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Article: Search for electron-antineutrinos associated with gravitational-wave events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay

TitleSearch for electron-antineutrinos associated with gravitational-wave events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay
Authors
Issue Date2021
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at https://iopscience.iop.org/journal/1674-1137
Citation
Chinese Physics C, High Energy Physics and Nuclear Physics, 2021, v. 45 n. 5, p. article no. 055001 How to Cite?
AbstractThe establishment of a possible connection between neutrino emission and gravitational-wave (GW) bursts is important to our understanding of the physical processes that occur when black holes or neutron stars merge. In the Daya Bay experiment, using the data collected from December 2011 to August 2017, a search was performed for electron-antineutrino signals that coincided with detected GW events, including GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817. We used three time windows of ±10, ±500, and ±1000 s relative to the occurrence of the GW events and a neutrino energy range of 1.8 to 100 MeV to search for correlated neutrino candidates. The detected electron-antineutrino candidates were consistent with the expected background rates for all the three time windows. Assuming monochromatic spectra, we found upper limits (90% confidence level) of the electron-antineutrino fluence of (1.13 − 2.44)×1011 cm−2 at 5 MeV to 8.0×107 cm−2 at 100 MeV for the three time windows. Under the assumption of a Fermi-Dirac spectrum, the upper limits were found to be (5.4 − 7.0)×109 cm−2 for the three time windows.
Persistent Identifierhttp://hdl.handle.net/10722/299740
ISSN
2023 Impact Factor: 3.6
2023 SCImago Journal Rankings: 1.184
ISI Accession Number ID

 

