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Exercises · 13.20

Q.Calculate the height of the potential barrier for a head on collision of two deuterons. (Hint: The height of the potential barrier is given by the Coulomb repulsion between the two deuterons when they just touch each other. Assume that they can be taken as hard spheres of radius 2.0 fm2.0\ \text{fm}.)

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The potential barrier height is the electrostatic potential energy at the point where two deuterons just touch. Treating them as point charges at a centre-to-centre distance of 4.0 fm4.0\ \text{fm}, the barrier height is 360 keV\boxed{360\ \text{keV}}.

The key insight here is that the "potential barrier" in nuclear fusion is the Coulomb repulsion that two positively charged nuclei must overcome before the strong nuclear force can bind them. For a head-on collision, the closest approach before the nuclear surfaces meet is when the centres are separated by the sum of their radii. At that instant, all the kinetic energy of approach has been converted into electrostatic potential energy — and that potential energy is the barrier height.

Let’s work through it step by step.

  1. Understand the geometry of "just touching" Each deuteron is a hydrogen isotope nucleus (one proton, one neutron) with charge +e+e. The problem tells us to treat them as hard spheres of radius r=2.0 fmr = 2.0\ \text{fm}. When they just touch in a head-on collision, the centre-to-centre distance dd is:

d=r+r=2.0 fm+2.0 fm=4.0 fm.d = r + r = 2.0\ \text{fm} + 2.0\ \text{fm} = 4.0\ \text{fm}.

This is the separation at which the Coulomb barrier is maximum — any closer and the strong force would begin to dominate, but we are finding the height of the barrier, i.e., the energy needed to reach this point.

  1. The Coulomb potential energy formula The electrostatic potential energy of two point charges q1q_1 and q2q_2 separated by distance dd is:

U=14πε0q1q2d.U = \frac{1}{4\pi\varepsilon_0} \frac{q_1 q_2}{d}.

Here, each deuteron has charge q=+e=1.602×10−19 Cq = +e = 1.602 \times 10^{-19}\ \text{C}. So q1q2=e2q_1 q_2 = e^2.

  1. Plug in the numbers — but watch the units We want the answer in electronvolts (eV) because nuclear energies are typically expressed that way. The constant 14πε0=8.987×109 N⋅m2/C2\frac{1}{4\pi\varepsilon_0} = 8.987 \times 10^9\ \text{N·m}^2/\text{C}^2. But a much cleaner route: use the known value ke2=1.44 MeV⋅fmke^2 = 1.44\ \text{MeV·fm}, where k=14πε0k = \frac{1}{4\pi\varepsilon_0}. This is a standard nuclear physics shortcut. …

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