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Universal class of type-IIB flux vacua with analytic mass spectrum

dc.contributor.authorBlanco Pillado, José Juan
dc.contributor.authorSousa, Kepa ORCID
dc.contributor.authorÁlvarez Urquiola, Mikel ORCID
dc.contributor.authorWachter, Jeremy M.
dc.date.accessioned2021-06-25T07:53:44Z
dc.date.available2021-06-25T07:53:44Z
dc.date.issued2021-05
dc.identifier.citationPhysical Review D 103(10) : (2021) // Article ID 106006es_ES
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttp://hdl.handle.net/10810/52010
dc.description.abstractWe report on a new class of flux vacua generically present in Calabi-Yau compactifications of type-IIB string theory. At these vacua, the mass spectrum of the complete axiodilaton/complex structure sector is given, to leading order in a' and g(s), by a simple analytic formula independent of the choice of Calabi-Yau. We provide a method to find these vacua and construct an ensemble of 17,054 solutions for the Calabi-Yau hypersurface WP[1,1,1,6,9]4, where the masses of the axiodilaton and the 272 complex structure fields can be explicitly computed.es_ES
dc.description.sponsorshipThis work is supported by the Spanish Ministry MCIU/AEI/FEDER Grant No. PGC2018-094626-B-C21, the Basque Government Grant No. IT-979-16, and the Basque Foundation for Science (IKERBASQUE). K. S. is supported by the Czech science foundation GACR Grant No. 19-01850S. M. A. U. is also supported by the University of the Basque Country Grant No. PIF17/74. For the numerical work, we used the computing infrastructure of the ARINA cluster at the University of the Basque Country (UPV/EHU).es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.relationinfo:eu-repo/grantAgreement/MINECO/PGC2018-094626-B-C21es_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectmirror symmetryes_ES
dc.titleUniversal class of type-IIB flux vacua with analytic mass spectrumes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation,and DOI. Funded by SCOAP.es_ES
dc.rights.holderAtribución 3.0 España*
dc.relation.publisherversionhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.106006es_ES
dc.identifier.doi10.1103/PhysRevD.103.106006
dc.departamentoesFísicaes_ES
dc.departamentoeuFisikaes_ES


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Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation,and DOI. Funded by SCOAP.
Except where otherwise noted, this item's license is described as Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation,and DOI. Funded by SCOAP.