Is there a law that represents what acceleration the nuclear
force causes at a given radius? I tried to use the fact that a
particle travels in a hyperbola when it gets close to another
particle to derive what this force would be, but the calculations
become too complex to carry out (at least for anyone who doesn't
like to simplify 10 lines of r's and thetas). Is there a reasonably
elegant way to derive the laws from the hyperbola bit, or is there
a way to show the hyperbolic path from another well known
law?
Brad
I think you mean the electromagnetic force
between protons and protons (the hyperbolic orbits of electrons
were used by Faraday to deduce the existence of the nucleus).
Anyway the derivation that hyperbolic paths correspond to a
repulsive inverse square law, is essentially the same that
attractive inverse law gives elliptic orbits, which I think has
been covered on NRICH before, but I can't find the link, does
anyone know it?
Sean
[I can't find it either. - The
Editor]
Thanks. I think I know what to do with this now that I know the
inverse square part. Who would've guessed that the electromagnetic
force would be just the opposite of the gravitational force,
though!
Thanks again,
Brad
Yes, at one level it is a nice
coincidence. Note that the sign is the same if the charges are
opposite. There are deeper theoretical reasons why it is the sort
of law of you might expect, on hindsight. Also, the inverse square
law for electromagnetism is just a static approximation (once the
charges start moving there are relativistic effects, for instance
you cannot get stable orbits in EM like you can with gravity, which
is why people need QM to describe the atom). And Newtonian inverse
square law is a low speed, low mass approximation to GR, so in a
sense an inverse square law is something that comes out naturally
as certain limits. But in any case it is certainly a nice thing,
and it allows many computational techniques to be imported from one
area of physics to another.
Sean
When I do the math to find what the electromagnetic orbit should
be, I come up with the general form of
r=1/[A×sin(q+D)+(1/k2)]
for k=r2dq/dt
First off, D just determines the angle of view, so we may neglect
it. And, that formula seems to produce correct results so long
as
either 1/k2 or A is negative (but not both)
and so long as
|1/k2|<|A|.
But the problem comes when I start to think about what k and A
actually are. It would seem as though k=r0v0,
and then by substitution,
A=1/r0-1/(r0v0)2.
Clearly the two requirements cannot be met under these conditions.
Is there something wrong that I have done (I'd think that if there
was, it'd be in the r0v0 part)?
Thanks,
Brad
Firstly, if you have D'Inverno, this is
all done nicely (for the elliptic case) starting on page 192. I
think the answer you should get is
r = C/(1+ecos(q - q0))
Which is basically what you got. The criterion that makes it a
hyperbaloid is that e (called the eccentricity) is > 1 (this is
in fact your second criterion, your first is I think incorrect, in
fact they are both positive). C is positive. I'm pretty sure this
will work.
Sean
I had the first result because when both are positive or both
negative, a parabola or ellipse is produced, so for a hyperbola
(one that turns around before the origin), one must be negative and
the other positive. Anyway, I think I see the error in my logic. It
occurs in the substitutions in the third paragraph.
I'm having a bit of trouble with D'Inverno's notation; what does
the r with the ^ on top mean, with the dots? I know that
mr^ must = G, but it
obviously has more significance than this.
Brad
The dot means differentiation. The ^ means
unit vector, so for instance r^ is the vector r divided by its
modulus. So whilst a vector normally gives you a direction and a
magnitude, a vector with a hat on it just gives a direction.
The coefficients are always positive, for ellipses, hyperbolae or
parabolae. The point is that if e<1 then the expression is never
zero, so the orbit never goes to inifinity and it is closed, whilst
if e >= 1 then there is a point at which the denominator goes to
zero and so r goes to infinity, because the cosine (or sine) can be
negative.
Sean