Ch 10 - WAVE OPTICS12th Physics
Corpuscular vs. Wave Theory of Light
What was the primary contradiction between Newton's corpuscular model and Huygens' wave theory regarding the speed of light in a denser medium?
What was the primary contradiction between Newton's corpuscular model and Huygens' wave theory regarding the speed of light in a denser medium?
Corpuscular Model (Descartes/Newton): Predicted that light bending towards the normal (refracting into a denser medium) meant its speed would be greater in the second medium.
Wave Theory (Huygens): Predicted that if light bends towards the normal, its speed must be less in the second medium.
Conclusion: Foucault's experiment (1850) definitively proved the wave theory correct; light travels slower in water than in air.
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The Wavefront
How is a wavefront physically defined, and what are its three primary shapes depending on the geometry of the source?
How is a wavefront physically defined, and what are its three primary shapes depending on the geometry of the source?
Definition: A wavefront is the locus of all particles of a medium oscillating in the same phase at a given instant.
1. Spherical Wavefront: Emanates from a point source of light.
2. Cylindrical Wavefront: Emanates from a linear source (like a narrow slit).
3. Plane Wavefront: Formed by a small portion of a spherical or cylindrical wavefront originating from a very distant source (like the Sun).
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Huygens' Principle
What are the two fundamental geometric assumptions of Huygens' principle used to determine wave propagation?
What are the two fundamental geometric assumptions of Huygens' principle used to determine wave propagation?
Assumption 1: Every point on a given primary wavefront acts as a fresh source of secondary wavelets, which spread out in all directions with the speed of the wave in that medium.
Assumption 2: The new position of the wavefront at any later instant is the forward tangential envelope of these secondary wavelets at that instant.
Boundary Condition: The backward propagation of wavelets (the backwave) is strictly assumed to have an amplitude of zero.
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Snell's Law via Wave Theory
Snell's Law via Wave Theory
State the standard formula for Snell's Law of refraction derived using the concept of wavefront velocities.
Variables & Units:
- = Angle of incidence (rad or degrees)
- = Angle of refraction (rad or degrees)
- = Speed of the wave in medium 1 and 2 (m/s)
- = Absolute refractive indices of medium 1 and 2
Conditions/Notes:
- The derivation relies on the geometric fact that the time taken by secondary wavelets to travel from the primary wavefront to the refracting surface is constant.
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Frequency & Wavelength upon Refraction
When a monochromatic light wave refracts from a rarer medium into a denser medium, how do its speed, wavelength, and frequency change?
When a monochromatic light wave refracts from a rarer medium into a denser medium, how do its speed, wavelength, and frequency change?
Speed (): Decreases () because the medium is optically denser.
Wavelength (): Decreases proportionally. The mathematical relation is .
Frequency (): Remains strictly constant. Frequency is an inherent characteristic of the oscillating source atoms, not the medium it travels through.
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Phase Reversal on Reflection (Stokes' Law)
What abrupt phase and path change occurs when a light wave is reflected from the boundary of an optically denser medium?
What abrupt phase and path change occurs when a light wave is reflected from the boundary of an optically denser medium?
Phase Change: When a wave is reflected from a denser medium (e.g., traveling in air and bouncing off glass), it suffers a sudden, abrupt phase change of radians ().
Path Difference Equivalent: This phase shift is mathematically equivalent to an additional optical path difference of .
Boundary Condition: A wave reflected from a rarer medium (e.g., traveling in glass and bouncing off air) suffers zero phase change.
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Principle of Superposition
What does the principle of superposition dictate when multiple light waves intersect at a common point in a medium?
What does the principle of superposition dictate when multiple light waves intersect at a common point in a medium?
It states that when two or more waves superimpose simultaneously at a point, the resultant displacement of the particle is exactly equal to the vector sum of the independent displacements produced by each individual wave.
Mathematically:
This principle forms the entire physical and mathematical foundation for both interference and diffraction phenomena.
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Fractional Doppler Shift
Fractional Doppler Shift
State the formula for the fractional change in frequency (Doppler shift) for light when the source velocity is small compared to the speed of light.
