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相关论文: The blackholic quantum

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We propose that the "inner engine" of a type I binary-driven hypernova (BdHN) is composed of a Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field $B_0$ aligned with the BH rotation axis, and surrounded by…

高能天体物理现象 · 物理学 2020-01-08 R. Ruffini , R. Moradi , J. A. Rueda , L. Becerra , C. L. Bianco , C. Cherubini , S. Filippi , Y. C. Chen , M. Karlica , N. Sahakyan , Y. Wang , S. S. Xue

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

We motivate how the most recent progress in the understanding the nature of the GeV radiation in most energetic gamma-ray bursts (GRBs), the binary-driven hypernovae (BdHNe), has led to the solution of a forty years unsolved problem in…

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

We address the physical origin of the ultrarelativistic prompt emission (UPE) phase of GRB 190114C observed in the interval 1.9-3.99 s, by the Fermi-GBM in 10 keV-10 MeV . Thanks to high S/N ratio of Fermi-GBM data, a time resolved spectral…

高能天体物理现象 · 物理学 2021-10-26 R. Moradi , J. A. Rueda , R. Ruffini , Liang Li , C. L. Bianco , S. Campion , C. Cherubini , S. Filippi , Y. Wang , S. S. Xue

Kerr black holes are energetically similar to spinning tops accompanied by frame dragging in the surrounding spacetime. Frame dragging is shown herein to be a universal causal agent for producing multi-messenger emissions. We discuss high…

高能天体物理现象 · 物理学 2010-02-04 Maurice H. P. M. van Putten

To explain the extremely high energy release, $>10^{53}$~erg, suggested by the observations of some Gamma Ray Bursts (GRBs) we propose a new energy extraction mechanism from the rotation energy of a Kerr-Newman black hole (BH) by a massive…

广义相对论与量子宇宙学 · 物理学 2017-11-22 Fabrizio Tamburini , Mariafelicia De Laurentis , Lorenzo Amati , Bo Thidé

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

The energetics of the long duration GRB phenomenon is compared with models of a rotating Black Hole (BH) in a strong magnetic field generated by an accreting torus. A rough estimate of the energy extracted from a rotating BH with the…

天体物理学 · 物理学 2009-11-07 G. Barbiellini , A. Celotti , F. Longo

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

We outline the main results of our GRB model, based on the three interpretation paradigms we proposed in July 2001, comparing and contrasting them with the ones in the current literature. Thanks to the observations by Swift and by VLT, this…

It has recently become clear that in both short and long gamma-ray bursts (GRBs) it coexists a sequence of different events, each characterized by specific physical processes and corresponding values of the Lorentz gamma factors. The…

Black holes surrounded by a disk or torus may drive the enigmatic cosmological gamma-ray bursts (GRBs). Equivalence in poloidal topology to pulsar magnetospheres shows a high incidence of the black hole-luminosity $L_H$ into the surrounding…

天体物理学 · 物理学 2014-10-13 Maurice H. P. M. van Putten , Amir Levinson

(Shortened) [...] After recalling the basic features of the "fireshell model", we emphasize the following novel results: 1) the interpretation of the X-ray flares in GRB afterglows as due to the interaction of the optically thin fireshell…

Black hole (BH) mergers are natural sources of gravitational waves (GWs) and are possibly associated with electromagnetic events. Such events from a charged rotating BH with an accretion on to it could be more energetic and…

高能天体物理现象 · 物理学 2024-11-27 Shad Ali

An energy $E=\omega J$ is derived for gravitational spin-orbit coupling by frame-dragging $\omega$ acting on angular momentum $J$. This interaction defines a no-boundary mechanism for linear acceleration of magnetized matter along the axis…

天体物理学 · 物理学 2007-05-23 Maurice H. P. M. van Putten

General relativity (GR) predicts the existence of black hole (BH). The rotating BH called as a Kerr Black hole and GR implies that there is an upper limit on the angular momentum per mass squared of black holes $\leq 1$, above which the…

广义相对论与量子宇宙学 · 物理学 2024-05-24 Sumit Panganti , Siba Prasad Das

We present a mechanism for long bursts of gravitational radiation from Kerr black holes surrounded by a torus. These systems are believed to form in core-collapse of massive stars in association with gamma-ray bursts. The torus catalyzes…

天体物理学 · 物理学 2007-05-23 Maurice H. P. M. van Putten

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
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