of the Institute of Theoretical Physics

- March 1, 2022
- Carter constant, photon region and black hole shadow in a general axially symmetric stationary spacetime in plasma
*Dr. Barbora Bezděková*- ITP
Problem of light rays propagating around compact relativistic objects (e.g. a black hole) is usually solved with a vacuum background. However, in real astrophysical applications a medium (plasma) surrounding a vicinity of the black hole has to be considered. Studies describing ray trajectories around relativistic objects in plasma typically focus on particular examples and discuss concrete spacetime and plasma effects. This problem can be effectively solved as the separation of the Hamilton-Jacobi equation. To be able to find a solution of such system, a Carter constant has to exist. In our work, we state general conditions for both the axially symmetric stationary metric and plasma density which guarantee that the Carter constant exists. General expressions for a photon region and black hole shadow for light rays penetrating around an axially symmetric stationary object in plasma are further derived. Moreover, the obtained general relations are applied to find the boundary of photon region and shadow for particular examples, such as Kerr metric or Melvin metric.

Recording:

- March 8, 2022
- Gravity of static thin discs: on Laplace transform of Bessel-function products
*Petr Kotlařík*- ITP
Thin discs are important structures in astrophysics. Whether treated in Newton's theory or in general relativity, in the static and axially symmetric case they generate potential determined by the Laplace equation. Though clear in principle, its solution is only known explicitly for several surface-density profiles. We show how to derive close-form potentials for the densities composed of powers of the radius. The method, due to Conway (2000), rests on the Laplace transform of products of Bessel functions. Finite as well as infinite discs will be included, possibly empty at their centre (i.e. annular).

Recording:

- March 15, 2022
- Asymptotic characterization of spacetimes with positive cosmological constant in all dimensions
*Dr. Carlos Peón-Nieto*- ITP
- We review the formalisms which allow to pose an asymptotic
Cauchy problem in all dimensions for Lambda positive vacuum spacetimes: the Friedrich conformal field equations in four spacetime dimensions and the Fefferman-Graham formalism in higher dimensions. We employ the initial data to asymptotically characterize Kerr-de Sitter and related spacetimes.

Recording:

- March 22, 2022
- How does an Unruh-DeWitt detector respond near an extremal black hole?
*Dr. Aindriú Conroy*- ITP
There is no well-defined notion of a particle in quantum field theory in curved spacetime due to the lack of global symmetries. The standard procedure in quantum field theory is to treat fields rather than particles as the fundamental object of interest. Nevertheless, in a seminal 1976 paper by W. G. Unruh, an operational meaning was given to the particle concept by examining the absorption and emission of field quanta by a two-level atom. This is the so-called Unruh-DeWitt detector and, in this operational sense, we say a particle is what a particle detector detects! Computing the response of an Unruh-DeWitt detector in black hole spacetimes is technically challenging – a fact which has largely limited the literature to stationary detectors. In this talk, we consider the response of an Unruh-DeWitt detector near an extremal charged black hole, modelling the near-horizon region of this extremal spacetime by the Bertotti-Robinson spacetime. The advantage of employing the Bertotti-Robinson limit is that the two-point functions for a massless scalar field are obtainable in closed form for a number of quantum states of interest, allowing us to explore the full gamut of the parameter space for a broader range of stationary and non-stationary trajectories. Particular attention will be paid to the thermalization of the detector, the anti-Unruh effect, and the anti-Hawking effect. If time allows, I will then move on to discussing some unpublished results on the open question of how to define surface gravity and temperature in dynamical spacetimes by shifting focus to a detector in a cosmological spacetime with an evolving horizon.

