Seminars

Summer term 2019


 

Black-hole evolution from stellar collapse

Abstract: We present a local approach towards black-hole evaporation, which relies on the absence of quantum phase transition across the stellar surface. We show that this approach augmented with Bekenstein’s black-hole entropy gives the Hawking effect if the null energy condition is violated in the initial quantum-field vacuum. If otherwise, an astrophysical black hole may then be expanding, that corresponds to the anti-Hawking effect, i.e. a positive-energy radiation flows into the black hole, taking its origin far away from the event horizon. This quantum process is reverse to the Hawking effect, as the latter is described by a negative-energy influx nearby the horizon, which goes over to a positive-energy outflux in the far-horizon region. We also provide examples of quantum vacua well-known in the literature, which give rise to both quantum effects from stellar collapse.

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Canonical quantization of minisuperspace models with variational symmetries

Abstract: In this talk I will describe how the symmetries of the minisuperspace action are used to integrate the system at the classical and quantum level. For the latter case, we use the canonical quantisation and impose the symmetries as operators on the wave function together with the constraints. This leads to a selection rule which prevents their simultaneous imposition on the wave function and consequently to the choice of subalgebras. Some of them lead to the classical solution but there are cases where we obtain quantum corrections. These, in the Bohmian interpretation we used, are indicated when the quantum potential in the quantum Hamilton–Jacobi equation does not vanish. I will discuss some examples of physical interest.

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The Cosmological Constant and the mass of the Local Group

Abstract: The two-body problem of M31 and the Milky Way (MW) galaxies with a cosmological constant background is studied, with emphasis on the possibility that they experienced past encounters. By implementing the initial conditions of the big bang and the last measured relative distance and velocities (i.e. the Timing Argument), it is shown that if M31 and the MW had more than one encounter then the mass of the Local Group (LG) would be a few times higher than if there had been no encounters. Past encounters are possible only for non-zero transverse velocity, and their viability is subject to observations of the imprints of such near collisions. While it has been previously shown that the presence of the cosmological constant requires a higher mass for the LG, here, using a recent Gaia - based measurement of the transverse velocity the derived LG mass is (3.36 +1.14 -0.7) · 10^(12) M☉ with no cosmological constant or (4.54 +1.2 -0.75) · 10^(12)M☉ with a cosmological constant background. If the LG has had one past encounter, LG mass is (9.70 +2.19 -1.55) · 10^(12) M☉ or (9.99 +2.22 -1.58) · 10^(12) M☉ with a cosmological constant background. Modified Newtonian Dynamics (MOND) is also studied, as the accelerations of the Local Group are fully in the deep MOND regime. MOND yields the order of magnitude for the expected baryonic mass only after one past encounter, assuming MOND does not include dark matter. While we only consider the LG as two point masses, our calculations provide a benchmark for future work with simulations to test the effect of the finite size of galaxies and tidal fields due to the neighbouring structures. This model can be also used to test screening mechanisms and alternative theories of gravity.

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On surface terms and double layers in quadratic gravity

Abstract: The talk consists of three parts.
In the first part it is demonstrated using the simple example of the spherically symmetric Weyl + Einstein gravity, that the junction conditions in the presence of the double layer admit the appearance of the arbitrary function determined by the bulk solutions and, on the other hand, the very stringent requirements are imposed on the structure of the matching surface, namely, its extrinsic curvature tensor has to be zero.
In the second part the junction conditions on the singular hypersurface (Israel equations) are derived from the least action principle.
And, in the third part, the same procedure is applied for the case of the quadratic gravity. It is shown how the abovementioned “unusual” features can be implemented quite naturally in the least action principle.

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How to construct wave packets with complete classical–quantum correspondence in quantum cosmology

Abstract: I discuss “canonical” wave packets in quantum cosmology which exhibit complete classical-quantum correspondence. I will present a prescription for initial conditions that leads to the classical description. I also study the situation from de-Broglie Bohm interpretation of quantum mechanics and show that the corresponding Bohmian trajectories are in complete agreement with the classical counterparts. As an interesting application, I will apply this method to the Schrödinger equation and obtain wave functions with complete classical-quantum correspondence for a large class of one-dimensional potentials.

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A covariant treatment of Lorentzian spacetimes in the Einstein–Hilbert truncation

Abstract: The perturbative non-renormalizability of pure Quantum Einstein Gravity at a 2-loop level signifies the need of a new treatment for the theory. Asymptotically Safe Gravity is a newly developed field of study where one using non-perturbative methods tries to prove the Ultraviolet completion of the theory within the framework of Quantum Field Theory. Such a completion is shown with the existence of a non-Gaussian fixed point at high energies, during the study of the renormalization group trajectories. Here, the tools essential to generate such trajectories for causal (Lorentzian) spacetimes are established. Furthermore, a careful treatment of the gravitational partition functional over foliatable spacetimes in a covariant manner takes place. Finally, employing a specific approximation (Einstein–Hilbert truncation) we bring the Functional Renormalization Group Equation in a solvable form, which provides evidence for the existence of the non-Gaussian fixed point.

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Affine Coherent State Quantization: A Brief Introduction and Some Applications

Abstract: I will go through the basics of affine coherent state quantization (ACSQ), and illustrate the advantages and drawbacks of ACSQ by discussing some examples, including the Lemaître–Tolman–Bondi model.

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Date Time Speaker Topic Room
April 2, 2019 12:00 Viacheslav Emelyanov
(KIT, Karlsruhe)
Black-hole evolution from stellar collapse Konferenzraum 1 (Neubau)
April 9 12:00 Adamantia Zampeli
(Charles University, Prague)
Canonical quantization of minisuperspace models with variational symmetries Konferenzraum 1 (Neubau)
April 23 12:00 Yi-Fan Wang
(Uni Cologne)
Dynamically assisted Schwinger effect Konferenzraum 1 (Neubau)
April 30 12:00 Tatevik Vardanyan
(Uni Bonn)
Wheeler–DeWitt quantum cosmology of Bianchi II model Konferenzraum 1 (Neubau)
May 14 12:00 David Chay Benisty
(BGU Negev / GU Frankfurt)
The Cosmological Constant and the mass of the Local Group Konferenzraum 1 (Neubau)
May 21 12:00 Victor Berezin
(INR RAS, Moscow)
On surface terms and double layers in quadratic gravity Konferenzraum 1 (Neubau)
June 4 12:00 Pouria Pedram
(IAU, Tehran)
How to construct wave packets with complete classical–quantum correspondence in quantum cosmology Konferenzraum 1 (Neubau)
June 6 10:00 (c.t.) Dimitrios Gkiatas
(Uni Bonn; Master Colloquium)
A covariant treatment of Lorentzian spacetimes in the Einstein–Hilbert truncation Seminarraum 1, BCTP
June 25 12:00 Benjamin Bahr
(Uni Hamburg)
Background–independent renormalization in spin foam quantum gravity Konferenzraum 1 (Neubau)
July 2 12:00 Tim Schmitz
(Uni Cologne)
Affine Coherent State Quantization: A Brief Introduction and Some Applications Konferenzraum 1 (Neubau)
September 16 14:00 Branislav Nikolic
(Uni Cologne; disputation)
TBA TBA

 


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