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Worked Examples · Example 5.11

Q.Slowing down of neutrons: In a nuclear reactor a neutron of high speed (typically 107 m s−110^{7}\ \text{m s}^{-1}) must be slowed to 103 m s−110^{3}\ \text{m s}^{-1} so that it can have a high probability of interacting with isotope 92235U^{235}_{92}\text{U} and causing it to fission. Show that a neutron can lose most of its kinetic energy in an elastic collision with a light nuclei like deuterium or carbon which has a mass of only a few times the neutron mass. The material making up the light nuclei, usually heavy water (D2O\text{D}_2\text{O}) or graphite, is called a moderator.

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In a head-on elastic collision, a neutron can transfer a large fraction of its kinetic energy to a stationary light nucleus. The fraction of energy lost depends only on the mass ratio, and for deuterium (mass ≈ 2 u) the neutron retains only about 11% of its initial energy per collision, showing why light nuclei make effective moderators.

The key insight here is Conservation of Momentum combined with Conservation of Kinetic Energy — the hallmark of an elastic collision. When a fast neutron hits a stationary nucleus, the two bounce off each other without any energy being lost to heat or deformation. The neutron slows down, and the nucleus recoils, carrying away the energy.

Why does a light target work best? Think of a ball hitting a wall versus hitting a pillow. A heavy wall barely moves — the ball bounces back with nearly the same speed. A light pillow flies backward, taking most of the ball’s energy with it. In nuclear terms, a light nucleus (mass close to the neutron’s) can “absorb” a large share of the kinetic energy, while a heavy nucleus (like uranium) barely budges, leaving the neutron still fast.

Let’s prove this quantitatively.


  1. Set up the collision in one dimension (head-on, maximum energy transfer). Let the neutron have mass mm and initial speed viv_i. The target nucleus has mass MM and is initially at rest. After the collision, the neutron moves with speed vfv_f and the nucleus with speed VV. By conservation of momentum:

mvi=mvf+MVm v_i = m v_f + M V

By conservation of kinetic energy (elastic):

12mvi2=12mvf2+12MV2\frac{1}{2} m v_i^2 = \frac{1}{2} m v_f^2 + \frac{1}{2} M V^2

  1. Solve for the final neutron speed vfv_f. From the momentum equation: V=mM(vi−vf)V = \frac{m}{M}(v_i - v_f). Substitute into the energy equation:

mvi2=mvf2+M[mM(vi−vf)]2m v_i^2 = m v_f^2 + M \left[ \frac{m}{M}(v_i - v_f) \right]^2

Simplify:

mvi2=mvf2+m2M(vi−vf)2m v_i^2 = m v_f^2 + \frac{m^2}{M}(v_i - v_f)^2

Divide through by mm:

vi2=vf2+mM(vi−vf)2v_i^2 = v_f^2 + \frac{m}{M}(v_i - v_f)^2

This is a quadratic in vfv_f. Expand and rearrange:

vi2=vf2+mM(vi2−2vivf+vf2)v_i^2 = v_f^2 + \frac{m}{M}(v_i^2 - 2 v_i v_f + v_f^2)

Multiply through by MM:

Mvi2=Mvf2+mvi2−2mvivf+mvf2M v_i^2 = M v_f^2 + m v_i^2 - 2 m v_i v_f + m v_f^2

Bring terms together:

(M−m)vi2=(M+m)vf2−2mvivf(M - m) v_i^2 = (M + m) v_f^2 - 2 m v_i v_f

Rearranging into standard quadratic form:

(M+m)vf2−2mvivf+(m−M)vi2=0(M + m) v_f^2 - 2 m v_i v_f + (m - M) v_i^2 = 0

  1. Solve the quadratic for vfv_f. Using the quadratic formula:

vf=2mvi±4m2vi2−4(M+m)(m−M)vi22(M+m)v_f = \frac{2 m v_i \pm \sqrt{4 m^2 v_i^2 - 4 (M+m)(m-M) v_i^2}}{2(M+m)}

Notice that (M+m)(m−M)=m2−M2(M+m)(m-M) = m^2 - M^2, so the discriminant becomes:

4m2vi2−4(m2−M2)vi2=4M2vi24 m^2 v_i^2 - 4(m^2 - M^2) v_i^2 = 4 M^2 v_i^2

Hence:

vf=2mvi±2Mvi2(M+m)=(m±M)viM+mv_f = \frac{2 m v_i \pm 2 M v_i}{2(M+m)} = \frac{(m \pm M) v_i}{M+m}

The plus sign gives vf=viv_f = v_i (no collision — the neutron passes through), which is physically trivial. The minus sign gives the real result:

vf=m−Mm+M viv_f = \frac{m - M}{m + M} \, v_i

vf=m−Mm+M viv_f = \frac{m - M}{m + M} \, v_i

For a head-on elastic collision, the final speed of the lighter particle (neutron) is reduced by the factor ∣m−M∣m+M\frac{|m-M|}{m+M}. If M>mM > m, the neutron reverses direction (negative vfv_f), but the magnitude is what matters for energy.

  1. Find the fraction of kinetic energy retained by the neutron. Initial kinetic energy: Ki=12mvi2K_i = \frac{1}{2} m v_i^2 Final kinetic energy: Kf=12mvf2=12m(m−Mm+M)2vi2K_f = \frac{1}{2} m v_f^2 = \frac{1}{2} m \left( \frac{m - M}{m + M} \right)^2 v_i^2 So the fraction retained is:

KfKi=(m−Mm+M)2\frac{K_f}{K_i} = \left( \frac{m - M}{m + M} \right)^2

The fraction lost to the nucleus is:

1−(m−Mm+M)2=4mM(m+M)21 - \left( \frac{m - M}{m + M} \right)^2 = \frac{4 m M}{(m + M)^2}

Watch out

A common mistake is to think the neutron loses all its energy when M=mM = m. Actually, for equal masses (M=mM = m), the fraction retained is (02m)2=0\left( \frac{0}{2m} \right)^2 = 0 — yes, the neutron stops dead, transferring all its energy. But for MM slightly larger, the retained fraction jumps quickly.

  1. Apply to real moderators. Neutron mass m≈1m \approx 1 u (atomic mass unit).
    • Deuterium (in heavy water): M≈2M \approx 2 u KfKi=(1−21+2)2=(−13)2=19≈0.111\frac{K_f}{K_i} = \left( \frac{1 - 2}{1 + 2} \right)^2 = \left( \frac{-1}{3} \right)^2 = \frac{1}{9} \approx 0.111 …

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