Variables & Units:
- = Change in frequency (Hz)
- = Original frequency (Hz)
- = Radial velocity of the source relative to the observer (m/s)
- = Speed of light in vacuum ()
Conditions/Notes:
- Valid strictly for non-relativistic speeds ().
- Sign Convention: is considered positive when the source moves away from the observer (yielding a negative frequency shift, i.e., Red Shift).
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Coherent vs. Incoherent Sources
What is the defining optical characteristic that strictly differentiates coherent light sources from incoherent ones?
What is the defining optical characteristic that strictly differentiates coherent light sources from incoherent ones?
Coherent Sources: Sources that continuously emit light waves of the exact same frequency (or wavelength) and maintain a strictly constant phase difference (which can be zero) over time.
Incoherent Sources: Sources where the phase difference between the emitted waves changes rapidly and randomly over time (e.g., two separate, independent sodium lamps illuminating a wall).
Result: Coherent sources produce stable interference patterns, whereas incoherent sources simply add up their overall average intensities () without forming sustained fringes.
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Constructive Interference
What specific conditions of phase difference and path difference must be met to achieve perfectly constructive interference (a bright fringe)?
What specific conditions of phase difference and path difference must be met to achieve perfectly constructive interference (a bright fringe)?
Phase Difference (): Must be an even integral multiple of .
Path Difference (): Must be a whole integral multiple of .
Result: The amplitudes sum up in phase, producing maximum light intensity. If the two sources have equal intensity (), the bright fringe has an intensity of .
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Destructive Interference
What specific conditions of phase difference and path difference strictly guarantee absolute destructive interference (a dark fringe)?
What specific conditions of phase difference and path difference strictly guarantee absolute destructive interference (a dark fringe)?
Phase Difference (): Must be an odd integral multiple of .
Path Difference (): Must be an odd multiple of .
Result: The wave amplitudes exactly oppose and cancel each other. If the two sources have equal intensity (), the resultant intensity drops perfectly to zero.
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Resultant Intensity of Superposing Waves
Resultant Intensity of Superposing Waves
State the general mathematical formula for the resultant intensity of two superposing coherent waves possessing a specific phase difference.
Variables & Units:
- = Resultant Intensity ()
- = Intensities of individual waves ()
- = Phase difference between the two waves at the point of observation (rad)
Conditions/Notes:
- The term is formally known as the interference term.
- For identical sources (), the formula simplifies beautifully to .
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Diffraction of Light
How is the diffraction of light defined, and under what strict dimensional condition does it become physically pronounced?
How is the diffraction of light defined, and under what strict dimensional condition does it become physically pronounced?
Definition: It is the phenomenon of light bending around the sharp corners of an obstacle or an aperture and physically spreading into the regions of the expected geometrical shadow.
Crucial Condition: Diffraction effects become distinctly noticeable and pronounced only when the size of the obstacle or aperture () is comparable to the wavelength () of the incident light ().
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Polarisation and Wave Nature
What specific property of light does the phenomenon of polarisation definitively prove, which directly distinguishes it from sound waves?
What specific property of light does the phenomenon of polarisation definitively prove, which directly distinguishes it from sound waves?
Transverse Nature: Polarisation provides conclusive proof that light is a transverse wave (specifically, a transverse electromagnetic wave).
Mechanism: In transverse waves, oscillations occur strictly perpendicular to the direction of propagation, allowing them to be mathematically restricted to a single plane.
Comparison: Longitudinal waves (like sound waves in air) inherently cannot be polarised because their particle oscillations occur strictly parallel to the direction of wave propagation.
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Unpolarised vs. Plane Polarised Light
What is the fundamental difference in the electric field oscillations between unpolarised natural light and plane-polarised light?
What is the fundamental difference in the electric field oscillations between unpolarised natural light and plane-polarised light?
Unpolarised Light: The electric field vectors vibrate rapidly and randomly in all possible directions within the transverse plane perpendicular to the direction of wave propagation.
Plane Polarised Light (Linearly Polarised): The electric field vectors are strictly restricted to vibrate in one single direction (one plane) that remains constant over time.
