Nobel-winning black hole physics by Penrose, Hawking stands on work of Indian physicist Amal Raychaudhuri
The Raychaudhuri Equation continues to be a key tool in investigating the behaviour of black hole horizons in modern physics.


This illustration depicts a cosmic homicide in action. A wayward star is being shredded by the intense gravitational pull of a black hole that contains tens of thousands of solar masses. Image credit: NASA, ESA and D. Player[/caption]A black hole is a region of spacetime where gravity is so strong that nothing—no particles or even electromagnetic radiation such as light—can escape from it. Einstein's theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.Singularities are locations in spacetime where the gravitational field of an object is thought to become infinite in a way that is independent of the coordinate systems. Singularities can be found in all the known black-hole spacetimes, which ties them together in the search for answers in astrophysics.The Penrose–Hawking singularity theorems try to explain the conditions under which gravitation produces 'singularities'. The Raychaudhuri Equation is a fundamental lemma for this series of theories on black holes. Penrose, in collaboration with cosmologist Stephen Hawking, used the Raychauduri equation published in the journal Physical Review in 1955, for a mathematical description of black holes in 1969. Even though General Relativity had predicted their existence, Einstein himself did not believe in them.

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