Cosmological constant in the semiclassical limit of quantum gravity

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Discussion Overview

The discussion revolves around the cosmological constant in the context of the semiclassical limit of quantum gravity, specifically within the framework of the Einstein-Hilbert action. Participants explore the implications of a small cosmological constant in Planck units and its relationship to the length scale ##\ell## and the gravitational constant ##G##. The conversation includes mathematical reasoning and conceptual clarifications related to anti-de Sitter (AdS) spacetime.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • Some participants question why the cosmological constant is small in Planck units and what this implies for the relationship between ##\ell## and ##G##.
  • One participant states that the smallness of the cosmological constant is an open area of research, indicating uncertainty in the field.
  • Another participant presents a series of inequalities involving ##\Lambda##, ##M_P##, and ##G_N##, seeking clarification on their validity.
  • A participant challenges the use of a negative sign in the expression ##\Lambda = -1/\ell^2##, prompting a discussion about the implications of sign in inequalities.
  • Some participants assert that the derivation discussed is only valid for AdS spacetime and inquire about references supporting the claim that ##\ell \gg G## in this context.
  • Concerns are raised regarding the units of ##G## and ##\ell##, suggesting that the correct formulation should involve their magnitudes rather than signs.
  • One participant emphasizes that the negative sign of ##\Lambda## does not affect the requirement for the semiclassical approximation, as the magnitude remains small compared to the Planck mass.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of the inequalities involving the cosmological constant and the implications of the negative sign. There is no consensus on the validity of the derivations or the correct formulation of the relationships discussed.

Contextual Notes

Participants note limitations regarding the assumptions made in the derivations and the dependence on the specific context of AdS spacetime. The discussion highlights the need for careful consideration of units and signs in the mathematical expressions.

Afonso Campos
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Why is it the case that, in a semiclassical description of the Einstein-Hilbert action, the cosmological constant is small in Planck units?

Why does this mean that

$$\ell \gg G$$

for ##\Lambda = - 1/\ell^{2}##?
 
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Afonso Campos said:
Why is it the case that, in a semiclassical description of the Einstein-Hilbert action, the cosmological constant is small in Planck units?

Nobody knows. This is an open area of research.
 
PeterDonis said:
Nobody knows. This is an open area of research.

Ah! Right!

For the second part, we have, in Planck units,

##\Lambda \ll M_{P}^{4}##

##-1/\ell^{2} \ll M_{P}^{4}##

##-1/\ell^{2} \ll 1/G^{2}_{N}##

##1/\ell^{2} \gg 1/G^{2}_{N}##

##G^{2}_{N} \gg \ell^{2}##

##\ell^{2} \ll G^{2}_{N}##

##\ell \ll G_{N}##

What have I done wrong here?
 
Afonso Campos said:
What have I done wrong here?

Why did you have ##\Lambda = - 1 / \ell^2## with a minus sign?
 
Let's say that we have ##AdS## spacetime.
 
Afonso Campos said:
Let's say that we have ##AdS## spacetime.

Then your derivation is only valid for ##AdS## spacetime. Do you have a reference that claims that ##\ell \gg G## for ##AdS## spacetime?
 
PeterDonis said:
Then your derivation is only valid for ##AdS## spacetime. Do you have a reference that claims that ##\ell \gg G## for ##AdS## spacetime?

It is in page 2 of this paper - https://arxiv.org/pdf/hep-th/9712251.pdf.

See equation (2.2) and the text above the equation.
 
Afonso Campos said:
See equation (2.2) and the text above the equation.

Hm. I think their statement that ##\ell \gg G## is only meant as a heuristic, because the two don't even have the same units; the units of ##G## are length squared (inverse mass squared), while the units of ##\ell## are, of course, length. So really it should be ##\ell^2 \gg G##.

Regarding your derivation, you should not be including the minus sign regardless of the sign of ##\Lambda##, since the inequality only refers to relative magnitudes, not signs. In other words, the strictly correct way of writing the above inequality (with units corrected) is ##\vert \ell \vert^2 \gg \vert G \vert##. Or, if you write it in terms of ##\Lambda## and ##M_P##, it is ##\vert \Lambda \vert \ll \vert M_P \vert^2##. (Note the exponent, btw; it's the Planck mass squared, since the units of ##\Lambda## are mass squared, or inverse length squared.) The fact that the sign of ##\Lambda## is negative in ##AdS## doesn't change any of the above--its magnitude is still small compared to the magnitude of ##M_P##, which is the necessary requirement for the semiclassical approximation.
 
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PeterDonis said:
Hm. I think their statement that ##\ell \gg G## is only meant as a heuristic, because the two don't even have the same units; the units of ##G## are length squared (inverse mass squared), while the units of ##\ell## are, of course, length. So really it should be ##\ell^2 \gg G##.

I find that the reviews of important results in section 2 and section 3 of the paper could have better written.

PeterDonis said:
Regarding your derivation, you should not be including the minus sign regardless of the sign of ##\Lambda##, since the inequality only refers to relative magnitudes, not signs. In other words, the strictly correct way of writing the above inequality (with units corrected) is ##\vert \ell \vert^2 \gg \vert G \vert##. Or, if you write it in terms of ##\Lambda## and ##M_P##, it is ##\vert \Lambda \vert \ll \vert M_P \vert^2##. (Note the exponent, btw; it's the Planck mass squared, since the units of ##\Lambda## are mass squared, or inverse length squared.) The fact that the sign of ##\Lambda## is negative in ##AdS## doesn't change any of the above--its magnitude is still small compared to the magnitude of ##M_P##, which is the necessary requirement for the semiclassical approximation.

Thanks for pointing this out!
 

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