Ampere's Law For Static Magnetic Field

  • #1
BlackMelon
43
7
Hi there!

Please refer to the picture below. I would like to understand the equation Curl(H) = J, where H is the magnetic field intensity and J is the current density. So, I inspect a simple problem.
There is a wire carrying current I in the z-axis direction. a_r, a_phi, and a_z are the unit vectors in the directions of the radius, the tangential line, and z-axis, respectively.

So, from H = I/(2*pi*r)a_phi. I take the curl of this vector (in cylindrical coordinate) and got 0. How does this relate to the current density?

Best
BlackMelon

1695964252946.jpeg
 
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  • #2
The field you've written down is the field outside a current carrying wire. What would you expect for the current density outside a wire?
 
  • #3
Ibix said:
The field you've written down is the field outside a current carrying wire. What would you expect for the current density outside a wire?
Oh well it's zero. That was the silly of me LOL. Thank you very much.

By the way, I have analyzed the inside of the wire H = I*r/(2*pi*R^2) a_phi.
where r is the radius from the center of the wire to the point of interest. R is the radius of the wire. And got the correct answer:
J = curl (H) = I/(pi*R^2) a_z

1695975871845.png
 
  • Like
Likes Dale and Ibix
  • #4
Adding more information to my previous comment, here is how I calculate the current density inside the wire using curl(H) = J
1696130017446.png
 
  • Like
Likes Dale
  • #5
The solution in local form is indeed given by using the magnetostatic Maxwell equations as follows:
$$\vec{\nabla} \cdot \vec{B}=0, \quad \vec{\nabla} \times \vec{B}=\mu_0 \vec{j}.$$
We have given
$$\vec{j}=\begin{cases}\frac{I}{\pi R^2} \vec{e}_z &\text{for} \quad \rho \leq R \\ 0 &\text{for} \quad \rho>R. \end{cases}$$
To solve this equations it's most simple to make the ansatz
$$\vec{B}=B(\rho) \vec{e}_{\varphi}.$$
Using the formula for the curl in cylinder coordinates you get
$$\vec{\nabla} \times \vec{B}=\frac{1}{\rho} \partial_{\rho} (\rho B) \vec{e}_z.$$
From this you get for ##\rho<R:##
$$\partial_{\rho} (\rho B)=\frac{\mu_0 I}{\pi R^2} \rho.$$
This can be immediately integrated to
$$B(\rho)=\frac{\mu_0 I}{2 \pi R^2}\rho + \frac{C}{\rho},$$
where ##C## is an integration constant. Since there's no singularity at ##\rho=0##, you get ##C=0##, i.e.,
$$B(\rho)=\frac{\mu_0 I}{2 \pi R^2}\rho \quad \text{for} \quad \rho<R.$$
For ##\rho \geq R## you have
$$\partial_{\rho} (\rho B)=0 \; \rightarrow \; B=\frac{B_0}{\rho} \quad \text{with} \quad B_0=\text{const}.$$
Now, at ##\rho=R##, ##B## must be continuous, which gives
$$B(\rho)=\frac{\mu_0 I}{2 \pi \rho} \quad \text{for} \quad \rho \geq R.$$
One should also check that ##\vec{\nabla} \cdot \vec{B}=0##, which however is already seen easily to be fufilled by the initial general ansatz.
 
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Likes BlackMelon
  • #6
vanhees71 said:
The solution in local form is indeed given by using the magnetostatic Maxwell equations as follows:
$$\vec{\nabla} \cdot \vec{B}=0, \quad \vec{\nabla} \times \vec{B}=\mu_0 \vec{j}.$$
We have given
$$\vec{j}=\begin{cases}\frac{I}{\pi R^2} \vec{e}_z &\text{for} \quad \rho \leq R \\ 0 &\text{for} \quad \rho>R. \end{cases}$$
To solve this equations it's most simple to make the ansatz
$$\vec{B}=B(\rho) \vec{e}_{\varphi}.$$
Using the formula for the curl in cylinder coordinates you get
$$\vec{\nabla} \times \vec{B}=\frac{1}{\rho} \partial_{\rho} (\rho B) \vec{e}_z.$$
From this you get for ##\rho<R:##
$$\partial_{\rho} (\rho B)=\frac{\mu_0 I}{\pi R^2} \rho.$$
This can be immediately integrated to
$$B(\rho)=\frac{\mu_0 I}{2 \pi R^2}\rho + \frac{C}{\rho},$$
where ##C## is an integration constant. Since there's no singularity at ##\rho=0##, you get ##C=0##, i.e.,
$$B(\rho)=\frac{\mu_0 I}{2 \pi R^2}\rho \quad \text{for} \quad \rho<R.$$
For ##\rho \geq R## you have
$$\partial_{\rho} (\rho B)=0 \; \rightarrow \; B=\frac{B_0}{\rho} \quad \text{with} \quad B_0=\text{const}.$$
Now, at ##\rho=R##, ##B## must be continuous, which gives
$$B(\rho)=\frac{\mu_0 I}{2 \pi \rho} \quad \text{for} \quad \rho \geq R.$$
One should also check that ##\vec{\nabla} \cdot \vec{B}=0##, which however is already seen easily to be fufilled by the initial general ansatz.
Thank you very much for the explanation :)
 

Related to Ampere's Law For Static Magnetic Field

What is Ampere's Law for static magnetic fields?

Ampere's Law for static magnetic fields states that the line integral of the magnetic field B around a closed loop is equal to the permeability of free space (μ₀) times the total current I passing through the loop. Mathematically, it is expressed as ∮ B · dl = μ₀I, where the integral is taken over a closed path.

How is Ampere's Law derived?

Ampere's Law can be derived from the Biot-Savart Law, which describes the magnetic field generated by a steady current. By considering the contributions of infinitesimal current elements and summing them over a closed loop, one can derive the integral form of Ampere's Law. Additionally, it can be derived from Maxwell's equations, specifically from the curl of the magnetic field equation.

What are the applications of Ampere's Law?

Ampere's Law is used in various applications to calculate magnetic fields in systems with high symmetry, such as solenoids, toroids, and coaxial cables. It simplifies the calculation of magnetic fields in these configurations by allowing the use of symmetry arguments to evaluate the line integral more easily.

What are the limitations of Ampere's Law?

Ampere's Law is primarily applicable to static or steady-state magnetic fields and does not account for time-varying fields. For dynamic fields, the full set of Maxwell's equations, including the displacement current term, must be used. Additionally, Ampere's Law is most useful in situations with high symmetry; in more complex geometries, it may be challenging to apply directly.

How does Ampere's Law relate to Maxwell's equations?

Ampere's Law is one of the four Maxwell's equations, which form the foundation of classical electromagnetism. In its generalized form, Ampere's Law includes the displacement current term and is written as ∮ B · dl = μ₀(I + ε₀ dΦ_E/dt), where ε₀ is the permittivity of free space and dΦ_E/dt is the rate of change of electric flux. This generalized form accounts for both steady and time-varying fields.

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