Cited by 83Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity Theories

The fate of the radion in models with metastable graviton

Open access
Pilo, Luigi, Rattazzi, Riccardo, Zaffaroni, Alberto·2000·Journal of High Energy Physics

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1088/1126-6708/2000/07/056

Cites

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • The self-accelerating branch suffers from a negative energy ghost instability.

    “However, as discussed in the introduction, SA branch suffers from a negative energy ghost instability.”

    From Out of the White Hole: A Holographic Origin for the Big Bang (2014) · cites this paper as [8]

    The Introduction and §3 describe a negative-kinetic-term radion and an associated negative-energy instability in the GRS model. They do not identify a self-accelerating (SA) branch or establish that this branch has the instability; that condition is unsupported by this source. (LLM, conf=0.84)

    Experimental — accuracy not yet measured
  • Self-accelerating DGP solutions suffer from ghosts and tachyons as well as some pathological singularities.

    “However, it turned out that SA solutions suffer from ghosts and tachyons [8][9][10][11] as well as some pathological singularities [12].”

    From Out of the White Hole: A Holographic Origin for the Big Bang (2014) · cites this paper as [8]

    The Introduction and section 3 discuss a ghost radion and negative-energy effects in the GRS model, not self-accelerating DGP solutions. Searches for self-acceleration, DGP, tachyons, and pathological singularities found no passage addressing the attributed claim. (LLM, conf=0.78)

    Experimental — accuracy not yet measured

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

No references could be resolved yet.

Research works printed but not linked: 18

  1. M. Gogberashvili, hep-th/9812296. · arXiv
  2. R. Gregory, V. A. Rubakov and S. M. Sibiryakov, hep-th/0002072. · arXiv
  3. I. Kogan, S. Mouslopoulus, A. Papazoglou, G. Ross and J. Santiago, hep- ph/9912552; I. Kogan and G. Ross, hep-th/0003074. · arXiv
  4. E. Witten, hep-ph/0002297. · arXiv
  5. G. Dvali, G. Gabadadze and M. Porrati, hep-th/0002190. · arXiv
  6. C. Csaki, J. Erlich and T. J. Hollowood, hep-th/0002161. · arXiv
  7. C. Csaki, J. Erlich and T. J. Hollowood, hep-th/0003020. · arXiv
  8. R. Gregory, V. A. Rubakov and S. M. Sibiryakov, hep-th/0003045. · arXiv
  9. G. Dvali, G. Gabadadze and M. Porrati, hep-th/0002190, hep-th/0003054. · arXiv
  10. C. Csaki, J. Erlich, T. J. Hollowood and J. Terning, hep-th/0003076. · arXiv
  11. G. Kang and Y.S. Myung, hep-th/0003162. · arXiv
  12. Phys. Rev. Lett. 83 (1999) 4922, hep-ph/9907447. · arXiv
  13. C. Csaki, M. Graesser, L. Randall, J. Terning, hep-ph/9911406. · arXiv
  14. W. D. Goldberger, M. B. Wise, hep-ph/9911457. · arXiv
  15. J. Garriga and T. Tanaka, hep-th/9911055. · arXiv
  16. S. B. Giddings, E. Katz and L. Randall, hep-th/0002091. · arXiv
  17. C. Charmousis, R. Gregory and V. A. Rubakov, hep-th/9912160. · arXiv
  18. T. Tanaka and X. Montes, hep-th/0001092. · arXiv

Cited by

Sorted by citations

Authors
Pilo, L., Rattazzi, R., & Zaffaroni, A.
Venue
Journal of High Energy Physics
Published
2000-07-31
Volume
2000
Issue
07
Pages
056-056
ISSN
1029-8479 (ISSN-L)
OpenAlex
W1995396476
Cited by
83
References
0
Citations by year
2026: 1 · 2025: 1 · 2023: 1 · 2022: 3 · 2019: 1 · 2018: 1 · 2017: 1 · 2016: 2 · 2014: 1 · 2012: 2
FWCI
7.73
Type
journal article
Language
en
Open access
Locations
  • Journal of High Energy Physics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila (submittedVersion)
  • BOA (University of Milano-Bicocca) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion)
  • Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion, cc-by-nc-nd)
  • arXiv (Cornell University)
Funders
European Commission (ERBFMRX-CT96-0045, ERBFMRX-CT96-0090)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
Keywords
radion, negative tension branes, negative energy, negative kinetic term, braneworld gravity

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review