2010
DOI: 10.1103/physrevd.82.026007
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Peak-dip-hump lineshape from holographic superconductivity

Abstract: We study the fermionic spectral function in a holographic superconductor model. At zero temperature, the black hole has zero horizon and hence the entropy of the system is zero after the back reaction of the condensate is taken into account. We find the system exhibits the famous peak-dip-hump lineshape with a sharp low-energy peak followed by a dip then a hump at higher energies. This feature is widely observed in the spectrum of several high-Tc superconductors. We also find a linear relation between the gap … Show more

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Cited by 40 publications
(45 citation statements)
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“…The difference between k F without the condensate and the surface of minimum gap will be small in the examples we study, which have T c small compared to µ, and are therefore close to the RN geometry as we review below. [48] appeared as this paper was being completed. The crucial Majorana coupling is not included there.…”
Section: Jhep03(2010)121mentioning
confidence: 99%
“…The difference between k F without the condensate and the surface of minimum gap will be small in the examples we study, which have T c small compared to µ, and are therefore close to the RN geometry as we review below. [48] appeared as this paper was being completed. The crucial Majorana coupling is not included there.…”
Section: Jhep03(2010)121mentioning
confidence: 99%
“…At low temperature, they can condense, spontaneously breaking the U (1) symmetry, changing the background [36][37][38]. The problem of the fermion response in various possible holographic superconducting phases has been studied [24,[76][77][78][79][80][81]. The superconducting condensate can open a gap in the fermion spectrum around the chemical potential [27] if a suitable bulk coupling between spinor and scalar is included.…”
Section: The Superconducting Statementioning
confidence: 99%
“…For the RN-AdS 4 background, fermion correlators in the dual boundary theory have been studied extensively; see, for example, [24,41,[46][47][48][49][50][51][52][53][54][55][56][57][58][59][60]. A similar kind of analysis can be done here for the electron star background.…”
Section: Discussionmentioning
confidence: 87%