Recording:

- March 29, 2022
- Uniqueness of extremal isolated horizons and their identification with horizons of type D black holes
*Dávid Matejov*- Mathematical Institute of the Czech Academy of Sciences
We investigate axisymmetric extremal isolated horizons (EIHs). They are described by an induced metric characterized by a single function. This function is subject to particular constraints following from Ricci identities in the Einstein-Maxwell theory. At first, we restrict our attention to asymptotically flat spacetimes. In the extremal case the solution is unique and depends on 5 independent parameters with direct geometrical or physical interpretation. The solution is possible to identify with extremal horizons in exact electrovacuum Plebański-Demiański spacetimes, that are all (double aligned) black holes of algebraic type D without a cosmological constant. Several interesting subclasses include accelerating extremely charged Reissner-Nordström black hole (C-metric) or extremal accelerating Kerr-Newman. As a natural extension, I will generalize the previous results to asymptotically (anti-) de Sitter spacetimes with non-zero cosmological constant and identify the EIHs geometry with the corresponding horizon geometry of a black hole in a special case of the famous Kerr-Newman-NUT-(A)dS metric.

Recording:

- April 5, 2022
- A look at the geometry of the 5-dimensional charged rotating black hole
*doc. Igor Khavkine*- Department of Algebra, Geometry and Mathematical Physics, Institute of Mathematics of the Czech Academy of Sciences
The Einstein-Maxwell equations for a charged rotating black hole in 5 dimensions with two equal-magnitude angular momenta has been reduced to a system of non-linear ODEs and studied numerically by Kuntz et al. We study some geometric aspects of these solutions, confirming that they have regular horizon and null infinity. In addition, we rule out the possibility that the Weyl tensor of these spacetimes has special algebraic type in the bulk, while verifying the "geometric horizon" conjecture by showing that the Weyl tensor reduces to Type II on the horizon and to Type D on the bifurcation sphere.

Recording:

- April 12, 2022
- Obscuring tori in active galactic nuclei: observations and simulations
*Prof. Elena Bannikova*- Institute of Radio Astronomy, National Academy of Sciences of Ukraine, V.N. Karazin Kharkiv National University
The recent paradigm of AGNs is to explain the differences between type I and II by the different orientation of an optically thick torus relative to the observer. The dynamics of the dusty clouds in such a torus was unclear due to the relative small scale of these objects. The unprecedented resolution of ALMA has recently allowed us to improve significantly the information about dynamics of clouds in the obscuring tori for some AGNs. On this ground, we present our N-body simulations of the toroidal structure of clouds moving around a supermassive black hole (SMBH). We also apply ray-tracing algorithm to take into account effects of obscuration of the central engine by the clouds. As the final result, we obtain the velocity and temperature maps which allow us to interpret the VLTI and ALMA observations. We also estimate the SMBH masses in the nearest Sy2 galaxies and provide a new explanation of the counter-rotation of the torus in NGC 1068.

Recording:

- April 19, 2022
- Interplay between spectral energy distribution and spectral line profiles in the context of gappy accretion discs
*Marcel Štolc*- Prague Relativistic Astrophysics group, Astronomical Institute of the Czech Academy of Sciences
Both spectral energy distribution of the continuum and the spectral lines offer a way to measure and model parameters of the inner and outer region of the black hole accretion disc. We introduce a perturbative term in the orbital plane of the accretion disc and assume different scenarios pointing towards a gappy accretion disc setup. Studying the radiative effects of the perturber, we discuss the application of the methods used to constrain the parameters of the system.

Recording:

- April 26, 2022
- EMRI from canonical perturbation theory
*Lukáš Polcar*- Prague Relativistic Astrophysics group, Astronomical Institute of the Czech Academy of Sciences
By employing the methods of canonical perturbation theory we can find an approximate analytical solution to a Hamiltonian system. We applied this approach to the geodesic equation in the spacetime describing a black hole superposed with a ring-like source. The solutions to the geodesic equation are then used to compute gravitational wave fluxes using the quadrupole formalism. This allows us to compute the extreme mass ratio inspiral (EMRI) in our spacetime by adiabatically evolving the constants of motion which parametrize the analytical solution of the geodesic equation.

