Video URL
https://pirsa.org/20120014New Pathways to the Relic Abundance of Vector-Portal Dark Matter
APA
Fitzpatrick, P. (2020). New Pathways to the Relic Abundance of Vector-Portal Dark Matter. Perimeter Institute for Theoretical Physics. https://pirsa.org/20120014
MLA
Fitzpatrick, Patrick. New Pathways to the Relic Abundance of Vector-Portal Dark Matter. Perimeter Institute for Theoretical Physics, Dec. 08, 2020, https://pirsa.org/20120014
BibTex
@misc{ scivideos_PIRSA:20120014, doi = {10.48660/20120014}, url = {https://pirsa.org/20120014}, author = {Fitzpatrick, Patrick}, keywords = {Particle Physics}, language = {en}, title = {New Pathways to the Relic Abundance of Vector-Portal Dark Matter}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2020}, month = {dec}, note = {PIRSA:20120014 see, \url{https://scivideos.org/pirsa/20120014}} }
Patrick Fitzpatrick Massachusetts Institute of Technology (MIT) - MIT Department of Nuclear Science and Engineering
Abstract
In the conventional weakly-interacting massive particle (WIMP) paradigm the late-time density of dark matter (DM) is set by the rate of two-body annihilations, but there has been considerable recent interest in exploring alternative DM scenarios where other interactions control the final abundance. I will show that by fully exploring the parameter space of a simple, weakly-coupled dark sector, we can find a rich set of novel pathways which lead to the observed relic density of DM. In particular, we can identify and characterize a general class of mechanisms in which the DM relic abundance is determined by processes controlling the thermal coupling of the DM and Standard Model (dubbed the KINetically DEcoupling Relic -- KINDER), generalizing previously-studied special cases of this behavior.