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The compact, nonthermal radio source Sgr A* at the Galactic Center appears to be coincident with a 2.6 million solar mass point-like object. Its energy source may be the release of gravitational energy as gas from the interstellar medium…

Astrophysics · Physics 2009-10-31 Robert F. Coker , Fulvio Melia

We investigate the consequences of acceleration of nuclei in jets of active galaxies not far from the surface of an accretion disk. The nuclei can be accelerated in the re-connection regions in the jet and/or at the jet boundary, between…

High Energy Astrophysical Phenomena · Physics 2016-12-23 W. Bednarek

Relativistic jets originating from protomagnetar central engines can lead to long duration gamma-ray bursts (GRBs) and are considered potential sources of ultrahigh-energy cosmic rays and secondary neutrinos. We explore the propagation of…

High Energy Astrophysical Phenomena · Physics 2023-04-03 Mukul Bhattacharya , Jose Alonso Carpio , Kohta Murase , Shunsaku Horiuchi

Black hole--neutron star (BHNS) binary mergers can form disks in which magnetorotational instability (MRI)-induced turbulence may drive accretion onto the remnant BH, supporting relativistic jets and providing the engine for a short-hard…

High Energy Astrophysical Phenomena · Physics 2012-10-10 Zachariah B. Etienne , Vasileios Paschalidis , Stuart L. Shapiro

A population of binary stellar-mass black hole (BBH) mergers are believed to occur embedded in the accretion disk of active galactic nuclei (AGNs). In this {\em Letter}, we demonstrate that the jets from these BBH mergers can propagate…

High Energy Astrophysical Phenomena · Physics 2023-11-21 Jin-Ping Zhu

Variability studies are a powerful tool for studying the structures of unresolved sources. One such type of variability study, called reverberation mapping (RM), established that the dominant source of infrared radiation from an active…

Instrumentation and Methods for Astrophysics · Physics 2025-10-21 Varoujan Gorjian , Michael W. Werner

We consider the gamma ray burst (GRB) central engine that is powered by the collapse of a massive rotating star or compact binary merger. The engine is a hot and dense accretion disk, which is composed of free nucleons, electron-positron…

High Energy Astrophysical Phenomena · Physics 2016-09-30 Agnieszka Janiuk

The exact time-dependent solution is obtained for a magnetic field growth during a spherically symmetric accretion into a black hole (BH) with a Schwarzschild metric. Magnetic field is increasing with time, changing from the initially…

High Energy Astrophysical Phenomena · Physics 2019-06-03 G. S. Bisnovatyi-Kogan

We discuss recent results in neutrino astronomy and their implications for the cosmic-ray acceleration in relativistic outflows, such as in Active Galactic Nuclei (AGN) jets, Gamma-Ray Bursts (GRBs), and Tidal Disruption Events (TDEs). We…

High Energy Astrophysical Phenomena · Physics 2024-05-09 Walter Winter

Inspiraling and merging binary neutron stars are not only important source of gravitational waves, but also promising candidates for coincident electromagnetic counterparts. These systems are thought to be progenitors of short gamma-ray…

High Energy Astrophysical Phenomena · Physics 2017-11-03 Milton Ruiz , Stuart L. Shapiro

The energy release L_s on the surface of a neutron star (NS) with a weak magnetic field and the energy release L_d in the surrounding accretion disk depend on two independent parameters that determine its state (for example, mass M and…

Astrophysics · Physics 2009-10-31 N. R. Sibgatullin , R. A. Sunyaev

This research is to determine at Earth the high-energy neutrino flux coming from the galactic core, and from the many other accretion disks within the galactic core. It is estimated there are 10,000 such accretion disk within the cubic…

High Energy Astrophysical Phenomena · Physics 2023-08-01 Ayshea Bains , Trent English , Nickolas Solomey

Analyses of absorption from disk winds and atmospheres in accreting compact objects typically treat the central emitting regions in these systems as point sources relative to the absorber. This assumption breaks down if the absorbing gas is…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Nicolas Trueba , J. M. Miller , A. C. Fabian , J. Kaastra , T. Kallman , A. Lohfink , R. M. Ludlam , D. Proga , J. Raymond , C. Reynolds , M. Reynolds , A. Zoghbi

We present our first numerical results of axisymmetric magnetohydrodynamic simulations for neutrino-cooled accretion tori around rotating black holes in general relativity. We consider tori of mass $\sim 0.1$--0.4$M_{\odot}$ around a black…

Astrophysics · Physics 2009-06-23 M. Shibata , Y. Sekiguchi , R. Takahashi

Black hole-neutron star (BHNS) binaries are expected to be among the leading sources of gravitational waves observable by ground-based detectors, and may be the progenitors of short-hard gamma ray bursts (SGRBs) as well. Here, we discuss…

We investigate the deposition of energy due to the annihilations of neutrinos and antineutrinos on the rotation axis of rotating neutron and quark stars, respectively. The source of the neutrinos is assumed to be a neutrino-cooled accretion…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Z. Kovacs , K. S. Cheng , T. Harko

AGNs exhibit a wide range of black hole masses and inflow/outflow properties. It is now possible to probe regions close to the event horizons of nearby SMBHs using VLBI with earth-sized baselines, as performed by the EHT. This study…

High Energy Astrophysical Phenomena · Physics 2025-05-23 Bidisha Bandyopadhyay , Christian Fendt , Dominik R. G. Schleicher , Neil M. Nagar , Felipe Agurto-Sepulveda , Javier Pedreros

Recently, two empirical correlations related to the minimum variability timescale ($\rm MTS$) of the lightcures are discovered in gamma-ray bursts (GRBs). One is the anti-correlation between $\rm MTS$ and Lorentz factor $\Gamma$, the other…

High Energy Astrophysical Phenomena · Physics 2017-04-12 Wei Xie , Wei-Hua Lei , Ding-Xiong Wang

Steady axisymmetric outflows originating at the hot coronal magnetosphere of a Schwarzschild black hole and surrounding accretion disk are studied in the framework of general relativistic magnetohydrodynamics (GRMHD). The assumption of…

Astrophysics · Physics 2009-11-11 Z. Meliani , C. Sauty , N. Vlahakis , K. Tsinganos , E. Trussoni

The recent detection of a gamma-ray flux from the direction of the Galactic center by EGRET on the Compton GRO raises the question of whether this is a point source (possibly coincident with the massive black hole candidate Sgr A*) or a…

Astrophysics · Physics 2009-10-30 S. Markoff , F. Melia , I. Sarcevic