Class 18: Outline Hour 1: Levitation Experiment 8: Magnetic Forces

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Class 18: Outline

Hour 1:

Levitation

Experiment 8: Magnetic Forces

Hour 2:

Ampere’s Law

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Review:

Right Hand Rules

1. Torque: Thumb = torque, fingers show rotation

2. Feel: Thumb = I, Fingers = B, Palm = F

3. Create: Thumb = I, Fingers (curl) = B

4. Moment: Fingers (curl) = I, Thumb = Moment

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Last Time:

Dipoles

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µ

IA

ˆ ≡

I A

Generate:

Feel:

U

Dipole

= -

G

G

µ B

1) Torque to align with external field

2) Forces as for bar magnets (seek field)

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Some Fun:

Magnetic Levitation

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Put a Frog in a 16 T Magnet…

For details: http://www.hfml.sci.kun.nl/levitate.html

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How does that work?

First a BRIEF intro to magnetic materials

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Para/Ferromagnetism

Applied external field B

0 tends to align the atomic magnetic moments (unpaired electrons)

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Diamagnetism

Everything is slightly diamagnetic. Why?

More later.

If no magnetic moments (unpaired electrons) then this effect dominates.

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Back to Levitation

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Levitating a Diamagnet

N

S

S

N

S

N

1) Create a strong field

(with a field gradient!)

2) Looks like a dipole field

3) Toss in a frog (diamagnet)

4) Looks like a bar magnet pointing opposite the field

5) Seeks lower field (force up ) which balances gravity

Most importantly, its stable:

Restoring force always towards the center

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Using ∇ B to Levitate

•Frog

•Strawberry

•Water Droplets

•Tomatoes

•Crickets

For details: http://www.hfml.ru.nl/levitation-movies.html

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Demonstrating:

Levitating Magnet over

Superconductor

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Perfect Diamagnetism:

“Magnetic Mirrors”

N

S

S

N

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Perfect Diamagnetism:

“Magnetic Mirrors”

N

S

S

N

No matter what the angle, it floats -- STABILITY

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Using ∇ B to Levitate

A Sumo Wrestler

For details: http://www.hfml.sci.kun.nl/levitate.html

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Two PRS Questions Related to

Experiment 8: Magnetic Forces

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Experiment 8: Magnetic Forces

(Calculating µ

0

) http://ocw.mit.edu/ans7870/8/8.02T/f04/visualizations/magnetostatics/16-

MagneticForceRepel/16-MagForceRepel_f65_320.html

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Experiment Summary:

Currents feel fields

Currents also create fields

Recall… Biot-Savart

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The Biot-Savart Law

Current element of length d s carrying current I produces a magnetic field: d

G

B

=

µ

π

0

I d

×

r

ˆ

4

r 2

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Today:

3

rd

Maxwell Equation:

Ampere’s Law

Analogous (in use) to Gauss’s

Law

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Gauss’s Law – The Idea

The total “flux” of field lines penetrating any of these surfaces is the same and depends only on the amount of charge inside

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Ampere’s Law: The Idea

In order to have a B field around a loop, there must be current punching through the loop

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Ampere’s Law: The Equation

G

B

d s

G

= µ

0

I enc

The line integral is around any closed contour bounding an open surface S.

I enc

I enc

= ⋅

S

J d A

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PRS Question:

Ampere’s Law

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Biot-

Savart

Law

Biot-Savart vs. Ampere

G

B =

µ

4

0

π

G

× ˆ r 2 general current source ex: finite wire wire loop

Ampere’s law

G

B ⋅ d = µ

0

I enc symmetric current source ex: infinite wire infinite current sheet

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Applying Ampere’s Law

1. Identify regions in which to calculate B field

Get B direction by right hand rule

2. Choose Amperian Loops S: Symmetry

3. Calculate

B ⋅ d s

4. Calculate current enclosed by loop S

G

B

d s

G

=

µ

0

I enc

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Always True,

Occasionally Useful

Like Gauss’s Law,

Ampere’s Law is always true

However, it is only useful for calculation in certain specific situations, involving highly symmetric currents.

