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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Main Authors: Jie Zhu, Bo-Qiang Ma
Format: Article
Language:English
Published: Elsevier 2021-09-01
Series:Physics Letters B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S037026932100486X
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spelling 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
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AT boqiangma preburstneutrinosofgammarayburstersaccompaniedbyhighenergyphotons
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