Euler Lagrange Equation - Classical Mechanics - Solved Past Paper, Exams of Classical Mechanics

This is the Solved Past Paper of Classical Mechanics which includes Euler Lagrange Equation, Potential Energy, Equation of Motion, Coriolis Force, Constants of Integration, Coordinate Origin, Minimum Escape Speed etc. Key important points are: Euler Lagrange Equation, Potential Energy, Equation of Motion, Coriolis Force, Constants of Integration, Coordinate Origin, Minimum Escape Speed, Arbitrarily Defined

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2012/2013

Uploaded on 02/20/2013

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PC2132 CLASSICAL MECHANICS
AY2005/2006 Semester 2
Part II
1.
x=acos ωt +bsin θ
y=asin ωt bcos θ˙x= sin ωt +b˙
θcos θ
˙y= cos ωt +b˙
θsin θ
v2= ˙x2+ ˙y2
=a2ω2sin2ωt 2abω ˙
θsin ωt cos θ+b2˙
θ2cos2θ+a2ω2cos2ωt + 2abω ˙
θcos ωt sin θ+b2˙
θ2sin2θ
=a2ω2+b2˙
θ2+ 2abω ˙
θsin(θωt).
T=1
2mv2=1
2m[a2ω2+b2˙
θ2+ 2abω ˙
θsin(θωt)].
V=mgy =mg(asin ωt bcos θ).
L=TV=m1
2a2ω2+1
2b2˙
θ2+abω ˙
θsin(θωt)ga sin ωt gb cos θ.
∂L
∂θ =mhabω ˙
theta cos(θωt) + gb sin θi.
∂L
˙
θ=mhb2˙
θ+abω sin(θωt)i.
Using the Euler-Lagrange equation,
d
dt ∂L
˙
θ∂L
∂θ = 0,
b2¨
θ+abω(˙
θω) cos(θωt)abω ˙
θcos(θωt) + gb sin θ= 0,
¨
θ=1
b2habω2cos(θωt)g b sin θi.
2a. Since potential energy can be arbitrarily defined, we can set K= 0.
mgz m
2ω2r2= 0,
ω=r2gz
r2
= 15.3 rad s1.
2b. Defining i: east, j: north and k: up, we have ˙x= 0, ˙y=800 cos 37and ˙z= 800 sin 37gt.
Using the equation of motion for Coriolis force,
m¨x= 2( ˙ycos θ˙zsin θ)
= 2(800 cos 3gt sin 40).
˙x=1600ωt cos 3gωt2sin 40.
x=800ωt2cos 31
3gωt3sin 40.(1)
1
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PC2132 CLASSICAL MECHANICS

AY2005/2006 Semester 2

Part II

x = a cos ωt + b sin θ

y = a sin ωt − b cos θ

x˙ = −aω sin ωt + b

θ cos θ

y ˙ = aω cos ωt + b

θ sin θ

v

2 = x˙

2

  • ˙y

2

= a

2

ω

2

sin

2

ωt − 2 abω

θ sin ωt cos θ + b

2 ˙ θ

2

cos

2

θ + a

2

ω

2

cos

2

ωt + 2abω

θ cos ωt sin θ + b

2 ˙ θ

2

sin

2

θ

= a

2 ω

2

  • b

θ

2

  • 2abω

θ sin(θ − ωt).

T =

mv

2

=

m[a

2

ω

2

  • b

2 ˙ θ

2

  • 2abω

θ sin(θ − ωt)].

V = mgy = mg(a sin ωt − b cos θ).

L = T − V = m

[

a

2

ω

2

b

2 ˙ θ

2

  • abω

θ sin(θ − ωt) − ga sin ωt − gb cos θ

]

∂L

∂θ

= m

[

abω

theta cos(θ − ωt) + gb sin θ

]

∂L

θ

= m

[

b

2 ˙ θ + abω sin(θ − ωt)

]

Using the Euler-Lagrange equation,

d

dt

(

∂L

θ

)

∂L

∂θ

b

2 ¨ θ + abω(

θ − ω) cos(θ − ωt) − abω

θ cos(θ − ωt) + gb sin θ = 0,

θ =

b

2

[

abω

2

cos(θ − ωt) − gb sin θ

]

2a. Since potential energy can be arbitrarily defined, we can set K = 0.

mgz −

m

ω

2

r

2

= 0 ,

ω =

2 gz

r

2

= 15 .3 rad s

− 1 .

2b. Defining i: east, j: north and k: up, we have ˙x = 0, ˙y = −800 cos 37

◦ and ˙z = 800 sin 37

◦ − gt.

Using the equation of motion for Coriolis force,

mx¨ = 2 mω( ˙y cos θ − z˙ sin θ)

= 2 mω(−800 cos 3

◦ − gt sin 40

◦ ).

x ˙ = − 1600 ωt cos 3

− gωt

2

sin 40

.

x = − 800 ωt

2 cos 3

◦ −

gωt

3 sin 40

. (1)

The constants of integration for ˙x and x can be dropped because ˙x = 0 initially and by re-defining

coordinate origin respectively. To find t, we solve for z = 0.

z˙ = 800 sin 37

− gt

z = 800t sin 37

◦ −

gt

2 = 0

t = 0 or t =

1600 sin 37

g

Substituting this into (1) and solving, one will find a deflection of 706 m to the west.

3a.

T

i

+ V

i

= T

f

+ V

f

For minimum escape speed, T f

= V

f

Ti = −Vi,

mv

2

esc

Gm E

m

r

v esc

2 Gm E

r

= 1. 07 × 10

4 m s

− 1 .

3b. By substituting θ = 0

◦ , r = (300 + 6372) km and θ = 180

◦ , r = (3500 + 6372) km into the equation

l

r

= 1 +  cos θ, we get

l

l

Solving (2) and (3) for , we get

6672

9872

6672

9872

(i) Solving (2) and (3) for l, we have l = 7962 km.

l

r

= 1 +  cos θ,

r + 6372

= 1 + 0.193 cos 90

,

r = 1590 km.

(ii)

a =

(300 + 6372 + 3500 + 6372) = 8272 km.