Effect of the Curved Spacetime on the Electrostatic PotentialEnergy Distribution of Strange Stars
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Abstract
The effect of the strong gravitational field of the strange core of a strange star on its surface electrostatic potential energy distribution is discussed. We present the general-relativistic hydrodynamics equations of fluids in the presence of the electric fields and investigate the surface electrostatic potential distribution of the strange core of a strange star in hydrostatic equilibrium to correct Alcock and coworker's result Astrophys. J.310(1986) 261. Also, we discuss the temperature distribution of the bare strange star surface and give the related formulae, which may be useful if we are concerned further about the physical processes near the quark matter surfaces of strange stars.
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CHEN Ci-Xing, ZHANG Jia-Lu. Effect of the Curved Spacetime on the Electrostatic PotentialEnergy Distribution of Strange Stars[J]. Chin. Phys. Lett., 2001, 18(1): 145-147.
CHEN Ci-Xing, ZHANG Jia-Lu. Effect of the Curved Spacetime on the Electrostatic PotentialEnergy Distribution of Strange Stars[J]. Chin. Phys. Lett., 2001, 18(1): 145-147.
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CHEN Ci-Xing, ZHANG Jia-Lu. Effect of the Curved Spacetime on the Electrostatic PotentialEnergy Distribution of Strange Stars[J]. Chin. Phys. Lett., 2001, 18(1): 145-147.
CHEN Ci-Xing, ZHANG Jia-Lu. Effect of the Curved Spacetime on the Electrostatic PotentialEnergy Distribution of Strange Stars[J]. Chin. Phys. Lett., 2001, 18(1): 145-147.
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