APA

D’Agnolo, R. (2016). Light Dark Matter from Boltzmann Tails. Perimeter Institute. https://pirsa.org/16050010

MLA

D’Agnolo, Raffaele. Light Dark Matter from Boltzmann Tails. Perimeter Institute, May. 17, 2016, https://pirsa.org/16050010

BibTex

@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}}
}
            

Abstract

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.