Quark stars admitting a one-parameter group of conformal motions
M. K. Mak, T. Harko
TL;DR
This paper presents an exact analytical model of a charged strange quark star with conformal symmetry, providing specific predictions for its radius and mass, contributing to the understanding of compact stellar objects.
Contribution
It introduces a new exact solution for a charged quark star under conformal symmetry, expanding the theoretical models of compact stars.
Findings
Star radius: 9.46 km
Star mass: 2.86 solar masses
Unique static charged configuration
Abstract
An exact analytical solution describing the interior of a charged strange quark star is found under the assumption of spherical symmetry and the existence of a one-parameter group of conformal motions. The solution describes a unique static charged configuration of quark matter with radius km and total mass .
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