Deriving Schwarz Metric Weak Limit: Carroll's Lecture Notes 1997

In summary, Carroll argues that the weak limit can be recovered as r approaches infinity, using the equation 7.27 which takes the form ##ds^{2}=-(1+\frac{\mu}{r})dt^{2}+(1+\frac{\mu}{r})^{-1}dr^{2}+r^{2}d\Omega^{2}##. He then equates the coefficient of ##g_{00}##, which is equal to -(1+2\phi), to the limit given by ##g_{00}(r\to\infty)=-(1+\frac{\mu}{r})##. However, he explains that this is not accurate enough and that the expansion should also consider ##g_{11}
  • #1
binbagsss
1,305
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I'm looking at Carroll's lecture notes 1997, intro to GR.

Equation 7.27 which is that he's argued the S metric up to the form ##ds^{2}=-(1+\frac{\mu}{r})dt^{2}+(1+\frac{\mu}{r})^{-1}dr^{2}+r^{2}d\Omega^{2}##

And argues that we expect to recover the weak limit as ##r \to \infty##.
So he then has ##g_{00}(r\to\infty)=-(1+\frac{\mu}{r}) ## [1]
where ##g_{00}=-(1+2\phi)## and equates these.

The reasoning is fine to me, but I don't understand the limit given by [1], surely as ##r\to\infty## ##g_{00} \to -1##

Thanks in advance.
 
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  • #2
You are looking for a power series in 1/r. The coefficient of [itex] g_{00} [/itex] needs no expansion. It is already a power series in 1/r. So correct to first order, this factor does not change. However, [itex] g_{11} [/itex] can be expanded in terms of 1/r by the binomial expansion. He then truncates this so that it is accurate to first order.

If you neglect 1/r in [itex] g_{00} [/itex], you have a zeroth order approximation, which is too severe.
 

FAQ: Deriving Schwarz Metric Weak Limit: Carroll's Lecture Notes 1997

What is the significance of deriving the Schwarz metric weak limit?

The Schwarz metric weak limit is important because it allows us to understand the behavior of certain types of metrics in curved spaces. This can be useful in various areas of physics, including general relativity and cosmology.

Can you explain the concept of a weak limit?

A weak limit is a mathematical concept that describes the behavior of a sequence of functions. It is a type of limit that is more general than the usual limit, as it allows for more flexibility in how the functions approach their limit.

How does Carroll's lecture notes from 1997 contribute to the understanding of the Schwarz metric weak limit?

Carroll's lecture notes provide a clear and concise explanation of how to derive the Schwarz metric weak limit. They also offer insights and examples that can help deepen the understanding of this concept.

Are there any specific prerequisites for understanding the derivation of the Schwarz metric weak limit?

Yes, a solid understanding of calculus and basic concepts in differential geometry is necessary to comprehend the derivation of the Schwarz metric weak limit. Familiarity with general relativity and curved spaces is also helpful.

How is the Schwarz metric weak limit used in practical applications?

The Schwarz metric weak limit is used in various fields of physics, such as in understanding the behavior of black holes and gravitational waves. It also has applications in the study of cosmology and the large-scale structure of the universe.

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