Effects of vacuum structure on neutron stars
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Abstract
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. © 2000 The American Physical Society.
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English
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Physical Review C - Nuclear Physics, v. 62, n. 5, p. 8-, 2000.
