| Abstract: | We solve the Einstein equations for the case of a static, spherically symmetric distribution of a perfect fluid. We propose a method yielding a broad class of exact solutions. We investigate the question of how to obtaina fortiori regular and equilibrium solutions. We find a new exact solution in a rather simple form and show that it describes a neutron star with mass limit of 0.33 solar masses.The work was done with the financial support of the Krasnoyarsk Regional Science Foundation, grant D(1F0019).Krasnoyarsk State University. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 9, pp. 44–48, September, 1994. |
