Proof of the induced EMF formula E = ∫ (v × B) · dl

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phantomvommand
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TL;DR
Why is ##E = \int (\vec v \times \vec B) \cdot d \vec l##?
Why is ##E = \int (\vec v \times \vec B) \cdot d \vec l##? This seems to be a general formula, and I would like to know its proof.

Thanks for all the help.
 
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Are you familiar with the Lorentz force ?
Then the energy per unit charge (in SI units: Joule/Coulomb) follows from ##\int {\vec F\over q} \cdot d\vec l## .

PS it's a bit confusing to use the symbol ##E## for this; it's actually a potential difference (or emf)
$$\text {EMF} = V_{AB} = \int_A^B {\vec F\over q} \cdot d\vec l $$##\ ##
 
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BvU said:
Are you familiar with the Lorentz force ?
Then the energy per unit charge (in SI units: Joule/Coulomb) follows from ##\int \vec F \cdot d\vec l## .

##\ ##
Yes, I am. Thanks for the help, I never realized this connection. I suppose this formula can be used in general? Would I be more accurate to use a loop integral instead of an integral?
 
phantomvommand said:
Yes, I am. Thanks for the help, I never realized this connection. I suppose this formula can be used in general? Would I be more accurate to use a loop integral instead of an integral?
The expression is correct, so it should be universally applicable (but for a loop I expect to get 0 : ##\ V_{AA}\equiv 0## ) .

Check out a few of the sections in the link (Force on a current-carrying wire, EMF).

##\ ##
 
As anything in electrodynamics the formula can be derived from Maxwell's equations in differential form, which are always valid. Here one integrates Faraday's Law (in SI units)
$$\vec{\nabla} \times \vec{E}=-\partial_t \vec{B}$$
over a surface ##A## with boundary curve ##\partial A## with the usual orientation of the path given by the right-hand rule.
$$\int_A \mathrm{d}^2 \vec{f} \cdot \vec{\nabla} \times \vec{E}=\int_{\partial A} \mathrm{d} \vec{r} \cdot \vec{E}=-\int_A \mathrm{d}^2 \vec{f} \cdot \partial_t \vec{B}.$$
Now the usual integral form of Faraday's Law is written in terms of the magnetic flux
$$\Phi_{B}=\int_{A} \mathrm{d}^2 \vec{f} \cdot \vec{B}.$$
If now the surface ##A## and its boundary ##\partial A## are time-dependent you have to use Reynold's transport theorem for surface integrals to take the time derivative. Together with ##\vec{\nabla} \cdot \vec{B}## this leads to the ONLY generally correct form of Faraday's Law in integral form:
$$\mathcal{E}=\int_{\partial A} \mathrm{d} \vec{r} \cdot (\vec{E}+\vec{v} \times \vec{B})=-\dot{\Phi}_B=-\frac{\mathrm{d}}{\mathrm{d} t} \Phi_B.$$
For a derivation of the corresponding Reynold's transport theorem, see

https://en.wikipedia.org/wiki/Faraday's_law_of_induction#Proof
 
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