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Related papers: Baryon-poor outflows from rotating black holes

200 papers

Introducing a spherical, steady, self-supported pair-plasma pressure mediated shock surface around a Schwarzschild black hole as the effective physical atmosphere which may be responsible for the generation of astrophysical mass outflows…

Astrophysics · Physics 2009-11-07 Tapas Kumar Das

Primordial black holes can represent all or most of the dark matter in the window $10^{17}-10^{22}\,$g. Here we present an extension of the constraints on PBHs of masses $10^{13}-10^{18}\,$g arising from the isotropic diffuse gamma ray…

Cosmology and Nongalactic Astrophysics · Physics 2020-01-29 Alexandre Arbey , Jérémy Auffinger , Joseph Silk

We present our recent results from numerical simulations of a magnetized flow in the vicinity of a black hole in the context of the collapsar model for GRBs. The simulations show that after an initial transient, the flow settles into a…

Astrophysics · Physics 2007-05-23 Daniel Proga

Despite that gamma-ray bursts is a phenomenon quite different from accreting compact objects, it could be that their hard X-ray emission is associated with a very similar mechanism of energy dissipation. In both cases, we could deal with…

Astrophysics · Physics 2007-05-23 Boris Stern

I show that Eddington accretion episodes in AGN are likely to produce winds with velocities $v \sim 0.1c$ and ionization parameters up to $\xi \sim 10^4$ (cgs), implying the presence of resonance lines of helium-- and hydrogenlike iron.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 A. R. King

Gamma-ray bursts (GRBs) show a dramatic pulse structure that requires bulk relativistic motion, but whose physical origin has remained murky. We focus on a hot, magnetized jet that is emitted by a black hole and interacts with a confining…

High Energy Astrophysical Phenomena · Physics 2014-06-23 Christopher Thompson , Ramandeep Gill

It is proposed that the gamma-ray photons that characterize the prompt emission of Gamma-Ray Bursts are produced through the Compton drag process, caused by the interaction of a relativistic fireball with a very dense soft photon bath. If…

Astrophysics · Physics 2009-10-31 Davide Lazzati , Gabriele Ghisellini , Annalisa Celotti , Martin J. Rees

The barycenter of a massive black hole binary will lie outside the event horizon of the primary black hole for modest values of mass ratio and binary separation. Analagous to radial velocity shifts in stellar emission lines caused by the…

High Energy Astrophysical Phenomena · Physics 2015-05-18 B. McKernan , K. E. S. Ford

We develop a model for gamma-ray emission from the outer magnetosphere of pulsars (the outer-gap model). The charge depletion causes a large electric field which accelerates electrons and positrons. We solve the electric field with…

Astrophysics · Physics 2007-05-23 Junpei Takata , Sinpei Shibata , Kouichi Hirotani

Active galaxies and quasers are believed to harbour Black Holes at their centers and at the same time produce cosmic radio jets through which immense amount of matter and energy are ejected out of the core of the galaxy. In our work we…

Astrophysics · Physics 2007-05-23 Tapas K. Das

Gamma-ray bursts and their afterglows are thought to be produced by an ultrarelativistic jet. One of the most important open questions is the outflow composition: the energy may be carried out from the central source either as kinetic…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Stefano Covino

A number of recent lines of evidence point towards the presence of hot, out-flowing plasma from the central regions of compact Galactic and extragalactic X-ray sources. Additionally, it has long been noted that many of these sources exhibit…

Astrophysics · Physics 2009-11-10 Lev Titarchuk , Chris Shrader

We investigate how magnetically driven outflows are powered by a rotating, weakly magnetized accretion flow onto a supermassive black hole using axisymmetric magnetohydrodynamic simulations. Our proposed model focuses on the accretion…

Astrophysics of Galaxies · Physics 2022-02-16 Shinsuke Takasao , Yuri Shuto , Keiichi Wada

Accreting black hole sources show variable outflows at different mass scales. For instance, in the case of galactic nuclei, our own galactic center Sgr A* exhibits flares and outbursts in the X-ray and infrared bands. Recent studies suggest…

High Energy Astrophysical Phenomena · Physics 2024-07-17 Bestin James , Agnieszka Janiuk , Vladimir Karas

We show that in the presence of a chemical potential, black hole evaporation generates baryon number. If the inflaton or Ricci scalar is derivatively coupled to the B-L current, the expansion of the universe acts as a chemical potential and…

High Energy Physics - Phenomenology · Physics 2015-01-06 Anson Hook

Relativistic jets powered by stellar mass black holes in X-ray binaries appear to come in two types: steady outflows associated with hard X-ray states and large scale discrete ejections associated with transient outbursts. We show that the…

Astrophysics · Physics 2009-11-10 Elena Gallo , Rob Fender , Christian Kaiser

We find that the Hawking radiation of black holes can create the baryon number in the Higgs phase vacuum of the extended standard model with 2-Higgs doublets. We propose new scenarios of baryogenesis based on the black holes, and one of our…

High Energy Physics - Phenomenology · Physics 2007-05-23 Yukinori Nagatani

If primordial black holes (PBHs) contribute more than 10 percent of the dark matter (DM) density, their energy density today is of the same order as that of the baryons. Such a cosmic coincidence might hint at a mutual origin for the…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-28 Yi-Peng Wu , Elena Pinetti , Joseph Silk

We consider the possible existence of a common channel of evolution of binary systems, which results in a gamma-ray burst during the formation of a black hole or the birth of a magnetar during the formation of a neutron star. We assume that…

High Energy Astrophysical Phenomena · Physics 2010-11-02 A. I. Bogomazov , S. B. Popov

Gamma-ray bursts (GRBs) are believed to originate from ultra-relativistic winds/fireballs to avoid the "compactness problem". However, the most energetic photons in GRBs may still suffer from $\gamma-\gamma$ absorption leading to…

Astrophysics · Physics 2009-11-10 Zhuo Li , Z. G. Dai , T. Lu , L. M. Song