M., Bernuzzi, S., & Radice, D

Camilletti, A · 2024 · Physical review. D/Physical review. D. · DOI 10.1103/physrevd.109.063023

1 Pith paper cite this work, alongside 12 external citations. Polarity classification is still indexing.

1 Pith paper citing it

12 external citations · OpenAlex

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representative citing papers

astro-ph.HE · 2025-06-11 · conditional · novelty 5.0

Strong poloidal magnetic fields deform neutron stars and reduce central density, suppressing the direct Urca process and slowing thermal cooling.

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Axisymmetric Cooling of Neutron Stars with Strong Magnetic Fields astro-ph.HE · 2025-06-11 · conditional · none · ref 5
Strong poloidal magnetic fields deform neutron stars and reduce central density, suppressing the direct Urca process and slowing thermal cooling.