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Related papers: Diffuse PeV neutrinos from gamma-ray bursts

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The recent IceCube detection of significant neutrino flux from the inner Galactic plane has provided us valuable insights on the spectrum of cosmic rays in our Galaxy. This flux can be produced either by a population of Galactic point…

High Energy Astrophysical Phenomena · Physics 2024-06-04 Abhijit Roy , Jagdish C. Joshi , Martina Cardillo , Prantik Sarmah , Ritabrata Sarkar , Sovan Chakraborty

The IceCube neutrino discovery presents an opportunity to answer long-standing questions in high-energy astrophysics. For their own sake and relations to other processes, it is important to understand neutrinos arising from the Milky Way,…

High Energy Astrophysical Phenomena · Physics 2015-11-18 Matthew D. Kistler

We show that a significant fraction of the energy of a gamma-ray burst(GRB) is probably converted to a burst of 10^{17}-10^{19} eV neutrinos and multiple GeV gammas that follow the GRB by > 10 s . If, as previously suggested, GRB's…

High Energy Physics - Phenomenology · Physics 2010-04-06 Eli Waxman , John Bahcall

Over the last 15 years there has been considerable interest in the possibility of quantum-gravity-induced in-vacuo dispersion, the possibility that spacetime itself might behave essentially like a dispersive medium for particle propagation.…

High Energy Astrophysical Phenomena · Physics 2017-06-13 Giovanni Amelino-Camelia , Giacomo D'Amico , Giacomo Rosati , Niccoló Loret

We argue that the excess of sub-PeV/PeV neutrinos recently reported by IceCube could plausibly originate through pion-production processes in the same sources responsible for cosmic rays (CRs) with energy above the second knee around…

High Energy Astrophysical Phenomena · Physics 2014-04-23 Ruo-Yu Liu , Xiang-Yu Wang , Susumu Inoue , Roland Crocker , Felix Aharonian

A search for neutrinos produced in coincidence with Gamma-Ray Bursts(GRB) was conducted with the Super-Kamiokande (SK) detector. Between December 2008 and March 2017, the Gamma-ray Coordinates Network recorded 2208 GRBs that occurred during…

High Energy Astrophysical Phenomena · Physics 2021-06-29 Kamiokande Collaboration , A. Orii , K. Abe , C. Bronner , Y. Hayato , M. Ikeda , S. Imaizumi , H. Ito , J. Kameda , Y. Kataoka , Y. Kato , Y. Kishimoto , M. Miura , S. Moriyama , T. Mochizuki , Y. Nagao , M. Nakahata , Y. Nakajima , S. Nakayama , T. Okada , K. Okamoto , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , T. Yano , S. Han , T. Kajita , K. Okumura , T. Tashiro , R. Wang , J. Xia , G. D. Megias , D. Bravo-Berguno , L. Labarga , Ll. Marti , B. Zaldivar , F. d. M. Blaszczyk , E. Kearns , J. L. Raaf , J. L. Stone , L. Wan , T. Wester , B. W. Pointon , J. Bian , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , M. B. Smy , H. W. Sobel , V. Takhistov , P. Weatherly , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , L. Bernard , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , M. Gonin , Th. A. Mueller , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , S. Matsuno , L. H. V. Anthony , R. P. Litchfield , A. A. Sztuc , Y. Uchida , V. Berardi , M. G. Catanesi , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , N. Ospina , L. Ludovici , Y. Nishimura , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , T. Boschi , F. Di Lodovico , S. Molina Sedgwick , M. Taani , S. Zsoldos , M. Hasegawa , Y. Isobe , H. Miyabe , Y. Nakano , T. Shiozawa , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , A. Ali , Y. Ashida , J. Feng , S. Hirota , M. Jiang , A. K. Ichikawa , T. Kikawa , M. Mori , KE. Nakamura , T. Nakaya , R. A. Wendell , K. Yasutome , P. Fernandez , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , T. Niwa , K. Sato , M. Tsukada , P. Mijakowski , K. Frankiewicz , C. K. Jung , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , M. Harada , K. Hagiwara , T. Horai , H. Ishino , S. Ito , Y. Koshio , W. Ma , N. Piplani , S. Sakai , M. Sakuda , Y. Takahira , C. Xu , Y. Kuno , G. Barr , D. Barrow , L. Cook , A. Goldsack , S. Samani , C. Simpson , D. Wark , F. Nova , J. Y. Yang , S. J. Jenkins , M. Malek , J. M. McElwee , O. Stone , M. D. Thiesse , L. F. Thompson , H. Okazawa , Y. Choi , S. B. Kim , I. Yu , K. Nishijima , M. Koshiba , K. Iwamoto , N. Ogawa , M. Yokoyama , K. Martens , M. R. Vagins , S. Izumiyama , M. Kuze , M. Tanaka , T. Yoshida , M. Inomoto , M. Ishitsuka , R. Matsumoto , K. Ohta , M. Shinoki , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , R. Akutsu , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , M. Posiadala-Zezula , B. Richards , B. Jamieson , J. Walker , A. Minamino , K. Okamoto , G. Pintaudi , R. Sasaki

