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This paper was written by D.J. Acheson while he was trying to give ...
In 1908 Stephenson found that the upper vertical position of the pe...
This paper is from 1993! I had thought it was much older on my firs...
As we can see in this video by Steve Mould the chain of pendulums c...
To prove this we are going to use the Lagrangian formulation and wi...
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Near $\alpha = 0$, $ \sqrt{-2\alpha} <\beta <0.450$. Since $\alpha_...
Also the larger the value of $N$, the smaller the value of $l$ beca...
A
pendulum
theoremt
BY
D.
J.
ACHESON
Jesus
College,
Oxford
OX1
3DW,
U.K.
We
consider N
linked
pendulums
which
are
inverted
and
balanced
on
top
of
one
another,
and
establish
a
general
theorem
which
shows
how
they may
be
stabilized
by
small vertical
oscillations
of
the
support.
1.
Introduction
Stephenson
(1908a,
b)
showed
that
it
is
possible
to
stabilize
a
single
rigid
pendulum
in
its
inverted,
or
upside-down,
equilibrium position
by
subjecting
the
pivot
to
small
vertical
oscillations
of
suitably
high
frequency.
He
confirmed
his
theoretical
predictions
by
a
practical
demonstration
of
the
phenomenon.
While
this
is
a
well-known
curiosity
of
classical
mechanics
it
does
not seem
to
be
generally
known
that
an
inverted
double,
or
even
triple
pendulum
can
be
stabilized
in
the same
way.
This
was,
again,
first
predicted
theoretically
by
Stephenson,
in
a
comparatively
overlooked
paper
of
1909,
though
the
idea
has
reappeared
in
a
number
of
subsequent
studies
(Lowenstern
1932;
Hsu
1961;
Kalmus
1970;
Otterbein
1982;
Leiber
&
Risken
1988).
Here
we
present
a
simple
but
general
theorem on
the
linear
stability
of
an
inverted
N-pendulum
of
any
kind.
The
generality
of
the theorem
is
achieved
by
relating
the
stability
question
to
just
two
elementary
properties
of
the
system
as
a
whole when
it
is
in
its
non-inverted,
or
downward-hanging,
state.
2.
The
stability
of
upside-down
pendulums
Theorem.
Let
N
pendulums
hang
down,
one
from
another,
under
gravity
g,
each
having
one
degree
of
freedom,
the
uppermost
being
suspended
from
a
pivot
point
O.
Let
O)max
and
wmin
denote
the
largest
and the
smallest
of
the
natural
frequencies
of
small
oscillation about
this
equilibrium
state.
Now
turn the
whole
system
upside-down.
The
resulting
configuration
of
the
pendulums
can
be stabilized
(according
to
linear
theory,
at
least)
if
we
subject
the
pivot
point
0
to
vertical
oscillations
of
suitable
amplitude
e
and
frequency
(o.
When
(O2
>
o)ax
the
stability
criterion
is
/V2g/oo
tmin
<
e
<
0.450g/2ma.
(2.1)
Note.
When
several
pendulums
are
involved,
T2ax
is
typically
much
greater
than
2i.
The
condition
o2
>
Omax
is
then
necessary
for
the
stability
of
the
inverted
state,
so
(2.1)
then
gives
the
whole
stability
region
in
the
e-o)0
plane,
as
in
figure
1.
t
This
paper
was
accepted
as
a
rapid
communication.
Proc. R.
Soc.
Lond.
A
(1993)
443,
239-245
?
1993
The
Royal
Society
Printed
in
Great
Britain
239
This content downloaded from 169.229.32.136 on Wed, 7 May 2014 15:58:31 PM
All use subject to
JSTOR Terms and Conditions
8*
?
Figure
1.
Typical
region
of linear
stability
for an
upside-down
N-pendulum,
as
given
by
(2.1).
Here
*
=
0.450
g/Oax
and
co
=
3.1432
ax/(min.
The
sketches
indicate theoretical
predictions
of
the
behaviour
just
outside
this
stability
region.
Thus,
if
at
a
given
frequency
w
the
amplitude
e
is
just
too
large,
the
system
is
unstable
to
rapidly
growing
buckling
oscillations
at
frequency
-o0.
If,
on
the
other
hand,
e
is
a
little
too
small,
the
pendulums
fall
over
comparatively
slowly,
keeping
to
the
same
side
of
the
vertical.
Proof.
Consider
first
small
disturbances
to
the
system
about
the
original,
i.e.
non-
inverted
equilibrium
state,
the
pivot point
0
being
fixed.
Let
the
natural
frequencies
be
oi,
and
let
Xi
be
the
corresponding
normal
coordinates,
each
of
which
will
be
some
linear
combination
of
the
(small)
angles
which
the
pendulums
make
with
the
downward
vertical.
We
then
have
Xi+?
Xi,=0,
i=l,...,N.
(2.2)
Now,
each
of
the
quantities
()2
will
be
simply
proportional
to
g;
this
follows from
the standard
theory
of
small
oscillations
based
on
Lagrange's
equations
of
motion
(see,
for
example,
Landau
&
Lifschitz
1976),
given
that
the uniform
gravitational
field
g
is
the
sole
source
of
potential
energy
in
this
problem.
If
we
tackle
the
stability
of
the
inverted
state
by
changing
the
sign
of
g
we
then find
that
small
disturbances
are
governed
instead
by
Xi-o
Xi
i=0,
i==l,...,N.
(2.3)
Suppose
now
that
the
pivot
point
0
oscillates
up
and
down
so
that
its
coordinate
in
the
direction
of
the
upward
vertical
is h
=
-ecoso0t.
We
may
allow
for
this
simply
by
replacing
g
in
the
above
argument
by
apparent
gravity
g
+h
=
g
+
e()
cos
o0
t.
In
this
way
we
find
that
X?--0~(?
1
+
(eo)/g)
coS
ot)Xi
=
0,
i
=
1,...,N.
On
introducing
the
scaling
T
=
(ot
we
therefore
obtain
N
uncoupled
Mathieu
equations:
d2Xi/dT2
+
(ci
+
ficosT)Xi
=
0,
i
=
1,...,N,
(2.4)
where
i
=-2/o2,
/=-i
=-
/g.
(2.5)
Proc.
R.
Soc. Lond.
A
(1993)
D.
J.
Acheson
240
This content downloaded from 169.229.32.136 on Wed, 7 May 2014 15:58:31 PM
All use subject to
JSTOR Terms and Conditions