Abstract
We derive the metric for a Schwarzschild black hole with global monopole charge by relaxing asymptotic flatness of the Schwarzschild field. We then study the effect of global monopole charge on particle orbits and the Hawking radiation. It turns out that existence, boundedness and stability of circular orbits scale up by (1−8πη 2)−1, and the perihelion shift and the light bending by (1−8πη 2)−3/2, while the Hawking temperature scales down by (1−8πη 2)2 the Schwarzschild values. Hereη is the global charge.
Similar content being viewed by others
References
M Barriola and A Vilenkin,Phys. Rev. Lett. 63, 341 (1989)
N Dadhich (1995) GR-14 abstracts, A. 98
A Banerjee, S Chatterjee and A A Sen,Class. Quantum Gravit. 13, 3141 (1996)
N Dadhich,On the Schwarzschild field, gr-qc/9704068
G W Gibbons, M E Ortiz, F Ruiz and T M Samols,Nucl. Phys. B385, 127 (1992)
D Harari and C Lousto,Phys. Rev. D42, 2626 (1990)
S Weinberg,Gravitation and Cosmology (John Wiley and Sons, New York, 1972) pp. 189–90, 194–96
K Lee, V P Nair and E J Weinberg,Gen. Relativ. Gravit. 24, 1203 (1992)
J J Bisognano and E H Wichmann,J. Math. Phys. 16, 985 (1975)
Jiliang Jing, Hongwei Yu and Yongjiu Wang,Phys. Lett. A178, 59 (1993)
B Jensen,Nucl. Phys. B453, 413 (1995)
N Dadhich, A duality relation: global monopole and texture, gr-qc/9712021
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Dadhich, N., Narayan, K. & Yajnik, U.A. Schwarzschild black hole with global monopole charge. Pramana - J Phys 50, 307–314 (1998). https://doi.org/10.1007/BF02845552
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF02845552