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# b_a - 1.1 One may use any reasonable equation to obtain the...

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1.1) One may use any reasonable equation to obtain the dimension of the questioned quantities. I) The Planck relation is 1 2 1 ] ][ [ ] [ ] [ ] ][ [ - - = = = = T ML E h E h E h ν ν ν (0.2) II) 1 ] [ - = LT c (0.2) III) 2 3 1 2 2 2 ] ][ ][ [ ] [ - - - = = = T L M m r F G r m m G F (0.2) IV) 1 2 2 1 ] [ ] [ ] [ - - - = = = K T ML E K K E B B θ θ (0.2) 1.2) Using the Stefan-Boltzmann's law, 4 θ σ = Area Power , or any equivalent relation, one obtains: (0.3) . ] [ ] [ ] [ 4 3 1 2 4 - - - - = = K MT T L E K σ σ (0.2) 1.3) The Stefan-Boltzmann's constant, up to a numerical coefficient, equals , δ γ β α σ B k G c h = where δ γ β α , , , can be determined by dimensional analysis. Indeed, , ] [ ] [ ] [ ] [ ] [ δ γ β α σ B k G c h = where e.g. . ] [ 4 3 - - = K MT σ ( ) ( ) ( ) ( ) , 2 2 2 3 2 1 2 2 2 3 1 1 1 2 4 3 δ δ γ β α δ γ β α δ γ α δ γ β α - - - - - + + + + - - - - - - - - - = = K T L M K T ML T L M LT T ML K MT (0.2) The above equality is satisfied if, - = - - = - - - - = + + + = + - , 4 , 3 2 2 , 0 2 3 2 , 1 δ δ γ β α δ γ β α δ γ α (Each one (0.1)) = = - = - = . 4 , 0 , 2 , 3 δ γ β α (Each one (0.1)) . 3 2 4 h c k B = σ 2.1) Since A , the area of the event horizon, is to be calculated in terms of m from a classical theory of relativistic gravity, e.g. the General Relativity, it is a combination of c

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