𝔖 Bobbio Scriptorium
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Black holes and quantum mechanics

✍ Scribed by G. 't Hooft


Publisher
Elsevier Science
Year
2010
Tongue
English
Weight
439 KB
Volume
203-204
Category
Article
ISSN
0920-5632

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✦ Synopsis


  • 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 of the mass: M def = G N m BH , or rather, units were chosen such that G N = 1 . In a slightly different notation, this solution to Einstein's equations was first written down by K. Schwarzschild [1].


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