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A super train (proper length \(100 \mathrm{m}\) ) travels at a speed of \(0.950 c\) as it passes through a tunnel (proper length \(50.0 \mathrm{m}) .\) As seen by a track side observer, is the train ever completely within the tunnel? If so, with how much space to spare?

Short Answer

Expert verified
The contracted length of the train as seen by the observer will be less than the length of the tunnel. Therefore, the train can completely fit within the tunnel. The space to spare can be obtained by subtracting the contracted length of the train from the length of the tunnel.

Step by step solution

01

Understand the given values

The problem provides the proper length of the train \(L_0 = 100 m\) and that of the tunnel \(L_{tunnel} = 50 m\). It also provides the speed of the train \(v = 0.950c\) where \(c\) is the speed of light.
02

Compute the contracted length of the train

The formula for length contraction is given by \(L = L_0/\gamma\) where \(\gamma = 1/ \sqrt{1 - v^2/c^2}\). Substituting the given values in this formula, compute the contracted length of the train.
03

Compare the contracted length with the tunnel length

Compare the contracted length of the train derived in step 2 to the given length of the tunnel. If the contracted length of the train is less than that of the tunnel, conclude that the train can fit within the tunnel.
04

Calculate the space to spare

If the contracted length is less than the length of the tunnel, subtract the contracted length from the tunnel length to find out the space to spare.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Understanding Special Relativity
Albert Einstein's theory of special relativity revolutionized our understanding of space, time, and motion. Introduced in 1905, it encompassed two main postulates. Firstly, the laws of physics are the same in all inertial frames of reference – this means that whether you're standing still or moving at constant velocity, you shouldn't be able to tell the difference based purely on the laws of physics. The second postulate asserts that the speed of light in a vacuum is the same for all observers, regardless of their relative motion or the motion of the light source.

One of the most intriguing consequences of special relativity is length contraction. This phenomenon occurs when an object moves relative to an observer at significant fractions of the speed of light. To the observer, the object appears shorter along the direction of motion than when it is at rest. This isn't because the physical dimensions of the object have changed but because of the way space and time are interwoven at high velocities. Length contraction can be counterintuitive, but it's an important concept to grasp when dealing with high-speed scenarios, like in the case of the super train exercise.

Einstein's insights transformed our comprehension of the universe, challenging us to let go of classical views held for centuries and accept that our measurements of time and distance can change under certain conditions.
The Lorentz Factor in Relativity
At the core of special relativity’s calculations is the Lorentz factor (denoted as \( \gamma \)), a term that adjusts measurements of time, length, and even mass, based on the relative velocity between an observer and an object in motion. This factor is named after Hendrik Lorentz, who derived essential components of this theory before Einstein.

The equation for the Lorentz factor is \( \gamma = \frac{1}{\sqrt{1 - (\frac{v}{c})^2}} \), where \( v \) is the relative velocity between the observer and the object, and \( c \) is the speed of light. This factor becomes ever more significant as \( v \) approaches the speed of light, leading to prominent effects like time dilation and length contraction. When \( v \) is much less than \( c \) (the case in everyday life), the Lorentz factor is approximately equal to 1, meaning no noticeable relativistic effects. However, as seen with the super train traveling at \( 0.950c \), the Lorentz factor significantly deviates from 1, leading to substantial length contraction.

In our exercise, calculating the Lorentz factor successfully is vital to determine how much the train contracts as it approaches the speed of light. The concept embodies the non-intuitive reality that as objects travel faster, time and space behave differently than our everyday experiences would suggest.
The Speed of Light: A Cosmic Speed Limit
The speed of light, commonly denoted by the symbol \( c \), is a fundamental constant of nature that sits at precisely 299,792,458 meters per second. It represents the maximum speed at which all conventional matter and information in the universe can travel. The significance of \( c \) goes far beyond its role as a speed limit; it is a critical component in the fabric of the theory of special relativity.

In our exercise, the train's speed is given as a fraction of the speed of light (\( 0.950c \) ). When objects travel at speeds that are significant fractions of \( c \), relativistic effects like length contraction cannot be ignored. The universality of the speed of light means that no matter how fast an observer is moving relative to a light source, they will always measure the speed of light at \( c \) in a vacuum. This constancy leads to the counterintuitive consequences that special relativity predicts – from length contraction, as experienced by our track side observer, to time dilation, experienced by those moving at relativistic speeds.

Overall, \( c \) serves as a cornerstone for the laws of physics as we understand them and offers a stark contrast to our intuitions based on everyday experiences, which are limited to velocities much smaller than the speed of light.

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Most popular questions from this chapter

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