dc.contributor.author
Zsembinszki, Gabriel
dc.date.accessioned
2024-12-05T21:46:10Z
dc.date.available
2024-12-05T21:46:10Z
dc.date.issued
2016-03-04T10:15:13Z
dc.date.issued
2016-03-04T10:15:13Z
dc.identifier
https://doi.org/10.1088/1751-8113/40/19/020
dc.identifier
http://hdl.handle.net/10459.1/56675
dc.identifier.uri
http://hdl.handle.net/10459.1/56675
dc.description.abstract
We present a model which contains a new complex scalar field Ψ, interacting with a new real
scalar field,
χ, and an effective potential whose symmetry is almost exact, being explicitly broken
by Planck-scale effects. We study the possibility of relatin
g inflation with the dark matter of the
universe. We find that for exponentially small explicit breaking, the model accounts for a period
of inflation in the early universe and gives a dark matter candidate particle.
dc.description.abstract
This work is supported by the Spanish grant FPA-2005-05904 and by Catalan DURSI grants 2005SGR00916 and 2003FI00138.
dc.publisher
IOP Publishing
dc.relation
info:eu-repo/grantAgreement/MEC//FPA2005-05904/ES/
dc.relation
Versió preprint del document publicat a https://doi.org/10.1088/1751-8113/40/19/020
dc.relation
Journal of Physics A: Mathematical and Theoretical, vol. 40, núm. 19
dc.rights
(c) IOP Publishing, 2007
dc.rights
info:eu-repo/semantics/openAccess
dc.title
Unified Model for Inflation and Dark Matter
