agenda chapter 13 problem 28 - sfsu physics & astronomy
TRANSCRIPT
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Agenda
• Today: HW quiz, More simple harmonic motion and waves
• Thursday: More waves • Midterm scores will be posted by
Thursday.
Chapter 13 Problem 28
Calculate the buoyant force due to the surrounding air on a man weighing 800N. Assume his average density is 1,000 kg/m3, about the same as water.
Density of air: 1.2 kg/m3 ρ = m/V FB = mliquidg
Frequency and Period The frequency of oscillation depends on physical properties of the oscillator; it does not depend on the amplitude of the oscillation.
f = 12π
km
f = 12π
gL
Equations of Motion for SHM:
• Acceleration is NOT constant! We can’t use our equations from kinematics.
x(t) = A cos (2π f t) v(t) = -vmax sin (2π f t) vmax = 2π f A a(t) = -amax cos (2π f t) amax = (2π f)2 A
What if we have friction or drag?
• This is called a “damped” oscillation: the amplitude will steadily decrease over time
• Spring: eventually will resettle back at equilibrium (friction with sliding surface, air resistance, friction at attachments)
• Pendulum: eventually will stop swinging (air resistance, friction at attachments)
Driven Oscillations; Resonance
• Imagine pushing a child on a swingset, applying force on every swing. – What if you push at exactly the right time, with
exactly the right force one every swing? – This “exact right time” is the resonant
frequency • Example: Conservation of energy problem
from the third midterm.
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Energy Changes
• Mass-on-a-spring: Exchange between kinetic energy (½ mv2) and potential spring energy (½ kx2)
• Pendulum: Exchange between kinetic energy (½ mv2) and gravitational potential energy (mgh)
• This provides a faster way to find the position or velocity of the oscillator at a particular time!
Example: A 0.5-kg, 0.75-m pendulum is pulled back at an
angle of 10º. • What are the frequency and period of the
pendulum? • If it just skims the ground at the bottom of
the swing, how much energy does the pendulum have?
• How fast is it going at the bottom of its swing?
Properties of Waves
• Wavelength is the distance between two wave peaks
• Frequency is the number of times per second that a wave vibrates up and down
wave speed = wavelength x frequency
More Wave Properties
• Amplitude: Distance from midpoint to crest of wave
• Period: Time to complete one vibration
Speed of a Wave
• v = λƒ = λ/T – Is derived from the basic speed equation of
distance/time • This is a general equation that can be
applied to many types of waves • For sound in air, v = 343 m/s • For light in a vacuum, v = c = 3.0 x 108 m/s
Types of Waves
• Transverse Waves: like ocean waves or waves created by shaking a string
• Longitudinal Waves: compression waves, such as sound
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Types of Waves – Transverse
• In a transverse wave, each element that is disturbed moves in a direction perpendicular to the wave motion
Types of Waves – Longitudinal
• In a longitudinal wave, the elements of the medium undergo displacements parallel to the motion of the wave
• A longitudinal wave is also called a compression wave
What exactly is doing the waving?
• Many waves require a medium: substance or object to move around – Sound waves – Water waves – Waves in a string – Waves in a spring/slinky
• Waves transmit energy without moving the entire medium through space
Agenda
• Today: Wave speed, sound vs. light, interference and standing waves
• Tuesday: HW #12 quiz, more superposition and interference, doppler effect
Waveform – A Picture of a Wave
• The brown curve is a “snapshot” of the wave at some instant in time
• The blue curve is later in time
• The high points are crests of the wave
• The low points are troughs of the wave
Sinusoidal Waves
• A wave can take on a variety of shapes, we’ll mostly look at sinusoidal waves
• These waveforms can be described by a sine function that changes in both space and time:
y(x, t) = Acos 2π x
λ+tT
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Longitudinal Wave Represented as a Sine Curve
• A longitudinal wave can also be represented as a sine curve
• Compressions correspond to crests and stretches correspond to troughs
• Also called density waves or pressure waves
Waves Lecture-Tutorial
• Work with a partner or two • Read directions and answer all questions
carefully. Take time to understand it now! • Come to a consensus answer you all agree
on before moving on to the next question. • If you get stuck, ask another group for help. • If you get really stuck, raise your hand and I
will come around.
Speed of a Wave on a String
• The speed on a wave stretched under some tension, F
– µ is called the linear density – F is the tension force in the string
• The speed depends only upon the properties of the medium through which the disturbance travels
F mv where
Lµ
µ= =
Speed of sound waves • “Room temperature” air allows sound waves
to travel at a speed of about 343 m/s. • Temperature of air can change the speed of
sound! – General rule of thumb: sound travels more slowly
in cold air, faster in hot air – Determine distance to a lightning strike by
counting seconds until you hear the thunder (every 5 s ~ 1 mile)
– Unless otherwise specified, assume room temperature air.
Sound waves:
• Human range of hearing is from about 20-20,000 Hz
• Frequency pitch
Example: A violin string playing an “A” note vibrates at a frequency of
440 Hz. It has a linear density of µ = 7 x 10-4 kg/m.
• What is the wave speed if the string is under a tension of 10 N?
• What is the wavelength in the string? • What is the wavelength of the 440 Hz
sound wave travelling through the air?
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Sound vs. Light
• Sound waves and light waves are not the same thing!
• You don’t actually hear radio waves, you hear sound waves that were picked up by the radio
• Ears are sensitive to vibrations/compressions in the air
• Eyes are sensitive to light waves (but only a very small portion of them…)
Wave Model of Light
• Can characterize light as either a wave or a particle (modern physics says both!)
• Light is electromagnetic radiation: waves that arise from the
• Light needs no medium to travel! (Michelson & Morley showed this in 1887, effectively disproving the existence of the “luminiferous ether”)
The Electromagnetic Spectrum
• Gamma Rays • X-rays • Ultraviolet Light • Visible Light (ROY G BIV)
– λ = 400-700nm • Infrared Light • Microwaves & Radio Waves
Interference & Superposition • Two traveling waves can meet and pass through
each other without being destroyed or even altered
• Waves obey the Superposition Principle – If two or more traveling waves are moving through a
medium, the resulting wave is found by adding together the displacements of the individual waves point by point
– Actually only true for waves with small amplitudes
Constructive Interference
• Two waves, a and b, have the same frequency and amplitude – Are in phase
• The combined wave, c, has the same frequency and a greater amplitude
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Constructive Interference in a String
• Two pulses are traveling in opposite directions • The net displacement when they overlap is the
sum of the displacements of the pulses • Note that the pulses are unchanged after the
interference
Destructive Interference
• Two waves, a and b, have the same amplitude and frequency
• They are 180° out of phase
• When they combine, the waveforms cancel
Destructive Interference in a String
• Two pulses are traveling in opposite directions • The net displacement when they overlap is
decreased since the displacements of the pulses subtract
• Note that the pulses are unchanged after the interference
Reflection of Waves – Fixed End
• Whenever a traveling wave reaches a boundary, some or all of the wave is reflected
• When it is reflected from a fixed end, the wave is inverted
• The shape remains the same
Reflected Wave – Free End
• When a traveling wave reaches a boundary, all or part of it is reflected
• When reflected from a free end, the pulse is not inverted
Standing Waves on a String
• Nodes must occur at the ends of the string because these points are fixed
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Standing Waves on a String
• The lowest frequency of vibration (b) is called the fundamental frequency
• ƒ1, ƒ2, ƒ3 form a harmonic series
1ƒ ƒ2n
n Fn
L µ= =