Title
Extended search for supernovalike neutrinos in NOvA coincident with LIGO/Virgo detections
Date Issued
15 September 2021
Access level
open access
Resource Type
journal article
Author(s)
Acero M.A.
Adamson P.
Anfimov N.
Antoshkin A.
Arrieta-Diaz E.
Asquith L.
Aurisano A.
Back A.
Backhouse C.
Baird M.
Balashov N.
Baldi P.
Bambah B.A.
Bashar S.
Bays K.
Bernstein R.
Bhatnagar V.
Bhuyan B.
Bian J.
Blair J.
Booth A.C.
Bowles R.
Bromberg C.
Buchanan N.
Butkevich A.
Calvez S.
Carroll T.J.
Catano-Mur E.
Choudhary B.C.
Christensen A.
Coan T.E.
Colo M.
Corwin L.
Cremonesi L.
Davies G.S.
Derwent P.F.
Ding P.
Djurcic Z.
Dolce M.
Doyle D.
Dueñas Tonguino D.
Dukes E.C.
Duyang H.
Edayath S.
Ehrlich R.
Elkins M.
Ewart E.
Feldman G.J.
Filip P.
Franc J.
Frank M.J.
Gallagher H.R.
Gandrajula R.
Gao F.
Giri A.
Gomes R.A.
Goodman M.C.
Grichine V.
Groh M.
Group R.
Guo B.
Habig A.
Hakl F.
Hall A.
Hartnell J.
Hatcher R.
Hatzikoutelis A.
Hausner H.
Heller K.
Hewes J.
Himmel A.
Holin A.
Huang J.
Jargowsky B.
Jarosz J.
Jediny F.
Johnson C.
Judah M.
Kakorin I.
Kalra D.
Kaplan D.M.
Kalitkina A.
Keloth R.
Klimov O.
Koerner L.W.
Kolupaeva L.
Kotelnikov S.
Kralik R.
Kullenberg C.
Kubu M.
Kumar A.
Kuruppu C.D.
Kus V.
Lackey T.
Lang K.
Lasorak P.
Lesmeister J.
Lin S.
Lister A.
Fermi National Accelerator Laboratory
Publisher(s)
American Physical Society
Abstract
A search is performed for supernovalike 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)×1010 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.
Volume
104
Issue
6
Number
063024
Language
English
OCDE Knowledge area
Astronomía
Física de partículas, Campos de la Física
Scopus EID
2-s2.0-85115418297
Source
Physical Review D
ISSN of the container
24700010
Sponsor(s)
This document was prepared by the NOvA Collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by the U.S. Department of Energy; the U.S. National Science Foundation; the Department of Science and Technology, India; the European Research Council; the MSMT CR, GA UK, Czech Republic; the RAS, RFBR, the Ministry of Education and Science of the Russian Federation (RMES), RSF, and BASIS Foundation, Russia; CNPq and FAPEG, Brazil; STFC, UKRI, and the Royal Society, United Kingdom; and the State and University of Minnesota. We are grateful for the contributions of the staffs of the University of Minnesota at the Ash River Laboratory and of Fermilab.
Russell Sage Foundation RSF
Rochester Academy of Science RAS
UK Research and Innovation UKRI
Science and Technology Facilities Council STFC
Department of Science and Technology, Ministry of Science and Technology, India डीएसटी
Ministerstvo Školství, Mládeže a Tělovýchovy MŠMT
Russian Foundation for Basic Research РФФИ
Conselho Nacional de Desenvolvimento Científico e Tecnológico CNPq
Fundação de Amparo à Pesquisa do Estado de Goiás FAPEG
Sources of information:
Directorio de Producción Científica
Scopus