Quantum Field Theory of Interacting Dark Matter/Dark Energy: Dark Monodromies
Nemanja Kaloper - University of California, Davis
D’Agnolo, R. (2016). Light Dark Matter from Boltzmann Tails. Perimeter Institute. https://pirsa.org/16050010
D’Agnolo, Raffaele. Light Dark Matter from Boltzmann Tails. Perimeter Institute, May. 17, 2016, https://pirsa.org/16050010
@misc{ pirsa_PIRSA:16050010,
doi = {10.48660/16050010},
url = {https://pirsa.org/16050010},
author = {D{\textquoteright}Agnolo, Raffaele},
keywords = {Particle Physics},
language = {en},
title = {Light Dark Matter from Boltzmann Tails},
publisher = {Perimeter Institute},
year = {2016},
month = {may},
note = {PIRSA:16050010 see, \url{https://pirsa.org}}
}
Dark matter can be a thermal relic exponentially lighter than
the weak scale without being exponentially weakly coupled. I will present
three mechanisms to obtain light thermal dark matter with sizable
self-interactions and couplings to the Standard Model.