Black holes and quantum mechanics
β
G. 't Hooft
π
Article
π
2010
π
Elsevier Science
π
English
β 439 KB
+ r 2 dΞ© 2 , (1) where spherical coordinates t, r, ΞΈ, Ο were chosen, dΞ© 2 def = dΞΈ 2 + sin 2 ΞΈ dΟ 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