Massive compact dwarf stars and C-field
arXiv:astro-ph/9601075 · doi:10.1007/BF02714850
Abstract
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.
10 pages (LaTex), one figure available upon request