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Magnetic Fields and the Crystallization of White Dwarfs

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conference contribution
posted on 2025-07-31, 18:26 authored by J Isern, E Garcia-Berro, B Kuelebi, P Loren-Aguilar
The evolution of white dwarfs can be described as a cooling process. When the temperature is low enough, the interior experiences a phase transition and crystallizes. Crystallization introduces two new sources of energy, latent heat and chemical sedimentation, and induces the formation of a convective mantle around the solid core. This structure, which is analogous to that of the Earth, could induce the formation of a magnetic field via dynamo mechanism. In this work we discuss the viability of such mechanism, and its use as a diagnostic tool of crystallization.

Funding

2014SGR0038

2014SGR1458

AYA2014-59084-P

ESP2013-47637-P

European Union

Generalitat de Catalunya

MINECO

History

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Rights

© 2017 Astronomical Society of the Pacific

Notes

This is the final version. Available from Astronomical Society of the Pacific via the link in this record EuroWD16: 20th European White Dwarf Workshop, 25-29 July 2016, Warwick, UK

Journal

Astronomical Society of the Pacific Conference Series

Publisher

Astronomical Society of the Pacific

Version

  • Version of Record

Language

en

FCD date

2019-03-27T13:30:09Z

FOA date

2019-03-27T13:35:09Z

Citation

Vol. 509, pp. 409 - 414

Department

  • Physics and Astronomy

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