| Entropy | |
| Thermal BEC Black Holes | |
| Roberto Casadio2  Andrea Giugno2  Octavian Micu1  Alessio Orlandi2  Remo Garattini3  | |
| [1] Institute of Space Science, Atomistilor 409, 077125 Magurele, Ilfov, Romania; E-Mail:;Dipartimento di Fisica e Astronomia, Alma Mater Università di Bologna, via Irnerio 46, 40126 Bologna, Italy; E-Mails:Dipartimento di Fisica e Astronomia, Alma Mater Università di Bologna, via Irnerio 46, 40126 Bologna, Italy; | |
| 关键词: black holes; horizon wave function; Hawking radiation; generalized uncertainty principle; | |
| DOI : 10.3390/e17106893 | |
| 来源: mdpi | |
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【 摘 要 】
We review some features of Bose–Einstein condensate (BEC) models of black holes obtained by means of the horizon wave function formalism. We consider the Klein–Gordon equation for a toy graviton field coupled to a static matter current in a spherically-symmetric setup. The classical field reproduces the Newtonian potential generated by the matter source, while the corresponding quantum state is given by a coherent superposition of scalar modes with a continuous occupation number. An attractive self-interaction is needed for bound states to form, the case in which one finds that (approximately) one mode is allowed, and the system of
【 授权许可】
CC BY
© 2015 by the authors; licensee MDPI, Basel, Switzerland.
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| RO202003190005167ZK.pdf | 477KB |
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