Forces and gauge groups beyond the standard model

The discovery of the Higgs boson in 2012 completed the particle content of the Standard Model, but brought into sharp relief two outstanding problems: why is the Higgs so light, and what is the identity of 80% of the matter content of the universe? Neither appears to have an answer within the Standard Model. This thesis attempts to address these problems with the introduction of new forces and gauge groups. I investigate a model where dark matter interacts through a new massive U(1) gauge boson which kinetically mixes with the photon, and show how this model can be tested at neutrino experiments. Supersymmetry may explain the smallness of the Higgs mass compared to the Planck scale, but reconciling the measured value of 126 GeV with the absence of super-partners at colliders is difficult. By gauging various global symmetries of the Standard Model, I show that a variant of Higgsed gauge mediation called auxiliary gauge mediation can provide acceptable supersymmetric spectra. Finally, the astrophysical dark sector may be complicated, with many kinds of allowed interactions, and I describe techniques to diagnose the presence of dark matter at direct-detection experiments independent of its velocity distribution.

Department dc:contributor.department

Massachusetts Institute of Technology. Department of Physics.

Grantor dc:publisher

Massachusetts Institute of Technology

Year dc:date.issued

2015

Author dc:creator

• Kahn, Yonatan Frederick

Advisor dc:contributor.advisor

• Jesse Diaz Thaler.

• Physics.

Statement dc:rights

• M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.

Licence dc:rights.uri

• http://dspace.mit.edu/handle/1721.1/7582

Language dc:language.iso

eng

Handle dc:identifier.uri

http://hdl.handle.net/1721.1/99311

OAI identifier oai:identifier

oai:dspace.mit.edu:1721.1/99311