Two identical particles of mass m approach each other at equal and opposite speeds, v. The collision is completely inelastic and results in a single particle at rest. What is the mass of the new particle? How much energy was lost in the collision? How much kinetic energy was lost in this collision?
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35. Special Relativity
Special Vs. Galilean Relativity
Problem 52a
Textbook Question
Calculate the speed of a proton (m = 1.67 x 10-27 kg) whose kinetic energy is exactly half its total energy.

1
Understand the relationship between total energy, rest energy, and kinetic energy in relativistic mechanics. The total energy \( E_{total} \) of a particle is given by \( E_{total} = \gamma m c^2 \), where \( \gamma \) is the Lorentz factor \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \), \( m \) is the rest mass, and \( c \) is the speed of light. The rest energy \( E_{rest} \) is \( m c^2 \), and the kinetic energy \( KE \) is \( KE = E_{total} - E_{rest} \).
For part (a), the problem states that the kinetic energy is half of the total energy. This means \( KE = \frac{1}{2} E_{total} \). Substituting \( KE = E_{total} - E_{rest} \), we get \( E_{total} - E_{rest} = \frac{1}{2} E_{total} \). Simplify this equation to express \( E_{total} \) in terms of \( E_{rest} \): \( E_{total} = 2 E_{rest} \).
Using \( E_{total} = \gamma m c^2 \) and \( E_{rest} = m c^2 \), substitute \( E_{total} = 2 E_{rest} \) into \( \gamma m c^2 = 2 m c^2 \). Cancel \( m c^2 \) on both sides to find \( \gamma = 2 \).
The Lorentz factor \( \gamma \) is defined as \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \). Substitute \( \gamma = 2 \) into this equation: \( 2 = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \). Solve for \( v \) by squaring both sides and isolating \( v^2 \): \( v^2 = \frac{3}{4} c^2 \), so \( v = \frac{\sqrt{3}}{2} c \).
For part (b), the problem states that the kinetic energy is half of the rest energy. This means \( KE = \frac{1}{2} E_{rest} \). Substituting \( KE = E_{total} - E_{rest} \), we get \( E_{total} - E_{rest} = \frac{1}{2} E_{rest} \). Simplify this equation to express \( E_{total} \) in terms of \( E_{rest} \): \( E_{total} = \frac{3}{2} E_{rest} \). Follow the same steps as in part (a) to find \( \gamma \) and solve for \( v \).

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Kinetic Energy
Kinetic energy is the energy an object possesses due to its motion, calculated using the formula KE = 1/2 mv², where m is mass and v is velocity. In the context of the question, understanding how kinetic energy relates to the total energy of a particle is crucial for determining the speed of the proton.
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Intro to Rotational Kinetic Energy
Total Energy
Total energy in the context of relativistic physics includes both kinetic energy and rest energy. For a particle, the total energy can be expressed as E = KE + E₀, where E₀ is the rest energy given by E₀ = mc². This concept is essential for solving part (a) of the question, where kinetic energy is half of the total energy.
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Total Internal Energy
Rest Energy
Rest energy is the energy contained in a particle due to its mass when it is at rest, calculated using E₀ = mc², where m is the mass and c is the speed of light. This concept is vital for part (b) of the question, as it provides a baseline for comparing kinetic energy and determining the speed of the proton when its kinetic energy is half of its rest energy.
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Intro to Energy & Types of Energy
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