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Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons
Physics Letters B, 2021 Previous researches on high-energy neutrino events from gamma-ray bursters (GRBs) suggest a neutrino speed variation v(E)=c(1±E/ELVν) with ELVν=(6.4±1.5)×1017 GeV, together with an intrinsic time difference Δtin=(−2.8±0.7)×102 s, which means that high ...
Jie Zhu, Bo-Qiang Ma
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The Central Engine of Gamma-Ray Bursters [PDF]
Astrophysical Journal, 1998 GRBs are thought to arise in relativistic blast-wave shocks at distances of 10 to 1000 AU from the point where the explosive energy is initially released. To account for the observed duration and variability of the gamma-ray emission in most GRBs, a central engine powering the shocks must remain active for several seconds to many minutes but must ...
W Kluźniak, M Ruderman
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How Far Away Are Gamma-Ray Bursters? [PDF]
Publications of the Astronomical Society of the Pacific, 1995 The positions of over 1000 gamma-ray bursts detected with the BATSE experiment on board of the Compton Gamma Ray Observatory are uniformly and randomly distributed in the sky, with no significant concentration to the galactic plane or to the galactic center.
exaly +3 more sources
Gamma-ray bursters at cosmological distances
Astrophysical Journal, 1986 It is proposed that some, perhaps most, gamma-ray bursters are at cosmological distances, like quasars, with a redshift of about 1 or 2. This proposition requires a release of supernova-like energy of about 10 to the 51st ergs within less than 1 s, making gamma-ray bursters the brightest objects known in the universe, many orders of magnitude brighter ...
B Paczynski
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Femtolensing of gamma-ray bursters
Astrophysical Journal, 1992 If gamma-ray bursters are at cosmological distances, they can be used to probe for «femtolenses» extremely small (∼10 −13 -10 −16 M ⊙ ) dark-matter objects. The time delay induced by such a lens would be ∼10 −17 -10 −20 s, approximately equal to the period of a gamma ray.
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Gamma-ray bursters as sources of cosmic rays [PDF]
Astroparticle Physics, 1996 The little we do know of the physical conditions in gamma-ray bursters makes them conducive to the acceleration of high-energy cosmic rays, especially if they are at cosmological distances. We find that, with the observed statistics and fluxes of gamma-ray bursts, cosmological bursters may be an important source of cosmic rays in two regions of the ...
Mordehai Milgrom
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Nonthermal Radiation of Cosmological Gamma‐Ray Bursters
Astrophysical Journal, 2000 37 pages, 11 figures, submitted to ...
Vladimir V Usov
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Classification of BATSE, Swift, and Fermi Gamma-Ray Bursts from Prompt Emission Alone
The Astrophysical Journal, 2023 Although it is generally assumed that there are two dominant classes of gamma-ray bursts (GRBs) with different typical durations, it has been difficult to classify GRBs unambiguously as short or long from summary properties such as duration, spectral ...
Charles L. Steinhardt +3 more
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Coalescing neutron stars as gamma ray bursters? [PDF]
Astrophysics and Space Science, 1995 extended abstract contribution to the proceedings of the 17th Texas Symposium, 2 pages, uuencoded compressed postscript.
Ruffert, M. +3 more
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Limits on Fast Radio Burst–like Counterparts to Gamma-Ray Bursts Using CHIME/FRB
The Astrophysical Journal, 2023 Fast radio bursts (FRBs) are a class of highly energetic, mostly extragalactic radio transients lasting for ∼milliseconds. While over 600 FRBs have been published so far, their origins are presently unclear, with some theories for extragalactic FRBs ...
Alice P. Curtin +23 more
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