From Wikipedia, the free encyclopedia
If anyone else takes a look here, note that these are not necessarily correct; there seems to be something wrong with my derivations, which is why I'm poking around here.
R
c
2
=
2
G
M
R
=
2
G
M
c
2
M
=
c
2
R
2
G
{\displaystyle Rc^{2}=2GM\;R={2G\,M \over c^{2}}\;M={c^{2}R \over 2G}}
E
=
M
c
2
=
c
4
R
2
G
{\displaystyle E=M\,c^{2}={c^{4}\,R \over 2G}}
S
=
k
A
4
ℓ
P
2
=
k
c
3
A
4
ℏ
G
=
π
k
c
3
A
2
h
G
{\displaystyle S={k\,A \over 4\ell _{P}^{2}}={kc^{3}\,A \over 4\hbar G}={\pi kc^{3}\,A \over 2hG}}
T
=
E
S
{\displaystyle T={E \over S}}
- no guarantee over this, or that the
E
{\displaystyle E}
here is the one equal to
M
c
2
{\displaystyle Mc^{2}}
.
σ
=
2
π
5
k
4
15
c
2
h
3
=
2
π
5
k
4
15
c
2
2
3
π
3
ℏ
3
=
π
2
k
4
60
c
2
ℏ
3
{\displaystyle \sigma ={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}={2\pi ^{5}k^{4} \over 15c^{2}2^{3}\pi ^{3}\hbar ^{3}}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}}
q
=
e
b
A
{\displaystyle q=e_{b}A\,}
A
=
4
π
R
2
=
4
π
(
2
G
M
c
2
)
2
=
4
π
4
G
2
M
2
c
4
=
16
π
G
2
M
2
c
4
{\displaystyle A=4\pi \,R^{2}=4\pi \left({2G\,M \over c^{2}}\right)^{2}=4\pi {4G^{2}\,M^{2} \over c^{4}}={16\pi G^{2}\,M^{2} \over c^{4}}}
- but see Weisstein's section below and New A section
S
=
π
k
c
3
R
2
ℏ
G
=
2
π
2
k
c
3
R
2
h
G
{\displaystyle S={\pi kc^{3}\,R^{2} \over \hbar G}={2\pi ^{2}kc^{3}\,R^{2} \over hG}}
S
=
4
π
k
G
M
2
ℏ
c
=
8
π
2
k
G
M
2
h
c
{\displaystyle S={4\pi kG\,M^{2} \over \hbar c}={8\pi ^{2}kG\,M^{2} \over hc}}
T
=
E
S
=
M
c
2
ℏ
c
4
π
k
G
M
2
=
c
4
R
2
G
ℏ
G
π
k
c
3
R
2
{\displaystyle T={E \over S}=M\,c^{2}{\hbar c \over 4\pi kG\,M^{2}}={c^{4}\,R \over 2G}{\hbar G \over \pi kc^{3}\,R^{2}}}
T
=
h
c
3
8
π
2
k
G
M
=
ℏ
c
3
4
π
k
G
M
{\displaystyle T={hc^{3} \over 8\pi ^{2}kG\,M}={\hbar c^{3} \over 4\pi kG\,M}}
T
=
h
c
4
π
2
k
R
=
ℏ
c
2
π
k
R
{\displaystyle T={hc \over 4\pi ^{2}k\,R}={\hbar c \over 2\pi k\,R}}
e
b
=
σ
T
4
=
π
2
k
4
60
c
2
ℏ
3
(
ℏ
c
3
4
π
k
G
M
)
4
=
2
π
5
k
4
15
c
2
h
3
(
h
c
3
8
π
2
k
G
M
)
4
{\displaystyle e_{b}=\sigma \,T^{4}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}\left({\hbar c^{3} \over 4\pi kG\,M}\right)^{4}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}\left({hc^{3} \over 8\pi ^{2}kG\,M}\right)^{4}}
e
b
=
π
2
k
4
60
c
2
ℏ
3
ℏ
4
c
12
256
π
4
k
4
G
4
M
4
=
2
π
5
k
4
15
c
2
h
3
h
4
c
12
4096
π
8
k
4
G
4
M
4
{\displaystyle e_{b}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}{\frac {\hbar ^{4}c^{12}}{256\pi ^{4}k^{4}G^{4}\,M^{4}}}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}{\frac {h^{4}c^{12}}{4096\pi ^{8}k^{4}G^{4}\,M^{4}}}}
e
b
=
ℏ
c
10
15
,
360
π
2
G
4
M
4
=
h
c
10
30
,
720
π
3
G
4
M
4
{\displaystyle e_{b}={\hbar c^{10} \over 15,360\pi ^{2}G^{4}\,M^{4}}={hc^{10} \over 30,720\pi ^{3}G^{4}\,M^{4}}}
q
=
σ
T
4
A
=
σ
h
4
c
4
64
π
7
k
4
R
2
=
h
c
2
480
π
2
R
2
