Stored magnetic energy of solenoid

In summary, The second integral represents the total energy given by the magnetic field, where the space is split into regions X and Y. The integral over Y is simplified by using the vector calculus identity and Ampere's equation, and the boundary ∂Y can be split into two contributions. The alphabet A is used for the vector potential A which generates the magnetic field.
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Szecska8
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TL;DR Summary
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,
[tex]\nabla \times \mathbf{A}=\mathbf{B}[/tex]
 
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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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FAQ: Stored magnetic energy of solenoid

What is the formula for the stored magnetic energy in a solenoid?

The stored magnetic energy (U) in a solenoid can be calculated using the formula: \( U = \frac{1}{2} L I^2 \), where \( L \) is the inductance of the solenoid and \( I \) is the current passing through it.

How do you calculate the inductance of a solenoid?

The inductance (L) of a solenoid can be calculated using the formula: \( L = \mu_0 \mu_r \frac{N^2 A}{l} \), where \( \mu_0 \) is the permeability of free space, \( \mu_r \) is the relative permeability of the core material, \( N \) is the number of turns, \( A \) is the cross-sectional area of the solenoid, and \( l \) is the length of the solenoid.

What factors affect the stored magnetic energy in a solenoid?

The stored magnetic energy in a solenoid is affected by the inductance (L) of the solenoid and the current (I) passing through it. The inductance itself depends on factors such as the number of turns (N), the cross-sectional area (A), the length (l) of the solenoid, and the permeability (\( \mu_0 \) and \( \mu_r \)) of the core material.

Why is the stored magnetic energy in a solenoid important?

The stored magnetic energy in a solenoid is important because it represents the energy that can be used to perform work, such as moving a magnetic core or generating electromagnetic fields. This energy is crucial in applications like inductors, transformers, electromagnets, and various types of sensors and actuators.

Can the stored magnetic energy in a solenoid be increased?

Yes, the stored magnetic energy in a solenoid can be increased by either increasing the inductance (L) of the solenoid or increasing the current (I) passing through it. This can be achieved by increasing the number of turns (N), using a core material with higher permeability (\( \mu_r \)), increasing the cross-sectional area (A), or increasing the current supply.

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