Video URL
https://pirsa.org/15100069Dark matter from the Fraternal Twin Higgs
APA
Lasenby, R. (2015). Dark matter from the Fraternal Twin Higgs. Perimeter Institute for Theoretical Physics. https://pirsa.org/15100069
MLA
Lasenby, Robert. Dark matter from the Fraternal Twin Higgs. Perimeter Institute for Theoretical Physics, Oct. 06, 2015, https://pirsa.org/15100069
BibTex
@misc{ scivideos_PIRSA:15100069, doi = {10.48660/15100069}, url = {https://pirsa.org/15100069}, author = {Lasenby, Robert}, keywords = {Particle Physics}, language = {en}, title = {Dark matter from the Fraternal Twin Higgs}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2015}, month = {oct}, note = {PIRSA:15100069 see, \url{https://scivideos.org/pirsa/15100069}} }
Robert Lasenby Anthropic
Abstract
Twin Higgs theories attempt to solve the little hierarchy problem - why has the LHC not yet observed new states stabilising the EW scale? - by introducing a SM-neutral twin sector, related to the SM by an approximate Z_2 symmetry. The physical Higgs is then a PNGB mixture from both sectors, and acts as a portal between them. In this talk, I will discuss the cosmology of minimal (“fraternal”) Twin Higgs models. Higgs portal interactions establish thermal equilibrium between the SM and twin sector at high temperatures, giving a thermal history with possibilities for both symmetric dark matter (through a “twin WIMP miracle”), and asymmetric dark matter (from twin QCD states which naturally have GeV-scale masses). More generally, relic abundances of cosmologically stable states place constraints on the parameters of the theory, and twin sector phase transitions need to be considered.