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Ch 01: Units, Physical Quantities & Vectors
Chapter 1, Problem 37

Compute the kinetic energy of a proton (mass 1.67 * 10-27 kg) using both the nonrelativistic and relativistic expressions, and compute the ratio of the two results (relativistic divided by nonrelativistic) for speeds of (a) 8.00 * 107 m/s and (b) 2.85 * 108 m/s.

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Step 1: Calculate the nonrelativistic kinetic energy using the formula KE = (1/2) * m * v^2, where m is the mass of the proton and v is its speed.
Step 2: Calculate the relativistic kinetic energy using the formula KE = (\gamma - 1) * m * c^2, where \gamma is the Lorentz factor given by \gamma = 1 / \sqrt{1 - (v^2/c^2)}, c is the speed of light, m is the mass of the proton, and v is its speed.
Step 3: Compute the Lorentz factor \gamma for each given speed v using the formula \gamma = 1 / \sqrt{1 - (v^2/c^2)}.
Step 4: Substitute the values of \gamma, m, and c into the relativistic kinetic energy formula to find the relativistic kinetic energy for each speed.
Step 5: Calculate the ratio of the relativistic kinetic energy to the nonrelativistic kinetic energy for each speed by dividing the relativistic result by the nonrelativistic result.

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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 for nonrelativistic speeds, where m is mass and v is velocity. In relativistic physics, the kinetic energy is given by KE = (γ - 1)mc², where γ (gamma) is the Lorentz factor, accounting for the effects of traveling at speeds close to the speed of light.
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Relativistic Effects

Relativistic effects become significant as an object's speed approaches the speed of light (approximately 3.00 x 10^8 m/s). These effects include time dilation and length contraction, which alter the behavior of objects in motion. The Lorentz factor, γ, is defined as γ = 1 / √(1 - v²/c²), and it increases as velocity v approaches the speed of light, affecting calculations of energy and momentum.
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Ratio of Energies

The ratio of relativistic to nonrelativistic kinetic energy provides insight into how much relativistic effects influence energy calculations at high speeds. This ratio is calculated by dividing the relativistic kinetic energy by the nonrelativistic kinetic energy. Analyzing this ratio at different speeds helps illustrate the transition from classical to relativistic physics and the significance of relativistic corrections in high-velocity scenarios.
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Related Practice
Textbook Question
Relativistic Baseball. Calculate the magnitude of the force required to give a 0.145-kg baseball an acceleration a = 1.00 m/s2 in the direction of the baseball's initial velocity when this velocity has a magnitude of (a) 10.0 m/s; (b) 0.900c; (c) 0.990c.
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Textbook Question
A proton (rest mass 1.67 * 10-27 kg) has total energy that is 4.00 times its rest energy. What are (a) the kinetic energy of the proton; (b) the magnitude of the momentum of the proton; (c) the speed of the proton?
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Textbook Question
Electrons are accelerated through a potential difference of 750 kV, so that their kinetic energy is 7.50 * 105 eV. (a) What is the ratio of the speed v of an electron having this energy to the speed of light, c? (b) What would the speed be if it were computed from the principles of classical mechanics?
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Textbook Question
Why Are We Bombarded by Muons? Muons are unstable subatomic particles that decay to electrons with a mean lifetime of 2.2 ms. They are produced when cosmic rays bombard the upper atmosphere about 10 km above the earth's surface, and they travel very close to the speed of light. The problem we want to address is why we see any of them at the earth's surface. (a) What is the greatest distance a muon could travel during its 2.2@ms lifetime? (b) According to your answer in part (a), it would seem that muons could never make it to the ground. But the 2.2@ms lifetime is measured in the frame of the muon, and muons are moving very fast. At a speed of 0.999c, what is the mean lifetime of a muon as measured by an observer at rest on the earth? How far would the muon travel in this time? Does this result explain why we find muons in cosmic rays? (c) From the point of view of the muon, it still lives for only 2.2 ms, so how does it make it to the ground? What is the thickness of the 10 km of atmosphere through which the muon must travel, as measured by the muon? Is it now clear how the muon is able to reach the ground?
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Textbook Question
As you pilot your space utility vehicle at a constant speed toward the moon, a race pilot flies past you in her spaceracer at a constant speed of 0.800c relative to you. At the instant the spaceracer passes you, both of you start timers at zero. (a) At the instant when you measure that the spaceracer has traveled 1.20 * 108 m past you, what does the race pilot read on her timer? (b) When the race pilot reads the value calculated in part (a) on her timer, what does she measure to be your distance from her? (c) At the instant when the race pilot reads the value calculated in part (a) on her timer, what do you read on yours?
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Textbook Question
A photon of green light has a wavelength of 520 nm. Find the photon's frequency, magnitude of momentum, and energy. Express the energy in both joules and electron volts.
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