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35. Special Relativity
Special Vs. Galilean Relativity
Problem 7
Textbook Question
At what speed do the relativistic formulas for (a) length and (b) time intervals differ from classical values by 1.00%? (This is a reasonable way to estimate when to use relativistic calculations rather than classical.)

1
Start by recalling the relativistic formulas for length contraction and time dilation. The length contraction formula is L = L₀√(1 - v²/c²), and the time dilation formula is Δt = Δt₀ / √(1 - v²/c²), where v is the object's speed, c is the speed of light, L₀ is the proper length, and Δt₀ is the proper time interval.
To determine when the relativistic formulas differ from classical values by 1.00%, set up the condition for each case. For length contraction, the condition is |L - L₀| / L₀ = 0.01. For time dilation, the condition is |Δt - Δt₀| / Δt₀ = 0.01.
Substitute the relativistic formulas into the conditions. For length contraction, this becomes |L₀√(1 - v²/c²) - L₀| / L₀ = 0.01. For time dilation, this becomes |Δt₀ / √(1 - v²/c²) - Δt₀| / Δt₀ = 0.01.
Simplify each equation to isolate the term involving v²/c². For length contraction, simplify to √(1 - v²/c²) = 0.99. For time dilation, simplify to 1 / √(1 - v²/c²) = 1.01.
Solve each equation for v²/c². For length contraction, square both sides to get 1 - v²/c² = 0.9801, then solve for v²/c² = 0.0199. For time dilation, square both sides to get 1 / (1 - v²/c²) = 1.0201, then solve for v²/c² = 0.0198. Finally, take the square root of v²/c² in each case to find the speed v as a fraction of the speed of light c.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Relativity
Relativity, formulated by Albert Einstein, fundamentally alters our understanding of space and time. It posits that the laws of physics are the same for all observers, regardless of their relative motion. This leads to the conclusion that measurements of time and length can vary depending on the observer's speed, particularly as they approach the speed of light.
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Intro to Relative Motion (Relative Velocity)
Lorentz Transformation
The Lorentz Transformation equations describe how measurements of time and space change for observers in different inertial frames. These equations account for the effects of relative velocity on time dilation and length contraction, which become significant at speeds close to the speed of light. They are essential for calculating the relativistic effects that deviate from classical physics.
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Lorentz Transformations of Velocity
Classical vs. Relativistic Physics
Classical physics, based on Newtonian mechanics, assumes that time and space are absolute and independent of the observer's motion. In contrast, relativistic physics introduces the idea that time and space are interwoven and relative, leading to phenomena such as time dilation and length contraction. Understanding the threshold at which relativistic effects become significant is crucial for determining when to apply relativistic formulas.
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Special Vs. Galilean Relativity
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Related Practice
Multiple Choice
Olive the astronaut is flying her spaceship back home to earth at . Her spaceship has lights on it; one at the front of her ship, and one at the back of the ship. Olive notes that the two lights flash simultaneously. Are they simultaneous according to an Earth-based observer? If not, which one blinked first?
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