p=∫∂t∂x′∂E
Δp=∫E+ΔEE∂t∂x′∂E
As ΔE→0,
∂p∂E=∂t∂x′
and
∂E∂p=∂x′∂t=v
If the particle is in circular motion in B orbits, the centripetal force is provided by,
πE=πFq=πmv2qx
then
∂E∂v=2mvqx
Let,
p=2mvqx
such that,
∂E∂p=qx2m∂E∂v=v
Wait a minute, does not E depends on x? In this case the integral is taken over changing values of E. x may or may not change over the integral interval. It is not a variable that the integral is dependent on.
∂p∂E=2mqx∂v∂E=∂t∂x′
and so,
∫∂t∂x′∂E=∫2mqx∂v=2mqxv
From the previous post "Maybe Not",
∂B2∂t=−i2∫∂t∂x′∂E{∂2V∂x2}
∂B2∂t=−i22mqxv{∂2V∂x2}
12μo∂B2∂t=−i12μo22mqxv{∂2V∂x2}
12μo∂B2∂t=−i2mμoqxv{∂2V∂x2}
Let ψ=12μoB2=−12εoE2,
∂ψ∂t=−2mμoqx(iv){∂2V∂x2}
where iv is along the x direction. And x is the orbit of the particle.
This equation shows the rate of change in total energy required as a particle subjected to a B field and is in circular motion along the B field line attains a velocity v, perpendicular to its orbit at the present orbital radius of x.