Here are examples…

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Example: Infinite Wire

I A cylindrical conductor has radius R and a uniform current density with total current I

Find B everywhere

Two regions:

(1) outside wire (r ≥ R)

(2) inside wire (r < R)

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Ampere’s Law Example:

Infinite Wire

I

B

I

Amperian Loop:

B is Constant & Parallel

I Penetrates

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Example: Wire of Radius R

Region 1: Outside wire (r ≥ R)

Cylindrical symmetry Æ

Amperian Circle

B-field counterclockwise v

G

B s

G

=

= µ

v

0

I enc s

G

=

=

B

µ

0

(

I

2 π r

)

G

B =

µ

2 π

0

I r counterclo ckwise

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Example: Wire of Radius R

Region 2: Inside wire (r < R)

v

G

B s =

= µ

v

0

I enc s

G

=

=

B 2 π r

µ

0

I

(

π

π r

)

R

2

2

G

B =

2

µ

π

0

Ir

R 2 counterclo ckwise

Could also say: J =

I

A

=

I

π R 2

; I enc

= JA enc

=

I

π R 2

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Example: Wire of Radius R

B in

=

µ

π

0

Ir

2 R 2

B out

=

µ

2

0

π r

I

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Group Problem: Non-Uniform

Cylindrical Wire

I A cylindrical conductor has radius R and a nonuniform current density with total current:

G

J = J

0

R r

Find B everywhere

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Applying Ampere’s Law

In Choosing Amperian Loop:

• Study & Follow Symmetry

• Determine Field Directions First

• Think About Where Field is Zero

• Loop Must

• Be Parallel to (Constant) Desired Field

• Be Perpendicular to Unknown Fields

• Or Be Located in Zero Field

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Other Geometries

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Helmholtz Coil

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Closer than Helmholtz Coil

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Multiple Wire Loops

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Multiple Wire Loops –

Solenoid

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Magnetic Field of Solenoid loosely wound tightly wound

For ideal solenoid, B is uniform inside & zero outside

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Magnetic Field of Ideal Solenoid v ∫

G

B ⋅

Using Ampere’s law: Think!

d

⎧ ⊥

G

=

G

B

1

=

G

Bl d

0 along side 3

⋅ d

G

G

along sides 2 and 4

+

+ ∫

2

G

B

0

⋅ d

G

+

+

3

G

B ⋅ d

0

G

+ ∫

4

+

G

B ⋅ d

0

G

I enc

= nlI v

n: turn density

G

B ⋅ d s = Bl = µ

0 nlI

µ

0 nlI

B = = µ

0 nI l

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Demonstration:

Long Solenoid

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Group Problem: Current Sheet y

A sheet of current (infinite in the y & z directions, of thickness 2d in the x direction) carries a uniform current density:

G

J s

= J

ˆ

Find B everywhere

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Ampere’s Law:

Infinite Current Sheet

B

I

B

Amperian Loops:

B is Constant & Parallel OR Perpendicular OR Zero

I Penetrates

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Solenoid is Two Current Sheets

Field outside current sheet should be half of solenoid, with the substitution: nI = 2 dJ

This is current per unit length

(equivalent of λ , but we don’t have a symbol for it)

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Long

Circular

Symmetry

Solenoid

=

2 Current

Sheets

B

X

X

X

X

X

X

X

X

X

X

X

X

G

B

d s

G

=

µ

I enc

B

I

B

(Infinite) Current Sheet

X

X

X

X

X

X

X

X

X

X

X

X

X

X

X

X

Torus

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Brief Review Thus Far…

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Maxwell’s Equations (So Far)

Gauss's Law: w

S

∫∫

G

⋅ d

G

E A =

Q in

ε

0

Electric charges make diverging Electric Fields

Magnetic Gauss's Law: w

S

∫∫

G

⋅ d

G

B A = 0

No Magnetic Monopoles! (No diverging B Fields)

Ampere's Law: v

C

G

B ⋅ d s = µ

0

I enc

Currents make curling Magnetic Fields

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