Correlation between gamma-ray bursts and gravitational waves

P. Tricarico, A. Ortolan, A. Solaroli, G. Vedovato, L. Baggio, M. Cerdonio, L. Taffarello, J. Zendri, R. Mezzena, G. A. Prodi, S. Vitale, P. Fortini, M. Bonaldi, and P. Falferi
Phys. Rev. D 63, 082002 – Published 19 March 2001
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Abstract

The cosmological origin of γ-ray bursts (GRB’s) is now commonly accepted and, according to several models for the central engine, GRB sources should also emit at the same time gravitational wave bursts (GWB’s). We have performed two correlation searches between the data of the resonant gravitational wave detector AURIGA and GRB arrival times collected in the BATSE 4B catalogue. No correlation was found and an upper limit hRMS<~1.5×1018 on the averaged amplitude of gravitational waves associated with γ-ray bursts has been set for the first time.

  • Received 20 November 2000

DOI:https://doi.org/10.1103/PhysRevD.63.082002

©2001 American Physical Society

Authors & Affiliations

P. Tricarico*, A. Ortolan, A. Solaroli, and G. Vedovato

  • I.N.F.N., Laboratori Nazionali di Legnaro, via Romea, 4, I-35020 Legnaro, Padova, Italy

L. Baggio, M. Cerdonio, L. Taffarello, and J. Zendri

  • Physics Department, University of Padova and I.N.F.N. Sezione di Padova, Via Marzolo, 8, I-35100 Padova, Italy

R. Mezzena, G. A. Prodi, and S. Vitale

  • Physics Department, University of Trento and I.N.F.N. Gruppo Collegato di Trento, Sezione di Padova, I-38050 Povo, Italy

P. Fortini

  • Physics Department, University of Ferrara, and I.N.F.N. Sezione di Ferrara, via Paradiso, 12, I-44100 Ferrara, Italy

M. Bonaldi and P. Falferi

  • Centro di Fisica degli Stati Aggregati, I.T.C.-C.N.R., Trento, Italy
  • I.N.F.N. Gruppo Collegato di Trento, Sezione di Padova, I-38050 Povo, Italy

  • *Corresponding author. Email address: pasquale.tricarico@lnl.infn.it

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Issue

Vol. 63, Iss. 8 — 15 April 2001

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