Please use this identifier to cite or link to this item: https://ir.swu.ac.th/jspui/handle/123456789/14350
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dc.contributor.authorSiopsis G.
dc.contributor.authorTherrien J.
dc.contributor.authorMusiri S.
dc.date.accessioned2021-04-05T03:34:20Z-
dc.date.available2021-04-05T03:34:20Z-
dc.date.issued2012
dc.identifier.issn2649381
dc.identifier.other2-s2.0-84859571597
dc.identifier.urihttps://ir.swu.ac.th/jspui/handle/123456789/14350-
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84859571597&doi=10.1088%2f0264-9381%2f29%2f8%2f085007&partnerID=40&md5=cd4c24bcdb2b5d4b3015dc604bd1358b
dc.description.abstractWe discuss holographic superconductors in an arbitrary dimension whose dual black holes have a scalar hair of mass near the Breitenlohner-Freedman bound. We concentrate on low temperatures in the probe limit. We show analytically that when the bound is saturated, the condensate diverges at low temperatures as |lnT| δ, where δ depends on the dimension. This mild divergence was missed in earlier numerical studies. We calculate the conductivity analytically and show that at low temperatures, all poles move toward the real axis. We obtain an increasingly large number of poles which approach the zeroes of the Airy function in 2+1 dimensions and of the Gamma function in 3+1 dimensions. Our analytic results are in good agreement with numerical results whenever the latter are available. © 2012 IOP Publishing Ltd.
dc.titleHolographic superconductors near the Breitenlohner-Freedman bound
dc.typeArticle
dc.rights.holderScopus
dc.identifier.bibliograpycitationClassical and Quantum Gravity. Vol 29, No.8 (2012), p.-
dc.identifier.doi10.1088/0264-9381/29/8/085007
Appears in Collections:Scopus 1983-2021

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