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Massive holographic QFTs in de Sitter
by Jos\'e Manuel Pen\'in, Kostas Skenderis, Benjamin Withers
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Submission summary
Authors (as Contributors):  Kostas Skenderis · Benjamin Withers 
Submission information  

Preprint link:  scipost_202201_00011v1 
Date submitted:  20220113 12:01 
Submitted by:  Withers, Benjamin 
Submitted to:  SciPost Physics 
Ontological classification  

Academic field:  Physics 
Specialties: 

Approach:  Theoretical 
Abstract
We study strongly coupled massdeformedCFT on a fixed de Sitter spacetime in three dimensions via holography. We elucidate the global causal structure of the fourdimensional spacetime dual to the de Sitter invariant vacuum state. The conformal boundaries of de Sitter appear as spacelike defects sourced by the mass deformation, which extend into the bulk as curvature singularities in AdS. We compute all one and twopoint functions of the deformedCFT stress tensor and a scalar operator orderbyorder in the mass deformation for a simple holographic model. These correlation functions admit a spectral representation as a sum of simple poles corresponding to normalisable modes in the bulk.
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Reports on this Submission
Anonymous Report 2 on 2022321 (Invited Report)
 Cite as: Anonymous, Report on arXiv:scipost_202201_00011v1, delivered 20220321, doi: 10.21468/SciPost.Report.4733
Strengths
1 Clear Presentation of Analytic Computations.
2 Well defined problem and results on the correlation functions.
Report
The authors discuss the strongly coupled holographic computation of the QFT correlation functions on de Sitter spacetime. To capture nontrivial de Sitter effects in their computation, a mass deformation is introduced to the CFT to break the conformal symmetry. In this way an extra scale m is introduced to represent the mass on top of the de Sitter Hubble constant that already exist in the undeformed theory. All the results of the authors are expected to be dependent on the ratio m/H, which can be used as the parameter for perturbative expansions.
The authors present the holographic background by solving perturbatively the gravity equation resulting from a gravity action coupled to a scalar with a mass term. Similar derivations/results already exist in the literature which the authors cite. The initial solution is found perturbatively in coordinates that the boundary covers the de Sitter inflationary patch. The global structure of the spacetime is also presented perturbatively with respect to the mass deformation parameter.
Then the onepoint function is obtained on the holographic background. For low values of m/H, it is in agreement with the results of the literature, e.g. ref. [27]. At large values of m/H the asymptotic behavior of the one point function is derived, up to a constant that is determined numerically. The authors proceed to compute the scalar, vector, tensor, two point functions by using the standard holographic methods. That is by solving the equations of motion for the linearised fluctuations on the domain wall background they are working on. The form of the correlators is not fixed in their theories since the conformal symmetry is broken. The perturbative result of the two point function is obtained, this is one of the main results of the paper. The m=0 limit reproduces the CFT results as it should. Then the authors discuss a massive free fermion theory on se Sitter and compare with their holographic results.
The computations of the paper are presented analytically and in a clear way. The problem that the manuscript discusses is well posed and defined and it is answered clearly following the standard methods of holography.
I have some minor suggestions and comments. The authors find that the correlation functions admit a spectral representation as a sum of certain poles corresponding to the normalisable modes of the bulk spacetime. They discuss (the absence of) the interpretation of these modes as quasinormal modes in their computation, mentioning briefly the literature. This discussion can be improved/extended. The thermal behavior of de Sitter is associated with the cosmological horizon seen by the observer. Its characteristic temperature is proportional to the de Sitter radius and the cosmological horizon is observer dependent (unlike the black holes thermal properties). Moreover, the domain walls are de Sitter invariant. Are all these facts essential/enough for the conclusions of the authors in the relevant discussion in section 7, regarding the mentioned unrelatedness to the quasinormal modes. I would suggest a slight extension of the relevant discussion in section 7, and a further elaboration on the interpretation of these results in comparison to the results of zero momenta e.g. ref [27].
The authors could also mention the reasons they have chosen to work in threedimensional model and if there are obstructions of extending their computation in higher dimensions where cosmological observations are relevant. As an extra minor remark, I find the title of the manuscript to be broader than its contents.
In summary the paper is well written. The question that the manuscript studies is well defined and it is answered clearly. I would suggest a minor revision of the manuscript.
Requested changes
1 Comments on the correlation function representation as a sum of poles, the normalisable modes of the bulk spacetime and the quasinormal modes(see report).
Anonymous Report 1 on 202233 (Invited Report)
 Cite as: Anonymous, Report on arXiv:scipost_202201_00011v1, delivered 20220303, doi: 10.21468/SciPost.Report.4610
Strengths
1 Clear and explicit exposition.
2 Discusses QFT on de Sitter at strong coupling.
3 Finds interesting results for the correlation function.
Weaknesses
Very minor (see report)
Report
Using a nice set of coordinates, this paper elucidates the global structure of the geometry sourced by a scalar of dual dimension $\Delta=2$ as first reported on in 1707.01030.
Afterwards, one and twopoint functions of scalars and tensor modes in this backgrounds are computed in order to extract strong coupling correlation functions of the stress tensor and dual operator of the scalar for the QFT on dS$_3$, as a function of the mass deformation.
The authors note that the resummation of the orderbyorder result can be understood as a shift in the spectral poles of the twopoint function, without any additional structure being introduced. The authors also compare these results to a massive fermionic QFT on dS$_3$.
I find these results intriguing and this paper easily meets the criterion of publication in Scipost Physics.
The only request I have is that the authors comment on the strong coupling interpretation of the order by order resummation in $m$ of their twopoint function result giving a sum of shifted poles. In the introduction, the authors make clear that they are aware of the IR issues that arise in perturbative calculation of correlation functions on dS at weak coupling. However, they do not touch on this in the resummation section. It would naively seem to me that the shifted poles, particularly if they lie at real values of $\nu$ imply that the strong coupling result is consistent with these field theories being stable.
Requested changes
Comments on the perturbative IR instability in dS in the resummation section.