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Problem Irodov 1.168

A particle of mass m1m_1, moving with some initial speed v0v_0, undergoes a perfectly elastic collision with a second particle of mass m2m_2 that is initially at rest. Find, as a fraction of the striking particle’s own initial kinetic energy, how much kinetic energy it loses if

  1. it ends up moving at a right angle to its original direction of motion;

  2. the collision is head-on, so both particles move along the same line before and after.

Momentum diagram for part (a): the two final momenta compose, by conservation, to the initial momentum m_1 v_0 (drawn for an illustrative m_2=3m_1; the construction holds for any m_1, m_2).

Momentum diagram for part (a): the two final momenta compose, by conservation, to the initial momentum m1v0m_1\vect v_0 (drawn for an illustrative m2=3m1m_2=3m_1; the construction holds for any m1m_1, m2m_2).

Given
  • m1m_1
  • m2m_2 (initially at rest)
  • perfectly elastic collision
Find
Find the fraction η\eta of the striking particle’s own kinetic energy lost in (a) a 90∘90^\circ recoil and (b) a head-on collision.

Solution

Step 1Part (a): momentum conservation with a right-angle recoil

Let v0v_0 be the initial speed of m1m_1, and v1′v_1', v2′v_2' the final speeds of m1m_1 and m2m_2, with the initial direction as the xx axis and m1m_1 recoiling along yy (90∘90^\circ to xx). Momentum conservation along each axis then reads

m2v2′cos⁡θ=m1v0,m2v2′sin⁡θ=m1v1′,\begin{align*} m_2v_2'\cos\theta &= m_1v_0, \\ m_2v_2'\sin\theta &= m_1v_1', \tag{1}\end{align*}

where θ\theta is the angle at which m2m_2 recoils, an unknown we do not need.

Step 2Eliminating the unknown angle

Squaring each line of (1) and adding them, the two θ\theta terms collapse through cos⁡2θ+sin⁡2θ=1\cos^2\theta+\sin^2\theta=1.

(m2v2′)2cos⁡2θ+(m2v2′)2sin⁡2θ=(m1v0)2+(m1v1′)2(m2v2′)2=m12(v02+v1′2)\begin{align*}(m_2v_2')^2\cos^2\theta+(m_2v_2')^2\sin^2\theta &= (m_1v_0)^2+(m_1v_1')^2 \\ (m_2v_2')^2 &= m_1^2\left(v_0^2+v_1'^2\right)\end{align*}

The collision is perfectly elastic, so kinetic energy is also conserved. Isolating m2v2′2m_2v_2'^2 and multiplying through by m2m_2 turns that into a second expression for the same square.

m1v02=m1v1′2+m2v2′2m2v2′2=m1(v02−v1′2)(m2v2′)2=m1m2(v02−v1′2)\begin{align*}m_1v_0^2 &= m_1v_1'^2+m_2v_2'^2 \\ m_2v_2'^2 &= m_1\left(v_0^2-v_1'^2\right) \\ (m_2v_2')^2 &= m_1m_2\left(v_0^2-v_1'^2\right)\end{align*}

Setting the two expressions for (m2v2′)2(m_2v_2')^2 equal, cancelling the common factor m1m_1 and collecting v02v_0^2 on one side and v1′2v_1'^2 on the other,

m1m2(v02−v1′2)=m12(v02+v1′2)m2(v02−v1′2)=m1(v02+v1′2)v02(m2−m1)=v1′2(m1+m2)\begin{align*}m_1m_2\left(v_0^2-v_1'^2\right) &= m_1^2\left(v_0^2+v_1'^2\right) \\ m_2\left(v_0^2-v_1'^2\right) &= m_1\left(v_0^2+v_1'^2\right) \\ v_0^2(m_2-m_1) &= v_1'^2(m_1+m_2)\end{align*}
v1′2=v02 m2−m1m1+m2v_1'^2 = v_0^2\,\dfrac{m_2-m_1}{m_1+m_2}
(2)
Step 3Fraction of kinetic energy lost, part (a)

The striking particle’s own kinetic energy falls from m1v02/2m_1v_0^2/2 to m1v1′2/2m_1v_1'^2/2, so the fraction lost is one minus the speed-squared ratio, which (2) supplies.

