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

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.

Talk by Andrea Dapor

Speaker: Andea Dapor, FAU-Erlangen, Germany
Place: 241 Nicholson
Date: Tuesday November 14th
Time: 9am

Title: Coherent States in LQG: Cosmology, Black Holes and Effective Dynamics

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

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.

Seminar by Andrzej Krolak

Seminar by Andrzej Krolak

 

Strong curvature singularities 

- past and future

 

Time: 12:30 PM 

Date: March 23, 2017

Gravity Suite

 

Seminar by Lucas Fabian

Seminar by Lucas Fabian

Talk time and date:

March 21th at 11:00 AM in Nicholson 241

 

 

 

 

 

 

 

 

Title: Review / progress report on entanglement of squeezed vacua

Abstract: There is a lot of ongoing work using complex structures to study power spectrum and entanglement entropy of scalar perturbations in cosmology. I will review our general methods and explain the machinery connecting entanglement entropy, correlation function and complex structure for Gaussian states. There are some subtleties when going from finitely many degrees of freedom to infinitely many, due to unitarily inequivalent representations. A recent progress provided an elegant method of finding adiabatic vacua using an ε expansion of the complex structure, rather than going through the standard WKB approximation. This aspect is still incomplete, but I will explain the general approach.

Seminar by Lucas Fabian

Seminar by Lucas Fabian

Talk time and date:

March 20th at 1:30 AM in Nicholson 241

 

 

 

 

 

 

 

 

Title: Entanglement production at parametric resonance

Abstract: The most prominent example in cosmology is the reheating phase where one couples a test scalar matter field to the inflaton field treated as a classical source.  Our result is a generic theorem stating that the entanglement entropy associated to a detector grows linearly in time with a slope given by the Floquet exponents associated to resonant modes.

Seminar by Alec Yonika

 

 

Talk time and date:

Jan 11th at 11:30 AM in Nicholson 241

 

 

 

 

 

 

 

 

Title: Numerical Analysis of the Schwarzschild Interior

Abstract: Loop quantum cosmology (LQC) is a theory attempting to unite the fields of quantum theory and general relativity. In these unification attempts, LQC takes the continuous spacetime of general relativity and makes it discrete. This discretization yields some interesting results; namely, the emergence of finite-difference (FD) equations where partial difference equations usually present. FD equations present some opportunities for analysis that are not normally present. This opportunity is that of numerical analysis. Largely, numerical analysis of LQC schemes has been ignored. To rectify this, we present a method of analyzing LQC schemes. We take the example of the scheme presented in Corichi and Singh [1]. However, the methods presented herein may be used in the general case.