Energy Approximation for Small Velocity - Schutz's "A First Course in GR

In summary, the Schutz book explains that for small v, the energy can be approximated as E = m + (1/2)mv2 through a Taylor expansion of the left hand side.
  • #1
mess1n
24
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In the Schutz book, "A First Course in General Relativity" (bottom of p.42 if you have it), it states the following:

For small v, the energy is:

E = po = m(1-v2)-(1/2) =(approx) m + (1/2)mv2

I can't figure out why this is! For small v, the LHS will tend to m, and the RHS will tend to m, so it's a valid relation. But how did they derive the RHS from the LHS?

Any help would be appreciated. Let me know if you need some more info.

Cheers,
Andrew
 
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  • #2
mess1n said:
In the Schutz book, "A First Course in General Relativity" (bottom of p.42 if you have it), it states the following:

For small v, the energy is:

E = po = m(1-v2)-(1/2) =(approx) m + (1/2)mv2

I can't figure out why this is! For small v, the LHS will tend to m, and the RHS will tend to m, so it's a valid relation. But how did they derive the RHS from the LHS?

Any help would be appreciated. Let me know if you need some more info.

Cheers,
Andrew

The right hand side is the Taylor expansion about v=0 of the left hand side. They stop the Taylor expansion at the second term because v is so small that third order and higher terms will be negligible.
 

1. What is the concept of energy approximation for small velocity in general relativity?

The concept of energy approximation for small velocity in general relativity refers to the method of approximating the total energy of a system in a region of space where the velocity of the objects involved is small compared to the speed of light. This approximation allows for a simplified calculation of the energy and momentum of the system, making it easier to analyze and understand the behavior of objects in this low-velocity region.

2. How does Schutz's "A First Course in GR" explain energy approximation for small velocity?

Schutz's "A First Course in GR" explains energy approximation for small velocity by using the concept of the energy-momentum tensor, which describes the energy and momentum of a system in terms of the curvature of spacetime. The book also introduces the concept of the weak field limit, which allows for a linear approximation of the Einstein field equations in low-velocity regions.

3. What is the significance of energy approximation for small velocity in general relativity?

The significance of energy approximation for small velocity in general relativity lies in its ability to simplify complex calculations and make them more manageable. This allows for a better understanding of the behavior of objects in low-velocity regions, such as the solar system, where the effects of gravity can be accurately described using this approximation.

4. Can energy approximation for small velocity be applied to all systems in general relativity?

No, energy approximation for small velocity is only applicable to systems in regions of low-velocity. In regions of high-velocity, such as near black holes, the effects of gravity are much stronger and cannot be accurately described using this approximation. In these cases, more complex calculations and methods are needed to accurately describe the system.

5. Are there any limitations to using energy approximation for small velocity in general relativity?

Yes, energy approximation for small velocity has its limitations. It can only be applied to systems with low velocities, and it does not take into account the effects of strong gravitational fields. In addition, this approximation may not be accurate for systems with significant energy exchange, such as those involving nuclear reactions. Therefore, it is important to use caution and understand the limitations when applying this approximation in general relativity.

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