Relativistic Energy Derivation

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Calu
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Whilst reading following a derivation of the Relativistic Energy equation I came across the following:

d/dt[mu/(1-u2/c2)1/2] = [m/(1-u2/c2)3/2] du/dt.

I was wondering how that step was done.
 
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mfb said:
This is just the chain rule and then some simplifications.

I see it now, thanks.
 
Okay, so I now have:

d/dt[mu/(1-u2/c2)-1/2]

= m((1-u2/c2)-1/2) + mu(-u/c2).(1-u2/c2)-3/2

I'm not sure how to simplify from here, any hints?
 
I have no clue, how you came to this derivative. First write the whole thing a bit more clearly with LaTeX:
[tex]E=\frac{m c^2}{\sqrt{1-u^2/c^2}}.[/tex]
Here, [itex]m[/itex] is the invariant mass of the particle and [itex]u=|\vec{u}|[/itex] the usual (non-covariant) velocity with respect to the computational (inertial) frame.

Now taking the derivative with respect to time, you indeed just have to use the chain rule:
[tex]\frac{\mathrm{d} E}{\mathrm{d} t}=\frac{\mathrm{d} \vec{u}}{\mathrm{d} t} \cdot \vec{\nabla}_{u} E.[/tex]
 
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Derivation of Relative Energy Equation

I have no idea how to write in Latex, sorry, I'll type out the entire thing:

Assume m and c are constants.

W = ∫x2x1 F . dx = ∫x2x1 dp/dt . dx

dp/dt = d/dt [mu . (1-u2/c2)-1/2]

by the product rule:

dp/dt = m(1-u2/c)-1/2) + mu.(1-u2/c)-3/2 . (-u/c2)

Then as γ = (1-u2/c)1/2

dp/dt = m (γ - u/c23))

I'm not sure how to simplify to get the intended answer of m(1-u2/c)-3/2 . du/dt
 
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You've differentiated with respect to u, not with respect to t.
Well that is easy to fix as m and c do not depend on t, but it is important to get it right.

You can combine both fractions to a single one if you expand the first one (the one that gives γ). Then simplify and you get the right result.
 
What do you mean by expand? Sorry I'm very confused.
 
@vela: Which factor of 2?

Calu said:
What do you mean by expand? Sorry I'm very confused.
Expand the fraction

Combining two fractions to a single one is taught several years before special relativity, you should know how to do that.
 
mfb said:
@vela: Which factor of 2?

Expand the fraction

Combining two fractions to a single one is taught several years before special relativity, you should know how to do that.

Oh I see, we don't call that "expanding" a fraction, sorry for the confusion.

Also I edited the post because I thought it easier just to continue with what we had.

EDIT: I'm sorry but could you help me out? I'm not sure what I'm meant to do. And as far as I know we have been taught little about "expanding" fractions as we are usually told to simplify (reduce) them. I can't think of a time I've been asked to do the opposite. Usually to combine 2 fractions I would cross multiply to get a common denominator.

Let me just step away from this a second, because I have done the above (cross multiplied and found a common denominator) and have arrived at an answer similar to one I arrived at earlier but decided I could go no further.

The answer I have is as follows:

dp/dt = m [γ - u2/c23)]

Is there a way to take out a factor of (1-u2/c2) (i.e. γ2) from this? Or am I completely wrong?

And I'll post my result from combining the fractions:

[m(1-u2/c2)3/2) - m(u2/cc)(1-u2/c2)1/2)] / (1-u2/c2)2

Which when we replace with γ is:

m(γ3 - (u2/c2)γ)

which as I said is similar to the answer I got earlier.
 
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Calu said:
The answer I have is as follows:

dp/dt = m [γ - u2/c23)]

Is there a way to take out a factor of (1-u2/c2) (i.e. γ2) from this?
First take a factor of ##\gamma## outside. Then rewrite the ##\gamma## that remains on the inside in terms of u. Then simplify and think about what the simplified result looks like.

Edit: I don't think that minus sign is correct.
 
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Right, so I finally did this after going back and differentiating wrt t as I was supposed to.

d/dt [mu(1-u2/c2)-1/2]

= m.du/dt.(1-u2/c2)-1/2 + (-1/2)mu((1-u2/c2)-3/2.2u/c2.du/dt

=m.du/dt.(1-u2/c2)-1/2 + u2/c2.m.((1-u2/c2)-3/2.du/dt

= m(1-u2/c2 + u2/c2)(1-u2/c2)-3/2).du/dt

=m(1-u2/c2)-3/2).du/dt as required.

Also, how would I solve:

m ∫uo [u(1-u2/c2)-3/2] . du

Would it be integration by parts?
 
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Looks good except that in the second line, 2u/c^2 should be (-2u/c^2), and there's also a left parenthesis too many.

No need to use integration by parts. You're supposed to write the integrand in a form that enables you to just use the formula ##\int_a^b f'(x)dx=f(b)-f(a)##.

The work can be expressed as ##\int_0^u mu\gamma^3\mathrm du## or as ##\int_0^t mu\gamma^3\dot u\mathrm dt##. Does either of the integrands look like a derivative?
 
I'm not sure how you would decide whether something "looks like" a derivative.
 
I managed to perform the integration by using a substitution of z = 1 - u2/c2.

I still don't see how either is equivalent to a derivative I calculated earlier though.
 
OK, I see that it's more difficult to see in your approach than in the one I've been using (because mine involves a calculation of ##\dot\gamma##):
\begin{align}
&\dot\gamma =\gamma^3u\dot u\\
&\dot p=\frac{d}{dt}(\gamma m u) =\dot\gamma m u+\gamma m\dot u =\dots=\gamma^3m\dot u\\
&W=\int F\mathrm dx =\int \frac{dp}{dt}u\mathrm dt =\int\gamma^3 m\dot u u\mathrm dt =\int\frac{d}{dt}(m\gamma)\mathrm dt.
\end{align} I have done this calculation a few times before, but it has actually never occurred to me that you can finish it with a simple variable substitution.

Edit: Here's another way:
$$W=\int \frac{dp}{dt}u\mathrm du =\int\gamma^3 m u\mathrm du =\int\frac{d}{du}(m\gamma)\mathrm du.$$
 
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Oh yes that makes a lot more sense now. Thanks very much to all of you!