Wave Phenomena (topic 4 & 9) Flashcards

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1
Q

Equation for Simple Harmonic Motion

A

a = -w^2 x,

where
a = acceleration (ms^-2),
x = displacement from equilibrium (m),
w = angular frequency (rad * sec^-1)

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1
Q

Frequency of Oscilations equation

A

w = 2pi * f (frequency)(Hz) OR w = 2pi / T

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2
Q

SHM Displacement Equation

A

x = x0 sin (wt),

where
x = actual displacement (m),
x0 = max. displacement (m),
t = time (sec),
w = angular frequency (rad * sec^-1)

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3
Q

SHM Velocity Equation

A

v = w x0 cos(wt),

where
v = velocity,
w = angular frequency,
x0 = max. displacement,
t = time

OR

v = +-w squareroot x0^2 - x^2,

where
v = velocity,
w = angular frequency,
x0 = max. displacement,
x = actual displacement.

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4
Q

SHM Kinetic Energy Equation

A

Ek = 1/2 m w^2 (x0^2 - x^2),

where
Ek = kinetic energy,
m = mass,
w = angular frequency,
x0 = max. displacement,
x = actual displacement

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5
Q

SHM Total Energy Equation

A

ET = Ekmax = 1/2 m w^2 x0^2,

where
m = mass,
w = angular frequency,
x0 = max. displacement

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6
Q

Pendulum Equation

A

T = 2pi squareroot of l/g,

where
T =period (sec),
l = length of pendulum (m),
g = acceleration due to gravity on earth (ms^-2)

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7
Q

Spring Equation

A

T = 2pi squareroot of m/k,

where
T = period (sec),
m = mass (kg),
k = spring constant (Nm^-1)

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8
Q

Single Slit Diffraction Equation (first minimum)

A

theta = lambda / b,

where
theta = angle (radians),
lambda = wavelenth (m),
b = slit width (m).

***Use l = r * theta to find length,

where
l = lenth,
r = radius,
theta = angle

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9
Q

Multiple Slit Interference Equation

A

n * lambda = d sin theta,

where
n = order (n = 0,1,2,3,…),
lambda = wavelength (m),
d = slit separation (m)

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10
Q

Constructive Interference

A

path interference = n * lambda,

where
n = order (0,1,2,3,…),
lambda = wavelength (m)

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11
Q

Thin Film Interference (constructive)

A

2dn = (m + 1/2 lambda),

where
d = thin film thickness (m),
n = index of refraction,
m = order (0,1,2,3,…),
lambda = wavelength of light (m)

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12
Q

Thin Film Interference (destructive)

A

2dn = m lambda,

where
d = thin film thickness (m),
n = index of refraction,
m = order (0,1,2,3,…),
lambda = wavelelngth of light (m)

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13
Q

Thin Film Thickness Equation

A

d = 1/N,

where
d = thin film thickness,
N = diffraction grating

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14
Q

Resolution (Rayleigh Criterion)

A

Two objects are just resolved if theta = (1.22 * lambda) / b,

where
theta = angle between the two interferenc patterns (rad),
lambda = wavelength of light (m),
b = aperture width (m)

If:
theta is less than (1.22 * lambda)/b -> can’t tell them apart
theta is greater than or equal to (1.22 * lambda) / b -> can tell then apart

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15
Q

Resolution (Resolvance)

A

R = lambda / delta lambda = mN,

where
R = resolvance,
lambda = wavelength being investigated (m),
delta lambda = smallest possible resolvable wavelength difference (m),
m = diffraction order (0,1,2,3,…),
N = total number of slits being illuminated

16
Q

Doppler Effect Moving Source Equation

A

f’ = f (v / v +-us),

where
f’ = observed frequency (Hz),
f = emitted frequency (Hz),
v = speed of sound (ms^-1),
us = speed of source (ms^-1)

smaller lambda = larger frequency
coming towards = higher pitch (frequency)
going away = lower pitch (frequency)

17
Q

Astronomy Doppler Effect Equation

A

delta f / f = delta lambda / lambda approx. equal to v (speed) / c (speed of light)

18
Q

Wave equation

A

v = fλ or c = fλ (for light)

where
v = speed (ms^-1)
f = frequency (Hz or sec^-1)
λ = wavelength (m)
c = speed of light (ms-1)

19
Q

Frequency equation

A

f = 1 / T

where
f = frequency (Hz or sec^-1)
T = period (sec)

20
Q

Transverse waves

A

Direction of oscillation is perpendicular to the direction of travel

21
Q

Longitudinal waves

A

Direction of oscillation is parallel to the direction of travel

22
Q

Intensity is proportional to the amplitude squared

A

I ∝ A^2

23
Q

Intensity is inversely proportional to the square of the distance

A

I ∝ r^2

24
Q

Reflection

A

θ1 = θ2

25
Q

Critical angle

A

When the refracted angle is 90°

26
Q

Total internal reflection

A

Any greater angle of 90° refraction (gets reflected)

27
Q

Diffraction

A

When waves go through an aperture, they spread out

28
Q

d > λ

A

When the slit width or aperture is bigger than the wavelength, not much diffraction

29
Q

d ≤ λ

A

When the aperture is smaller or equal to the wavelength, more diffraction

30
Q

Interference

A

When two waves meet, they can superpose with each other

31
Q

Constructive interference

A

‘Add up’

32
Q

Destructive interference

A

‘Cancel out’

33
Q

Polarization

A

Plane of vibration of an electromagnetic wave (light)

34
Q

Standing waves

A

Frequency and amplitude are constant, two waves meeting in superposition (in opposite directions)

35
Q

Standing waves examples

A
  1. Fixed at both ends
  2. Open at one end, closed at the other
  3. Open at both ends
36
Q

For small θ

A

sin θ = θ