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相关论文: Cosmic Ray Generation by Quasar Remnants: Constrai…

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Considerations of the collision losses for protons traversing the 2.7 K black body microwave radiation field have led to the conclusion that the highest energy cosmic rays, those observed at $\geq 10^{20}$ eV, must come from sources within…

天体物理学 · 物理学 2011-02-21 Elihu Boldt , Pranab Ghosh

As recently suggested, nearby quasar remnants are plausible sites of black-hole based compact dynamos that could be capable of accelerating ultra-high energy cosmic rays (UHECRs). In such a model, UHECRs would originate at the nuclei of…

天体物理学 · 物理学 2009-11-07 Diego F. Torres , Elihu Boldt , Timothy Hamilton , Michael Loewenstein

The origin of Galactic cosmic rays remains a matter of debate, but supernova remnants are commonly considered to be the main place where high-energy cosmic rays are accelerated. Nevertheless, current models predict cosmic-ray spectra that…

高能天体物理现象 · 物理学 2021-06-23 G. J. Escobar , L. J. Pellizza , G. E. Romero

We propose that nearly every accelerated CR was part of the parallel current that maintains all force-free (f-f) magnetic fields. Charged particles are accelerated by the E-parallel (to the magnetic filed B) produced by reconnection. The…

天体物理学 · 物理学 2015-06-24 Stirling A. Colgate , Hui Li

Origin of ultra high energy cosmic rays is an unsolved problem. Several proposals such as Z-burst, decay of super massive matter, susy particles as a primary, neutrino as a primary in extra dimension models exist in the literature which try…

天体物理学 · 物理学 2007-05-23 Pankaj Jain , Sukanta Panda

Simple arguments concerning power and acceleration efficiency show that ultra-high energy cosmic rays (UHECRS) with energies >~ 10^{19} eV could originate from GRBs. Neutrons formed through photo-pion production processes in GRB blast waves…

天体物理学 · 物理学 2009-11-06 C. D. Dermer

Protons with energies up to 10^15 eV are the main component[1] of cosmic rays, but evidence for the specific locations where they could have been accelerated to these energies has been lacking[2]. Electrons are known to be accelerated to…

天体物理学 · 物理学 2012-08-27 II Collaboration , R. Enomoto

It is widely believe that galactic cosmic rays are originated in supernova remnants (SNRs) where they are accelerated by diffusive shock acceleration process at supernova blast waves driven by expanding SNRs. In recent theoretical…

高能天体物理现象 · 物理学 2017-08-02 Prabir Banik , Arunava Bhadra

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

高能天体物理现象 · 物理学 2018-04-25 Giovanni Morlino

One of the models recently proposed to explain the origin of the ultra high energy cosmic rays assumes that these particles may be accelerated by the electromotive force around presently inactive quasar remnants. We study predictions for…

天体物理学 · 物理学 2007-05-23 C. Isola , G. Sigl , G. Bertone

The recent detection of the gravitational wave source GW150914 by the LIGO collaboration motivates a speculative source for the origin of ultrahigh energy cosmic rays as a possible byproduct of the immense energies achieved in black hole…

高能天体物理现象 · 物理学 2016-06-01 Kumiko Kotera , Joseph Silk

Suppose that even the highest energy cosmic rays (CRs) observed on Earth are protons accelerated in local Milky Way Galaxy sources, with few if any from more distant sources. In this paper we treat the problem that supernovae remnants…

高能天体物理现象 · 物理学 2013-05-06 Richard Shurtleff

We investigate the idea that ultrahigh energy gamma-rays (E>10 TeV) can be produced when charged particles are accelerated by microscopic black holes. We begin by showing that microscopic black holes may exist as remnants of primordial…

天体物理学 · 物理学 2009-11-07 Roberto Casadio , Benjamin Harms , Octavian Micu

It is thought that Galactic cosmic ray (CR) nuclei are gradually accelerated to high energies (up to ~300 TeV/nucleon, where 1TeV=10^12eV) in the expanding shock-waves connected with the remnants of powerful supernova explosions. However,…

天体物理学 · 物理学 2015-06-24 Yousaf M. Butt , Diego F. Torres , Gustavo E. Romero , Thomas M. Dame , Jorge A. Combi

Although Galactic cosmic rays (protons and nuclei) are widely believed to be dominantly accelerated by the winds and supernovae of massive stars, definitive evidence of this origin remains elusive nearly a century after their discovery [1].…

The origin of cosmic rays with energies higher than 10$^{20}$ eV remains a mystery. Accelerating particles up to these energies is a challenge even for the most energetic astrophysical objects known. While the isotropy in arrival directions…

天体物理学 · 物理学 2017-08-23 A. V. Olinto

The Auger Collaboration reports that the arrival directions of >60 EeV ultra-high energy cosmic rays (UHECRs) cluster along the supergalactic plane and correlate with active galactic nuclei (AGN) within ~100 Mpc. The association of several…

天体物理学 · 物理学 2009-08-05 C. D. Dermer , S. Razzaque , J. D. Finke , A. Atoyan

The origin of ultrahigh-energy cosmic rays (UHECRs) is a half-century old enigma (Linsley 1963). The mystery has been deepened by an intriguing coincidence: over ten orders of magnitude in energy, the energy generation rates of UHECRs, PeV…

高能天体物理现象 · 物理学 2018-10-16 Ke Fang , Kohta Murase

The possibility that rapidly rotating supermassive black holes associated with quasar remnants may provide sites for the acceleration of ultra-high energy cosmic rays (UHECRs) is considered. It is shown that prodigious TeV emission through…

天体物理学 · 物理学 2010-11-19 Amir Levinson

We review the hypothesis that the acceleration of protons at internal shocks in Gamma Ray Bursts (GRB) could be the origin of the ultra-high energy cosmic rays (UHECR) observed at earth, E_max > 10^19 eV. We find that, even though protons…

天体物理学 · 物理学 2010-12-13 Jorg P. Rachen , P. Meszaros
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