Publication Date:
2012-09-29
Description:
It is shown for a spherically symmetric black hole of general type that it is impossible to observe the infinite future of the Universe external to the hole during the finite proper time interval of the free fall. Quantitative evaluations of the effect of time dilatation for circular orbits around the Kerr black hole are obtained and it is shown that the effect is essential for ultrarelativistic energies of the rotating particle. Content Type Journal Article Category Research Article Pages 1-9 DOI 10.1007/s10714-012-1453-1 Authors Yuri V. Pavlov, Institute of Problems in Mechanical Engineering, Russian Academy of Sciences, Bol’shoy pr. 61, V.O., Saint Petersburg, 199178 Russia Journal General Relativity and Gravitation Online ISSN 1572-9532 Print ISSN 0001-7701
Print ISSN:
0001-7701
Electronic ISSN:
1572-9532
Topics:
Physics