angle–action variables
DESCRIPTION
action angle variable and othrsTRANSCRIPT
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p
q
q0
Rotation
p is periodic function of q configuration of the system is the same under q q + q0:p(t+ T ) = p(t); q(t+ T ) = q(t) + q0
eg rotating pendulum
6.3.1 Definition of the AngleAction variables
For either type of motion, define action variable
J =1
2pi
complete period
pdq J() , angular momentum= area in phase space swept out in one period/2pi .
[Note alternative convention without 2pi. Then in following.]Now use J to replace . So (q, p) (, J) via a generating function, F2(q, J) W (q, J) so that
p =W
q, =
W
J,
where is the coordinate conjugate to J the action variable.
p
q
J
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Hamiltonian is
K(J) = H , ( cyclic) ,
and so equations of motion are
J = H
= 0 = J = constant
=H
J= (J) = = (J)t+ with (J) = H
J.
In one period, the change in is
=
d =
qdq
=
2W
qJdq
=
J
W
qdq as J is constant
=
J
pdq
= 2pi .
Hence if T (or ) is the period we have
2pi = = (t+ T ) (t) = [(t+ T ) + ] [t+ ] = T ,
so
=2pi
T,
thus can be identified as the (angular) frequency of the periodic motion.
So frequency may be obtained without finding a complete solution for the motion,once H is determined as a function of J .
Harmonic Oscillator
Frequency of the SHO using angleaction variables
H =p2
2m+
1
2m2q2 .
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HJ equation is
1
2m
(W
q
)2+
1
2m2q2 = E ,
so
J =1
2pi
pdq
=1
2pi
W
qdq
=
2m
2pi
dq 12m2q2 q =
2
m2sin
=
.
So
H = = J = HJ
= ,
as required.
6.4 f dof Conservative System
Need separable HJ equation W =
i Wi(qi, ~) as canonical transformation is thenseparable
pi =Wiqi
= pi = pi(qi, ~) .
so if we assume that the orbit equation of the projection of the system point on the(qi, pi) plane is periodic (ie libration or rotation), then we can define action variablesas for the 1-dof case. Hence, as previously
i =2pi
Ti.
Note that this does not imply that the system motion is periodic unless the fre-quencies are commensurate. (ie ratio of any two frequencies is a rational number, cfclosed Lissajous figures and open Lissajous figures.)
Define action variables
Ji =1
2pi
pi dqi , (no sum) .
Formal variation, not necessarily actual variation as in 1-dimensional case
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If a qi is cyclic then pi = constant orbit is horizontal straight line motion of arbitrary period
Since qi always an angle, then
Ji = pi , cyclic variables qi .
In general
Ji =1
2pi
Wi(qi, ~)
qidqi Ji(~) ,
are independent (from independence of separate variable pairs (qi, pi)) and somay be taken to be the new constant momenta.
Thus we may write
W =
fi=1
Wi(qi, ~J) , H = H( ~J) K .
Conjugate angle variables are
i =W
Ji=Wi(qi, ~J)
Ji,
and satisfy equation of motion
i =H
Ji= i( ~J) , or i = it+ i .
So are the (angular) frequencies of the motion. We see this from how the qsdepend on the s.
The change in i due to small changes in qs are
i =j
iqj
qj , cf virtual work with no time Goldstein p459
=j
2W
Jiqjqj
=
Ji
j
Wjqj
qj
=
Ji
j
pj(qj , ~J)qj .
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So total change in i when each qj is taken through (eg) mj cycles (libration orrotation) is
i =
Ji
j
mj
pj(qj , ~J) dqj integration over mj cycles
= 2pi
Ji
j
mjJj
= 2pimi ,
or
~ = 2pi~m ,
(so again, as before, we may identify i as angular frequencies).
6.4.1 Libration
Under a change ~ = 2pi~m, qs and ps all return to their initial values, ie qj is a
periodic function of ~.
qj =
k1=k1=
kf =kf=
aj~k( ~J) ei
~k~ ~k
aj~k( ~J) ei
~k~ ,
or
qj(t) =~k
aj~k( ~J) ei
~k(~t+~) .
