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Short distance non-perturbative effects of large distance modified gravity
High Energy Physics - Theory · Submitted 26 Aug 2005
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim These effects reduce, by a factor of a few, the predictions for the additional precession of the orbits in the Solar system, still rendering them in an observationally interesting range.
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The abstract, sentence by sentence
In a model of large distance modified gravity we compare the nonperturbative Schwarzschild solution of hep-th/0407049 to approximate solutions obtained previously. In the regions where there is a good qualitative agreement between the two, the nonperturbative solution yields effects that could have observational significance. These effects reduce, by a factor of a few, the predictions for the additional precession of the orbits in the Solar system, still rendering them in an observationally interesting range. The very same effects lead to a mild anomalous scaling of the additional scale-invariant precession rate found by Lue and Starkman.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In a model of large distance modified gravity we compare the nonperturbative Schwarzschild solution of hep-th/0407049 to approximate solutions obtained previously. | contribution 0.87 | 0.77 | 0.06 | asserted 0.95 |
| s1 | In the regions where there is a good qualitative agreement between the two, the nonperturbative solution yields effects that could have observational significance. | result 0.87 | 0.67 | 0.26 | hedged possibility 0.99 |
| s2 | These effects reduce, by a factor of a few, the predictions for the additional precession of the orbits in the Solar system, still rendering them in an observationally interesting range. | result 0.94 | 0.79 | 0.46 | asserted 0.92 |
| s3 | The very same effects lead to a mild anomalous scaling of the additional scale-invariant precession rate found by Lue and Starkman. | result 0.93 | 0.48 | 0.15 | asserted 1.00 |
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Original abstract
In a model of large distance modified gravity we compare the nonperturbative Schwarzschild solution of hep-th/0407049 to approximate solutions obtained previously. In the regions where there is a good qualitative agreement between the two, the nonperturbative solution yields effects that could have observational significance. These effects reduce, by a factor of a few, the predictions for the additional precession of the orbits in the Solar system, still rendering them in an observationally interesting range. The very same effects lead to a mild anomalous scaling of the additional scale-invariant precession rate found by Lue and Starkman.
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3 arXiv papers cite this in 7 sentences
Papers citing it · 6 sentences without a confident label
Uses its data or values 1 paper
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This difference has been calculated [ref] : ϵ_NPSϵ_PS ≃0.59 (rr_*)^0.04 .
Cargese Lectures on Brane Induced Gravity · Role of non-linearities · 0.90
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