Cartesian Coordinates - Classical Mechanics - Solved Exam, Exams of Classical Mechanics

These are the Solved Exam of Classical Mechanics which includes Homogeneous Solution, Function of Time, Friction Force, Forces and Dynamics etc. Key important points are: Cartesian Coordinates, Lagrangian for System, Uninteresting Constants, Equations of Motion, Lagrange’s Equations, Linear and Angular Momentum, Equilibrium Position, Kinetic Energy

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Physics 205—Final Exam Fall 2003
Solutions
x
θ
M
m
g
l
1) (40 pts) A plane pendulum consists of
a bob of mass msuspended by a massless
rigid rod of length lthat is hinged to a sled
of mass M. The sled slides without friction
on a horizontal rail. Gravity acts with the
usual downward acceleration g.
a) Taking xand θas generalized coordinates write the Lagrangian for the system.
Solution: We start by computing the Cartesian coordinates of the bob
x1=x+lsin θ=˙x1= ˙x+˙
θl cos θ
y1=y+lcos θ=˙y1= ˙y+˙
θl sin θ
thus
T=m
2¡˙x2
1+ ˙y2
1¢+M
2˙x2= (m+M)/over2 + m
2³2˙
θ˙xl cos θ+˙
θ2l2´
and
V=mgl (1 cos θ)
hence
L=TV=(m+M)
2+m
2³2˙
θ˙xl cos θ+˙
θ2l2´+mgl cos θ
where uninteresting constants have been dropped.
b) Use Lagrange’s equations to derive the equations of motion for the system.
Solution: For xwe have
d
dt
∂L
˙xL
∂x = (m+M)¨x+ml¨
θcos θm˙
θ2lsin θ= 0
and for θd
dt
∂L
˙
θ∂L
∂θ =m¨xl cos θ+m¨
θl2+mgl sin θ= 0
c) Use the equations from part (b) to find the frequency ωfor small oscillations of the
bob about the vertical. (Hint: You will need to make some approximations.)
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Physics 205—Final Exam Fall 2003

Solutions

x

M

m

g

l

  1. (40 pts) A plane pendulum consists of

a bob of mass m suspended by a massless

rigid rod of length l that is hinged to a sled

of mass M. The sled slides without friction

on a horizontal rail. Gravity acts with the

usual downward acceleration g.

a) Taking x and θ as generalized coordinates write the Lagrangian for the system.

Solution: We start by computing the Cartesian coordinates of the bob

x 1 = x + l sin θ =⇒ x˙ 1 = ˙x +

θl cos θ

y 1

= y + l cos θ =⇒ y˙ 1

= ˙y +

θl sin θ

thus

T =

m

2

1

  • ˙y

2

1

M

2

= (m + M )/over2 +

m

θ xl˙ cos θ +

θ

2

l

2

and

V = mgl (1 − cos θ)

hence

L = T − V =

(m + M )

m

θ xl˙ cos θ +

θ

2

l

2

  • mgl cos θ

where uninteresting constants have been dropped.

b) Use Lagrange’s equations to derive the equations of motion for the system.

Solution: For x we have

d

dt

∂L

∂ x˙

∂L

∂x

= (m + M )¨x + ml

θ cos θ − m

θ

2

l sin θ = 0

and for θ

d

dt

∂L

θ

∂L

∂θ

= mxl¨ cos θ + m

θl

2

  • mgl sin θ = 0

c) Use the equations from part (b) to find the frequency ω for small oscillations of the

bob about the vertical. (Hint: You will need to make some approximations.)

Solution: For small oscillations, θ, x, and their derivatives will be small, so we can neglect

terms containing

θ

2 and ˙x

θ. Also cos θ ' 1 and sin θ ' θ. With this we obtain

(m + M )¨x + ml

θ ' 0 =⇒ x¨ ' −

m

m + M

l

θ

and

x¨ +

θl + gθ ' 0 =⇒

m

m + M

l

θ ' −gθ

yielding

ωosc '

g

m

m+M

l

g(m + M )

lM

d) At time t = 0 the bob and the sled, which had previously been at rest, are set in

motion by a sharp tap delivered to the bob. The tap imparts a horizontal impulse

∆P = F ∆t to the bob. Find expressions for the values of

θ and ˙x just after the

impulse.

Solution: Here we conserve linear and angular momentum.

