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5.1.1 The Vector Potential

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Chapter 5. Magnetostatics

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5.4 Magnetic Vector Potential

5.1.1 The Vector Potential

In electrostatics,    E 0  Scalar potential (V) 0

    B

In magnetostatics, B   AVector potential (A)

E   V

So far, for a steady current where the Magnetic field is defined by the Biot-Savart law:

This Magnetic field given by the Biot-Savart law always satisfies the relations of

(as long as the current is steady, ) (always zero, even for not steady current)

/ 0

J

t

     

(If the current is not steady,  B0J0(D/t))

B

0

J

 

The relations of , called Ampere’s Law, is very useful, just like the Gauss’s Law in E.

The relations of is always satisfied for any current flow, therefore we may put the B field, either

B   A

( )

B   A   

(for any arbitrary vector A)

(for any arbitrary vector A and any scalar , since )

Or,    0

(Note) The name is “potential”, but A cannot be interpreted as potential energy per unit charge.

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 

2 0

B A A AJ

         

B    A WHY not ? B    ( A    )

B

0

J

 

Actually we want to use the Ampere’s Law, , to find out B field.

B    A (1) Let’s use the form of

2

A

0

J

  

If we choose A so as to eliminate the divergence of A:

   A 0

B

0

J

 

This is a Poisson’s equation.

We know how to solve it, just like the electrostatic potential problems.

2

A

0J

  

In summary, the definition B    A under the condition of    A 0

make it possible to transform the Ampere’s law into a Poisson’s equation on A and J !

If goes to zero at infinite,

If J goes to zero at infinite,

(If the current does not go to zero at infinite, we have to find other ways to get A.) If I goes to zero at infinite,

If K goes to zero at infinite, Ampere’s Law

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B    A WHY not ? B    ( A    )

(2) Now consider the other form,

B   (A  

)

Suppose that a vector potential A0satisfying B    A0, but it is not divergenceless,  A0  0.

If we add to A0 the gradient of any scalar , AA0  

since )

   0

0

(  A  

   AB

, A is also satisfied B    A.

The divergence of A is

     A A

0

 

2

We can accommodate the condition of

as long as a scalar function  can be found that satisfies,

   A 0    

2

A

0

But this is mathematically identical to Poisson's equation, thus

We can always find  to make

   A 0

 Therefore, let’s use the simple form of with the divergenceless vector potential, B    A

   A 0

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May we use a scalar potential, , just like used in ?

The introduction of Vector Potential (A) may not be as useful as V,

It is still a vector with many components.

It would be nice if we could get away with a scalar potential, for instant,

 But, this is incompatible with Ampere's law, since the curl of a gradient is always zero 

B   U B

0

J

 

0

B U

   

B   U E   V

 Such a magnetostatic scalar potential could be used,

if you stick scrupulously to simply-connected current-free regions (J = 0).

Suppose that .

Show, by applying Ampere's law to a path that starts at a and circles the wire returning to b

that the scalar potential cannot be single-valued, , even if they are the same point (a = b).

Prob. 5-29

B  U

(by the gradient theorem),

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The Vector Potential

Example 5.11

A spherical shell, of radius R, carrying a uniform surface charge , is set spinning at angular velocity .

Find the vector potential it produces at point r.

For surface current 

In fact the integration is easier if we let r lie on the z axis,

so that is tilted at an angle , and orient the x axis so that lies in the xz plane.

The velocity of a point r' in a rotating rigid body is

Since

Go back to the original coordinates, in which  coincides with the z axis and the position r is at

 Curiously, the field inside this spherical shell is uniform!

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The Vector Potential

Example 5.12

Find the vector potential of an infinite solenoid with n turns per unit length, radius R, and current I.

Since the current itself extends to infinity we cannot use such a form of

We need to use other methods. Here's a cute method that does the job:

 This means the flux of B through the loop.

To find B, we can use the Ampere’s law in integral form,

 Uniform longitudinal magnetic field inside the solenoid and no field outside) Using a circular "amperian loop" at radius s inside the solenoid,

Note that

For an amperian loop outside the solenoid, since no field out to R,

If so, we’re done.

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5.4.2 Summary; Relations of B – J – A

J

A

From just two experimental observations:

(1) the principle of superposition - a broad general rule

(2) Biot-Savert’s law - the fundamental law of magnetorostatics.

Poisson's equation Ampere’s Law

Stoke’s theorem

B – J – A

2

A

0J

  

  B

0

J

B   A

B

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E –– V B – J – A

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5.4.2 Summary; Magnetostatic Boundary Conditions

(Normal components)

(Tangential components)

For an amperian loop running perpendicular to the current,

For an amperian loop running parallel to the current,

Finally, we can summarize in a single formula:

The vector potential is continuous across any boundary:

(Because, guarantees the normal continuity; the tangential one.) (the flux through an amperian loop of vanishing thickness is zero)

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E  B Summary of Boundary conditions:

above below

VV A

above

A

below

Note that the derivative of vector potential A inherits the discontinuity of B Problem 5.32 (Prove it)

Because Aabove = Abelowat every point on the surface, it follows that are the same above and below.

Any discontinuity is confined to the normal derivative. z

x

Let’s take the Cartesian coordinates with z perpendicular to the surface and x parallel to the current.

KK x

y

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5.4.3 Multipole Expansion of the Vector Potential

If we want an approximate formula for the vector potential of a localized current distribution, valid at distant points, a multipole expansion is required.

(Eq. 3.94) Multipole expansion means

 to write the potential in the form of a power series in 1/r, if r is sufficiently large.

monopole dipole quadrupole

monopole dipole quadrupole

Just for comparison:

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Multipole Expansion of the Vector Potential

monopole dipole quadrupole

(Magnetic Monopole Term) Always zero!

 For the integral is just the total displacement around a closed path,

 This reflects the fact that there are (apparently) no magnetic monopoles in nature.

(Magnetic Dipole Term) It is dominant !

 Magnetic dipole moment

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Magnetic Dipole field

Magnetic dipole moment is independent of the choice of origin.

(Electric dipole moment was independent of the choice of origin, only when the total charge Q = 0)

 The Independence of origin for magnetic dipole moment is therefore corresponding to no magnetic monopole.

Magnetic field of a (pure) dipole moment placed at the origin.

Field B of a "pure" dipole Field B of a “physical" dipole

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