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Standard thin-disk luminosity
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Astrophysics
Astrophysical disk
Accretion disk
Alpha disk
Shakura--Sunyaev thin disk
Standard thin-disk dissipation flux
2026-09-28
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Integrating the
standard thin-disk dissipation flux
gives
L
thin
=
2
R
in
GM
M
˙
=
2
1
M
˙
R
in
2
Ω
K
,
in
2
.
(1)
Half of the
Newtonian potential
-
energy
decrease remains
as
orbital
kinetic energy
until the inner edge.
Ancestors
(9)
Standard thin-disk dissipation flux
Shakura--Sunyaev thin disk
Alpha disk
Accretion disk
Astrophysical disk
Astrophysics
Branch of physics
Physics
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(1)
Past exam of the mathematics course of the University of Cambridge
/
2024
/
iii
/
Paper 347
/
3
/
c
/
Solution
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