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Neutrino Astrophysics with the MACRO Detector

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Gamma-Ray Bursts in the Afterglow Era

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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Abstract.

A sample of 1197 neutrino induced upward-going muons is used to look for point-like sources and for space-time correlations with BATSE and BeppoSAX gammaray bursts. We set an upper limit (90% c.l.) of 6.9 10-10 cm-2 upward-going muons per average burst. A search for high multiplicity events in coincidence with GRBs has been performed using the supernova trigger.

Teresa Montaruli: for the MACRO Collaboration

Fabrizio Cei: for the MACRO Collaboration

Roberto Pazzi: for the MACRO Collaboration

Francesco Ronga: for the MACRO Collaboration

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Authors and Affiliations

  1. Dipartimento di Fisica dell’Università di Bari and I.N.F.N., 70126, Bari

    Teresa Montaruli

  2. Dipartimento di Fisica dell’Università di Pisa and I.N.F.N., 56010, Pisa

    Fabrizio Cei & Roberto Pazzi

  3. Laboratori Nazionali di Frascati dell’I.N.F.N., 00044, Frascati (Roma)

    Teresa Montaruli & Francesco Ronga

Authors
  1. Teresa Montaruli
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  2. Fabrizio Cei
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  3. Roberto Pazzi
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  4. Francesco Ronga
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Editor information

Enrico Costa Filippo Frontera Jens Hjorth

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Montaruli, T., Cei, F., Pazzi, R., Ronga, F. Neutrino Astrophysics with the MACRO Detector. In: Costa, E., Frontera, F., Hjorth, J. (eds) Gamma-Ray Bursts in the Afterglow Era. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10853853_20

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  • DOI: https://doi.org/10.1007/10853853_20

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-42771-1

  • Online ISBN: 978-3-540-45505-9

  • eBook Packages: Springer Book Archive

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