lecture 32 - physics and astronomy

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Lecture 32 PHYC 161 Fall 2016

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Page 1: Lecture 32 - Physics and Astronomy

Lecture 32PHYC 161 Fall 2016

Page 2: Lecture 32 - Physics and Astronomy

Applying Ampereā€™s Law ā€¢ We can look at the magnetic field

inside a conducting wire with some (cylindrically symmetric) current density:

ļæ½ ļæ½

0 encClosed Path

20

0 encCircle 0

0

0

inside wire2

outside wire

inside wire2

outside wire2

B dl I

J rB dl rB I

I

Jr

BIr

P

P SS P

P

P

PS

ļæ½ ļæ½

Ā­Ā°ļæ½ Ā®Ā°Ģ„

Ā­Ā°Ā° Ā®Ā°Ā°Ģ„

Ā³

Ā³

Page 3: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Field of a solenoidā€¢ A solenoid consists of a helical winding of wire on a cylinder.

ā€¢ Follow Example 28.9 using the figures below.

Page 4: Lecture 32 - Physics and Astronomy

Applying Ampereā€™s Law

ā€¢ If we have a current, I, and N turns per unit length, L, then:

0 encClosed Path

a b

B dl I

B dl B

P

o

ļæ½ ļæ½

ļæ½ ļæ½ ļæ½

Ā³

Ā³b c

dl Bo

ļæ½Ā³c d

dl Bo

ļæ½ ļæ½ ļæ½Ā³ 0d a

0

0

dl NI

BL NINB IL

P

P

P

o

ļæ½

ļæ½

Ā³

Page 5: Lecture 32 - Physics and Astronomy

HW - Apply Amperes Law to a current sheet

Infinite sheet => B is constant outside the sheet

Page 6: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Faradayā€™s law of inductionā€¢ When the magnetic flux through a single closed loop changes

with time, there is an induced emf that can drive a current around the loop:

ā€¢ Recall that the unit of magnetic flux is the weber (Wb).

ā€¢ 1 T Ā· m2 = 1 Wb, so 1 V = 1 Wb/s.

Page 7: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Determining the direction of the induced emf: Slide 1 of 4

Page 8: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Determining the direction of the induced emf: Slide 2 of 4

Page 9: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Determining the direction of the induced emf: Slide 3 of 4

Page 10: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Determining the direction of the induced emf: Slide 4 of 4

Page 11: Lecture 32 - Physics and Astronomy

Example ā€¢ Letā€™s put some numbers in to see how this might work:

ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½Surface

22 4

24

24

cos

1 0.020 1 0.012 2.4 10

2.4 104.8 10

5.0

BAd dBN B dA N Adt dt

TmT s ms

TmTmsI

R s

T

ļæ½

ļæ½

ļæ½

ĀŖ Āŗ ļæ½ ļæ½ ļæ½Ā« Ā»

Ā¬ Ā¼

ļæ½ u

u u

: :

Ā³E

E

Page 12: Lecture 32 - Physics and Astronomy

Unit Check!!! ā€¢ Letā€™s put some numbers in to see how this might work:

ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½ ļæ½Surface

22 4

24

24

cos

1 0.020 1 0.012 2.4 10

2.4 104.8 10

5.0

BAd dBN B dA N Adt dt

TmT s ms

TmTmsI

R s

T

ļæ½

ļæ½

ļæ½

ĀŖ Āŗ ļæ½ ļæ½ ļæ½Ā« Ā»

Ā¬ Ā¼

ļæ½ u

u u

: :

Ā³E

E

dF Idl BN AmT

NTAm

u ļæ½ ļæ½

V IRNm AC

NmAC

ļæ½

:ļæ½

:

22

N mTm CAm ANms ssAC

ļæ½ :

Page 13: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Faradayā€™s law for a coilā€¢ A commercial alternator uses

many loops of wire wound around a barrel-like structure called an armature.

ā€¢ The resulting induced emf is far larger than would be possible with a single loop of wire.

