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Griffiths Chapter 7

This document provides an example problem and explanation of calculating the induced electric field from a long straight wire with a time-dependent current using the quasistatic approximation. It summarizes the steps as: 1) Use Ampere's law to find the magnetic field B(t). 2) Use this to find the magnetic flux Φ and its time derivative dΦ/dt. 3) Apply Faraday's law to find the induced electric field E(t). It notes that this approximation is valid when changes occur sufficiently slowly compared to the speed of light and observers are sufficiently close to the wire.

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0% found this document useful (0 votes)
392 views37 pages

Griffiths Chapter 7

This document provides an example problem and explanation of calculating the induced electric field from a long straight wire with a time-dependent current using the quasistatic approximation. It summarizes the steps as: 1) Use Ampere's law to find the magnetic field B(t). 2) Use this to find the magnetic flux Φ and its time derivative dΦ/dt. 3) Apply Faraday's law to find the induced electric field E(t). It notes that this approximation is valid when changes occur sufficiently slowly compared to the speed of light and observers are sufficiently close to the wire.

Uploaded by

mustafa alasady
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
Available Formats
Download as PPTX, PDF, TXT or read online on Scribd
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E&M I

Griffiths Chapter 7
Example 7.9 Long straight wire with time dependent
current. What is the induced electric field?

changing

Recipe
1. Find B(t) using Ampere’s law
2. Find magnetic flux current –dF/dt
3. Find E(t) using Faraday’s law

Amperian loop
Step 1:

Ampere’s law:
Step 2: Flux current

Direction is consistent with


Lenz’s law

Step 3: Faraday’s law:

E(s,t)
But this is because wire was infinitely long

This was an example of a method called the Quasistatic approximation.

We used an equation from magneto-statics (Ampere’s law) to find B.


Then we used an equation from electrodynamics (Faraday’s law) to find E.

This approximation is valid if we can ignore “retardation”. That means that all
parts of space see the changes in current instantaneously.

That means we have to be sufficiently close to the wire, and the changes have
to be sufficiently slow:

Speed of light Characteristic time for changes in current


Because B1 is proportional to I1

Coefficient of proportionality, “Mutual Inductance”


2

Purely geometric, and symmetric under exchange 1 2.


Symmetry of mutual inductance has a practical benefit

Complicated loop 1 Simple loop 2

The symmetry of M12 means that the flux through loop 2 when there is current I in loop 1
is the same as the flux through loop 1 when the same current I is in loop 2.

Subscripts can be dropped M12 = M.


A change in I1, creates a change in B1 by Ampere’s law.
The change in B1 induces an EMF in loop 2 by Faraday’s law.

A change in I1 induces an EMF in any nearby loop, including in loop 1 (itself).

-dF1/dt “Self inductance”

Lenz’s law: self EMF opposes change in I1


Close the switch.
Current starts tries to start flowing.
“Back EMF” appears to oppose this current.

Practical examples of mutual and self inductance

Voltage transformer: Step up, step down.


Wire-wound resistor: No good for high frequencies.
Pulse transformer: Transmit voltage pulse without transmitting background voltage.
Bias-T: Separate DC power supply from high-frequency signals.
Etc, etc.
Magnetic energy.

Work is required to push current into an inductor against the back EMF.

d
= a voltage
= potential
= potential energy per unit
charge

Gravitational analogy
This work gets stored
dW = -F dx as potential energy
d

Total work done becomes an integral


over current, from 0 to I.

The work done depends only on geometry (L)


and on the final current I.
As for electric energy, there are different ways to express magnetic energy.
This integral is over the
volume of the wire, but
it can be extended to all
space considering that J
= 0 outside the wire.
Integral follows the
wire with current I By Ampere’s law

Product rule #6

div. Thm.

Magnetic Fields at infinite


energy boundary are zero
density
Example 7.10. Coaxial solenoids
1: Radius a, n1 turns per unit length
2: Radius b, n2 turns per unit length

If current = I in coil 1, what is magnetic


flux F2 through coil 2?

