Please use this identifier to cite or link to this item:
http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3428Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.creator | Barceló, Carlos | - |
| dc.creator | Liberati, Stefano | - |
| dc.creator | Sonego, Sebastiano | - |
| dc.creator | Visser, Matt | - |
| dc.date | 2008-04-03T01:11:29Z | - |
| dc.date | 2008-04-03T01:11:29Z | - |
| dc.date | 2006-07-03 | - |
| dc.date.accessioned | 2017-01-31T01:01:27Z | - |
| dc.date.available | 2017-01-31T01:01:27Z | - |
| dc.identifier | Phys.Rev.Lett. 97 (2006) 171301 | - |
| dc.identifier | arXiv:gr-qc/0607008v1 | - |
| dc.identifier | 0031-9007 | - |
| dc.identifier | http://hdl.handle.net/10261/3428 | - |
| dc.identifier.uri | http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3428 | - |
| dc.description | revtex4, 4 pages, 1 figure.-- Final version of the paper available at: http://prl.aps.org/ | - |
| dc.description | We 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 a trapped region in the acoustic spacetime (corresponding to a supersonic regime in the fluid flow). It is sufficient to set up a dynamically changing flow asymptotically approaching a sonic regime with sufficient rapidity in laboratory time. | - |
| dc.description | Peer reviewed | - |
| dc.format | 133050 bytes | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | American Physical Society | - |
| dc.relation | Preprint | - |
| dc.rights | openAccess | - |
| dc.subject | General Relativity and Quantum Cosmology | - |
| dc.subject | Hawking radiation | - |
| dc.subject | Trapped regions | - |
| dc.subject | Horizons | - |
| dc.subject | Acoustic spacetimess | - |
| dc.title | Hawking-like radiation does not require a trapped region | - |
| dc.type | Pre-print | - |
| Appears in Collections: | Digital Csic | |
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.