The DOI matches its Crossref record; 44 of the 44 references it cites were found in a registry or an index.
Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments
Open accessAbstract
As direct dark matter experiments continue to increase in size, they will become sensitive to neutrinos from astrophysical sources. For experiments that do not have directional sensitivity, coherent neutrino scattering from several sources represents an important background to understand, as it can almost perfectly mimic an authentic weakly interacting massive particle (WIMP) signal. Here we explore in detail the effect of neutrino backgrounds on the discovery potential of WIMPs over the entire mass range of 500 MeV to 10 TeV. We show that, given the theoretical and measured uncertainties on the neutrino backgrounds, direct detection experiments lose sensitivity to light ($\ensuremath{\sim}10\text{ }\text{ }\mathrm{GeV}$) and heavy ($\ensuremath{\sim}100\text{ }\text{ }\mathrm{GeV}$) WIMPs with a spin-independent cross section below ${10}^{\ensuremath{-}45}$ and ${\text{10}}^{\ensuremath{-}49}\text{ }\text{ }{\mathrm{cm}}^{2}$, respectively.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Particle dark matter: evidence, candidates and constraints
Bertone, G., Hooper, D., & Silk, J. (2005) · Physics Reports · doi:10.1016/j.physrep.2004.08.031 · Cited by 4,979
Jungman, G., Kamionkowski, M., & Griest, K. (1996) · Physics Reports · doi:10.1016/0370-1573(95)00058-5 · Cited by 4,172
Asymptotic formulae for likelihood-based tests of new physics
Cowan, G., Cranmer, K., Gross, E., & Vitells, O. (2011) · The European Physical Journal C · doi:10.1140/epjc/s10052-011-1554-0 · Cited by 3,199
Ahmad, Q. R., Allen, R. C., Andersen, T. C., D.Anglin, J., Barton, J. C., Beier, E. W., Bercovitch, M., Bigu, J., Biller, S. D., Black, R. A., et al. (2002) · Physical Review Letters · doi:10.1103/physrevlett.89.011301 · Cited by 2,990
Dark Matter Results from 225 Live Days of XENON100 Data
Aprile, E., Alfonsi, M., Arisaka, K., Arneodo, F., Balan, C., Baudis, L., Bauermeister, B., Behrens, A., Beltrame, P., Bokeloh, K., et al. (2012) · Physical Review Letters · doi:10.1103/physrevlett.109.181301 · Cited by 1,394
Lewin, J. D., & Smith, P. F. (1996) · Astroparticle Physics · doi:10.1016/s0927-6505(96)00047-3 · Cited by 1,350
The universal rotation curve of spiral galaxies — I. The dark matter connection
Persic, M., Salucci, P., & Stel, F. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/278.1.27 · Cited by 1,238
Cowan, G. (1998) · doi:10.1093/oso/9780198501565.001.0001 · Cited by 844
Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., d’Angelo, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, X. H., et al. (2010) · The European Physical Journal C · doi:10.1140/epjc/s10052-010-1303-9 · Cited by 817
Dark Matter Search Results from the CDMS II Experiment
The CDMS II Collaboration (2010) · Science · doi:10.1126/science.1186112 · Cited by 813
Cited by
DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS
Aalseth, C. E., Acerbi, F., Agnes, P., Albuquerque, I. F. M., Alexander, T., Alici, A., Alton, A. K., Antonioli, P., Arcelli, S., Ardito, R., et al. (2018) · The European Physical Journal Plus · doi:10.1140/epjp/i2018-11973-4 · Cited by 616
Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.161301 · Cited by 386
Supernova Neutrinos: Production, Oscillations and Detection
Mirizzi, A., Tamborra, I., Janka, H., Saviano, N., Scholberg, K., Bollig, R., Hüdepohl, L., & Chakraborty, S. (2015) · arXiv (Cornell University) · doi:10.15161/oar.it/1446204340.05 · Cited by 366
A Universe Built on Shadows: Evidence, Candidates, and Detection Strategies for Dark Matter
Felizardo, M. (2026) · Particles · doi:10.3390/particles9040095
Metadata
- Authors
- Billard, J., Figueroa-Feliciano, E., & Strigari, L.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2014-01-27
- Volume
- 89
- Issue
- 2
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W2132803409
- Cited by
- 719
- References
- 44
- FWCI
- 28.89
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments. https://app.cochat.ai/papers/10.1103/physrevd.89.023524
- The paper
- Billard, J., Figueroa-Feliciano, E., & Strigari, L. (2014). Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments. Physical Review D. https://doi.org/10.1103/physrevd.89.023524
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.