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Title: Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX

Abstract

We report the first result of a direct search for a Cosmic axion Background (CaB) – a relativistic background of axions that is not dark matter – performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX). Conventional haloscope analyses search for a signal with a narrow bandwidth, as predicted for dark matter, whereas the CaB will be broad. We introduce a novel analysis strategy, which searches for a CaB induced daily modulation in the power measured by the haloscope. Using this, we repurpose data collected to search for dark matter to set a limit on the axion photon coupling of the CaB originating from dark matter decay in the 800–995 MHz frequency range. We find that the present sensitivity is limited by fluctuations in the cavity readout as the instrument scans across dark matter masses. Nevertheless, we demonstrate that these challenges can be surmounted with the use of superconducting qubits as single photon counters, and allow ADMX to operate as a telescope searching for axions emerging from the decay of dark matter. The daily modulation analysis technique we introduce can be deployed for various broadband RF signals, such as other forms of a CaB or even high-frequency gravitationalmore » waves.« less

Authors:
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Publication Date:
Research Org.:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Pacific Northwest National Laboratory (PNNL), Richland, WA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (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:
1999309
Alternate Identifier(s):
OSTI ID: 1969688; OSTI ID: 2305518
Report Number(s):
FERMILAB-PUB-23-109-PPD-SQMS; arXiv:2303.06282; LLNL-JRNL-845987; PNNL-SA-185846
Journal ID: ISSN 0031-9007; PRLTAO; 101002
Grant/Contract Number:  
SC0009800; DESC0009723; SC0010296; SC0010280; SC0011665; DEFG02-97ER41029; DEFG02-96ER40956; DEC03-76SF00098; SC0017987; AC02-07CH11359; AC05-76RL01830; SC0009723; FG02-97ER41029; FG02-96ER40956; C03-76SF00098; AC52-07NA27344
Resource Type:
Published Article
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Name: Physical Review Letters Journal Volume: 131 Journal Issue: 10; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; dark matter; particle dark matter; axions; dark matter detectors; microwave techniques

Citation Formats

Nitta, T., Braine, T., Du, N., Guzzetti, M., Hanretty, C., Leum, G., Rosenberg, L. J., Rybka, G., Sinnis, J., Clarke, John, Siddiqi, I., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Gleason, J. R., Hipp, A. T., Sikivie, P., Sullivan, N. S., Tanner, D. B., Khatiwada, R., Carosi, G., Robertson, N., Duffy, L. D., Boutan, C., Lentz, E., Oblath, N. S., Taubman, M. S., Yang, J., Daw, E. J., Perry, M. G., Bartram, C., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Goryachev, M., Hartman, E., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E., Dror, J. A., Murayama, H., Rodd, N. L., and ADMX Collaboration. Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX. United States: N. p., 2023. Web. doi:10.1103/PhysRevLett.131.101002.
Nitta, T., Braine, T., Du, N., Guzzetti, M., Hanretty, C., Leum, G., Rosenberg, L. J., Rybka, G., Sinnis, J., Clarke, John, Siddiqi, I., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Gleason, J. R., Hipp, A. T., Sikivie, P., Sullivan, N. S., Tanner, D. B., Khatiwada, R., Carosi, G., Robertson, N., Duffy, L. D., Boutan, C., Lentz, E., Oblath, N. S., Taubman, M. S., Yang, J., Daw, E. J., Perry, M. G., Bartram, C., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Goryachev, M., Hartman, E., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E., Dror, J. A., Murayama, H., Rodd, N. L., & ADMX Collaboration. Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX. United States. https://doi.org/10.1103/PhysRevLett.131.101002
Nitta, T., Braine, T., Du, N., Guzzetti, M., Hanretty, C., Leum, G., Rosenberg, L. J., Rybka, G., Sinnis, J., Clarke, John, Siddiqi, I., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Gleason, J. R., Hipp, A. T., Sikivie, P., Sullivan, N. S., Tanner, D. B., Khatiwada, R., Carosi, G., Robertson, N., Duffy, L. D., Boutan, C., Lentz, E., Oblath, N. S., Taubman, M. S., Yang, J., Daw, E. J., Perry, M. G., Bartram, C., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Goryachev, M., Hartman, E., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E., Dror, J. A., Murayama, H., Rodd, N. L., and ADMX Collaboration. Fri . "Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX". United States. https://doi.org/10.1103/PhysRevLett.131.101002.
@article{osti_1999309,
title = {Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX},
author = {Nitta, T. and Braine, T. and Du, N. and Guzzetti, M. and Hanretty, C. and Leum, G. and Rosenberg, L. J. and Rybka, G. and Sinnis, J. and Clarke, John and Siddiqi, I. and Awida, M. H. and Chou, A. S. and Hollister, M. and Knirck, S. and Sonnenschein, A. and Wester, W. and Gleason, J. R. and Hipp, A. T. and Sikivie, P. and Sullivan, N. S. and Tanner, D. B. and Khatiwada, R. and Carosi, G. and Robertson, N. and Duffy, L. D. and Boutan, C. and Lentz, E. and Oblath, N. S. and Taubman, M. S. and Yang, J. and Daw, E. J. and Perry, M. G. and Bartram, C. and Buckley, J. H. and Gaikwad, C. and Hoffman, J. and Murch, K. W. and Goryachev, M. and Hartman, E. and McAllister, B. T. and Quiskamp, A. and Thomson, C. and Tobar, M. E. and Dror, J. A. and Murayama, H. and Rodd, N. L. and ADMX Collaboration},
abstractNote = {We report the first result of a direct search for a Cosmic axion Background (CaB) – a relativistic background of axions that is not dark matter – performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX). Conventional haloscope analyses search for a signal with a narrow bandwidth, as predicted for dark matter, whereas the CaB will be broad. We introduce a novel analysis strategy, which searches for a CaB induced daily modulation in the power measured by the haloscope. Using this, we repurpose data collected to search for dark matter to set a limit on the axion photon coupling of the CaB originating from dark matter decay in the 800–995 MHz frequency range. We find that the present sensitivity is limited by fluctuations in the cavity readout as the instrument scans across dark matter masses. Nevertheless, we demonstrate that these challenges can be surmounted with the use of superconducting qubits as single photon counters, and allow ADMX to operate as a telescope searching for axions emerging from the decay of dark matter. The daily modulation analysis technique we introduce can be deployed for various broadband RF signals, such as other forms of a CaB or even high-frequency gravitational waves.},
doi = {10.1103/PhysRevLett.131.101002},
journal = {Physical Review Letters},
number = 10,
volume = 131,
place = {United States},
year = {Fri Sep 08 00:00:00 EDT 2023},
month = {Fri Sep 08 00:00:00 EDT 2023}
}

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