Why Is the Accelerated Friedmann Equation Giving Incorrect Signs?

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Discussion Overview

The discussion revolves around the derivation of the accelerated Friedmann equation in cosmology, specifically addressing issues related to the signs and factors in the equations derived from the Einstein Equations. Participants explore the implications of these signs and factors on the resulting equations.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant expresses difficulty in deriving the accelerated Friedmann equation and questions the sign of the term involving the cosmological constant, Λ.
  • Another participant challenges the sign used for the trace of the Λ term, asserting it should be +4Λ instead of -4Λ.
  • A subsequent reply confirms the correction regarding the trace of the Λ term and notes that this affects the expression for \(\ddot{a}/a\).
  • One participant suggests that the issue may not be solely about the sign but also about the factors involved, such as the 1/6 factor in front of the density and pressure terms.
  • Another participant provides an alternative approach by taking the time derivative of the Friedmann equations, leading to a different expression for \(\ddot{a}/a\) that includes a correction to the factors used.
  • A later reply indicates that the original participant has resolved their issue, attributing it to both sign and factor errors.

Areas of Agreement / Disagreement

Participants generally agree on the correction of the sign for the trace of the Λ term, but there remains some disagreement regarding the factors involved in the equations. The discussion reflects multiple viewpoints on the derivation process and the resulting expressions.

Contextual Notes

Participants reference specific terms and factors in the equations, indicating potential limitations in their derivations that depend on the definitions and assumptions made in the context of the Friedmann equations.

Cancer
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Hi!

I'm struggling to derive the accelerated Friedmann equation (shame on me!)...

I'll tell you what I'm doing and maybe you can find where the mistake is.

First of all, we know that:

H^2 = \frac{\rho}{2M^2_p}+\frac{\Lambda}{3}

Now, using the Einstein Equations and doing the trace of these, we get:
-R-4\Lambda = \frac{T}{M^2_p} = \frac{-\rho+3p}{M^2_p}
Where R=6[ \frac{\ddot{a}}{a}+H^2].
Using this, I get:
\frac{\ddot{a}}{a} = -\Lambda - \frac{1}{6}\frac{\rho+3p}{M^2_p}

The problem is that I shouldn't get a minus sing in the \Lambda and divided by 3, but I just CAN'T see what I'm doing wrong, as you can see here:
http://ned.ipac.caltech.edu/level5/Carroll2/Carroll1_2.html
I've tried to look for a book that does this derivation but I haven't found any...

If you could help me I would really appreciate it!
Thanks
 
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Why do you have the trace of the \Lambda as -4\Lambda? I don't think that's right.
 
Chalnoth said:
Why do you have the trace of the \Lambda as -4\Lambda? I don't think that's right.

The trace of the ##\Lambda g_{\mu \nu}## term is ##+4 \Lambda##, which then gives a ##+ \Lambda/3## in the expression for ##\ddot{a}/a##.
 
George Jones said:
The trace of the ##\Lambda g_{\mu \nu}## term is ##+4 \Lambda##, which then gives a ##+ \Lambda/3## in the expression for ##\ddot{a}/a##.

Oh my god, thank you, I was using
R_{\mu \nu} -\frac{1}{2}R g_{\mu \nu} -\Lambda g_{\mu \nu} = 8\pi G T_{\mu \nu}
Because that's what the problem said, but I see now that it is a typo in the sign... I'm going to kill my professor he has done 3 typos in this problem already T_T

Thanks a lot people!
 
Please don't kill your professor
 
Are you sure about your result? It doesn't seem like only a matter of sign, but also a matter of your factors (like 1/6 in front of the density/momentum)

I find it easier to take the FE and take the time derivative of it. Doing so (and using the fluid continuity equation) the answer would be like:

\frac{\ddot{a}}{a} = \frac{\Lambda}{3} - \frac{1}{2} \frac{\rho +3p}{2M_{Pl}^2}

This coincides also with the bibliography of 8 \pi G /3 since in your case you have written that as \frac{1}{2 M_{Pl}^2}. If you prefer ##G##, it would be:

\frac{\ddot{a}}{a} = \frac{\Lambda}{3} - \frac{4 \pi G }{3} (\rho +3p)
 
Last edited:
bapowell said:
Please don't kill your professor

Just kidding ;)

ChrisVer said:
Are you sure about your result? It doesn't seem like only a matter of sign, but also a matter of your factors (like 1/6 in front of the density/momentum)

I find it easier to take the FE and take the time derivative of it. Doing so (and using the fluid continuity equation) the answer would be like:

\frac{\ddot{a}}{a} = \frac{\Lambda}{3} - \frac{1}{2} \frac{\rho +3p}{2M_{Pl}^2}

This coincides also with the bibliography of 8 \pi G /3 since in your case you have written that as \frac{1}{2 M_{Pl}^2}. If you prefer ##G##, it would be:

\frac{\ddot{a}}{a} = \frac{\Lambda}{3} - \frac{4 \pi G }{3} (\rho +3p)
As I said, it was a problem of the sign and also the factor 3.
I've already solved my problem, thanks a lot! ^^
 
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