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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: 9780137488179Non è quello che usi tu?Cambia libro di testo
Capitolo 35, Problema 54

Suppose a spacecraft of mass 17,000 kg was accelerated to 0.22c.
(a) How much kinetic energy would it have?
(b) If you used the classical formula for kinetic energy, by what percentage would you be in error?

Guida verificata passo dopo passo
1
Step 1: Recognize that the problem involves relativistic kinetic energy because the spacecraft's velocity (0.22c) is a significant fraction of the speed of light (c). The relativistic kinetic energy formula is \( KE = (\gamma - 1)m c^2 \), where \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \), \( m \) is the mass, \( v \) is the velocity, and \( c \) is the speed of light.
Step 2: Calculate the Lorentz factor \( \gamma \) using \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \). Substitute \( v = 0.22c \) into the equation: \( \gamma = \frac{1}{\sqrt{1 - (0.22)^2}} \). Simplify the expression to find \( \gamma \).
Step 3: Substitute the values of \( \gamma \), \( m = 17,000 \ \text{kg} \), and \( c = 3.00 \times 10^8 \ \text{m/s} \) into the relativistic kinetic energy formula \( KE = (\gamma - 1)m c^2 \). This will give the relativistic kinetic energy of the spacecraft.
Step 4: For the classical kinetic energy, use the formula \( KE_{\text{classical}} = \frac{1}{2} m v^2 \). Substitute \( m = 17,000 \ \text{kg} \) and \( v = 0.22c \) into the equation. Simplify to find the classical kinetic energy.
Step 5: Calculate the percentage error using the formula \( \text{Percentage Error} = \frac{|KE_{\text{relativistic}} - KE_{\text{classical}}|}{KE_{\text{relativistic}}} \times 100 \). Substitute the values of \( KE_{\text{relativistic}} \) and \( KE_{\text{classical}} \) from the previous steps to determine the error.

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Relativistic Kinetic Energy

In relativistic physics, the kinetic energy of an object moving at a significant fraction of the speed of light (denoted as 'c') is calculated using the formula KE = (γ - 1)mc², where γ (gamma) is the Lorentz factor. The Lorentz factor accounts for the effects of relativity, which become significant as an object's speed approaches the speed of light. This formula differs from the classical kinetic energy formula, highlighting the need for relativistic considerations at high velocities.
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Classical Kinetic Energy

The classical kinetic energy formula is given by KE = 0.5mv², where 'm' is the mass of the object and 'v' is its velocity. This formula is valid for objects moving at speeds much less than the speed of light. However, it fails to accurately predict the kinetic energy of objects moving at relativistic speeds, leading to significant errors when applied in such contexts.
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Lorentz Factor

The Lorentz factor, denoted as γ (gamma), is a crucial component in the equations of special relativity. It is defined as γ = 1 / √(1 - v²/c²), where 'v' is the object's velocity and 'c' is the speed of light. As an object's speed approaches the speed of light, the Lorentz factor increases, indicating that time dilation and length contraction effects become significant, which must be considered when calculating energy and momentum in relativistic scenarios.
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(These transformation equations hold, actually, for any direction of p→\(\overrightarrow{\mathbf{p}\)}, as long as the motion of S' is along the x axis.) (b) Show that px, py, pz, E/c transform according to the Lorentz transformation in the same way as x, y, z, ct.

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(b) How much earlier did he fire?

(c) Who was struck first?

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