Recording:

- May 3, 2022
- Higher-dimensional Robinson-Trautman spacetimes coupled to conformally invariant electrodynamics
*David Kokoška*- Department of Algebra, Geometry and Mathematical Physics, Institute of Mathematics of the Czech Academy of Sciences
We present the complete family of higher-dimensional Robinson-Trautman (RT) spacetimes sourced by (aligned) conformally invariant non-linear electrodynamics with an arbitrary cosmological constant. We also briefly compare the obtained results with the known ones in the case of RT spacetimes with linear Maxwell field in higher dimensions. Subsequently, some properties of a static subclass are also investigated. It contains dyonic black holes with various horizon geometries and different asymptotics. Finally, we discuss the special case of stealth solutions.

Recording:

- May 10, 2022
- Holographic reconstruction of asymptotically flat spacetimes
*Finnian Gray*- Perimeter Institute for Theoretical Physics, Waterloo, Ontario, Canada
We present a "holographic" reconstruction of bulk spacetime geometry using correlation functions of a massless field living at the "future boundary" of the spacetime, namely future null infinity I+. It is holographic in the sense that there exists a one-to-one correspondence between correlation functions of a massless field in four-dimensional spacetime M and those of another massless field living in three-dimensional null boundary I+. The idea is to first reconstruct the bulk metric by "inverting" the bulk correlation functions and re-express the latter in terms of boundary correlators via the correspondence. This effectively allows asymptotic observers close to I+ to reconstruct the deep interior of the spacetime using only correlation functions localized near I+.

Recording:

- May 17, 2022
- Self-intersecting marginally outer-trapped surfaces in black holes
*Kam To Billy Chan*- Department of Physics and Physical Oceanography, Memorial University, St. John’s, Newfoundland and Labrador, Canada
The advent of gravitational wave detectors had facilitated a constant stream of black hole merger observations. Despite this, black hole mergers are not fully understood. The details of the two apparent horizons becoming one is unclear due to the non-linear nature of the merger process. Recent numerical work has shown that there is an appearance of self-intersecting marginally outer-trapped surfaces (MOTS) during the black hole merger [Pook-Kolb et. al. arXiv:1903.05626]. Following papers have found similarly behaving MOTS in a simpler and static scenario, that of a Schwarzschild black hole, where a seemingly infinite number of self-intersecting MOTS were found [Booth et. al., arXiv:2005.05350]. This talk introduces new phenomena that occur in the presence of an inner horizon. For Reissner-Nordstrom and Gauss-Bonnet black holes, we find that the maximum number of self-intersections becomes finite with the MOTS parameter space deeply dependent on the interior structure of the black hole and in particular the stability of the inner horizon [Hennigar et. al., arXiv:2111.09373].

Recording:

- June 10, 2022
- FRIDAY FROM 11:00
- The strong cosmic censorship conjecture: The fall and the rise
*Dr. Sumanta Chakraborty*- School of Physical Sciences, Indian Association for the Cultivation of Science (IACS), Kolkata
- Deterministic nature of general relativity abhors existence of Cauchy horizons through the strong cosmic censorship conjecture. I will first discuss the recent claims, invalidating the conjecture, and then I will describe how it is again restored to its former glory.

Recording:

- current semester
- fall 2023
- spring 2023
- fall 2022
- spring 2022
- fall 2021
- spring 2021
- fall 2020
- spring 2020
- fall 2019
- spring 2019
- fall 2018
- spring 2018
- fall 2017
- spring 2017
- fall 2016
- spring 2016
- fall 2015
- spring 2015
- fall 2014
- spring 2014
- fall 2013
- spring 2013
- fall 2012
- spring 2012
- fall 2011
- spring 2011
- fall 2010
- spring 2010
- fall 2009
- spring 2009
- fall 2008
- spring 2008
- fall 2007
- spring 2007
- fall 2006
- spring 2006
- fall 2005
- spring 2005
- fall 2004
- spring 2004
- fall 2003
- spring 2003
- spring 2002
- fall 2001
- spring 2001
- fall 2000
- spring 2000
- fall 1999
- spring 1999
- fall 1998
- spring 1998
- fall 1997

© September 26, 2022; Oldřich Semerák

© February 12, 2024; generated by application