The Universe Is Expanding — Question 8

Section 44-10 · Physics pages 7486–7487

Question 8 Comoving coordinates remove the uniform part of the expansion Two galaxies have fixed comoving separation chi=40 Mpc, with proper separation D=a chi. At one epoch a=.50 and ˙a = .040 Gyr−1. expansion earlier later Schematic; labels, not drawing lengths, specify the data. (a) Calculate D, H and the rate of change of proper separation. (b) If a third object has peculiar velocity u relative to this flow, derive the additional term in its physical velocity for time-dependent chi.
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Question 8 - Solution Comoving coordinates remove the uniform part of the expansion expansion earlier later (a) Method and calculation D = .50(40) = 20 Mpc, H = ˙a/a = .080 Gyr−1 . ˙D = ˙aχ = 1.60 Mpc/Gyr = HD . (b) Interpretation and further calculation ˙D = d(aχ) dt = ˙aχ + a ˙χ. ˙D = HD + u, u = a ˙χ . Physical check Expansion does not imply that every object has fixed comoving position; gravitationally bound systems and peculiar motions break that simplification.

Question 8

Comoving coordinates remove the uniform part of the expansion

Two galaxies have fixed comoving separation chi=40 Mpc, with proper separation D=a chi. At one epoch a=.50 and ȧ=.040\dot a=.040 Gyr−1^{-1}.

Diagram shown in the original SVG worksheet.

  1. Calculate D, H and the rate of change of proper separation.

  2. If a third object has peculiar velocity u relative to this flow, derive the additional term in its physical velocity for time-dependent chi.

Question 8 - Solution

Comoving coordinates remove the uniform part of the expansion

Diagram shown in the original SVG worksheet.

(a) Method and calculation

D=.50(40)=20Mpc,H=ȧ/a=.080Gyr−1.\boxed{D=.50(40)=20\ {\mathrm{Mpc}},\quad H=\dot a/a=.080\ {\mathrm{Gyr}}^{-1}}.Ḋ=ȧχ=1.60Mpc/Gyr=HD.\boxed{\dot D=\dot a\chi=1.60\ {\mathrm{Mpc/Gyr}}=HD}.

(b) Interpretation and further calculation

Ḋ=d(aχ)dt=ȧχ+aχ̇.\dot D=\frac{d(a\chi)}{dt}=\dot a\chi+a\dot\chi.Ḋ=HD+u,u=aχ̇.\boxed{\dot D=HD+u,\quad u=a\dot\chi}.

Physical check

Expansion does not imply that every object has fixed comoving position; gravitationally bound systems and peculiar motions break that simplification.