On Black Holes in Massive Gravity
APA
Berezhiani, L. (2011). On Black Holes in Massive Gravity. Perimeter Institute. https://pirsa.org/11120043
MLA
Berezhiani, Lasha. On Black Holes in Massive Gravity. Perimeter Institute, Dec. 09, 2011, https://pirsa.org/11120043
BibTex
@misc{ pirsa_PIRSA:11120043, doi = {10.48660/11120043}, url = {https://pirsa.org/11120043}, author = {Berezhiani, Lasha}, keywords = {Particle Physics}, language = {en}, title = {On Black Holes in Massive Gravity}, publisher = {Perimeter Institute}, year = {2011}, month = {dec}, note = {PIRSA:11120043 see, \url{https://pirsa.org}} }
University of Pennsylvania
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Abstract
In massive gravity the so-far-found black hole solutions on Minkowski space happen to convert horizons into a certain type of singularities. I will discuss whether these singularities can be avoided if space-time is not asymptotically Minkowskian. As an illustration, I will present an exact analytic black hole solution which evades the above problem by a transition at large scales to self-induced de Sitter space-time. The solution demonstrates that in massive GR, in the Schwarzschild coordinate system, a BH metric has to be accompanied by the St\"uckelberg fields with nontrivial backgrounds to prevent the horizons to convert into the singularities.