13
Physics 2210 Fall 2015 smartPhysics 21 Simple Harmonic Motion 22 Simple and Physical Pendulum 11/25/2015

Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

  • Upload
    others

  • View
    3

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Physics 2210 Fall 2015

smartPhysics 21 Simple Harmonic Motion

22 Simple and Physical Pendulum 11/25/2015

Page 2: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Exam 4: smartPhysics units 14-20 Midterm Exam 4: Day: Fri Dec. 04, 2015 Time: regular class time Section 01 12:55 – 1:45 pm Section 10 02:00 – 02:50 pm

Location: FMAB 15 practice problems for Exam 4 posted on CANVAS and to the Class Web Page (http://www.physics.utah.edu/~woolf/2210_Jui/rev4.pdf)

Page 3: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Derivation Already Given in Pre-lecture 1/4

In each case we have the usual relationship between force (exerted by the spring on the block) and the position (displacement from equilibrium) of the block:

�⃗� = −𝑘𝑘𝚤̂ Applying Newton’s 2nd Law then we have (noting that 𝑎𝑥 = 𝑑2𝑘 𝑑𝑑2⁄ ):

𝑑2𝑘𝑑𝑑2 = −

𝑘𝑚𝑘

This is an equation that involves the 2nd derivative of position, 𝒙, with respect to time, t

𝐿 = 𝐿0 − 𝑏 𝑚

𝑘 = −𝑏

𝐿 = 𝐿0 𝑚

𝑘 = 0

𝐿 = 𝐿0 + 𝑏 𝑚

𝑘 = +𝑏

�⃗� = +𝑘𝑏𝚤̂ 𝑏 is a positive length

�⃗� = 0

�⃗� = −𝑘𝑏𝚤̂

Equilibrium Position

Page 4: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Derivation Already Given in Pre-lecture 2/4

The solution to the equation is equivalent to integrating twice: in other words, it will have TWO “integration” constants that are to be determined by the particular conditions But first: let’s guess at the solution we can try 𝑘1 = 𝑐1 sin𝜔𝑑 :

𝑑𝑘1𝑑𝑑 = 𝜔𝑐1 cos𝜔𝑑 →

𝑑2𝑘1𝑑𝑑2 =

𝑑𝑑𝑑

𝑑𝑘1𝑑𝑑 =

𝑑𝑑𝑑

𝜔𝑐1 cos𝜔𝑑 = −𝜔 ∙ 𝜔𝑐1 cos𝜔𝑑

= −𝜔2𝑐1 cos𝜔𝑑 But the equation requires:

𝑑2𝑘1𝑑𝑑2 = −

𝑘𝑚𝑘1 → −𝜔2𝑐1 cos𝜔𝑑 = −

𝑘𝑚 𝑐1 cos𝜔𝑑

This means 𝑘1 = 𝑐1 sin𝜔𝑑 can be a solution provided we satisfy the condition:

𝜔2 =𝑘𝑚 → 𝜔 = 𝑘 𝑚⁄

Unit check:

𝑘 𝑚⁄ =N m⁄

kg =kg ∙ m

s2 ∙1m ∙

1kg = s−2 = s−1

This is what we need: because the argument of a sine/cosine function needs to be unitless.

𝐿 = 𝐿0 + 𝑘 𝑚

𝑘

�⃗� = −𝑘𝑘𝚤̂

Page 5: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Derivation Already Given in Pre-lecture 3/4

We can also try 𝑘2 = 𝑐2 cos𝜔𝑑 : 𝑑𝑘2𝑑𝑑 = −𝜔𝑐2 sin𝜔𝑑 →

𝑑2𝑘2𝑑𝑑2 =

𝑑𝑑𝑑

𝑑𝑘2𝑑𝑑 =

𝑑𝑑𝑑

−𝜔𝑐2 sin𝜔𝑑 = 𝜔 ∙ −𝜔𝑐2 cos𝜔𝑑

= −𝜔2𝑐2 cos𝜔𝑑 But the equation requires:

