Black Holes in String Theory - calculation help needed

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Discussion Overview

The discussion revolves around the derivation of equations related to black holes in string theory, specifically from the paper by Callan, Myers, and Perry. Participants are exploring the application of covariant derivatives and the appearance of first derivatives in certain equations, as well as clarifying the implications of using different notations for scalar fields.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • Chris expresses confusion about deriving equations (2.5) and (2.6) from (2.1) and (2.4), particularly regarding the absence of first derivatives of the scalar field φ.
  • Chris questions the presence of φ' terms in the (tt) and (θθ) equations, suggesting that only the (rr) equation should contain a φ-term based on his understanding of the covariant derivative.
  • Chris argues that since ∇φ is first-order in λ, then (∇φ)² should be second-order in λ and thus irrelevant for equation (2.6).
  • Another participant notes a distinction between φ' and ϕ′, acknowledging the confusion but still questioning the appearance of ϕ′ in equations (2.5).
  • A participant points out that the equality ∇ₐ∇ₑφ = ∂ₐ∂ₑϕ(r) is incorrect in curved spacetime, indicating that additional terms related to connection coefficients must be considered.
  • Chris acknowledges the oversight regarding the covariant derivative and expresses gratitude for the clarification provided by another participant.
  • Chris confirms the need to use the d'Alembertian operator in the context of the equations being discussed.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the initial confusion regarding the appearance of first derivatives in the equations. However, there is agreement on the necessity of considering connection coefficients in curved spacetime when dealing with covariant derivatives.

Contextual Notes

The discussion highlights limitations in understanding the application of covariant derivatives in curved spacetime and the potential for confusion arising from notation differences. The participants' varying levels of experience with the material also contribute to the complexity of the discussion.

ilp89
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I have a question about the paper:

C. G. . Callan, R. C. Myers and M. J. Perry, “Black Holes In String Theory,” Nucl. Phys. B
311, 673 (1989).

I have attached the relevant section.

I am having trouble using equations (2.1) and (2.4) to derive (2.5) and (2.6). When I do the calculation, I do not get any [itex]\phi'[/itex] terms (i.e. first derivatives --- I do get all the second-derivatives of phi and all other terms).

For example, I don't understand how the (tt) and (θθ) equations can have [itex]\phi'[/itex] terms. Doesn't (2.1a) contain
[itex]\nabla_{a}\nabla_{b}\phi = \partial_a \partial_b \varphi(r) = 0[/itex] unless [itex]a = b = r[/itex]?
Thus shouldn't only the (rr) equation contain a [itex]\phi[/itex]-term... and shouldn't it just be a second derivative?

For another example, since [itex]\nabla \phi[/itex] is first-order in [itex]\lambda[/itex], isn't [itex](\nabla \phi)^2[/itex] second-order in [itex]\lambda[/itex] and thus irrelevant for equation (2.6)? This would lead me to conclude that there should be no first derivative of [itex]\phi[/itex] in (2.6). Where does it come from?

I would greatly appreciate some insight. Tell me where I am going wrong!

Thanks in advance,
Chris
 

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Maybe I should clarify my question, in order not to scare people away. What I am asking should not take too much time for someone familiar with general relativity.

I am only asking that you look at equation (2.1a), mentally insert (2.4) into it, and let me know how a phi-prime appeared in all three equations (2.5).

I am very grateful to anyone who tries to help.

Thanks!
Chris
 
Does anyone have any ideas?

I might need to reproduce this calculation in front of my professor tomorrow evening, so I will be extremely grateful for any help soon.

Chris
 
I have no idea how to understand these equations and have very little experience but from a computer programming perspective I can usually look through foreign "code" and get a general idea.

From the excerpt provided I looked at figure (2.5) and looked very closely at lines (tt) and (θθ) I don't see the phi-prime symbol ϕ′ but I do see φ' several times.

Sorry if this is no help at all, I'm trying to learn these things coming from a different perspective.
 
You are right - I have accidentally been using [itex]\phi'[/itex] and [itex]\varphi'[/itex] interchangeably, since they differ only by a multiplicative factor. You can see this from equation (2.4) since [itex]\phi_0[/itex] is an arbitrary constant.

But I still don't understand why [itex]\varphi'[/itex] should appear anywhere in any equation of (2.5).

I can rephrase the question as:

Using (2.4), what is [itex]\nabla_a \nabla_b \phi[/itex] ?

It seems like a very easy question to me, but my answer to that questions seems to be in contradiction with what is in (2.5).

Please keep asking questions so we can figure this out together.

Thank you,
Chris
 
ilp89 said:
[itex]\nabla_{a}\nabla_{b}\phi = \partial_a \partial_b \varphi(r)[/itex]

This equality is not correct in curved spacetime, and it looks like the text is using curved spacetime (i.e., gravity is present). In curved spacetime there are extra terms in the covariant derivative [itex]\nabla_a[/itex] involving the connection coefficients.
 
PeterDonis -

Thank you very much! You figured it out. Indeed [itex]\nabla_a \phi = \partial_a \phi[/itex] since [itex]\phi[/itex] is a scalar field, but the second covariant derivative must incorporate the connection coefficients and the [itex]\partial_a \phi[/itex]'s. I feel silly for overlooking this - my mind was stuck for very long.

Anyway, thanks again for the help. I am very grateful.

Chris
 
Just to check:

I also need to use [itex]\square \phi = g^{ab} \nabla_a \nabla_b \phi[/itex] - correct?
 
Yes, it is. Alright - everything works out perfectly now.

Thanks again.
 

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