Towards high temperature holographic superconductors
Mahya Mohammadi, Ahmad Sheykhi

TL;DR
This paper investigates how non-minimal coupling functions and hyperscaling violation influence phase transitions and conductivity in holographic superconductors, revealing universal behaviors and optimal coupling forms for better understanding.
Contribution
It introduces various non-minimal coupling functions in holographic superconductor models and analyzes their effects on phase transition properties and conductivity, including the impact of hyperscaling violation.
Findings
Larger non-minimal coupling parameter $oldsymbol{eta}$ facilitates phase transition.
Hyperscaling violation parameter $ heta$ increases critical temperature.
Universal behaviors like infinite DC conductivity are observed.
Abstract
We explore a holographic superconductor model in which a real scalar field is non-minimally coupled to a gauge field. We consider several types of the non-minimal coupling function h() including exponential, hyperbolic (cosh), power-law and fractional forms. We investigate the influences of the non-minimal coupling parameter on condensation, critical temperature and conductivity. We can categorize our results in two groups. In the first group, conductor/superconductor phase transition is easier to occur for larger values of , while in the second group stronger effects of the non-minimal coupling makes the formation of scalar hair harder. Although the real and imaginary parts of conductivity are impressed by different forms of h(), they follow some universal behaviors such as connecting with each other through Kramers-Kronig relation in low frequency regime…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena
