000364076 001__ 364076
000364076 005__ 20260216083712.0
000364076 0247_ $$2doi$$a10.1103/jg14-8p4l
000364076 0247_ $$2ISSN$$a2470-0010
000364076 0247_ $$2ISSN$$a2470-0037
000364076 0247_ $$2ISSN$$a2470-0029
000364076 0247_ $$2WOS$$aWOS:001578773300024
000364076 037__ $$aGSI-2026-00255
000364076 082__ $$a530
000364076 1001_ $$00000-0003-2472-3863$$aPadilla-Gay, Ian$$b0$$eCorresponding author
000364076 245__ $$aFlavor equilibration of supernova neutrinos: Exploring the dynamics of slow modes
000364076 260__ $$aRidge, NY$$bAmerican Physical Society$$c2025
000364076 3367_ $$2DRIVER$$aarticle
000364076 3367_ $$2DataCite$$aOutput Types/Journal article
000364076 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1768569732_2234522
000364076 3367_ $$2BibTeX$$aARTICLE
000364076 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000364076 3367_ $$00$$2EndNote$$aJournal Article
000364076 500__ $$aERC Starting Grant (NeuTrAE, No. 101165138)
000364076 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000364076 536__ $$0G:(EU-Grant)885281$$aKILONOVA - Probing r-process nucleosynthesis through its electromagnetic signatures (885281)$$c885281$$fERC-2019-ADG$$x1
000364076 588__ $$aDataset connected to CrossRef, Journals: repository.gsi.de
000364076 693__ $$0EXP:(DE-Ds200)no_experiment-20200803$$1EXP:(DE-Ds200)theory-20200803$$5EXP:(DE-Ds200)no_experiment-20200803$$atheory$$eno experiment theory work (theory)$$x0
000364076 7001_ $$00009-0006-3633-010X$$aChen, Heng-Hao$$b1
000364076 7001_ $$00000-0001-8276-997X$$aAbbar, Sajad$$b2
000364076 7001_ $$00000-0003-4960-8706$$aWu, Meng-Ru$$b3
000364076 7001_ $$0P:(DE-Ds200)OR10336$$aXiong, Zewei$$b4$$ugsi
000364076 773__ $$0PERI:(DE-600)2844732-3$$a10.1103/jg14-8p4l$$gVol. 112, no. 4, p. 043039$$n4$$p043039$$tPhysical review / D$$v112$$x2470-0010$$y2025
000364076 909CO $$ooai:repository.gsi.de:364076$$pec_fundedresources$$pVDB$$popenaire
000364076 9101_ $$0I:(DE-Ds200)20121206GSI$$6P:(DE-Ds200)OR10336$$aGSI Helmholtzzentrum für Schwerionenforschung GmbH$$b4$$kGSI
000364076 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
000364076 9141_ $$y2025
000364076 915__ $$0StatID:(DE-HGF)0571$$2StatID$$aDBCoverage$$bSCOAP3 sponsored Journal$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV D : 2022$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0020$$2StatID$$aNo Peer Review$$bASC$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)1230$$2StatID$$aDBCoverage$$bCurrent Contents - Electronics and Telecommunications Collection$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2024-12-10
000364076 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bPHYS REV D : 2022$$d2024-12-10
000364076 9201_ $$0I:(DE-Ds200)KNA-20160901OR396$$kKNA$$lNukleare Astrophysik & Struktur$$x0
000364076 980__ $$ajournal
000364076 980__ $$aVDB
000364076 980__ $$aI:(DE-Ds200)KNA-20160901OR396
000364076 980__ $$aUNRESTRICTED