Three-dimensional magneto-thermal evolution of off-centred dipole magnetic field configurations in neutron stars

TL;DR

This paper models the magneto-thermal evolution of neutron stars with off-centred dipole magnetic fields, revealing how initial conditions and magnetic field strength influence magnetic decay, surface temperature distribution, and observable emission properties.

Contribution

First to simulate magneto-thermal evolution of neutron stars with off-centred dipole fields, showing how initial magnetic configurations affect decay and surface emission characteristics.

Findings

Dipole shift decays over time if no toroidal field is present.

Surface thermal maps vary significantly with magnetic field strength.

Magnetic field strength influences pulsed fraction and spectral modeling.

Abstract

Off-centred dipole configurations have been suggested to explain different phenomena in neutron stars, such as natal kicks, irregularities in polarisation of radio pulsars and properties of X-ray emission from millisecond pulsars. Here for the first time we model magneto-thermal evolution of neutron stars with crust-confined magnetic fields and off-centred dipole moments. We find that the dipole shift decays with time if the initial configuration has no toroidal magnetic field. The decay timescale is inversely proportional to magnetic field. The octupole moment decreases much faster than the quadrupole. Alternatively, if the initial condition includes strong dipolar toroidal magnetic field, the external poloidal magnetic field evolves from centred dipole to off-centred dipole. The surface thermal maps are very different for configurations with weak $B = 10^{13}$ G and strong $B = 10^{14}$ G magnetic fields. In the former case, the magnetic equator is cold while in the latter case it is hot. We model lightcurves and spectra of our magneto-thermal configurations. We found that in the case of cold equator, the pulsed fraction is small (below a few percent in most cases) and spectra are well described with a single blackbody. Under the same conditions models with stronger magnetic fields produce lightcurves with pulsed fraction of tens of percent. Their spectra are significantly better described with two blackbodies. Overall, the magnetic field strength has a more significant effect on bulk thermal emission of neutron stars than does the field geometry.