Zapraszamy na spotkanie o godzinie 11:15

Arman Taghavi-Chabert (Politechnika Łódzka)
In 1976, Charles Fefferman constructed, in a canonical way, a Lorentzian conformal structure on a circle bundle over a given strictly pseudoconvex Cauchy-Riemann (CR) manifolds of hypersurface type. It is also known, notably through the work of Sir Roger Penrose and his associates, and that of the Warsaw group led by Andrzej Trautman, that CR three-manifolds underlie Einstein Lorentzian four-manifolds whose Weyl tensors are said to be algebraically special. I will show how these two perspectives are related to each other, by presenting modifications of Fefferman’s original construction, where the conformal structure is "perturbed" by some semi-basic one-form, which encodes additional data on the CR three-manifold.Metrics in such a perturbed Fefferman conformal class whose Ricci tensor satisfies certain degeneracy conditions are only defined off sections of the Fefferman bundle, which may be viewed as "conformal infinity". The prescriptions on the Ricci tensor can then be reduced to differential constraints on the CR three-manifold in terms of a "complex density" and the CR data of the perturbation one-form. One such constraint turns out to arise from a non-linear, or gauged, analogue of a second-order differential operator on densities, closely related to so-called BGG operators. A solution thereof provides a criterion for the existence of a CR function and, under certain conditions, for CR embeddability. Our setup allows us to reinterpret previous works by Lewandowski, Nurowski, Tafel, Hill, and independently, by Mason.Time permitting, I will discuss the higher-dimensional story.This talk is based on arXiv:2303.07328 and arXiv:2309.16986. Broadcast in room 1.40
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15

Cong Zhang (BNU Beijing and FAU, Erlangen)
The longstanding issue of general covariance in effective models of quantum gravity is addressed, which arises when canonical quantum gravity leads to a semiclassical model described by an effective Hamiltonian constraint. In the context of spherically symmetric models, general covariance is precisely formulated into a set of equations, leading to the necessary and sufficient conditions for ensuring covariance. With the aid of these conditions, we derive the equations for the effective Hamiltonian constraint. The equations yield two candidates for effective Hamiltonian constraints dependent on a quantum parameter. The resulting quantum modified black hole spacetimes are analyzed. Our models show improvement by casting off the known limitations of previous works with similar results.
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15

Tomasz Taylor (Northeastern University and IFT UW)
I will construct the S-matrix describing elementary particles scattering in global de Sitter spacetime.
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15

Marek Lewicki (IFT UW)
We are currently witnessing the dawn of a new era in astrophysics and cosmology, started by the LIGO/Virgo observations of Gravitational Waves(GWs). Recently, also the detection of a stochastic background of GWs at very low frequencies was announced by the Pulsar Timing Array collaborations. Thanks to the fact that these signals propagate freely from the moment of their production they open a new window into processes taking place in the first moments of our Universe. Before we had to rely on photon based signals which could only propagate freely since the Universe became transparent due to recombination when it was about 370k years old. In this talk, I will discuss how GW signals are produced in cosmological phase transitions and examine the possible implications of current data for this source as well as the prospectsfor detection in the upcoming next generation of experiments.
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15

Maciej Ossowski (IFT UW)
In a spacetime where the Misner string is present - due to the NUT parameter or a time-shift - the axis of rotation is singular and cannot be a part of the spacetime manifold. I will discuss a geometric definition of the axis, the corresponding axial symmetry and the associated measure of the conical singularity - namely the conicity. It turns out that in the generic case, the conicity is necessarily observer-dependent and in particular in the spacetime with a NUT parameter there exists an observer measuring no difference of conicities for both parts of the axis. Consequently, any calculation concerning the Misner string - e.g. black holes thermodynamics or acceleration - should take the observer-dependency into account. The definition of conicity correctly reproduces the previously known results for Plebański-Demiański spacetimes.Based on a joint work with Ivan Kolář and Pavel Krtouš.
Zapraszamy na spotkanie o godzinie 11:15

Antony Valentini (Imperial College London)
We have recently developed a new understanding of probability in quantum gravity. In this talk we provide an overview of this new approach and its implications. Adopting the pilot-wave formulation of quantum physics, we argue that there is no Born rule at the fundamental level of quantum gravity with a non-normalisable Wheeler-DeWitt wave function. Instead, the universe is in a perpetual state of ‘quantum nonequilibrium’. Dynamical relaxation to the Born rule can occur only after the early universe has emerged into a semiclassical or Schrödinger approximation, with a time-dependent and normalisable wave function. We also show that quantum-gravitational corrections to the Schrödinger approximation can generate tiny deviations from the Born rule. The possibility of observing these effects is discussed. [Reference: A. Valentini, Beyond the Born rule in quantum gravity, Found. Phys. 53, 6 (2023).] Broadcast in room 1.40