首页|Physical Implications of Pure Lovelock Geometry on Stellar Structure
Physical Implications of Pure Lovelock Geometry on Stellar Structure
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NSTL
Wiley
Abstract An exact anisotropic star model with a linear barotropic equation?of state and with Finch‐Skea potential is constructed within the framework of pure Lovelock gravity. A comparison with the corresponding Einstein model in a suitable limit is easily deduced. Evidently higher curvature effects induced by the Lovelock contributions generate lower densities, pressures, surface tensions, and anisotropy factors when compared to its Einstein counterpart. The maximum moment of inertia is attained for the Einstein case and hence it may be inferred that Lovelock effects soften the equation?of state. The model satisfies various stability?tests.
NSTL
Wiley
