Falling Harmonic-Classical and Relativistic Mechanics-Lecture Handout, Exercises of Classical and Relativistic Mechanics

This lecture handout is part of Advanced Classical and Relativistic Mechanics course. Prof. Manasi Singh provided this handout at Punjab Engineering College. It includes: Failing, Harmonics, Influence, Gravity, Initial, Position, Constant, Acceleration, Integration

Typology: Exercises

2011/2012

Uploaded on 07/19/2012

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m= (0,0,g).
In other words, acceleration ¨qis a constant. Since there’s no increase in difficulty, we’ll just solve
all constant acceleration problems in any dimension, i.e. differential equations of the form
¨q=a
where aRnis a constant. Then we’ll set n= 3 and a= (0,0,g) to solve this special case.
It’s straightforward to integrate
¨q=a
once and get
˙q=v+ta
where our constant of integration vRnis seen, upon setting t= 0, to be the initial velocity
˙q(0) = v
so we have
˙q= ˙q(0) + ta
thus far, and we integrate again to get
q=x+t˙q(0) + 1
2t2a
where, just as before, our constant of integration xRnis seen, upon setting t= 0, to be the initial
positon
q(0) = x
So our full solution is thus
q=q(0) + t˙q(0) + 1
2t2a
Now back to our original problem, where n= 3 and a= (0,0,g). Taking the initial position
and velocity to be
q(0) = (x0, y0, z0)
and
˙q(0) = (vx, vy, vz)
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m

= (0, 0 , −g).

In other words, acceleration ¨q is a constant. Since there’s no increase in difficulty, we’ll just solve all constant acceleration problems in any dimension, i.e. differential equations of the form

q¨ = a

where a ∈ Rn^ is a constant. Then we’ll set n = 3 and a = (0, 0 , −g) to solve this special case. It’s straightforward to integrate q¨ = a

once and get q˙ = v + ta

where our constant of integration v ∈ Rn^ is seen, upon setting t = 0, to be the initial velocity

q˙(0) = v

so we have q˙ = ˙q(0) + ta

thus far, and we integrate again to get

q = x + t q˙(0) +

t^2 a

where, just as before, our constant of integration x ∈ Rn^ is seen, upon setting t = 0, to be the initial positon q(0) = x

So our full solution is thus

q = q(0) + t q˙(0) +

t^2 a

Now back to our original problem, where n = 3 and a = (0, 0 , −g). Taking the initial position and velocity to be q(0) = (x 0 , y 0 , z 0 )

and q˙(0) = (vx, vy , vz )

we get that our position at time t is

q(t) = (xo + vxt, yo + vy t, zo + vz t −

gt^2 )

in terms of its components. In particular, if we take the z-axis to point in the vertical direction, we have that the particle’s height at time t is

qz (t) = zo + vz t −

gt^2 ,

the familiar formula from any freshman physics text.

Homework 2

Solve Newton’s second law for q(t) ∈ R when the force is given by Hooke’s law

F (t) = −kq(t)

in terms of m, k, q(0), and ˙q(0), and then find the period P of the oscillation and the frequency ω,

where ω =

2 π P

Solution

Plugging this force into Newton’s second law, we get

q¨ = −

k m

q

or

q¨ + k m

q = 0

a slightly more difficult differential equation than the one in the first problem. To solve it, we turn to the arcane techniques of the theory of ordinary differential equations: we find the characteristic polynomial of this equation,

λ^2 + k m

which is the polynomial that looks like the differential equation, if we replace each nth derivative of q with the nth power of λ. Now we find the roots of this polynomial,

λ = ±i

k m

= ±iω

where we’ve defined ω =

k m. Since the characteristic polynomial has no repeated roots, the most general complex-valued solution to our differential equation is of the form

q˜(t) = Aeiωt^ + Be−iωt

where A and B are complex constants to be determined by initial conditions. But we don’t want a complex-valued solution; we want a real solution. This is easy to obtain, because the real part of ˜q,

q(t) = Re(˜q(t) = A′^ cos(ωt) + B′^ sin(ωt)