Axion Dark Matter eXperiment: Run 1A analysis details
Abstract
The ADMX collaboration gathered data for its Run 1A axion dark matter search from January to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at DFSZ sensitivity. The resulting axion search found no axion-like signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.
- Authors:
- more »
- Publication Date:
- Research Org.:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Pacific Northwest National Laboratory (PNNL), Richland, WA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Laboratory Directed Research and Development (LDRD) Program
- Contributing Org.:
- ADMX Collaboration
- OSTI Identifier:
- 2282919
- Alternate Identifier(s):
- OSTI ID: 2283706; OSTI ID: 2283953
- Report Number(s):
- FERMILAB-PUB-23-0834-AD-PPD; arXiv:2312.16668; PNNL-SA-185330
Journal ID: ISSN 2470-0010; PRVDAQ; 012009
- Grant/Contract Number:
- SC0009800; DESC0009723; SC0010296; SC0010280; SC0011665; DEFG02-97ER41029; DEFG02-96ER40956; DEAC52-07NA27344; DEC03-76SF00098; SC0017987; SC0022148; AC02-07CH11359; LLNL-JRNL-848336; SC0009723; FG02-97ER41029; FG02-96ER40956; AC52-07NA27344; AC03-76SF00098; AC05-76RL01830
- Resource Type:
- Published Article
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Name: Physical Review. D. Journal Volume: 109 Journal Issue: 1; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTRONOMY AND ASTROPHYSICS; 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
Citation Formats
Boutan, C., LaRoque, B. H., Lentz, E., Oblath, N. S., Taubman, M. S., Tedeschi, J., Yang, J., Jones, A. M., Braine, T., Crisosto, N., Rosenberg, L. J., Rybka, G., Will, D., Zhang, D., Kimes, S., Ottens, R., Bartram, C., Bowring, D., Cervantes, R., Chou, A. S., Knirck, S., Mitchell, D. V., Sonnenschein, A., Wester, W., Khatiwada, R., Carosi, G., Du, N., Durham, S., O’Kelley, S. R., Woollett, N., Duffy, L. D., Bradley, R., Clarke, J., Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Buckley, J. H., Gaikwad, C., Henriksen, E. A., Hoffman, J., Murch, K. W., Harrington, P. M., Daw, E. J., Perry, M. G., Hilton, G. C., and ADMX Collaboration. Axion Dark Matter eXperiment: Run 1A analysis details. United States: N. p., 2024.
Web. doi:10.1103/PhysRevD.109.012009.
Boutan, C., LaRoque, B. H., Lentz, E., Oblath, N. S., Taubman, M. S., Tedeschi, J., Yang, J., Jones, A. M., Braine, T., Crisosto, N., Rosenberg, L. J., Rybka, G., Will, D., Zhang, D., Kimes, S., Ottens, R., Bartram, C., Bowring, D., Cervantes, R., Chou, A. S., Knirck, S., Mitchell, D. V., Sonnenschein, A., Wester, W., Khatiwada, R., Carosi, G., Du, N., Durham, S., O’Kelley, S. R., Woollett, N., Duffy, L. D., Bradley, R., Clarke, J., Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Buckley, J. H., Gaikwad, C., Henriksen, E. A., Hoffman, J., Murch, K. W., Harrington, P. M., Daw, E. J., Perry, M. G., Hilton, G. C., & ADMX Collaboration. Axion Dark Matter eXperiment: Run 1A analysis details. United States. https://doi.org/10.1103/PhysRevD.109.012009
Boutan, C., LaRoque, B. H., Lentz, E., Oblath, N. S., Taubman, M. S., Tedeschi, J., Yang, J., Jones, A. M., Braine, T., Crisosto, N., Rosenberg, L. J., Rybka, G., Will, D., Zhang, D., Kimes, S., Ottens, R., Bartram, C., Bowring, D., Cervantes, R., Chou, A. S., Knirck, S., Mitchell, D. V., Sonnenschein, A., Wester, W., Khatiwada, R., Carosi, G., Du, N., Durham, S., O’Kelley, S. R., Woollett, N., Duffy, L. D., Bradley, R., Clarke, J., Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Buckley, J. H., Gaikwad, C., Henriksen, E. A., Hoffman, J., Murch, K. W., Harrington, P. M., Daw, E. J., Perry, M. G., Hilton, G. C., and ADMX Collaboration. Fri .
"Axion Dark Matter eXperiment: Run 1A analysis details". United States. https://doi.org/10.1103/PhysRevD.109.012009.
@article{osti_2282919,
title = {Axion Dark Matter eXperiment: Run 1A analysis details},
author = {Boutan, C. and LaRoque, B. H. and Lentz, E. and Oblath, N. S. and Taubman, M. S. and Tedeschi, J. and Yang, J. and Jones, A. M. and Braine, T. and Crisosto, N. and Rosenberg, L. J. and Rybka, G. and Will, D. and Zhang, D. and Kimes, S. and Ottens, R. and Bartram, C. and Bowring, D. and Cervantes, R. and Chou, A. S. and Knirck, S. and Mitchell, D. V. and Sonnenschein, A. and Wester, W. and Khatiwada, R. and Carosi, G. and Du, N. and Durham, S. and O’Kelley, S. R. and Woollett, N. and Duffy, L. D. and Bradley, R. and Clarke, J. and Siddiqi, I. and Agrawal, A. and Dixit, A. V. and Gleason, J. R. and Hipp, A. T. and Jois, S. and Sikivie, P. and Sullivan, N. S. and Tanner, D. B. and Buckley, J. H. and Gaikwad, C. and Henriksen, E. A. and Hoffman, J. and Murch, K. W. and Harrington, P. M. and Daw, E. J. and Perry, M. G. and Hilton, G. C. and ADMX Collaboration},
abstractNote = {The ADMX collaboration gathered data for its Run 1A axion dark matter search from January to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 μeV in axion mass) at DFSZ sensitivity. The resulting axion search found no axion-like signals comprising all the dark matter in the form of a virialized galactic halo over the entire frequency range, implying lower bound exclusion limits at or below DFSZ coupling at the 90% confidence level. This paper presents expanded details of the axion search analysis of Run 1A, including review of relevant experimental systems, data-taking operations, preparation and interpretation of raw data, axion search methodology, candidate handling, and final axion limits.},
doi = {10.1103/PhysRevD.109.012009},
journal = {Physical Review. D.},
number = 1,
volume = 109,
place = {United States},
year = {Fri Jan 26 00:00:00 EST 2024},
month = {Fri Jan 26 00:00:00 EST 2024}
}
https://doi.org/10.1103/PhysRevD.109.012009
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