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Title: Search for Solar Axions via Axion-Photon Coupling with the Majorana Demonstrator

Abstract

Axions were originally proposed to explain the strong-CP problem in QCD. Through axion-photon coupling, the Sun could be a major source of axions, which could be measured in solid state detection experiments with enhancements due to coherent Primakoff-Bragg scattering. The Majorana Demonstrator experiment has searched for solar axions with a set of ^{76}Ge-enriched high purity germanium detectors using a 33 kg-yr exposure collected between January, 2017 and November, 2019. A temporal-energy analysis gives a new limit on the axion-photon coupling as g_{aγ} <1.45×10^{-9} GeV^{-1} (95% confidence level) for axions with mass up to 100 eV/c^{2}. This improves laboratory-based limits between about 1 eV/c^{2} and 100 eV/c^{2}.

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ORCiD logo; ; ; Majorana Collaboration"" class="biblio-detail-author-link"> « less
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Pacific Northwest National Laboratory (PNNL), Richland, WA (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF); University of North Carolina, Chapel Hill, NC (United States); Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); USDOE Laboratory Directed Research and Development (LDRD) Program; USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
MAJORANA Collaboration
OSTI Identifier:
1882456
Alternate Identifier(s):
OSTI ID: 1883665; OSTI ID: 1889418; OSTI ID: 1889989; OSTI ID: 1907285; OSTI ID: 1907633; OSTI ID: 1924035
Report Number(s):
PNNL-SA-172847; LA-UR-22-23621
Journal ID: ISSN 0031-9007; PRLTAO; 081803
Grant/Contract Number:  
AC02-05CH11231; AC05-00OR22725; AC05-76RL0130; FG02-97ER41020; FG02-97ER41033; FG02-97ER41041; SC0012612; SC0014445; SC0018060; LANLEM77/LANLEM78; MRI-0923142; PHY-1003399; PHY-1102292; PHY-1206314; PHY-1614611; PHY-1812409; PHY-1812356; PHY-2111140; AC05-76RL01830; 89233218CNA000001
Resource Type:
Published Article
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Name: Physical Review Letters Journal Volume: 129 Journal Issue: 8; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
axions; solid-state detectors; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Atomic, Nuclear and Particle Physics; Dark Matter, Majorana, Double-beta decay; 73 NUCLEAR PHYSICS AND RADIATION PHYSICS