{\displaystyle q=\sigma \,T^{4}A={\sigma h^{4}c^{4} \over 64\pi ^{7}k^{4}\,R^{2}}={hc^{2} \over 480\pi ^{2}\,R^{2}}}
q
=
π
2
k
4
60
c
2
ℏ
3
(
ℏ
c
3
4
π
k
G
M
)
4
16
π
G
2
M
2
c
4
{\displaystyle q={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}\left({\hbar c^{3} \over 4\pi kG\,M}\right)^{4}{16\pi G^{2}\,M^{2} \over c^{4}}}
q
=
π
2
k
4
60
c
2
ℏ
3
ℏ
4
c
12
256
π
4
k
4
G
4
M
4
16
π
G
2
M
2
c
4
{\displaystyle q={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}{\frac {\hbar ^{4}c^{12}}{256\pi ^{4}k^{4}G^{4}\,M^{4}}}{16\pi G^{2}\,M^{2} \over c^{4}}}
q
=
c
6
ℏ
960
π
G
2
M
2
{\displaystyle q={\frac {c^{6}\hbar }{960\pi G^{2}\,M^{2}}}}
R
c
2
=
2
G
M
R
=
2
G
M
c
2
M
=
c
2
R
2
G
{\displaystyle Rc^{2}=2GM\;R={2G\,M \over c^{2}}\;M={c^{2}R \over 2G}}
E
=
M
c
2
=
c
4
R
2
G
{\displaystyle E=M\,c^{2}={c^{4}\,R \over 2G}}
S
=
k
A
4
ℓ
P
2
=
k
c
3
A
4
ℏ
G
=
π
k
c
3
A
2
h
G
{\displaystyle S={k\,A \over 4\ell _{P}^{2}}={kc^{3}\,A \over 4\hbar G}={\pi kc^{3}\,A \over 2hG}}
T
=
E
S
{\displaystyle T={E \over S}}
- no guarantee over this, or that the
E
{\displaystyle E}
here is the one equal to
M
c
2
{\displaystyle Mc^{2}}
.
σ
=
2
π
5
k
4
15
c
2
h
3
=
2
π
5
k
4
15
c
2
2
3
π
3
ℏ
3
=
π
2
k
4
60
c
2
ℏ
3
{\displaystyle \sigma ={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}={2\pi ^{5}k^{4} \over 15c^{2}2^{3}\pi ^{3}\hbar ^{3}}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}}
q
=
e
b
A
{\displaystyle q=e_{b}A\,}
A
=
8
π
G
2
M
2
c
4
=
8
π
G
2
c
4
(
c
2
R
2
G
)
2
=
8
π
G
2
c
4
c
4
R
2
4
G
2
{\displaystyle A={8\pi G^{2}\,M^{2} \over c^{4}}={8\pi G^{2} \over c^{4}}\left({c^{2}\,R \over 2G}\right)^{2}={8\pi G^{2} \over c^{4}}{c^{4}\,R^{2} \over 4G^{2}}}
- see Weisstein's section below
A
=
2
π
R
2
{\displaystyle A={2\pi R^{2}}\,}
S
=
k
c
3
4
ℏ
G
2
π
R
2
=
π
k
c
3
2
h
G
2
π
R
2
=
k
c
3
4
ℏ
G
8
π
G
2
M
2
c
4
=
π
k
c
3
2
h
G
8
π
G
2
M
2
c
4
{\displaystyle S={kc^{3} \over 4\hbar G}{2\pi R^{2}}={\pi kc^{3} \over 2hG}{2\pi R^{2}}={kc^{3} \over 4\hbar G}{8\pi G^{2}\,M^{2} \over c^{4}}={\pi kc^{3} \over 2hG}{8\pi G^{2}\,M^{2} \over c^{4}}}
S
=
π
k
c
3
R
2
2
ℏ
G
=
π
2
k
c
3
R
2
h
G
=
2
π
k
G
M
2
ℏ
c
=
4
π
2
k
G
M
2
h
c
{\displaystyle S={\pi kc^{3}\,R^{2} \over 2\hbar G}={\pi ^{2}kc^{3}\,R^{2} \over hG}={2\pi kG\,M^{2} \over \hbar c}={4\pi ^{2}kG\,M^{2} \over hc}}
T
=
E
S
{\displaystyle T={E \over S}}
T
=
c
4
R
2
G
2
ℏ
G
π
k
c
3
R
2
=
c
4
R
2
G
h
G
π
2
k
c
3
R
2
=
M
c
2
ℏ
c
2
π
k
G
M
2
=
M
c
2
h
c
4
π
2
k
G
M
2
{\displaystyle T={c^{4}\,R \over 2G}{2\hbar G \over \pi kc^{3}\,R^{2}}={c^{4}\,R \over 2G}{hG \over \pi ^{2}kc^{3}\,R^{2}}=M\,c^{2}{\hbar c \over 2\pi kG\,M^{2}}=M\,c^{2}{hc \over 4\pi ^{2}kG\,M^{2}}}
T
=
ℏ
c
π
k
R
=
h
c
2
π
2
k
R
=
ℏ
c
3
2
π
k
G
M
=
h
c
3
4
π
2
k
G
M
{\displaystyle T={\hbar c \over \pi k\,R}={hc \over 2\pi ^{2}k\,R}={\hbar c^{3} \over 2\pi kG\,M}={hc^{3} \over 4\pi ^{2}kG\,M}}
Damn, the different area formula is making things even worse?!?
