High Energy Physics - Phenomenology · arXiv:hep-ph/9702290 v1 · submitted 7 Feb 1997
Spin-Dependent Neutralino-Nucleus Scattering for A ∼ 127 Nuclei
The paper says
“We find good agreement with the observed magnetic moment as well as other obervables for the four nuclei considered: ^127I, ^129,131Xe, and ^125Te.”
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The paper
Abstract
We perform nuclear shell model calculations of the neutralino-nucleus cross section for several nuclei in the A = 127 region. Each of the four nuclei considered is a primary target in a direct dark matter detection experiment. The calculations are valid for all relevant values of the momentum transfer. Our calculations are performed in the 3s2d1g7/21h11/2 model space using extremely large bases, allowing us to include all relevant correlations. We also study the dependence of the nuclear response upon the assumed nuclear Hamiltonian and find it to be small. We find good agreement with the observed magnetic moment as well as other obervables for the four nuclei considered: ^127I, ^129,131Xe, and ^125Te.
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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 0.15 · human participants 0.02 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.09 · compares with prior results 0.47 · mentions code or data availability 0.02
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v1). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| We perform nuclear shell model calculations of the neutralino-nucleus cross section for several nuclei in the A = 127 region. | contribution 0.94 | 0.97 | 0.09 | asserted 1.00 |
| Each of the four nuclei considered is a primary target in a direct dark matter detection experiment. | background 0.79 | 0.18 | 0.05 | asserted 1.00 |
| The calculations are valid for all relevant values of the momentum transfer. | result 0.50 | 0.60 | 0.07 | asserted 1.00 |
| Our calculations are performed in the $3s 2d 1g_{7/2} 1h_{11/2}$ model space using extremely large bases, allowing us to include all relevant correlations. | method 1.00 | 0.95 | 0.05 | asserted 1.00 |
| We also study the dependence of the nuclear response upon the assumed nuclear Hamiltonian and find it to be small. | result 0.94 | 0.97 | 0.13 | asserted 1.00 |
| We find good agreement with the observed magnetic moment as well as other obervables for the four nuclei considered: ^{127}I, ^{129,131}Xe, and ^{125}Te. | result 0.99 | 0.95 | 0.27 | asserted 1.00 |
What kind of paper the classifier reports this is: simulation study 0.85 · evidence from simulation or computation 1.00
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
How the labels were made
Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,929 input tokens, $0.0002 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 22 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- Dark matter in the solar system I: The distribution function of WIMPs at the Earth from solar capture astro-ph.HE · Feb 2009
- Direct Detection of Dark Matter with MadDM v.2.0 hep-ph · May 2015
- New Limits on Dark Matter from Super-Kamiokande hep-ph · Apr 2011
- Magnetic Inelastic Dark Matter hep-ph · Jul 2010
- Compatibility of DAMA/LIBRA dark matter detection with other searches astro-ph · Aug 2008
- Dark matter direct detection rate in a generic model with micrOMEGAs2.2 hep-ph · Mar 2008
- Elastic Scattering and Direct Detection of Kaluza-Klein Dark Matter hep-ph · Sep 2002
- A new dark matter direct search based on archaeological Pb physics.ins-det · Jan 2025
- Spin-Dependent Weakly-Interacting-Massive-Particle--Nucleon Cross Section Limits from First Data of PandaX-II Experiment hep-ex · Nov 2016
- On the Effect of Nuclear Response Functions in Dark Matter Direct Detection hep-ph · Jan 2014
- Model Independent Direct Detection Analyses hep-ph · Nov 2012
- Direct Detection of Leptophilic Dark Matter in a Model with Radiative Neutrino Masses hep-ph · Jan 2012
- The New DAMA Dark-Matter Window and Energetic-Neutrino Searches hep-ph · Aug 2008
- Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors astro-ph.HE · Jun 2026
- Directional detection of dark matter in universal bound states hep-ph · May 2015
- WIMP physics with ensembles of direct-detection experiments astro-ph.CO · Oct 2013
- Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data astro-ph.CO · Jan 2013
- Direct dark matter detection: the next decade astro-ph.IM · Nov 2012
- Appendiciario -- A hands-on manual on the theory of direct Dark Matter detection hep-ph · Apr 2021
- TASI lectures on dark matter models and direct detection hep-ph · Apr 2019
- Dark matter direct-detection experiments physics.ins-det · Sep 2015
- Nuclear spin structure in dark matter search: The zero momentum transfer limit hep-ph · Jun 2004
How the literature uses it
30 arXiv papers cite this in 48 sentences
Papers citing it · 23 sentences without a confident label
Uses its method or tool 2 papers
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This issue was explored by Ref. [ref] , who developed a parametrisation for the spin structure functions in terms of the parameter $u = (qb)^2/2$, where [equation] is the oscillator size parameter [ref] .
Probing WIMP particle physics and astrophysics with direct detection and neutrino telescope data · Direct detection · 0.84
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Calculations of the expectation values $⟨S_p, S_n⟩$ and of the structure functions $S(p)$ are based on the shell-model with various nucleon-nucleon potentials and truncation schemes of the valence space used in the computation [ref] .
Direct dark matter detection: the next decade · Input from particle and nuclear physics · 0.83
Uses its data or values 13 papers
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The function $F_11$ for is taken from Ref. [ref] , for $^73$Ge is obtained from the function $S_11$ of Ref. [ref] , for from the function $S_11$ of Ref. [ref] (set calculated with the Bonn A potential).
On the formalism and upper limits for spin-dependent cross sections in dark matter elastic scattering with nuclei · Structure functions and “form factors” · 0.98
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For $^19$F we use the spin matrix elements of Ref. [ref] that give $Ω^19_p =1.646$ and $Ω^19_n = -0.030$; for $^73$Ge the results of Ref. [ref] , $Ω^73_p =0.066$ and $Ω^73_n = 0.836$; finally for $^127$I the set obtained with the potential Bonn-A from Ref. [ref] that furnishes $Ω^127_p =0.731$ and $Ω^127_n =0.177$.
A scheme for the extraction of WIMP-nucleon scattering cross sections from total event rates · An analytical scheme for extracting the elementary cross sections · 1.00
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We take the structure functions for Aluminum from Ref. [ref] ; for Sodium, Iodine, and Xenon from Ref. [ref] ; and for Silicon and Germanium from Ref. [ref] .
Compatibility of DAMA/LIBRA dark matter detection with other searches · Cross-Section · 0.99
Cites it as background 2 papers
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The list of the models includes the Odd Group Model (OGM) of Engel and Vogel [ref] and their extended OGM (EOGM) [ref] ; Interacting Boson Fermion Model (IBFM) of Iachello, Krauss, and Maino [ref] ; Theory of Finite Fermi Systems (TFFS) of Nikolaev and Klapdor-Kleingrothaus [ref] ; Quasi Tamm-Dancoff Approximation (QTDA) of Engel [ref] ; different shell model treatments (SM) by Pacheco and Strottman [ref] ; by Engel, Pittel, Ormand and Vogel [ref] and Engel, Ressell, Towner and Ormand, [ref] , by Ressell et al. [ref] and Ressell and Dean [ref] ; by Kosmas, Vergados et al. [ref] ; the so-called “hybrid” model of Dimitrov, Engel and Pittel [ref] and perturbation theory based on calculations of Engel et al. [ref] .
Direct Search for Dark Matter - Striking the Balance - and the Future · Event rate and cross sections · 0.90
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A standard reference with a clear explanation of the spin form factors can be found in Ref. [ref] .
TASI lectures on dark matter models and direct detection · Nuclear recoils from DM scattering · 0.88
Challenges and discussion
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