Thermodynamics of the statistical model of atoms in a very strong magnetic field: An approach to the properties of condensed matter in the outer crust of pulsars-Reference-Cited by-同舟云学术

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Thermodynamics of the statistical model of atoms in a very strong magnetic field: An approach to the properties of condensed matter in the outer crust of pulsars

Published:1978-09-15 Issue:6 Volume:18 Page:1820-1828
ISSN:0556-2821
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Constantinescu D. H.,Moruzzi G.

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.18.1820/fulltext

Reference30 articles.

1. EQUATION OF STATE FOR CONDENSED MATTER IN A VERY STRONG MAGNETIC FIELD

2. Condensed matter in a very strong magnetic field, at high pressure and zero temperature

3. Statistical Model of Atoms in Intense Magnetic Fields

4. Thomas-Fermi and Thomas-Fermi-Dirac calculations for atoms in a very strong magnetic field

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2. Unified treatment for accurate and fast evaluation of the Fermi–Dirac functions;Chinese Physics B;2010-05

3. Matter in strong magnetic fields;Reviews of Modern Physics;2001-08-29

4. Partially ionized hydrogen plasma in strong magnetic fields;Physical Review E;1999-08-01

5. Thomas‐Fermi Calculations of Atoms and Matter in Magnetic Neutron Stars. II. Finite Temperature Effects;The Astrophysical Journal;1998-08

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