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

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SUMMARY

The discussion focuses on solving the Friedmann equations in cosmology, specifically for the Hubble parameter H over the interval 0 < t < 10^7. The equations are defined as H^2 = (dot a/a)^2 = (8πG/3)ρ and (ddot a/a) = -(4πG/3)(ρ + 3p), where ρ and p are expressed in terms of the scalar field φ. To derive H(t), the user is advised to utilize a different form of the Friedmann equation and numerically integrate the function f(a) to obtain t(a) for specific values of a, leveraging online tools for assistance.

PREREQUISITES
  • Understanding of Friedmann equations in cosmology
  • Familiarity with differential equations and numerical integration
  • Knowledge of scalar fields in cosmology
  • Experience with online mathematical tools for integration
NEXT STEPS
  • Research the different forms of the Friedmann equations
  • Learn numerical integration techniques for differential equations
  • Explore the implications of density ratio parameters (Ωs) in cosmology
  • Investigate the use of online tools for solving integrals in physics
USEFUL FOR

Cosmologists, physicists, and mathematicians interested in solving differential equations related to the Friedmann equations and those looking to understand the dynamics of the universe's expansion.

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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