Use this URL to cite or link to this record in EThOS: https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.792611
Title: Dark matter genesis
Author: Kirk, Russell
Awarding Body: Royal Holloway, University of London
Current Institution: Royal Holloway, University of London
Date of Award: 2017
Availability of Full Text:
Access from EThOS:
Access from Institution:
Abstract:
There is abundant evidence pointing to an unseen component of the Universe comprising approximately 80% of its mass; this dark matter cannot be any known particle, and so demands new physics. Very little is known about dark matter, however from the cosmic microwave background, its abundance has been accurately measured. How this is produced then dictates the requirements placed on a theory of dark matter. Here four works [1-4] are described where theories of dark matter genesis are explored. The first mechanism considers an additional source of dark matter from decaying topological defects in the early Universe. Topological defects are massive structures formed during spontaneous symmetry breaking phase transitions, which evolve under their own tension and decay, possibly producing dark matter during freeze-out. This allows the annihilation cross-section to rise above what is required in standard freeze-out, as the losses in abundance it predicts, may be recuperated by the contributions from the decaying defects. Given this, the constraints standard freeze-out imposes on dark matter models can be loosen. This is illustrated by implementing the mechanism in an example theory, the Inert Doublet Model, where it opens up large swathes of parameter space and allows for lighter dark matter masses. Furthermore this mechanism is employed to resolve issues with dark matter interpretations of the galactic centre gamma-ray excess seen by Fermi-LAT. The cross-section required to produce this signal is in tension with limits from searches in dwarf spheroidal satellite galaxies. Using this mechanism in a p-wave annihilating model of dark matter, this tension is avoided while producing the correct relic abundance of dark matter. Additionally we examine the direct detection signatures in upcoming detectors, DEAP-3600 and XENON1T, of nuclear dark matter: bound states of strongly-interacting dark nucleons, formed during a synthesis period in the early Universe. Scatterings of states in this model produce characteristic recoil spectra, which we found can be distinguished to 3 sigma confidence level from WIMP spectra with as few as ~24 events. Subsequently there is potential for discovery in the not too distant future.
Supervisor: Not available Sponsor: Not available
Qualification Name: Thesis (Ph.D.) Qualification Level: Doctoral
EThOS ID: uk.bl.ethos.792611  DOI: Not available
Share: