Work

Formation of bound composite vortices of a singly quantized 1 S 0 vortex and half-quantized 3 P 2 vortices in the 1 S 0 - 3 P 2 coexisting phase in neutron stars

Year: 2026

Type: article

Abstract: Pulsar glitches are believed to originate from the dynamics of quantized vortices in the neutron superfluid interior. The outer core of a neutron star hosts a $^3\text{P}_2$ spin-triplet superfluid, whose half-integer quantum vortices (HQVs) are qualitatively different from the $^1\text{S}_0$ singly quantized vortices (SQVs) in the inner crust. It has recently been proposed that the coupling between these two vortex species gives rise to a large-scale vortex network, providing a candidate mechanism for the diversity of observed pulsar glitch phenomena. Using the Gross--Pitaevskii equations for the $^1\text{S}_0$ and $^3\text{P}_2$ condensates, we perform two-dimensional simulations of one SQV and two HQVs in a coexistence phase near the crust-core boundary, varying the density--density and Josephson coupling constants. We find that the Josephson term, arising from the relative phase between the two condensates, induces a strong attractive interaction between the two HQVs and the SQV, which dominates over the density--density coupling. When pinning potentials are applied to the HQVs and the SQV at spatially separated locations, this attraction is found to be sufficiently strong to drive vortex depinning. These results suggest that two HQVs and one SQV can form a tightly bound composite vortex at the crust-core boundary, with implications for the glitch mechanism in neutron stars.

Source: Physical Review C

DOI: 10.1103/yycf-9kcx

Authors: Tatsuhiro Hattori, Muneto Nitta, Kazuyuki Sekizawa

Language: English

Topic: Pulsars and Gravitational Waves Research

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

Funders: Yukawa Institute for Theoretical Physics, Kyoto University, Japan Society for the Promotion of Science

Awards: Inhomogeneous neutron matter properties and origin of pulsar glitches, Neutron Stars as the Largest Condensed Matter Systems in Universe, G725975793, Exploring Properties of the Inner Crust of Neutron Stars Through Band Theory Calculations Based on Superfluid Density Functional Theory, G7951016028, G8470815915

OpenAlex ID: W7162677109

FWCI:

Cites:

Cited by:

Related to: 10