Issue |
A&A
Volume 645, January 2021
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202038347e | |
Published online | 08 January 2021 |
Inner crust of a neutron star at the point of crystallization in a multicomponent approach (Corrigendum)
1
LPC (CNRS/ENSICAEN/Université de Caen Normandie), UMR6534, 14050 Caen Cédex, France
e-mail: carreau@lpccaen.in2p3.fr, gulminelli@lpccaen.in2p3.fr
2
Grand Accélérateur National d’Ions Lourds (GANIL), CEA/DRF - CNRS/IN2P3, Boulevard Henri Becquerel, 14076 Caen, France
Key words: stars: neutron / dense matter / plasmas / errata, addenda
The original article contains two misprints, which are corrected below. These misprints do not affect any of the published numerical results, the calculations having been performed using the correct expressions.
Section 2.1.
In the first paragraph, it is the proton chemical potential μp that never exceeds −20 MeV in the density and temperature domain studied in the paper, and not the proton fugacity zp = exp[(μp − mpc2)/(kBT)], where mp is the proton mass, c the speed of light, and kB the Boltzmann constant.
Section 2.3.
Deriving the expression of the nuclear finite-size correction from the Gauss theorem for a spherical cluster of charge Z, mass A, asymmetry I = 1 − 2 Z/A, and average density n0 in a spherical Wigner-Seitz cell characterized by proton density np, the factor 3/10 is missing with respect to Eq. (32):
where r0 = (4πn0/3)−1/3 and e is the elementary charge.
© T. Carreau et al. 2021
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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