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The extractable energy from a black hole, as origin of the Gamma-Ray Burst (GRB) phenomenon is reviewed.

天体物理学 · 物理学 2009-09-29 Remo Ruffini

It has been thought for decades that rotating black holes (BHs) power the energetic gamma-ray bursts (GRBs) and active galactic nuclei (AGNs), but the mechanism that extracts the BH energy has remained elusive. We here show that the…

高能天体物理现象 · 物理学 2023-10-17 J. A. Rueda , R. Ruffini

A multi-decade theoretical effort has been devoted to finding an efficient mechanism to use the rotational and electrodynamical extractable energy of a Kerr-Newman black hole (BH), to power the most energetic astrophysical sources such as…

高能天体物理现象 · 物理学 2021-06-02 R. Moradi , J. A. Rueda , R. Ruffini , Y. Wang

We show that the gravitomagnetic interaction of a Kerr black hole (BH) with a surrounding magnetic field induces an electric field that accelerates charged particles to ultra-relativistic energies in the vicinity of the BH. Along the BH…

高能天体物理现象 · 物理学 2022-04-20 J. A. Rueda , R. Ruffini , R. P. Kerr

Gamma-ray bursts (GRBs) are violent explosions, coming from cosmological distances. They are detected in gamma-rays (also X-rays, UV, optical, radio) almost every day, and have typical durations of a few seconds to a few minutes. Some GRBs…

高能天体物理现象 · 物理学 2015-06-10 Antonios Nathanail , Ioannis Contopoulos

Gamma-Ray Bursts (GRBs) are extra-galactic and extremely energetic transient emissions of gamma rays, which are thought to be associated with the death of massive stars or the merger of compact objects in binary systems. Their huge…

高能天体物理现象 · 物理学 2016-07-20 F. Piron

We suggest that an extreme Kerr black hole with a mass $\sim 10^6M_\odot$, a dimensionless angular momentum $A\sim 1$ and a marginal stable orbital radius $r_{ms}\sim 3r_s\sim 10^{12}M_6 cm$ located in a normal galaxy, may produced a…

天体物理学 · 物理学 2009-10-31 K. S. Cheng , Y. Lu

Cosmological gamma-ray bursts (GRBs) are probably powered by systems harboring a rotating black hole. These may result from hypernovae or black hole-neutron star coalescence. We identify short/long bursts with hyper- and suspended-accretion…

天体物理学 · 物理学 2017-08-23 Maurice H. P. M. van Putten

Gamma-ray bursts (GRBs) appear as the brightest transient phenomena in the Universe. The nature of the central engine in GRBs is a missing link in the theory of fireballs to their stellar mass progenitors. Here it is shown that rotating…

天体物理学 · 物理学 2008-11-26 Maurice H. P. M. van Putten

If the threshold for $e^{-}e^{+}$ pair production depends on an angle between photon momenta, and if the $\gamma$-rays are collimated right in gamma-ray burst (GRB) source then another solution of the compactness problem is possible. The…

天体物理学 · 物理学 2008-05-22 V. V. Sokolov

A long march of fifty years of successive theoretical progress and new physics discovered using observations of gamma-ray bursts, has finally led to the formulation of an efficient mechanism able to extract the rotational energy of a Kerr…

广义相对论与量子宇宙学 · 物理学 2022-01-26 J. A. Rueda , R. Ruffini

Gamma-ray bursts (GRBs) are still an enigma. In particular the central engine, the total energy, and the very narrow distribution of peak energies challenge model builders. Motivated by recent theoretical developments (string theory,…

天体物理学 · 物理学 2009-10-31 James S. Graber

A variety of arguments suggest that the most common form of gamma-ray bursts (GRBs), those longer than a few seconds, involve the formation of black holes in supernova-like events. Two kinds of ``collapsar'' models are discussed, those in…

天体物理学 · 物理学 2009-10-31 S. E. Woosley

Whether a short gamma-ray burst (GRB) is caused by a black hole (BH) or a neutron star (NS) after the merger of a NS binary is a crucial problem. We propose a BH model that explains short GRBs with long-lasting activities such as extended…

高能天体物理现象 · 物理学 2015-06-24 Shota Kisaka , Kunihito Ioka

We outline the confluence of three novel theoretical fields in our modeling of Gamma-Ray Bursts (GRBs): 1) the ultrarelativistic regime of a shock front expanding with a Lorentz gamma factor $\sim 300$; 2) the quantum vacuum polarization…

The source of cosmic gamma-ray bursts (hereafter GRBs) is usually believed to be a stellar mass black hole accreting material from a thick disk. The mechanism for the production of a relativistic wind by such a system is still unknown. We…

天体物理学 · 物理学 2009-10-31 Frederic Daigne , Robert Mochkovitch

The Gamma-Ray Bursts (GRBs) offer the unprecedented opportunity to observe for the first time the blackholic energy extracted by the vacuum polarization during the process of gravitational collapse to a black hole leading to the formation…

The idea that the vacuum polarization process occurring during gravitational collapse to a black hole endowed with electromagnetic structure (EMBH) could be the origin of gamma ray bursts (GRBs) is further developed. EMBHs in the range 3.2…

天体物理学 · 物理学 2017-08-23 Remo J. Ruffini

Relativistic jets have been found for decades as a key phenomenon in active galactic nuclei (AGNs), compact binary systems, and gamma-ray bursts (GRBs), yet their energy resources remain a mystery. Two competing ideas prevail: one…

高能天体物理现象 · 物理学 2026-02-10 Shu-Xu Yi , Tian-Yong Cao , Shuang-Nan Zhang , Hua Feng

A complete model for the origin of high-energy >~10^{14} eV) cosmic rays from gamma-ray bursts (GRBs) and implications of this hypothesis are described. Detection of high-energy neutrinos from GRBs provide an unambiguous test of the model.…

天体物理学 · 物理学 2010-11-11 C. Dermer
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