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Related papers: Axion-photon conversion of GRB221009A

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The detection of very high-energy neutrinos by IceCube experiment supports the existence of a comparable gamma-ray counterpart from the same cosmic accelerators. Under the likely assumption that the sources of these particles are of…

We search for possible GeV-TeV gamma-ray imprints of ultrahigh-energy (UHE; $\gtrsim 0.1$ EeV) cosmic ray (CR) acceleration in the large-scale structures surrounding the brightest gamma-ray burst (GRB) explosion, GRB 221009A. Using 1.25…

High Energy Astrophysical Phenomena · Physics 2025-04-23 Saikat Das , Soebur Razzaque , Nestor Mirabal , Nicola Omodei , Kohta Murase , Israel Martinez-Castellanos

A search for solar axions has been performed using an axion helioscope which is equipped with a 2.3m-long 4T superconducting magnet, a gas container to hold dispersion-matching gas, PIN-photodiode X-ray detectors, and a telescope mount…

Astrophysics · Physics 2011-06-07 Y. Inoue , Y. Akimoto , R. Ohta , T. Mizumoto , A. Yamamoto , M. Minowa

The brightest ever gamma-ray burst (GRB) 221009A displays a significant emission line component around 10 MeV. As the GRB central engine is neutron-rich, we propose that the emission line could be originally due to the 2.223 MeV gamma-rays…

High Energy Astrophysical Phenomena · Physics 2025-04-02 Jiahuan Zhu , Hua Feng , Tong Liu

Axions produced copiously in core-collapse supernovae can convert into photons as they propagate through various astrophysical magnetic fields. The cumulative emission from the cosmic population of supernovae can therefore generate a…

High Energy Physics - Phenomenology · Physics 2026-04-21 Brijesh Kanodia , Debajit Bose , Subhadip Bouri , Ranjan Laha

We present the IXPE observation of GRB 221009A which includes upper limits on the linear polarization degree of both prompt and afterglow emission in the soft X-ray energy band. GRB 221009A is an exceptionally bright gamma-ray burst (GRB)…

High Energy Astrophysical Phenomena · Physics 2023-05-22 Michela Negro , Niccoló Di Lalla , Nicola Omodei , Péter Veres , Stefano Silvestri , Alberto Manfreda , Eric Burns , Luca Baldini , Enrico Costa , Steven R. Ehlert , Jamie A. Kennea , Ioannis Liodakis , Herman L. Marshall , Sandro Mereghetti , Riccardo Middei , Fabio Muleri , Stephen L. O'Dell , Oliver J. Roberts , Roger W. Romani , Carmelo Sgró , Alessandro Di Marco , Simonetta Puccetti , Masanobu Terashima , Andrea Tiengo , Domenico Viscolo , Fabio La Monaca , Luca Latronico , Giorgio Matt , Matteo Perri , Juri Poutanen , Ajay Ratheesh , Daniele Rogantini , Patrick Slane , Paolo Soffitta , Elina Lindfors , Kari Nilsson , Anni Kasikov , Alan P. Marscher , Fabrizio Tavecchio , Shuichi Gunji , Christian Malacaria , Alessandro Paggi , Yi-Jung Yang , Silvia Zane , Martin C. Weisskopf , Iván Agudo , Lucio A. Antonelli , Wayne H. Baumgartner , Ronaldo Bellazzini , Stefano Bianchi , Raffaella Bonino , Alessandro Brez , Niccol Bucciantini , Simone Castellano , Elisabetta Cavazzuti , Chien-Ting Chen , Alessandra De Rosa , Ettore Del Monte , Laura Di Gesu , Immacolata Donnarumma , Victor Doroshenko , Michal Dovciak , Teruaki Enoto , Matteo Bachetti , Stephen D. Bongiorno , Fiamma Capitanio , Stefano Ciprini , Yuri Evangelista , Sergio Fabiani , Riccardo Ferrazzoli , Javier A. Garcia , Kiyoshi Hayashida , Jeremy Heyl , Wataru Iwakiri , Svetlana G. Jorstad , Philip Kaaret , Vladimir Karas , Fabian Kislat , Takao Kitaguchi , Jeffery J. Kolodziejczak , Henric Krawczynski , Simone Maldera , Frédéric Marin , Andrea Marinucci , Ikuyuki Mitsuishi , Tsunefumi Mizuno , C. -Y. Ng , Chiara Oppedisano , Alessandro Papitto , George G. Pavlov , Abel L. Peirson , Melissa Pesce-Rollins , Pierre-Olivier Petrucci , Brian D. Ramsey , John Rankin , Gloria Spandre , Maura Pilia , Andrea Possenti , Douglas A. Swartz , Toru Tamagawa , Roberto Taverna , Yuzuru Tawara , Allyn F. Tennant , Nicholas E. Thomas , Francesco Tombesi , Alessio Trois , Sergey S. Tsygankov , Roberto Turolla , Jacco Vink , Kinwah Wu , Fei Xie

