(II) You travel to a star 115 light-years from Earth at a speed of 2.90 x 108 m/s. What do you measure this distance to be?
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35. Special Relativity
Consequences of Relativity
Problem 32
Textbook Question
Calculate the maximum kinetic energy of the electron when a muon decays from rest via μ⁻ ⟶ e⁻ + vₑ + vμ. [Hint: In what direction do the two neutrinos move relative to the electron in order to give the electron the maximum kinetic energy? Both energy and momentum are conserved; use relativistic formulas.]

1
Understand the problem: A muon decays into an electron, an electron neutrino, and a muon neutrino. To find the maximum kinetic energy of the electron, we need to consider the conservation of energy and momentum, and the relativistic nature of the particles involved.
Step 1: Write the conservation of energy equation. The total energy of the system before and after the decay must be equal. The initial energy is the rest energy of the muon, given by \( E_{\mu} = m_{\mu}c^2 \), where \( m_{\mu} \) is the mass of the muon and \( c \) is the speed of light. After the decay, the total energy is the sum of the relativistic energies of the electron, electron neutrino, and muon neutrino: \( E_{\mu} = E_e + E_{v_e} + E_{v_\mu} \).
Step 2: Write the conservation of momentum equation. The total momentum of the system before and after the decay must also be equal. Since the muon is initially at rest, its momentum is zero. After the decay, the sum of the momenta of the electron, electron neutrino, and muon neutrino must also be zero: \( \vec{p}_e + \vec{p}_{v_e} + \vec{p}_{v_\mu} = 0 \).
Step 3: Determine the configuration for maximum kinetic energy of the electron. The electron will have maximum kinetic energy when the two neutrinos move in the same direction, opposite to the electron. This configuration maximizes the electron's energy while conserving momentum.
Step 4: Use the relativistic energy-momentum relation to express the electron's energy. The total energy of the electron is given by \( E_e = \sqrt{(p_e c)^2 + (m_e c^2)^2} \), where \( p_e \) is the momentum of the electron and \( m_e \) is its mass. The kinetic energy of the electron is then \( K_e = E_e - m_e c^2 \). Solve for \( p_e \) and \( E_e \) using the conservation equations from Steps 1 and 2, considering the maximum energy configuration.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Conservation of Energy
The principle of conservation of energy states that the total energy in a closed system remains constant over time. In particle decay processes, the energy before the decay must equal the energy after the decay. This includes the rest mass energy of the particles involved and their kinetic energy. Understanding this concept is crucial for calculating the maximum kinetic energy of the electron produced in the decay.
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Conservation of Momentum
Conservation of momentum is a fundamental principle stating that the total momentum of a closed system remains constant if no external forces act on it. In the context of particle decay, the momentum before the decay must equal the total momentum after the decay. This principle helps determine the directions and magnitudes of the velocities of the decay products, which is essential for maximizing the kinetic energy of the electron.
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Relativistic Kinetic Energy
Relativistic kinetic energy accounts for the effects of special relativity when particles move at speeds close to the speed of light. The formula for relativistic kinetic energy is given by K.E. = (γ - 1)mc², where γ (gamma) is the Lorentz factor. This concept is important for accurately calculating the kinetic energy of the electron after the muon decay, especially since the decay products can have significant velocities.
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