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Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

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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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D. S. Akerib (Co-chair, Case Western Reserve University), E. Aprile (Co-chair, Columbia University), E. A. Baltz (Kavli Institute for Particle Astrophysics, Cosmology, SLAC), M. R. Dragowsky (Case Western Reserve University)
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R. J. Gaitskell (Brown University), P. Gondolo (University of Utah), A. Hime (Los Alamos National Laboratory), C. J. Martoff (Temple University), D.-M. Mei (Los Alamos National Laboratory), H. Nelson (University of California, Santa Barbara), B. Sadoulet (University of California, Berkeley), R. W. Schnee (Case Western Reserve University), A. H. Sonnenschein (Fermi National Accelerator Laboratory), L. E. Strigari (University of California, Irvine)

Astrophysics · Submitted 30 May 2006

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

The authors' main claim A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S.

how it is stated · asserted 0.96 read the record →

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arXiv IDastro-ph/0605719 (version 3)
Pith IDROHEOXKI, Pith's permanent record of this paper and its review
CitationA. Hime (Los Alamos National Laboratory), A. H. Sonnenschein (Fermi National Accelerator Laboratory), Berkeley), B. Sadoulet (University of California, Case Western Reserve University), C. J. Martoff (Temple University), Columbia University), Cosmology, D.-M. Mei (Los Alamos National Laboratory), D. S. Akerib (Co-chair, E. A. Baltz (Kavli Institute for Particle Astrophysics, E. Aprile (Co-chair, H. Nelson (University of California, Irvine), L. E. Strigari (University of California, M. R. Dragowsky (Case Western Reserve University), P. Gondolo (University of Utah), R. J. Gaitskell (Brown University), R. W. Schnee (Case Western Reserve University), Santa Barbara), SLAC). "Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group." arXiv:astro-ph/0605719 (2006). https://pith.science/paper/ROHEOXKI
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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,547 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.07 · human participants 0.05 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.05 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. The table of contents follows: 1. Overview 2. WIMP Dark Matter: Cosmology, Astrophysics, and Particle Physics 3. Direct Detection of WIMPs 4. Indirect Detection of WIMPs 5. Dark Matter Candidates and New Physics in the Laboratory 6. Synergies with Other Sub-Fields 7. Direct Detection Experiments: Status and Future Prospects 8. Infrastructure 9. International Context 10. Summary and Outlook 11. Acknowledgments

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 A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. contribution 0.86 0.59 0.10 asserted 0.96
s1 The table of contents follows: 1. Overview 2. background 0.74 0.16 0.02 unclear 0.55
s2 WIMP Dark Matter: Cosmology, Astrophysics, and Particle Physics 3. background 0.86 0.05 0.02 unclear 0.99
s3 Direct Detection of WIMPs 4. background 0.77 0.04 0.02 unclear 0.99
s4 Indirect Detection of WIMPs 5. background 0.73 0.04 0.02 unclear 0.99
s5 Dark Matter Candidates and New Physics in the Laboratory 6. background 0.76 0.05 0.02 unclear 0.99
s6 Synergies with Other Sub-Fields 7. background 0.66 0.05 0.02 unclear 0.99
s7 Direct Detection Experiments: Status and Future Prospects 8. Infrastructure 9. background 0.72 0.06 0.02 unclear 0.98
s8 International Context 10. Summary and Outlook 11. Acknowledgments future work 0.56 0.05 0.06 unclear 0.99

What kind of paper the classifier reports this is: review 0.88 · evidence from literature 0.97.

What was examined, and what was not

sources read
  • arXiv listing abstract v3
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

A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. The table of contents follows: 1. Overview 2. WIMP Dark Matter: Cosmology, Astrophysics, and Particle Physics 3. Direct Detection of WIMPs 4. Indirect Detection of WIMPs 5. Dark Matter Candidates and New Physics in the Laboratory 6. Synergies with Other Sub-Fields 7. Direct Detection Experiments: Status and Future Prospects 8. Infrastructure 9. International Context 10. Summary and Outlook 11. Acknowledgments

Human review

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References
How the literature uses it

4 arXiv papers cite this in 6 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

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