ηa=1−v1′2v02=1−m2−m1m1+m2=(m1+m2)−(m2−m1)m1+m2.\eta_a = 1-\frac{v_1'^2}{v_0^2} = 1-\frac{m_2-m_1}{m_1+m_2} = \frac{(m_1+m_2)-(m_2-m_1)}{m_1+m_2}.
ηa=2m1m1+m2\eta_a = \dfrac{2m_1}{m_1+m_2}
(3)
Step 4Part (b): the head-on collision

Now m1m_1 and m2m_2 move along one line after the collision, with final speeds v1′v_1', v2′v_2' signed along the original direction of motion. Momentum and energy conservation give

m1v0=m1v1′+m2v2′,m1v02=m1v1′2+m2v2′2.m_1v_0 = m_1v_1'+m_2v_2', \qquad m_1v_0^2 = m_1v_1'^2+m_2v_2'^2.

Rearranging each equation isolates the same factor m1(v0−v1′)m_1(v_0-v_1') on the right:

m2v2′=m1(v0−v1′),m2v2′2=m1(v0−v1′)(v0+v1′).\begin{align*}m_2v_2' &= m_1(v_0-v_1'), \\ m_2v_2'^2 &= m_1(v_0-v_1')(v_0+v_1').\end{align*}

Dividing the second line by the first (valid whenever m2v2′≠0m_2v_2'\neq0, i.e. a collision actually occurs) cancels the shared factor, leaving

v2′=v0+v1′.v_2' = v_0+v_1'.

Substituting back into the momentum equation and collecting the v1′v_1' terms on one side,

m1v0=m1v1′+m2(v0+v1′)m1v0−m2v0=m1v1′+m2v1′v0(m1−m2)=v1′(m1+m2)\begin{align*}m_1v_0 &= m_1v_1'+m_2(v_0+v_1') \\ m_1v_0-m_2v_0 &= m_1v_1'+m_2v_1' \\ v_0(m_1-m_2) &= v_1'(m_1+m_2)\end{align*}
v1′=v0 m1−m2m1+m2v_1' = v_0\,\dfrac{m_1-m_2}{m_1+m_2}
(4)
Step 5Fraction of kinetic energy lost, part (b)

The same fraction-lost bookkeeping as in Step 3, now with (4),

ηb=1−v1′2v02=1−(m1−m2m1+m2)2=(m1+m2)2−(m1−m2)2(m1+m2)2.\eta_b = 1-\frac{v_1'^2}{v_0^2} = 1-\left(\frac{m_1-m_2}{m_1+m_2}\right)^2 = \frac{(m_1+m_2)^2-(m_1-m_2)^2}{(m_1+m_2)^2}.

The numerator is a difference of two squares, (a+b)2−(a−b)2=4ab(a+b)^2-(a-b)^2=4ab with a=m1a=m_1, b=m2b=m_2:

ηb=4m1m2(m1+m2)2\eta_b = \dfrac{4m_1m_2}{(m_1+m_2)^2}
(5)
Check

Setting m1=m2m_1=m_2 in part (b) gives ηb=1\eta_b=1: an elastic head-on collision between equal masses stops the striking particle dead and hands all of its kinetic energy to the target, the familiar Newton’s-cradle result. Part (a) carries its own restriction: the right-hand side of (2) stays nonnegative, and ηa\eta_a stays under 11, only when m2>m1m_2>m_1, so a right-angle recoil of the striking particle is possible only off a heavier target.

Remark

As m2→∞m_2\to\infty, part (a) gives ηa→0\eta_a\to0: recoiling at right angles off an effectively immovable target is a pure change of direction, exactly the elastic reflection off a rigid wall, and costs the striking particle no speed at all.