Phase structure of neutron superfluids in strong magnetic fields in neutron stars
arXiv:1810.04901 · doi:10.1103/PhysRevC.99.035213
Abstract
We discuss the effect of a strong magnetic field on neutron superfluidity. Based on the attraction in the pair of two neutrons, we derive the Ginzburg-Landau equation in the path-integral formalism by adopting the bosonization technique and leave the next-to-leading order in the expansion of the magnetic field . We determine the phase diagram with temperature , comprising three phases: the uniaxial nematic (UN) phase for , D-biaxial nematic (BN) and D-BN phases in finite and strong such as magnetars, respectively, where D and D are dihedral groups. We find that, compared with the leading order in the magnetic field known before, the region of the D-BN phase in the plane is extended by the effect of the next-to-leading-order terms of the magnetic field. We also present the thermodynamic properties, such as heat capacities and spin susceptibility, and find that the spin susceptibility exhibits anisotropies in the UN, D-BN, and D-BN phases. This information will be useful to understand the internal structures of magnetars.
11 pages, 3 figures
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