Modern Cosmology Dodelson Problem 6.12b (Inflation)

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SUMMARY

The discussion focuses on solving the Dodelson Problem 6.12b related to inflation in modern cosmology, specifically demonstrating the equation ##4\pi G(\dot \phi)^2=\epsilon a^2 H^2##. Participants detail their attempts to manipulate equations involving the Hubble parameter ##H##, the energy density ##\rho##, and pressure ##P##, leading to a critical evaluation of the relationship between ##\frac{d^2 a}{dt^2}## and ##\ddot a##. The final resolution involved correcting a typographical error regarding the pressure term, confirming that the correct form is ##3P## instead of ##-P##.

PREREQUISITES
  • Understanding of cosmological equations, particularly the Friedmann equations.
  • Familiarity with the concepts of inflation and scalar fields in cosmology.
  • Proficiency in calculus, specifically derivatives and their physical interpretations.
  • Knowledge of the Hubble parameter and its significance in cosmological models.
NEXT STEPS
  • Study the Friedmann equations in detail to understand their implications for cosmic evolution.
  • Explore the role of scalar fields in inflationary models, focusing on the dynamics of the inflaton field.
  • Learn about the derivation and significance of the Hubble parameter in cosmology.
  • Investigate the relationship between energy density, pressure, and the equation of state in cosmological contexts.
USEFUL FOR

Students and researchers in theoretical physics, particularly those focusing on cosmology and the dynamics of the early universe. This discussion is also beneficial for anyone studying inflationary models and their mathematical foundations.

travelingscienceman
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Homework Statement



Show that ##4\pi G(\dot \phi)^2=\epsilon a^2 H^2##

Homework Equations



Over dots mean derivative with respect to ##\eta##.
$$\frac{1}{a}\frac{d}{d\eta}=\frac{d}{dt}$$
$$H=\frac{\dot a}{a^2}$$
$$\epsilon=\frac{-\dot H}{aH^2}$$
$$(\frac{\dot a}{a^2})^2=(\frac{da/dt}{a})^2=\frac{8\pi G\rho}{3}$$
$$\frac{\ddot a}{a^3}=\frac{d^2 a/dt^2}{a}=-\frac{4\pi G}{3}(\rho-P)$$
$$\rho=\frac{1}{2}(\frac{d\phi}{dt})^2 + V(\phi)$$
$$P=\frac{1}{2}(\frac{d\phi}{dt})^2 - V(\phi)$$
$$\frac{d\phi}{dt}=\frac{\dot\phi}{a}$$

The Attempt at a Solution



First I plug ##\epsilon## into the main equation so I get ##4\pi G(\dot phi)^2=-a \dot H##. Then I find
$$\dot H=\frac{\ddot a a-2\dot a^2}{a^3}$$
$$-a\dot H=\frac{2\dot a^2-\ddot a a}{a^2}=2a^2(\frac{\dot a}{a^2})^2-a^2\frac{\ddot a}{a^3}$$
$$=a^2(\frac{16\pi G}{3}\rho+\frac{4\pi G}{3}(\rho+3P))$$
$$=a^2\frac{4\pi G}{3}(4\rho +\rho+3P)=a^2\frac{4\pi G}{3}(5\rho +3P)$$
$$=a^2\frac{4\pi G}{3}(\frac{5}{2}\frac{\dot\phi^2}{a^2}+5V+\frac{3}{2}\frac{\dot\phi^2}{a^2}-3V)$$
$$=a^2\frac{4\pi G}{3}(4\frac{\dot\phi^2}{a^2}+2V)$$

Which is where I have problems as I cannot simplify things further to get the desired ##4\pi G(\dot \phi)^2##. If the 2V was gone and there was one less factor of ##\dot \phi^2## then I would get the right answer, but I keep coming to this same equation. Any help would be appreciated. Thanks in advance!
 
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travelingscienceman said:
$$ \frac{\ddot a}{a^3}=\frac{d^2 a/dt^2}{a}=-\frac{4\pi G}{3}(\rho-P)$$
##\large \frac{\ddot a}{a^3} \neq \frac{d^2 a/dt^2}{a}## You will need to be careful when relating ##\large \frac{d^2 a}{dt^2}## to ##\ddot a##.

Also, ##\large \frac{d^2 a/dt^2}{a}## ##\neq -\frac{4\pi G}{3}(\rho-P)##. Looks like a typographical error here. Shouldn't the ##-P## be ##+3P##?
 
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Thanks for your help once again! I was able to solve it after reevaluating ##\frac{d^2 a}{dt^2}## and got ##\frac{\ddot a a-\dot a^2}{a^3}##.

And yeah it's 3P, messed up typing it in.
 
travelingscienceman said:
I was able to solve it after reevaluating ##\frac{d^2 a}{dt^2}## and got ##\frac{\ddot a a-\dot a^2}{a^3}##.
Looks good.
 

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