What Are the Timelike and Null Coordinates Used in the Schwarzschild Metric?

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Discussion Overview

The discussion revolves around the nature of timelike and null coordinates in the context of the Schwarzschild metric, particularly focusing on the Eddington-Finkelstein coordinates and their implications. Participants explore the definitions and properties of these coordinates, as well as the confusion arising from different coordinate systems.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant introduces the Eddington-Finkelstein coordinates and questions how to determine whether a coordinate is timelike, null, or spacelike, seeking explicit calculations for verification.
  • Another participant suggests using the chain rule and vectors represented by partial derivative operators to analyze the coordinates.
  • A later reply discusses the subtlety in the definitions of coordinates, referencing HEL's definition and the conditions under which a coordinate is classified as timelike, null, or spacelike.
  • It is argued that the coordinate p in Eddington-Finkelstein coordinates is actually a timelike coordinate, contrary to claims made in the referenced text, while also noting that it can be null in Kruskal coordinates.
  • One participant expresses confusion regarding the classification of p and the implications of HEL's definitions, questioning the consistency of the definitions across different coordinate systems.
  • There is a mention of a potential mistake in the referenced text regarding the classification of p as a null coordinate, leading to further confusion about the introduction of the advanced Eddington-Finkelstein coordinate.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the classification of the coordinate p, with multiple competing views presented regarding its nature in different coordinate systems. The discussion remains unresolved, with ongoing confusion and requests for further clarification.

Contextual Notes

Participants reference specific pages and equations from texts, indicating that the discussion is heavily dependent on the definitions and interpretations provided in those sources. There are unresolved aspects regarding the implications of Woodhouse's "second fundamental confusion of calculus" and the differing classifications of coordinates in various contexts.

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Now I'm study the Schwarzschild geometry from "General Relativity (M.P. Hobson)".

Since the Schwarzschild metric has coordinate singularity at [tex]r=2M[/tex] so to remove this singularity they use the Eddington-Finkelstein coordinate,

first they begin with introduces new time parameter "p"

[tex]p=ct+r+2M ln\left |\frac{r}{2M}-1 \right |[/tex]
which is

[tex]dp=c dt+\frac{r}{r-2M}dr[/tex]
and they said that it's a null coordinate

after that , they said "since p is a null coordinate, which might be intuitively unfamiliar, it is common practice to work instead with the related timelike coordinate [itex]t^\prime[/itex]defined by"

[tex]ct^{\prime}=p-r=ct+2M ln\left |\frac{r}{2M}-1 \right |[/tex]

and it is a timelike coordinate which called "advanced Eddingtion-Finkelstein coordinate"

My question is how can I check that which coordinate are timelike nulllike or spacelike? Is there any explicit calculation to check this?

What wrong with the former coordinate which defined as p? Why should we use the new one instead?
 
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Are you familiar with vectors represented by partial derivative operators? If you are, then use the chain rule.
 
"vectors represented by partial derivative operators"

like this? [tex]V=V^{\mu}\partial_{\mu}[/tex]

sorry, but I have no idea about what you are said. Could you please tell me more about it?
 
off-diagonal said:
"vectors represented by partial derivative operators"

like this? [tex]V=V^{\mu}\partial_{\mu}[/tex]

Yes!

Unfortunately, there is some subtlety here, and this subtlety seems to have confused Hobson, Efstathiou, and Lasenby (HEL). Most of the subtlety has to do with Woodhouse's "second fundamental confusion of calculus."

By HEL's own definition on page 248,
... fix the other coordinates at their values at P and consider an infinitesimal variation [itex]dx^\mu[/itex] in the coordinate of interest. If the corresponding change in the interval [itex]ds^2[/itex] is positive, zero or negative, then [itex]x^\mu[/itex] is timelike, null or spacelike respectively.

[itex]p[/itex] in Eddington-FinkelStein coordinates [itex]\left(p,r,\theta,\phi \right)[/itex] is a timelike coordinate, not a null coordinate. To see this, apply HEL's prescription on page 248 to equation (11.6). Varing [itex]p[/itex] while holding [itex]r[/itex], [itex]\theta[/itex], and [itex]\phi[/itex] constant gives [itex]dr = d\theta = d\phi = 0[/itex] and

[tex]ds^2 = \left( 1 - \frac{2M}{r} \right) dp^2.[/tex]

Hence, (when [itex]r > 2M[/itex]) [itex]ds^2[/itex] is positive, and [itex]p[/itex] is a timelike coordinate.

HEL are thinking of [itex]p[/itex] in Kruskal coordinates [itex]\left(p,q,\theta,\phi \right).[/itex]. In this case, applying the page 248 prescription to equation (11.16) gives that [itex]p[/itex] is a null coordinate. Do you see why?

What type of coordinate is [itex]r[/itex] in Eddington-FinkelStein coordinates [itex]\left(p,r,\theta,\phi \right)[/itex]?

By now, you should be thoroughly confused! How can the "same" [itex]p[/itex] be timelike in one set of coordinates and null in another set of coordinates? If you want, I am willing to spend some time explaining in detail what is going on here, and what Woodhouse's "second fundamental confusion of calculus" is.
 
So , according to your comment when I apply the prescription in P.248 to the metric in Kruskal Coordinates [tex](p,r,\theta,\phi)[/tex].


[tex]ds^{2}=\left(1-\frac{2M}{r}\right)dp dq-r^{2}d\Omega^{2}_{s^{2}}[/tex]

then as [tex]dq=d\theta=d\phi=0[/tex] so we conclude that [tex]p[/tex] is null coordinate.

Am I right?

If that were the case, then in P.255 they made some mistake because they told that [tex]p[/tex] is null coordinate. In stead, as your suggestion then coordinate [tex]p[/tex] as defined in (11.5) is already timelike coordinate. so What is HEL's propose to introduce new coordinate called "advanced Eddington-Finkelstein"(11.8) which claim to be a timelike coordinate.

I found in Black Hole Physics (Frolov & Novikov) they also said that [tex]v[/tex] is null coordinate,which defined slightly different from HEL but still get the same metric as HEL (11.6). So right now I'm so confused about that

George Jones said:
I am willing to spend some time explaining in detail what is going on here, and what Woodhouse's "second fundamental confusion of calculus" is.

Yes, sure I want to. Thank you so much I appreciated that
 

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