The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
First Results from ABRACADABRA-10 cm: A Search for Sub- μeV Axion Dark Matter
Open accessAbstract
The axion is a promising dark matter candidate, which was originally proposed to solve the strong-$CP$ problem in particle physics. To date, the available parameter space for axion and axionlike particle dark matter is relatively unexplored, particularly at masses ${m}_{a}\ensuremath{\lesssim}1\text{ }\text{ }\ensuremath{\mu}\mathrm{eV}$. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, ${10}^{\ensuremath{-}12}\ensuremath{\lesssim}{m}_{a}\ensuremath{\lesssim}{10}^{\ensuremath{-}6}\text{ }\text{ }\mathrm{eV}$. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between ${g}_{a\ensuremath{\gamma}\ensuremath{\gamma}}<1.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}10}$ and ${g}_{a\ensuremath{\gamma}\ensuremath{\gamma}}<3.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}9}\text{ }\text{ }{\mathrm{GeV}}^{\ensuremath{-}1}$ over the mass range $3.1\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}10}--8.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}9}\text{ }\text{ }\mathrm{eV}$. These results are competitive with the most stringent astrophysical constraints in this mass range.
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
The Design and Implementation of FFTW3
Frigo, M., & Johnson, S. G. (2005) · Proceedings of the IEEE · doi:10.1109/jproc.2004.840301 · Cited by 5,086
Discovering the QCD axion with black holes and gravitational waves
Arvanitaki, A., Baryakhtar, M., & Huang, X. (2015) · Physical Review D · doi:10.1103/physrevd.91.084011 · Cited by 543
Dimensionless constants, cosmology, and other dark matters
Tegmark, M., Aguirre, A., Rees, M. J., & Wilczek, F. (2006) · Physical Review D · doi:10.1103/physrevd.73.023505 · Cited by 401
Cited by
The landscape of QCD axion models
Di Luzio, L., Giannotti, M., Nardi, E., & Visinelli, L. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.06.002 · Cited by 657
Di Valentino, E., Said, J. L., Riess, A., Pollo, A., Poulin, V., Gómez-Valent, A., Weltman, A., Palmese, A., Huang, C. D., Bruck, C. V. D., et al. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101965 · Cited by 319
Metadata
- Authors
- Ouellet, J. L., Salemi, C. P., Foster, J. W., Henning, R., Bogorad, Z., Conrad, J. M., Formaggio, J. A., Kahn, Y., Minervini, J., Radovinsky, A., Rodd, N. L., Safdi, B. R., Thaler, J., Winklehner, D., & Winslow, L.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2019-03-29
- Volume
- 122
- Issue
- 12
- Pages
- 121802-121802
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2898353231
- Cited by
- 274
- References
- 3
- FWCI
- 21.80
- Type
- journal article
- Language
- en
- Open access
- hybrid
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: First Results from ABRACADABRA-10 cm: A Search for Sub- μeV Axion Dark Matter. https://app.cochat.ai/papers/10.1103/physrevlett.122.121802
- The paper
- Ouellet, J. L., Salemi, C. P., Foster, J. W., Henning, R., Bogorad, Z., Conrad, J. M., Formaggio, J. A., Kahn, Y., Minervini, J., Radovinsky, A., Rodd, N. L., Safdi, B. R., Thaler, J., Winklehner, D., & Winslow, L. (2019). First Results from ABRACADABRA-10 cm: A Search for Sub- μeV Axion Dark Matter. Physical Review Letters. https://doi.org/10.1103/physrevlett.122.121802
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.