𝑑2𝑘2𝑑𝑑2 = −

𝑘𝑚𝑘2 → −𝜔2𝑐2 cos𝜔𝑑 = −

𝑘𝑚 𝑐2 cos𝜔𝑑

This means 𝑘2 = 𝑐2 cos𝜔𝑑 can ALSO be a solution provided we satisfy the SAME condition:

𝜔2 =𝑘𝑚 → 𝜔 = 𝑘 𝑚⁄

NOTE: The equation involves only the function 𝒙(𝒕), and its 2nd derivative �̈� ≡ 𝒅𝟐𝒙 𝒅𝒕𝟐⁄ , BUT NOT its powers (like 𝒙𝟐, or �̈�𝟐). We say that the equation is LINEAR This means any linear combination of the two solutions is also a solution

𝑘(𝑑) = 𝑐1 sin𝜔𝑑 + 𝑐2 cos𝜔𝑑 is also a solution for 𝜔 = 𝑘 𝑚⁄ Since this form involves TWO integration constants, 𝑐1 and 𝑐2, it is a GENERAL solution Another general solution (smartPhysics is inconsistent) has the form 𝑘 𝑑 = 𝐴 cos 𝜔𝑑 + 𝜙

𝐿 = 𝐿0 + 𝑘 𝑚

𝑘

�⃗� = −𝑘𝑘𝚤̂

Page 6: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Derivation Already Given in Pre-lecture 4/4

For 𝜔 = 𝑘 𝑚⁄ , 𝑘(𝑑) = 𝑐1 sin𝜔𝑑 + 𝑐2 cos𝜔𝑑 and 𝑘 𝑑 = 𝐴 cos 𝜔𝑑 + 𝜙 are equivalent : Trigonometric identity

sin 𝑢 + 𝑣 = sin𝑢 cos𝑣 + sin 𝑣 cos𝑢 cos 𝑢 + 𝑣 = cos𝑢 cos𝑣 − sin𝑣 sin𝑢

So we can apply the second to

𝐴 cos 𝜔𝑑 + 𝜙 = 𝐴 cos𝜔𝑑 cos𝜙 − 𝐴 sin𝜙 sin𝜔𝑑

Now recalling that sine is an odd function, and cosine an even function

𝐴 cos 𝜔𝑑 + 𝜙 = − 𝐴 sin𝜙 sin𝜔𝑑 + 𝐴 cos𝜙 cos𝜔𝑑

In other words to make the two forms be equivalent, we identify

𝑐1 = −𝐴 sin𝜙 , 𝑐2 = 𝐴 cos𝜙

Or conversely

𝐴 = 𝑐12 + 𝑐22, 𝜙 = tan−1−𝑐1𝑐2

𝐿 = 𝐿0 + 𝑘 𝑚

𝑘

�⃗� = −𝑘𝑘𝚤̂

Page 7: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Unit of angular frequency 𝜔: s−1 or rad/s*** To complete one period of the motion, the argument to the cosine/sine must advance by 2𝜋 i.e. the period, T, is given by 𝜔𝑇 = 2𝜋 → 𝑇 = 2𝜋/𝜔 (unit of period: seconds) The “frequency” (number of complete cycles per unit time) is given by 𝑓 = 1 𝑇⁄ = 𝜔/2𝜋 Unit of frequency: s−1 ≡ ℎ𝑒𝑒𝑑𝑒 (Hz) The maximum displacement from equilibrium is 𝐴, known as the amplitude (unit: meters) Maximum speed: 𝑣𝑚𝑚𝑥 = 𝜔𝐴, maximum acceleration: 𝑎𝑚𝑚𝑥 = 𝜔2𝐴

Page 8: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Uniform Circular Motion Model of Simple Harmonic Motion

Top: Particle in uniform circular motion with radius 𝑒 = 𝐴 and constant angular velocity 𝜔 and initial angle 𝜙

Its Cartesian coordinates are: 𝑘 = 𝐴 cos 𝜔𝑑 + 𝜙 𝑦 = 𝐴 sin 𝜔𝑑 + 𝜙

In this context, 𝜙 = 𝜃 𝑑 = 0 is the angular position of the particle at 𝑑 = 0

Bottom: Harmonic oscillator with amplitude 𝑨, frequency 𝒇 = 𝝎 𝟐𝝅⁄ , initial phase angle 𝝓. i.e at time 𝑑 = 0:

