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Condensate flow in holographic models in the presence of dark matter
A bstract Holographic model of a three-dimensional current carrying superconductor or superfluid with dark matter sector described by the additional U(1)-gauge field coupled to the ordinary Maxwell one, has been studied in the probe limit. We investigated an-alytically by the Sturm-Liouville variati...
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Published in: | The journal of high energy physics 2016-10, Vol.2016 (10), p.1-37, Article 152 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | A
bstract
Holographic model of a three-dimensional current carrying superconductor or superfluid with
dark matter
sector described by the additional U(1)-gauge field coupled to the ordinary Maxwell one, has been studied in the probe limit. We investigated an-alytically by the Sturm-Liouville variational method, the holographic s-wave and p-wave models in the background of the AdS soliton as well as five-dimensional AdS black hole spacetimes. The two models of p-wave superfluids were considered, the so called SU(2) and the Maxwell-vector. Special attention has been paid to the dependence of the critical chemical potential and critical transition temperature on the velocity of the condensate and
dark matter
parameters. The current
J
in holographic three-dimensional superconductor studied here, shows the linear dependence on
T
c
−
T
for both s and p-wave symmetry. This is in a significant contrast with the previously obtained results for two-dimensional super-conductors, which reveal the (
T
−
T
c
)
3/2
temperature dependence. The coupling constant
α
, as well as, chemical potential
μ
D
and the velocity
S
D
of the
dark matter
, affect the critical chemical potential of the p-wave holographic SU(2) system. On the other hand,
α
,
dark matter
velocity
S
D
and density
ρ
D
determine the actual value of the transition temperature of the same superconductor/superfluid set up. However, the
dark matter
does not affect the value of the current. |
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ISSN: | 1029-8479 1029-8479 |
DOI: | 10.1007/JHEP10(2016)152 |