Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

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Main Authors:	ADMX Collaboration, Carosi, G., Cisneros, C., Du, N., Durham, S., Robertson, N., Goodman, C., Guzzetti, M., Hanretty, C., Enzian, K., Rosenberg, L. J, Rybka, G., Sinnis, J., Zhang, D., Clarke, John, Siddiqi, I., Chou, A. S., Hollister, M., Sonnenschein, A., Knirck, S., Caligiure, T. J., Gleason, J. R., Hipp, A. T., Sikivie, P., Solano, M. E., Sullivan, N. S., Tanner, D. B., Khatiwada, R., Duffy, L. D., Boutan, C., Braine, T., Lentz, E., Oblath, N. S., Taubman, M. S., Daw, E. J., Mostyn, C., Perry, M. G., Bartram, C., Laurel, J., Yi, A., Dyson, T. A., Ruppert, S., Withers, M. O., Kuo, C. L., McAllister, B. T., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K., Goryachev, M., Hartman, E., Quiskamp, A., Tobar, M. E.
Format:	Preprint
Published:	2025
Subjects:	High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics
Online Access:	Acceder al recurso
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author	ADMX Collaboration Carosi, G. Cisneros, C. Du, N. Durham, S. Robertson, N. Goodman, C. Guzzetti, M. Hanretty, C. Enzian, K. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Clarke, John Siddiqi, I. Chou, A. S. Hollister, M. Sonnenschein, A. Knirck, S. Caligiure, T. J. Gleason, J. R. Hipp, A. T. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Khatiwada, R. Duffy, L. D. Boutan, C. Braine, T. Lentz, E. Oblath, N. S. Taubman, M. S. Daw, E. J. Mostyn, C. Perry, M. G. Bartram, C. Laurel, J. Yi, A. Dyson, T. A. Ruppert, S. Withers, M. O. Kuo, C. L. McAllister, B. T. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. Goryachev, M. Hartman, E. Quiskamp, A. Tobar, M. E.
author_facet	ADMX Collaboration Carosi, G. Cisneros, C. Du, N. Durham, S. Robertson, N. Goodman, C. Guzzetti, M. Hanretty, C. Enzian, K. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Clarke, John Siddiqi, I. Chou, A. S. Hollister, M. Sonnenschein, A. Knirck, S. Caligiure, T. J. Gleason, J. R. Hipp, A. T. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Khatiwada, R. Duffy, L. D. Boutan, C. Braine, T. Lentz, E. Oblath, N. S. Taubman, M. S. Daw, E. J. Mostyn, C. Perry, M. G. Bartram, C. Laurel, J. Yi, A. Dyson, T. A. Ruppert, S. Withers, M. O. Kuo, C. L. McAllister, B. T. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. Goryachev, M. Hartman, E. Quiskamp, A. Tobar, M. E.
contents	Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10-1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov (KSVZ) sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.
format	Preprint
id	arxiv_https___arxiv_org_abs_2504_07279
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX ADMX Collaboration Carosi, G. Cisneros, C. Du, N. Durham, S. Robertson, N. Goodman, C. Guzzetti, M. Hanretty, C. Enzian, K. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Clarke, John Siddiqi, I. Chou, A. S. Hollister, M. Sonnenschein, A. Knirck, S. Caligiure, T. J. Gleason, J. R. Hipp, A. T. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Khatiwada, R. Duffy, L. D. Boutan, C. Braine, T. Lentz, E. Oblath, N. S. Taubman, M. S. Daw, E. J. Mostyn, C. Perry, M. G. Bartram, C. Laurel, J. Yi, A. Dyson, T. A. Ruppert, S. Withers, M. O. Kuo, C. L. McAllister, B. T. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. Goryachev, M. Hartman, E. Quiskamp, A. Tobar, M. E. High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark matter search using a haloscope to convert axions to photons in an external magnetic field. Key to this conversion is the use of a microwave resonator that enhances the sensitivity at the frequency of interest. The ADMX experiment boosts its sensitivity using a dilution refrigerator and near quantum-limited amplifier to reduce the noise level in the experimental apparatus. In the most recent run, ADMX searched for axions between 1.10-1.31 GHz to extended Kim-Shifman-Vainshtein-Zakharov (KSVZ) sensitivity. This Letter reports on the results of that run, as well as unique aspects of this experimental setup.
title	Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX
topic	High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2504.07279