Apparently this 2nd-order ODE has 3 solutions?

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Discussion Overview

The discussion revolves around a second-order ordinary differential equation (ODE) related to motion in polar coordinates under a central force. Participants explore the nature of the solutions to the equation, which is proposed to have three solutions, and seek to understand how to derive these additional solutions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant presents the ODE and suggests that it has three solutions, including a specific exponential form for one solution.
  • Another participant questions the form of the function f and proposes an alternative interpretation of the equation, leading to a different simplification and solution form.
  • A third participant elaborates on the physical context of the ODE, relating it to Newton's laws and central forces, and expresses confusion about finding additional solutions.
  • Several participants discuss the general properties of second-order linear differential equations, noting that they typically have two linearly independent solutions unless specific conditions are met.
  • One participant emphasizes the need for boundary conditions to determine unique solutions and mentions the existence and uniqueness theorem in relation to ODEs.
  • Another participant suggests using the reduction of order method to find additional solutions if one solution is already known.

Areas of Agreement / Disagreement

There is no consensus on the number of solutions to the ODE, as some participants assert that there should only be two solutions based on standard theory, while others argue for the existence of a third solution under specific conditions. The discussion remains unresolved regarding the nature and derivation of the additional solutions.

Contextual Notes

Participants express uncertainty about the function f and its implications for the ODE. There are also discussions about the completeness of the problem and the necessity of boundary conditions for determining unique solutions.

Farina
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Apparently this 2nd-order ODE has 3 solutions??

The following apparently has 3 solultions:

[tex] \frac {d^2u}{d\theta^2} + u = -\frac {1}{ml^2u^2}f(u^{-1})[/tex]

where:

u = 1/r
m = mass
l = angular momentum

One of the solutions is:

[tex]r=r_0e^{k\theta} \text{ where } \theta \text { varies logarithmically with time}[/tex]

Apparently there are also 2 additional solutions (depending on the value of the constant [tex]\alpha[/tex])
that could be in the form of:

[tex]r=Ae^{\sqrt{\alpha x}}+Be^{-\sqrt{\alpha x}} \text{ or }[/tex]
[tex]r=A\theta + B \text{ or }[/tex]
[tex]r=Asin({\sqrt{\alpha x}})+Bcos({\sqrt{\alpha x}})[/tex]

So, knowing:

[tex] \frac {d^2u}{d\theta^2} + u = -\frac {1}{ml^2u^2}f(u^{-1})[/tex]

and

[tex]r=r_0e^{k\theta}[/tex]

How does one specifically determine the equations of the additional solutions?

Thanks!
 
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Farina said:
The following apparently has 3 solultions:

[tex] \frac {d^2u}{d\theta^2} + u = -\frac {1}{ml^2u^2}f(u^{-1})[/tex]

I saw your other post, and really wasn't able to understand the equation. What function is [tex]f[/tex]?

Something like:

[tex] \frac {d^2}{d\theta^2}u(\theta)^2+ u(\theta) = -\frac {1}{ml^2u(\theta)^2}[/tex]

Makes more sense, but if you plug in [tex]u(\theta)=\cos \theta[/tex] which represents a solution to your original problem you get:
[tex]-\cos \theta + \cos \theta = k \sec(\theta)^2[/tex]
or
[tex]0 = k \sec(\theta)^2[/tex]
which is...problematic.

Perhaps you mean that [tex]f(u^{-1})=f(r)=-\frac{1}{r^3}=-u^3[/tex]
then your equation simplifies to:
[tex] \frac {d^2}{d\theta^2}u(\theta)^2+ u(\theta) = \frac {u(\theta)}{ml^2}[/tex]
or
[tex]\frac{d^2}{d\theta^2}u(\theta)^2 + (1-\frac{1}{ml^2}) u(\theta)=0[/tex]
which has solutions of the form
[tex]u(\theta)=k_1e^{i(\theta)\sqrt{1-\frac{1}{ml^2}}}[/tex]
so
[tex]r(\theta)=k e^{-i(\theta) \sqrt{(1-\frac{1}{ml^2}}}[/tex]
It's relatively easy to see that if [tex]1-\frac{1}{ml^2} < 0[/tex] the functions are not orbits.
 
