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High Energy Physics - Phenomenology · arXiv:hep-ph/9701205 v1 · submitted 2 Jan 1997

Cold Dark Matter in SUSY Theories. The Role of Nuclear Form Factors and the Folding with the LSP Velocity

T.S. Kosmas, J.D. Vergados

The paper says

“For the coherent cross sections it is shown that, since the momentum transfer can be quite big for large mass of the LSP and heavy nuclei even though the energy transfer is small (≤ 100KeV), the total cross section can in such instances be reduced by a factor of about five.”

from the abstract · picked out as the main claim by a classifier

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The paper

Abstract

The momentum transfer dependence of the total cross section for elastic scattering of cold dark matter candidates, i.e. lightest supersymmetric particle (LSP), with nuclei is examined. The presented calculations of the event rates refer to a number of representative nuclear targets throughout the periodic table and have been obtained in a relatively wide phenomenologically allowed SUSY parameter space. For the coherent cross sections it is shown that, since the momentum transfer can be quite big for large mass of the LSP and heavy nuclei even though the energy transfer is small (≤ 100KeV), the total cross section can in such instances be reduced by a factor of about five. For the spin induced cross section of odd-A nuclear targets, as is the case of 207Pb studied in this work, we found that the reduction is less pronounced, since the high multipoles tend to enhance the cross section as the momentum transfer increases (for LSP mass < 200GeV) and partially cancell the momentum retardation. The effect of the Earth's revolution around the sun on these event rates is also studied by folding with a Maxwellian LSP-velocity distribution which is consistent with its density in the halos. We thus found that the convoluted event rates do not appreciably change compared to those obtained with an average velocity. The event rates increase with A and, in the SUSY parameter space considered, they can reach values up to 140 y−1Kg−1 for Pb. The modulation effect, however, was found to be small (less than $\pm 5%$).

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

How the main claim is stated: asserted 0.98

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.50 · human participants 0.01 · controlled comparison 0.36 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.68 · 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.

SentenceRoleThe authors' own workStates the main conclusionStrength
The momentum transfer dependence of the total cross section for elastic scattering of cold dark matter candidates, i.e. lightest supersymmetric particle (LSP), with nuclei is examined. contribution 0.87 0.67 0.04 asserted 0.74
The presented calculations of the event rates refer to a number of representative nuclear targets throughout the periodic table and have been obtained in a relatively wide phenomenologically allowed SUSY parameter space. method 0.65 0.93 0.04 asserted 1.00
For the coherent cross sections it is shown that, since the momentum transfer can be quite big for large mass of the LSP and heavy nuclei even though the energy transfer is small ($\le 100 KeV$), the total cross section can in such instances be reduced by a factor of about five. result 1.00 0.90 0.27 asserted 0.98
For the spin induced cross section of odd-A nuclear targets, as is the case of $^{207}Pb$ studied in this work, we found that the reduction is less pronounced, since the high multipoles tend to enhance the cross section as the momentum transfer increases (for LSP $mass < 200 GeV$) and partially cancell the momentum retardation. result 0.98 0.96 0.12 asserted 1.00
The effect of the Earth's revolution around the sun on these event rates is also studied by folding with a Maxwellian LSP-velocity distribution which is consistent with its density in the halos. method 0.77 0.91 0.04 asserted 0.96
We thus found that the convoluted event rates do not appreciably change compared to those obtained with an average velocity. result 1.00 0.96 0.16 asserted 1.00
The event rates increase with A and, in the SUSY parameter space considered, they can reach values up to 140 $y^{-1}Kg^{-1}$ for Pb. result 1.00 0.92 0.20 asserted 0.94
The modulation effect, however, was found to be small (less than $\pm 5%$). result 1.00 0.96 0.13 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.60 · evidence from simulation or computation 0.99

What was examined, and what was not

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  • S sections
  • T body sentences
  • C citations
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How the labels were made

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,557 input tokens, $0.0003 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
How the literature uses it

6 arXiv papers cite this in 12 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 · 9 sentences without a confident label

Uses its method or tool 1 paper
Cites it as background 2 papers
  • 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

  • In most cases, it is the lightest neutralino which is a linear combination of the four neutral fermions $B̃$, $W̃_̃3̃$, $H̃_̃1̃$, and $H̃_̃2̃$, with $B̃$ and $W̃_̃3̃$ being the supersymmetric (SUSY) partners of the $U(1)$ gauge field $B$ and the third component of the SU(2) gauge field $W_3$, while $H̃_̃1̃$ and $H̃_̃2̃$ are the SUSY partners of the light and heavy Higgs scalars [ref] .

    Elastic and inelastic scattering of neutrinos and weakly interacting massive particles on nuclei · Introduction · 0.86

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