A Data Driven Solution to the Dark Matter Problem

A Data Driven Solution to the Dark Matter Problem

dc.creatorHoeneisen, Bruce
dc.date2023-05-16
dc.date.accessioned2023-08-08T20:20:06Z
dc.date.available2023-08-08T20:20:06Z
dc.identifierhttps://revistas.usfq.edu.ec/index.php/avances/article/view/2961
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8068327
dc.descriptionA data driven solution to the dark matter problem is presented. This short and self-contained overview is intended for a wide audience, with full technical details available in the cited references. We present redundant, independent and consistent measurements of the dark matter particle comoving root-mean-square velocity vhrms(1), or equivalently, of the dark matter temperature-to-mass ratio. These measurements agree with the “no freeze-in and no freeze-out” scenario of spin zero dark matter that decouples early on from the Standard Model sector, e.g. spin zero dark matter coupled to the Higgs boson or to the top quark. About this paperThe present article was published on April 13th, 2023 in the European Journal of Applied Sciences and it has been assigned a DOI by the EJAS. The work is republished by ACI Avances en Ciencias e Ingenierías according to the creative commons license (Attribution 4.0 International, CC BY 4.0) used by the EJAS, and according to the copyright preserved by the author, Bruce Hoeneisen. Readers can access the original publication via the following link: https://journals.scholarpublishing.org/index.php/AIVP/article/view/14383 or through the DOI: https://doi.org/10.14738/aivp.112.14383.en-US
dc.descriptionA data driven solution to the dark matter problem is presented. This short and self-contained overview is intended for a wide audience, with full technical details available in the cited references. We present redundant, independent and consistent measurements of the dark matter particle comoving root-mean-square velocity vhrms(1), or equivalently, of the dark matter temperature-to-mass ratio. These measurements agree with the “no freeze-in and no freeze-out” scenario of spin zero dark matter that decouples early on from the Standard Model sector, e.g. spin zero dark matter coupled to the Higgs boson or to the top quark. About this paperThe present article was published on April 13th, 2023 in the European Journal of Applied Sciences and it has been assigned a DOI by the EJAS. The work is republished by ACI Avances en Ciencias e Ingenierías according to the creative commons license (Attribution 4.0 International, CC BY 4.0) used by the EJAS, and according to the copyright preserved by the author, Bruce Hoeneisen. Readers can access the original publication via the following link: https://journals.scholarpublishing.org/index.php/AIVP/article/view/14383 or through the DOI: https://doi.org/10.14738/aivp.112.14383.es-ES
dc.formatapplication/pdf
dc.formattext/html
dc.formattext/xml
dc.languagespa
dc.languageeng
dc.publisherUSFQ PRESS, departamento editorial de la Universidad San Francisco de Quito USFQes-ES
dc.relationhttps://revistas.usfq.edu.ec/index.php/avances/article/view/2961/3373
dc.relationhttps://revistas.usfq.edu.ec/index.php/avances/article/view/2961/3409
dc.relationhttps://revistas.usfq.edu.ec/index.php/avances/article/view/2961/3410
dc.rightsDerechos de autor 2023 Bruce Hoeneisenes-ES
dc.rightshttps://creativecommons.org/licenses/by-nc/4.0es-ES
dc.sourceACI Avances en Ciencias e Ingenierías; Vol. 15 No. 1 (2023)en-US
dc.sourceACI Avances en Ciencias e Ingenierías; Vol. 15 Núm. 1 (2023)es-ES
dc.source2528-7788
dc.source1390-5384
dc.source10.18272/aci.v15i1
dc.subjectWarm Dark Matteren-US
dc.subjectGalaxy Rotation Curvesen-US
dc.subjectGalaxy UV Luminosityen-US
dc.subjectDwarf Galaxiesen-US
dc.subjectWarm Dark Matteres-ES
dc.subjectGalaxy Rotation Curveses-ES
dc.subjectGalaxy UV Luminosityes-ES
dc.subjectDwarf Galaxieses-ES
dc.titleA Data Driven Solution to the Dark Matter Problemen-US
dc.titleA Data Driven Solution to the Dark Matter Problemes-ES
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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