A class of solutions for anisotropic stars admitting conformal motion

Abstract

We provide a new class of interior solutions for anisotropic stars admitting conformal motion. The Einstein's field equations in this construction are solved for specific choices of the density/mass functions. We analyze the behavior of the model parameters like radial and transverse pressures, density and surface tension.

9 pages, 16 figures, accepted for publication in "Astrophysics and Space Science"

References in corpus (7)

• Quark stars admitting a one-parameter group of conformal motions
• A class of relativistic stars with a linear equation of state
• Anisotropic Stars: Exact Solutions and Stability
• On the role of pressure anisotropy for relativistic stars admitting conformal motion
• The fastest rotating pulsar: A strange star?
• Magnetized Quark and Strange Quark Matter in the Spherical Symmetric Space-Time Admitting Conformal Motion
• On surface tension for compact stars

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• A Comprehensive Study of Massive Compact Star Admitting Conformal Motion Under Bardeen Geometry
• Relativistic compact stars in Tolman spacetime via an anisotropic approach
• Anisotropic Tolman V Solutions by Decoupling Approach in $f(R,T^2)$ Gravity