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Transcript
1.
A body of mass m moves along the x-axis subject to a potential V (x). Show that the period
τ of small oscillations about a stable equilibrium point x0 , is given by
r
m
.
τ = 2π
00
V (x0 )
Consider the potential
V (x) =
x2 x4
−
2
4
.
If a body of unit mass is released from the point of stable equilibrium with velocity u, for what
values of u does it
(i)
oscillate
(ii)
escape to infinity?
1
For the case u = √ show that the position at time t, is given by
2
√
1 − e− 2t
√
x=
1 + e− 2t
2.
.
Consider the equation of motion for an undamped, forced oscillator
ẍ + ω02 x = F0 cos ωt ,
where ω, ω0 , F0 are constants.
If the body is released from the origin with zero velocity at t = 0, show that its position
at later times is given by
x=
2F0
− ω2
ω02
sin(ω0 + ω)t
2
sin(ω0 − ω)t
2
.
Derive an expression for the time dependence of the mechanical energy E(t) exactly at
resonance, ω = ω0 .
M1A1 MECHANICS (2007)
Page 2 of 4
3.
Consider the motion of a plane pendulum of length a. Using appropriate intrinsic co-ordinates
(s, ψ), derive the expression for the conservation of energy
E=
1
s
mṡ2 + 2mg a sin2
2
2a
,
where g is the acceleration due to gravity. If the body is projected from s = 0 with velocity
√
ṡ = 4ga , show that at later times
r !
gt
.
s = 2a cos−1 sech
a
What type of motion does this correspond to qualitatively?
4.
A body of mass m moves in a central force field F (r) directed away from the origin. Given
that the radial and transverse accelerations in polar co-ordinates are
arad = r̈ − rθ̇2
show that
where u =
and atrans = rθ̈ + 2ṙθ̇
1
d2 u
+u=−
2
dθ
mh2 u2
1
r
1
F
u
,
,
and h is the angular momentum per unit mass.
A body is projected from the point r = a, θ = 0 with transverse velocity
1
vtrans = a2 2 and zero radial velocity (vrad ≡ ṙ = 0) , in a force field
3a
−m
F (r) = 2 1 +
.
r
2r
Show that the equation for the orbit is
r=
M1A1 MECHANICS (2007)
a
2 − cos 2θ
.
Page 3 of 4
5. (a) A rocket of mass m(t) moves in a straight line under the influence of an external force
F . Exhaust gas is expelled at constant velocity u relative to the rocket. Show that the
equation of motion for the rocket is
mv̇ + uṁ = F
(b)
where v̇ ≡
dv
dt
,
, etc.
Next consider the same rocket but moving around a circular track of radius a. Show
that the equation of motion in polar co-ordinates is
b − maθ̇2b
maθ̈ + uṁ θ
r=F ,
where b
r and θb are the radial and transverse unit vectors and F is the external force.
M1A1 MECHANICS (2007)
Page 4 of 4