2001/01/05 by P. Tricarico, A. Ortolan, A. Solaroli +13 · 13 citations
Physics and Astronomy · #Amplitude #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Correlation #Gamma-ray burst #Gamma-ray bursts and supernovae #Geometry #Gravitational wave #Gravitational-wave observatory #Optics #Physics #Pulsars and Gravitational Waves Research #gr-qc
paper · pdf · doi:10.1103/physrevd.63.082002
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 63(8) (American Physical Society) · 7 pages, 3 figures, submitted to Phys. Rev. D
arxiv created 2001/01/05 · openalex publication_date 2001/03/19 · arxiv updated 2019/08/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The cosmological origin of \ensuremathγ-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\ifmmode×\else\texttimes\fi10^\ensuremath-18 on the averaged amplitude of gravitational waves associated with \ensuremathγ-ray bursts has been set for the first time.