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dc.creatorTruong, Phuongmai N
dc.date.accessioned2009-06-09T18:53:33Z
dc.date.available2009-06-09T18:53:33Z
dc.date.issued2009-06-09
dc.identifier.urihttps://hdl.handle.net/1969.1/86486
dc.description.abstractSupercritical String Cosmology (SSC) introduces a time-dependent dilaton and a central charge deficit into the history of the development of the universe. To balance the effect of the dilaton and the central charge deficit, the so-called exotic matter, which includes any type of matter but baryonic and dark matters, is also introduced. These three quantities inadvertently alter the relic density of all particles, including dark matter candidates. In this work, we are interested in the correlation between the dark matter density and the equation of state of exotic matter. Using numerical method, we show that there can only be a dilution of dark matter, which ranges approximately between 0.02 – 0.1, depending on how strictly we require the various constraints to be satisfieden
dc.format.mediumelectronicen
dc.language.isoen_US
dc.subjectmodified Boltzmann equationen
dc.subjecttime-dependent dilatonen
dc.subjectdark matteren
dc.subjectsupercritical string cosmologyen
dc.titleThe Effect of Supercritical String Cosmology on the Relic Density of Dark Matteren
dc.typeThesisen
dc.type.genreThesisen
dc.type.materialtexten
dc.format.digitalOriginborn digitalen


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