∆P =

∆p i

= m( ˙x +

θl) + M x˙

and

∆L = ∆P l =

Li = ml

θ =⇒

θ =

∆P

ml

Note that since

∆P = ml

θ =⇒ x˙ = 0

a

m

g

θ

Ω

  1. (45 pts) A bead of mass m slides with-

out friction on a rotating circular hoop. The

hoop is forced to rotate about a vertical axis

along its diameter at a constant angular ve-

locity Ω. The position of the bead can be

described by the angle θ, which is the angle

that a line running between the center of the

hoop and the bead makes with the vertical.

a) What is the Lagrangian for the system?

Solution:

L = T − V =

ma

2

θ

2

  • Ω

2

sin

2

θ

− mga(1 − cos θ)

as shown in the sketch. Calculate the displacement of the oscillator for times t >

T /2.

Solution: Starting with the general Green function solution

x(t) =

t

−∞

dt

F (t

′ )

mω 1

e

−γ(t−t

′ )

sin [ω 1

(t − t

)]

where since there is no damping γ = 0 and ω 1

= ω 0

. We thus have

x(t) =

t

−∞

dt

F (t

′ )

mω 0

sin [ω 1

(t − t

)]

since the force is zero prior to −T /2 and after T /2 and we only want to know x(t) for

t > T /2, we can write

x(t) =

T / 2

−T / 2

dt

F 0 sin(ω 0 t

)

mω 0

sin [ω 0

(t − t

)]

F

0

mω 0

[

sin ω 0

t

T / 2

−T / 2

sin ω 0

t

cos ω 0

t

dt

− cos ω 0

t

T / 2

−T / 2

sin

2

ω 0

t

dt

]

where we have used the standard trig. ID for the sine of a difference. The first term in

the integral vanishes and the second can be evaluated by noting that the average of sin

2

ωt

over one period is 1/2. This yields

x(t) = −

F 0

mω 0

cos ω 0 t

T

F 0 π

2

0

cos ω 0 t

e

3

  1. (40 pts) A quarterback in American foot-

ball throws the ball in such a way that it ap-

pears to “wobble” rather than spinning smoothly

as it flies. For this problem assume that the foot-

ball can be treated as an axisymmetric top having

I

1

= I

2

= 2I

3

, where the ˆe 3

axis is the long axis of

the football. Assume further that the football is

released with a rapid spin, i.e., ω 3 6 = 0, where ω 3

is the component of the football’s angular velocity

along the ˆe 3

body axis.

a) What does the wobbling motion indicate? In particular what does it imply about

the other (ˆe 1 and ˆe 2 ) components of ω? (No calculation is required here.)

Solution: This worked out to be a little bit more open ended than I had intended. The

answer I was looking for was that it means that the angular velocity was not aligned with

a body axis, meaning that it would also not be aligned with the angular momentum, which

is a vector fixed in space (conservation of angular momentum with no external torques). I

accepted most reasonable variations on this theme.

b) Expressing vectors with respect to the body fixed axes, ˆe 1 , ˆe 2 , eˆ 3 , derive three equa-

tions that relate the components of ~ω to one another and to the moments of inertia

I

1

, I

2

, I

3

Solution: Euler’s equation is

d

L

dt

inertial

d

L

dt

body

  • ~ω ×

L =

Γexternal = 0

If we choose body axes that are principal axes then

dL i

dt

body

d

dt

I

ii

ω i

body

= I

i

ω˙ i

combining this with Euler’s equation and writing it by components yields

I

1

ω˙ 1

= ω 2

ω 3

(I

2

− I

3

I

2

ω˙ 2

= ω 3

ω 1

(I

3

− I

1

I

3

ω˙ 3

= ω 1

ω 2

(I

1

− I

2

c) If the football is spinning rapidly, then one can assume that ω 3

¿ ω 1 , 2

. Use this

assumption to derive an approximate expression for ~ω as a function of time. Find

the period of the wobble in terms of I 1 = I 2 , I 3 , and ω 3.

Solution: Since the football is axisymmetric I 1 = I 2 = I and ω˙ 3 = 0. Defining Ω ≡

(I

3

− I)/Iω 3

yields

ω˙ 1

= −Ωω 2

and ω˙ 2

= +Ωω 1

which, when differentiated, can be solved to yield

ω¨ 1

2

ω 1

and ω¨ 2

2

ω 2

Thus both ω 1 and ω 2 vary harmonically with frequency

ω 3

and the period of the wobble is

T =

2 π

4 π

ω 3