Maybe it's the definition of
E
{\displaystyle E}
that's not what I'd expect? It needn't be the mass-energy equivalence of the entire mass of the black hole.
T
=
E
S
=
E
2
π
k
G
M
2
ℏ
c
=
E
ℏ
c
2
π
k
G
M
2
=
ℏ
c
3
8
π
k
G
M
{\displaystyle T={E \over S}={E \over {2\pi kG\,M^{2} \over \hbar c}}={E\hbar c \over 2\pi kG\,M^{2}}={\hbar c^{3} \over 8\pi kG\,M}}
E
=
ℏ
c
3
8
π
k
G
M
2
π
k
G
M
2
ℏ
c
=
c
2
M
4
{\displaystyle E={\hbar c^{3} \over 8\pi kG\,M}{2\pi kG\,M^{2} \over \hbar c}={c^{2}\,M \over 4}}
- Why this apparent equivalence? I have no idea. It could also be that
T
=
E
4
S
{\displaystyle T={E \over 4S}}
.
Let's try a comparison with the gravitational binding energy formula. I doubt it has any relevance, but I'll see what it generates.
U
=
3
G
M
2
5
r
=
3
G
M
2
5
2
G
M
c
2
=
3
G
c
2
M
2
10
G
M
=
3
c
2
M
10
{\displaystyle U={3G\,M^{2} \over 5\,r}={3G\,M^{2} \over 5{2G\,M \over c^{2}}}={3Gc^{2}\,M^{2} \over 10G\,M}={3c^{2}\,M \over 10}}
- Well, it's in the ballpark, and I'm pretty sure that binding energy formula doesn't allow for relativistic effects. But I still don't think it has anything to do with it.
Continued: emission [ edit ]
e
b
=
σ
T
4
=
2
π
5
k
4
15
c
2
h
3
(
h
c
3
4
π
2
k
G
M
)
4
=
π
2
k
4
60
c
2
ℏ
3
(
ℏ
c
3
2
π
k
G
M
)
4
{\displaystyle e_{b}=\sigma \,T^{4}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}\left({hc^{3} \over 4\pi ^{2}kG\,M}\right)^{4}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}\left({\hbar c^{3} \over 2\pi kG\,M}\right)^{4}}
e
b
=
2
π
5
k
4
15
c
2
h
3
h
4
c
12
256
π
8
k
4
G
4
M
4
=
π
2
k
4
60
c
2
ℏ
3
ℏ
4
c
12
16
π
4
k
4
G
4
M
4
{\displaystyle e_{b}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}{\frac {h^{4}c^{12}}{256\pi ^{8}k^{4}G^{4}\,M^{4}}}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}{\frac {\hbar ^{4}c^{12}}{16\pi ^{4}k^{4}G^{4}\,M^{4}}}}
e
b
=
h
c
10
1920
π
3
G
4
M
4
=
ℏ
c
10
960
π
2
G
4
M
4
{\displaystyle e_{b}={hc^{10} \over 1920\pi ^{3}G^{4}\,M^{4}}={\hbar c^{10} \over 960\pi ^{2}G^{4}\,M^{4}}}
q
=
h
c
10
1920
π
3
G
4
M
4
A
=
ℏ
c
10
960
π
2
G
4
M
4
A
{\displaystyle q={hc^{10} \over 1920\pi ^{3}G^{4}\,M^{4}}A={\hbar c^{10} \over 960\pi ^{2}G^{4}\,M^{4}}A}
q
=
h
c
10
1920
π
3
G
4
M
4
8
π
G
2
M
2
c
4
=
ℏ
c
10
960
π
2
G
4
M
4
8
π
G
2
M
2
c
4
{\displaystyle q={hc^{10} \over 1920\pi ^{3}G^{4}\,M^{4}}{8\pi G^{2}\,M^{2} \over c^{4}}={\hbar c^{10} \over 960\pi ^{2}G^{4}\,M^{4}}{8\pi G^{2}\,M^{2} \over c^{4}}}
q
=
h
c
6
240
π
2
G
2
M
2
=
ℏ
c
6
120
π
G
2
M
2
{\displaystyle q={hc^{6} \over 240\pi ^{2}G^{2}\,M^{2}}={\hbar c^{6} \over 120\pi G^{2}\,M^{2}}}
ℏ
c
3
8
π
k
G
M
=
h
c
3
16
π
2
k
G
M
{\displaystyle {\hbar c^{3} \over 8\pi kG\,M}={hc^{3} \over 16\pi ^{2}kG\,M}}
e
b
=
σ
T
4
=
