An analytical stellar model

Physics

Scientific paper

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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.

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