We present the results of a Monte-Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the…

Astrophysics · Physics 2008-11-26 The IceCube Collaboration , J. Ahrens

Gamma-ray bursts (GRBs) are expected to provide a source of ultra high energy cosmic rays, accompanied with potentially detectable neutrinos at neutrino telescopes. Recently, IceCube has set an upper bound on this neutrino flux well below…

High Energy Physics - Phenomenology · Physics 2013-11-21 L. Dorame , O. G. Miranda , J. W. F. Valle

Gamma-ray bursts (GRB) are generally believed to be efficient particle accelerators. In the presence of energetic protons in a GRB jet, interactions between these protons and intense radiation field of the GRB are supposed to induce…

High Energy Astrophysical Phenomena · Physics 2023-02-01 Ruo-Yu Liu , Hai-Ming Zhang , Xiang-Yu Wang

Despite the spectacular discovery of an astrophysical neutrino flux by IceCube in 2013, its origin remains a mystery. Whatever its sources, we expect the neutrino flux to be accompanied by a comparable gamma-ray flux. These photons should…

High Energy Physics - Phenomenology · Physics 2021-02-23 Antonio Capanema , Arman Esmaili , Pasquale Dario Serpico

The discovery of extraterrestrial very-high-energy neutrinos by the IceCube collaboration has launched a quest for the identification of their astrophysical sources. Gamma-ray blazars have been predicted to yield a cumulative neutrino…

We revisit the neutrino and ultra high-energy cosmic ray (UHECR) production from gamma-ray bursts (GRBs) with time-dependent simulations for the proton-induced cascades. This method can generate self-consistent photon, neutrino and escaped…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Katsuaki Asano , Peter Meszaros

The number of neutrino induced upward going muons from a single Gamma Ray Burst (GRB) expected to be detected by the proposed kilometer scale IceCube detector at the South Pole location has been calculated. The effects of the Lorentz…

Astrophysics · Physics 2010-11-15 Nayantara Gupta

The origins of the diffuse flux of cosmogenic PeV neutrinos detected in the IceCube experiment during 2010 - 2017 remain unidentified. A population of extragalactic newly born fast spinning pulsars are investigated as possible candidates…

High Energy Astrophysical Phenomena · Physics 2021-11-09 Rajat K. Dey , Animesh Basak , Sabyasachi Ray , Tamal Sarkar

The recent extremely bright gamma-ray burst (GRB), GRB 230307A from a binary neutron star merger may offer a good probe for the production of GRB-neutrinos. Within the constraint from IceCube neutrino non-detection, the limits for key…

High Energy Astrophysical Phenomena · Physics 2023-11-21 Xin-Ying Song

Gamma Ray Burst sources are apparently evolving around us in a harder and brighter samples at far and far redshift. The average output may range from a near Supernova (nearest events) output to a billion time that power for most distant…

High Energy Astrophysical Phenomena · Physics 2012-06-18 Daniele Fargion

The IceCube Collaboration has recently reported evidence for a high-energy extraterrestrial neutrino flux. During two years of operation 28 events with energies between 30 TeV and 1.2 PeV were observed while only 10.6 events were expected…

High Energy Astrophysical Phenomena · Physics 2014-07-16 Markus Ahlers , Kohta Murase

The IceCube neutrino discovery was punctuated by three showers with $E_\nu$ ~ 1-2 PeV. Interest is intense in possible fluxes at higher energies, though a marked deficit of $E_\nu$ ~ 6 PeV Glashow resonance events implies a spectrum that is…

High Energy Astrophysical Phenomena · Physics 2018-06-27 Matthew D. Kistler , Ranjan Laha

Starburst galaxies represent one of the most plausible origins of the cosmic high-energy neutrino flux recently discovered by IceCube. At $\sim$ PeV energies, the neutrino flux from starburst galaxies is expected to exhibit a characteristic…

High Energy Astrophysical Phenomena · Physics 2015-09-22 I. Bartos , S. Marka

Gamma-ray bursts (GRB) are powerful and highly variable sources of gamma rays that indicate the existence of cosmic particle accelerators. Under the assumption of hadronic acceleration in the jet, the expected neutrino energy spectrum is…

Astrophysics · Physics 2008-10-09 D. Dornic , G. Lelaizant
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