Relativistic electron in static electric field

Hybird
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Homework Statement


Electron placed in static electric field \vec{E} = -\Psi\hat{x} , its initial velocity is 0. Calculate V(t).


Homework Equations



F_{e}=\frac{d}{dt}p(t)

p(t) = \gamma(t)mv(t)

Gamma is 1/sqrt(1-v^2/c^2) of course


The Attempt at a Solution



This is how I go about it and want to know if I'm on the right track.

i) First you multiply the electric field by the charge of an electron to get:

F_{e} = \frac{d}{dt}p(t) = e\Psi

ii) Then you integrate wrt time to get:

p(t) = e\Psit

iii) Then you relate momentum to velocity by:

p(t) = \gammamv(t)

iv) Finally you solve for V(t) from the above equation, expressing gamma explicitly I get the following formula:

v(t) = \frac{e{\Psi}t}{m}*\frac{1}{ {\sqrt{1+ {\frac{ e^{2}{\Psi}^{2}t^{2} }{ m^{2}c^{2} }} }} }

Does this seem to be the right method? I have to integrate this eventually to get x(t)..
 
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This doesn't seem right because V(t) is unbounded as t goes to infinity and thus we would pass the speed of light correct?
 
Hybird said:
This doesn't seem right because V(t) is unbounded as t goes to infinity and thus we would pass the speed of light correct?
No. This expression

Hybird said:
v(t) = \frac{e{\Psi}t}{m}*\frac{1}{ {\sqrt{1+ {\frac{ e^{2}{\Psi}^{2}t^{2} }{ m^{2}c^{2} }} }} }

approaches c as t goes to infinity.
 
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So maybe I am on the right track. Just curious, how do you get that limit? Do you have to binomial expand the square root?
 
Hybird said:
how do you get that limit? Do you have to binomial expand the square root?
I don't know what you mean by that, but probably not. After you do about 100 million of these kinds of limits, you just start to smell the approach. In this case, I just know that the other stuff under the radical will be much larger than 1, so I ignore the 1. The rest is straightforward. I think the more mathy way to do it is to divide top and bottom by t or something ...
 
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Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
The value of H equals ## 10^{3}## in natural units, According to : https://en.wikipedia.org/wiki/Natural_units, ## t \sim 10^{-21} sec = 10^{21} Hz ##, and since ## \text{GeV} \sim 10^{24} \text{Hz } ##, ## GeV \sim 10^{24} \times 10^{-21} = 10^3 ## in natural units. So is this conversion correct? Also in the above formula, can I convert H to that natural units , since it’s a constant, while keeping k in Hz ?
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