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E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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Page 1: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

E&M Demo and More

Chris Tully

Princeton

NJAAPT, March 16, 2013

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Page 2: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

The ElectrophorusA device that uses induction to produce a substantial charge.

Insulating handle

Metal disk Hard rubber

1. The hard rubber pallet is charged (-)by rubbing with fur.Positive charge movesdown and negative moves up.

2. The electrophorus is moved to contact the metal case. Negative charge, repelled by the negative charge on the rubber, tries to get as far away as possible.

3. Once again isolatedfrom the case, the electrophorus carriesa substantial net (+)charge.

Metal plate

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Page 3: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

The Electroscope

Demo: Charge flows onto the conductor and causes the foil to deflect.

A simple device for measuring charge.

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Page 4: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Charging an electroscope by induction.

1. Bring charge close, without touching.

2. Momentarily ground the electroscope, thus allowing some of the positive charge to escape.

3. Move the charge away, leaving the electroscope charged.

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Page 5: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Wimshurst machine

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Page 6: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Rainforest

+ + + + + + + + + + + + + + + + + + + + + + + +

- - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -

Negative Charge

Positive Charge

+++

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Page 7: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Ohm’s Law

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Page 8: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Charging a Capacitor

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I

V

I

Sunlight

Current Source(For example, solar panel)Voltage Source

Q3. Starting from the same initial charging current and ending at the same maximum voltage, which will charge up a capacitor faster?

a) b)

c) Tie – no difference in charging rate

Page 9: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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Page 10: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Storing energy in capacitors

Capacitors can store energy

The stored energy can be quickly released with spectacular effect.

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Page 11: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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Field of Permanent Dipole Magnet

There are no“magnetic charges” analogous to electric charges (monopoles).

Fields are due to currents and do not terminate on “magnetic charges”

Field lines are continuous inside objects.

North pole: where field comes outSouth pole: where the field goes in

Page 12: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Magnetic Levitation

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Page 13: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

The “Ring Toss”

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Page 14: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Force on a current ring

B increasingI clockwise from aboveForce up

B

BxI

F

B

Binduced 14

Page 15: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Alternating current with Inductor

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Page 16: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Alternating current with capacitor

V =Vmax cos(t)

V Q

C0

Q VC = VmaxC cos(t)

I dQ

dtVmaxC sin(t)

Vmax

1/Csin(t)

Vmax

X c

sin(t)

X c 1

C "capacitive reactance"

"Current leads voltage"

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Page 17: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Transporting and Rotating B field flux

I1(t)

I2(t)

I3(t)

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Page 18: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

3-Phase Power

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Page 19: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

3-Phase Power

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47Ω connected from V1 to ground 33Ω to ground

3.3KΩ to ground3.3KΩ to ground

1µF connected to V1

100mH connected to V2 .15µF connected

to V2

Page 20: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Eddy Currents

• Lenz’s Law holds for “eddy currents”.

Here, part of the current loop is outside the B-field and has no force on it, and part is inside the B-field with a force.

• The net result is a force that tries to oppose the change in flux, acting opposite the velocity.

No force here (B=0)

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Page 21: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Tesla Coil

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Page 22: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

EM waves from accelerating charge on antenna

B

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Page 23: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Anatomy of a EM Wave

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Note that the velocityis in the direction of ExB:

r v

r E

r B

Page 24: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

The dipole antenna oscillator and receiver

The 200 MHz oscillator(at rear) generates EMwaves with the dipoleantenna. The polarization(E-field) is horizontal.

The dipole receiver (infront) detects the waves.The bulb lights up when thesignal is strong. Expected polarization and intensity patternare observed.

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Page 25: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Polarization

The orientation of the E field could be vertical, horizontal, “circular,” or random.

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Page 26: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Polarization

Radio waves will be polarized along the direction of the radiating element.

The receiving antenna should have the same polarization to work efficiently.

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Page 27: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Standing Waves

Just as one can have standing waves on a string, one can have standing electromagnetic waves.

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Page 28: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

Standing Waves- Photo

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Page 29: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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Heat Dissipation of Light Bulbs

• Heat capacity of water:– Takes 4.2 Joules to raise 1gram=1cm3 of water

by 1 degree C– 1 Watt = 1 Joule/sec

Pdissipated (4.2J /goC)(1000g)(25oC)

3000sec35 Watts

Page 30: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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• The Universe was not always as cold and dark as it is today – there are a host of landmark measurements that track the history of the universe

• None of these measurements, however, reach back as far in time as ~1 second after the Big Bang– At ~1 second the hot, expanding universe is

believed to have become transparent to neutrinos

– In the present universe, relic neutrinos are predicted to be at a temperature of 1.9K (1.7x10-4 eV) and to have an average number density of ~56/cm3 of electron neutrinos EVERYWHERE IN SPACE!

Dicke, Peebles, Roll, Wilkinson (1965)

1 sec

Looking Back in Time

Page 31: E&M Demo and More Chris Tully Princeton NJAAPT, March 16, 2013 1

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Princeton Tritium Observatory for Light, Early-Universe, Massive-Neutrino Yield