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The methodology of the search for a correlated signal from a supernova explosion using the data of gravitational wave detectors and neutrino observatories

  • The International Session-Conference of SNP PSD RAS “Physics of Fundamental Interactions”
  • Session 6—Neutrino Physics
  • Published:
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Abstract

The proposed methodology developed in cooperation of the LIGO, VIRGO, Borexino, LVD, and IceCube collaborations is based on a joint analysis of data from neutrino and gravitational wave detectors which record corresponding radiations, almost undistorted by the interstellar medium and propagating with similar speeds. This approach allows to increase the reliability of observations, detect the so-called Silent supernovae and explore the properties and generation mechanisms of gravitational waves.

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Authors and Affiliations

  1. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119234, Russia

    M. B. Gromov

  2. Faculty of Physics, Moscow State University, Moscow, 119234, Russia

    M. B. Gromov

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  1. M. B. Gromov
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Correspondence to M. B. Gromov.

Additional information

Original Russian Text © M.B. Gromov, 2017, published in Fizika Elementarnykh Chastits i Atomnogo Yadra, 2017, Vol. 48, No. 6.

Talk at the International Session-Conference of SNP PSD RAS “Physics of Fundamental Interactions”, JINR, Dubna, April 12–15, 2016.

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Gromov, M.B. The methodology of the search for a correlated signal from a supernova explosion using the data of gravitational wave detectors and neutrino observatories. Phys. Part. Nuclei 48, 977–980 (2017). https://doi.org/10.1134/S1063779617060181

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  • DOI: https://doi.org/10.1134/S1063779617060181

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