it is possible to reformulate the
Wilsonian renormalisation group non-perturbatively directly at the
operator (Hamiltonian) level. Hamiltonian renormalisation would be the
natural route to follow if one had easier access to an interacting
Hamiltonian operator rather than to a path integral, at least in the
presence of UV and/or IR cut-off, which is generically the case in
complicated gauge theories such as General Relativity. Our guiding
principle for the definition of the direct Hamiltonian renormalisation
group is that it results in the same continuum theory as the covariant
(path integral) renormalisation group. We will investigate this direct
Hamiltonian Renormalisation for the case of the free massive quantum
scalar field and point out its necessity in a concrete cosmological
example for Quantum Gravity.Date: Dec 11, 2017
Time: 9 AM
255 Nicholson
Tuesday, December 5, 2017
Visit by Andrzej Krolak
Prof. Krolak from Institute of Mathematics, Polish Academy of Sciences at Warsaw is visiting us from Nov 27-Dec 6, 2017. Prof. Krolak has made very seminal contributions to our understanding of strength of singularities, and various aspects of theoretical gravity and gravitational waves. He is the head of the Polish gravitatioanal wave community involved with Virgo gravitational wave detector.
You are welcome to discuss with Andrzej in room 255.
Friday, November 10, 2017
Talk by Andrea Dapor
Place: 241 Nicholson
Date: Tuesday November 14th
Time: 9am
Title: Coherent States in LQG: Cosmology, Black Holes and Effective Dynamics
Monday, August 28, 2017
Seminar by Prof. Christian Fleischhack
Seminar by
Prof. Christian Fleischhack
Symmetries in loop quantum gravity
Date: Aug 30, 2017
Time: 11:30 AM
Gravity Suite
Friday, May 12, 2017
Talk by Raul Carballo-Rubio
Seminar by Raul Carballo-Rubio
Talk time and date:
May 17th at 11:00 AM in Nicholson 241
Title: Exponential decay of black holes into white holes
Abstract: In recent years, it has been proposed by different authors that non-perturbative quantum gravity effects may turn black holes into white holes. To evaluate the characteristic time scale of this transition, a theory of quantum gravity that assigns probabilities to geometric interpolations between black hole and white hole geometries is needed. In this talk, I will explain the results that are obtained in a truncation of the problem that assigns probabilities à la Euclidean quantum gravity to a reduced set of interpolating geometries. I will show how an exact exponential decay law is found, extract the characteristic time scale that follows from it, and discuss the astrophysical relevance of this calculation.
Wednesday, March 22, 2017
Seminar by Andrzej Krolak
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