I have been thinking hard about the scenario from my previous post. I have decided that it might produce an interesting result, but I am now thinking it will not be very relevant for reasons I will discuss later. Here are some beginning results.
I decided to chose for D
m the distance from the Milky Way (MW) center, P
MW, at which the escape velocity equals the Hubble velocity.
Vesc = √(2 G MMW / Dm)
Vh = h Dm
G = MMW = 6.69 x 10-11 m3 kg-1 s-2
MMW = 1.4 x 1042 kg
h-1 = 5.45 x 1017 s
Dm = (2 G MMW / h2)3/2 = 3.82 x 1022 m
I assumed all of the MW mass is at the galaxy's center, and at time t = 0, a DM particle is at distance y
0 = D
m with zero velocity. The particle falls radially toward the center on a radial line that passes through the sun. The time t at which the particle is at distance y is given by:
where μ = G M
MW.
(See
https://en.wikipedia.org/wiki/Free_fall Inverse-square law gravitational field.)
The time at which the test particle reaches P
MW is
t(0) = 8.56 x 1017 s = 27.2 Gy.
The distance between the sun and P
MW is
ysun = 2.57 x 1021 m.
The time at which the test particle reaches the sun is
t(ysun) = 1.37 x 1017 s = 4.34 Gy.
I will add in a later post calculations for the velocity of the test particle at y = 0 and y = y
sun.
My reasons for expecting the results this scenario to not be very relevant are the following.
I think that the way DM in the MW halo actually passes by the sun is not radially. Also the time frame for the particle to fall is too long for the scenario to have much relevance.
I think a scenario closer to reality is to consider that the DM halo is (1) more-or-less on the average not moving, and (2) it has a density ρ(y) that varies with the distance y from P
MW. Also, at the time the sun and it's system was being formed, (3) the baryonic material that was to become the solar system was passing through the halo DM at an approximate radial distance y
sun with the DM density being ρ
DM(y
sun), and (4) this proto-solar system material having in it's orbit with respect to P
MW a velocity through the DM. This velocity can be compared with the MW's escape velocity at y
sun.
It may be that (a) the orbital velocity of the sun about P
MW is too fast for the sun to accumulate enough DM around it to effect planet orbits, and (b) without the sun being able to capture DM, the ρ
DM(y
sun) density might be too small to effect the orbits of the sun's planets. I think this scenario would be more relevant than the one in my previous post for answering the thread's question.
Any comments or questions?