Is the cosmological constant a nonlocal quantum residue of discreteness of the causal set type?
APA
Sorkin, R. (2009). Is the cosmological constant a nonlocal quantum residue of discreteness of the causal set type?. Perimeter Institute. https://pirsa.org/09050087
MLA
Sorkin, Rafael. Is the cosmological constant a nonlocal quantum residue of discreteness of the causal set type?. Perimeter Institute, May. 27, 2009, https://pirsa.org/09050087
BibTex
@misc{ pirsa_PIRSA:09050087, doi = {10.48660/09050087}, url = {https://pirsa.org/09050087}, author = {Sorkin, Rafael}, keywords = {Quantum Gravity, Quantum Fields and Strings, Particle Physics, Cosmology}, language = {en}, title = {Is the cosmological constant a nonlocal quantum residue of discreteness of the causal set type?}, publisher = {Perimeter Institute}, year = {2009}, month = {may}, note = {PIRSA:09050087 see, \url{https://pirsa.org}} }
Perimeter Institute for Theoretical Physics
Talk Type
Abstract
The currently accelerating Hubble expansion is in accord with the old heuristic prediction, from causal set theory, of a fluctuating and ever-present cosmological "constant''. More recently, a phenomenological model based on certain of the ideas behind the prediction has been devised, but it remains incomplete. I will review these developments and also mention a possible consequence for the dimensionality of spacetime.