Effects of rotochemical heating on the thermal evolution of superfluid neutron stars
Chun-Mei Pi
TL;DR
This paper investigates how rotochemical heating influences the thermal evolution of superfluid neutron stars, showing that including this effect aligns models more closely with observational data.
Contribution
It introduces a model that incorporates rotochemical heating into neutron star cooling, providing a more accurate description of their thermal evolution.
Findings
Rotochemical heating significantly affects neutron star cooling curves.
The model aligns well with observational data.
Inclusion of superfluid effects improves thermal evolution predictions.
Abstract
The authors take the rotochemical heating effect into account, which may make the cooling scenario different. Their model is consistent with the observation data.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Quantum, superfluid, helium dynamics