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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dc.contributor.authorEkinci, B.
dc.contributor.authorPehlivan, Y.
dc.contributor.authorPatwardhan, Amol, V
dc.date.accessioned2025-01-09T20:12:16Z
dc.date.available2025-01-09T20:12:16Z
dc.date.issued2021
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.103.043016
dc.identifier.urihttps://hdl.handle.net/20.500.14124/8524
dc.description.abstractWe calculate the response of a lead-based detector, such as the Helium and Lead Observatory (HALO) or its planned upgrade HALO-1kt to a Galactic core-collapse supernova. We pay particular attention to the time dependence of the reaction rates. All reaction rates decrease as the neutrino luminosity exponentially drops during the cooling period, but the ratio of one-neutron (1n) to two-neutron (2n) event rates in HALO is independent of this overall decrease. Nevertheless, we find that this ratio still changes with time due to the changing character of neutrino flavor transformations with the evolving conditions in the supernova. In the case of inverted hierarchy, this is caused by the fact that the spectral splits become less and less sharp with the decreasing luminosity. In the case of normal hierarchy, it is caused by the passage of the shock wave through the Mikheyev-Smirnov-Wolfenstein resonance region. However, in both cases, we find that the change in the ratio of 1n to 2n event rates is limited to a few percent.en_US
dc.description.sponsorshipAPS Gordon and Betty Moore Foundation for its Visitor Award [GBMF6210]; Scientific and Technological Research Council of Turkey (TUBITAK) [2214A]; TUBITAK [117F327]; NSF [PHY-1630782]; HeisingSimons Foundation [2017-228]; U.S. Department of Energy [DEAC02-76SF00515]en_US
dc.description.sponsorshipY. P. thanks the APS Gordon and Betty Moore Foundation for its Visitor Award, which provided funding for a visit to University of Wisconsin-Madison (Grant No. GBMF6210). B. E. acknowledges the 2214A travel fellowship from the Scientific and Technological Research Council of Turkey (TUBITAK). Y. P. and B. E. thanks the University of Wisconsin-Madison for its hospitality. This work was supported in part by TUBITAK under Project No. 117F327. The work of A. V. P. was supported in part by the NSF (Grant No. PHY-1630782) and the HeisingSimons Foundation (Grant No. 2017-228) and in part by the U.S. Department of Energy under Contract No. DEAC02-76SF00515.en_US
dc.language.isoengen_US
dc.publisherAmer Physical Socen_US
dc.relation.ispartofPhysical Review Den_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.titleTime dependent signatures of core-collapse supernova neutrinos at HALOen_US
dc.typearticleen_US
dc.authoridPatwardhan, Amol/0000-0002-2281-799X
dc.authoridPehlivan Deliduman, Yamac/0000-0003-4475-8203
dc.departmentMimar Sinan Güzel Sanatlar Üniversitesien_US
dc.identifier.doi10.1103/PhysRevD.103.043016
dc.identifier.volume103en_US
dc.identifier.issue4en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.wosqualityQ1
dc.identifier.wosWOS:000621333400002
dc.indekslendigikaynakWeb of Scienceen_US
dc.snmzKA_20250105


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