Seminarium Teorii Względności i Grawitacji
2006/2007 | 2007/2008 | 2008/2009 | 2009/2010 | 2010/2011 | 2011/2012 | 2012/2013 | 2013/2014 | 2014/2015 | 2015/2016 | 2016/2017 | 2017/2018 | 2018/2019 | 2019/2020 | 2020/2021 | 2021/2022 | 2022/2023 | 2023/2024 | 2024/2025 | Strona własna seminarium
2025-05-23 (Piątek)
Alejandro Casallas Lagos (IFT UW)
The two faces of the gravitational wave signals: Insights from compact binary coalescence and core-collapse supernovae
Since the groundbreaking first detection of a gravitational wave (GW) by LIGO in September 2015, the field of GW astronomy has rapidly advanced. Improvements in the rate of confirmed events, the sensitivity and accuracy of GW interferometers, and the expansion of the LIGO-Virgo-KAGRA (LVK) detector network have opened unprecedented avenues for investigating diverse physical phenomena encoded in GW signals. In this talk, I will explore two distinct frontiers of GW signal characterization. Firstly, I will discuss methods to characterize the amplitude intensity of tensorial and non-tensorial polarization modes generated by binary systems during their inspiral phase, specifically within the framework of alternative theories of gravity. Secondly, I will present contemporary approaches to parameter estimation for GWs from core-collapse supernovae, focusing on how we decode information embedded in these burst signals using real LVK interferometric data and advanced machine learning techniques. Finally, I will highlight how these findings underscore the significant potential in our ongoing quest to detect and interpret gravitational wave signals.
2025-05-16 (Piątek)
Ilkka Mäkinen (NCBJ)
Dynamics in quantum-reduced loop gravity
Quantum-reduced loop gravity is a model of loop quantum gravity, whose simplified kinematical structure makes it possible to explore practical applications which would be very challenging, if not completely intractable to analyze within the framework of the full theory. After giving a brief introduction to the quantum-reduced model and its relation with full loop quantum gravity, we present a proposal for a Hamiltonian constraint operator governing the dynamics of the model. In contrast to Thiemann's well-known construction of the Hamiltonian constraint in loop quantum gravity, the Lorentzian part of our Hamiltonian is given by an operator representing the scalar curvature of the spatial manifold. As a concrete physical application, we study the dynamics generated by the Hamiltonian in a cosmological setting, both at the level of semiclassical effective dynamics, and in terms of numerical simulations of the time evolution of quantum states describing homogeneous and isotropic spatial geometries.
2025-04-11 (Piątek)
Jerzy Kowalski-Glikman (NCBJ and UWr)
The corner conjecture for Quantum Gravity
In my talk, I will begin by introducing the Universal Corner Algebra (UCA), a universal algebra of symmetries associated with corners (the boundaries of regions), within the context of classical General Relativity (GR). I will then argue that the UCA should play a role in Quantum Gravity similar to the role the Poincaré algebra plays in quantum field theory. Moving on to a two-dimensional example, I will explain how the UCA acquires a central extension in quantum theory and explore how the resulting representation theory of Quantum Corner Algebra (QCA) can be used to combine two regions into one. Additionally, I will demonstrate how these representations can be applied to compute the entanglement entropy of two regions and speculate on how this might be used to reconstruct the semiclassical spacetime. Finally, if time permits, I will briefly discuss the structure of QCA in 3 dimensions.
2025-04-04 (Piątek)
no seminar
2025-03-28 (Piątek)
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)
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)
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)
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)
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)
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