Search for High-Energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

V. L. Zurbanov; V. D. Rushay; E. V. Rjabov; M. I. Rozanov; E. N. Pliskovsky; D. P. Petukhov; L. V. Pan’kov; A. I. Panfilov; E. R. Osipova; R. A. Mirgazov; M. B. Milenin; D. A. Kuleshov; G. B. Safronov; F. Simkovic; A. V. Zagorodnikov; S. A. Yakovlev; B. A. Tarashansky; V. A. Tabolenko; O. V. Suvorova; I. Shtekl; M. D. Shelepov; M. N. Sorokovikov; A. G. Solovjev; B. A. Shoibonov; A. V. Skurikhin; V. F. Kulepov; V. A. Kozhin; Zh.-A. M. Dzhilkibaev; A. N. Dyachok; R. Dvornický; G. V. Domogatsky; A. A. Doroshenko; N. M. Budnev; V. M. Brudanin; I. A. Belolaptikov; R. Bannash; V. M. Aynutdinov; A. V. Avrorin; L. Fajt; S. V. Fialkovsky; A. P. Koshechkin; A. P. Korobchenko; K. V. Konischev; M. M. Kolbin; E. V. Khramov; O. G. Kebkal; K. G. Kebkal; Z. Honz; T. I. Gres; K. V. Golubkov; A. R. Gafarov; A. D. Avrorin

doi:10.1134/S0021364018240025

Search for High-Energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

Autores: Zurbanov V.L.¹, Rushay V.D.², Rjabov E.V.¹, Rozanov M.I.³, Pliskovsky E.N.², Petukhov D.P.¹, Pan’kov L.V.¹, Panfilov A.I.⁴, Osipova E.R.⁵, Mirgazov R.A.¹, Milenin M.B.⁶, Kuleshov D.A.⁴, Safronov G.B.², Simkovic F.²^,7, Zagorodnikov A.V.¹, Yakovlev S.A.⁸, Tarashansky B.A.¹, Tabolenko V.A.¹, Suvorova O.V.⁴, Shtekl I.²^,9, Shelepov M.D.⁴, Sorokovikov M.N.², Solovjev A.G.², Shoibonov B.A.², Skurikhin A.V.⁵, Kulepov V.F.⁶, Kozhin V.A.⁵, Dzhilkibaev Z.M.⁴, Dyachok A.N.¹, Dvornický R.²^,7, Domogatsky G.V.⁴, Doroshenko A.A.⁴, Budnev N.M.¹, Brudanin V.M.², Belolaptikov I.A.², Bannash R.⁸, Aynutdinov V.M.⁴, Avrorin A.V.⁴, Fajt L.²^,7^,9, Fialkovsky S.V.⁶, Koshechkin A.P.⁴, Korobchenko A.P.², Konischev K.V.², Kolbin M.M.², Khramov E.V.², Kebkal O.G.⁸, Kebkal K.G.⁸, Honz Z.², Gres T.I.¹, Golubkov K.V.⁴, Gafarov A.R.¹, Avrorin A.D.⁴
Afiliações:
1. Irkutsk State University
2. Joint Institute for Nuclear Research
3. St. Petersburg State Marine Technical University
4. Institute for Nuclear Research
5. Skobeltsyn Institute of Nuclear Physics
6. Nizhny Novgorod State Technical University
7. Comenius University
8. EvoLogics
9. Czech Technical University
Edição: Volume 108, Nº 12 (2018)
Páginas: 787-790
Seção: Fields, Particles, and Nuclei
URL: https://journals.rcsi.science/0021-3640/article/view/161352
DOI: https://doi.org/10.1134/S0021364018240025
ID: 161352

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The Advanced Laser Interferometer Gravitational-Wave Observatory and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst that followed the merger of this binary was also recorded by Fermi gamma-ray burst monitor and International Gamma-Ray Astrophysics Laboratory, indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the energy range of 1 TeV–100 PeV using the Baikal Gigaton Volume Detector. No neutrinos directionally coincident with the source were detected within ±500 s around the merger time, as well as during a 14-day period after the gravitational wave detection. We derived 90% C.L. upper limits on the neutrino fluence from GW170817 during a ±500 s window centered on the gravitational wave trigger time, and a 14-day window following the gravitational wave signal under the assumption of an E⁻² neutrino energy spectrum.

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Search for High-Energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

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