2
π
5
k
4
15
c
2
h
3
(
h
c
3
16
π
2
k
G
M
)
4
=
π
2
k
4
60
c
2
ℏ
3
(
ℏ
c
3
8
π
k
G
M
)
4
{\displaystyle e_{b}=\sigma \,T^{4}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}\left({hc^{3} \over 16\pi ^{2}kG\,M}\right)^{4}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}\left({\hbar c^{3} \over 8\pi kG\,M}\right)^{4}}
e
b
=
2
π
5
k
4
15
c
2
h
3
h
4
c
12
65
,
536
π
8
k
4
G
4
M
4
=
π
2
k
4
60
c
2
ℏ
3
ℏ
4
c
12
4
,
096
π
4
k
4
G
4
M
4
{\displaystyle e_{b}={2\pi ^{5}k^{4} \over 15c^{2}h^{3}}{h^{4}c^{12} \over 65,536\pi ^{8}k^{4}G^{4}\,M^{4}}={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}{\hbar ^{4}c^{12} \over 4,096\pi ^{4}k^{4}G^{4}\,M^{4}}}
e
b
=
h
c
10
491
,
520
π
3
G
4
M
4
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
{\displaystyle e_{b}={hc^{10} \over 491,520\pi ^{3}G^{4}\,M^{4}}={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}}
P
=
h
c
10
491
,
520
π
3
G
4
M
4
A
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
A
{\displaystyle P={hc^{10} \over 491,520\pi ^{3}G^{4}\,M^{4}}A={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}A}
P
=
h
c
10
491
,
520
π
3
G
4
M
4
8
π
G
2
M
2
c
4
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
8
π
G
2
M
2
c
4
{\displaystyle P={hc^{10} \over 491,520\pi ^{3}G^{4}\,M^{4}}{8\pi G^{2}\,M^{2} \over c^{4}}={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}{8\pi G^{2}\,M^{2} \over c^{4}}}
P
=
h
c
6
61
,
440
π
2
G
2
M
2
=
ℏ
c
6
30
,
720
π
G
2
M
2
{\displaystyle P={hc^{6} \over 61,440\pi ^{2}G^{2}\,M^{2}}={\hbar c^{6} \over 30,720\pi G^{2}\,M^{2}}}
T
H
=
κ
2
π
{\displaystyle T_{H}={\kappa \over 2\pi }}
(natural units )
T
=
ℏ
c
3
8
π
G
M
k
{\displaystyle T={\hbar \,c^{3} \over 8\pi GMk}}
P
=
ℏ
c
6
15360
π
G
2
M
2
{\displaystyle P={\hbar \,c^{6} \over 15360\,\pi \,G^{2}M^{2}}}
t
ev
=
5120
π
G
2
M
0
3
ℏ
c
4
{\displaystyle t_{\operatorname {ev} }={5120\,\pi \,G^{2}M_{0}^{\,3} \over \hbar \,c^{4}}}
examples in article [ edit ]
T
B
H
s
o
l
=
60
n
K
=
6
×
10
−
8
K
{\displaystyle T_{BH_{sol}}=60\mathrm {nK} =6\times 10^{-8}\mathrm {K} }
T
B
H
(
4.5
×
10
22
k
g
)
=
2.7
K
{\displaystyle T_{BH}(4.5\times 10^{22}\mathrm {kg} )=2.7\mathrm {K} }
P
s
o
l
=
10
−
28
W
{\displaystyle P_{sol}=10^{-28}\mathrm {W} \,}
t
e
v
s
o
l
=
10
67
y
e
a
r
=
3
×
10
74
s
{\displaystyle t_{\mathrm {ev} _{sol}}=10^{67}\mathrm {year} =3\times 10^{74}\mathrm {s} }
t
e
v
(
10
11
k
g
)
=
3
×
10
9
y
e
a
r
=
9
×
10
16
s
{\displaystyle t_{\mathrm {ev} }(10^{11}\mathrm {kg} )=3\times 10^{9}\mathrm {year} =9\times 10^{16}\mathrm {s} }
P
=
3.563
45
×
10
32
[
k
g
M
]
2
W
{\displaystyle P=3.563\,45\times 10^{32}\left[{\frac {\mathrm {kg} }{M}}\right]^{2}\mathrm {W} }
t
e
v
=
8.407
16
×
10
−
17
[
M
0
k
g
]
3
s
≈
