Faculty of Engineering and Applied Science
2007 Fall
Use the method of Gaussian elimination to solve the linear system
which obviously has the unique solution
[Note that one cannot simply drop the fourth row and
reduce the resulting square 3×3 matrix.
One must guard against the possibility of an
inconsistent system (which has no solution at all).]
A pair of simultaneous first order ODEs is defined by
Near any critical point (a, b), the
non-linear system may be approximated by the linear system
Near (0, 0):
The eigenvalues are of opposite sign. This critical
point is therefore a
saddle point |
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(which is automatically unstable).
Near (-4, 0):
The eigenvalues are a pure imaginary pair. For the
linear approximation, this critical point is a centre.
The corresponding critical point in the original non-linear
system could therefore be any of a stable focus, a centre
or an unstable focus.
However, the non-linear system of first order ODEs can be
rewritten as the single second order ODE
which has no damping term (first derivative).
It is therefore likely that the critical point at
(-4, 0), in the non-linear system, is
also a
centre |
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(which is automatically stable but not asymptotically stable).
For the centre, the orientation of the trajectories
is easily determined to be clockwise, upon noting that
For the saddle point, the exact equations of the asymptotes
were not required. Again, the directions of the
trajectories are determined by the fact that all
trajectories must move to the right above the
x axis and to the left below it.
The equations of the asymptotes can be found from the
eigenvectors of the linear system:
The equations of the asymptotes are therefore
.
BONUS QUESTION
All trajectories are solutions to the differential
equation
Separating the variables,
The separatrix divides the region of closed orbits about
the centre from the open trajectories further away.
The separatrix passes through the saddle point.
Therefore the point (0, 0) must be on the separatrix.
In simplified form, the equation of the separatrix is therefore
To find all x axis intercepts for the separatrix:
The intercepts are therefore at
A function f (x) is defined by
f (x) is monotonically increasing. [If an accurate sketch or plot is available, then |
|
xn | ![]() |
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-0.500 000 000 | +0.481 530 660 | +1.356 530 660 | -0.354 972 190 |
-0.854 972 190 | -0.199 670 370 | +2.618 227 358 | +0.076 261 662 |
-0.778 710 528 | -0.013 204 851 | +2.278 167 754 | +0.005 796 259 |
-0.772 914 269 | -0.000 070 566 | +2.253 855 090 | +0.000 031 309 |
-0.772 882 960 | -0.000 000 002 |
[An Excel spreadsheet for this question is available here. It allows you to experiment with various choices of x0.]
Find the path y = f (x) between the points (0, 1) and (1, 1) for which the integral
has an extremum and determine whether the extremum is a maximum or a minimum.
The Euler-Lagrange equation
becomes
But this path must pass through both (0, 1) and (1, 1):
Therefore the extremal to the functional I is
Evaluating the integrand at the only extremum,
We need to compare this value of the integral to the value along
any other path.
The simplest path between two points is a straight line.
The straight-line path through (0, 1) and (1, 1) is
y = 1.
The value of I along this other path is
Therefore the extremum of I is a
minimum. |
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Find the Fourier series expansion of the function
f (x) is an even function of
x
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An arbitrary purely radial vector field F may be
defined in spherical polar coordinates by
,
where f (r) is some
differentiable function of the distance r
from the origin.
But f (r) is a function of
r only. Therefore
(where k is a constant).
Therefore, in order for a purely radial vector field to be
source free (zero divergence) everywhere (except possibly
at the origin), f (r) must
have the functional form
[Note that the central force laws of nature, the gravitational and electrostatic forces, are both of this type.]