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Ch. 36 - The Special Theory of Relativity
Giancoli Douglas - Physics for Scientists and Engineers 5th edition
Giancoli Douglas5th editionPhysics for Scientists and EngineersISBN: 9780137488179Not the one you use?Change textbook
Chapter 35, Problem 85

A pi meson of mass mπ decays at rest into a muon (mass mμ) and a neutrino of negligible or zero mass. Show that the kinetic energy of the muon is Kμ = (mπ - mμ)² c² / (2mπ).

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Start by applying the principle of conservation of energy. Since the pi meson is initially at rest, its total energy is equal to its rest energy, which is given by E_π = m_π c². After the decay, the total energy is shared between the muon and the neutrino.
Next, apply the principle of conservation of momentum. Since the pi meson is initially at rest, the total momentum of the system after the decay must also be zero. This means the muon and the neutrino must have equal and opposite momenta.
Express the total energy of the muon and neutrino. The muon's total energy is E_μ = √(p²c² + m_μ²c⁴), where p is the magnitude of the muon's momentum. The neutrino's energy is E_ν = pc, since its mass is negligible.
Use conservation of energy to write E_π = E_μ + E_ν. Substituting the expressions for E_μ and E_ν, you get m_π c² = √(p²c² + m_μ²c⁴) + pc.
Square both sides of the equation to eliminate the square root, simplify, and solve for the muon's kinetic energy K_μ = E_μ - m_μ c². After algebraic manipulation, you will find K_μ = (m_π - m_μ)² c² / (2m_π).

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Conservation of Energy

In any physical process, the total energy before the event must equal the total energy after the event. In the case of the decay of a pi meson, the initial rest energy of the meson is converted into the kinetic energy of the resulting particles, the muon and the neutrino. This principle allows us to relate the masses of the particles involved to their kinetic energies.
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Rest Mass Energy

The rest mass energy of a particle is given by Einstein's equation E = mc², where m is the rest mass and c is the speed of light. For the pi meson at rest, its total energy is simply its rest mass energy. This energy is crucial for calculating the kinetic energy of the decay products, as it provides the initial energy available for conversion into kinetic energy.
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Kinetic Energy in Relativistic Physics

In relativistic physics, the kinetic energy of a particle is not simply given by the classical formula (1/2)mv², especially when dealing with particles moving at speeds close to the speed of light. Instead, the kinetic energy can be derived from the difference in rest mass energy before and after a decay process, which is essential for deriving the expression for the muon's kinetic energy in this decay scenario.
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Related Practice
Textbook Question

How much energy would be required to break a helium nucleus into its constituents, two protons and two neutrons? The rest masses of a proton (including an electron), a neutron, and neutral helium are, respectively, 1.00783 u, 1.00867 u, and 4.00260 u. (This energy difference is called the total binding energy of the 24He_2^4\(\text{He}\) nucleus.)

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Textbook Question

The Sun radiates energy at a rate of about 4 x 10²⁶ W.

(a) At what rate is the Sun’s mass decreasing?

(b) How long does it take for the Sun to lose a mass equal to that of Earth?

(c) Estimate how long the Sun could last if it radiated constantly at this rate.

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Textbook Question

A spaceship and its occupants have a total mass of 160,000 kg. The occupants would like to travel to a star that is 32 light-years away at a speed of 0.70c. To accelerate, the engine of the spaceship changes mass directly to energy.

(a) Estimate how much mass will be converted to energy to accelerate the spaceship to this speed.

(b) Assuming the acceleration is rapid, so the speed for the entire trip can be taken to be 0.70c, determine how long the trip will take according to the astronauts on board.

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Textbook Question

For a 1.0-kg mass, make a plot of the kinetic energy as a function of speed for speeds from 0 to 0.9c, using both the classical formula ( K = 1/2 mv²) and the correct relativistic formula ( K = ( γ -1)mc²).

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Textbook Question

A quasar emits familiar hydrogen lines whose wavelengths are 8.5% longer than what we measure in the laboratory.

(a) Using the Doppler formula for light, estimate the speed of this quasar.

(b) What result would you obtain if you used the “classical” Doppler shift discussed in Chapter 16?

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Textbook Question

Two protons, each having a speed of 0.945c in the laboratory, are moving toward each other. Determine (a) the momentum of each proton in the laboratory, (b) the total momentum of the two protons in the laboratory, and (c) the momentum of one proton as seen by the other proton.

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