Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons
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-energy neutrinos come out about 300 s earlier th...
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doaj-6267c01e75504025acbf0ab632b3684d2021-10-09T04:36:09ZengElsevierPhysics Letters B0370-26932021-09-01820136546Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photonsJie Zhu0Bo-Qiang Ma1School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, ChinaSchool of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China; Center for High Energy Physics, Peking University, Beijing 100871, China; Collaborative Innovation Center of Quantum Matter, Beijing, China; Corresponding author at: School of Physics, Peking University, Beijing 100871, China.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-energy neutrinos come out about 300 s earlier than low-energy photons in the source reference system. Considering the possibility that pre-bursts of neutrinos may be accompanied by high-energy photons, in this work we search for high-energy photon events with earlier emission time from 100 to 1000 s before low-energy photons at source by analyzing Fermi Gamma-ray Space Telescope (FGST) data. We perform the searching of photon events with energies larger than 100 MeV, and find 14 events from 48 GRBs with known redshifts. Combining these events with a 1.07TeV photon event observed by the Major Atmospheric Gamma Imaging Cherenkov telescopes (MAGIC), we suggest a pre-burst stage with a long duration period of several minutes of high energy neutrino emissions accompanied by high energy photons at the GRB source.http://www.sciencedirect.com/science/article/pii/S037026932100486XPre-burstGamma ray burstLight speed variationNeutrino speed variationLorentz invariance violation |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Jie Zhu Bo-Qiang Ma |
spellingShingle |
Jie Zhu Bo-Qiang Ma Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons Physics Letters B Pre-burst Gamma ray burst Light speed variation Neutrino speed variation Lorentz invariance violation |
author_facet |
Jie Zhu Bo-Qiang Ma |
author_sort |
Jie Zhu |
title |
Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
title_short |
Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
title_full |
Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
title_fullStr |
Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
title_full_unstemmed |
Pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
title_sort |
pre-burst neutrinos of gamma-ray bursters accompanied by high-energy photons |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2021-09-01 |
description |
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-energy neutrinos come out about 300 s earlier than low-energy photons in the source reference system. Considering the possibility that pre-bursts of neutrinos may be accompanied by high-energy photons, in this work we search for high-energy photon events with earlier emission time from 100 to 1000 s before low-energy photons at source by analyzing Fermi Gamma-ray Space Telescope (FGST) data. We perform the searching of photon events with energies larger than 100 MeV, and find 14 events from 48 GRBs with known redshifts. Combining these events with a 1.07TeV photon event observed by the Major Atmospheric Gamma Imaging Cherenkov telescopes (MAGIC), we suggest a pre-burst stage with a long duration period of several minutes of high energy neutrino emissions accompanied by high energy photons at the GRB source. |
topic |
Pre-burst Gamma ray burst Light speed variation Neutrino speed variation Lorentz invariance violation |
url |
http://www.sciencedirect.com/science/article/pii/S037026932100486X |
work_keys_str_mv |
AT jiezhu preburstneutrinosofgammarayburstersaccompaniedbyhighenergyphotons AT boqiangma preburstneutrinosofgammarayburstersaccompaniedbyhighenergyphotons |
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