Remarks on bosonic super-WIMP search experiments
DC Field | Value | Language |
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dc.contributor.author | Young Ju Ko | - |
dc.contributor.author | Park, HyangKyu | - |
dc.date.accessioned | 2021-12-16T04:50:01Z | - |
dc.date.available | 2021-12-16T04:50:01Z | - |
dc.date.created | 2021-12-15 | - |
dc.date.issued | 2021-10-26 | - |
dc.identifier.issn | 2470-0010 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/10861 | - |
dc.description.abstract | © 2021 authors.Bosonic super-weakly interacting massive particles (WIMPs), including pseudoscalar and vector particles, are dark-matter candidates. To date, many underground experiments searches for super-WIMPs have been performed in the mass range of a few keV/c2 to 1 MeV/c2. All these searches utilize the absorption process of a super-WIMP by a target atom in the detector, which is similar to the photoelectric effect. We consider another process - namely, a Compton-like process. As an example, we compare the cross section of a germanium atom for the absorption process with that of a Compton-like process. Our findings indicate that the cross section for the Compton-like process becomes dominant relative to that for the absorption process for mass above approximately 150 keV/c2 for both pseudoscalar and vector super-WIMPs. In particular, the cross section for the Compton-like process for a vector super-WIMP becomes increasingly greater than that for the absorption process by 1 to 2 orders of magnitude in the 400 keV/c2 to 1 MeV/c2 mass range, respectively. By including the Compton-like process, which has not been used in any other super-WIMP search experiments, the experimental upper limits can be improved. | - |
dc.language | 영어 | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.title | Remarks on bosonic super-WIMP search experiments | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000712088400005 | - |
dc.identifier.scopusid | 2-s2.0-85119410033 | - |
dc.identifier.rimsid | 76829 | - |
dc.contributor.affiliatedAuthor | Young Ju Ko | - |
dc.identifier.doi | 10.1103/PhysRevD.104.083030 | - |
dc.identifier.bibliographicCitation | Physical Review d, v.104, no.8 | - |
dc.relation.isPartOf | Physical Review d | - |
dc.citation.title | Physical Review d | - |
dc.citation.volume | 104 | - |
dc.citation.number | 8 | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | N | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalResearchArea | Physics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Physics, Particles & Fields | - |
dc.subject.keywordPlus | DARK-MATTER | - |
dc.subject.keywordPlus | STERILE NEUTRINOS | - |
dc.subject.keywordPlus | PARTICLE PHYSICS | - |
dc.subject.keywordPlus | CANDIDATES | - |