Oscillations and Waves Microworld Macroworld Lect 5 Equilibrium
Oscillations and Waves Micro-world Macro-world Lect 5
Equilibrium (Fnet = 0)
Examples of unstable Equilibrium
Examples of Stable equilibrium
Destabilizing forces NF = 0 net W
Destabilizing forces N Fnet = away from equil W
Destabilizing forces Fnet = away from equil N W destabilizing forces always push the system further away from equilibrium
restoring forces N Fnet = 0 W
restoring forces N Fnet = toward equil. W
restoring forces Fnet N = toward equil. W Restoring forces always push the system back toward equilibrium
Pendulum N W
Mass on a spring
Displacement vs time Displaced systems oscillate around stable equil. points amplitude Equil. point period (=T)
Simple harmonic motion Pure Sine-like curve T Equil. point T= period = time for 1 complete oscillation f = frequency = # of oscillations/time = 1/T
Masses on springs Animations courtesy of Dr. Dan Russell, Kettering University
Not all oscillations are nice Sine curves A Equil. point T f=1/T
Natural frequency f= (1/2 p) g/l f= (1/2 p) k/m
Driven oscillators natural freq. = f 0 f = 0. 4 f 0 f = 1. 1 f 0 f = 1. 6 f 0
Resonance (f=f 0)
Waves Animations courtesy of Dr. Dan Russell, Kettering University
Wave in a string Animations courtesy of Dr. Dan Russell, Kettering University
Pulsed Sound Wave
Harmonic sound wave
Harmonic sound wave
Harmonic wave Shake end of string up & down with SHM period = T Wave speed wavelength =v =l distance time =v= = V=fl or f=V/ l wavelength period l = = fl T but 1/T=f
Reflection (from a fixed end) Animations courtesy of Dr. Dan Russell, Kettering University
Reflection (from a loose end) Animations courtesy of Dr. Dan Russell, Kettering University
Adding waves pulsed waves Animations courtesy of Dr. Dan Russell, Kettering University
Adding waves Two waves in same direction with slightly different frequencies Wave 1 Wave 2 resultant wave “Beats” Animations courtesy of Dr. Dan Russell, Kettering University
Adding waves harmonic waves in opposite directions incident wave reflected wave resultant wave (standing wave) Animations courtesy of Dr. Dan Russell, Kettering University
Two wave sources e v i t ce c ru ren t ns fe o c er int de in str te u rf cti er ve en ce
Confined waves Only waves with wavelengths that just fit (all others cancel themselves out) in survive
Confined waves
Allowed frequencies l= 2 L f 0=V/l = V/2 L Fundamental tone l=L l=(2/3)L f 1=V/l = V/L=2 f 0 1 st overtone f 2=V/l=V/(2/3)L=3 f 0 2 nd overtone l=L/2 f 3=V/l=V/(1/2)L=4 f 0 3 rd overtone l=(2/5)L f 4=V/l=V/(2/5)L=5 f 0 4 th overtone
Ukuleles, etc L l 0 = 2 L; f 0 = V/2 L l 1= L; f 1 = V/L =2 f 0 l 2= 2 L/3; f 2 = 3 f 0 l 3= L/2; f 3 = 4 f 0 Etc… (V depends on the Tension & thickness Of the string)
Vocal Range – Fundamental Pitch ♩ 329 Hz ♩ 392 Hz ♩ 82 Hz ♩ 98 Hz ♩ 523 Hz ♩ 131 Hz ♩ 587 Hz ♩ 147 Hz ♩ 880 Hz ♩ 1175 Hz ♩ 165 Hz ♩ 196 Hz Tenor Soprano Mezzo- G – D ♂: C 2 – C 5 ♀: 3 6 Soprano Baritone E 3 – A 5 Bass E 2 G 2 – G 4 Contralt – E 4 o. D 3 – D 5 Thanks to Kristine Ayson
Doppler effect
Sound wave stationary source Wavelength same in all directions
Sound wave moving source Wavelength in forward direction is shorter (frequency is higher) Wavelength in backward direction is longer (frequency is lower)
Waves from a stationary source Wavelength same in all directions
Waves from a moving source v Wavelength in forward direction is shorter (frequency is higher) Wavelength in backward direction is longer (frequency is higher)
Visible light Short wavelengths Long wavelengths
receding source red-shifted approaching source blue-shifted
Edwin Hubble
More distant galaxies have bigger red shifts
The universe is expanding!!
Use red- & blue-shifts to study orbital motion of stars in galaxies ap bl pro ue a -s ch hi ing ft ed g din ted e c re -shif red
A typical galactic rotation curve NGC 6503
Large planets create red-shifts and blue shifts in the light of their star Use this to detect planets & measure their orbital frequency
Planetary motion induced stellar velocity
- Slides: 51