期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 6, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/1475-7516/2022/06/018
关键词
neutrino detectors; neutrino experiments; solar and atmospheric neutrinos; dark matter experiments
资金
- Centre National de la Recherche Scientifique (CNRS)
- Commissariat a l'energie atomique et aux energies alternatives (CEA)
- Commission Europeenne
- Institut Universitaire de France (IUF)
- LabEx UnivEarthS [ANR-10-LABX-0023, ANR18-IDEX-0001]
- Region Ile-de-France (DIM-ACAV)
- Region Alsace (contrat CPER)
- Region Provence-Alpes-Cote d'Azur
- Departement du Var and Ville de La Seyne-sur-Mer, France
- Wetenschappelijk Onderzoek (NWO), the Netherlands
- Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania
- Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento(MCIU/FEDER) [PGC2018096663-B-C41, PGC2018096663-A-C42, PGC2018096663-B-C43, PGC2018096663-B-C44]
- Generalitat Valenciana [PROMETEO/2020/019, GRISOLIA/2018/119, GRISOLIA/2021/192, CIDEGENT/2018/034, CIDEGENT/2019/043, CIDEGENT/2020/049, CIDEGENT/2021/023]
- Programa Operativo FEDER 2014-2020/Junta de Andalucia-Consejeria de Economia y Conocimiento/Proyecto [A-FQM-053-UGR18]
- La Caixa Foundation [LCF/BQ/IN17/11620019]
- EU: MSC program, Spain [101025085]
- Ministry of Higher Education, Scientific Research and Innovation, Morocco
- Arab Fund for Economic and Social Development, Kuwait
Solar atmospheric neutrinos are produced by the interaction of cosmic rays with the solar medium. Detecting these neutrinos can provide information about the composition of cosmic rays and the density of the Sun, and play a significant role in indirect searches for dark matter and assessing uncertainties.
Solar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar medium. The detection of SA nu s would provide useful information on the composition of primary cosmic rays as well as the solar density. These neutrinos represent an irreducible source of background for indirect searches for dark matter towards the Sun and the measurement of their flux would allow for a better assessment of the uncertainties related to these searches. In this paper we report on the analysis performed, based on an unbinned likelihood maximisation, to search for SA nu s with the ANTARES neutrino telescope. After analysing the data collected over 11 years, no evidence for a solar atmospheric neutrino signal has been found. An upper limit at 90% confidence level on the flux of solar atmospheric neutrinos has been obtained, equal to 7x10(-11) [TeV-1 cm(-2) s(-1)] b at E-nu = 1 TeV for the reference cosmic ray model assumed.
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