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Magnetic fields in neutron stars: A theoretical perspective

Andreas Reisenegger·Joaquin Prieto·Rafael Benguria·Dong Lai·Pablo Araya
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Abstract

We present our view of the main physical ingredients determining the evolution of neutron star magnetic fields. This includes the basic properties of neutron star matter, possible scenarios for the origin of the magnetic field, constraints and mechanisms for its evolution, and a discussion of our recent work on the Hall drift.

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Andreas Reisenegger, Joaquin Prieto, Rafael Benguria, Dong Lai, Pablo Araya. 2005-03-02. Magnetic fields in neutron stars: A theoretical perspective. https://doi.org/10.1063/1.2077190

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