Erratum: “A Search for Electron Antineutrinos Associated with Gravitational-wave Events GW150914 and GW151226 Using KamLAND” (2016, ApJL, 829, L34)

Gando, A.; Gando, Y.; Hachiya, Takahiko; Hayashi, Akio; Hayashida, S.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Karino, Yoshiji; Koga, M.; Matsuda, Sumio; Mitsui, Tadao; Nakamura, Ko; Obara, Shigeru; Oura, Toshiaki; Ozaki, H.; Shimizu, I.; Shirahata, Y.; Shirai, J.; Suzuki, A.; Takai, Toshiaki; Tamae, K.; Teraoka, Y.; Ueshima, K.; Watanabe, H.; Kozlov, A.; Takemoto, Y.; Yoshida, S.; Fushimi, K.; Piepke, A.; Banks, Thomas; Berger, B. E.; Fujikawa, B. K.; O’Donnell, T.; Learned, J. G.; Maricic, J.; Sakai, M.; Winslow, L. A.; Krupczak, Emmett; Ouellet, J. L.; Efremenko, Yu.; Karwowski, H. J.; Markoff, D. M.; Tornow, W.; Detwiler, J. A.; Enomoto, S.; Decowski, M. P.

doi:10.3847/2041-8213/aa9a32

Cited by 3 publications

(3 citation statements)

References 19 publications

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“…The KamLAND experiment (Gando et al 2016 were found for each GW event, however these signals do not satisfy the spatial and temporal requirements.…”

Section: Experimental Searchesmentioning

confidence: 93%

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A global analysis searching for neutrinos associated with black hole merger gravitational wave events

Yang¹,

Ling²,

Wang³

et al. 2018

Res. Astron. Astrophys.

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Several neutrino observatories have searched for coincident neutrino signals associated with gravitational waves induced by the merging of two black holes. No statistically significant neutrino signal in excess of background level was observed. These experiments use different neutrino detection technologies and are sensitive to various neutrino types. A combined analysis was performed on the KamLAND, Super-Kamiokande and Borexino experimental data with a frequentist statistical approach to achieve a global picture of the associated neutrino fluence. Both monochromatic and Fermi-Dirac neutrino spectra were assumed in the calculation. The final results are consistent with null neutrino signals associated with a binary of black holes merging process. The derived 90% confidence level upper limits on the fluence and luminosity of various neutrino types are presented for neutrino energy less than 110 MeV.

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“…The KamLAND experiment (Gando et al 2016 were found for each GW event, however these signals do not satisfy the spatial and temporal requirements.…”

Section: Experimental Searchesmentioning

confidence: 93%

“…Two observed GW events in 2015 were both generated by the coalescence of binary BHs into a single BH. The first event, GW150914 (Abbott et al 2016c) The KamLAND experiment (Gando et al 2016) is located under 2700 meter water equivalent (m.w.e.) of vertical rock, below Mt.…”

Section: Introductionmentioning

confidence: 99%

A global analysis searching for neutrinos associated with black hole merger gravitational wave events

Yang¹,

Ling²,

Wang³

et al. 2018

Res. Astron. Astrophys.

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“…All follow up observations were negative, with the exception of [89], that suggested the possible presence of a weak transient above 50 keV, 0.4 s after the merger (see also [131], [90]). The neutrino searches with AUGER [1], ANTARES and IceCube [47], KamLAND [120], Super-Kamiokande [42] were also negative. The follow up of GW151226 included the optical observations by Pan-STARRS1…”

Section: Binary Black Hole Mergers In O1 O2mentioning

confidence: 99%

Gravitational wave astronomy with compact binary mergers

Poggiani¹

2021

Proceedings of the Golden Age of Cataclysmic Variables and Related Objects v — PoS(GOLDEN2019)

