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THE NATURE OF LIGHT

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This nominal contradiction is an example of. COMPLEMENTARITY or DUALITY in QUANTUM MECHANICS. ... while the PARTICLE part of the duality in Quantum Mechanics CAN! ... – PowerPoint PPT presentation

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Title: THE NATURE OF LIGHT


1
THE NATURE OF LIGHT
  • Light is an ELECTROMAGNETIC WAVE
  • Light is also a PARTICLE the PHOTON
  • This nominal contradiction is an example of
  • COMPLEMENTARITY or DUALITY in QUANTUM MECHANICS.
    Depending on
    circumstances it is preferable to use one or the
    other point of view for light,
    electrons, protons, atoms anything which is too
    small to be described by normal physics requires
    quantum mechanics

2
First, the Wave Nature
  • Light is a TRANSVERSE ELECTROMAGNETIC
    WAVE.
  • Electric (E) fields oscillate perpendicular to
  • Magnetic (B) fields and the ENERGY FLOWS
    PERPENDICULAR to both fields.
  • Other transverse waves WATER waves,
    SECONDARY (shear) SEISMIC waves.
  • LONGITUDINAL WAVES have ENERGY FLOWS PARALLEL to
    oscillations SOUND, PRIMARY (compressional)
    SEISMIC waves.

3
Transverse Electromagnetic (EM) Wave
4
Electric and Magnetic Fields
  • Charged particles (protons or ions , electrons
    -) attract or repel each other.
  • Electric fields accelerate charged particles
    along the lines.
  • Charged particles orbit around magnetic field
    lines.

5
Characteristics of All Waves
  • Frequency (? or f) oscillations per sec (Hz)
  • Speed (v) depends on medium, sometimes ? (cm/s
    or m/s)
  • Wavelength (?) distance between crests (cm)
  • Amplitude (A) strength of oscillation

6
Key Relations for ALL Waves
  • Speed Wavelength x Frequency v
    ??
  • Or ? v/ ? or ? v/?
  • Power ?Amplitude2 P ? A2

7
Anatomy of A Wave Applet
  • /Users/paulwiita/Documents/Presentations/anatomy_o
    f_a_wave.htm

8
Wavelength and Frequency for Light
  • wavelength x frequency speed of light constant

9
First POP Quiz (5 minutes)
  • Put away all books and notes.
  • Take out a sheet of paper.
  • Neatly print your name. (1 pt)
  • Neatly print my name. (2 pts)
  • Explain what is meant by the word theory in
    science. Contrast this with the words meaning
    in common speech. (8 pts)

10
For EM Waves ONLY
  • v c 2.9979x108 m s-1 3.00x1010 cm s-1
  • 3.00x105 km s-1 186,000 miles/s
  • The speed of light does not depend upon direction
    or frequency in a vacuum and doesnt need a
    medium.
    It is a CONSTANT of
    NATURE.
  • In matter, v lt c and the same frequency has a
    shorter wavelength than in vacuum.
    The INDEX OF REFRACTION,
    n c/v gt 1. In air, n 1.0003
    in normal glass, n ? 1.5

11
Special Topic Polarized Light
  • EM WAVES CAN ALSO BE POLARIZED
  • E field in a particular plane B field in one
    perpendicular plane ? LINEAR POLARIZATION
    this is the only kind of polarization we'll worry
    about.
  • Reflection can change the polarization of light
  • Polarized sunglasses block light that reflects
    off of horizontal surfaces

12
The Seven Bands of the EM Spectrum
? Microwave or millimeter between Radio and IR
13
Atmospheric Transmission
  • Radio ? gt 1 cm -- The longest waves or lowest
    frequencies.
  • Penetrates atmosphere if ?lt15 m
  • So AM reflects off ionosphere while FM penetrates
  • Millimeter or microwave 1 cm gt ? gt 0.003 cm --
    partially penetrates atm molecules absorb.
  • Infrared (IR) 0.003 cm gt ? gt 7.2x10-5 cm
    720 nm
  • CO2 , H2O etc absorb most but some ?s penetrate

14
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15
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16
Visible Wavelengths
  • VISIBLE (OPTICAL)
    720 nm 7200 Å gt ? gt 380 nm 3800 Å,
    4.2 x 1014 Hz lt ? lt 7.9 x 1014 Hz.
  • Penetrates atmosphere (shorter scatter more)
  • Visible spectrum RED (longest wavelength),
    ORANGE, YELLOW, GREEN, BLUE, VIOLET (shortest
    wavelength -- highest frequency)
  • Our eyes evolved to see this light, since the Sun
    produces most of its radiation in this band, and
    since nearly all of this radiation gets through
    the atmosphere.