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Phase and Path Difference Relation
Phase and Path Difference Relation
State the core mathematical relation that directly converts a spatial path difference into an angular phase difference.
Variables & Units:
- = Phase difference (rad)
- = Path difference (m)
- = Wavelength of the wave (m)
Conditions/Notes:
- A spatial path difference of exactly one full wavelength () conceptually and mathematically corresponds to a phase shift of one complete cyclic rotation ( radians).
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Young's Double Slit Experiment (YDSE)
How did Thomas Young ingeniously solve the physical impossibility of finding two perfectly coherent independent light sources?
How did Thomas Young ingeniously solve the physical impossibility of finding two perfectly coherent independent light sources?
Wavefront Splitting: He passed monochromatic light from a single primary pinhole/slit () to illuminate two closely spaced secondary slits ( and ).
Phase Locking: Because the light at and originates from the exact same primary wavefront, any random, abrupt phase change in the original source manifests equally and simultaneously at and .
Result: and act as perfectly coherent sources locked in phase, successfully generating stable, observable interference fringes on the screen.
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Path Difference in YDSE
Path Difference in YDSE
State the geometric formula for calculating the path difference between the two light waves reaching an arbitrary point P on the screen in YDSE.
Variables & Units:
- = Path difference (m)
- = Distance of the observation point P from the central maximum (m)
- = Separation distance between the two slits (m)
- = Distance from the plane of the slits to the viewing screen (m)
Conditions/Notes:
- The formula strictly relies on two paraxial approximations: and , meaning the angle is extremely small so .
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Position of Bright Fringes (YDSE)
Position of Bright Fringes (YDSE)
State the formula for the linear position (distance from the center) of the n-th bright fringe (maximum) on the screen in YDSE.
Variables & Units:
- = Distance of the -th bright fringe from the central maximum (m)
- = Order of the bright fringe ()
- = Wavelength of light (m)
- = Distance to screen (m)
- = Slit separation (m)
Conditions/Notes:
- Derived by equating the path difference to the absolute condition for constructive interference ().
- At , , forming the Central Bright Fringe exactly on the perpendicular bisector.
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Position of Dark Fringes (YDSE)
Position of Dark Fringes (YDSE)
State the formula for the linear position of the n-th dark fringe (minimum) from the central maximum in YDSE.
Variables & Units:
- = Distance of the -th dark fringe from the central bright fringe (m)
- = Order of the dark fringe ()
- = Standard YDSE geometric parameters (m)
Conditions/Notes:
- Derived by equating the path difference to the absolute condition for destructive interference .
- The very first dark fringe flanking the center occurs at , meaning .
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Fringe Width in YDSE
Fringe Width in YDSE
State the standard formula calculating the linear width of an interference fringe.
Derivation
- The distance to the -th bright fringe is .
- The distance to the next adjacent bright fringe is .
- The width of a single dark fringe trapped between them is exactly .
- .
Variables & Units:
- = Fringe width (m)
- = Wavelength of the light (m)
- = Distance from the slit plane to the screen (m)
- = Separation distance between the two coherent slits (m)
Conditions/Notes:
- In Young's Double Slit Experiment, the widths of all bright fringes and all dark fringes are strictly equal.
- If the entire experimental setup is immersed in a liquid of refractive index , the wavelength drops to , and the new fringe width shrinks identically: .
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Lateral Shift due to a Glass Slab in YDSE
Lateral Shift due to a Glass Slab in YDSE
State the formula determining the lateral shift of the entire interference fringe pattern when a thin transparent plate is introduced in front of one of the slits.
Variables & Units:
- Shift = Linear distance the entire pattern moves (m)
- = Refractive index of the inserted transparent plate
- = Thickness of the plate (m)
- = Original fringe width (m)
Conditions/Notes:
- The pattern unequivocally shifts towards the side of the slit covered by the glass plate.
- The actual fringe width () remains absolutely unchanged.
- The optical path length increases, introducing an additional path difference of .
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Single Slit Diffraction - Minima
Single Slit Diffraction - Minima
State the mathematical condition for locating the dark bands (minima) in a single-slit Fraunhofer diffraction pattern.
