JUNO探測器對來自太陽暗質湮滅所產生之MeV微中子流之靈敏度

Full metadata record

DC Field	Value	Language
dc.contributor.author	馬如亞	zh_TW
dc.contributor.author	林貴林	zh_TW
dc.contributor.author	Mariia Redchuk	en_US
dc.contributor.author	Lin, Guey-Lin	en_US
dc.date.accessioned	2018-01-24T07:37:06Z	-
dc.date.available	2018-01-24T07:37:06Z	-
dc.date.issued	2016	en_US
dc.identifier.uri	http://etd.lib.nctu.edu.tw/cdrfb3/record/nctu/#GT070352702	en_US
dc.identifier.uri	http://hdl.handle.net/11536/138965	-
dc.description.abstract	We study the MeV neutrino flux resulting from dark matter annihilation into light quarks \chi\chi -> q \bar q in the Sun where q = u, d and s. Such neutrinos are produced from the decays of stopped pi and K mesons. We show that the signal neutrino flux is able to overcome the huge atmospheric background due to the large multiplicity of aforementioned pi and K mesons. We discuss the feasibility of detecting such neutrinos by JUNO detector and the resulting constraints on dark matter interaction cross-sections.	zh_TW
dc.description.abstract	We study the MeV neutrino flux resulting from dark matter annihilation into light quarks \chi\chi -> q \bar q in the Sun where q = u, d and s. Such neutrinos are produced from the decays of stopped pi and K mesons. We show that the signal neutrino flux is able to overcome the huge atmospheric background due to the large multiplicity of aforementioned pi and K mesons. We discuss the feasibility of detecting such neutrinos by JUNO detector and the resulting constraints on dark matter interaction cross-sections.	en_US
dc.language.iso	en_US	en_US
dc.subject	JUNO探測器	zh_TW
dc.subject	暗物質	zh_TW
dc.subject	微中子	zh_TW
dc.subject	JUNO detector	en_US
dc.subject	dark matter	en_US
dc.subject	neutrino	en_US
dc.title	JUNO探測器對來自太陽暗質湮滅所產生之MeV微中子流之靈敏度	zh_TW
dc.title	Sensitivity of the JUNO Detector to MeV Neutrino Flux Arising from Dark Matter Annihilation in the Sun	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
Appears in Collections:	Thesis