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AdS in Warped Spacetimes

High Energy Physics - Theory · Submitted 25 May 2000

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

The authors' main claim We obtain a large class of AdS spacetimes warped with certain internal spaces in eleven-dimensional and type IIA/IIB supergravities.

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arXiv IDhep-th/0005246 (version 2)
Pith ID7EZBCUUN, Pith's permanent record of this paper and its review
CitationC.N. Pope, H. Lu, J.F. Vazquez-Poritz, M. Cvetic. "AdS in Warped Spacetimes." arXiv:hep-th/0005246 (2000). https://pith.science/paper/7EZBCUUN
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.09 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.12 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We obtain a large class of AdS spacetimes warped with certain internal spaces in eleven-dimensional and type IIA/IIB supergravities. The warp factors depend only on the internal coordinates. These solutions arise as the near-horizon geometries of more general semi-localised multi-intersections of $p$-branes. We achieve this by noting that any sphere (or AdS spacetime) of dimension greater than 3 can be viewed as a foliation involving S^3 (or AdS_3). Then the S^3 (or AdS_3) can be replaced by a three-dimensional lens space (or a BTZ black hole), which arises naturally from the introduction of a NUT (or a pp-wave) to the M-branes or the D3-brane. We then obtain multi-intersections by performing a Kaluza-Klein reduction or Hopf T-duality transformation on the fibre coordinate of the lens space (or the BTZ black hole). These geometries provide further possible examples of the AdS/CFT correspondence and of consistent embeddings of lower-dimensional gauged supergravities in D=11 or D=10.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We obtain a large class of AdS spacetimes warped with certain internal spaces in eleven-dimensional and type IIA/IIB supergravities. contribution 0.65 0.95 0.70 asserted 1.00
s1 The warp factors depend only on the internal coordinates. result 0.94 0.75 0.06 asserted 1.00
s2 These solutions arise as the near-horizon geometries of more general semi-localised multi-intersections of $p$-branes. result 0.65 0.60 0.20 asserted 1.00
s3 We achieve this by noting that any sphere (or AdS spacetime) of dimension greater than 3 can be viewed as a foliation involving S^3 (or AdS_3). method 0.98 0.48 0.06 asserted 1.00
s4 Then the S^3 (or AdS_3) can be replaced by a three-dimensional lens space (or a BTZ black hole), which arises naturally from the introduction of a NUT (or a pp-wave) to the M-branes or the D3-brane. method 0.91 0.69 0.07 asserted 1.00
s5 We then obtain multi-intersections by performing a Kaluza-Klein reduction or Hopf T-duality transformation on the fibre coordinate of the lens space (or the BTZ black hole). method 0.97 0.90 0.08 asserted 1.00
s6 These geometries provide further possible examples of the AdS/CFT correspondence and of consistent embeddings of lower-dimensional gauged supergravities in D=11 or D=10. interpretation 0.99 0.61 0.40 hedged possibility 0.95

What kind of paper the classifier reports this is: theoretical result 0.98 · evidence from proof or derivation 0.99.

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The paper
Original abstract

We obtain a large class of AdS spacetimes warped with certain internal spaces in eleven-dimensional and type IIA/IIB supergravities. The warp factors depend only on the internal coordinates. These solutions arise as the near-horizon geometries of more general semi-localised multi-intersections of $p$-branes. We achieve this by noting that any sphere (or AdS spacetime) of dimension greater than 3 can be viewed as a foliation involving S^3 (or AdS_3). Then the S^3 (or AdS_3) can be replaced by a three-dimensional lens space (or a BTZ black hole), which arises naturally from the introduction of a NUT (or a pp-wave) to the M-branes or the D3-brane. We then obtain multi-intersections by performing a Kaluza-Klein reduction or Hopf T-duality transformation on the fibre coordinate of the lens space (or the BTZ black hole). These geometries provide further possible examples of the AdS/CFT correspondence and of consistent embeddings of lower-dimensional gauged supergravities in D=11 or D=10.

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References
How the literature uses it

30 arXiv papers cite this in 50 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 · 32 sentences without a confident label

Builds on it 3 papers
  • These backgrounds are obtained as near horizon geometries of 1/8-BPS brane intersections consisting on D1-F1-D3 defect branes introduced in the D5-NS5-D7 background branes realising the AdS$_6×S^2×Σ_2$ solution to Type IIB supergravity constructed in [ref] in its near-horizon.

    AdS$_2$ near-horizons, defects and string dualities · Introduction · 0.89

  • Our analysis extends[And corrects, as explained in section [ref].] the results in [ref] , where AdS$_3$ solutions dual to surface defect CFTs embedded in the 6d $(1,0)$ CFT dual to the AdS$_7$ solution to massless Type IIA supergravity [ref] were constructed, allowing now for $F_0≠0$.

    New AdS$_3$/CFT$_2$ pairs in massive IIA with $(0,4)$ and $(4,4)$ supersymmetries · Conclusions · 0.91

  • The metric form D2D6:metric:Eq is a straightforward generalization of the case of a static D2-D6 brane system with a dilaton coupling [ref] .

    Cosmological brane systems in warped spacetime · AdS$_4$ spacetime in the D2-D6 brane system · 0.93

Uses its method or tool 1 paper
  • With this choice of $Q_3$, one precisely obtains $k=Q_5$ via T-duality.] [ref] [equation] and cast it into the new parametrization [ref] [equation] In these new coordinates the D3-KK background [ref] can be rewritten as [ref] [equation] The $S^5/ℤ_k$ metric is precisely the same obtained with T-duality, given in [ref], with $k=Q_KK$.

    Defects in 4d SCFTs from supergravity and holographic renormalization · The Type IIB picture · 0.80

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Cites it as background 11 papers

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