Undergrad How Does the Hubble Parameter Relate to Galaxy Movement?

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The discussion focuses on the relationship between the Hubble parameter and galaxy movement, specifically how to derive the equation for galaxy velocity. The key equation involves the time derivative of the scale factor, represented as da/dt, and its relation to the distance between galaxies. The transformation from da/dt(xi - x1) to (∙a/a)a(t)(xi - x1) is clarified, emphasizing the importance of defining variables consistently. Participants highlight that understanding these derivations may require familiarity with different conventions in equations. The thread suggests that further clarification can be found in Leonard Susskind's work for those needing additional context.
Komorebi
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This is the time derivative to calculate the speed which a galaxy moves away from another galaxy. I don't understand how they get from da/dt (xi − x1) to (∙a)/a a(t). (xi − x1). Could anyone explain this? vi(t) = d/dt (ri(t) − r1(t))
= d/dt a(t)(xi − x1)
= da/dt (xi − x1)
= (∙a)/a a(t). (xi − x1) !
=(∙a)/a (ri(t) − r1(t))
= H(t) (ri(t) − r1(t))

[ ∙a= da/dt ]
 
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It's a good idea to define the variables in an equation. Not everyone uses the same 'conventions'.
 
Komorebi said:
how they get from da/dt (xi − x1) to (∙a)/a a(t). (xi − x1)
Since ##\frac{da}{dt}=\dot a##
and ##\frac{a}{a}=1##
You have ##\frac{da}{dt} \Delta x## multiplied by 1 to net you ##\frac{\dot a}{a}a\Delta x##.

If it still doesn't click, Leonard Susskind derives this here in a slightly different, but essentially the same manner:

(starting at 21:22 mark)
 
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