Abstract
After discussing the Coulomb properties of neutron star envelopes in Chapter 2, we will mainly focus on the nuclear part of the problem. Following a widespread convention we will often call an entire neutron star envelope as a crust (see a discussion on this point in the introductory part of Chapter 2).
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(2007). Structure and Equation of State of Neutron Star Crusts. In: Haensel, P., Potekhin, A.Y., Yakovlev, D.G. (eds) Neutron Stars 1. Astrophysics and Space Science Library, vol 326. Springer, New York, NY. https://doi.org/10.1007/978-0-387-47301-7_3
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DOI: https://doi.org/10.1007/978-0-387-47301-7_3
Publisher Name: Springer, New York, NY
Print ISBN: 978-0-387-33543-8
Online ISBN: 978-0-387-47301-7
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