On holography for (pseudo-)conformal cosmology

M. Libanov; S. Sibiryakov; V. Rubakov

RECORD

On holography for (pseudo-)conformal cosmology

M. Libanov, V. Rubakov, S. Sibiryakov

High Energy Physics - Theory · Submitted 15 Sep 2014

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We propose a holographic dual for (pseudo-)conformal cosmological scenario, with a scalar field that forms a moving domain wall in adS_5.

how it is stated · asserted 0.76 read the record →

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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,861 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.10 · states limitation 0.11 · human participants 0.01 · controlled comparison 0.11 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.92 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; show every role.

We propose a holographic dual for (pseudo-)conformal cosmological scenario, with a scalar field that forms a moving domain wall in adS_5. The domain wall separates two vacua with unequal energy densities. Unlike in the existing construction, the 5d solution is regular in the relevant space-time domain.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	We propose a holographic dual for (pseudo-)conformal cosmological scenario, with a scalar field that forms a moving domain wall in adS_5.	contribution 1.00	0.90	0.50	asserted 0.76
s1	The domain wall separates two vacua with unequal energy densities.	contribution 0.50	0.56	0.08	asserted 1.00
s2	Unlike in the existing construction, the 5d solution is regular in the relevant space-time domain.	result 0.85	0.77	0.25	asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.97 · evidence from proof or derivation 0.87.

What was examined, and what was not

sources read

arXiv listing abstract v2

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

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S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

We propose a holographic dual for (pseudo-)conformal cosmological scenario, with a scalar field that forms a moving domain wall in adS_5. The domain wall separates two vacua with unequal energy densities. Unlike in the existing construction, the 5d solution is regular in the relevant space-time domain.

Human review

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How the literature uses it

6 arXiv papers cite this in 12 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 8 sentences without a confident label

Builds on it 1 paper

One of our main purposes is to see what happens in a model with a single brane, that generalizes the model of Ref. [ref] in the sense that it includes effects of the 5d gravity.

Perturbations on and off de Sitter brane in anti-de Sitter bulk · Introduction · 0.95

Compares with it 1 paper

So, our model is essentially the same as in Ref. [ref] .

Conformal Universe as false vacuum decay · Holographic model · 0.89

What it cites

Uses the method or tool of 1 paper

For $v < -1$, we change the variable, $v = - coshρ$ (cf. Ref. [ref] ) and write eq.

Holography for a Non-Inflationary Early Universe · Introduction · 0.91

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