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Astrophysical inputs on the SUSY dark matter annihilation detectability

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Francisco Prada (IAA-CSIC), Anatoly Klypin (NMSU), J. Flix (IFAE), M. Martinez (IFAE), E. Simonneau (IAP)

Astrophysics · Submitted 23 Jan 2004

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

The authors' main claim Our models predict that spatially extended annihilation signal should be detected at high confidence levels by incoming experiments assuming that neutralinos make up most of the DM in the Universe and that they annihilate according to current SUSY models.

how it is stated · asserted 0.67 read the record →

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arXiv IDastro-ph/0401512 (version 1)
Pith IDGPLEBL5B, Pith's permanent record of this paper and its review
CitationAnatoly Klypin (NMSU), E. Simonneau (IAP), Francisco Prada (IAA-CSIC), J. Flix (IFAE), M. Martinez (IFAE). "Astrophysical inputs on the SUSY dark matter annihilation detectability." arXiv:astro-ph/0401512 (2004). https://pith.science/paper/GPLEBL5B
Claim paper

The compiled record

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. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,700 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.37 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.10 · compares with prior results 0.11 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

If dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric (SUSY) particles, the centers of galaxies should emit gamma-rays produced by their self-annihilation. We present accurate estimates of continuum gamma-ray fluxes due to neutralino annihilation in the central regions of the Milky Way. We use detailed models of our Galaxy, which satisfy available observational data, and include some important physical processes, which were previously neglected. Our models predict that spatially extended annihilation signal should be detected at high confidence levels by incoming experiments assuming that neutralinos make up most of the DM in the Universe and that they annihilate according to current SUSY models.

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 If dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric (SUSY) particles, the centers of galaxies should emit gamma-rays produced by their self-annihilation. background 1.00 0.04 0.06 hedged possibility 0.58
s1 We present accurate estimates of continuum gamma-ray fluxes due to neutralino annihilation in the central regions of the Milky Way. contribution 0.99 0.95 0.08 asserted 1.00
s2 We use detailed models of our Galaxy, which satisfy available observational data, and include some important physical processes, which were previously neglected. method 0.99 0.84 0.03 asserted 1.00
s3 Our models predict that spatially extended annihilation signal should be detected at high confidence levels by incoming experiments assuming that neutralinos make up most of the DM in the Universe and that they annihilate according to current SUSY models. result 0.80 0.83 0.88 asserted 0.67

What kind of paper the classifier reports this is: simulation study 0.63 · evidence from simulation or computation 0.99.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
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

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

If dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric (SUSY) particles, the centers of galaxies should emit gamma-rays produced by their self-annihilation. We present accurate estimates of continuum gamma-ray fluxes due to neutralino annihilation in the central regions of the Milky Way. We use detailed models of our Galaxy, which satisfy available observational data, and include some important physical processes, which were previously neglected. Our models predict that spatially extended annihilation signal should be detected at high confidence levels by incoming experiments assuming that neutralinos make up most of the DM in the Universe and that they annihilate according to current SUSY models.

Human review

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References
How the literature uses it

22 arXiv papers cite this in 23 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 · 22 sentences without a confident label

Cites it as support 1 paper
  • However, as explained above, baryonic effects could potentially increase the chances for a CTA discovery of higgsino dark matter as baryons can drag dark matter towards the Galactic center during their cooling, leading to a more cuspy profile [ref] .

    Indirect and direct detection prospect for TeV dark matter in the MSSM-9 · Gamma-ray upper limits and prospects · 0.97

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