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Structure Formation during an early period of matter domination

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Structure Formation during an early period of matter domination

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dc.contributor.author Barenboim Szuchman, Gabriela Alejandra
dc.contributor.author Rasero Daparte, Javier
dc.date.accessioned 2014-09-19T10:55:31Z
dc.date.available 2014-09-19T10:55:31Z
dc.date.issued 2014
dc.identifier.citation Barenboim Szuchman, Gabriela Alejandra Rasero Daparte, Javier 2014 Structure Formation during an early period of matter domination Journal of High Energy Physics 04 04 138
dc.identifier.uri http://hdl.handle.net/10550/38927
dc.description.abstract In this work we show that modifying the thermal history of the Universe by including an early period of matter domination can lead to the formation of astronomical objects. However, the survival of these objects can only be possible if the dominating matter decays to a daughter particle which is not only almost degenerate with the parent particle but also has an open coannihilation channel. This requirement translates in an upper bound for the coupling of such a channel and makes the early structure formation viable.
dc.language.iso eng
dc.relation.ispartof Journal of High Energy Physics, 2014, vol. 04, num. 04, p. 138
dc.subject Física
dc.title Structure Formation during an early period of matter domination
dc.type journal article es_ES
dc.date.updated 2014-09-19T10:55:32Z
dc.identifier.doi 10.1007/JHEP04(2014)138
dc.identifier.idgrec 093000
dc.rights.accessRights open access es_ES

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