The factor γ appears in many relativistic expressions. A value γ = 1.01 implies that relativity changes the Newtonian values by approximately 1% and that relativistic effects can no longer be ignored. At what kinetic energy, in MeV, is γ = 1.01 for (a) an electron, (b) a proton, and (c) an alpha particle?
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35. Special Relativity
Consequences of Relativity
Problem 65
Textbook Question
(III) A certain atom emits light of frequency ƒ₀ when at rest. A monatomic gas composed of these atoms is at temperature T. Some of the gas atoms move toward, and others away from, an observer due to their random thermal motion. Using the rms speed of thermal motion, (a) show that the fractional difference between the Doppler-shifted frequencies for atoms moving directly toward the observer and directly away from the observer is ∆ƒ/ƒ₀ ≈ 2 √3kT/mc². Assume mc² ≫ 3kT. (b) Evaluate ∆ƒ/ƒ₀ for a gas of hydrogen atoms at 650 K. [This “Doppler-broadening” effect is commonly used to measure gas temperature, such as in astronomy.]

1
Step 1: Start by recalling the Doppler effect formula for light. The observed frequency for an atom moving directly toward the observer is given by f₁ = f₀(1 + v/c), and for an atom moving directly away, it is f₂ = f₀(1 - v/c), where v is the speed of the atom relative to the observer, c is the speed of light, and f₀ is the emitted frequency when the atom is at rest.
Step 2: The fractional difference in frequency is defined as Δf/f₀ = (f₁ - f₂)/f₀. Substitute the expressions for f₁ and f₂ into this formula: Δf/f₀ = [(f₀(1 + v/c) - f₀(1 - v/c))]/f₀. Simplify the numerator to get Δf/f₀ = 2v/c.
Step 3: To relate the speed v to the temperature T, use the root-mean-square (rms) speed of the gas atoms, which is derived from the kinetic theory of gases. The rms speed is given by v_rms = √(3kT/m), where k is the Boltzmann constant, T is the temperature, and m is the mass of a single atom. For the Doppler effect, we approximate v ≈ v_rms.
Step 4: Substitute v_rms into the fractional difference formula: Δf/f₀ ≈ 2(√(3kT/m))/c. This simplifies to Δf/f₀ ≈ 2√(3kT/mc²). The assumption mc² ≫ 3kT ensures that the relativistic effects are negligible, and the classical approximation holds.
Step 5: For part (b), substitute the given values for hydrogen gas at T = 650 K. Use m = 1.67 × 10⁻²⁷ kg (mass of a hydrogen atom), k = 1.38 × 10⁻²³ J/K (Boltzmann constant), and c = 3 × 10⁸ m/s (speed of light). Plug these into the formula Δf/f₀ ≈ 2√(3kT/mc²) to evaluate the fractional difference numerically.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Doppler Effect
The Doppler Effect describes the change in frequency or wavelength of a wave in relation to an observer moving relative to the source of the wave. When a source moves toward an observer, the waves are compressed, resulting in a higher frequency (blue shift), while if it moves away, the waves are stretched, leading to a lower frequency (red shift). This effect is crucial for understanding how the motion of gas atoms affects the light they emit.
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The Doppler Effect
Root Mean Square (RMS) Speed
The root mean square speed is a statistical measure of the speed of particles in a gas, representing the average speed of particles in a thermal motion context. It is calculated as the square root of the average of the squares of the speeds of all particles. This concept is essential for determining the thermal motion of gas atoms and how it contributes to the Doppler shift in frequency.
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Root-Mean-Square Speed of Ideal Gases
Thermal Energy and Temperature
Thermal energy is the total kinetic energy of the particles in a substance, which is directly related to its temperature. In the context of gases, temperature is a measure of the average kinetic energy of the gas particles. The relationship between temperature, kinetic energy, and the motion of gas atoms is fundamental for calculating the Doppler shift and understanding how temperature influences the observed frequency of emitted light.
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Volume Thermal Expansion
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