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Where Motion Doubles a Particle's Energy

Irodov 1.373DifficultyDifficulty 2 of 5UniquenessUniqueness 2 of 5

Problem Irodov 1.373

A particle of rest mass m0m_0 moves with a speed vv at which its kinetic energy comes out exactly equal to its rest energy m0c2m_0c^2. Find that speed.

Given
  • m0m_0
  • T=m0c2T = m_0c^2
  • β=v/c\beta = v/c
  • c=3.00×108c = 3.00\times10^8 m/s
Find
The speed vv at which the kinetic energy reaches the rest energy

Solution

Step 1Turn the condition into a condition on the Lorentz factor

The kinetic energy of a moving particle is everything its total energy carries beyond the rest energy, so writing the total energy as γm0c2\gamma m_0c^2 with γ=(1−β2)−1/2\gamma = (1-\beta^2)^{-1/2} gives the kinetic energy in the same terms.

T=γm0c2−m0c2=(γ−1) m0c2T = \gamma m_0c^2-m_0c^2 = (\gamma-1)\,m_0c^2

Setting this equal to the rest energy and dividing both sides by m0c2m_0c^2 removes the mass from the problem entirely.

(γ−1) m0c2=m0c2γ−1=1\begin{align*}(\gamma-1)\,m_0c^2 &= m_0c^2 \\ \gamma-1 &= 1\end{align*}

so the required state is the one whose Lorentz factor is two.

γ=2\gamma = 2
(1)
Step 2Invert the Lorentz factor for the speed

The definition of γ\gamma is a statement about 1−β2\sqrt{1-\beta^2}, so it inverts by squaring and solving for β2\beta^2, and the inversion is worth doing once for a general γ\gamma rather than for the value at hand.

γ=11−β21−β2=1γ2β2=1−1γ2(2) \begin{aligned} \gamma &= \frac{1}{\sqrt{1-\beta^2}} \\ 1-\beta^2 &= \frac{1}{\gamma^2} \\ \beta^2 &= 1-\frac{1}{\gamma^2} \end{aligned} \tag{2}

The speed is cc times the positive root of this, so the whole problem now rests on the single number γ\gamma of (1).

Step 3Put the number in

Substituting the required γ=2\gamma = 2 of (1) into (2), one factor at a time:

1γ2=14,1−1γ2=34,34=0.866\frac{1}{\gamma^2} = \frac14, \qquad 1-\frac{1}{\gamma^2} = \frac34, \qquad \sqrt{\frac34} = 0.866

Multiplying that fraction of cc by c=3.00×108c = 3.00\times10^8 m/s gives the speed itself.

v=c1−1γ2=32 c=2.6×108 m/sv = c\sqrt{1-\frac{1}{\gamma^2}} = \frac{\sqrt3}{2}\,c = 2.6\times10^8\ \text{m/s}
(3)
Kinetic energy in units of the rest energy, against speed. The gold curve is the relativistic γ-1, the royal one the classical β^2/2. Gold reaches 1 at the marked abscissa 0.87, where the classical curve stands at 0.38.

Kinetic energy in units of the rest energy, against speed. The gold curve is the relativistic γ−1\gamma-1, the royal one the classical β2/2\beta^2/2. Gold reaches 11 at the marked abscissa 0.870.87, where the classical curve stands at 0.380.38.

Check

Run the speed back through the condition (1). At β=3/2\beta = \sqrt3/2 the quantity 1−β21-\beta^2 is 1/41/4, its square root is 1/21/2, and the Lorentz factor is its reciprocal, γ=2\gamma = 2; then T=(γ−1)m0c2T = (\gamma-1)m_0c^2 is m0c2m_0c^2, the rest energy, as required. The classical formula would have answered this question with 12m0v2=m0c2\frac{1}{2}m_0v^2 = m_0c^2, that is v=c2v = c\sqrt2, a speed no particle can have, so the relativistic treatment is not a refinement here but the only one that can answer at all.

Remark

At this speed the particle’s total energy in the laboratory frame is 2m0c22m_0c^2, half of it rest energy and half of it kinetic: below this speed most of a particle’s energy is rest energy, above it most is kinetic, so 3 c/2\sqrt3\,c/2 is the crossover. Two other readings of the same γ=2\gamma = 2, both in that same laboratory frame: the particle’s relativistic momentum is twice the Newtonian m0vm_0v, and one second of its own proper time corresponds to two seconds of laboratory time. The kinetic energy this costs is 0.510.51 MeV for an electron and 938938 MeV for a proton, so the very same speed is routine bench physics for the one and accelerator work for the other.