Massive compact dwarf stars and C-field

Astronomy and Astrophysics – Astrophysics

Scientific paper

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10 pages (LaTex), one figure available upon request

Scientific paper

10.1007/BF02714850

The effect of C-field in high density matter has been studied. We find that
the negative energy and negative pressure of the C-field helps in formation of
massive compact stable neutron stars of mass $\sim$ 0.5 solar mass which is in
the range of 0.01 to 1.0 solar mass of recently observed dwarf stars.

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