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Wydział Fizyki UW > Badania > Seminaria i konwersatoria > Seminarium Teorii Względności i Grawitacji
2025-04-04 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon

no seminar

2025-03-28 (Piątek)
Zapraszamy na spotkanie o godzinie 11:15  Calendar icon
Arman Taghavi-Chabert (Politechnika Łódzka)

Perturbations of Fefferman spaces over (almost) CR manifolds

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
2025-03-21 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Cong Zhang (BNU Beijing and FAU, Erlangen)

Black Holes and Covariance in Effective Quantum Gravity

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.
2025-03-14 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Tomasz Taylor (Northeastern University and IFT UW)

De S-matrix

I will construct the S-matrix describing elementary particles scattering in global de Sitter spacetime.
2025-03-07 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Marek Lewicki (IFT UW)

Search for cosmological phase transitions through their gravitational wave signals

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.
2025-02-28 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Maciej Ossowski (IFT UW)

Axis and conicity in the presence of the NUT parameter

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.
2025-01-24 (Piątek)
Zapraszamy na spotkanie o godzinie 11:15  Calendar icon
Antony Valentini (Imperial College London)

Beyond the Born rule in quantum gravity

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
2025-01-17 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Maciej Dunajski (DAMTP, University of Cambridge)

Integrability of quantum dots

2025-01-10 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Luca Cafaro (IFT UW)

Stellar collapse with pressure in effective loop quantum gravity

Recently, a substantial amount of work has been conducted on the spherically symmetric dust collapse within the framework of effective loop quantum gravity. I will outline those results as well as explore more general collapse scenarios with pressure. Numerical investigations show that the shell-focusing singularity characterizing the end state of any classical stellar collapse is here resolved by quantum gravitational effects and replaced by a bounce of the star. However, they also show that shell-crossing singularities remain a general feature of these models and that the inclusion of pressure does not alter the qualitative picture emerging from semiclassical models of inhomogeneous dust collapse.
2024-12-20 (Piątek)
Zapraszamy do sali 1.40, ul. Pasteura 5 o godzinie 11:15  Calendar icon
Anna Liu (The Chinese University of Hong Kong)

Exploring the Universe with Gravitational Waves: From Lensing to Testing General Relativity

Since the first detection of gravitational waves in 2015, the LIGO-Virgo-KAGRA detectors observed over 90 signals, a number expected to triple by the end of the current observing run. These detections have opened a new window into the universe, enabling groundbreaking tests of gravity in the strong-field regime and offering insights into the distribution of matter in the universe. Yet, extracting the full physics potential from gravitational wave signals remains a challenge.Gravitational lensing is emerging as a powerful tool in gravitational-wave astronomy, but detecting and interpreting lensed gravitational waves presents unique challenges due to weaker signals, limited detectors, and the complex nature of gravitational-wave sources. In this talk, I will outline recent progress in identifying and analyzing lensed gravitational waves, highlight how lensing can mimic or obscure key physical signatures, and discuss the implications for astrophysics and cosmology. I will also touch on how unaccounted-for lensing effects can bias tests of general relativity, and provide a brief overview of recent advancements in performing these tests with gravitational waves. These developments underscore the exciting potential of gravitational-wave astronomy to uncover new physics and deepen our understanding of the universe.
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