Effects of vacuum structure on neutron stars
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Data
2000-11-01
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Panda, P. K. [UNESP]
Sahu, R.
Mishra, S.
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We study the equation of state for neutron matter using the Walecka model including quantum corrections for baryons and sigma mesons through a realignment of the vacuum. We next use this equation of state to calculate the radius, mass, and other properties of rotating neutron stars.
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Physical Review C - Nuclear Physics, v. 62, n. 5, p. 558021-558028, 2000.