Non-Lorentzian geometry in gravity, string theory and holography
APA
Obers, N. (2018). Non-Lorentzian geometry in gravity, string theory and holography. Perimeter Institute. https://pirsa.org/18050067
MLA
Obers, Niels. Non-Lorentzian geometry in gravity, string theory and holography. Perimeter Institute, May. 29, 2018, https://pirsa.org/18050067
BibTex
@misc{ pirsa_PIRSA:18050067, doi = {10.48660/18050067}, url = {https://pirsa.org/18050067}, author = {Obers, Niels}, keywords = {Quantum Fields and Strings}, language = {en}, title = {Non-Lorentzian geometry in gravity, string theory and holography}, publisher = {Perimeter Institute}, year = {2018}, month = {may}, note = {PIRSA:18050067 see, \url{https://pirsa.org}} }
I will present a brief introduction to non-Lorentzian geometries, an important example of such geometries being Newton-Cartan geometry and its torsionful generalization, which is the natural geometry to which non-relativistic field theories couple to. The talk will subsequently review how such geometries have in recent years appeared in gravity, string theory and holography. In particular, torsional Newton-Cartan geometry has been shown to appear as the boundary geometry for Lifshitz spacetimes. Furthermore, dynamical Newton-Cartan geometry is related to Horava-Lifsthiz gravity theories and appears in novel Chern-Simons theories of gravity in three dimensions. The latter can be obtained from a well-defined limit of the AdS3/CFT2 correspondence. Finally, I will briefly comment on how Newton-Cartan geometry appears in non-relativistic string theory.