17
Colors of Light
  • White light is made up of many different colors

18
Shortest Wavelengths
  • ULTRAVIOLET (UV) 380 nm gt ? gt 300Å
    Mostly absorbed in atmosphere ozone (O3)
    Good thing, since UV radiation causes skin
    cancer.
  • X-RAY 300 Å gt ? gt 0.1 Å,
    Absorbed in atmosphere by any atom (N, O)
    A good thing too X-rays can penetrate
    the body and cause cancer in many organs.
  • GAMMA-RAY (?-ray) ? lt 0.1 Å,
    The most energetic form of EM radiation.
    Absorbed high in atmosphere by any atomic
    nucleus.
    A VERY good thing
    gamma-rays quickly cause severe burns and
    cancer.

19
Blue light is (compared to red light),
  1. Shorter wavelength
  2. Longer wavelength
  3. Higher energy photons
  4. 1 and 3
  5. None of the above

20
Blue light is (compared to red light),
  1. Shorter wavelength
  2. Longer wavelength
  3. Higher energy photons
  4. 1 and 3
  5. None of the above

21
We cant see infrared, but we can perceive it as
  1. Heat
  2. Radar
  3. Sound
  4. AM
  5. FM

22
We cant see infrared, but we can perceive it as
  1. Heat
  2. Radar
  3. Sound
  4. AM
  5. FM

23
How are Electromagnetic Waves Made?
  • Most come from
    ATOMIC,
    MOLECULAR or
    NUCLEAR
    TRANSITIONS. I.e.,
    electrons or protons changing quantum states.
  • BUT FUNDAMENTALLY, EM RADIATION IS PRODUCED BY
    AN ACCELERATED CHARGED PARTICLE.
  • Since ELECTRONS have the LOWEST MASSES they are
    MOST EASILY ACCELERATED, therefore, electrons
    produce most EM waves.

24
Examples of EM Wave Generation
  • Radio - TV - Cell Phone transmission towers.
    Electrons oscillate up down
  • Synchrotron Radiation produced by electrons
    spiraling around magnetic field lines, when
    moving at nearly speed of light.
  • The circular part of the motion is ACCELERATED
    and produces the radiation. Synchrotron
    radiation is strongly POLARIZED most EM
    radiation is basically UNPOLARIZED

25
How do Waves Interact with Matter?
  • EMIT (light is sent out when a bulb is turned on)
  • REFLECT (angle of incidence angle of
    reflection) or Scatter (spread out reflection)
  • TRANSMIT (low opacity)
  • ABSORB (high opacity)
  • REFRACT (bend towards normal when entering a
    medium with a slower propagation speed)
  • INTERFERE (only a WAVE can do this) Either
    CONSTRUCTIVE (waves add when in phase)
    DESTRUCTIVE (waves cancel when out of
    phase)
  • DIFFRACT (only a WAVE can do this)
    Waves spread out when passing through a hole
    or slit. This is important only if the size of
    the hole or slit is comparable to the
    wavelength.

26
Reflection and Scattering
Mirror reflects light in a particular direction
Movie screen scatters light in all directions
27
Interactions of Light with Matter
Interactions between light and matter determine
the appearance of everything around us objects
reflect some wavelengths, absorb others and emit
others.
28
When light approaches matter, it can
  1. Be absorbed by the atoms in the matter
  2. Go through the matter, and be transmitted
  3. Bounce off the matter, and be reflected
  4. Any of the above
  5. Only 2 or 3

29
When light approaches matter, it can
  1. Be absorbed by the atoms in the matter
  2. Go through the matter, and be transmitted
  3. Bounce off the matter, and be reflected
  4. Any of the above
  5. Only 2 or 3

30
Thought QuestionWhy is a rose red?
  1. The rose absorbs red light.
  2. The rose transmits red light.
  3. The rose emits red light.
  4. The rose reflects red light.

31
Thought QuestionWhy is a rose red?
  1. The rose absorbs red light.
  2. The rose transmits red light.
  3. The rose emits red light.
  4. The rose reflects red light.

