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相关论文: Gamma-ray emission from primordial black hole-neut…

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Using the BATSE survey data I find that quite small fraction of GRBs numbering 37 sources seems to emit the radiation similar to thermal bremsstrahlung in the range 20 to 300 keV. I suggest that these bursts may perhaps occur from collision…

天体物理学 · 物理学 2009-06-25 B. E. Zhilyaev

Recently, an alleged plausible astrophysical scenario was proposed for the production of observed thermal gamma-ray bursts, via Hawking radiation emitted from a primordial black hole (PBH) freely falling into a more massive black hole. Here…

广义相对论与量子宇宙学 · 物理学 2022-02-08 Tyler McMaken

Asteroid-mass primordial black holes (PBH) can explain the observed dark matter abundance while being consistent with the current indirect detection constraints. These PBH can produce gamma-ray signals from Hawking radiation that are within…

宇宙学与河外天体物理 · 物理学 2023-01-18 Kaustubh Agashe , Jae Hyeok Chang , Steven J. Clark , Bhaskar Dutta , Yuhsin Tsai , Tao Xu

The 511 keV gamma emission from the galactic core may originate from a high concentration ($\sim 10^{22}$) of primordial black holes (PBHs) in the core each of whose Hawking radiation includes $\sim 10^{21}$ positrons per second. The PBHs…

高能物理 - 唯象学 · 物理学 2009-11-11 Paul H. Frampton , Thomas W. Kephart

Cosmological GRBs are discussed with an emphasis on their plausible connection with black holes. GRBs can be triggered by collapse of stellar-mass objects that leads to formation of a black hole and a transient debris disk with a huge…

天体物理学 · 物理学 2008-11-26 Andrei M. Beloborodov

Ultracompact primordial black hole binaries with masses > 10^{16} g are considered. If PBHB's contribute significant part of the dark matter of the Galaxy one can expect an existence of high-frequent non-thermal diffuse gravitational…

天体物理学 · 物理学 2009-09-25 J. N. Abdurashitov , V. E. Yants , C. V. Parfenov

Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermasive black hole. In this work, we study the interaction of early-type…

高能天体物理现象 · 物理学 2015-06-17 Anabella Araudo , Valenti Bosch-Ramon , Gustavo E. Romero

Black holes with masses below approximately $10^{15}$ g are expected to emit gamma rays with energies above a few tens of MeV, which can be detected by the Fermi Large Area Telescope (LAT). Although black holes with these masses cannot be…

高能天体物理现象 · 物理学 2018-02-02 LAT Collaboration

We investigate the gravitational wave (GW) signals emitted by planetary-mass primordial black holes (PBHs) passing nearby or traversing neutron stars (NSs). While previous studies mainly focused on the detailed waveforms of the signals, we…

高能天体物理现象 · 物理学 2026-03-02 Nicolas Esser , Juan García-Bellido , Peter Tinyakov

Short Gamma-Ray Bursts (GRBs) are explosions of cosmic origin believed to be associated with the merger of two compact objects, either two neutron stars, or a neutron star and a black hole. The presence of at least one neutron star has long…

高能天体物理现象 · 物理学 2016-04-27 Rosalba Perna , Davide Lazzati , Bruno Giacomazzo

Primordial Black Holes (PBHs), which may have been created in the early Universe, are predicted to be detectable by their Hawking radiation. The Fermi Gamma-ray Space Telescope observatory offers increased sensitivity to the gamma-ray…

高能天体物理现象 · 物理学 2010-03-26 T. N. Ukwatta , Jane H. MacGibbon , W. C. Parke , K. S. Dhuga , S. Rhodes , A. Eskandarian , N. Gehrels , L. Maximon , D. C. Morris

Within the next few years gravitational waves (GWs) from merging black holes (BHs) and neutron stars (NSs) may be directly detected, making a thorough theoretical understanding of these systems a high priority. As an additional motivation,…

高能天体物理现象 · 物理学 2013-03-08 Branson C. Stephens , William E. East , Frans Pretorius

Primordial Black Holes (PBHs), which may have been created in the early Universe, are predicted to be detectable by their Hawking radiation. PBHs with an initial mass of 5.0 * 10^14 g should be expiring today with a burst of high energy…

高能天体物理现象 · 物理学 2010-03-29 T. N. Ukwatta , J. H. MacGibbon , W. C. Parke , K. S. Dhuga , A. Eskandarian , N. Gehrels , L. Maximon , D. C. Morris

We put forward a novel class of exotic celestial objects that can be produced through phase transitions occurred in the primordial Universe. These objects appear as bubbles of stellar sizes and can be dominated by primordial black holes…

宇宙学与河外天体物理 · 物理学 2022-06-03 Yi-Fu Cai , Chao Chen , Qianhang Ding , Yi Wang

In this $\textit{Letter}$, we search for the signal of the primordial black holes (PBHs) by correlating the $\gamma$-ray emissions in the MeV energy band produced by the Hawking evaporation and the lensing effect of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2022-11-16 Xiu-Hui Tan , Yang-Jie Yan , Taotao Qiu , Jun-Qing Xia

We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies…

高能天体物理现象 · 物理学 2015-06-17 Anabella T. Araudo , Valenti Bosch-Ramon , Gustavo E. Romero

Primordial black holes (PBHs) are predicted in many models via different formation mechanisms. Identifying the origin of PBHs is of the same importance as probing their existence. We propose to probe the asteroid-mass PBHs…

宇宙学与河外天体物理 · 物理学 2023-06-14 Ke-Pan Xie

We propose several novel scenarios how capture of small sublunar-mass primordial black holes (PBHs) by compact stars, white dwarfs or neutron stars, can lead to distinct short gamma-ray bursts (sGRBs) as well as microquasars (MQs). In…

高能天体物理现象 · 物理学 2019-01-15 Volodymyr Takhistov

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

A nearby primordial-black-hole (PBH) evaporation burst would produce a curved gamma-ray wavefront, leading to detectable departures from plane-wave inter-satellite delays. We introduce a purely geometric method that combines imaging…

天体物理仪器与方法 · 物理学 2026-03-18 Shuo Xiao , Shuang-Nan Zhang
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