Physical-process first law for a rotating black hole

For horizon generator

ξ = k + Ω_{H} m

, a small matter flux into an initially and finally stationary rotating black hole satisfies

Δ M - Ω_{H} Δ J = \frac{κ}{8 π} Δ A .

 Ancestors (8)

 Incoming links (6)

Horizon flux inequality for causal matter
Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 54 / 4 / a / Solution
Past exam of the mathematics course of the University of Cambridge / 2018 / iii / Paper 311 / 2 / b / Solution
Past exam of the mathematics course of the University of Cambridge / 2018 / iii / Paper 311 / 2 / c / Solution
Past exam of the mathematics course of the University of Cambridge / 2021 / iii / Paper 311 / 3 / a / Solution
Past exam of the mathematics course of the University of Cambridge / 2023 / iii / Paper 311 / 3 / a / Solution

 View article source

 Discussion (0)

There are no discussions about this article yet.

 Articles by others on the same topic (0)

There are currently no matching articles.

  See all articles in the same topic Create my own version