Finite volume of baryons and the mass limit for neutron stars

Details Finite volume of baryons and the mass limit for neutron stars Finite volume of baryons and the mass limit for neutron stars

1992-10-26

arxiv.org/abs/nucl-th/9210019v1

J.Phys. G18 (1992) 2051-2060

Physics

Nuclear Physics

Nuclear Theory

15 pages, to be published in J.Phys.G

Scientific paper

10.1088/0954-3899/18/12/020

We confirmed the following idea by numerical calculation: The extended structure of baryons may make the nuclear equation of state stiffer at higher density while keeping the compression modulus for normal nuclear matter around its empirical value $K=240MeV$.The model built in this wayy fits all empirical data for normal nuclear matter and gives the mass limit of neutron stars compatible with the observation.

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