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Neutrostriction in Neutron stars

V. K. Ignatovich
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Abstract

It is demonstrated that not only gravity, but also neutrostriction forces due to optical potential created by coherent elastic neutron-neutron scattering can hold a neutron star together. The latter forces can be stronger than gravitational ones. The effect of these forces on mass, radius and structure of the neutron star is estimated.

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V. K. Ignatovich. 2006-06-29. Neutrostriction in Neutron stars. https://arxiv.org/abs/astro-ph/0311471

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