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dc.creatorBarceló, Carlos-
dc.creatorLiberati, Stefano-
dc.creatorSonego, Sebastiano-
dc.creatorVisser, Matt-
dc.date2008-04-04T01:09:23Z-
dc.date2008-04-04T01:09:23Z-
dc.date2006-04-12-
dc.date.accessioned2017-01-31T01:01:29Z-
dc.date.available2017-01-31T01:01:29Z-
dc.identifierClass.Quant.Grav. 23 (2006) 5341-5366-
dc.identifierarXiv:gr-qc/0604058v1-
dc.identifier1361-6382-
dc.identifierhttp://hdl.handle.net/10261/3440-
dc.identifier.urihttp://dspace.mediu.edu.my:8181/xmlui/handle/10261/3440-
dc.description30 pages, 16 figures.-
dc.descriptionWe discuss the issue of quasi-particle production by "analogue black holes" with particular attention to the possibility of reproducing Hawking radiation in a laboratory. By constructing simple geometric acoustic models, we obtain a somewhat unexpected result: We show that in order to obtain a stationary and Planckian emission of quasi-particles, it is not necessary to create an ergoregion in the acoustic spacetime (corresponding to a supersonic regime in the flow). It is sufficient to set up a dynamically changing flow either eventually generating an arbitrarily small sonic region v=c, but without any ergoregion, or even just asymptotically, in laboratory time, approaching a sonic regime with sufficient rapidity.-
dc.descriptionC.B. has been funded by the spanish MEC under project FIS2005-05736-C03-01 with a partial FEDER contribution. C.B. and S.L. are also supported by a INFN-MEC collaboration. The research of M.V. was funded in part by the Marsden Fund administered by the Royal Society of New Zealand.-
dc.descriptionPeer reviewed-
dc.format394705 bytes-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherInstitute of Physics Publishing-
dc.relationPreprint-
dc.rightsopenAccess-
dc.subjectAnalogue models-
dc.subjectAcoustic spacetimes-
dc.subjectHawking radiation-
dc.titleQuasi-particle creation by analogue black holes-
dc.typePre-print-
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