Massive compact dwarf stars and C-field
  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. 
L.P. Singh (Utkal Unv.) and P.K. Sahu (PRL, Ahmedabad)