Exponential potential for inflation

shooride
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hi
I want to solve inflation problem for exponential potential.
v(\phi) = v_0 exp(-\alpha \phi)
(it's known as barrow or pawer law inflation )
we have 2 main equations:
H^2 = 8π G / 3 (1/2 (\dot{\phi})^2 + v(\phi))
\ddot{\phi} + 3H \dot{\phi} + v(\phi)'=0
I must solve this 2 equ and find \phi(t) and H(Hubble).
in the book of cosmology by weinberg has written,it is easy but i can't do it.can anyone help me?
best
 
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shooride said:
hi
I want to solve inflation problem for exponential potential.
v(\phi) = v_0 exp(-\alpha \phi)
(it's known as barrow or pawer law inflation )
we have 2 main equations:
H^2 = 8π G / 3 (1/2 (\dot{\phi})^2 + v(\phi))
\ddot{\phi} + 3H \dot{\phi} + v(\phi)'=0
I must solve this 2 equ and find \phi(t) and H(Hubble).
in the book of cosmology by weinberg has written,it is easy but i can't do it.can anyone help me?
best
The assumption of slow-roll inflation is that \ddot{\phi} is small compared to the "friction" term 3H\dot{\phi}, and thus can be neglected.

So your job is basically two-fold:
1. Solve the equations in the slow-roll regime.
2. Show the parameter values for which the slow-roll regime is valid.
 
You made this problem way too easy to solve, Chalnoth.
 
Chalnoth said:
The assumption of slow-roll inflation is that \ddot{\phi} is small compared to the "friction" term 3H\dot{\phi}, and thus can be neglected.

So your job is basically two-fold:
1. Solve the equations in the slow-roll regime.
2. Show the parameter values for which the slow-roll regime is valid.

thanks,but I think that it has exact solution.without slow-roll condition..
 

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