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Lecture 20 Electromagnetic Waves Nature of Light Reflection and Refraction

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Lecture 20. Electromagnetic Waves Nature of Light Reflection and Refraction. Fig. 22-CO, p.726. Electromagnetic Waves are Transverse Waves. The and fields are perpendicular to each other Both fields are perpendicular to the direction of motion Therefore, em waves are transverse waves. - PowerPoint PPT Presentation

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Page 1: Lecture 20

Lecture 20

Electromagnetic Waves Nature of Light Reflection and Refraction

Page 2: Lecture 20

Fig. 22-CO, p.726

Page 3: Lecture 20

Electromagnetic Waves are Transverse Waves

The and fields are perpendicular to each other

Both fields are perpendicular to the direction of motion

Therefore, em waves are transverse waves

E

B

Page 4: Lecture 20

Properties of EM Waves Electromagnetic waves are transverse

waves Electromagnetic waves travel at the

speed of light

Because em waves travel at a speed that is precisely the speed of light, light is an electromagnetic wave

1

o o

c

Page 5: Lecture 20

Properties of EM Waves, 2 The ratio of the electric field to the

magnetic field is equal to the speed of light

Electromagnetic waves carry energy as they travel through space, and this energy can be transferred to objects placed in their path

Ec

B

Page 6: Lecture 20

Properties of EM Waves, 3 Energy carried by em waves is

shared equally by the electric and magnetic fields

2 2max max max max

2 2 2o o o

Average power per unit area

E B E c BI

c

Page 7: Lecture 20

Properties of EM Waves, final Electromagnetic waves transport

linear momentum as well as energy For complete absorption of energy U,

p=U/c For complete reflection of energy U,

p=(2U)/c Radiation pressures can be

determined experimentally

Page 8: Lecture 20

Determining Radiation Pressure This is an apparatus

for measuring radiation pressure

In practice, the system is contained in a vacuum

The pressure is determined by the angle at which equilibrium occurs

Page 9: Lecture 20

The Spectrum of EM Waves Forms of electromagnetic waves

exist that are distinguished by their frequencies and wavelengths c = ƒλ

Wavelengths for visible light range from 400 nm to 700 nm

There is no sharp division between one kind of em wave and the next

Page 10: Lecture 20

The EMSpectrum

Note the overlap between types of waves

Visible light is a small portion of the spectrum

Types are distinguished by frequency or wavelength

Page 11: Lecture 20

Notes on The EM Spectrum Radio Waves

Used in radio and television communication systems

Microwaves Wavelengths from about 1 mm to 30

cm Well suited for radar systems Microwave ovens are an application

Page 12: Lecture 20

Notes on the EM Spectrum, 2

Infrared waves Incorrectly called “heat waves” Produced by hot objects and

molecules Readily absorbed by most materials

Visible light Part of the spectrum detected by the

human eye Most sensitive at about 560 nm

(yellow-green)

Page 13: Lecture 20

Notes on the EM Spectrum, 3 Ultraviolet light

Covers about 400 nm to 0.6 nm Sun is an important source of uv light Most uv light from the sun is absorbed in

the stratosphere by ozone X-rays

Most common source is acceleration of high-energy electrons striking a metal target

Used as a diagnostic tool in medicine

Page 14: Lecture 20

Notes on the EM Spectrum, final Gamma rays

Emitted by radioactive nuclei Highly penetrating and cause serious

damage when absorbed by living tissue

Looking at objects in different portions of the spectrum can produce different information

Page 15: Lecture 20

Fig. 21-CO, p.693

Page 16: Lecture 20

Fig. 21-23d, p.717

Radio

Page 17: Lecture 20

Fig. 21-23a, p.717

X-ray

Page 18: Lecture 20

Fig. 21-23b, p.717

optical

Page 19: Lecture 20

Fig. 21-23c, p.717

Infra-red

Page 20: Lecture 20

A Brief History of Light 1000 AD

It was proposed that light consisted of tiny particles

Newton Used this particle model to explain

reflection and refraction Huygens

1678 Explained many properties of light by

proposing light was wave-like

Page 21: Lecture 20

A Brief History of Light, cont Young

1801 Strong support for wave theory by

showing interference Maxwell

1865 Electromagnetic waves travel at the

speed of light

Page 22: Lecture 20

A Brief History of Light, final Planck

EM radiation is quantized Implies particles

Explained light spectrum emitted by hot objects

Einstein Particle nature of light Explained the photoelectric effect

Page 23: Lecture 20

The Particle Nature of Light “Particles” of light are called photons Each photon has a particular energy

E = h ƒ h is Planck’s constant

h = 6.63 x 10-34 J s Encompasses both natures of light

Interacts like a particle Has a given frequency like a wave

Page 24: Lecture 20

Dual Nature of Light Experiments can be devised that

will display either the wave nature or the particle nature of light In some experiments light acts as a

wave and in others it acts as a particle

Nature prevents testing both qualities at the same time