Mimar Sinan Güzel Sanatlar Üniversitesi Açık Bilim, Sanat Arşivi

Açık Bilim, Sanat Arşivi, Mimar Sinan Güzel Sanatlar Üniversitesi tarafından doğrudan ve dolaylı olarak yayınlanan; kitap, makale, tez, bildiri, rapor gibi tüm akademik kaynakları uluslararası standartlarda dijital ortamda depolar, Üniversitenin akademik performansını izlemeye aracılık eder, kaynakları uzun süreli saklar ve yayınların etkisini artırmak için telif haklarına uygun olarak Açık Erişime sunar.

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Solution to Big-Bang nucleosynthesis in hybrid axion dark matter model

dc.contributor.authorKusakabe, Motohiko
dc.contributor.authorBalantekin, A. B.
dc.contributor.authorKajino, Toshitaka
dc.contributor.authorPehlivan, Y.
dc.date.accessioned2025-01-09T20:14:36Z
dc.date.available2025-01-09T20:14:36Z
dc.date.issued2013
dc.identifier.issn0370-2693
dc.identifier.issn1873-2445
dc.identifier.urihttps://doi.org/10.1016/j.physletb.2012.11.007
dc.identifier.urihttps://hdl.handle.net/20.500.14124/9161
dc.description.abstractFollowing a recent suggestion of axion cooling of photons between the nucleosynthesis and recombination epochs in the Early Universe, we investigate a hybrid model with both axions and relic supersymmetric particles. In this model we demonstrate that the Li-7 abundance can be consistent with observations without destroying the important concordance of deuterium abundance. (c) 2012 Elsevier B.V. All rights reserved.en_US
dc.description.sponsorshipJSPS [200244035, 21.6817]; MEXT [20105004]; U.S. National Science Foundation [PHY-0855082, PHY-1205024]; Council of Higher Education of Turkey; University of Wisconsin Research Committee; Wisconsin Alumni Research Foundation; Grants-in-Aid for Scientific Research [20105004] Funding Source: KAKEN; Direct For Mathematical & Physical Scien; Division Of Physics [0855082] Funding Source: National Science Foundation; Division Of Physics; Direct For Mathematical & Physical Scien [1205024] Funding Source: National Science Foundationen_US
dc.description.sponsorshipThis work was supported in part by Grants-in-Aid for Scientific Research of the JSPS (200244035) and for Scientific Research on Innovative Area of MEXT (20105004), in part by JSPS Grant No. 21.6817, in part by the U.S. National Science Foundation Grant No. PHY-0855082 and PHY-1205024, in part by the Council of Higher Education of Turkey, and in part by the University of Wisconsin Research Committee with funds granted by the Wisconsin Alumni Research Foundation.en_US
dc.language.isoengen_US
dc.publisherElsevieren_US
dc.relation.ispartofPhysics Letters Ben_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectBig-Bang nucleosynthesisen_US
dc.subjectEarly Universeen_US
dc.subjectObservational cosmologyen_US
dc.subjectAbundances of the elementsen_US
dc.titleSolution to Big-Bang nucleosynthesis in hybrid axion dark matter modelen_US
dc.typearticleen_US
dc.authoridBalantekin, Akif/0000-0002-2999-0111
dc.authoridKusakabe, Motohiko/0000-0003-3083-6565
dc.departmentMimar Sinan Güzel Sanatlar Üniversitesien_US
dc.identifier.doi10.1016/j.physletb.2012.11.007
dc.identifier.volume718en_US
dc.identifier.issue3en_US
dc.identifier.startpage704en_US
dc.identifier.endpage708en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.wosqualityQ1
dc.identifier.wosWOS:000314259500002
dc.indekslendigikaynakWeb of Scienceen_US
dc.snmzKA_20250105


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