Optics Final
PHYSICS 1220
March 1997
- A plano-convex lens is placed on a flat glass surface and
illuminated with light from below as shown in the diagram below (the
angles are exaggerated for clarity). A set of circular fringes is seen
by an observer looking straight down. The surface of the convex side of
the lens is given by y = bx2, where b = 1.00 × 10-4
cm-1 and x and y are in centimetres. The light is
monochromatic with λ = 579.0 nm.
(a) Is the centre of the lens dark or bright? Explain.
(b) What is the linear distance (i.e. Δx)
of the m = 3 and m = 4 bright fringes.
(c) If the lens is 5.00 cm wide, how many bright fringes can be seen in
total?
- A N-slit grating produces the pattern on a screen 2.00 m distant.
A portion of the pattern is shown below (The thick black lines
represent maxima and the thin black lines represent secondary maxima).
The light source had a wavelength of 555.0 nm.
(a) What was N (i.e. how many slits are there)? Explain how you can
tell.
(b) What is the spacing of the slits?
(c) What would the width of the slits be for the rightmost and leftmost
maxima in the diagram side to disappear but leave the rest visible?
- (a) Two converging are used to make a telescope. The lenses are
92 cm apart and the telescope magnifies objects 200 times. What are the
focal lengths of the lenses? Specify which is the objective and which
is the eyepiece.
(b) How much energy would a 30 × 10-12 m photon
lose in a collision with a stationary electron, if the photon is
scattered at 55°? What would be the
velocity of the electron after the collision?
- A thin layer of oil (t = 500 nm, noil = 1.46) is coated
on a glass slide (nglass = 1.80). White light (all
wavelengths between 400 nm and 700 nm) shines on the oil from above in
diagram (a) and through the oil from below in diagram (b). In each
case, determine which wavelengths are enhanced and which are
diminished.
- In the diagram below, an object of height h = 0.500 cm is placed
30.0 cm to the left of the convex lens.
(a) Locate the final image.
(b) Characterize the final image and determine its size.
(c) Sketch a ray diagram on the diagram.
- (a) A beam of aluminum atoms is used to "dope" a semiconductor to
give it the proper electrical properties. If the atoms' velocity is
required to be (4.5000 ± 0.00001) × 104 m/s, how
accurately can the atoms be localized? The mass of a mole of aluminum
atoms is 26.98 g and a mole is 6.022 × 1023.
(b) The tungsten filament in a 100 Watt lightbulb burns at a
temperature of 3200 Kelvin. Treating the filament like a blackbody,
what is the surface area of the filament? Note that this is an
overestimate since not all the 100 W goes into producing light. What is
the peak wavelength emitted by the filament?
- (a) Lithium, beryllium, and Mercury have work functions of 2.3
eV, 3.9 eV, and 4.5 eV, respectively. If 400-nm light is incident on
each of these metals, determine (i) which metals will release
photoelectrons, and (ii) the maximum kinetic energy for the
photoelectrons in each case.
(b) Lithium has three protons in its nucleus. If it is ionized
to Li++, what is the wavelength of light emitted when its remaining
electron undergoes a transition from n = 6 state to n = 2 state?
Formulas
Reflection, Refraction, & Polarization:
| θi = θr |
n = c/v |
n1sinθ1 = n2sinθ2 |
| sinθcritical= n2/n1 |
I = I0cos2θ |
tanθp = nlower/nupper |
Mirrors & Lenses:
| f = ½R |
1/o + 1/i = 1/f |
1/fcombined = 1/f1 + 1/f2 |
| dapparent = -n2dactual/n1 |
M = -i/o |
|
| Mirrors |
Lenses |
| o |
= + object in front of mirror |
o |
= + object on incident side |
| o |
= - object is behind mirror |
o |
= - object on transmission side |
| i |
= - image is behind mirror |
i |
= + image is on transmission side |
| i |
= + image is in front of mirror |
i |
= - image on incident side side |
| f,R |
= + concave side is mirror |
f |
= + converging lens, centre is thicker |
| f,R |
= - convex side is mirror |
f |
= - diverging lens, centre is thin |
Optical Instruments:
| Msimple = θ/θo = xNP/f |
f-number = f/D |
| Lfilm µ ID2t |
MMicroscope = -(L/fobjective)(xNP/feyepiece) |
| MTelescope = -fobjective/feyepiece |
Thin Films
|
δreflection = 0 |
δreflection = π |
|
| C.I. |
2t/λ' = m |
2t/λ' = m + ½ |
m = 0,1,2,... |
| D.I. |
2t/λ' = m + ½ |
2t/λ' = m |
Interference and Diffraction
| C.I. |
dsinθ/λ
= m |
m = 0,1,2,... |
| D.I. |
dsinθ/λ
= m + ½ |
| y = mλL/d for small angles |
asinθ/λ
= m |
m = 1,2,3,... |
| I = 4I0cos(δ/2)sin2(β)/β2 |
δ = 2πdsinθ/λ |
β = πasinθ/λ |
| αc ≈
1.22λ/D |
R = λ/Δλ = mN |
Black Body Radiation
| λmax = 2.898 mm-K/T |
S = ΣT4 |
Σ = 5.67 × 10-8 W/K4m2 |
Photoelectric Effect, X-Rays, and Compton Scattering
| c = fλ |
E = hf |
p = h/λ |
| KEmax = eV0 |
KE = hf - φ |
λmin = hc/eV |
| Δλ = λc(1-cosθ) |
λc = 2.43 × 10-3
nm |
λ = h/mv |
Spectral Lines and the Atom
| En = -(13.6eV)Z2/n2 |
ΔxΔp ≥ h / 4π |
λ = h/p |
| p = mv |
E = p2/2m |
|
Miscellaneous
| visible light : 400 nm ≤ λ ≤ 700 nm |
melectron = 9.11 × 10-31 kg |
| h = 6.626 × 10-34 J-s |
1 eV = 1.602 × 10-19 J |
| hc = 1240 nm-eV |
hbar = h/2π |
| c = 2.998 × 108 m/s |
|
Questions? mike.coombes@kwantlen.ca