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Limits to the analog Hawking temperature in a Bose-Einstein condensate

dc.contributor.authorWuester, Sebastian
dc.contributor.authorSavage, Craig
dc.date.accessioned2015-12-07T22:54:04Z
dc.date.issued2007
dc.date.updated2015-12-07T12:46:08Z
dc.description.abstractQuasi-one-dimensional outflow from a dilute gas Bose-Einstein condensate reservoir is a promising system for the creation of analog Hawking radiation. We use numerical modeling to show that stable sonic horizons exist in such a system under realistic conditions, taking into account the transverse dimensions and three-body loss. We find that loss limits the analog Hawking temperatures achievable in the hydrodynamic regime, with sodium condensates allowing the highest temperatures. A condensate of 30 000 atoms, with transverse confinement frequency ω =6800×2π Hz, yields horizon temperatures of about 20 nK over a period of 50 ms. This is at least four times higher than for other atoms commonly used for Bose-Einstein condensates.
dc.identifier.issn1050-2947
dc.identifier.urihttp://hdl.handle.net/1885/28009
dc.publisherAmerican Physical Society
dc.sourcePhysical Review A: Atomic, Molecular and Optical Physics
dc.subjectKeywords: Atomic physics; Gas dynamics; Hydrodynamics; Thermal effects; Bose-Einstein condensate reservoir; Hawking radiation; Quasi-one-dimensional outflow; Sodium condensates; Bose-Einstein condensation
dc.titleLimits to the analog Hawking temperature in a Bose-Einstein condensate
dc.typeJournal article
local.bibliographicCitation.issue013608
local.bibliographicCitation.lastpage8
local.bibliographicCitation.startpage1
local.contributor.affiliationWuester, Sebastian, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSavage, Craig, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidWuester, Sebastian, u4058311
local.contributor.authoruidSavage, Craig, u8905287
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020604 - Quantum Optics
local.identifier.ariespublicationu4103646xPUB55
local.identifier.citationvolume76
local.identifier.doi10.1103/PhysRevA.76.013608
local.identifier.scopusID2-s2.0-34547357910
local.type.statusPublished Version

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