𝑘 = 𝑘0 = 𝐴 cos𝜙 𝑣 = 𝑣0 = −𝜔𝐴 sin𝜙

𝑘

𝑦

𝐴 𝜃 = 𝜙 + 𝜔𝑑

Equilibrium at 𝑘 = 0 𝑚

𝑘 = 𝐴 cos 𝜔𝑑 + 𝜙

Page 9: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

https://www.youtube.com/watch?v=5L_vuX0xeJY

Page 10: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Poll 11-25-01

A mass on a spring moves with simple harmonic motion as shown.

Where is the acceleration of the mass most positive?

A. x = -A B. x = 0 C. x = +A

Page 11: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Poll 11-25-02

In the two cases shown the mass and the spring are identical but the amplitude of the simple harmonic motion is twice as big in Case 2 as in Case 1.

How are the maximum velocities in the two cases related?

A. Vmax,2 = Vmax,1 B. Vmax,2 = 2 Vmax,1 C. Vmax,2 = 4 Vmax,1

Page 12: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Demo/Example 21.1 1. Hang vertically from pivot, relaxed 2. With 500 g mass attached: the spring is

stretched from relaxed length to the NEW equilibrium

3. With extra 100 g attached, stretches ∆𝐿 from relaxed length

Calculate Spring Constant:

𝑘 ≡∆𝐹∆𝐿

=0.100 kg ∙ 9.8 m s2⁄

𝟎.𝟏𝟎 m = 9.8 N m⁄

If we just hang a 500 g mass, and take configuration (2) to be equilibrium Then for displacement 𝑘 about the equilibrium configuration of (2) we have

𝜔 = 𝑘 𝑚⁄ = 9.8 N m⁄ 0.50 kg⁄= 𝟒.𝟒𝟒 s−1

The period is predicted to be

𝑇 =2𝜋𝜔 =

2𝜋𝟒.𝟒𝟒s−1 = 𝟏.𝟒𝟐 S

Measurement: time for 10 cycles: 14.7 s Measured period = 1.47 s

500 g

500 g

100 g

∆𝐿

(1)

(2)

(3)

𝑘

𝐿0

EQULIBRIUM

Page 13: Physics 2210 Fall 2015woolf/2210_Jui/nov25.pdf · Derivation Already Given in Pre-lecture 2/4 . The solution to the equation is equivalent to integrating twice: in other words, it

Demo/Example 22.1 Simple Pendulum

This is the rotational (approximate) equivalent of a simple harmonic oscillator The moment of inertia about the pivot for a small particle is

𝐼 = 𝑚𝑒2 = 𝑚𝐿2 The torque exerted by the force of gravity is

𝜏 = 𝑒𝐹 sin𝜙𝑟𝑟 = 𝐿 ∙ 𝑚𝑚 ∙ sin −𝜃 = −𝑚𝑚𝐿 sin𝜃 Where we have observed that SINE is an odd function: sin −𝜃 = − sin𝜃, so the equation of motion is:

𝑑2𝜃𝑑𝑑2 =

𝜏𝐼 =

−𝑚𝑚𝐿 sin𝜃𝑚𝐿2 = −

𝑚𝐿 sin𝜃 ≈ −

𝑚𝐿 𝜃

𝜃

P

𝑚𝑚 −𝜃

𝑚

𝐿

Which has the form

𝑑2𝜃𝑑𝑑2 = −𝜔2𝜃, 𝜔 =

𝑚𝐿 =

9.8 m s2⁄𝟎.𝟓𝟎m = 𝟒.𝟒𝟒 s−1

And the period is related to the angular velocity/frequency by (period is the time it takes to do one cycle: i.e. 𝜔𝑇 = 2𝜋

𝑇 =2𝜋𝜔 =

2𝜋𝟒.𝟒𝟒s−1 = 𝟏.𝟒𝟐s

Measured Period: 14.3s/10 = 1.43 s