WolfOfTheSteps
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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 centripital 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!