The field from coil 1 is non-uniform inside


coil 2, which makes this problem hard.

But, Symmetry of M!

Let current I flow in coil 2 instead. Its field


is uniform over coil 1.

So if I flows in coil 1,
Same M

I
Example 7.11. Toroidal coil.
N total turns of wire.
What is self inductance L?

Up arrows are currents in individual wires on


inner surface of toroid.
These are enclosed by Amperian loop, radius s.
Total enclosed current = NI

Total magnetic flux through all N


turns of toroid

= LI
Example 7.12. L-R circuit.
Close the switch. What is I(t)?

Kirchoff’s law

1st order inhomogenous diff. eq.

Initial condition
One undetermined coefficient
Example 7.13.

While there is current, the coax stores magnetic energy. How much?

Energy density, u =

Integrate over cylindrical shells


Radius s, thickness ds, length l

But So
Two recipes to find L.

1. Find flux for given I, then use F = LI

2. Find magnetic energy W for given I, then use W = (1/2) L I 2

The second method is a volume integral of a scalar, and it is usually the easier method.
Electrodynamics so far

Something missing
Problem:

Not
Mathematically zero necessarily
zero

Continuity equation

We can fix the problem


New Ampere’s law by adding the opposite
of this to Ampere’s law.
+
Maxwell’s correction: A
changing E can induce a B-field

Acts like a current: “The displacement current”


Old Ampere’s law and a charging capacitor

The perimeter is the


This current pierces same, but no usual
the surface bounded current penetrates the
by the loop surface
New Ampere’s law

Now any surface with the


same perimeter gives the
same answer
Basic equations to solve any Electrodynamics problem

1. Maxwell’s Equations for the fields


Gauss

Faraday

Ampere + Maxwell

2. Force law

Lorentz

3. Plus boundary conditions


Maxwell’s Equations
determine how
charges affect the
fields

Fields Charges
Lorentz force law tells
how fields affect the
charges

Fields
Charges

Maxwell’s equations would be symmetric if there were magnetic charges,


but there are not any.
Maxwell’s equations include all charges and all currents.
In matter, some are bound and some are free.
(I.e. some are intrinsic and some are extraneous.)

Bound charge

Bound current density

Polarization current density


Total charge

Total current density


Maxwell’s equations in terms of D and H and free charge

8 differential equations for 12 quantities E, B, D, H: Not enough equations!


“Constitutive Equations” are additional relations between E and D, H and B.
These depend on the medium.

For linear media


To obtain the needed boundary conditions, use integral form of Maxwell’s equations
Normal component of electric induction D is discontinuous by the surface free-charge density.
If there is none, then this component of D is continuous.

Normal component of magnetic induction B is always continuous across any boundary.


H1

Surface free H2 Amperian loop


current
density A/m
Goes to zero:
Displacement
current is
finite, but loop
is infinitesimal

or

Tangential components of H are discontinuous by free surface current


density components that flow perpendicular to them.
Loop

Goes to zero:
Magnetic flux
current is
finite, but loop
is infinitesimal

Tangential component of electric field is continuous


at a boundary
The total charge in some volume V is

If charge flows out of this volume through the


boundary surface

Div Theorem

Integrands have to be the same at


every point if equality holds for any
volume V

Continuity Equation
Some volume containing If a charge moves, then work
charges and currents and fields. is done on it by the field.

Rate at which work is done on


a single charge by the fields =

Rate at which work is done on all


the charges in V by the fields =

Power density delivered by the fields


Using Ampere-Maxwell Eq.
Product rule #6

Faraday’s law

Div Theorem

Poynting’s Theorem

Work done on Decrease in Rate of field


charges by fields field energy energy loss
per unit time per unit time through boundary
Energy per unit
Energy flux density
time per unit area

Energy flux Energy per unit time

Poynting’s Theorem

The work dW done on the charges increases their mechanical energy

Statement of Energy
Conservation
Cylindrical wire
with current I

Integrate over the cylindrical surface

The source of Joule


heat is field energy that
flows into the wire
from outside.

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