2.66
×
10
−
24
[
M
0
k
g
]
3
y
r
{\displaystyle t_{\mathrm {ev} }=8.407\,16\times 10^{-17}\left[{\frac {M_{0}}{\mathrm {kg} }}\right]^{3}\mathrm {s} \ \ \approx \ 2.66\times 10^{-24}\left[{\frac {M_{0}}{\mathrm {kg} }}\right]^{3}\mathrm {yr} }
M
0
=
2.282
71
×
10
5
[
t
e
v
s
]
1
/
3
k
g
≈
7.2
×
10
7
[
t
e
v
y
r
]
1
/
3
k
g
{\displaystyle M_{0}=2.282\,71\times 10^{5}\left[{\frac {t_{\mathrm {ev} }}{\mathrm {s} }}\right]^{1/3}\mathrm {kg} \ \ \approx \ 7.2\times 10^{7}\left[{\frac {t_{\mathrm {ev} }}{\mathrm {yr} }}\right]^{1/3}\mathrm {kg} }
t
e
v
(
2.28
×
10
5
k
g
)
=
1
s
{\displaystyle t_{\mathrm {ev} }(2.28\times 10^{5}\mathrm {kg} )=1\mathrm {s} }
E
(
2.28
×
10
5
k
g
)
=
2.05
×
10
22
J
{\displaystyle E(2.28\times 10^{5}\mathrm {kg} )=2.05\times 10^{22}\mathrm {J} }
P
(
2.28
×
10
5
k
g
)
=
6.84
×
10
21
W
{\displaystyle P(2.28\times 10^{5}\mathrm {kg} )=6.84\times 10^{21}\mathrm {W} }
P
=
σ
T
4
A
=
π
2
k
4
60
c
2
ℏ
3
(
ℏ
c
3
8
π
G
M
k
)
4
A
{\displaystyle P=\sigma T^{4}A={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}\left({\hbar \,c^{3} \over 8\pi GMk}\right)^{4}A}
P
=
π
2
k
4
60
c
2
ℏ
3
ℏ
4
c
12
4096
π
4
k
4
G
4
M
4
A
{\displaystyle P={\pi ^{2}k^{4} \over 60c^{2}\hbar ^{3}}{\frac {\hbar ^{4}c^{12}}{4096\pi ^{4}k^{4}G^{4}M^{4}}}A}
P
=
c
10
ℏ
245
,
760
π
2
G
4
M
4
A
{\displaystyle P={c^{10}\hbar \over 245,760\pi ^{2}G^{4}M^{4}}A}
A
c
10
ℏ
245
,
760
π
2
G
4
M
4
=
ℏ
c
6
15360
π
G
2
M
2
{\displaystyle A{c^{10}\hbar \over 245,760\pi ^{2}G^{4}M^{4}}={\hbar \,c^{6} \over 15360\,\pi \,G^{2}M^{2}}}
A
=
ℏ
c
6
15
,
360
π
G
2
M
2
c
10
ℏ
245
,
760
π
2
G
4
M
4
{\displaystyle A={\frac {\frac {\hbar \,c^{6}}{15,360\,\pi \,G^{2}M^{2}}}{\frac {c^{10}\hbar }{245,760\pi ^{2}G^{4}M^{4}}}}}
A
=
ℏ
c
6
15
,
360
π
G
2
M
2
245
,
760
π
2
G
4
M
4
c
10
ℏ
{\displaystyle A={\frac {\hbar \,c^{6}}{15,360\,\pi \,G^{2}M^{2}}}{\frac {245,760\pi ^{2}G^{4}M^{4}}{c^{10}\hbar }}}
A
=
16
π
G
2
M
2
c
4
{\displaystyle A={\frac {16\pi G^{2}M^{2}}{c^{4}}}}
Odd, it does come out the same as the usual formula as surface area of a sphere. My mistake must lie elsewhere.
compared to my derivations [ edit ]
T
a
r
t
i
c
l
e
=
T
m
i
n
e
2
{\displaystyle T_{article}={T_{mine} \over 2}}
P
a
r
t
i
c
l
e
=
q
m
i
n
e
16
{\displaystyle P_{article}={q_{mine} \over 16}}
For some reason,
T
m
i
n
e
{\displaystyle T_{mine}}
is coming out twice as large as
T
a
r
t
i
c
l
e
{\displaystyle T_{article}}
. It naturally follows that this would lead to
q
m
i
n
e
{\displaystyle q_{mine}}
being 16 times larger than
P
a
r
t
i
c
l
e
{\displaystyle P_{article}}
. I thought event horizons might have a surface area that was not equal to that of a conventional sphere, but that doesn't seem to explain it.
