Black Hole;
Impact Parameter;
Deflection Angle;
Null Energy Condition;
Cauchy Horizon;
D O I:
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摘要:
The models of wormholes with a topology based on a Reissner-Nordström black and white hole are considered. In these models, there are one entrance in one universe (a black hole) and one exit into another universe (a white hole) corresponding to this entrance. The passage of matter through the wormhole in these models is possible only in one direction (from past to future). All models are considered under the assumption of spherical symmetry. It is shown that all models without a throat do not violate the null energy condition. The model of a Reissner-Nordström black hole containing no singularities inside the horizon has been constructed. The trajectories of particles and light rays passing from one universe into another have been constructed for the simplest Reissner-Nordström black and white hole. Distinctive features have been found for the images of objects from another universe observed through such objects. The characteristics of these images are compared with those for ordinary wormholes.
机构:
Inst Space Sci ICE, CSIC, C Can Magrans S-N, Barcelona 08193, Spain
ICREA, Passeig Luis Co 23, Barcelona 08010, SpainNagoya Univ, Dept Phys, Nagoya 4648602, Japan
Odintsov, S. D.
Folomeev, Vladimir
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机构:
Inst Nucl Phys, Alma Ata 050032, Kazakhstan
Academician J Jeenbaev Inst Phys, NAS Kyrgyz Republ, 265 A Chui St, Bishkek 720071, KyrgyzstanNagoya Univ, Dept Phys, Nagoya 4648602, Japan
机构:
Univ Sao Paulo, Escola Artes Ciencias & Humanidades, BR-03828000 Sao Paulo, BrazilUniv Sao Paulo, Escola Artes Ciencias & Humanidades, BR-03828000 Sao Paulo, Brazil
Molina, C.
Neves, J. C. S.
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机构:
Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, BrazilUniv Sao Paulo, Escola Artes Ciencias & Humanidades, BR-03828000 Sao Paulo, Brazil