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Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers

Fuente: arXiv

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Auteurs principaux:	Hipp, A. T., Quiskamp, A., Caligiure, T. J., Gleason, J. R., Han, Y., Jois, S., Sikivie, P., Solano, M. E., Sullivan, N. S., Tanner, D. B., Goryachev, M., Hartman, E., Tobar, M. E., McAllister, B. T., Duffy, L. D., Braine, T., Burns, E., Cervantes, R., Crisosto, N., Goodman, C., Guzzetti, M., Hanretty, C., Lee, S., Korandla, H., Leum, G., Mohapatra, P., Nitta, T., Rosenberg, L. J, Rybka, G., Sinnis, J., Zhang, D., Bartram, C., Dyson, T. A., Kuo, C. L., Ruppert, S., Withers, M. O., Awida, M. H., Bowring, D., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Brodsky, J., Carosi, G., Du, N., Roberston, N., Woollett, N., Boutan, C., Jones, A. M., LaRoque, B. H., Lentz, E., Man, N. E., Oblath, N. S., Taubman, M. S., Yang, J., Khatiwada, R., Clarke, John, Siddiqi, I., Agrawal, A., Dixit, A. V., Daw, E. J., Perry, M. G., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Russell, J.
Format:	Preprint
Publié:	2024
Sujets:	Cosmology and Nongalactic Astrophysics
Accès en ligne:	Acceder al recurso
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_version_	1866914985240690688
author	Hipp, A. T. Quiskamp, A. Caligiure, T. J. Gleason, J. R. Han, Y. Jois, S. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Goryachev, M. Hartman, E. Tobar, M. E. McAllister, B. T. Duffy, L. D. Braine, T. Burns, E. Cervantes, R. Crisosto, N. Goodman, C. Guzzetti, M. Hanretty, C. Lee, S. Korandla, H. Leum, G. Mohapatra, P. Nitta, T. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Bartram, C. Dyson, T. A. Kuo, C. L. Ruppert, S. Withers, M. O. Awida, M. H. Bowring, D. Chou, A. S. Hollister, M. Knirck, S. Sonnenschein, A. Wester, W. Brodsky, J. Carosi, G. Du, N. Roberston, N. Woollett, N. Boutan, C. Jones, A. M. LaRoque, B. H. Lentz, E. Man, N. E. Oblath, N. S. Taubman, M. S. Yang, J. Khatiwada, R. Clarke, John Siddiqi, I. Agrawal, A. Dixit, A. V. Daw, E. J. Perry, M. G. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. W. Russell, J.
author_facet	Hipp, A. T. Quiskamp, A. Caligiure, T. J. Gleason, J. R. Han, Y. Jois, S. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Goryachev, M. Hartman, E. Tobar, M. E. McAllister, B. T. Duffy, L. D. Braine, T. Burns, E. Cervantes, R. Crisosto, N. Goodman, C. Guzzetti, M. Hanretty, C. Lee, S. Korandla, H. Leum, G. Mohapatra, P. Nitta, T. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Bartram, C. Dyson, T. A. Kuo, C. L. Ruppert, S. Withers, M. O. Awida, M. H. Bowring, D. Chou, A. S. Hollister, M. Knirck, S. Sonnenschein, A. Wester, W. Brodsky, J. Carosi, G. Du, N. Roberston, N. Woollett, N. Boutan, C. Jones, A. M. LaRoque, B. H. Lentz, E. Man, N. E. Oblath, N. S. Taubman, M. S. Yang, J. Khatiwada, R. Clarke, John Siddiqi, I. Agrawal, A. Dixit, A. V. Daw, E. J. Perry, M. G. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. W. Russell, J.
contents	The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth's motion. We report an exclusion on the local axion dark matter density in narrow flows of $ρ_a \gtrsim 0.03\,\mathrm{GeV/cm^3}$ and $ρ_a \gtrsim 0.004\,\mathrm{GeV/cm^3}$ for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range $3.3-4.2\,μ\text{eV}$. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.
format	Preprint
id	arxiv_https___arxiv_org_abs_2410_09203
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers Hipp, A. T. Quiskamp, A. Caligiure, T. J. Gleason, J. R. Han, Y. Jois, S. Sikivie, P. Solano, M. E. Sullivan, N. S. Tanner, D. B. Goryachev, M. Hartman, E. Tobar, M. E. McAllister, B. T. Duffy, L. D. Braine, T. Burns, E. Cervantes, R. Crisosto, N. Goodman, C. Guzzetti, M. Hanretty, C. Lee, S. Korandla, H. Leum, G. Mohapatra, P. Nitta, T. Rosenberg, L. J Rybka, G. Sinnis, J. Zhang, D. Bartram, C. Dyson, T. A. Kuo, C. L. Ruppert, S. Withers, M. O. Awida, M. H. Bowring, D. Chou, A. S. Hollister, M. Knirck, S. Sonnenschein, A. Wester, W. Brodsky, J. Carosi, G. Du, N. Roberston, N. Woollett, N. Boutan, C. Jones, A. M. LaRoque, B. H. Lentz, E. Man, N. E. Oblath, N. S. Taubman, M. S. Yang, J. Khatiwada, R. Clarke, John Siddiqi, I. Agrawal, A. Dixit, A. V. Daw, E. J. Perry, M. G. Buckley, J. H. Gaikwad, C. Hoffman, J. Murch, K. W. Russell, J. Cosmology and Nongalactic Astrophysics The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-velocity dispersion flows requires a high spectral resolution and careful attention to the expected signal modulation due to Earth's motion. We report an exclusion on the local axion dark matter density in narrow flows of $ρ_a \gtrsim 0.03\,\mathrm{GeV/cm^3}$ and $ρ_a \gtrsim 0.004\,\mathrm{GeV/cm^3}$ for Dine-Fischler-Srednicki-Zhitnitski and Kim-Shifman-Vainshtein-Zakharov axion-photon couplings, respectively, over the mass range $3.3-4.2\,μ\text{eV}$. Measurements were made at selected resolving powers to allow for a range of possible velocity dispersions.
title	Search for non-virialized axions with 3.3-4.2 $μ$eV mass at selected resolving powers
topic	Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2410.09203