Effects of vacuum structure on neutron star
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Data
2001-01-01
Autores
Panda, P. K.
Sahu, R.
Mishra, S.
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World Scientific Publ Co Pte Ltd
Resumo
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 star.
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Como citar
International Workshop on Hadron Physics 2000. Singapore: World Scientific Publ Co Pte Ltd, p. 405-408, 2001.