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相关论文: Does the gravitomagnetic monopole exist? A clue fr…

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Einstein-dilaton-Gauss-Bonnet gravity is a theoretically well-motivated alternative theory of gravity emerging as a low-energy 4-dimensional model from heterotic string theory. Its rotating black hole solutions are known numerically and can…

广义相对论与量子宇宙学 · 物理学 2017-06-01 Hao Zhang , Menglei Zhou , Cosimo Bambi , Burkhard Kleihaus , Jutta Kunz , Eugen Radu

The possible transition of large mass magnetic monopole solutions to monopole black hole solutions in Yang-Mills-Higgs theory with spontaneous symmetry breaking (SSB) coupled to the low energy effective theory of superstring with only…

综合物理 · 物理学 2019-06-03 Hongsu Kim

Recent X-ray timing and spectral observations of black hole binaries in outburst have redefined methods for investigating the properties of Galactic black holes and the physics of accretion flows. High-frequency X-ray QPOs in 5 systems…

天体物理学 · 物理学 2007-05-23 R. A. Remillard

Magnetic monopoles have been a subject of interest since Dirac established the relation between the existence of a monopole and charge quantization. 't Hooft and Polyakov proved that they can arise from gauge theories as the result of a non…

高能物理 - 唯象学 · 物理学 2014-05-05 Vicente Vento , Valentina Sarti Mantovani

A primordial black hole (PBH) is thought to be made of the regular matter or ordinary mass ($M$) only, and hence could have already been decayed due to the Hawking radiation if its initial ordinary mass were $\lesssim 5 \times 10^{11}$ kg.…

高能天体物理现象 · 物理学 2022-11-23 Chandrachur Chakraborty , Sudip Bhattacharyya

The case for collapsed objects in some X-ray binary systems continues to strengthen. But there is now even firmer evidence for supermassive black holes in galactic centres. Gravitational collapse seems to have occurred in the centres of…

天体物理学 · 物理学 2008-02-03 Martin J. Rees

Accreting black holes often show iron line emission in their X-ray spectra. When this line emission is very broad or variable then it is likely to originate from close to the black hole. The theory and observations of such broad and…

天体物理学 · 物理学 2015-06-24 A. C. Fabian

We pioneer the black hole mass gap as a powerful new tool for constraining modified gravity theories. These theories predict fifth forces that alter the structure and evolution of population-III stars, exacerbating the pair-instability.…

广义相对论与量子宇宙学 · 物理学 2020-12-16 Maria C. Straight , Jeremy Sakstein , Eric J. Baxter

We investigate the gravitational energy-momentum distribution in the space-time of two black holes in circular orbit, in the context of the teleparallel equivalent of general relativity. This field configuration is important because…

广义相对论与量子宇宙学 · 物理学 2012-02-01 J. W. Maluf , S. C. Ulhoa , J. F. da Rocha-Neto

We review the properties and behavior X-ray binaries that contain an accreting black hole. The larger majority of such systems are X-ray transients, and many of them were observed in daily pointings with RXTE throughout the course of their…

天体物理学 · 物理学 2008-11-26 Ronald A. Remillard , Jeffrey E. McClintock

Asymmetric binary systems radiate linear momentum through gravitational waves, leading to the recoil of the merger remnant. Black-hole kicks have attracted much attention because of their astrophysical implications. However, little…

广义相对论与量子宇宙学 · 物理学 2021-06-07 Angela Borchers , Frank Ohme

We use population inference to explore the impact that uncertainties in the distribution of binary black holes (BBH) have on the astrophysical gravitational-wave background (AGWB). Our results show that the AGWB monopole is sensitive to the…

宇宙学与河外天体物理 · 物理学 2019-03-25 Alexander C. Jenkins , Richard O'Shaughnessy , Mairi Sakellariadou , Daniel Wysocki

Magnetic monopoles --- particles that behave as isolated north or south magnetic poles --- have been the subject of speculation since the first detailed observations of magnetism several hundred years ago. Numerous theoretical…

量子气体 · 物理学 2014-08-15 M. W. Ray , E. Ruokokoski , S. Kandel , M. Möttönen , D. S. Hall

Black hole spin will have a large impact on searches for gravitational waves with advanced detectors. While only a few stellar mass black hole spins have been measured using X-ray techniques, gravitational wave detectors have the capacity…

高能天体物理现象 · 物理学 2016-06-22 Alex B. Nielsen

We study a complex Dirac field in the chiral representation minimally coupled to gravity in 3+1 dimensions in the context of Einstein-Cartan theory. Generically the matter content gravitates in two different ways: On the one hand, the…

广义相对论与量子宇宙学 · 物理学 2015-03-12 Adolfo Toloza

Compact binary coalescences are the most promising sources of gravitational waves (GWs) for ground based detectors. Binary systems containing one or two spinning black holes are particularly interesting due to spin-orbit (and eventual…

广义相对论与量子宇宙学 · 物理学 2014-07-02 Salvatore Vitale , Ryan Lynch , John Veitch , Vivien Raymond , Riccardo Sturani

Observational evidence for the existence of Dark Matter is limited to its gravitational effects. The extensive program for dedicated searches has yielded null results so far, challenging the most popular models. Here we propose that this is…

X-ray reflection spectroscopy (or iron line method) is a powerful tool to probe the strong gravity region of black holes, and currently is the only technique for measuring the spin of the supermassive ones. While all the available…

高能天体物理现象 · 物理学 2020-05-27 Shafqat Riaz , Dimitry Ayzenberg , Cosimo Bambi , Sourabh Nampalliwar

Beyond the Newtonian approximation, gravitational fields in general relativity can be described using a formalism known as gravitoelectromagnetism. In this formalism a vector potential, the gravitomagnetic potential, arises as a result of…

广义相对论与量子宇宙学 · 物理学 2021-09-02 Viktor T. Toth

We consider the integral light polarization from optically thick accretion disks. Basic mechanism is the multiple light scattering on free electrons (Milne's problem) in magnetized atmosphere. The Faraday rotation of the polarization plane…

星系天体物理 · 物理学 2009-08-20 N. A. Silant'ev , M. Yu. Piotrovich , Yu. N. Gnedin , T. M. Natsvlishvili