Physics
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cqgra...4.1691d&link_type=abstract
Classical and Quantum Gravity (ISSN 0264-9381), vol. 4, Nov. 1, 1987, p. 1691-1696. Research supported by the Council of Scienti
Physics
3
Einstein Equations, Neutron Stars, Relativistic Theory, Stellar Models, Field Theory (Physics), Red Shift, Space-Time Functions
Scientific paper
A new analytical solution is obtained for stellar models by solving Einstein's field equations for the spherically symmetric and static cases. The density variation is found to be smooth and positive under all conditions. The reduction of the equations to a form which is easier to solve is demonstrated. The solution is applicable to neutron stars with a density of 2 x 10 to the 14th g/cu cm or less.
Duorah Hira Lal
Ray Rajarshi
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