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A theory that describes how matter interacts dynamically with the geometry of space and time. It was first published by Einstein in 1915 and is currently used to study the structure and evolution of the universe, as well as having practical applications like GPS.

2 votes
0 answers
102 views

On separability of wave equation in Kerr metric

In Kerr background given by Boyer-Lindquist(BL) coordinates ($t,\, r,\, \theta,\, \phi $): $$ g_{\mu\nu} dx^{\mu}dx^{\nu}=-(1-\frac{2Mr}{r^2+a^2\cos^2{\theta}})\,dt^2-\frac{r^2+a^2\cos^2{\theta}}{r^ …
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5 votes
1 answer
1k views

Ring singularity of Kerr metric

I have been reading about the Kerr metric using various sources (Wald's textbook, Visser's The Kerr spacetime: A brief introduction etc.). I could not understand exactly why the singularity structure …
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  • 329
4 votes
2 answers
475 views

Global symmetries of spacetime and general covariance

I am self learning GR. This is a rather long post but I needed to clarify few things about the effect of general coordinate transformations on the global symmetries of metric. Any comments, insights a …
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  • 329
4 votes
1 answer
546 views

Planck's constant, Boltzmann constant and Hawking Temperature

The Hawking temperature of a Schwarzschild black hole is given in SI units as $$T_{H}=\frac{\hbar c^3}{8 \pi G k_{B} M},$$ where $k_{B}$ is the Boltzmann constant. I would like to know how $\hbar$ and …
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