Stored magnetic energy of solenoid

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SUMMARY

The discussion focuses on the calculation of the stored magnetic energy in a solenoid, represented by the integral (1/2μ_0)∫B²dV. The integral is split into two regions: X, containing the solenoid, and Y, the surrounding space. By applying vector calculus identities and Ampere’s equation, the relationship between the magnetic field B and vector potential A is established. The final expression for the total magnetic energy incorporates contributions from both regions, emphasizing the significance of boundary conditions in the evaluation of the integral.

PREREQUISITES
  • Vector calculus, specifically the use of curl and divergence operators
  • Understanding of magnetic fields and vector potentials
  • Familiarity with Ampere's law and Gauss' theorem
  • Knowledge of electromagnetic theory, particularly in static fields
NEXT STEPS
  • Study the derivation of the vector potential A in electromagnetic theory
  • Explore the implications of Gauss' theorem in electromagnetic contexts
  • Learn about the applications of Ampere’s law in calculating magnetic fields
  • Investigate the energy density of magnetic fields in different geometries
USEFUL FOR

Physicists, electrical engineers, and students studying electromagnetism, particularly those interested in the energy storage capabilities of magnetic fields in solenoids.

Szecska8
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In my electrodynamics class there was a problem where self-inductance was calculated from the stored magnetic energy of the solenoid, which was calculated with the equation below.
Screenshot (62).png

Can someone explain to me what the second integral represents and what is A?
 
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Usually alphabet A is used for vector potential which generates magnetic field,
\nabla \times \mathbf{A}=\mathbf{B}
 
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The answer I got on reddit, that helped me understand it.

The total energy is given by

(1/2μ_0)∫B2dV

where the integral is taken over all space. Let us now split the space into a region X which contains the solenoid, and a region Y which is everything else. We can now write the integral as

∫B2dV=∫_X B2dV + ∫_Y B2dV

If you start from the vector calculus identity

∇•(AxB)=B•(∇xA)-A•(∇xB)

then insert the definition

∇xA=B

and Ampere’s equation

∇xB=μ_0j

which will be valid assuming static fields, you get

∇•(AxB)=B2-μ_0Aj

Outside the solenoid where there is zero current this simplifies to just

∇•(AxB)=B2

so by Gauss’ theorem we must have

∫_Y B2dV=∮_∂Y (AxB)•dS

Now the boundary ∂Y can be split into two contributions. The first is the boundary at infinity which does not contribute to the integral because the fields decay to zero sufficiently quickly. The second is the boundary shared with region X. This is exactly the same as the boundary of X with the exception that on ∂X the unit normal is oriented in the opposite direction since unit normals always point outwards. Thus

∮_∂Y (AxB)•dS=-∮_∂X (AxB)•dS

and therefore

∫B2dV=∫_X B2dV -∮_∂X (AxB)•dS
 
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