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Constant Push Behind a Quadratic Pull

Irodov 1.126DifficultyDifficulty 2 of 5UniquenessUniqueness 3 of 5

Problem Irodov 1.126

A particle of mass mm moves along a circular path of radius RR, starting from rest, with its normal (centripetal) acceleration growing as wn=at2w_n=at^2, where aa is a given constant. Find the power P(t)P(t) developed by the combined action of all the forces on the particle as a function of time, and the mean power ⟨P⟩\langle P\rangle of that same combination averaged over the first tt seconds of the motion.

The particle of mass m on the circle of radius R, with the resultant force F resolved into normal F_n and tangential F_τ parts; φ is its angle with the velocity v.

The particle of mass mm on the circle of radius RR, with the resultant force F\vect F resolved into normal FnF_n and tangential FτF_\tau parts; φ\varphi is its angle with the velocity v\vect v.

Given
  • mm
  • RR
  • wn=at2w_n=at^2
Find
P(t)P(t) · ⟨P⟩\langle P\rangle over the first tt seconds

Solution

Step 1Speed from the normal acceleration

The normal acceleration of circular motion is wn=v2/Rw_n=v^2/R; equating this to the given wn=at2w_n=at^2 and taking the positive root (the particle starts from rest, so v≥0v\ge0) gives v(t)v(t).

v2R=at2  ⟹  v2=aRt2\frac{v^2}{R} = at^2 \;\Longrightarrow\; v^2 = aRt^2
v(t)=aR tv(t) = \sqrt{aR}\,t
(1)
Step 2Tangential force from the growth of speed

The tangential acceleration is the time derivative of (1), a constant; Newton’s second law along the tangent then gives the tangential force FτF_\tau, the only component of the resultant that can do work.

wτ=dvdt=aRw_\tau = \frac{dv}{dt} = \sqrt{aR}
Fτ=maRF_\tau = m\sqrt{aR}
(2)
Step 3Instantaneous power

Only the tangential force does work, since the normal force is always perpendicular to v\vect v, so the power is FτF_\tau (2) times the speed (1).

P(t)=Fτ v(t)=maR⋅aR tP(t) = F_\tau\,v(t) = m\sqrt{aR}\cdot\sqrt{aR}\,t
P(t)=maRtP(t) = maRt
(3)
Step 4Mean power over the first tt seconds

The power (3) is linear in time and starts from zero, so averaging it over [0,t][0,t] integrates a straight line through the origin, which halves its endpoint value.

⟨P⟩=1t∫0tmaRτ dτ=maRt[τ22]0t\langle P\rangle = \frac1t\int_0^t maR\tau\,d\tau = \frac{maR}{t}\left[\frac{\tau^2}{2}\right]_0^t
⟨P⟩=maRt2\langle P\rangle = \dfrac{maRt}{2}
(4)
Check

Dimensionally, wn=at2w_n=at^2 forces [a]=m/s4[a]=\mathrm{m/s^4}, so [m][a][R][t]=kg⋅(m/s4)⋅m⋅s=kg m2/s3=W[m][a][R][t]=\mathrm{kg}\cdot(\mathrm{m/s^4})\cdot\mathrm m\cdot\mathrm s=\mathrm{kg\,m^2/s^3}=\mathrm W, a power, as required. At t=0t=0 the particle is at rest and both P(0)=0P(0)=0 and ⟨P⟩→0\langle P\rangle\to0 as t→0t\to0, consistent with no work yet done; and since P(t)P(t) is linear starting from the origin, its average over [0,t][0,t] is exactly half its value at tt, matching ⟨P⟩=P(t)/2\langle P\rangle=P(t)/2 read off the two boxed results.

Remark

The normal acceleration was given growing as t2t^2, which looks like the more complicated ingredient, yet it never entered FτF_\tau or P(t)P(t) at all: FnF_n only feeds the wasted, work-free part of the resultant force, so however fast wnw_n grows, the entire power comes from FτF_\tau alone, which here happens to be constant because wn=at2w_n=at^2 was exactly the profile that makes vv linear in tt. A different growth law for wnw_n would still leave the normal force powerless, but FτF_\tau and P(t)P(t) would no longer be so simple.