Black holes and quantum mechanics
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G. 't Hooft
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Article
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2010
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Elsevier Science
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English
โ 439 KB
+ r 2 dฮฉ 2 , (1) where spherical coordinates t, r, ฮธ, ฯ were chosen, dฮฉ 2 def = dฮธ 2 + sin 2 ฮธ dฯ 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