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Direct central impact and restitution

Short answer

In direct central impact, velocities lie along the line of centres. Coefficient of restitution e = (v₂ – v₁)/(u₁ – u₂). Using conservation of momentum and the restitution equation, final velocities are obtained; the loss of kinetic energy equals m₁ m₂ (1 – e²)(u₁ – u₂)² / [2(m₁ + m₂)].

Explain direct central impact. Define coefficient of restitution. For two smooth spheres of masses m1 and m2 moving with velocities u1 and u2 (u1 > u2) along the line of centres, derive expressions for their velocities after impact and the loss of kinetic energy.

Direct central impact

Two bodies collide in direct central impact when their centres of mass lie on the line of impact, which is also the common normal at the contact point, and the velocities before and after impact are along this line. If the surfaces are smooth, the impulses act only along the line of impact.

  before:  (m1)--> u1      (m2)--> u2      u1 > u2
  after :  (m1)--> v1      (m2)--> v2      v2 >= v1

The impact has two phases: deformation (from first contact to maximum compression, when both bodies have a common velocity) and restitution (the bodies regain shape and separate).

Coefficient of restitution

ee is the ratio of the impulse during restitution to the impulse during deformation, which for a direct central impact equals

e=velocity of separationvelocity of approach=v2−v1u1−u2e = \frac{\text{velocity of separation}}{\text{velocity of approach}} = \frac{v_2 - v_1}{u_1 - u_2}

e=1e = 1 for a perfectly elastic impact and e=0e = 0 for a perfectly plastic impact; 0<e<10 < e < 1 in practice.

Final velocities

Conservation of momentum (no external impulse):

m1u1+m2u2=m1v1+m2v2(1)m_1 u_1 + m_2 u_2 = m_1 v_1 + m_2 v_2 \quad (1)

Definition of ee: v2−v1=e(u1−u2)v_2 - v_1 = e(u_1 - u_2) (2)

Solving (1) and (2):

v1=m1u1+m2u2−m2e(u1−u2)m1+m2v2=m1u1+m2u2+m1e(u1−u2)m1+m2v_1 = \frac{m_1 u_1 + m_2 u_2 - m_2 e(u_1 - u_2)}{m_1 + m_2} \qquad v_2 = \frac{m_1 u_1 + m_2 u_2 + m_1 e(u_1 - u_2)}{m_1 + m_2}

Loss of kinetic energy

ΔT=12m1u12+12m2u22−12m1v12−12m2v22\Delta T = \tfrac12 m_1 u_1^2 + \tfrac12 m_2 u_2^2 - \tfrac12 m_1 v_1^2 - \tfrac12 m_2 v_2^2

Substituting the velocities and simplifying:

ΔT=m1m22(m1+m2) (1−e2) (u1−u2)2\Delta T = \frac{m_1 m_2}{2(m_1 + m_2)}\,(1 - e^2)\,(u_1 - u_2)^2

For e=1e = 1, ΔT=0\Delta T = 0 (kinetic energy conserved); for e=0e = 0 the loss is maximum and both bodies move together with velocity (m1u1+m2u2)/(m1+m2)(m_1u_1 + m_2u_2)/(m_1+m_2). The lost energy becomes heat, sound and permanent deformation.

✓ Answer checked by Claude Opus 5.5 (high effort)

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