A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era

We describe the theoretical modeling and analysis techniques associated with a preliminary search for correlated neutrino emission from GRB980703a, which triggered the Burst and Transient Source Experiment (BATSE GRB trigger 6891), using archived data from the Antarctic Muon and Neutrino Detector Ar...

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Main Authors: Stamatikos, Michael, Band, David
Format: Text
Language:unknown
Published: arXiv 2006
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Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0602481
https://arxiv.org/abs/astro-ph/0602481
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spelling ftdatacite:10.48550/arxiv.astro-ph/0602481 2023-05-15T13:56:22+02:00 A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era Stamatikos, Michael Band, David 2006 https://dx.doi.org/10.48550/arxiv.astro-ph/0602481 https://arxiv.org/abs/astro-ph/0602481 unknown arXiv https://dx.doi.org/10.1063/1.2207961 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2006 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0602481 https://doi.org/10.1063/1.2207961 2022-04-01T15:57:26Z We describe the theoretical modeling and analysis techniques associated with a preliminary search for correlated neutrino emission from GRB980703a, which triggered the Burst and Transient Source Experiment (BATSE GRB trigger 6891), using archived data from the Antarctic Muon and Neutrino Detector Array (AMANDA-B10). Under the assumption of associated hadronic acceleration, the expected observed neutrino energy flux is directly derived, based upon confronting the fireball phenomenology with the discrete set of observed electromagnetic parameters of GRB980703a, gleaned from ground-based and satellite observations, for four models, corrected for oscillations. Models 1 and 2, based upon spectral analysis featuring a prompt photon energy fit to the Band function, utilize an observed spectroscopic redshift, for isotropic and anisotropic emission geometry, respectively. Model 3 is based upon averaged burst parameters, assuming isotropic emission. Model 4, based upon a Band fit, features an estimated redshift from the lag-luminosity relation with isotropic emission. Consistent with our AMANDA-II analysis of GRB030329, which resulted in a flux upper limit of ~0.150 GeV/cm^2/s for model 1, we find differences in excess of an order of magnitude in the response of AMANDA-B10, among the various models for GRB980703a. Implications for future searches in the era of Swift and IceCube are discussed. : 7 pages, 4 figures, 4 tables, Contributed to the Proceedings of The 16th Annual Astrophysics Conference in Maryland: Gamma Ray Bursts in the Swift Era. Edited by Stephen S. Holt, Neil Gehrels and John A. Nousek (2006) Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Stamatikos, Michael
Band, David
A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We describe the theoretical modeling and analysis techniques associated with a preliminary search for correlated neutrino emission from GRB980703a, which triggered the Burst and Transient Source Experiment (BATSE GRB trigger 6891), using archived data from the Antarctic Muon and Neutrino Detector Array (AMANDA-B10). Under the assumption of associated hadronic acceleration, the expected observed neutrino energy flux is directly derived, based upon confronting the fireball phenomenology with the discrete set of observed electromagnetic parameters of GRB980703a, gleaned from ground-based and satellite observations, for four models, corrected for oscillations. Models 1 and 2, based upon spectral analysis featuring a prompt photon energy fit to the Band function, utilize an observed spectroscopic redshift, for isotropic and anisotropic emission geometry, respectively. Model 3 is based upon averaged burst parameters, assuming isotropic emission. Model 4, based upon a Band fit, features an estimated redshift from the lag-luminosity relation with isotropic emission. Consistent with our AMANDA-II analysis of GRB030329, which resulted in a flux upper limit of ~0.150 GeV/cm^2/s for model 1, we find differences in excess of an order of magnitude in the response of AMANDA-B10, among the various models for GRB980703a. Implications for future searches in the era of Swift and IceCube are discussed. : 7 pages, 4 figures, 4 tables, Contributed to the Proceedings of The 16th Annual Astrophysics Conference in Maryland: Gamma Ray Bursts in the Swift Era. Edited by Stephen S. Holt, Neil Gehrels and John A. Nousek (2006)
format Text
author Stamatikos, Michael
Band, David
author_facet Stamatikos, Michael
Band, David
author_sort Stamatikos, Michael
title A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
title_short A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
title_full A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
title_fullStr A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
title_full_unstemmed A New Search Paradigm for Correlated Neutrino Emission from Discrete GRBs using Antarctic Cherenkov Telescopes in the Swift Era
title_sort new search paradigm for correlated neutrino emission from discrete grbs using antarctic cherenkov telescopes in the swift era
publisher arXiv
publishDate 2006
url https://dx.doi.org/10.48550/arxiv.astro-ph/0602481
https://arxiv.org/abs/astro-ph/0602481
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
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Antarctic
genre_facet Antarc*
Antarctic
op_relation https://dx.doi.org/10.1063/1.2207961
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0602481
https://doi.org/10.1063/1.2207961
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