S
=
A
k
c
3
4
ℏ
G
{\displaystyle S={\frac {Akc^{3}}{4\hbar G}}}
T
=
ℏ
c
3
8
π
k
G
M
{\displaystyle T={\frac {\hbar c^{3}}{8\pi kGM}}}
(was Black hole entropy )
S
B
H
=
k
A
4
l
P
2
{\displaystyle S_{BH}={\frac {kA}{4l_{\mathrm {P} }^{2}}}}
l
P
=
G
ℏ
c
3
{\displaystyle l_{\mathrm {P} }={\sqrt {G\hbar \over c^{3}}}}
(was Laws of black hole mechanics )
T
H
=
κ
2
π
{\displaystyle T_{H}={\frac {\kappa }{2\pi }}}
(natural units )
S
B
H
=
A
4
{\displaystyle S_{BH}={\frac {A}{4}}}
(natural units )
I noticed this in the table of equations with their nondimensionalized equivalents:
Thermal energy per particle per degree of freedom
E
=
1
2
k
T
{\displaystyle E={\frac {1}{2}}kT}
This may be the key, if it's half of
k
T
{\displaystyle kT}
, much like
E
=
1
2
m
v
2
{\displaystyle E={\frac {1}{2}}mv^{2}}
threw me off with that half, when I was very young.
2
E
=
k
T
{\displaystyle 2E=kT\,}
E
=
k
T
2
{\displaystyle E={\frac {kT}{2}}}
,
T
=
2
E
k
{\displaystyle T={\frac {2E}{k}}}
,
k
=
2
E
T
{\displaystyle k={\frac {2E}{T}}}
r
s
=
2
G
m
c
2
{\displaystyle r_{s}={\frac {2Gm}{c^{2}}}}
r
s
=
m
×
1.48
×
10
−
27
{\displaystyle r_{s}=m\times 1.48\times 10^{-27}}
S
=
A
k
c
3
4
G
ℏ
{\displaystyle S={Akc^{3} \over 4G\hbar }}
A
=
8
π
M
2
G
2
c
4
{\displaystyle A={8\pi M^{2}G^{2} \over c^{4}}}
- Here's where it's different! That's not the formula for an undistorted sphere.
S
=
2
π
k
G
M
2
ℏ
c
{\displaystyle S={2\pi kGM^{2} \over \hbar c}}
P
S
H
=
G
ρ
ℏ
90
{\displaystyle P_{SH}={G\rho \hbar \over 90}}
P
S
H
=
ℏ
c
6
960
π
G
2
M
2
{\displaystyle P_{SH}={\hbar c^{6} \over 960\pi G^{2}\,M^{2}}}
ρ
=
M
(
4
π
3
)
R
H
3
=
M
(
4
π
3
)
(
2
G
M
c
2
)
3
=
3
c
6
32
π
G
3
M
2
{\displaystyle \rho ={M \over ({4\pi \over 3})R_{H}^{3}}={M \over ({4\pi \over 3})({2G\,M \over c^{2}})^{3}}={3c^{6} \over 32\pi G^{3}\,M^{2}}}
S
b
h
=
k
A
c
3
12
ℏ
G
{\displaystyle S_{bh}={kAc^{3} \over 12\hbar G}}
S
b
h
=
1
3
S
B
e
k
=
1
3
[
k
A
c
3
4
ℏ
G
]
{\displaystyle S_{bh}={\frac {1}{3}}S_{Bek}={\frac {1}{3}}\left[{kAc^{3} \over 4\hbar G}\right]}
Solar-mass black hole [ edit ]
M
=
1.9889
×
10
30
k
g
{\displaystyle M=1.9889\times 10^{30}\mathrm {kg} }
R
=
2953.3
m
{\displaystyle R=2953.3\mathrm {m} \,}
E
=
1.7876
×
10
47
J
{\displaystyle E=1.7876\times 10^{47}\mathrm {J} }
A
=
2
π
R
2
=
5.4800
×
10
7
m
2
{\displaystyle A=2\pi R^{2}=5.4800\times 10^{7}\mathrm {m^{2}} }
or
A
=
4
π
R
2
=
1.0960
×
10
8
m
2
{\displaystyle A=4\pi R^{2}=1.0960\times 10^{8}\mathrm {m^{2}} }
S
=
2
π
k
G
M
2
ℏ
c
=
