White holes and high energy astrophysics
| dc.contributor.author | Narlikar, J. V. | |
| dc.contributor.author | Apparao, K. M. V. | |
| dc.date.accessioned | 2012-03-09T13:17:18Z | |
| dc.date.available | 2012-03-09T13:17:18Z | |
| dc.date.issued | 1975-01-01 | |
| dc.description.abstract | The role of exploding objects in high-energy astrophysics is discussed. Quantitative results are obtained for the simple case of the canonical white hole which explodes from a singularity and consists of pressure-free matter in the comoving frame of reference. General relativity is used for calculating the dynamical results. Applications to X-ray background, transient X-ray sources, gamma-ray bursts, and high energy cosmic rays are considered. White holes of more general types are discussed in a qualitative manner. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/1119 | |
| dc.language.iso | en | en_US |
| dc.publisher | Kluwer Academic Publishers | en_US |
| dc.relation.ispartofseries | Astrophysics and Space Science;Vol. 35, 1975 | |
| dc.subject | White holes | en_US |
| dc.subject | High energy | en_US |
| dc.subject | Astrophysics | en_US |
| dc.subject | Relativity | en_US |
| dc.subject | X-Rays sources | en_US |
| dc.subject | Cosmic rays | en_US |
| dc.subject | Cosmology | en_US |
| dc.subject | Light transmission | en_US |
| dc.subject | Monochromatic radiation | en_US |
| dc.title | White holes and high energy astrophysics | en_US |
| dc.type | Article | en_US |