Citation Formats

Arnquist, I. J., Avignone, F. T., Barabash, A. S., Barton, C. J., Bhimani, K. H., Blalock, E., Bos, B., Busch, M., Buuck, M., Caldwell, T. S., Chan, Y-D., Christofferson, C. D., Chu, P. -H., Clark, M. L., Cuesta, C., Detwiler, J. A., Efremenko, Yu., Ejiri, H., Elliott, S. R., Giovanetti, G. K., Green, M. P., Gruszko, J., Guinn, I. S., Guiseppe, V. E., Haufe, C. R., Henning, R., Hervas Aguilar, D., Hoppe, E. W., Hostiuc, A., Kidd, M. F., Kim, I., Kouzes, R. T., Lannen V., T. E., Li, A., Lopez, A. M., López-Castaño, J. M., Martin, E. L., Martin, R. D., Massarczyk, R., Meijer, S. J., Oli, T. K., Othman, G., Paudel, L. S., Pettus, W., Poon, A. W. P., Radford, D. C., Reine, A. L., Rielage, K., Ruof, N. W., Schaper, D. C., Tedeschi, D., Varner, R. L., Vasilyev, S., Wilkerson, J. F., Wiseman, C., Xu, W., Yu, C. -H., Zhu, B. X., and Majorana Collaboration. Search for Solar Axions via Axion-Photon Coupling with the Majorana Demonstrator. United States: N. p., 2022. Web. doi:10.1103/PhysRevLett.129.081803.
Arnquist, I. J., Avignone, F. T., Barabash, A. S., Barton, C. J., Bhimani, K. H., Blalock, E., Bos, B., Busch, M., Buuck, M., Caldwell, T. S., Chan, Y-D., Christofferson, C. D., Chu, P. -H., Clark, M. L., Cuesta, C., Detwiler, J. A., Efremenko, Yu., Ejiri, H., Elliott, S. R., Giovanetti, G. K., Green, M. P., Gruszko, J., Guinn, I. S., Guiseppe, V. E., Haufe, C. R., Henning, R., Hervas Aguilar, D., Hoppe, E. W., Hostiuc, A., Kidd, M. F., Kim, I., Kouzes, R. T., Lannen V., T. E., Li, A., Lopez, A. M., López-Castaño, J. M., Martin, E. L., Martin, R. D., Massarczyk, R., Meijer, S. J., Oli, T. K., Othman, G., Paudel, L. S., Pettus, W., Poon, A. W. P., Radford, D. C., Reine, A. L., Rielage, K., Ruof, N. W., Schaper, D. C., Tedeschi, D., Varner, R. L., Vasilyev, S., Wilkerson, J. F., Wiseman, C., Xu, W., Yu, C. -H., Zhu, B. X., & Majorana Collaboration. Search for Solar Axions via Axion-Photon Coupling with the Majorana Demonstrator. United States. https://doi.org/10.1103/PhysRevLett.129.081803
Arnquist, I. J., Avignone, F. T., Barabash, A. S., Barton, C. J., Bhimani, K. H., Blalock, E., Bos, B., Busch, M., Buuck, M., Caldwell, T. S., Chan, Y-D., Christofferson, C. D., Chu, P. -H., Clark, M. L., Cuesta, C., Detwiler, J. A., Efremenko, Yu., Ejiri, H., Elliott, S. R., Giovanetti, G. K., Green, M. P., Gruszko, J., Guinn, I. S., Guiseppe, V. E., Haufe, C. R., Henning, R., Hervas Aguilar, D., Hoppe, E. W., Hostiuc, A., Kidd, M. F., Kim, I., Kouzes, R. T., Lannen V., T. E., Li, A., Lopez, A. M., López-Castaño, J. M., Martin, E. L., Martin, R. D., Massarczyk, R., Meijer, S. J., Oli, T. K., Othman, G., Paudel, L. S., Pettus, W., Poon, A. W. P., Radford, D. C., Reine, A. L., Rielage, K., Ruof, N. W., Schaper, D. C., Tedeschi, D., Varner, R. L., Vasilyev, S., Wilkerson, J. F., Wiseman, C., Xu, W., Yu, C. -H., Zhu, B. X., and Majorana Collaboration. Fri . "Search for Solar Axions via Axion-Photon Coupling with the Majorana Demonstrator". United States. https://doi.org/10.1103/PhysRevLett.129.081803.
@article{osti_1882456,
title = {Search for Solar Axions via Axion-Photon Coupling with the Majorana Demonstrator},
author = {Arnquist, I. J. and Avignone, F. T. and Barabash, A. S. and Barton, C. J. and Bhimani, K. H. and Blalock, E. and Bos, B. and Busch, M. and Buuck, M. and Caldwell, T. S. and Chan, Y-D. and Christofferson, C. D. and Chu, P. -H. and Clark, M. L. and Cuesta, C. and Detwiler, J. A. and Efremenko, Yu. and Ejiri, H. and Elliott, S. R. and Giovanetti, G. K. and Green, M. P. and Gruszko, J. and Guinn, I. S. and Guiseppe, V. E. and Haufe, C. R. and Henning, R. and Hervas Aguilar, D. and Hoppe, E. W. and Hostiuc, A. and Kidd, M. F. and Kim, I. and Kouzes, R. T. and Lannen V., T. E. and Li, A. and Lopez, A. M. and López-Castaño, J. M. and Martin, E. L. and Martin, R. D. and Massarczyk, R. and Meijer, S. J. and Oli, T. K. and Othman, G. and Paudel, L. S. and Pettus, W. and Poon, A. W. P. and Radford, D. C. and Reine, A. L. and Rielage, K. and Ruof, N. W. and Schaper, D. C. and Tedeschi, D. and Varner, R. L. and Vasilyev, S. and Wilkerson, J. F. and Wiseman, C. and Xu, W. and Yu, C. -H. and Zhu, B. X. and Majorana Collaboration},
abstractNote = {Axions were originally proposed to explain the strong-CP problem in QCD. Through axion-photon coupling, the Sun could be a major source of axions, which could be measured in solid state detection experiments with enhancements due to coherent Primakoff-Bragg scattering. The Majorana Demonstrator experiment has searched for solar axions with a set of ^{76}Ge-enriched high purity germanium detectors using a 33 kg-yr exposure collected between January, 2017 and November, 2019. A temporal-energy analysis gives a new limit on the axion-photon coupling as g_{aγ} <1.45×10^{-9} GeV^{-1} (95% confidence level) for axions with mass up to 100 eV/c^{2}. This improves laboratory-based limits between about 1 eV/c^{2} and 100 eV/c^{2}.},
doi = {10.1103/PhysRevLett.129.081803},
journal = {Physical Review Letters},
number = 8,
volume = 129,
place = {United States},
year = {Fri Aug 19 00:00:00 EDT 2022},
month = {Fri Aug 19 00:00:00 EDT 2022}
}

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