We study for the first time the case in which Dark Matter (DM) is made of Feebly Interacting Massive Particles (FIMP) interacting just gravitationally with the standard model particles in an extra-dimensional Randall-Sundrum scenario. We assume that both the dark matter and the standard model are localized in the IR-brane and only interact via gravitational mediators, namely the graviton, the Kaluza-Klein gravitons and the radion. We found that in the early Universe DM could be generated via two main processes: the direct freeze-in and the sequential freeze-in. The regions where the observed DM relic abundance is produced are largely compatible with cosmological and collider bounds.
{ "_oai": { "updated": "2021-01-22T10:43:23Z", "id": "oai:repo.scoap3.org:57144", "sets": [ "JHEP" ] }, "authors": [ { "affiliations": [ { "country": "Colombia", "value": "Centro de Investigaciones, Universidad Antonio Nari\u00f1o, Carrera 3 Este # 47A-15, Bogot\u00e1, Colombia", "organization": "Universidad Antonio Nari\u00f1o" } ], "surname": "Bernal", "email": "nicolas.bernal@uan.edu.co", "full_name": "Bernal, Nicol\u00e1s", "given_names": "Nicol\u00e1s" }, { "affiliations": [ { "country": "Spain", "value": "Instituto de F\u00edsica Corpuscular, Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n, Catedr\u00e1tico Jose Beltr\u00e1n 2, Paterna, 46980, Spain", "organization": "Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n" } ], "surname": "Donini", "email": "donini@ific.uv.es", "full_name": "Donini, Andrea", "given_names": "Andrea" }, { "affiliations": [ { "country": "Spain", "value": "Instituto de F\u00edsica Corpuscular, Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n, Catedr\u00e1tico Jose Beltr\u00e1n 2, Paterna, 46980, Spain", "organization": "Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n" } ], "surname": "Folgado", "email": "migarfol@ific.uv.es", "full_name": "Folgado, Miguel", "given_names": "Miguel" }, { "affiliations": [ { "country": "Spain", "value": "Instituto de F\u00edsica Corpuscular, Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n, Catedr\u00e1tico Jose Beltr\u00e1n 2, Paterna, 46980, Spain", "organization": "Universidad de Valencia and CSIC, Edificio Institutos Investigaci\u00f3n" } ], "surname": "Rius", "email": "nuria.rius@ific.uv.es", "full_name": "Rius, Nuria", "given_names": "Nuria" } ], "titles": [ { "source": "Springer", "title": "Kaluza-Klein FIMP dark matter in warped extra-dimensions" } ], "dois": [ { "value": "10.1007/JHEP09(2020)142" } ], "publication_info": [ { "page_end": "31", "journal_title": "Journal of High Energy Physics", "material": "article", "journal_volume": "2020", "artid": "JHEP09(2020)142", "year": 2020, "page_start": "1", "journal_issue": "9" } ], "$schema": "http://repo.scoap3.org/schemas/hep.json", "acquisition_source": { "date": "2020-12-25T01:31:09.831512", "source": "Springer", "method": "Springer", "submission_number": "5299df22464811ebbd0e02163e01809a" }, "page_nr": [ 31 ], "license": [ { "url": "https://creativecommons.org/licenses//by/4.0", "license": "CC-BY-4.0" } ], "copyright": [ { "holder": "The Author(s)", "year": "2020" } ], "control_number": "57144", "record_creation_date": "2020-09-23T05:30:21.556321", "_files": [ { "checksum": "md5:da0dff4f7d4ed1429ec2ec054bdde699", "filetype": "xml", "bucket": "d7c5ce0c-59b1-49a0-bd85-1c00c37ba1e2", "version_id": "5002a8a2-0964-4216-9ae2-fac182a5fc3a", "key": "10.1007/JHEP09(2020)142.xml", "size": 11549 }, { "checksum": "md5:340da2261f2996167277edac43715451", "filetype": "pdf/a", "bucket": "d7c5ce0c-59b1-49a0-bd85-1c00c37ba1e2", "version_id": "140c38b4-3144-4b80-8bd0-6e1f06650b87", "key": "10.1007/JHEP09(2020)142_a.pdf", "size": 624653 } ], "collections": [ { "primary": "Journal of High Energy Physics" } ], "arxiv_eprints": [ { "categories": [ "hep-ph", "astro-ph.CO" ], "value": "2004.14403" } ], "abstracts": [ { "source": "Springer", "value": "We study for the first time the case in which Dark Matter (DM) is made of Feebly Interacting Massive Particles (FIMP) interacting just gravitationally with the standard model particles in an extra-dimensional Randall-Sundrum scenario. We assume that both the dark matter and the standard model are localized in the IR-brane and only interact via gravitational mediators, namely the graviton, the Kaluza-Klein gravitons and the radion. We found that in the early Universe DM could be generated via two main processes: the direct freeze-in and the sequential freeze-in. The regions where the observed DM relic abundance is produced are largely compatible with cosmological and collider bounds." } ], "imprints": [ { "date": "2020-09-22", "publisher": "Springer" } ] }