Variables & Units:
- = Linear width of the single slit (m)
- = Angle of diffraction to the minimum (rad or degrees)
- = Order of the minimum (). Note:
- = Wavelength of the incident light (m)
Conditions/Notes:
- Contrast this heavily with YDSE: is the path difference condition for maxima in interference, but for minima in single-slit diffraction.
- Mechanically, the slit is theoretically divided into an even number of equal zones () that undergo complete destructive cancellation.
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Single Slit Diffraction - Secondary Maxima
Single Slit Diffraction - Secondary Maxima
State the mathematical condition for locating the secondary bright bands (maxima) in a single-slit diffraction pattern.
Variables & Units:
- = Linear width of the single slit (m)
- = Angle of diffraction to the maximum (rad or degrees)
- = Order of the secondary maximum ()
- = Wavelength of the incident light (m)
Conditions/Notes:
- These secondary maxima become progressively significantly weaker in intensity as increases because only a tiny unbound fraction of the slit (e.g., , ) contributes constructively while the rest cancels out.
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Width of Central Maximum (Single Slit)
Width of Central Maximum (Single Slit)
State the formula for the total linear width of the bright central maximum in a single-slit diffraction pattern.
Variables & Units:
- = Linear width of the central maximum on the screen (m)
- = Wavelength of the incident light (m)
- = Distance from the diffracting slit to the viewing screen (m)
- = Linear width of the slit (m)
Conditions/Notes:
- The central maximum is structurally exactly twice as wide as any of the secondary maxima (which have a width of ).
- Counter-intuitive note: If the physical slit is narrowed ( decreases), the central bright maximum optically widens (spreads out more on the screen).
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Angular Resolution of a Telescope
Angular Resolution of a Telescope
State Rayleigh's Criterion formula for the limit of resolution (angular separation) of a telescope.
Variables & Units:
- = Angular resolution / limit of resolution (rad)
- = Wavelength of incident light (m)
- = Diameter (aperture) of the objective lens (m)
Conditions/Notes:
- The formula determines the minimum angular separation required between two distant point sources (like stars) for them to be seen as distinct images.
- A larger diameter gives a smaller , which means higher resolving power.
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Limit of Resolution of a Microscope
Limit of Resolution of a Microscope
State the formula for the minimum separation distance between two point objects to be just resolved by a microscope.
Variables & Units:
- = Minimum separation distance (m)
- = Wavelength of light used (m)
- = Refractive index of the medium between the object and the objective lens
- = Semi-vertical angle subtended by the objective at the object (rad or degrees)
Conditions/Notes:
- The denominator term is known as the Numerical Aperture.
- Using an oil-immersion objective increases , which decreases and strictly increases resolving power.
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Fresnel Distance
Fresnel Distance
State the formula for the Fresnel distance, beyond which the spreading of light due to diffraction becomes significant.
Variables & Units:
- = Fresnel distance (m)
- = Size (width) of the aperture or slit (m)
- = Wavelength of the incident light (m)
Conditions/Notes:
- This distance mathematically dictates the validity of ray optics.
- For distances , diffraction spreading is negligible, and light travels roughly in straight lines. For , wave optics must be strictly applied.
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Malus's Law
Malus's Law
State the mathematical law that determines the intensity of polarised light transmitted through an analyser.
Derivation
- Let the electric field amplitude of the polarised light incident on the analyser be .
- The analyser only transmits the component of the electric field parallel to its pass-axis, which is .
- Intensity is directly proportional to the square of the amplitude ().
- Therefore, .
- Since , we obtain .
Variables & Units:
- = Transmitted intensity through the analyser ()
- = Maximum intensity of the incident polarised light ()
- = Angle between the pass-axes of the polariser and the analyser (rad or degrees)
Conditions/Notes:
- If (parallel axes), (maximum transmission).
- If (crossed polaroids), (complete darkness).
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Doppler Effect in Light
In astronomy, what do the terms 'Red Shift' and 'Blue Shift' signify regarding the relative motion of a celestial body?
