Search for multimessenger signals in NOvA coincident with LIGO/Virgo detections

Acero, M. A.; Adamson, P.; Aliaga, L.; Alion, T.; Allakhverdian, V.; Анфимов, Н.; Antoshkin, A.; Asquith, L.; Aurisano, A.; Back, A.; Backhouse, C.; Baird, M.; Balashov, N.; Baldi, Pierre; Bambah, Bindu A.; Bashar, S.; Bays, K.; Bending, S.; Bernstein, R. H.; Bhatnagar, V.; Bhuyan, B.; Bian, J. M.; Blair, J. T.; Booth, Alexander; Bour, P.; Bromberg, C.; Buchanan, N. J.; Butkevich, A.; Calvez, S.; Carroll, Timothy J.; Catano-Mur, E.; Childress, S.; Choudhary, B. C.; Coan, T. E.; Colo, M.; Corwin, L. A.; Cremonesi, L.; Davies, G. S.; Derwent, P. F.; Dharmapalan, R.; Ding, P. F.; Djurcic, Z.; Doyle, D.; Dukes, E. C.; Duyang, H.; Edayath, S.; Ehrlich, R.; Feldman, G. J.; Filip, P.; Flanagan, W.; Frank, M. J.; Gallagher, H.; Gandrajula, Reddy Pratap; Gao, Feng; Germani, S.; Giri, A.; Gomes, R. A.; Goodman, M. C.; Grichine, V.; Groh, M.; Guo, B.; Habig, A.; Hakl, F.; Hartnell, J.; Hatcher, R.; Heller, K.; Hewes, J.; Himmel, A.; Holin, A.; Hylen, J.; Jediny, F.; Johnson, C. A.; Judah, M.; Kakorin, I.; Kalra, D.; Kaplan, Daniel M.; Keloth, R.; Klimov, O.; Koerner, L. W.; Kolupaeva, L.; Kotelnikov, S.K.; Kullenberg, Ch.; Kumar, Arun; Kuruppu, C.; Kus, V.; Lackey, T.; Lang, K.; Li, L.; Lin, S.; Lokajíček, M.; Luchuk, S.; Magill, S.; Mann, W. A.; Маршак, М. Л.; Martinez-Casales, M.; Matveev, V.; Mayes, B.; Méndez, D. P.; Messier, M. D.; Meyer, H.; Miao, T.; Miller, William H.; Mishra, S. R.; Mislivec, A.; Mohanta, Rukmani; Moren, A.; Mualem, L.; Muether, M.; Mufson, S.; Mulder, K.; Murphy, Robert; Musser, J.; Naples, D.; Nayak, N.; Nelson, J. K.; Nichol, R. J.; Niner, E.; Norman, A.; Norrick, A.; Nosek, T.; Olshevskiy, A.; Olson, Timothy S.; Paley, J.; Patterson, R. B.; Pawloski, G.; Petrova, O.; Petti, R.; Plunkett, R.; Rafique, A.; Psihas, F.; Raj, V.; Rebel, B.; Rojas, Pablo Fierro; Ryabov, V. A.; Samoylov, O.; Sanchez, M. C.; Falero, S. Sánchez; Shanahan, P.; Sheshukov, A.; Singh, Prabhjot; Singh, V.; Smith, E.; Smolík, J.; Snopok, P.; Solomey, N.; Sousa, A.; Soustružnı́k, K.; Strait, M.; Suter, L.; Sutton, Andrew D.; Talaga, R. L.; Oregui, B. Tapia; Tas, P.; Thayyullathil, Ramesh Babu; Thomas, J.; Tiras, E.; Torbunov, D.; Tripathi, J.; Torun, Y.; Urheim, J.; Vahle, P.; Vasel, J.; Vokáč, P.; Vrba, T.; Wallbank, M.; Warburton, Thomas; Wetstein, M.; Whittington, D.; Wojcicki, S. G.; Wolcott, J.; Dombara, A. Yallappa; Yonehara, K.; Yu, Shiqi; Yu, Y.; Zadorozhnyy, S.; Zálešâk, J.; Zhang, Y.; Zwaska, R.

