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Quantum corrections and extremal black holes

✍ Scribed by G Alejandro; F.D Mazzitelli; C Núñez


Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
560 KB
Volume
355
Category
Article
ISSN
0370-2693

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+ r 2 dΩ 2 , (1) where spherical coordinates t, r, θ, ϕ were chosen, dΩ 2 def = dθ 2 + sin 2 θ dϕ 2 , and the radial coordinate r was chosen such that the angular component in this expression coincides with that of empty space-time. Furthermore, we absorbed Newton's constant G N into the definition