Very-high energy photons emitted by distant cosmic sources are absorbed on the extragalactic background light (EBL) during their propagation. This effect can be characterized in terms of a photon transfer function at Earth. The presence of…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Alessandro Mirizzi , Daniele Montanino

Heavy axion-like particles have been introduced in several scenarios beyond the Standard Model and their production in some astrophysical systems should be possible. In this work, we re-examine the possibility that these type of particles…

High Energy Astrophysical Phenomena · Physics 2017-12-06 Matias M. Reynoso

We show that photons with energies above the GZK cutoff can reach us from very distant sources if they mix with light axions in extragalactic magnetic fields. The effect which enables this is the conversion of photons into axions, which are…

High Energy Physics - Phenomenology · Physics 2009-09-17 Csaba Csaki , Nemanja Kaloper , Marco Peloso , John Terning

The Pseudo-Goldstone Boson (PGB) emission could provide a very efficient mechanism for explaining the cosmic Gamma Ray Bursts (GRBs). The PGBs could be produced during the merging of two compact objects like two neutron stars or neutron…

High Energy Physics - Phenomenology · Physics 2009-10-31 Zurab Berezhiani , Alessandro Drago

Gamma Ray Bursts are being searched in many ground based experiments detecting the high energy component (GeV $\div$ TeV energy range) of the photon bursts. In this paper, Fluorescence Detectors are considered as possible candidate devices…

Astrophysics · Physics 2013-06-11 R. Aloisio , D. Boncioli , A. F. Grillo , C. Macolino , S. Petrera , P. Privitera , V. Rizi , F. Salamida

The recent detection of a transient absorption feature in the prompt emission of GRB 990705 has sparked multiple attempts to fit this feature in terms of photoelectric absorption or resonance scattering out of the line of sight to the…

Astrophysics · Physics 2009-11-07 M. Boettcher , C. L. Fryer , C. D. Dermer

Recent experiments suggest that polarized photons may couple significantly to pseudoscalar particles such as axions. We study the possible observational signatures of axion-photon coupling for radiation from magnetic stars, with particular…

Astrophysics · Physics 2008-11-26 Dong Lai , Jeremy Heyl

As very high energy (~100 GeV) gamma rays travel over cosmological distances, their flux is attenuated through interactions with the extragalactic background light. Observations of distant gamma ray sources at energies between ~200 GeV and…

High Energy Astrophysical Phenomena · Physics 2011-03-31 Alexander V. Belikov , Lisa Goodenough , Dan Hooper

The tera-electronvolt (TeV) light curve of gamma-ray burst (GRB) 221009A shows an unprecedentedly rapid rise at the beginning epoch. This phenomenon could be due to the strong absorption of photons and electrons within the emitting region.…

High Energy Astrophysical Phenomena · Physics 2023-12-08 Jun-Yi Shen , Yuan-Chuan Zou , A. M. Chen , Duan-Yuan Gao

Axion-Like Particles (ALPs), if exist in nature, are expected to mix with photons in the presence of an external magnetic field. The energy range of photons which undergo strong mixing with ALPs depends on the ALP mass, on its coupling with…

High Energy Astrophysical Phenomena · Physics 2013-11-13 Olga Mena , Soebur Razzaque

Photons couple to Axion-Like Particles (ALPs) or more generally to any pseudo Nambu-Goldstone boson in the presence of an external electromagnetic field. Mixing between photons and ALPs in the strong magnetic field of a Gamma-Ray Burst…

High Energy Astrophysical Phenomena · Physics 2011-03-18 Olga Mena , Soebur Razzaque , F. Villaescusa-Navarro

Axion-Like Particles (ALPs) are the focus of intense current research. We analyze photon-ALP conversion in the context of relativistic jet models of Active Galactic Nuclei (AGN) for more than 100 sources. Contrary to previous claims, we…

High Energy Astrophysical Phenomena · Physics 2009-05-26 Nicola Bassan , Marco Roncadelli

Gamma-rays from cosmological sources contain information about gamma-ray interactions. Standard model and non-standard model photon interactions along the path between the source and the observer can lead to changes in the energy or state…

High Energy Astrophysical Phenomena · Physics 2014-08-19 Rebecca Reesman , T. P. Walker

For the first time, we predict the axion spectra and their associated luminosities for several low-mass stars -- one and two solar masses stars in the main sequence and post-main sequence stages of evolution. Equally, we also compute the…

High Energy Astrophysical Phenomena · Physics 2021-08-03 Ilídio Lopes
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