More Light and Optics

1. More Light and Optics

2. Light – Wave or particle? • For many years scientists argued over the nature of light, "Is light a wave or a stream of particles?" • In some experiments light exhibits wave like properties, the Doppler effect, interference, refraction, diffraction • and in other experiments, like the photo electric effect, it exhibits particle like properties • The fact is that light exhibits behaviors which are characteristic of both waves and particles.

3. Models of Light - Waves • Electromagnetic waves (light) originate from vibrating or accelerating electric charges • Electromagnetic waves are made up of an electric field and a magnetic field oscillating at right angles relative to one another • An electromagnetic wave (light) is a transverse wave Unlike other waves, light waves can travel through a vacuum

4. Models of Light - Particles • Particle of light are called photons • Photons have zero rest mass and travel at the speed of light through a vacuum.

5. Speed of Light - c • In the early 17th century, many scientists believed that there was no such thing as the "speed of light"; they thought light could travel any distance in no time at all. • In the 1670's Roemer was able to calculate a value for the speed of light by carefully studying the orbit of one of Jupiter’s moons, Io. He noticed that the time between the eclipses of the moons of Jupiter was less as the distance away from Earth is decreasing than when it is increasing. • In 1926 scientist Albert Michelson used the reflection from a rotating mirror on a distant mountain and measured the speed of light at 299,796 km/second • The current accepted value is 300,000,000 meters per second (3 x 108 m/s) or 186,000 miles per second. Light waves obey the wave equation, c = lf

6. Things the produce electromagnetic waves • Radio waves • electrons moving up and down an antenna • Visible Light • electrons changing energy states in an atom

7. Wave/Particle

8. Light and Energy • For waves, the amplitude or intensity is usually related to the energy of the wave • For light, this is not true. The energy of light waves was found to be directly related it is frequency. • An experiment demonstrating the photoelectric effect demonstrated the particle nature of light and that E = hf, where E is energy, h is Planks constant, and f is frequency. http://phet.colorado.edu/new/simulations/sims.php?sim=Photoelectric_Effect

9. The Photoelectric Effect • Laws of photoelectric emission • For a given metal and frequency of incident radiation, the rate at which photoelectrons are ejected is directly proportional to the intensity of the incident light. • For a given metal, there exists a certain minimum frequency of incident radiation below which no photoelectrons can be emitted. This frequency is called the threshold frequency. • Above the threshold frequency, the maximum kinetic energy of the emitted photoelectron is independent of the intensity of the incident light but depends on the frequency of the incident light. • The time lag between the incidence of radiation and the emission of a photoelectron is very small, less than 10-9 second The equation is , where h is Planck's constant, f is the frequency of the incident photon,Φ is the work function (sometimes denoted W instead), the minimum energy required to remove a delocalised electron from the surface of any given metal.

10. The Electromagnetic Spectrum The electromagnetic spectrum is the range of electromagnetic waves extending from radio waves to gamma rays Increasing frequency R O Y G B I V

11. The Visible Spectrum • We can only see a small part of the electromagnetic spectrum • The visible spectrum is a range of light waves extending in wavelength from about 400 to 700 nanometers. Increasing wavelength Increasing frequency Increasing energy

12. Things that can separate white light • Prism • Raindrops • CD’s • Diffraction Grating

13. Young’s Double-Slit Experiment • The wave theory of light came to prominence with Thomas Young’s double-slit experiment, performed in 1801. • The double-slit experiment proves that light has wave properties because it relies on the principles of constructive interference and destructive interference, which are unique to waves.

14. Single-Slit Diffraction

15. Diffraction Grating • A diffraction grating is a screen with a bunch of parallel slits, each spaced a distance d apart • The condition for maximum intensity is the same as that for a double slit. However, angular separation of the maxima is generally much greater because the slit spacing is so small for a diffraction grating.

16. Constructive and Destructive Interference • At any point P on the back screen, there is light from two different sources: the two slits. The line joining P to the point exactly between the two slits intersects the perpendicular to the front screen at an angle . • The light from the right slit—the bottom slit in our diagram—travels a distance of l = d sin more than the light from the other slit before it reaches the screen at the point P. • As a result, the two beams of light arrive at P out of phase by d sin. If d sin = (n + 1/2), where n is an integer, then the two waves are half a wavelength out of phase and will destructively interfere. • On the other hand, if d sin = n, then the two waves are in phase and constructively interfere, so the most light hits the screen at these points. Accordingly, these points are called the maxima of the pattern.

17. Polarization • As an electromagnetic wave traveled towards you, then you would observe the vibrations of the slinky occurring in more than one plane of vibration • A light wave which is vibrating in more than one plane is referred to as unpolarized light. • Light emitted by the sun, by a lamp in the classroom, or by a candle flame is unpolarized light

18. The Structure of the Atom and Emission • An atom is composed of electrons, protons and neutrons. • When an electron is raised to a higher energy level, the atom is said to be excited. • When the electron returns to a lower energy level, energy is released in the form of light. • Different transitions from high levels to low levels result in different colors of light.

19. The Kirchhoff-Bunsen Experiment • These two scientists found that burning chemicals over an open flame resulted in a spectrum with bright lines. • They found that each chemical element produced its own characteristic pattern of bright spectral lines.

20. Emission Spectra of Hydrogen Hot gas produces a bright line emission spectrum. RH is 1.09678 x 10-2 nm-1 Discrete Emission Spectrum Slit Film Low Density Glowing Hydrogen Gas Prism Photographic Film

21. Calculating the energy in a transition 1 eV = 1.6 x 10-19 J The Rydberg Equation: RH is 1.09678 x 10-2 nm-1

22. Every element can be “fingerprinted” by it spectra. Hydrogen Helium Oxygen Carbon

23. Incandescence • Hot, dense solids produce a continuous spectrum. • The brightness and color of light emitted by a hot object changes with its temperature. • Glowing object colors: • Reddish coolest glowing object • Orange-ish • Yellowish • White • Bluish  hottest glowing object Continuous Spectrum

24. Absorption Spectra • Cool gas in front of a continuous source of light produces an absorption line spectrum. • Fraunhofer lines in our Sun's spectrum showed that cool helium gas surrounds the Sun Absorption Spectrum

25. Absorption Spectra of Hydrogen Discrete Emission Spectrum Discrete Absorption Spectrum Slit Hydrogen Gas Film White Light Source Prism Photographic Film

26. Sources • Conceptual Physics by Paul Hewitt • www.physicsclassroom.com • http://observe.phy.sfasu.edu/courses/phy101/lectures101/