Equivalence principle - light beam through a rocket

In summary, the question is about how an observer inside a rocket, experiencing acceleration and gravity, will see a light beam that is traveling horizontally through the rocket. The answer is that the light beam will appear to bend due to the relativistic effects of the rocket's movement. This is because, from the perspective of the observer inside the rocket, the light will have to travel a longer distance to reach the other side of the rocket due to the rocket's movement. This can be explained using the equation ##\sqrt{c^2t^2 +s^2}>ct##, where ##c## is the speed of light, ##t## is the time it takes for light to travel from one side of the rocket to the
  • #1
Bohr1227
13
0
An observer outside the rocket sees a light beam through a rocket that's accelerating. How will an observer inside the rocket see the light beam? (The problem is showed in the picture below)

physics.png

My friends and I had this problem at school today, and we couldn't decide which is right. Here are our thoughts:

1) The rocket has a speed relative to the observer outside.

2) The person inside will experience a acceleration, which is equivalence to gravity. After reading the books and seen some pictures, I think the right answer is that the light beam will bend.

I hope someone can explain it in details. I don't understand why the observer outside don't see a bend light beam because the rocket has a speed and acceleration.

Thanks for the help!
 
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  • #2
Yes you are right the light beam will bend, the trick is to think of the question relativistically, i.e. light always travels the same speed in any referance frame. Therefore, let's say it takes time t for light to go from one side of the rocket to the other if the rocket was standing still, the light then travels a distance ##ct##. Then if the light went horizontal through the rocket with respect to the rockets floor, if the rocket moves distance ##s## in time ##t##, the light will actually travel a distance ##\sqrt{c^2t^2 +s^2}>ct##. Therefore the light seems to bend for the observer inside the rocket, as if the light enters the rocket at distance ##H## above the floor of the rocket, it needs to exit the other side of the rocket at a distance ##H-s## such that we have ##\sqrt{c^2t^2 +[(H-s)+s]^2}=\sqrt{c^2t^2}=ct##
 

Related to Equivalence principle - light beam through a rocket

1. What is the Equivalence Principle?

The Equivalence Principle is a fundamental principle in physics that states that the gravitational force experienced by an object is equivalent to an acceleration in a non-inertial reference frame. In simpler terms, the effects of gravity can be indistinguishable from an acceleration in the opposite direction.

2. How does the Equivalence Principle apply to a light beam through a rocket?

In the case of a light beam through a rocket, the Equivalence Principle applies because the rocket is accelerating upwards, creating a non-inertial reference frame for the light beam. This means that the light beam will experience the same effects of gravity as if it were in a stationary reference frame on Earth.

3. What is the significance of the Equivalence Principle in understanding gravity?

The Equivalence Principle is significant because it helps us understand that gravity is not a force between two objects, but rather a curvature of spacetime caused by the mass and energy of those objects. This principle is a cornerstone of Einstein's theory of general relativity, which explains gravity as the curvature of spacetime.

4. How does the Equivalence Principle relate to Einstein's theory of general relativity?

Einstein's theory of general relativity is based on the Equivalence Principle, as it shows that gravity is not a force between objects, but rather a result of the curvature of spacetime. This theory has been extensively tested and has been shown to accurately describe the effects of gravity on a large scale.

5. Are there any exceptions to the Equivalence Principle?

While the Equivalence Principle holds true in most cases, there are some exceptions, such as in extreme conditions like near a black hole or in the early stages of the universe. In these cases, the effects of gravity can be significantly different and cannot be described by the Equivalence Principle alone.

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