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Sensitivity of the SHiP experiment to light dark matter

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dc.contributor.authorAhdida, C.
dc.contributor.authorAkmete, A.
dc.contributor.authorAlbanese, R.
dc.contributor.authorAlexandrov, A.
dc.contributor.authorAtkin, E.
dc.contributor.authorDmitrenko, V.
dc.contributor.authorEtenko, A.
dc.contributor.authorFilippov, K.
dc.contributor.authorGrachev, V.
dc.contributor.authorKudenko, Y.
dc.contributor.authorNovikov, A.
dc.contributor.authorPolukhina, N.
dc.contributor.authorSamsonov, V.
dc.contributor.authorShustov, A.
dc.contributor.authorSkorokhvatov, M.
dc.contributor.authorSmirnov, S.
dc.contributor.authorTeterin, P.
dc.contributor.authorUlin, S.
dc.contributor.authorUteshev, Z.
dc.contributor.authorVlasik, K.
dc.contributor.authorАткин, Эдуард Викторович
dc.contributor.authorДмитренко, Валерий Васильевич
dc.contributor.authorЭтенко, Александр Владимирович
dc.contributor.authorГрачев, Виктор Михайлович
dc.contributor.authorКуденко, Юрий Григорьевич
dc.contributor.authorПолухина, Наталья Геннадьевна
dc.contributor.authorШустов, Александр Евгеньевич
dc.contributor.authorСкорохватов, Михаил Дмитриевич
dc.contributor.authorСмирнов, Сергей Юрьевич
dc.contributor.authorТетерин, Пётр Евгеньевич
dc.contributor.authorУлин, Сергей Евгеньевич
dc.contributor.authorУтешев, Зияэтдин Мухамедович
dc.contributor.authorВласик, Константин Федорович
dc.date.accessioned2024-11-29T13:35:46Z
dc.date.available2024-11-29T13:35:46Z
dc.date.issued2021
dc.description.abstract© 2021, The Author(s).Dark matter is a well-established theoretical addition to the Standard Model supported by many observations in modern astrophysics and cosmology. In this context, the existence of weakly interacting massive particles represents an appealing solution to the observed thermal relic in the Universe. Indeed, a large experimental campaign is ongoing for the detection of such particles in the sub-GeV mass range. Adopting the benchmark scenario for light dark matter particles produced in the decay of a dark photon, with αD = 0.1 and mA′ = 3mχ, we study the potential of the SHiP experiment to detect such elusive particles through its Scattering and Neutrino detector (SND). In its 5-years run, corresponding to 2 · 1020 protons on target from the CERN SPS, we find that SHiP will improve the current limits in the mass range for the dark matter from about 1 MeV to 300 MeV. In particular, we show that SHiP will probe the thermal target for Majorana candidates in most of this mass window and even reach the Pseudo-Dirac thermal relic. [Figure not available: see fulltext.]
dc.identifier.citationSensitivity of the SHiP experiment to light dark matter / Ahdida, C. [et al.] // Journal of High Energy Physics. - 2021. - 2021. - № 4. - 10.1007/JHEP04(2021)199
dc.identifier.doi10.1007/JHEP04(2021)199
dc.identifier.urihttps://www.doi.org/10.1007/JHEP04(2021)199
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dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000644180900001
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/23945
dc.relation.ispartofJournal of High Energy Physics
dc.titleSensitivity of the SHiP experiment to light dark matter
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume2021
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