Undergrad Solve Nonlinear DE: Friedmann Eqns for H 0-10^7

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The discussion focuses on solving the Friedmann equations to determine H(t) for the time interval 0<t<10^7. The equations relate the expansion rate of the universe to density and pressure, with specific forms provided for H and its derivatives. A suggested approach involves expressing dt in terms of the scale factor a, allowing for numerical integration to find t(a). An online tool is recommended for performing definite integrals, and a substitution is offered for potential integration difficulties. This method aims to facilitate the solution of the differential equations involved.
shinobi20
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From cosmology, the friedmann equations are given by,
##H^2 = (\frac{\dot a}{a})^2 = \frac{8\pi G}{3} \rho \, , \quad \frac{\ddot a}{a} = -\frac{4\pi G}{3}(\rho+3p) \, , \quad## where ##\rho = \frac{1}{2}(\dot \phi^2 + \phi^2)## and ##p = \frac{1}{2}(\dot \phi^2 - \phi^2)##

To get ##\dot H##,
##\dot H = \frac{d}{dt}(\frac{\dot a}{a}) = \frac{\ddot a}{a} - (\frac{\dot a}{a})^2 = -4\pi G(\rho + p) = -4\pi G \dot \phi^2##.

I want to solve for ##H## using this equation, where ##0<t<10^7##. How should I solve this DE? It's ok if the solution is in the implicit form.
 
Hi shinobi:

When solving for H(t) I would generally work with a different form of the Friedmann equation.
The one I mean is in the article just above "Useful Solutions".

H is given as a function of a, together with the parameter H0, and several density ratio parameters, the Ωs with various subscripts.
Since H = (1/a) (da/dt), dt can be expressed in the form f(a) da. This can be numerically integrated to get t(a) for a specific value of a. I found the following online tool useful for this.
You many want to substitute a = e-x if you find problems with the tool when integrating the f(a) form.

I hope this is helpful.

Regards,
Buzz
 

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