reading:taylor 4.6 (thornton and marion 2.6) giancoli 8.9 ph421: oscillations – lecture 1 1

15
Reading: Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Upload: roland-parrish

Post on 13-Jan-2016

217 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Reading: Taylor 4.6 (Thornton and Marion 2.6)

Giancoli 8.9

PH421: Oscillations – lecture 1

1

Page 2: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Goals for the pendulum module:(1) CALCULATE the period of oscillation if we know the

potential energy (using exact and approximate forms); specific example is the pendulum

(2) MEASURE the period of oscillation as a function of oscillation amplitude

(3) COMPARE the measured period to models that make different assumptions about the potential

(4) PRESENT the data and a discussion of the models in a coherent form consistent with the norms in physics writing

(5) CALCULATE the (approximate) motion of a pendulum by solving Newton's F=ma equation

2

Page 3: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

How do you calculate how long it takes to get from one point to another?

Separation of x and t variables!

But what if v is not constant?

3

Page 4: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Suppose total energy is CONSTANT (we have to know it, or be able to find out what it is)

The case of a conservative force

4

Page 5: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Classical turning points

xL xR

B

x0

Example: U(x) = ½ kx2 , the harmonic oscillator

5

Page 6: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

xL xRx0

Symmetry - time to go there is the same as time to go back (no damping)

SHO - symmetry about x0

xL -> x0 same time as for x0 -> xR

6

Page 7: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

xL=-A xR=Ax0

SHO - do we get what we expect?

Another way to specify E is via the amplitude A

Independent of A!

x0=0

http://www.wellesley.edu/Physics/Yhu/Animations/sho.html

7

Page 8: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

xL=-A xR=Ax0

You have seen this before in intro PH, but you didn't derive it this way. 8

Page 9: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Period of SHO is INDEPENDENT OF AMPLITUDEWhy is this surprising or interesting?

As A increases, the distance and velocity change. How does this affect the period for ANY potential?

A increases -> further to travel -> distance increases -> period increases

A increases -> more energy -> velocity increases -> period decreases

Which one wins, or is it a tie?

9

Page 10: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Look at example of simple pendulum (point mass on massless string). This is still a 1-dimensional problem in the sense that the motion is specified by one variable,

Your lab example is a plane pendulum. You will have to generalize: what length does L represent in this case? 10

Page 11: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Plot these to compare to SHO to pendulum…… 11

Page 12: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Period increases because v(x) decreases (E decreases) for the same amplitude. Effect is magnified for larger amplitudes. 12

Page 13: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Equivalent angular version?

13

Page 14: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

Integrate both sides

E and U() are known - put them in

Resulting integral• do approximately by hand using series expansion (pendulum period worksheet on web page)OR• do numerically with Mathematica (notebook on web page) 14

Page 15: Reading:Taylor 4.6 (Thornton and Marion 2.6) Giancoli 8.9 PH421: Oscillations – lecture 1 1

xL xR

B

x0

“Everything is a SHO!”

15