In astronomy, what do the terms 'Red Shift' and 'Blue Shift' signify regarding the relative motion of a celestial body?
Red Shift: Occurs when the source is moving away from the observer. The apparent wavelength increases, shifting the spectral lines towards the red end of the visible spectrum.
Blue Shift: Occurs when the source is moving towards the observer. The apparent wavelength decreases, shifting the spectral lines towards the violet/blue end of the spectrum.
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Brewster's Law
Brewster's Law
State the mathematical relationship connecting Brewster's angle of incidence to the refractive index of the reflecting medium.
Derivation
- Apply Snell's Law at the interface: .
- At Brewster's angle, the reflected and refracted rays are at . Therefore, .
- Substitute into Snell's Law: .
- Since , this becomes .
- Rearranging gives: .
- Thus, .
Variables & Units:
- = Brewster's Angle / Polarising Angle (rad or degrees)
- (or ) = Refractive index of the denser reflecting medium relative to the rarer incident medium (dimensionless)
Conditions/Notes:
- Assumes unpolarised light is incident on the interface.
- If a polariser blocks the component perpendicular to the plane of incidence, and light strikes at , there will be zero reflection (100% transmission).
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YDSE with White Light
What is the physical nature of the interference pattern observed if the monochromatic source in YDSE is entirely replaced by a white light source?
What is the physical nature of the interference pattern observed if the monochromatic source in YDSE is entirely replaced by a white light source?
Central Fringe: The central maximum remains perfectly white because all visible component colors have zero path difference there and constructively interfere simultaneously.
Coloured Fringes: On either side of the center, a few coloured fringes will uniquely emerge.
Order of Colours: The inner edge of the first fringe closest to the central white fringe will appear Red (because Blue destructively interferes first at a smaller angle, since ).
After a few fringes, the wavelengths overlap completely out of phase and the pattern washes out into uniform white illumination.
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Ratio of Maximum to Minimum Intensity
Ratio of Maximum to Minimum Intensity
State the mathematical formula for the ratio of maximum to minimum intensity in an interference pattern, in terms of individual intensities and amplitudes.
Variables & Units:
- = Maximum intensity at constructive interference ()
- = Minimum intensity at destructive interference ()
- = Intensities of individual coherent waves
- = Amplitudes of individual coherent waves
Conditions/Notes:
- The Average Intensity over the entire pattern is given by .
- A highly tested concept for calculating amplitude ratios given fringe visibility.
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Interference vs. Diffraction
What is the fundamental physical distinction between an interference pattern and a single-slit diffraction pattern?
What is the fundamental physical distinction between an interference pattern and a single-slit diffraction pattern?
Interference (e.g., YDSE): Results from the superposition of waves coming from two distinctly separate coherent sources. The fringes typically have perfectly equal intensity and equal width.
Diffraction: Results from the superposition of a continuous family of secondary wavelets originating from different parts of the exact same wavefront (like across a single slit). The central maximum is twice as wide and far brighter than all secondary maxima, whose intensities fall off rapidly.
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Unpolarised Light through a Polariser
When an unpolarised light beam of intensity passes through a single ideal polaroid, what happens to its transmitted intensity?
When an unpolarised light beam of intensity passes through a single ideal polaroid, what happens to its transmitted intensity?
Transmitted Intensity: It becomes exactly half of the initial incident intensity ().
Reason: A polaroid only allows the component of the electric field parallel to its unique pass-axis to transmit. Since unpolarised light oscillates symmetrically and randomly in all directions, averaging the square of the cosine over all angles yields exactly . Thus, exactly 50% of the wave's energy is absorbed.
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Coincidence of Fringes in YDSE
Coincidence of Fringes in YDSE
State the condition used to calculate the exact exact position where the bright fringes of two different wavelengths coincide in a double-slit experiment.
Variables & Units:
- = Order of the bright fringes for light 1 and light 2 (integers)
- = Wavelengths of the two monochromatic light beams (m)
Conditions/Notes:
- Derived from equating the linear positions: .
- This equation is fundamentally used to find the lowest integer combination of and to locate the nearest point from the central maximum where overlapping occurs.