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dc.contributor.authorAn, FP-
dc.contributor.authorBalantekin, AB-
dc.contributor.authorBand, HR-
dc.contributor.authorBishai, M-
dc.contributor.authorBlyth, S-
dc.contributor.authorCao, GF-
dc.contributor.authorCao, J-
dc.contributor.authorChang, JF-
dc.contributor.authorChang, Y-
dc.contributor.authorChen, HS-
dc.contributor.authorChen, SM-
dc.contributor.authorZhang, ZY-
dc.contributor.authorZhao, J-
dc.contributor.authorZhou, L-
dc.contributor.authorZhuang, HL-
dc.contributor.authorZou, JH-
dc.contributor.authorDeng, FS-
dc.contributor.authorDing, YY-
dc.contributor.authorDiwan, MV-
dc.contributor.authorDohnal, T-
dc.contributor.authorDove, J-
dc.contributor.authorNapolitano, J-
dc.contributor.authorDvořák, M-
dc.contributor.authorDwyer, DA-
dc.contributor.authorGallo, JP-
dc.contributor.authorGonchar, M-
dc.contributor.authorGong, GH-
dc.contributor.authorGong, H-
dc.contributor.authorGu, WQ-
dc.contributor.authorGuo, JY-
dc.contributor.authorGuo, L-
dc.contributor.authorGuo, XH-
dc.contributor.authorNaumov, D-
dc.contributor.authorGuo, YH-
dc.contributor.authorGuo, Z-
dc.contributor.authorHackenburg, RW-
dc.contributor.authorHans, S-
dc.contributor.authorHe, M-
dc.contributor.authorHeeger, KM-
dc.contributor.authorHeng, YK-
dc.contributor.authorHiguera, A-
dc.contributor.authorHor, YK-
dc.contributor.authorHsiung, YB-
dc.contributor.authorNaumova, E-
dc.contributor.authorHu, BZ-
dc.contributor.authorHu, JR-
dc.contributor.authorHu, T-
dc.contributor.authorHu, ZJ-
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dc.contributor.authorHuang, XT-
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dc.contributor.authorHuber, P-
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dc.contributor.authorJones, D-
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dc.contributor.authorKettell, SH-
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dc.contributor.authorLangford, TJ-
dc.contributor.authorLee, J-
dc.contributor.authorOlshevskiy, A-
dc.contributor.authorLee, HCJ-
dc.contributor.authorLei, RT-
dc.contributor.authorLeitner, R-
dc.contributor.authorLeung, JKC-
dc.contributor.authorLi, F-
dc.contributor.authorLi, JJ-
dc.contributor.authorLi, QJ-
dc.contributor.authorLi, S-
dc.contributor.authorLi, SC-
dc.contributor.authorLi, WD-
dc.contributor.authorPan, HR-
dc.contributor.authorLi, XN-
dc.contributor.authorLi, XQ-
dc.contributor.authorLi, YF-
dc.contributor.authorLi, ZB-
dc.contributor.authorLiang, H-
dc.contributor.authorLin, CJ-
dc.contributor.authorLin, GL-
dc.contributor.authorLin, S-
dc.contributor.authorLing, JJ-
dc.contributor.authorLink, JM-
dc.contributor.authorPark, J-
dc.contributor.authorLittenberg, L-
dc.contributor.authorLittlejohn, BR-
dc.contributor.authorLiu, JC-
dc.contributor.authorLiu, JL-
dc.contributor.authorLu, C-
dc.contributor.authorLu, HQ-
dc.contributor.authorLu, JS-
dc.contributor.authorLuk, KB-
dc.contributor.authorMa, XB-
dc.contributor.authorMa, XY-
dc.contributor.authorPatton, S-
dc.contributor.authorMa, YQ-
dc.contributor.authorMarshall, C-
dc.contributor.authorMartinez Caicedo, DA-
dc.contributor.authorMcDonald, KT-
dc.contributor.authorMcKeown, RD-
dc.contributor.authorMeng, Y-
dc.contributor.authorPeng, JC-
dc.contributor.authorPun, JCS-
dc.contributor.authorChen, Y-
dc.contributor.authorQi, FZ-
dc.contributor.authorQi, M-
dc.contributor.authorQian, X-
dc.contributor.authorRaper, N-
dc.contributor.authorRen, J-
dc.contributor.authorMorales Reveco, C-
dc.contributor.authorRosero, R-
dc.contributor.authorRoskovec, B-
dc.contributor.authorRuan, XC-
dc.contributor.authorSteiner, H-
dc.contributor.authorChen, YX-
dc.contributor.authorSun, JL-
dc.contributor.authorTmej, T-
dc.contributor.authorTreskov, K-
dc.contributor.authorTse, WH-
dc.contributor.authorTull, CE-
dc.contributor.authorViren, B-
dc.contributor.authorVorobel, V-
dc.contributor.authorWang, CH-
dc.contributor.authorWang, J-
dc.contributor.authorWang, M-
dc.contributor.authorCheng, J-
dc.contributor.authorWang, NY-
dc.contributor.authorWang, RG-
dc.contributor.authorWang, W-
dc.contributor.authorWang, W-
dc.contributor.authorWang, X-
dc.contributor.authorWang, Y-
dc.contributor.authorWang, YF-
dc.contributor.authorWang, Z-
dc.contributor.authorWang, Z-
dc.contributor.authorWang, ZM-
dc.contributor.authorCheng, ZK-
dc.contributor.authorWei, HY-
dc.contributor.authorWei, LH-
dc.contributor.authorWen, LJ-
dc.contributor.authorWhisnant, K-
dc.contributor.authorWhite, CG-
dc.contributor.authorWong, HLH-
dc.contributor.authorWorcester, E-
dc.contributor.authorWu, DR-
dc.contributor.authorWu, FL-
dc.contributor.authorWu, Q-
dc.contributor.authorCherwinka, JJ-
dc.contributor.authorWu, WJ-
dc.contributor.authorXia, DM-
dc.contributor.authorXie, ZQ-
dc.contributor.authorXing, ZZ-
dc.contributor.authorXu, JL-
dc.contributor.authorXu, T-
dc.contributor.authorXue, T-
dc.contributor.authorYang, CG-
dc.contributor.authorYang, L-
dc.contributor.authorYang, YZ-
dc.contributor.authorChu, MC-
dc.contributor.authorYao, HF-
dc.contributor.authorYe, M-
dc.contributor.authorYeh, M-
dc.contributor.authorYoung, BL-
dc.contributor.authorYu, HZ-
dc.contributor.authorYu, ZY-
dc.contributor.authorYue, BB-
dc.contributor.authorZeng, S-
dc.contributor.authorZeng, Y-
dc.contributor.authorZhan, L-
dc.contributor.authorCummings, JP-
dc.contributor.authorZhang, C-
dc.contributor.authorZhang, FY-
dc.contributor.authorZhang, HH-
dc.contributor.authorZhang, JW-
dc.contributor.authorZhang, QM-
dc.contributor.authorZhang, XT-
dc.contributor.authorZhang, YM-
dc.contributor.authorZhang, YX-
dc.contributor.authorZhang, YY-
dc.contributor.authorZhang, ZJ-
dc.contributor.authorDalager, O-
dc.contributor.authorZhang, ZP-
dc.date.accessioned2021-05-26T03:28:24Z-
dc.date.available2021-05-26T03:28:24Z-
dc.date.issued2021-
dc.identifier.citationChinese Physics C, High Energy Physics and Nuclear Physics, 2021, v. 45 n. 5, p. article no. 055001-
dc.identifier.issn1674-1137-
dc.identifier.urihttp://hdl.handle.net/10722/299740-
dc.description.abstractThe establishment of a possible connection between neutrino emission and gravitational-wave (GW) bursts is important to our understanding of the physical processes that occur when black holes or neutron stars merge. In the Daya Bay experiment, using the data collected from December 2011 to August 2017, a search was performed for electron-antineutrino signals that coincided with detected GW events, including GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817. We used three time windows of ±10, ±500, and ±1000 s relative to the occurrence of the GW events and a neutrino energy range of 1.8 to 100 MeV to search for correlated neutrino candidates. The detected electron-antineutrino candidates were consistent with the expected background rates for all the three time windows. Assuming monochromatic spectra, we found upper limits (90% confidence level) of the electron-antineutrino fluence of (1.13 − 2.44)×1011 cm−2 at 5 MeV to 8.0×107 cm−2 at 100 MeV for the three time windows. Under the assumption of a Fermi-Dirac spectrum, the upper limits were found to be (5.4 − 7.0)×109 cm−2 for the three time windows.-
dc.languageeng-
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at https://iopscience.iop.org/journal/1674-1137-
dc.relation.ispartofChinese Physics C, High Energy Physics and Nuclear Physics-
dc.rightsChinese Physics C, High Energy Physics and Nuclear Physics. Copyright © Institute of Physics Publishing Ltd.-
dc.rightsThis is an author-created, un-copyedited version of an article published in [insert name of journal]. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://dx.doi.org/[insert DOI].-
dc.titleSearch for electron-antineutrinos associated with gravitational-wave events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay-
dc.typeArticle-
dc.identifier.emailLee, HCJ: jleehc@hku.hk-
dc.identifier.emailPun, JCS: jcspun@hku.hk-
dc.identifier.authorityLee, HCJ=rp01902-
dc.identifier.authorityLeung, JKC=rp00732-
dc.identifier.authorityPun, JCS=rp00772-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1088/1674-1137/abe84b-
dc.identifier.scopuseid_2-s2.0-85105855523-
dc.identifier.hkuros322551-
dc.identifier.volume45-
dc.identifier.issue5-
dc.identifier.spagearticle no. 055001-
dc.identifier.epagearticle no. 055001-
dc.identifier.isiWOS:000646857800001-
dc.publisher.placeUnited Kingdom-

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