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Event m 1 (M) m 2 (M) M c (M) χ e f f M f (M) a f E r (M c 2) l peak (erg s −1) d L (Mpc) z ∆Ω(deg 2) GW150914 35.6 +4.7 −3.1 30.6 +3.0 −4.4 28.6 +1.7 −1.5-0.01 +0.12 −0.13 63.1 +3.4 −3.0 0.69 +0.05 −0.04 3.1 +0.4 −0.4 3.6 +0.4 −0.4 × 10 56 440 +150 −170 0.09 +0.03 −0.03 182 GW151012 23.2 +14.9 −5.5 13.6 +4.1 −4.8 15.2 +2.1 −1.2 0.05 +0.31 −0.20 35.6 +10.8 −3.8 0.67 +0.13 −0.11 1.6 +0.6 −0.5 3.2 +0.8 −1.7 × 10 56 1080 +550 −490 0.21 +0.09 −0.09 1523 GW151226 13.7 +8.8 −3.2 7.7 +2.2 −2.5 8.9 +0.3 −0.3 0.18 +0.20 −0.12 20.5 +6.4 −1.5 0.74 +0.07 −0.05 1.0 +0.1 −0.2 3.4 +0.7 −1.7 × 10 56 450 +180 −190 0.09 +0.04 −0.04 1033 GW170104 30.8 +7.3 −5.6 20.0 +4.9 −4.6 21.4 +2.2 −1.8-0.04 +0.17 −0.21 48.9 +5.1 −4.0 0.66 +0.08 −0.11 2.2 +0.5 −0.5 3.3 +0.6 −1.0 × 10 56 990 +440 −430 0.20 +0.08 −0.08 921 GW170608 11.0 +5.5 −1.7 7.6 +1.4 −2.2 7.9 +0.2 −0.2 0.03 +0.19 −0.07 17.8 +3.4 −0.7 0.69 +0.04 −0.04 0.9 +0.0 −0.1 3.5 +0.4 −1.3 × 10 56 320 +120 −110 0.07 +0.02 −0.02 392 GW170729 50.2 +16.2 −10.2 34.0 +9.1 −10.1 35.4 +6.5 −4.8 0.37 +0.21 −0.25 79.5 +14.7 −10.2 0.81 +0.07 −0.13 4.8 +1.7 −1.7 4.2 +0.9 −1.5 × 10 56 2840 +1400 −1360 0.49 +0.19 −0.21 1041 GW170809 35.0 +8.3 −5.9 23.8 +5.1 −5.2 24.9 +2.1 −1.7 0.08 +0.17 −0.17 56.3 +5.2 −3.8 0.70 +0.08 −0.09 2.7 +0.6 −0.6 3.5 +0.6 −0.9 × 10 56 1030 +320 −390 0.20 +0.05 −0.07 308 GW170814 30.6 +5.6 −3.0 25.2 +2.8 −4.0 24.1 +1.4 −1.1 0.07 +0.12 −0.12 53.2 +3.2 −2.4 0.72 +0.07 −0.05 2.7 +0.4 −0.3 3.7 +0.4 −0.5 × 10 56 600 +150 −220 0.12 +0.03 −0.04 87 GW170817 1.46 +0.12 −0.10 1.27 +0.09 −0.09 1.186 +0.001 −0.001 0.00 +0.02 −0.01 ≤ 2.8 ≤ 0.89 ≥ 0.04 ≥ 0.1 × 10 56 40 +7 −15 0.01 +0.00 −0.00 16 GW170818 35.4 +7.5 −4.7 26.7 +4.3 −5.2 26.5 +2.1 −1.7-0.09 +0.18 −0.21 59.4 +4.9 −3.8 0.67 +0.07 −0.08 2.7 +0.5 −0.5 3.4 +0.5 −0.7 × 10 56 1060 +420 −380 0.21 +0.07 −0.07 39 GW170823 39.5 +11.2 −6.7 29.0 +6.7 −7.8 29.2 +4.6 −3.6 0.09 +0.22 −0.26 65.4 +10.1 −7.4 0.72 +0.09 −0.12 3.3 +1.0 −0.9 3.6 +0.7 −1.1 × 10 56 1940 +970 −900 0.35 +0.

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Borexino’s search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database

Collaboration¹,

Bellini²,

Benziger³

et al. 2023

Eur. Phys. J. C

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The search for neutrino events in correlation with gravitational wave (GW) events for three observing runs (O1, O2 and O3) from 09/2015 to 03/2020 has been performed using the Borexino data-set of the same period. We have searched for signals of neutrino-electron scattering and inverse beta-decay (IBD) within a time window of $$\pm \, 1000$$ ± 1000 s centered at the detection moment of a particular GW event. The search was done with three visible energy thresholds of 0.25, 0.8 and 3.0 MeV. Two types of incoming neutrino spectra were considered: the mono-energetic line and the supernova-like spectrum. GW candidates originated by merging binaries of black holes (BHBH), neutron stars (NSNS) and neutron star and black hole (NSBH) were analyzed separately. Additionally, the subset of most intensive BHBH mergers at closer distances and with larger radiative mass than the rest was considered. In total, follow-ups of 74 out of 93 gravitational waves reported in the GWTC-3 catalog were analyzed and no statistically significant excess over the background was observed. As a result, the strongest upper limits on GW-associated neutrino and antineutrino fluences for all flavors ($$\nu _e, \nu _\mu , \nu _\tau $$ ν e , ν μ , ν τ ) at the level $$10^9{-}10^{15}~\textrm{cm}^{-2}\,\textrm{GW}^{-1}$$ 10 9 - 10 15 cm - 2 GW - 1 have been obtained in the 0.5–5 MeV neutrino energy range.

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Erratum: “A Search for Electron Antineutrinos Associated with Gravitational-wave Events GW150914 and GW151226 Using KamLAND” (2016, ApJL, 829, L34)

Cited by 3 publications

References 19 publications

A global analysis searching for neutrinos associated with black hole merger gravitational wave events

A global analysis searching for neutrinos associated with black hole merger gravitational wave events

Gravitational wave astronomy with compact binary mergers

Borexino’s search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database

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