I think you've addressed this NateTG, but I still
have some digesting to do...

The following is basically Newton's DE of motion using two-dimensional polar coordinates instead of three:

[tex] \frac {d^2u}{d\theta^2} + u = -\frac {1}{ml^2u^2}f(u^{-1})[/tex]

where:

u = 1/r
m = mass
l = angular momentum
[tex]f(u^{-1}) \text { = the central force}[/tex]

And, yes, l = angular momentum per unit mass (thanks ehild!).

There is a fair amount of derivation provided in the text. The DE is labled as "the differential equation of the orbit of a particle moving under a central force."

Setting u = 1/r you thus have:

[tex]u={r_0}^{-1}e^{-k\theta}[/tex]

Referring back to the DE and using

[tex]\text{u, } \frac {d^2u}{d\theta^2}[/tex]

then simply re-arranging and solving algebraically
for [tex]f(u^{-1} )[/tex] you get

[tex]f(r)=-(k^2+1)ml^2\cdot \frac {1}{r^3}[/tex]

which shows that the central field corresponds to an inverse-cube force.

I'm stuck at the proposition of having to find two other types of possible orbits (and their equations). I was thinking it was a simple matter of expressing the solution to the DE in basic alternative forms -- but maybe not??

NateTG said:
I saw your other post, and really wasn't able to understand the equation. What function is [tex]f[/tex]?

Something like:

[tex] \frac {d^2}{d\theta^2}u(\theta)^2+ u(\theta) = -\frac {1}{ml^2u(\theta)^2}[/tex]

Makes more sense, but if you plug in [tex]u(\theta)=\cos \theta[/tex] which represents a solution to your original problem you get:
[tex]-\cos \theta + \cos \theta = k \sec(\theta)^2[/tex]
or
[tex]0 = k \sec(\theta)^2[/tex]
which is...problematic.

Perhaps you mean that [tex]f(u^{-1})=f(r)=-\frac{1}{r^3}=-u^3[/tex]
then your equation simplifies to:
[tex] \frac {d^2}{d\theta^2}u(\theta)^2+ u(\theta) = \frac {u(\theta)}{ml^2}[/tex]
or
[tex]\frac{d^2}{d\theta^2}u(\theta)^2 + (1-\frac{1}{ml^2}) u(\theta)=0[/tex]
which has solutions of the form
[tex]u(\theta)=k_1e^{i(\theta)\sqrt{1-\frac{1}{ml^2}}}[/tex]
so
[tex]r(\theta)=k e^{-i(\theta) \sqrt{(1-\frac{1}{ml^2}}}[/tex]
It's relatively easy to see that if [tex]1-\frac{1}{ml^2} < 0[/tex] the functions are not orbits.
 
If the diff. equation is of the form au'' + bu' + cu = 0, then shouldn't it only have two possible solutions? Unless of course you are cosidering u = 0 a solution.
 
e(ho0n3 said:
If the diff. equation is of the form au'' + bu' + cu = 0, then shouldn't it only have two possible solutions? Unless of course you are cosidering u = 0 a solution.

I was thinking the same thing, but I also seem to
remember that DE of this form have a bunch of solutions
based on the sign of a combination of constants.

I guess I need to refresh my working knowledge of DE.
 
e(ho0n3 said:
If the diff. equation is of the form au'' + bu' + cu = 0, then shouldn't it only have two possible solutions? Unless of course you are cosidering u = 0 a solution.

Your problem is incomplete. You need two boundary conditions in order to set a unique solution for the ode. Also you need to consider under which circumstances au'' + bu' + cu = 0 + (boundary conditions) has a solution and if this solution is unique. (Existence and Uniqueness Theory).

In the case that au'' + bu' + cu = 0 + (boundary conditions) satisfies the uniqueness and existence theorem, the there is only two l.i. solutions to the ode.

On relation to 1 If you already founded a solution, use the reduction of order method to find the second solution ie
[tex]y_{2}(x)=v(x)y_{1}(x)[/tex]
 
Last edited:

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