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Massive compact dwarf stars and C-field

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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.

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Singh, L.P., Sahu, P.K. Massive compact dwarf stars and C-field. J Astrophys Astron 18, 15–21 (1997). https://doi.org/10.1007/BF02714850

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  • DOI: https://doi.org/10.1007/BF02714850

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