7.2427
×
10
53
J
/
K
{\displaystyle S={2\pi kG\,M^{2} \over \hbar c}=7.2427\times 10^{53}\mathrm {J/K} }
T
=
ℏ
c
3
8
π
k
G
M
=
6.1702
×
10
−
8
K
{\displaystyle T={\hbar c^{3} \over 8\pi kG\,M}=6.1702\times 10^{-8}\mathrm {K} }
P
=
ℏ
c
6
15
,
360
π
G
2
M
2
=
9.0081
×
10
−
29
W
{\displaystyle P={\hbar c^{6} \over 15,360\pi G^{2}\,M^{2}}=9.0081\times 10^{-29}\mathrm {W} }
e
b
=
P
A
{\displaystyle e_{b}={P \over A}}
e
b
=
P
2
π
R
2
=
1.6438
×
10
−
36
W
/
m
2
{\displaystyle e_{b}={P \over 2\pi R^{2}}=1.6438\times 10^{-36}\mathrm {W/m^{2}} }
or
e
b
=
P
4
π
R
2
=
8.2191
×
10
−
37
W
/
m
2
{\displaystyle e_{b}={P \over 4\pi R^{2}}=8.2191\times 10^{-37}\mathrm {W/m^{2}} }
e
b
=
σ
T
4
=
5.6705
×
10
−
8
W
m
2
K
4
(
6.1702
×
10
−
8
K
)
4
=
8.2191
×
10
−
37
W
/
m
2
{\displaystyle e_{b}=\sigma T^{4}=5.6705\times 10^{-8}\mathrm {W \over m^{2}K^{4}} \,(6.1702\times 10^{-8}\mathrm {K} )^{4}=8.2191\times 10^{-37}\mathrm {W/m^{2}} }
e
b
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
=
8.2191
×
10
−
37
W
/
m
2
{\displaystyle e_{b}={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}=8.2191\times 10^{-37}\mathrm {W/m^{2}} }
1-second black hole [ edit ]
M
=
2.2827
×
10
5
k
g
{\displaystyle M=2.2827\times 10^{5}\mathrm {kg} }
R
=
3.3895
×
10
−
22
m
{\displaystyle R=3.3895\times 10^{-22}\mathrm {m} }
E
=
2.0516
×
10
22
J
=
5
×
10
12
t
o
n
T
N
T
{\displaystyle E=2.0516\times 10^{22}\mathrm {J} =5\times 10^{12}\mathrm {ton_{TNT}} }
A
=
2
π
R
2
=
7.2185
×
10
−
43
m
2
{\displaystyle A=2\pi R^{2}=7.2185\times 10^{-43}\mathrm {m^{2}} }
or
A
=
4
π
R
2
=
1.4437
×
10
−
42
m
2
{\displaystyle A=4\pi R^{2}=1.4437\times 10^{-42}\mathrm {m^{2}} }
S
=
2
π
k
G
M
2
ℏ
c
=
9540.3
J
/
K
{\displaystyle S={2\pi kG\,M^{2} \over \hbar c}=9540.3\mathrm {J/K} }
T
=
ℏ
c
3
8
π
k
G
M
=
5.3761
×
10
17
K
{\displaystyle T={\hbar c^{3} \over 8\pi kG\,M}=5.3761\times 10^{17}\mathrm {K} }
P
=
ℏ
c
6
15
,
360
π
G
2
M
2
=
6.8386
×
10
21
W
{\displaystyle P={\hbar c^{6} \over 15,360\pi G^{2}\,M^{2}}=6.8386\times 10^{21}\mathrm {W} }
e
b
=
P
2
π
R
2
=
9.4738
×
10
63
W
/
m
2
{\displaystyle e_{b}={P \over 2\pi R^{2}}=9.4738\times 10^{63}\mathrm {W/m^{2}} }
or
e
b
=
P
4
π
R
2
=
4.7369
×
10
63
W
/
m
2
{\displaystyle e_{b}={P \over 4\pi R^{2}}=4.7369\times 10^{63}\mathrm {W/m^{2}} }
e
b
=
σ
T
4
=
5.6705
×
10
−
8
W
m
2
K
4
(
5.3761
×
10
17
K
)
4
=
4.7369
×
10
63
W
/
m
2
{\displaystyle e_{b}=\sigma T^{4}=5.6705\times 10^{-8}\mathrm {W \over m^{2}K^{4}} \,(5.3761\times 10^{17}\mathrm {K} )^{4}=4.7369\times 10^{63}\mathrm {W/m^{2}} }
