BMS-like symmetries in cosmology
APA
Bonga, B. (2022). BMS-like symmetries in cosmology. Perimeter Institute. https://pirsa.org/22090081
MLA
Bonga, Beatrice. BMS-like symmetries in cosmology. Perimeter Institute, Sep. 15, 2022, https://pirsa.org/22090081
BibTex
@misc{ pirsa_PIRSA:22090081, doi = {10.48660/22090081}, url = {https://pirsa.org/22090081}, author = {Bonga, Beatrice}, keywords = {Quantum Gravity}, language = {en}, title = {BMS-like symmetries in cosmology}, publisher = {Perimeter Institute}, year = {2022}, month = {sep}, note = {PIRSA:22090081 see, \url{https://pirsa.org}} }
There exists a solid framework to study gravitational waves in full, non-linear general relativity when the spacetime is asymptotically flat. An essential aspect of this framework is asymptotic symmetries. These symmetries are the BMS symmetries. The situation for cosmological spacetimes is different, however. Expanding spacetimes, whose expansion is decelerating such as matter- or radiation-dominated universes, share some similarities with the asymptotically flat case nonetheless. Not surprisingly, their asymptotic symmetries also share similarities with the BMS symmetries, but are not the same.
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