正在加载页面…
2020-01-20
Search for multi-messenger signals in NOvA coincident with LIGO/Virgo detections
NOvA CollaborationM. A. AceroP. AdamsonL. AliagaT. AlionV. AllakhverdianN. AnfimovA. AntoshkinL. AsquithA. AurisanoA. BackC. BackhouseM. BairdN. BalashovP. BaldiB. A. BambahS. BasharK. BaysS. BendingR. BernsteinV. BhatnagarB. BhuyanJ. BianJ. BlairA. C. BoothP. BourC. BrombergN. BuchananA. ButkevichS. CalvezT. J. CarrollE. Catano-MurS. ChildressB. C. ChoudharyT. E. CoanM. ColoL. CorwinL. CremonesiG. S. DaviesP. F. DerwentR. DharmapalanP. DingZ. DjurcicD. DoyleE. C. DukesH. DuyangS. EdayathR. EhrlichG. J. FeldmanP. FilipW. FlanaganM. J. FrankH. R. GallagherR. GandrajulaF. GaoS. GermaniA. GiriR. A. GomesM. C. GoodmanV. GrichineM. GrohR. GroupB. GuoA. HabigF. HaklJ. HartnellR. HatcherK. HellerV HewesA. HimmelA. HolinJ. HylenF. JedinyC. JohnsonM. JudahI. KakorinD. KalraD. M. KaplanR. KelothO. KlimovL. W. KoernerL. KolupaevaS. KotelnikovCh. KullenbergA. KumarC. D. KuruppuV. KusT. LackeyK. LangL. LiS. LinM. LokajicekS. LuchukS. MagillW. A. MannM. L. MarshakM. Martinez-CasalesV. MatveevB. MayesD. P. MéndezM. D. MessierH. MeyerT. MiaoW. H. MillerS. R. MishraA. MislivecR. MohantaA. MorenL. MualemM. MuetherS. MufsonK. MulderR. MurphyJ. MusserD. NaplesN. NayakJ. K. NelsonR. NicholE. NinerA. NormanA. NorrickT. NosekA. OlshevskiyT. OlsonJ. PaleyR. B. PattersonG. PawloskiO. PetrovaR. PettiR. K. PlunkettA. RafiqueF. PsihasV. RajB. RebelP. RojasV. RyabovO. SamoylovM. C. SanchezS. Sánchez FaleroP. ShanahanA. SheshukovP. SinghV. SinghE. SmithJ. SmolikP. SnopokN. SolomeyA. SousaK. SoustruznikM. StraitL. SuterA. SuttonR. L. TalagaB. Tapia OreguiP. TasR. B. ThayyullathilJ. ThomasE. TirasD. TorbunovJ. TripathiY. TorunJ. UrheimP. VahleJ. VaselP. VokacT. VrbaM. WallbankT. K. WarburtonM. WetsteinD. WhittingtonS. G. WojcickiJ. WolcottA. Yallappa DombaraK. YoneharaS. YuY. YuS. ZadorozhnyyJ. ZalesakY. ZhangR. Zwaska
文献摘要
Using the NOvA neutrino detectors, a broad search has been performed for any signal coincident with 28 gravitational wave events detected by the LIGO/Virgo Collaboration between September 2015 and July 2019. For all of these events, NOvA is sensitive to possible arrival of neutrinos and cosmic rays of GeV and higher energies. For five (seven) events in the NOvA Far (Near) Detector, timely public alerts from the LIGO/Virgo Collaboration allowed recording of MeV-scale events. No signal candidates were found.
讨论
0讲解博客
生成讲解博客的中文版本
AI智能校验
生成AI智能校验的中文版本