Appendix C
Concerning
the
Kepler
Action
Variables
The two closed curves of integration in the integrals
are fixed by requiring the vanishing
of
the corresponding velocities
or,
better,
of
the corresponding momenta
p8
and
pr
expressed,
of
course, in terms
of
variables
re
and
rv.
In
this way, the integration limits are fixed by
Therefore, the
“6”
integration must be performed between the
limits
$1
and
192
given by the solutions of
where
Eq.
(4.25)
has been used. Since
19
itself always lies between
0
and
r,
where sin8
>
0,
we have
sin291
=
sin&
=
COSLY.
Thus, the integration goes
406