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Cosmological Constant, Conical Defect and Classical Tests of General Relativity

Wilson H. C. Freire·V. B. Bezerra·J. A. S. Lima
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Abstract

We investigate the perihelion shift of the planetary motion and the bending of starlight in the Schwarzschild field modified by the presence of a $Λ$-term plus a conical defect. This analysis generalizes an earlier result obtained by Islam (Phys. Lett. A 97, 239, 1983) to the case of a pure cosmological constant. By using the experimental data we obtain that the parameter $ε$ characterizing the conical defect is less than $10^{-9}$ and $10^{-7}$, respectively, on the length scales associated with such phenomena. In particular, if the defect is generated by a cosmic string, these values correspond to limits on the linear mass densities of $10^{19}g/cm$ and $10^{21}g/cm$, respectively.

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Wilson H. C. Freire, V. B. Bezerra, J. A. S. Lima. 2002-01-11. Cosmological Constant, Conical Defect and Classical Tests of General Relativity. https://doi.org/10.1023/a%3A1012013809911

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