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Up: Definitions of Number and
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The equation of motion for a scalar field in an expanding universe
is
![\begin{displaymath}
\ddot{f} + 3 {\dot{a} \over a} \dot{f} - {1 \over a^2} \nabla^2 f
+ {\partial V \over \partial f} = 0.
\end{displaymath}](img150.png) |
(5.10) |
To define an adiabatic invariant occupation number for this field
we need to switch to conformal variables in which this equation
becomes a more standard oscillator equation. These variables are
![\begin{displaymath}
f_c \equiv a f;\;dt_c \equiv {1 \over a} dt.
\end{displaymath}](img151.png) |
(5.11) |
Using conformal time and noting that
![\begin{displaymath}
\dot{f} = {1 \over a} f';\;\ddot{f} = {1 \over a^2} f'' - {a'
\over a^3} f'
\end{displaymath}](img152.png) |
(5.12) |
the equation of motion becomes
![\begin{displaymath}
f'' + 2 {a' \over a} f' - \nabla^2 f + a^2 {\partial V \over
\partial f} = 0.
\end{displaymath}](img153.png) |
(5.13) |
Then switching to conformal field values note that
![\begin{displaymath}
f' = {1 \over a} f_c' - {a' \over a^2} f_c;\;f'' = {1 \over ...
...\over a^2} f_c' + 2 {a'^2 \over a^3} f_c - {a''
\over a^2} f_c
\end{displaymath}](img154.png) |
(5.14) |
and thus
![\begin{displaymath}
f_c'' - {a'' \over a} f_c - \nabla^2 f_c + a^4 {\partial V \over
\partial f_c} = 0.
\end{displaymath}](img155.png) |
(5.15) |
This equation can be approximated in Fourier space by
![\begin{displaymath}
\tilde{F}_{k,c}'' + \omega_k \tilde{F}_{k,c} = 0
\end{displaymath}](img156.png) |
(5.16) |
where
and
![\begin{displaymath}
\omega_k^2 \equiv k^2 + a^4 \left<{\partial^2 V \over \parti...
...left<{\partial^2 V
\over \partial f^2}\right> - {a'' \over a}.
\end{displaymath}](img158.png) |
(5.17) |
Next: Occupation Number and Energy
Up: Definitions of Number and
Previous: Rescaled Fourier Transforms
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This
documentation was generated on 2008-01-21