Ultralight dark photons are dark matter candidates supported by a burgeoning direct-detection program searching for their kinetic mixing with the ordinary photon. A dark photon's dynamics in the early Universe, however, can easily breach the validity of the low-energy effective theory for a massive vector field, with disastrous consequences for its viability as a dark matter candidate. I will assess the extent to which the direct detection of dark photon dark matter would require a nonminimal dark sector. Specifically, I will survey the detection prospects of known dark photon production mechanisms, outline model-building strategies that are viable in expanded parameter space, and discuss complementary cosmological and astrophysical signatures that could probe the physics responsible for dark photon production.
| Building: | Randall Laboratory |
|---|---|
| Event Type: | Lecture / Discussion |
| Tags: | brown bag, Brown Bag Seminar, Physics |
| Source: | Happening @ Michigan from Leinweber Institute for Theoretical Physics, Department of Physics, HET Brown Bag Series, Leinweber Institute for Theoretical Physics Seminars, Leinweber Institute for Theoretical Physics Brown Bag Seminars |
Events
May
05
Cosmo-Astro Seminar | The progenitor’s impact on globular cluster stellar stream models
Brian Cook, University of North Carolina
2:00 PM
302 (Serpens)
West Hall
May
07
Cosmo-Astro Seminar | Taming projection effects in EFTofLSS analysis of DESI DR1 and beyond
Marco Bonici (University of Waterloo)
11:00 AM
3247 Neal Lab
Randall Laboratory
