High Energy Physics - Phenomenology · arXiv:hep-ph/0308218 v2 · submitted 21 Aug 2003
Fermionic partner of Quintessence field as candidate for dark matter
The paper says
“Our results show that, for suitable choices of the model parameters, the Quintessino is a good candidate for cold or warm dark matter.”
from the abstract · picked out as the main claim by a classifier
Reviews
Reviews by people
No person has reviewed this paper on Pith yet. A scientist listed on Pith can review it for a fee, and their review is published here whatever it concludes.
The paper
Abstract
Quintessence is a possible candidate for dark energy. In this paper we study the phenomenologies of the fermionic partner of Quintessence, the Quintessino. Our results show that, for suitable choices of the model parameters, the Quintessino is a good candidate for cold or warm dark matter. In our scenario, dark energy and dark matter of the Universe are connected in one chiral superfield.
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 0.91
What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.29 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.05 · mentions code or data availability 0.02
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| Quintessence is a possible candidate for dark energy. | background 1.00 | 0.05 | 0.02 | hedged possibility 0.98 |
| In this paper we study the phenomenologies of the fermionic partner of Quintessence, the Quintessino. | contribution 1.00 | 0.82 | 0.04 | asserted 0.79 |
| Our results show that, for suitable choices of the model parameters, the Quintessino is a good candidate for cold or warm dark matter. | result 0.96 | 0.94 | 0.89 | asserted 0.91 |
| In our scenario, dark energy and dark matter of the Universe are connected in one chiral superfield. | contribution 0.67 | 0.57 | 0.12 | asserted 1.00 |
What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.58
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
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, 3,501 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 4 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- Supergravity with a Gravitino LSP hep-ph · Apr 2004
- SuperWIMP Solutions to Small Scale Structure Problems hep-ph · Jul 2005
- Particle decays during the cosmic dark ages astro-ph · Oct 2003
- Dark Matter Candidates from Particle Physics and Methods of Detection astro-ph.CO · Mar 2010
How the literature uses it
6 arXiv papers cite this in 8 sentences
Papers citing it · 6 sentences without a confident label
Cites it as support 1 paper
-
However, in our model the DM particles are produced non-thermally, so the high velocity of the DM particles will lower the phase space density of DM and lead to a DM profile with a constant density core [ref] .
Non-Thermal Production of WIMPs, Cosmic $e^\pm$ Excesses and $\gamma$-rays from the Galactic Center · Introduction · 0.97
Challenges and discussion
Know something about this paper? Leave a comment.
Come back by email
A short list of the week's newly reviewed papers. Nothing is sent until you confirm from your inbox, and every email has a link that stops it. No account.
No comments yet.
Sign in to comment