How Long Would an Electron Take to Spiral into the Nucleus?

  • Thread starter Thread starter WolfOfTheSteps
  • Start date Start date
  • Tags Tags
    Electron Orbit
Click For Summary

Homework Help Overview

The discussion revolves around the classical mechanics of an electron in circular orbit around a proton, specifically focusing on the time it would take for the electron to spiral into the nucleus due to energy radiation as described by the Larmor formula. The original poster considers the implications of centripetal acceleration and energy loss in this context.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to calculate centripetal acceleration and considers whether to treat it as constant or to integrate it over the distance to the nucleus. Some participants question the validity of their approach and explore the relationship between energy, acceleration, and time.

Discussion Status

Participants are actively engaging with the problem, suggesting various methods to express energy as a function of radius and differentiate it with respect to time. There is a recognition of the complexity involved in the integration process and the implications of treating variables as functions of time.

Contextual Notes

There is an acknowledgment of the challenges posed by the infinite nature of certain integrals and the need to consider the electron's position as a function of time. The discussion reflects on the assumptions made regarding the nucleus as a point charge and the implications for the calculations involved.

WolfOfTheSteps
Messages
134
Reaction score
0

Homework Statement



Since an electron on a circular orbit around a proton has a centripetal acceleration, it should radiate energy according to the Larmor relation

\frac{dE}{dt} = -2/3(q^2/4\pi\epsilon_o)(a^2/c^3)

where q, a, \epsilon_o and c are respectively the electron charge, its acceleration, the vacuum permittivity and the velocity of light in a vacuum. Therefore, in classical, mechanics, it should spiral and crash on the nucleus. How long would this decay take, supposing that the size of the initial orbit is 10^{-10}m and the nucleus is a point charge (radius=0)?

Homework Equations



a = \frac{F_{coulombic}}{m} = \frac{v^2}{r_n} = \frac{1}{m} \frac{q^2}{4 \pi \epsilon_o r^2_n}

The Attempt at a Solution



I can easily do this if I calculate the centripetal acceleration, a, out at 10^{-10}m, and treat it as constant in the Larmor relation.

My question is, do you think this is what the problem wants me to do? Or do you think I have to set up an integral somewhere to vary the acceleration with the distance from the nucleus?

I tried getting a function a(r) by integrating a with respect to r from r=0 to r=10^{-10}m, but then I realized that the integral would be infinite, since r is in the denominator. Which makes me think they want me to treat a as a constant.

Any ideas or thoughts?

Thanks!
 
Physics news on Phys.org
My last paragraph was really stupid. a is already a function of r. I did try to find the average acceleration by integrating from 0 to r and dividing by r. But of course the integral is infinite, and that's the problem.
 
Try this: First express E as a function of radius. Then take the derivative with respect to time and set it equal to the Larmor formula; integrate to find time.
 
Awesome! That definitely makes sense, and I wish I would have thought of it!

Thanks, Doc Al.
 
Doc Al said:
Try this: First express E as a function of radius. Then take the derivative with respect to time and set it equal to the Larmor formula; integrate to find time.

Doc Al,

But if you have E as a function of radius, and you differentiate with respect to time, you get 0, since there is no t in that function. Is this what you intended?
 
Wolf of the Ste said:
Doc Al,

But if you have E as a function of radius, and you differentiate with respect to time, you get 0, since there is no t in that function. Is this what you intended?

Your speed "v" is an implicit function of time, and r is a function of time as well.
 
Perhaps it would be helpful to note that;

v = \frac{ds}{dt} = 2\pi\cdot\frac{dr}{dt}

Edit: Dammit patrick
 
Is this the idea?

<br /> <br /> \textnormal{Let A, B, and C be the product of the constants in the functions E, a, and dE/dt respectively. Then,} \\<br />

<br /> E = \frac{-A}{r} \ \textnormal{(1)}\\<br />

<br /> a = \frac{B}{r^2} \ \textnormal{(2)}\\<br />

<br /> \frac{dE}{dt} = C a^2 = \frac{C B^2}{r^4}\ \textnormal{(3)} \ \textnormal{(Lamar Relation)} \\<br />

<br /> \textnormal{Then, using (1)}, \\<br />

<br /> \frac{dE}{dt} = \frac{A}{r^2} \frac{dr}{dt} \textnormal{(4)} \\<br />

<br /> \textnormal{Setting (3) and (4) equal, we get:} \\<br />

<br /> \frac{A}{r^2} \frac{dr}{dt} = \frac{C B^2}{r^4} \\<br />

<br /> A r^2 dr = C B^2 dt \\<br />

<br /> \int{A r^2}dr = \int{C B^2}dt \\<br />

<br /> \frac{A}{3} r^3 = C B^2 t \\<br />

<br /> t = \frac{A r^3}{3C B^2} \\<br />So is this a valid expression for time t needed for the electron to crash into the point nucleus, given an initial distance, r, from the point nucleus??

Thanks.
 
Last edited:
Wolf of the Ste said:
Doc Al,

But if you have E as a function of radius, and you differentiate with respect to time, you get 0, since there is no t in that function. Is this what you intended?
Since the electron is crashing into the nucleus, r must be a function of time and thus E is a function of time (as noted by nrqed and Hoot). If
E = E(r)

Then
dE/dt = E&#039;(r) dr/dt

Start by finding E(r) explicitly, where E is the total energy. (Use the Bohr model.)


Wolf of the Ste said:
Is this the idea?

...
Exactly!
 
  • #10
Thanks again. I'm finished, at last! :)
 

Similar threads

Replies
1
Views
2K
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
13
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 7 ·
Replies
7
Views
3K
Replies
4
Views
2K
  • · Replies 23 ·
Replies
23
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 16 ·
Replies
16
Views
2K