Pressure dependence of upper critical fields in FeSe single crystals

TL;DR

This study explores how pressure influences the upper critical magnetic fields in FeSe single crystals, revealing a critical pressure where magnetic order coexists with superconductivity and significantly impacts their properties.

Contribution

It provides new insights into the pressure-dependent behavior of upper critical fields and magnetic effects in FeSe, highlighting the role of magnetic order in superconductivity suppression.

Findings

Upper critical fields are smaller than the orbital limit, indicating additional effects.

The Maki parameter increases with pressure for H//c, showing enhanced Pauli effects.

Pressure-induced magnetic order negatively impacts superconducting properties.

Abstract

We investigate the pressure dependence of the upper critical fields ({\mu}$_0$$H$$_{c2}$) for FeSe single crystals with pressure up to 2.57 GPa. The superconducting (SC) properties show a disparate behavior across a critical pressure where the pressure-induced antiferromagnetic phase coexists with superconductivity. The magnetoresistance for $H//ab$ and $H//c$ is very different: for $H//c$, magnetic field induces and enhances a hump in the resistivity close to the $T_c$ for pressures higher than 1.2 GPa, while it is absent for $H//ab$. Since the measured {\mu}$_0$$H$$_{c2}$ for FeSe samples is smaller than the orbital limited upper critical field ($H$$^{orb}$$_{c2}$) estimated by the Werthamer Helfand and Hohenberg (WHH) model, the Maki parameter ({\alpha}) related to Pauli spin-paramagnetic effects is additionally considered to describe the temperature dependence of {\mu}$_0$$H$$_{c2}$($T$). Interestingly, the {\alpha} value is hardly affected by pressure for $H//ab$, while it strongly increases with pressure for $H//c$. The pressure evolution of the {\mu}$_0$$H$$_{c2}$(0)s for the FeSe single crystals is found to be almost similar to that of $T_c$($P$), suggesting that the pressure-induced magnetic order adversely affects the upper critical fields as well as the SC transition temperature.