e
b
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
=
4.7369
×
10
63
W
/
m
2
{\displaystyle e_{b}={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}=4.7369\times 10^{63}\mathrm {W/m^{2}} }
E
P
=
m
P
ℓ
P
2
t
P
2
{\displaystyle E_{\mathrm {P} }={m_{\mathrm {P} }\ell _{\mathrm {P} }^{2} \over t_{\mathrm {P} }^{2}}}
P
P
=
m
P
ℓ
P
2
t
P
3
{\displaystyle P_{\mathrm {P} }={m_{\mathrm {P} }\ell _{\mathrm {P} }^{2} \over t_{\mathrm {P} }^{3}}}
σ
=
π
2
60
=
0.16449
E
P
t
P
ℓ
P
2
T
P
4
=
0.16449
m
P
t
P
3
T
P
4
{\displaystyle \sigma ={\pi ^{2} \over 60}=0.16449{E_{\mathrm {P} } \over t_{\mathrm {P} }\ell _{\mathrm {P} }^{2}T_{\mathrm {P} }^{4}}=0.16449{m_{\mathrm {P} } \over t_{\mathrm {P} }^{3}T_{\mathrm {P} }^{4}}}
Solar-mass black hole [ edit ]
M
=
9.1373
×
10
37
m
P
{\displaystyle M=9.1373\times 10^{37}m_{\mathrm {P} }}
R
=
1.8275
×
10
38
ℓ
P
{\displaystyle R=1.8275\times 10^{38}\ell _{\mathrm {P} }}
E
=
9.1373
×
10
37
E
P
{\displaystyle E=9.1373\times 10^{37}E_{\mathrm {P} }}
A
=
2
π
R
2
=
2.0983
×
10
77
ℓ
P
2
{\displaystyle A=2\pi \,R^{2}=2.0983\times 10^{77}\ell _{\mathrm {P} }^{2}}
or
A
=
4
π
R
2
=
4.1966
×
10
77
ℓ
P
2
{\displaystyle A=4\pi \,R^{2}=4.1966\times 10^{77}\ell _{\mathrm {P} }^{2}}
S
=
2
π
k
G
M
2
ℏ
c
=
5.2458
×
10
76
E
P
/
T
P
{\displaystyle S={2\pi kG\,M^{2} \over \hbar c}=5.2458\times 10^{76}E_{\mathrm {P} }/T_{\mathrm {P} }}
T
=
ℏ
c
3
8
π
k
G
M
=
4.3546
×
10
−
40
T
P
{\displaystyle T={\hbar c^{3} \over 8\pi kG\,M}=4.3546\times 10^{-40}T_{\mathrm {P} }}
P
=
ℏ
c
6
15
,
360
π
G
2
M
2
=
2.4821
×
10
−
81
P
P
{\displaystyle P={\hbar c^{6} \over 15,360\pi G^{2}\,M^{2}}=2.4821\times 10^{-81}P_{\mathrm {P} }}
e
b
=
P
2
π
R
2
=
1.1829
×
10
−
158
P
P
/
ℓ
P
2
{\displaystyle e_{b}={P \over 2\pi \,R^{2}}=1.1829\times 10^{-158}P_{\mathrm {P} }/\ell _{\mathrm {P} }^{2}}
or
e
b
=
P
4
π
R
2
=
5.9146
×
10
−
159
P
P
/
ℓ
P
2
{\displaystyle e_{b}={P \over 4\pi \,R^{2}}=5.9146\times 10^{-159}P_{\mathrm {P} }/\ell _{\mathrm {P} }^{2}}
e
b
=
σ
T
4
=
5.9146
×
10
−
159
P
P
/
ℓ
P
2
T
4
=
3.5956
×
10
−
158
T
P
4
{\displaystyle e_{b}=\sigma T^{4}=5.9146\times 10^{-159}P_{\mathrm {P} }/\ell _{\mathrm {P} }^{2}\quad T^{4}=3.5956\times 10^{-158}T_{\mathrm {P} }^{4}}
e
b
=
ℏ
c
10
245
,
760
π
2
G
4
M
4
=
5.9146
×
10
−
159
P
P
/
ℓ
P
2
{\displaystyle e_{b}={\hbar c^{10} \over 245,760\pi ^{2}G^{4}\,M^{4}}=5.9146\times 10^{-159}P_{\mathrm {P} }/\ell _{\mathrm {P} }^{2}}
1-second black hole [ edit ]