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By solving a nonlinear Klein-Gordon equation in Kerr geometry, we uncover new phenomena and key characteristics of quantized vortices in quantum fluids near a Kerr black hole. The formation of these vortices induces rotational or turbulent…

广义相对论与量子宇宙学 · 物理学 2025-12-04 Shilong Jin , Xiaofei Zhao , Yong Zhang , Chi Xiong

Fluid discs and tori around black holes are discussed within different approaches and with the emphasis on the role of disc gravity. First reviewed are the prospects of investigating the gravitational field of a black hole--disc system by…

天体物理学 · 物理学 2011-07-19 V. Karas , J. -M. Hure , O. Semerak

We derive a viscosity from gravitational instability in self-gravitating accretion disks, which has the required properties to account for the observed fast formation of the first super-massive black holes in highly redshifted quasars and…

天体物理学 · 物理学 2009-11-11 Wolfgang J. Duschl , Markward Britsch

In the gravitational field of a Schwarzschild-like black hole, particles infalling from rest at infinity, and black hole "wind" particles with relativistic velocity leaking radially out from the nominal horizon, both have the same magnitude…

广义相对论与量子宇宙学 · 物理学 2023-01-03 Stephen L. Adler

Stellar-mass black holes offer what is perhaps the best scenario to test theories of gravity in the strong-field regime. In particular, f(R) theories, which have been widely discuss in a cosmological context, can be constrained through…

宇宙学与河外天体物理 · 物理学 2012-12-13 Daniela Pérez , Gustavo E. Romero , Santiago E. Perez Bergliaffa

Quasi-periodic oscillations of high density thick accretion disks orbiting a Schwarzschild black hole have been recently addressed as interesting sources of gravitational waves. The aim of this paper is to compare the gravitational…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Alessandro Nagar , Jose A. Font , Olindo Zanotti , Roberto De Pietri

There is no source for cosmic vorticity within the cold dark matter cosmology. However, vorticity has been observed in the universe, especially on the scales of clusters, filaments, galaxies, etc. Recent results from high-resolution general…

宇宙学与河外天体物理 · 物理学 2023-12-14 Obinna Umeh

Using the generally covariant magnetofluid formalism for a hot plasma, a new curvature (of space time) driven mechanism for generating seed vorticity/magnetic field is presented. The "battery" owes its origin to the interaction between…

高能天体物理现象 · 物理学 2012-10-09 Swadesh M. Mahajan , Felipe A. Asenjo

Gas falling quasi-spherically onto a black hole forms an inner accretion disc if its specific angular momentum $l$ exceeds $\lmin\sim r_gc$ where $r_g$ is the Schwarzschild radius. The standard disc model assumes $l\gg\lmin$. We argue that,…

天体物理学 · 物理学 2009-10-31 Andrei M. Beloborodov , Andrei F. Illarionov

In the interstellar medium the turbulence is believed to be forced mostly through supernova explosions. In a first approximation these flows can be written as a gradient of a potential being thus devoid of vorticity. There are several…

星系天体物理 · 物理学 2011-08-19 Fabio Del Sordo , Axel Brandenburg

To investigate the formation mechanism of relativistic jets in active galactic nuclei and micro-quasars, we have developed a new general relativistic magnetohydrodynamic code in Kerr geometry. Here we report on the first numerical…

天体物理学 · 物理学 2009-10-31 Shinji Koide , David L. Meier , Kazunari Shibata , Takahiro Kudoh

This paper discusses the behavior of a rotating relativistic kinetic gas surrounding a Schwarzschild black hole. We are interested in the description and analysis of the morphology of the resulting configurations for kinetic gas clouds with…

广义相对论与量子宇宙学 · 物理学 2026-03-10 Carlos Gabarrete , Roger Raudales

Recent observations of Galactic Black Hole Candidates (BHCs) suggest that those that are superluminal jet sources have more rapid black hole spin rates than otherwise normal BHCs. This provides observational support for models of…

天体物理学 · 物理学 2007-05-23 Shinji Koide , David L. Meier , Kazunari Shibata , Takahiro Kudoh

We describe stationary and axisymmetric gas configurations surrounding black holes. They consist of a collisionless relativistic kinetic gas of identical massive particles following bound orbits in a Schwarzschild exterior spacetime and are…

广义相对论与量子宇宙学 · 物理学 2022-02-02 Carlos Gabarrete , Olivier Sarbach

We study strong gravitational lensing due to a Schwarzschild black hole. Apart from the primary and the secondary images we find a sequence of images on both sides of the optic axis; we call them {\em relativistic images}. These images are…

天体物理学 · 物理学 2009-10-31 K. S. Virbhadra , George F. R. Ellis

In this paper we present the global baroclinic instability as a source for vigorous turbulence leading to angular momentum transport in Keplerian accretion disks. We show by analytical considerations and three-dimensional radiation hydro…

天体物理学 · 物理学 2009-11-07 Hubert Klahr , Peter Bodenheimer

The current popular model for launching, accelerating and collimating astrophysical jets is based on magnetohydrodynamics (MHD). AGN jets are most probably powered by energy extracted from either an accretion disk or a rapidly rotating…

天体物理学 · 物理学 2007-05-23 Max Camenzind

I study the generation and evolution of magnetic fields in the plasma surrounding a rotating black hole. Attention is focused on effects of the gravitomagnetic potential. The gravitomagnetic force appears as battery term in the generalized…

天体物理学 · 物理学 2007-05-23 Ramon Khanna

The generation of relativistic jets in active sources such as blazars is a complex problem with many aspects, most of them still not fully understood. Relativistic jets are likely produced by the accretion of matter and magnetic fields onto…

高能天体物理现象 · 物理学 2020-07-21 Gustavo E. Romero , Eduardo M. Gutiérrez

Scalar Tensor Vector Gravity (STVG) is an alternative theory of gravitation that has successfully explained the rotation curves of nearby galaxies, the dynamics of galactic clusters, and cosmological data without dark matter, but has hardly…

高能天体物理现象 · 物理学 2017-06-28 Daniela Pérez , Federico G. Lopez Armengol , Gustavo E. Romero
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