Thermodynamics and Holography for de Sitter Space
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}} }
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.