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Polarisation by Scattering (Sky Light)
Why does the scattered blue light from the sky appear partially or completely plane-polarised when viewed at a angle from the Sun?
Why does the scattered blue light from the sky appear partially or completely plane-polarised when viewed at a angle from the Sun?
Mechanism: Unpolarised incident sunlight causes the electrons in atmospheric gas molecules to oscillate in both transverse directions (in the plane perpendicular to the sun's rays).
The 90-Degree Effect: Accelerating charges do not radiate energy along their own axis of oscillation. An observer looking at exactly to the incident sunlight only receives radiation from electrons oscillating perpendicular to the observer's line of sight.
Result: The radiation component parallel to the observer's line of sight contributes zero intensity. Thus, the scattered light viewed at is completely linearly polarised.
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Number of Fringes Shifted by a Glass Slab
Number of Fringes Shifted by a Glass Slab
State the formula calculating the exact number of fringes by which the central maximum shifts when a thin transparent slab is introduced in front of one slit.
Variables & Units:
- = Number of fringes shifted (dimensionless)
- = Refractive index of the transparent slab
- = Thickness of the slab (m)
- = Wavelength of the incident light in a vacuum/air (m)
Conditions/Notes:
- The total extra optical path difference introduced is .
- Equating this to the condition for bright fringes () yields the formula.
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Polarisation by Reflection
What strictly required geometric condition between the reflected and refracted rays guarantees that the reflected light is completely plane-polarised?
What strictly required geometric condition between the reflected and refracted rays guarantees that the reflected light is completely plane-polarised?
Condition: The reflected ray and the refracted ray must be exactly perpendicular () to each other.
Outcome: At this specific angle of incidence (Brewster's angle), the reflected light is 100% plane-polarised, with its electric field vector vibrating strictly perpendicular to the plane of incidence.
Note: The refracted (transmitted) ray remains only partially polarised.
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Metamaterials & Negative Refractive Index
According to V. Veselago's postulate for metamaterials, what dictates the refractive index of a medium where both relative permittivity and permeability are less than zero?
According to V. Veselago's postulate for metamaterials, what dictates the refractive index of a medium where both relative permittivity and permeability are less than zero?
Postulate: For artificially produced metamaterials where relative permittivity () and relative permeability () are both negative, the refractive index is strictly defined as .
Optical Consequence: When light enters such a medium from air, the phase travels away from the direction of propagation. A ray entering from the 1st quadrant will anomalously refract into the 3rd quadrant rather than the usual 4th quadrant, although Snell's Law mathematically still holds.
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Resolving Power of a Telescope
Resolving Power of a Telescope
State the formula for the resolving power of a telescope, defined as the reciprocal of its limit of angular resolution.
Variables & Units:
- RP = Resolving Power (rad)
- = Diameter (aperture) of the objective lens or mirror (m)
- = Wavelength of the incident light (m)
Conditions/Notes:
- Resolving Power directly indicates a telescope's ability to clearly separate two closely spaced celestial bodies.
- To maximize RP, telescopes are built with massive objective diameters ().
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Resolving Power of a Microscope
Resolving Power of a Microscope
State the formula for the resolving power of a microscope, defined as the reciprocal of the minimum resolvable separation distance.
Variables & Units:
- RP = Resolving Power (m)
- = Refractive index of the medium between the objective lens and object
- = Semi-vertical angle subtended by the objective at the object
- = Wavelength of light used (m)
Conditions/Notes:
- The denominator term is the actual spatial resolution limit.
- Using an oil-immersion objective increases , thereby significantly boosting the Resolving Power.
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Percentage of Polarisation
Percentage of Polarisation
State the formula used to calculate the percentage of polarisation of a partially polarised light beam passing through an analyser.
Variables & Units:
- = Percentage of polarisation (%)
- = Maximum transmitted intensity observed upon rotating the analyser ()
- = Minimum transmitted intensity observed upon rotating the analyser ()
Conditions/Notes:
- If , the light is 100% plane-polarised.
- If , the percentage is 0%, indicating completely unpolarised light.
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