Dolan, Brian P. (1988) A group-theoretical approach to black-hole radiation. Il Nuovo Cimento B, 102 (6). pp. 649-659. ISSN 1826-9877
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Abstract
It is shown that, for static space-times, the phenomenon of Hawking radiation can be understood in terms of representations of the twodimensional Poincaré group. Thero zero-energy basis vector of one representation contains positive-energy basis vectors of another representation. An action of the two-dimensional Poincaré group is globally defined over the whole of space-time, but only generates isometries at the event horizon and in the asymptotically flat region (where it degenerates to simple translations). Some simple space-times are discussed.
Item Type: | Article |
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Additional Information: | Cite as: Dolan, B.P. Nuov Cim B (1988) 102: 649. https://doi.org/10.1007/BF02725620 |
Keywords: | group-theoretical approach; black-hole radiation; |
Academic Unit: | Faculty of Science and Engineering > Mathematical Physics |
Item ID: | 10521 |
Identification Number: | 10.1007/BF02725620 |
Depositing User: | Dr. Brian Dolan |
Date Deposited: | 20 Feb 2019 15:14 |
Journal or Publication Title: | Il Nuovo Cimento B |
Publisher: | Springer |
Refereed: | Yes |
Related URLs: | |
URI: | https://mu.eprints-hosting.org/id/eprint/10521 |
Use Licence: | This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available here |
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