Chapter 38 Diffraction Patterns and Polarization.

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Presentation transcript:

Chapter 38 Diffraction Patterns and Polarization

Diffraction and Polarization Diffraction can be described only with a wave model for light. A diffraction pattern occurs when the light from an aperture is allowed to fall on a screen.  The features of this diffraction pattern can be investigated. Under certain conditions transverse waves with electric field vectors in all directions can be polarized in various ways.  Only certain directions of the electric field vectors are present in the polarized wave. Introduction

Diffraction Light of wavelength comparable to or larger than the width of a slit spreads out in all forward directions upon passing through the slit. This phenomena is called diffraction.  This indicates that light spreads beyond the narrow path defined by the slit into regions that would be in shadow if light traveled in straight lines. Section 38.1

Diffraction Pattern A single slit placed between a distant light source and a screen produces a diffraction pattern.  It will have a broad, intense central band  Called the central maximum  The central band will be flanked by a series of narrower, less intense secondary bands.  Called side maxima or secondary maxima  The central band will also be flanked by a series of dark bands.  Called minima Section 38.1

Diffraction Pattern, Single Slit The diffraction pattern consists of the central maximum and a series of secondary maxima and minima. The pattern is similar to an interference pattern. Section 38.1

Diffraction Pattern, Object Edge This shows the upper half of the diffraction pattern formed by light from a single source passing by the edge of an opaque object. The diffraction pattern is vertical with the central maximum at the bottom. Section 38.1

Confirming Wave Nature Ray optics would predict a dark spot in the center. Wave theory predicts the presence of the center spot. There is a bright spot at the center.  Confirms wave theory The circular fringes extend outward from the shadow’s edge. Section 38.1

Fraunhofer Diffraction Pattern A Fraunhofer diffraction pattern occurs when the rays leave the diffracting object in parallel directions.  Screen very far from the slit  Could be accomplished by a converging lens Section 38.2

Fraunhofer Diffraction Pattern Photo A bright fringe is seen along the axis (θ = 0). Alternating bright and dark fringes are seen on each side. Section 38.2

Diffraction vs. Diffraction Pattern Diffraction refers to the general behavior of waves spreading out as they pass through a slit. A diffraction pattern is actually a misnomer that is deeply entrenched.  The pattern seen on the screen is actually another interference pattern.  The interference is between parts of the incident light illuminating different regions of the slit. Section 38.2

Single-Slit Diffraction The finite width of slits is the basis for understanding Fraunhofer diffraction. According to Huygens’s principle, each portion of the slit acts as a source of light waves. Therefore, light from one portion of the slit can interfere with light from another portion. The resultant light intensity on a viewing screen depends on the direction θ. The diffraction pattern is actually an interference pattern.  The different sources of light are different portions of the single slit. Section 38.2

Single-Slit Diffraction, Analysis All the waves are in phase as they leave the slit. Wave 1 travels farther than wave 3 by an amount equal to the path difference.  (a/2) sin θ If this path difference is exactly half of a wavelength, the two waves cancel each other and destructive interference results. In general, destructive interference occurs for a single slit of width a when sin θ dark = mλ / a.  m = ±1, ±2, ±3, … Section 38.2

Single-Slit Diffraction, Intensity The general features of the intensity distribution are shown. A broad central bright fringe is flanked by much weaker bright fringes alternating with dark fringes. Each bright fringe peak lies approximately halfway between the dark fringes. The central bright maximum is twice as wide as the secondary maxima. There is no central dark fringe.  Corresponds to no m = 0 in the equation Section 38.2

Intensity, equation The intensity can be expressed as Minima occur at Section 38.2

Intensity, final Most of the light intensity is concentrated in the central maximum. The graph shows a plot of light intensity vs. (  ) a sin  Section 38.2

Intensity of Two-Slit Diffraction Patterns When more than one slit is present, consideration must be made of  The diffraction patterns due to individual slits  The interference due to the wave coming from different slits The single-slit diffraction pattern will act as an “envelope” for a two-slit interference pattern. Section 38.2

Intensity of Two-Slit Diffraction Patterns, Equation To determine the maximum intensity:  The factor in the square brackets represents the single-slit diffraction pattern.  This acts as the envelope.  The two-slit interference term is the cos 2 term. Section 38.2

Intensity of Two-Slit Diffraction Patterns, Graph of Pattern The broken blue line is the diffraction pattern. The brown curve shows the cos 2 term.  This term, by itself, would result in peaks with all the same heights.  The uneven heights result from the diffraction term (square brackets in the equation). Section 38.2

Two-Slit Diffraction Patterns, Maxima and Minima To find which interference maximum coincides with the first diffraction minimum.  The conditions for the first interference maximum  d sin θ = m λ  The conditions for the first diffraction minimum  a sin θ = λ Section 38.2

Resolution The ability of optical systems to distinguish between closely spaced objects is limited because of the wave nature of light. If two sources are far enough apart to keep their central maxima from overlapping, their images can be distinguished.  The images are said to be resolved. If the two sources are close together, the two central maxima overlap and the images are not resolved. Section 38.3

Resolved Images, Example The images are far enough apart to keep their central maxima from overlapping. The angle subtended by the sources at the slit is large enough for the diffraction patterns to be distinguishable. The images are resolved. Section 38.3

Images Not Resolved, Example The sources are so close together that their central maxima do overlap. The angle subtended by the sources is so small that their diffraction patterns overlap. The images are not resolved. Section 38.3

Resolution, Rayleigh’s Criterion When the central maximum of one image falls on the first minimum of another image, the images are said to be just resolved. This limiting condition of resolution is called Rayleigh’s criterion. Section 38.3

Resolution, Rayleigh’s Criterion, Equation The angle of separation, θ min, is the angle subtended by the sources for which the images are just resolved. Since λ << a in most situations, sin θ is very small and sin θ ≈ θ. Therefore, the limiting angle (in rad) of resolution for a slit of width a is To be resolved, the angle subtended by the two sources must be greater than θ min. Section 38.3

Circular Apertures The diffraction pattern of a circular aperture consists of a central bright disk surrounded by progressively fainter bright and dark rings. The limiting angle of resolution of the circular aperture is  D is the diameter of the aperture. Section 38.3

Circular Apertures, Well Resolved The sources are far apart. The images are well resolved. The solid curves are the individual diffraction patterns. The dashed lines are the resultant pattern. Section 38.3

Circular Apertures, Just Resolved The sources are separated by an angle that satisfies Rayleigh’s criterion. The images are just resolved. The solid curves are the individual diffraction patterns. The dashed lines are the resultant pattern. Section 38.3

Circular Apertures, Not Resolved The sources are close together. The images are unresolved. The solid curves are the individual diffraction patterns. The dashed lines are the resultant pattern. The pattern looks like that of a single source. Section 38.3

Resolution, Example Pluto and its moon, Charon Left: Earth-based telescope is blurred Right: Hubble Space Telescope clearly resolves the two objects Section 38.3