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.
Similar content being viewed by others
References
C. D. Ott, “The gravitational wave signature of corecollapse supernovae”, Class. Quant. Grav. 26, 063001 (2009).
B. P. Abbott et al. (LIGO Scientific Collab. and Virgo Collab.), “Observation of gravitational waves from a binary black hole merger”, Phys. Rev. Lett. 116(6), 061102 (2016).
N. Y. Agafonova et al. (LVD Collab.), “Implication for the core collapse supernova rate from 21 years of data of the Large Volume Detector”, Ap. J. 802(1), 47 (2015); arXiv:1411.1709v2.
B. P. Abbott et al. (LIGO Scientific Collab. and Virgo Collab.), “Prospects for observing and localizing gravitational- wave transients with Advanced LIGO and Advanced Virgo”, Living Reviews in Relativity, 19, 1 (2016); arXiv:1304.0670v3.
J. Aasi et al. (LIGO Scientific Collab. and Virgo Collab.), “Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO600, LIGO, and Virgo detectors”, Phys. Rev. D 89, 122004 (2014); arXiv:1405.1053v2.
P. Antonioli, et al., “SNEWS: The SuperNova early warning system”, New J. Phys. 6, 114 (2004); arXiv:astro-ph/0406214v2.
K. Scholberg, “The SuperNova early warning system”, Astron. Nachr. 329(3), 337–339 (2008); arXiv:0803.0531v1.
P. J. Sutton, “Upper limits from counting experiments with multiple pipelines”, Class. Quant. Grav. 26(24), 245007 (2009); arXiv:0905.4089v2.
S. Klimenko, I. Yakushin, A. Mercer, G. Mitselmakher, “A coherent method for detection of gravitational wave bursts”, Class. Quant. Grav. 25(11), 114029 (2008); arXiv:0802.3232v2.
W. Fulgione, N. Mengotti-Silva, L. Panaro, “Neutrino burst identification in underground detectors”, NIMPA 368(2), 512–516 (1996).
G. Pagliaroli, F. Vissani, M. L. Costantini, A. Ianni, “Improved analysis of SN1987A antineutrino events”, Astropart. Phys. 31(3), 163–176 (2009); arXiv:0810.0466v1.
T. Totani, K. Sato, H. E. Dalhed, J. R. Wilson, “Future detection of supernova neutrino burst and explosion mechanism”, Astrophys. J. 496(1), 216–225 (1998); arXiv:astro-ph/9710203v1.
L. Hüdepohl, B. Müller, H.-Th. Janka, A. Marek, G. G. Raffelt, “Neutrino signal of electron-capture supernovae from core collapse to cooling”, Phys. Rev. Lett. 104(25), 251101 (2010); Erratum-ibid. 105(24), 249901 (2010); arXiv:0912.0260v3.
K. Sumiyoshi, S. Yamada, H. Suzuki, “Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence”, Astrophys. J. 667(1), 382–394 (2007); arXiv:0706.3762v1.
Author information
Authors and Affiliations
Corresponding author
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.
Rights and permissions
About this article
Cite this article
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
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063779617060181