doi:10.1103/physrevd.101.112006

Cited by 8 publications

(3 citation statements)

References 30 publications

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“…During the third observing run, LIGO-O3, the LIGO/Virgo collaboration initiated the online GW candidate event database (GraceDB) (LIGO Scientific Collaboration 2020), providing public alerts and a centralized location for aggregating and retrieving event information. For such transient GW events, various neutrino detectors reported correlation searches: Super-Kamiokande (Abe et al 2016(Abe et al , 2018, Borexino (Agostini et al 2017), NOvA (Acero et al 2020), Bikal-GVD Neutrino Telescope (Avrorin et al 2018), Daya Bay (An et al 2020), XMASS (Collaboration et al 2020), and IceCube/ANTARES (Adrián-Martínez et al 2016;Albert et al 2017b;Aartsen et al 2020). The Kamioka Liquid scintillator AntiNeutrino Detector (KamLAND) has also performed a search for electron antineutrinos coincident with gravitational waves GW150914 and GW151226, and then candidate event LVT151012 (Gando et al 2016a).…”

Section: Introductionmentioning

confidence: 99%

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

Abe¹,

Asami²,

Gando³

et al. 2021

ApJ

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We present the results of a search for MeV-scale electron antineutrino events in KamLAND coincident with the 60 gravitational wave events/candidates reported by the LIGO/Virgo collaboration during their second and third observing runs. We find no significant coincident signals within a ±500 s timing window from each gravitational wave and present 90% C.L. upper limits on the electron antineutrino fluence between 108 and 1013 cm−2 for neutrino energies in the energy range of 1.8–111 MeV.

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Section: Introductionmentioning

confidence: 99%

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

Abe¹,

Asami²,

Gando³

et al. 2021

ApJ

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show abstract

“…Relative to our previous report [7], the clustering algorithm for grouping hits into supernova neutrino event candidates has been greatly improved. Previously, a cluster was defined as a pair of hits with one hit in each view.…”

Section: Discussionmentioning

confidence: 99%

“…In a previous paper [7] we described a broad search * now at San José State University for signals, across the MeV to TeV range, associated with 26 gravitational wave events. We now focus on the possibility of detecting supernova-like neutrinos and present an improved search using the now-available larger catalog of gravitational wave events.…”

Section: Introductionmentioning

confidence: 99%

Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections

Acero,

Adamson,

Aliaga

et al. 2021

Preprint

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A search is performed for supernova-like neutrino interactions coincident with 76 gravitational wave events detected by the LIGO/Virgo Collaboration. For 40 of these events, full readout of the time around the gravitational wave is available from the NOvA Far Detector. For these events, we set limits on the fluence of the sum of all neutrino flavors of F < 7(4) × 10 10 cm −2 at 90% C.L. assuming energy and time distributions corresponding to the Garching supernova models with masses 9.6( 27) M . Under the hypothesis that any given gravitational wave event was caused by a supernova, this corresponds to a distance of r > 29(50) kpc at 90% C.L. Weaker limits are set for other gravitational wave events with partial Far Detector data and/or Near Detector data.

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The LIGO‐Virgo O3 Run and the Multi‐Messenger Investigations of Compact Binary Mergers

Poggiani

2023

Annalen der Physik

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The third observing run (O3) of Advanced LIGO and Advanced Virgo started in April 2019 and ended in March 2020 due to the pandemic. From the O3 run three catalogs of compact binary mergers, GWTC‐2, GWTC‐2.1, and GWTC‐3, that include also some exceptional events, are produced by the LIGO/Virgo Collaboration. The paper will review the science results about compact binary mergers during the O3 run and the follow‐up of gravitational wave candidate events involving the whole electromagnetic spectrum and neutrinos. No confirmed counterpart is found during the O3 run for any candidate. The impact of detected events on astrophysics and cosmology will also be discussed. The paper will also briefly summarize additional multi‐messenger investigations involving candidates not initially associated to gravitational events.

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Search for multimessenger signals in NOvA coincident with LIGO/Virgo detections

Cited by 8 publications

References 30 publications

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections

The LIGO‐Virgo O3 Run and the Multi‐Messenger Investigations of Compact Binary Mergers

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