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

Click For Summary
SUMMARY

The discussion centers on deriving the Schwarz metric weak limit as presented in Sean Carroll's 1997 lecture notes on General Relativity (GR). The equation in focus is Equation 7.27, which describes the Schwarzschild metric in the form ##ds^{2}=-(1+\frac{\mu}{r})dt^{2}+(1+\frac{\mu}{r})^{-1}dr^{2}+r^{2}d\Omega^{2}##. The key point of contention is the limit of ##g_{00}## as ##r \to \infty##, where it is argued that ##g_{00}## approaches -1, contradicting the expectation that it retains a power series form. The discussion emphasizes the importance of correctly interpreting the coefficients in the metric and the necessity of not neglecting terms in the expansion.

PREREQUISITES
  • Understanding of General Relativity concepts, specifically the Schwarzschild metric.
  • Familiarity with tensor notation and metric components in GR.
  • Knowledge of power series expansions and binomial expansion techniques.
  • Ability to interpret limits and asymptotic behavior in mathematical expressions.
NEXT STEPS
  • Study the derivation of the Schwarzschild metric in detail, focusing on the implications of the weak limit.
  • Learn about the significance of the metric components ##g_{00}## and ##g_{11}## in the context of GR.
  • Explore power series expansions in the context of physics, particularly in gravitational theories.
  • Review the binomial expansion and its applications in approximating functions in GR.
USEFUL FOR

This discussion is beneficial for physicists, students of General Relativity, and researchers interested in the mathematical foundations of gravitational theories, particularly those focusing on metric derivations and asymptotic analysis.

binbagsss
Messages
1,291
Reaction score
12
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.
 
Physics news on Phys.org
You are looking for a power series in 1/r. The coefficient of g_{00} needs no expansion. It is already a power series in 1/r. So correct to first order, this factor does not change. However, g_{11} 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 g_{00}, you have a zeroth order approximation, which is too severe.
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
1K
  • · Replies 24 ·
Replies
24
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
Replies
9
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 53 ·
2
Replies
53
Views
4K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 32 ·
2
Replies
32
Views
4K
  • · Replies 43 ·
2
Replies
43
Views
5K