High Energy Physics - Phenomenology · arXiv:hep-ph/0310052 v4 · submitted 3 Oct 2003
Radion Induced Spontaneous Baryogenesis
The paper says
“We show that the radion field can naturally induce spontaneous baryogenesis when the cosmological evolution for the matter on the branes is taken into account.”
from the abstract · picked out as the main claim by a classifier
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The paper
Abstract
We describe a possible scenario for the baryogenesis arising when matter is added on the branes of a Randall-Sundrum model with a radion stabilizing potential. We show that the radion field can naturally induce spontaneous baryogenesis when the cosmological evolution for the matter on the branes is taken into account.
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. No sentence in this record was written by a model.
abstract compiled · 2026-09-23 · no language-model review
How the main claim is stated: asserted 1.00
What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.05 · mentions code or data availability 0.01
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v4). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| We describe a possible scenario for the baryogenesis arising when matter is added on the branes of a Randall-Sundrum model with a radion stabilizing potential. | contribution 0.94 | 0.74 | 0.16 | hedged possibility 0.99 |
| We show that the radion field can naturally induce spontaneous baryogenesis when the cosmological evolution for the matter on the branes is taken into account. | result 0.92 | 0.92 | 0.78 | asserted 1.00 |
What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.84
What was examined, and what was not
Sources read
- arXiv listing abstract v4
Not examined
- full text
- figures and tables
- references and citing sentences
- relations to other papers
Levels run
- P abstract
Not run
- S sections
- T body sentences
- C citations
- R cross-paper relations
How the labels were made
Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,277 input tokens, $0.0001 reported.
Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON
Cited by 3 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- Asymmetric Dark Matter via Spontaneous Co-Genesis hep-ph · Jun 2011
- Cosmological CPT violating effect on CMB polarization astro-ph · Oct 2008
- Searching for CPT Violation with Cosmic Microwave Background Data from WMAP and BOOMERANG astro-ph · Jan 2006
How the literature uses it
7 arXiv papers cite this in 8 sentences
Papers citing it · 3 sentences without a confident label
Cites it as background 5 papers
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The model suggested in [ref] was the subject of several studies on gravitational baryogenesis and leptogenesis in different models of cosmology [ref] .
A Note on Gravitational Baryogenesis · Introduction · 0.83
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This idea is first implemented in the context of “spontaneous baryogenesis” [ref] scenario and has subsequently been elaborated upon in various ways [ref] .
Spontaneous Lorentz Violation and Baryogenesis · Introduction · 0.82
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A candidate for the scalar $ϕ$ can emerge in a variety of contexts: , inflatons [ref] , flat directions [ref] , radions [ref] , quintessence fields [ref] , scalar curvature [ref] , Higgs fields [ref] , However, scalars with an approximate shift symmetry such as pseudo–Nambu Goldstone bosons (pNGB) are particularly well-motivated in this context [ref] .
Deformation of Axion Potentials: Implications for Spontaneous Baryogenesis, Dark Matter, and Isocurvature Perturbations · Introduction · 0.95
Challenges and discussion
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