Exponential potential for inflation

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Discussion Overview

The discussion centers around solving the inflation problem associated with an exponential potential, specifically the potential given by v(φ) = v₀ exp(-αφ). Participants are examining the relevant equations governing this inflationary model and exploring the conditions under which solutions can be derived, including the possibility of exact solutions versus those requiring the slow-roll approximation.

Discussion Character

  • Homework-related
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant seeks assistance in solving the equations for inflation with the exponential potential, specifically looking for φ(t) and H (Hubble parameter).
  • Another participant suggests that the problem can be approached using the slow-roll approximation, where the term \(\ddot{\phi}\) is negligible compared to the friction term \(3H\dot{\phi}\).
  • A different participant challenges the simplification proposed by the previous contributor, asserting that an exact solution exists without relying on the slow-roll condition.

Areas of Agreement / Disagreement

There is disagreement among participants regarding the necessity of the slow-roll approximation. Some participants advocate for its use, while others believe that an exact solution is possible without it.

Contextual Notes

The discussion does not resolve the mathematical steps required to find the solutions, and the validity of the slow-roll approximation remains contested. Participants have not reached a consensus on the approach to take.

shooride
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hi
I want to solve inflation problem for exponential potential.
[tex]v(\phi) = v_0 exp(-\alpha \phi)[/tex]
(it's known as barrow or pawer law inflation )
we have 2 main equations:
[tex]H^2 = 8π G / 3 (1/2 (\dot{\phi})^2 + v(\phi))[/tex]
[tex]\ddot{\phi} + 3H \dot{\phi} + v(\phi)'=0[/tex]
I must solve this 2 equ and find [itex]\phi(t)[/itex] 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
 
Last edited:
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shooride said:
hi
I want to solve inflation problem for exponential potential.
[tex]v(\phi) = v_0 exp(-\alpha \phi)[/tex]
(it's known as barrow or pawer law inflation )
we have 2 main equations:
[tex]H^2 = 8π G / 3 (1/2 (\dot{\phi})^2 + v(\phi))[/tex]
[tex]\ddot{\phi} + 3H \dot{\phi} + v(\phi)'=0[/tex]
I must solve this 2 equ and find [itex]\phi(t)[/itex] 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 [itex]\ddot{\phi}[/itex] is small compared to the "friction" term [itex]3H\dot{\phi}[/itex], 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 [itex]\ddot{\phi}[/itex] is small compared to the "friction" term [itex]3H\dot{\phi}[/itex], 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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