ā€¢ If a coil has N identical turns and if the flux varies at the same rate through each turn, total emf is:

Page 14: Lecture 32 - Physics and Astronomy

Lenzā€™s Law ā€¢ To get the direction of the induced

EMF (and thus, the current in a circuit), remember:

Bddt

ļæ½ )E

Page 15: Lecture 32 - Physics and Astronomy

CPS 32-1 A circular loop of wire is in a region of spatially uniform magnetic field. The magnetic field is directed into the plane of the figure. If the magnetic field magnitude is decreasing,

A. the induced emf is clockwise.

B. the induced emf is counterclockwise.

C. the induced emf is zero.

D. The answer depends on the strength of the field.

Page 16: Lecture 32 - Physics and Astronomy

CPS 32-2 A circular loop of wire is placed next to a long straight wire. The current I in the long straight wire is increasing. What current does this induce in the circular loop?

A. a clockwise current

B. a counterclockwise current

C. zero current

D. not enough information given to decide

Page 17: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Motional electromotive force ā€¢ When a conducting rod moves perpendicular to a uniform

magnetic field, there is a motional emf induced.

Page 18: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Induced electric fieldsā€¢ A long, thin solenoid is

encircled by a circular conducting loop.

ā€¢ Electric field in the loop is what must drive the current.

ā€¢ When the solenoid current I changes with time, the magnetic flux also changes, and the induced emf can be written in terms of induced electric field:

Page 19: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Eddy currentsā€¢ When a piece of metal moves through a magnetic field or is

located in a changing magnetic field, eddy currents of electric current are induced.

ā€¢ The metal detectors used at airport security checkpoints operate by detecting eddy currents induced in metallic objects.

Page 20: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Displacement currentā€¢ Ampereā€™s law is incomplete, as can be shown by considering the

process of charging a capacitor, as shown.

ā€¢ For the plane circular area bounded by the circle, Iencl is the current iC in the left conductor.

ā€¢ But the surface that bulges out to the right is bounded by the same circle, and the current through that surface is zero.

ā€¢ This leads to a contradiction.

Page 21: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Displacement currentā€¢ When a capacitor is charging, the

electric field is increasing between the plates.

ā€¢ We can define a fictitious displacement current iD in the region between the plates.

ā€¢ This can be regarded as the source of the magnetic field between the plates.

Page 22: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Maxwellā€™s equations of electromagnetismā€¢ All the relationships between electric and magnetic fields and

their sources are summarized by four equations, called Maxwellā€™s equations.

ā€¢ The first Maxwell equation is Gaussā€™s law for electric fields from Chapter 22:

ā€¢ The second Maxwell equation is Gaussā€™s law for magnetic fields from Chapter 27:

Page 23: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Maxwellā€™s equations of electromagnetismā€¢ The third Maxwell equation is this chapterā€™s formulation of

Faradayā€™s law:

ā€¢ The fourth Maxwell equation is Ampereā€™s law, including displacement current:

Page 24: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Maxwellā€™s equations in empty spaceā€¢ There is a remarkable

symmetry in Maxwellā€™s equations.

ā€¢ In empty space where there is no charge, the first two equations are identical in form.

ā€¢ The third equation says that a changing magnetic flux creates an electric field, and the fourth says that a changing electric flux creates a magnetic field.

Page 25: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

Superconductivity in a magnetic fieldā€¢ When a superconductor is cooled below its critical

temperature Tc, it loses all electrical resistance.

ā€¢ For any superconducting material the critical temperature Tc changes when the material is placed in an externally produced magnetic field.

ā€¢ Shown is this dependence for mercury.

ā€¢ As the external field magnitude increases, the superconducting transition occurs at a lower and lower temperature.

Page 26: Lecture 32 - Physics and Astronomy

Ā© 2016 Pearson Education Inc.

The Meissner effectā€¢ If we place a superconducting material in a uniform applied

magnetic field, and then lower the temperature until the superconducting transition occurs, then all of the magnetic flux is expelled from the superconductor.

ā€¢ The expulsion of magnetic flux is called the Meissner effect.