dc.contributor.author | Jannes, Gil | |
dc.contributor.author | Philbin, Thomas G. | |
dc.contributor.author | Rousseaux, Germain | |
dc.date.accessioned | 2013-06-21T14:42:28Z | |
dc.date.issued | 2012-07-07 | |
dc.description.abstract | Massive particles are radiated from black holes through the Hawking mechanism together with the more familiar radiation of massless particles. For E ≥ m, the emission rate is identical to the massless case. But E < m particles can also tunnel across the horizon. A study of the dispersion relation and wave packet simulations show that their classical trajectory is similar to that of a boomerang. The tunneling formalism is used to calculate the probability for detecting such E < m particles, for a Schwarzschild black hole of astrophysical size or in an analogue gravity experiment, as a function of the distance from the horizon and the energy of the particle. | en_GB |
dc.identifier.citation | Vol. 1458, pp. 435-438 | en_GB |
dc.identifier.doi | 10.1063/1.4734453 | |
dc.identifier.uri | http://hdl.handle.net/10871/11325 | |
dc.language.iso | en | en_GB |
dc.publisher | American Institute of Physics | en_GB |
dc.subject | black holes | en_GB |
dc.subject | Schwarzschild metric | en_GB |
dc.subject | Hawking radiation | en_GB |
dc.subject | semiclassical approximation | en_GB |
dc.title | Hawking tunneling and boomerang behaviour of massive particles with E < m | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2013-06-21T14:42:28Z | |
dc.identifier.isbn | 9780735410602 | |
dc.identifier.issn | 0094-243X | |
dc.description | Copyright © 2012 American Institute of Physics | en_GB |
dc.description | Towards New Paradigms: Proceeding of the Spanish Relativity Meeting 2011 (ERE2011), 29 August–2 September 2011, Madrid, Spain | en_GB |
dc.identifier.eissn | 1551-7616 | |
dc.identifier.journal | AIP Conference Proceedings | en_GB |