Video URL
https://pirsa.org/21020015Tidal heating: a hunt for the horizon
APA
Datta, S. (2021). Tidal heating: a hunt for the horizon. Perimeter Institute for Theoretical Physics. https://pirsa.org/21020015
MLA
Datta, Sayak. Tidal heating: a hunt for the horizon. Perimeter Institute for Theoretical Physics, Feb. 04, 2021, https://pirsa.org/21020015
BibTex
@misc{ scivideos_PIRSA:21020015, doi = {10.48660/21020015}, url = {https://pirsa.org/21020015}, author = {Datta, Sayak}, keywords = {Strong Gravity}, language = {en}, title = {Tidal heating: a hunt for the horizon}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2021}, month = {feb}, note = {PIRSA:21020015 see, \url{https://scivideos.org/pirsa/21020015}} }
Sayak Datta IUCAA - The Inter-University Centre for Astronomy and Astrophysics
Abstract
The defining feature of a classical black hole horizon is that it is a "perfect absorber". Any evidence showing otherwise
would indicate a departure from the standard black-hole picture. Due to the presence of the horizon, black holes in binaries exchange
energy with their orbit, which backreacts on the orbit. This is called tidal heating. Tidal heating can be used to test the presence of a horizon.
I will discuss the prospect of tidal heating as a discriminator between black holes and horizonless compact objects, especially supermassive ones, in LISA.
I will also discuss a similar prospect for distinguishing between neutron stars and black holes in the LIGO band.