Overview
Refraction is the bending of light as it passes from one medium to another. Lenses use refraction to form images and are essential components in cameras, eyeglasses, microscopes, and telescopes.
Index of Refraction
n=vc
Where:
- c = speed of light in vacuum (3×108 m/s)
- v = speed of light in medium
- n≥1 (n=1 for vacuum)
Common Values
| Material | n |
|---|
| Vacuum | 1.00 |
| Air | 1.0003 |
| Water | 1.33 |
| Glass | 1.5 |
| Diamond | 2.42 |
Snell's Law
n1sin(θ1)=n2sin(θ2)
Where:
- n1,n2 = indices of refraction
- θ1 = angle of incidence
- θ2 = angle of refraction
Bending Direction
- From less dense to more dense (n1<n2): bends toward normal
- From more dense to less dense (n1>n2): bends away from normal
Total Internal Reflection
Occurs when light goes from denser to less dense medium at angles greater than critical angle.
Critical Angle
sin(θc)=n1n2(for n1>n2)
Applications: fiber optics, prisms, diamond brilliance
Lenses
Converging (Convex) Lens
- Thicker in the middle
- Positive focal length
- Converges parallel rays to focal point
Diverging (Concave) Lens
- Thinner in the middle
- Negative focal length
- Diverges parallel rays (appear to come from focal point)
Lensmaker's Equation
f1=(n−1)(R11−R21)
Where R1,R2 are radii of curvature of the surfaces.
Thin Lens Equation
do1+di1=f1
Same as mirror equation!
Magnification
m=hohi=−dodi
Same conventions as mirrors:
- m>0: upright
- m<0: inverted
- ∣m∣>1: enlarged
Converging Lens - Image Formation
| Object Position | Image Position | Image Type |
|---|
| Beyond 2F | Between F and 2F | Real, inverted, diminished |
| At 2F | At 2F | Real, inverted, same size |
| Between F and 2F | Beyond 2F | Real, inverted, enlarged |
| At F | At infinity | — |
| Inside F | Same side | Virtual, upright, enlarged |
Diverging Lens - Image Formation
- Always virtual
- Always upright
- Always diminished
- Between lens and F (same side as object)
Power of a Lens
P=f1
Unit: Diopter (D) = m⁻¹
- Positive P: converging lens
- Negative P: diverging lens
Lenses in Combination
Close Together
Ptotal=P1+P2+P3+⋯
feq1=f11+f21+⋯
Separated by Distance d
Use image from first lens as object for second.
Ray Diagrams for Lenses
Converging Lens Rules
- Parallel ray → refracts through F (far side)
- Ray through F (near side) → refracts parallel
- Ray through center → passes straight through
Diverging Lens Rules
- Parallel ray → refracts as if from F (near side)
- Ray toward F (far side) → refracts parallel
- Ray through center → passes straight through
Examples
Example 1: Snell's Law
Light goes from air to glass (n=1.5) at 45°.
sin(θ2)=n2n1sin(θ1)=1.51×sin(45°)=1.50.707=0.471
θ2=28.1°
Example 2: Critical Angle
Find critical angle for glass-air interface (nglass=1.5).
sin(θc)=nglassnair=1.51=0.667
θc=41.8°
Example 3: Converging Lens - Real Image
A lens (f=20 cm) has an object at do=60 cm.
di1=f1−do1=201−601=603−601=602
di=30 cm (real, opposite side)
m=−6030=−0.5 (inverted, diminished)
Example 4: Converging Lens - Virtual Image
Same lens, object at do=10 cm (inside F).
di1=201−101=201−202=−201
di=−20 cm (virtual, same side)
m=−10−20=2 (upright, magnified)
Example 5: Diverging Lens
A lens (f=−15 cm) has an object at do=30 cm.
di1=−151−301=−302−301=−303
di=−10 cm (virtual, same side)
m=−30−10=0.33 (upright, diminished)
Example 6: Lens Combination
Two lenses (f1=10 cm, f2=20 cm) are in contact.
P=0.11+0.21=10+5=15 D
f=151 m=6.67 cm
Example 7: Vision Correction
A nearsighted person can't see beyond 100 cm. What lens corrects to infinity?
Object at infinity should form image at 100 cm (far point):
∞1+−11=f1
f=−1 m=−100 cm
P=−1 D (diverging lens)
Sign Convention Summary
| Quantity | Positive | Negative |
|---|
| do | Object in front | Object behind |
| di | Image behind (real) | Image in front (virtual) |
| f | Converging lens | Diverging lens |
| R | Center on opposite side | Center on same side |