Sissy
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Hello,
I don't understand how to solve this problem. I do not want a solution because I will calculate it by my own but I need some hints how to start.
I don't know what to do
Here is the exercise:
Show that, if the cosmical constant term is retained in Einstein's equation, it reduces in empty space to R_{ij}+\Lambda g_{ij} = 0. Deduce that the spherically symmetric Schwarzschild solution (cf. equation (52.9)) is given by
b = 1- \dfrac{2m}{r} - \dfrac{1}{3} \Lambda r^2
Using the approximate equation (48.17), show that this implies the existence of an additional force of repulsion from the centre proportional to the radius r.
With
Equation (52.9) b = e^\beta = 1- \dfrac{2m}{r}
Equation (48.17) g_{44} = 1 + \dfrac{2U}{c^2}
U is probably the Newtonian potential function.
I have no idea how to start.
Thank you for giving me some hints.
greetings
I don't understand how to solve this problem. I do not want a solution because I will calculate it by my own but I need some hints how to start.
I don't know what to do

Show that, if the cosmical constant term is retained in Einstein's equation, it reduces in empty space to R_{ij}+\Lambda g_{ij} = 0. Deduce that the spherically symmetric Schwarzschild solution (cf. equation (52.9)) is given by
b = 1- \dfrac{2m}{r} - \dfrac{1}{3} \Lambda r^2
Using the approximate equation (48.17), show that this implies the existence of an additional force of repulsion from the centre proportional to the radius r.
With
Equation (52.9) b = e^\beta = 1- \dfrac{2m}{r}
Equation (48.17) g_{44} = 1 + \dfrac{2U}{c^2}
U is probably the Newtonian potential function.
I have no idea how to start.
Thank you for giving me some hints.
greetings