A Holographic Superconductor in an External Magnetic Field
Tameem Albash, Clifford V. Johnson

TL;DR
This paper investigates a holographic superconductor model in anti-de Sitter space with an external magnetic field, revealing how magnetic fields influence condensate formation and structure, including a solvable profile akin to the quantum harmonic oscillator.
Contribution
It introduces a model of a holographic superconductor in a magnetic field, analyzing condensate behavior and structure, including a solvable profile and Meissner-like effect.
Findings
Condensates form in a magnetic field and are localized in one dimension.
The condensate profile maps to the quantum harmonic oscillator.
Increasing magnetic field shrinks the condensate, showing a Meissner effect.
Abstract
We study a system of a complex charged scalar coupled to a Reissner-Nordstrom black hole in 3+1 dimensional anti-de Sitter spacetime, neglecting back-reaction. With suitable boundary conditions, the cases of a neutral and purely electric black hole have been studied in various limits and were shown to yield key elements of superconductivity in the dual 2+1 dimensional field theory, forming a condensate below a critical temperature. By adding magnetic charge to the black hole, we immerse the superconductor into an external magnetic field. We show that a family of condensates can form and we examine their structure. For finite magnetic field, they are localized in one dimension with a profile that is exactly solvable, since it maps to the quantum harmonic oscillator. As the magnetic field increases, the condensate shrinks in size, which is reminiscent of the Meissner effect.
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