Composition and equation of state of the outer shell of a neutron star under a strong magnetic field

Details Composition and equation of state of the outer shell of a neutron star under a strong magnetic field Composition and equation of state of the outer shell of a neutron star under a strong magnetic field

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cha%26a..17..187d&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 17, Issue 2, p. 187-194.

Astronomy and Astrophysics

Astrophysics

Neutron Star-Magnetic Field-Equation Of State

Scientific paper

In this paper we calculate and discuss the composition and equation of state of the outer shell of a neutron star composed of cold catalyzed matter. We consider the contributions by the lattice energy and exchange energy of a uniform electron gas under a strong magnetic field. Our conclusions are: (1) a strong magnetic field softens the equation of state for low density regions; (2) it has almost no effect in high density regions; (3) the nuclear mass formula has a more marked effect on the composition of the outer shell.

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