APA

Visser, M. (2018). Thermodynamics and Holography for de Sitter Space. Perimeter Institute. https://pirsa.org/18010074

MLA

Visser, Manus. Thermodynamics and Holography for de Sitter Space. Perimeter Institute, Jan. 09, 2018, https://pirsa.org/18010074

BibTex

@misc{ pirsa_PIRSA:18010074,
  doi = {10.48660/18010074},
  url = {https://pirsa.org/18010074},
  author = {Visser, Manus},
  keywords = {Cosmology},
  language = {en},
  title = {Thermodynamics and Holography for de Sitter Space},
  publisher = {Perimeter Institute},
  year = {2018},
  month = {jan},
  note = {PIRSA:18010074 see, \url{https://pirsa.org}}
}
            

Abstract

In this talk I will present new insights on a microscopic holographic theory for de Sitter space. I will focus on the static patch of dS, which describes our universe to a good approximation at late times. We use a conformal map between dS and the BTZ black hole times a sphere to relate the general microscopic properties of dS to those of symmetric product CFTs. In 2d CFT language, de Sitter space corresponds to a thermal bath of long string. The long string phenomenon exhibited by these CFTs implies that the excitation energy decreases at large distances in dS (contrary to the UV/IR relation in AdS/CFT). It also explains the smallness of the vacuum energy of dS. Similar results apply to Minkowski space and AdS below its curvature radius.