It is not an exaggeration to say that one of the most exciting predictions of Einstein's theory of gravitation is that there may exist "black holes": putative objects whose gravitational fields are so strong that no physical bodies or signals can break free of their pull and escape. The proof that black holes do exist, and an analysis of their properties, would have a significance going far beyond astrophysics. Indeed, what is involved is not just the discovery of yet another even if extremely remarkable, astro physical object, but a test of the correctness of our understanding of the properties of space and time in extremely strong gravitational fields. Theoretical research into the properties of black holes, and into the possible corol laries of the hypothesis that they exist, has been carried out with special vigor since the beginning of the 1970's. In addition to those specific features of black holes that are important for the interpretation of their possible astrophysical manifestations, the theory has revealed a number of unexpected characteristics of physical interactions involving black holes. By the middle of the 1980's a fairly detailed understanding had been achieved of the properties of the black holes, their possible astrophysical manifestations, and the specifics of the various physical processes involved. Even though a completely reliable detection of a black hole had not yet been made at that time, several objects among those scrutinized by astrophysicists were considered as strong candidates to be confirmed as being black holes.
Can objects similar to black holes be used for space and time travel? This book discusses these and many other questions providing the reader with the tools required to explore the Black Hole Land independently.
One of the most exciting predictions of Einstein's theory of gravitationisthat there may exist 'black holes': putative objects whose gravitational fields are so strong that no physical bodies and signals can break free of their pull and ...
The present volume serves as a tutorial, high-level guided tour through the black-hole landscape: information paradox and blackhole thermodynamics, numerical simulations of black-hole formation and collisions, braneworld scenarios and ...
T. Regge, J.A. Wheeler, Stability of a Schwarzschild singularity. Phys. Rev. 108, 1063–1069 (1957) 18. D. Finkelstein, Past-future asymmetry of the gravitational field of a point particle. Phys. Rev. 110, 965–967 (1958) 19.
The Little Book of Black Holes takes readers deep into the mysterious heart of the subject, offering rare clarity of insight into the physics that makes black holes simple yet destructive manifestations of geometric destiny.
Weber's signal from the center of the Milky Way implied that 1,000 solar masses per year were being converted into gravitational wave energy. The young theorist Martin Rees calculated that such a loss of mass would cause the galaxy to ...
The book contains an extensive bibliography the contents of which are amply cited throughout the text. The book well documents the historical development of the theory of Hawking radiation and related topics.
Philosophical Transactions of the Royal Society of London 155 (1865): 459–512. ———. “Introductory Lecture on Experimental Physics.” In The Scientific Papers of James Clerk Maxwell, vol. 2, ed. W. D. Niven, 241–55.
10Named after the mathematician Kurt O. Friedrichs, whose name also is linked to the well-known Courant–Friedrichs–Lewy condition used in the numerical solution of the partial differential equations in fluid flow.
This book is based on the lecture notes of a one-semester course on black hole astrophysics given by the author and is aimed at advanced undergraduate and graduate students with an interest in astrophysics.