32
Interference and Diffraction
33
Light as Particles
  • ELECTROMAGNETIC ENERGY IS CARRIED BY PHOTONS
  • A PHOTON is a SINGLE QUANTUM OF LIGHT.
    The energy of one photon
    of a particular frequency is
  • E h? h c / ?
    h 6.63 x
    10-34 Joule sec 6.63 x 10-27 erg sec is
    PLANCK's CONSTANT.
  • Along with c, the speed of light
    e, the charge on an electron
    (or proton) and G (Newton's constant of
    gravity), h is one of the
  • FUNDAMENTAL CONSTANTS of NATURE.

34
Thought QuestionThe higher the photon energy
  1. the longer its wavelength.
  2. the shorter its wavelength.
  3. energy is independent of wavelength.

35
Thought QuestionThe higher the photon energy
  1. the longer its wavelength.
  2. the shorter its wavelength.
  3. energy is independent of wavelength.

36
Photons vs. Waves
  • These PHOTONS can equally well explain
  • REFLECTION,
  • REFRACTION,
  • TRANSMISSION and
  • ABSORPTION
  • as can the Wave picture,
  • BUT they can't explain
  • INTERFERENCE and
  • DIFFRACTION.

37
Photons vs. Waves, Round 2
  • On the other hand the WAVE picture can't explain
  • The PHOTOELECTRIC EFFECT
  • (where metals emit electrons when
    light shines on them)
  • and SPECTRAL LINES
  • (where only specific wavelengths of light
    emerge from particular elements)
  • while the PARTICLE part of the duality in Quantum
    Mechanics CAN!
  • Well soon discuss each of these key aspects of
    light the latter is at the core of modern
    astronomy.

38
How can light behave as both a wave and a
particle?
  1. It doesnt really
  2. It really is both a wave and a particle
  3. Light and small objects such as atoms behave in
    ways we never see in everyday objects, so we
    cant describe them in everyday terms
  4. This is what quantum mechanics describes
  5. 3 and 4

39
How can light behave as both a wave and a
particle?
  1. It doesnt really
  2. It really is both a wave and a particle
  3. Light and small objects such as atoms behave in
    ways we never see in everyday objects, so we
    cant describe them in everyday terms
  4. This is what quantum mechanics describes
  5. 3 and 4

40
Radiation, Temperature and Power
  • Crudely, hotter matter produces more highly
    accelerated charged particles, which therefore
    produces more powerful EM radiation.
  • Heat energy is proportional to temperature
  • E k T
    (where T is in Kelvins, 0 at
    ABSOLUTE ZERO).
  • So the thermal (heat) energy in atoms should be
    proportional to the photon energy using math
  • h ? ? kT OR
  • ? ? 1/T

41
Temperature Scales
  • Only the US has stuck with Fahrenheit
    temperatures
  • The rest of the world normally uses Celcius, but
  • ENERGIES VANISH AT ABSOLUTE ZERO THE NATURAL
    TEMPERATURE SCALE IS KELVINS.
  • The size of 1 degree C 1 K and 1.8 degrees F.
  • 0 C 273.16 K (round it off)
  • The conversion formula is F (9/5)C 32
  • or C (5/9)(F - 32)

42
Wiens Law
  • Or, ?max2,900,000/T (nm)
  • This is the PEAK WAVELENGTH for BLACKBODY (or
    Thermal, or Planckian) emission from a SOLID, a
    LIQUID or a DENSE GAS.
  • Ex T 5800K 5.8x103K

0.5x10-4cm5x10-5cm 500 nm 5000Å
43
Thermal Spectra
44
Properties of Thermal Radiation
  • Hotter objects emit more light at all frequencies
    per unit area.
  • Hotter objects emit photons with a higher average
    energy.

45
Thought QuestionWhich is hotter?
  1. A blue star.
  2. A red star.
  3. A planet that emits only infrared light.

46
Thought QuestionWhich is hotter?
  1. A blue star.
  2. A red star.
  3. A planet that emits only infrared light.

47
Thought QuestionWhy dont we glow in the dark?
  1. People do not emit any kind of light.
  2. People essentially only emit light that is
    invisible to our eyes.
  3. People are too small to emit enough light for us
    to see.
  4. People do not contain enough radioactive material.

48
Thought QuestionWhy dont we glow in the dark?
  1. People do not emit any kind of light.
  2. People essentially only emit light that is
    invisible to our eyes.
  3. People are too small to emit enough light for us
    to see.
  4. People do not contain enough radioactive material.
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