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 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