Das Alter des Thread's ist ja noch im Rahmen.
Was ist eigentlich der Unterschied zwischen der Formel:
t = t_0/sqrt(1 - (2 g r)/c^2)
----------------------------------------------------------
t | time seen by stationary observer
g | gravitational acceleration
t_0 | time in rest frame
r | radius
c | speed of light in vacuum (≈ 2.998×10^8 m/s)
(assuming a nonrotating spherical body)
und der Formel:
t = t_0/sqrt(1 - (2 G M)/(r c^2))
----------------------------------------------------------
t | time seen by stationary observer
M | mass
t_0 | time in rest frame
r | radius
G | Newtonian gravitational constant (≈ 6.674×10^-11 m^3/(kg s^2))
c | speed of light in vacuum (≈ 2.998×10^8 m/s)
(assuming a nonrotating spherical body
Kann jemand kurz was dazu sagen?