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相关论文: Dyadosphere formed in gravitational collapse

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The dynamical properties of an electron--positron--photon plasma created by the vacuum polarization process occurring around a charged gravitationally collapsing core of an initially neutral star are examined within the framework of General…

天体物理学 · 物理学 2015-06-24 R. Ruffini , L. Vitagliano , S. -S. Xue

Basic energy requirements of Gamma Ray Burst(GRB) sources can be easily accounted for by a pair creation process occurring in the "Dyadosphere" of a Black Hole endowed with an electromagnetic field (abbreviated to EMBH for "electromagnetic…

天体物理学 · 物理学 2008-11-26 Giuliano Preparata , Remo Ruffini , She-Sheng Xue

We describe electron-positron pairs creation around an electrically charged star core collapsing to an electromagnetic black hole (EMBH), as well as pairs annihilation into photons. We use the kinetic Vlasov equation formalism for the pairs…

天体物理学 · 物理学 2017-08-23 R. Ruffini , L. Vitagliano , S. -S. Xue

The "dyadosphere" (from the Greek word "duas-duados" for pairs) is here defined as the region outside the horizon of a black hole endowed with an electromagnetic field (abbreviated to EMBH for "electromagnetic black hole") where the…

天体物理学 · 物理学 2007-05-23 Remo Ruffini

The "dyadosphere" has been defined (Ruffini, Preparata et al.) as the region outside the horizon of a black hole endowed with an electromagnetic field (abbreviated to EMBH for "electromagnetic black hole") where the electromagnetic field…

天体物理学 · 物理学 2011-05-23 Giuliano Preparata , Remo Ruffini , She-Sheng Xue

Electron-positron ($e^{+}e^{-}$) pair creation by vacuum breakdown around compact objects is believed to power high-energy astrophysical transients like gamma-ray bursts (GRBs). In this work, we focus on vacuum breakdown around a Kerr black…

广义相对论与量子宇宙学 · 物理学 2026-05-22 Ruixin Yang , Songbai Chen , Jiliang Jing

The concept of "dyadotorus" was recently introduced to identify in the Kerr-Newman geometry the region where vacuum polarization processes may occur, leading to the creation of $e^--e^+$ pairs. This concept generalizes the original concept…

高能天体物理现象 · 物理学 2009-06-30 C. Cherubini , A. Geralico , J. Rueda , R. Ruffini

From the interaction of physics and astrophysics we are witnessing in these years a splendid synthesis of theoretical, experimental and observational results originating from three fundametal physical processes. They were originally…

高能天体物理现象 · 物理学 2014-11-20 Remo Ruffini , Gregory Vereshchagin , She-Sheng Xue

The main issue of the pulsar magnetosphere is how the rotation power is converted into both particle beams which causes pulsed emissions, and a highly relativistic wind of electron-positron plasmas which forms surrounding nebulae shining in…

高能天体物理现象 · 物理学 2015-05-30 Tomohide Wada , Shinpei Shibata

We present the invariant characterization of the region where vacuum breakdown into electron-positron ($e^+e^-$) pairs occurs due to an overcritical electric field, the dyadoregion, in the case of a Kerr black hole (BH) in the presence of…

广义相对论与量子宇宙学 · 物理学 2025-12-24 C. Cherubini , R. Moradi , J. A. Rueda , R. Ruffini

We study the process of energy conversion from overcritical electric field into electron-positron-photon plasma. We solve numerically Vlasov-Boltzmann equations for pairs and photons assuming the system to be homogeneous and anisotropic.…

宇宙学与河外天体物理 · 物理学 2013-03-13 Alberto Benedetti , Remo Ruffini , Gregory Vereshchagin

(Shortened) We show by example how the uncoding of Gamma-Ray Bursts (GRBs) offers unprecedented possibilities to foster new knowledge in fundamental physics and in astrophysics. After recalling some of the classic work on vacuum…

We study the dynamical Schwinger effect in the vacuum excitation of the electron-positron plasma under action of a "laser pulse" of the simplest configuration: a linearly polarized, time-dependent and spatially homogeneous electric field.…

等离子体物理 · 物理学 2015-09-04 D. Blaschke , L. Juchnowski , A. Panferov , S. Smolyansky

The spontaneous production of electron-positron pairs from the vacuum--in a field configuration composed of a high-frequency electric mode of weak intensity and a strong constant electric field--is investigated. Asymptotic expressions for…

高能物理 - 唯象学 · 物理学 2019-12-25 Selym Villalba-Chávez , Carsten Müller

We examine energy conversion from accreting pair plasma to outgoing Poynting flux by black hole rotation. Our approach is based on a two-fluid model consisting of collisionless pair plasma. The electric potential is not constant along…

高能天体物理现象 · 物理学 2015-11-04 Yasufumi Kojima

The possibility to observe vacuum electron-positron pair creation due to a powerful optical laser pulse is discussed. We employ a quantum kinetic formulation of the problem with a source term describing the vacuum pair production in a…

等离子体物理 · 物理学 2007-05-23 D. B. Blaschke , A. V. Prozorkevich , S. A. Smolyansky , A. V. Tarakanov

The production of electron-positron pairs in a vacuum neutron star magnetosphere is investigated for both low (compared to the Schwinger one) and high magnetic fields. The case of a strong longitudinal electric field where the produced…

高能天体物理现象 · 物理学 2011-11-02 Ya. N. Istomin , D. N. Sob'yanin

The problem of the backreaction during the process of electron-positron pair production by a circularly polarized electromagnetic wave propagating in a plasma is investigated. A model based on the relativistic Boltzmann-Vlasov equation with…

高能物理 - 唯象学 · 物理学 2016-09-06 S. S. Bulanov , A. M. Fedotov , F. Pegoraro

We present theoretical predictions for the spectral, temporal and intensity signatures of the electromagnetic radiation emitted during the process of the gravitational collapse of a stellar core to a black hole, during which electromagnetic…

天体物理学 · 物理学 2009-11-10 R. Ruffini , F. Fraschetti , L. Vitagliano , S. -S. Xue

The electron-positron pair production accompanying interaction of a circularly polarized laser pulse with a foil is studied for laser intensities higher than $10^{24}$W cm$^{-2}$. The laser energy penetrates into the foil due to the effect…

等离子体物理 · 物理学 2016-11-03 I. Yu. Kostyukov , E. N. Nerush
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