Note that qj is not a periodic function of time unless js are commensurate. For if
qi(t+ T ) = qi(t) then ei~k~T = 1 or need
~T = 2pi ~N .
This can be solved if the ~s are commensurate, then
j = Ni orij
=NiNj
T = 2pi.
6.4.2 Rotation
Under one complete cycle (t t+ 2pi/j of the pair (qj , pj)) qj is increased by itsperiod q0j , j is increased by 2pi = qj (j/2pi)q0j returns to its initial value andso is periodic in ~. So as before we have
qj(t) =q0j2pi
(jt+ j) +~k
aj~k( ~J) ei
~k(~t+~) .
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6.5 The Kepler Problem using ActionAngle vari-
ables
V (r) = kr, (k > 0, bound state) .
1. k = GmM Gravitational (planets)
2. k = e1e24pi
Coulombe1 = e2 = e Hydrogen atom. With quantisation gives the Bohr atom.
In either case
~r = (r, 0, 0) , ~r = (r, r, r sin ) .
and
L = T V=
1
2m(r2 + r22 + r2 sin2 2) +
k
r.
Giving
pr =L
r= mr
p =L
= mr2
p =L
= mr2 sin = const. = Lz as is cyclic .
Thus
H = T + V
=1
2m
(p2r +
1
r2p2 +
1
r2 sin 2p2
) kr
= E = |E| < 0 as bound state .
The HJ equation is
1
2m
[(W
r
)2+
1
r2
(W
)2+
1
r2 sin2
(W
)2] kr= |E| .
Seek separated solution
W =Wr(r, ~) +W(, ~) +W(, ~) .
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As is cyclic, we have p = W/ = const. = . This gives(Wrr
)2+2r2
= 2m
(|E|+ k
r
)(W
)2+
2sin2
= 2
W
= .
What does represent?
~L = (r, 0, 0) (mr,mr,mr sin )=(0, p
sin , p
),
giving
~L2 = p2 +p2
sin2 =
(W
)2+
2sin2
= 2 ,
so AM magnitude is constant.
6.5.1 Actionangle variables
Jr =1
2pi
prdr =
1
2pi
Wrr
dr =1
2pi
2m
(|E|+ k
r
)
2
r2dr
J =1
2pi
pd =
1
2pi
W
d =1
2pi
2
2sin2
d
J =1
2pi
pd =
1
2pi
W
d = .
Integrating
Jr = + k2
2m
|E|J = J = ,
Trick for Jr:[See eg Goldstein for proof using contour integrals.]
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Integral easier to find if square root in denominator.
Jr|E| =
m
2pi2
r+r
rdr2m|E|r2 + 2mkr 2= 1
2pi
m
2|E| r+r
rdr(r r
)(r+ r)
,
(turning points on ellipse perihelion and apehelion are at r, r+ when pr vanishes).
Setting
r = 12(r+ + r) k
2|E| , =12(r+ r) .
Changing variables
r = r + cos ,
gives (r r)(r+ r) = 2 sin2 and r(pi) = r, r(0) = r+, so we have
Jr|E| =
1
pi
m
2|E| pi
0
(r + cos )d = k2
m
2
1
|E| 32 ,
and thus
Jr = const. +k
2
m
2|E| .
To determine the constant, consider a circular orbit, r = a, then pr = 0. So as
H =1
2m
(p2r +
2r2
),
then from Hamiltons equation
pr = Hr
= 2
mr3+
k
r2= 0 = a =
2
mk, and E = 1
2
mk2
2.
As in this case Jr = 0 (as pr = 0) then substituting E in the equation for Jr givesthe constant as .Trick for J:Use fact that motion is in a plane ~L = const. ([H, ~L] = 0 or d~L/dt = 0 or Lz = const.,z arbitrary.)
So in cylindrical coordinates (r, , z), z axis along ~L,
~L = (r, 0, 0) (mr,mr, 0) = mr2~ez ,
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