Bends in Space-Time vs Invariance

In summary, this conversation discusses the behavior of a beam of light as it travels from a massive body, such as a neutron star, to an observer located at the source of the beam. The question posed is whether the speed of light, when traveling along a geodesic path in curved space-time, varies or remains constant. The thread referenced provides further discussion on the topic.
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WCOLtd
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Imagine a beam of light being turned on at the surface of a massive body such as a neutron star, the beam of light travels along a geodesic path towards a mirror located at radius r from the planet's surface, when the light beam hits the mirror, the light bounces back to the observer located at the source of the original beam.

My question is does the speed of light (c), when traveling along a geodesic from a massive body to an observer vary according to bends in space-time? (as if light has traveled a greater distance according to the curvature of space-time) or does light travel at the speed of light (c) in a geodesic no matter what the curvature of space-time is?

In the example, would the observer's observations for the time the light beam to reach his eyes be the same as if it were located at the distance (r) in flat space-time?
 
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According to Einstein's theory of general relativity, the curvature of space-time is caused by the presence of massive objects. This means that the path of the light beam will be affected by the curvature of space-time as it travels towards the mirror. However, the speed of light (c) is considered to be a constant in all frames of reference, meaning that it will travel at the same speed regardless of the curvature of space-time.

In other words, the light beam will still travel at the speed of light (c) along the geodesic path towards the mirror, even though the path may be curved due to the presence of the massive body. This is because the speed of light is not affected by the curvature of space-time, but rather it is the path that is affected.

Therefore, the observer's observations for the time it takes for the light beam to reach their eyes will be the same as if they were located at the distance (r) in flat space-time. This is because the light beam will still travel at the same speed, and the observer will perceive the same amount of time passing, regardless of the curvature of space-time.
 

What is a bend in space-time?

A bend in space-time refers to the curvature or deformation of the fabric of space and time caused by massive objects such as planets, stars, and galaxies. This curvature is what creates the force of gravity and allows objects to move in a curved path.

How does a bend in space-time affect the concept of invariance?

Invariance is the idea that the laws of physics remain the same regardless of the observer's perspective or frame of reference. A bend in space-time can affect this concept because the curvature of space-time can cause measurements of time and space to vary for different observers, leading to different interpretations of physical laws.

Can we observe or measure bends in space-time?

Yes, we can observe and measure bends in space-time through various methods, such as gravitational lensing, which is the bending of light rays by massive objects, and the detection of gravitational waves, which are ripples in the fabric of space-time caused by the movement of massive objects.

How does the theory of relativity explain bends in space-time?

The theory of relativity, specifically general relativity, explains bends in space-time as the result of the interaction between matter and energy. According to this theory, massive objects create a curvature in space-time, and this curvature determines the paths of objects moving through space.

Are there any practical applications of understanding bends in space-time?

Yes, understanding bends in space-time has practical applications in various fields, such as astronomy, physics, and engineering. For example, the precise measurement of gravitational lensing can help us study the distribution of dark matter in the universe, and the detection of gravitational waves can provide insights into the behavior of black holes and other massive objects.

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