Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Rosenberg, L J"'
Autor:
Bartram, C., Boutan, C., Braine, T., Buckley, J. H., Caligiure, T. J., Carosi, G., Chou, A. S., Cisneros, C., Clarke, John, Daw, E. J., Du, N., Duffy, L. D., Dyson, T. A., Gaikwad, C., Gleason, J. R., Goodman, C., Goryachev, M., Guzzetti, M., Hanretty, C., Hartman, E., Hipp, A. T., Hoffman, J., Hollister, M., Khatiwada, R., Knirck, S., Kuo, C. L., Lentz, E., McAllister, B. T., Mostyn, C., Murch, K., Oblath, N. S., Perry, M. G., Quiskamp, A., Robertson, N., Rosenberg, L. J, Ruppert, S., Rybka, G., Siddiqi, I., Sikivie, P., Sinnis, J., Solano, M. E., Sonnenschein, A., Sullivan, N. S., Tanner, D. B., Taubman, M. S., Tobar, M. E., Withers, M. O., Woollett, N., Zhang, D.
We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise Josephson parametric ampli
Externí odkaz:
http://arxiv.org/abs/2408.15227
Autor:
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.
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 ueV in axion mass) at DFSZ sensitivity. The resulting axion searc
Externí odkaz:
http://arxiv.org/abs/2312.16668
Autor:
Bartram, C., Braine, T., Cervantes, R., Crisosto, N., Du, N., Goodman, C., Guzzetti, M., Hanretty, C., Lee, S., Leum, G., Rosenberg, L. J., Rybka, G., Sinnis, J., Zhang, D., Awida, M. H., Bowring, D., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Khatiwada, R., Brodsky, J., Carosi, G., Duffy, L. D., Goryachev, M., McAllister, B., Quiskamp, A., Thomson, C., Tobar, M. E., Boutan, C., Jones, M., LaRoque, B. H., Lentz, E., Man, N. E., Oblath, N. S., Taubman, M. S., Yang, J., Clarke, John, Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Han, Y., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Daw, E. J., Perry, M. G., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Russell, J.
The Axion Dark Matter eXperiment (ADMX) has previously excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions between 680-790 MHz under the assumption that the dark matter is described by the isothermal halo model. However, the precise nature of th
Externí odkaz:
http://arxiv.org/abs/2311.07748
Autor:
ADMX Collaboration, 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.
Publikováno v:
Phys. Rev. Lett., 131, 101002 (2023)
We report the first result of a direct search for a Cosmic ${\it axion}$ Background (C$a$B) - a relativistic background of axions that is not dark matter - performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX). Conventional halo
Externí odkaz:
http://arxiv.org/abs/2303.06282
Autor:
Chakrabarty, S., Gleason, J. R., Han, Y., Hipp, A. T., Solano, M., Sikivie, P., Sullivan, N. S., Tanner, D. B., Goryachev, M., Hartman, E., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Braine, T., Guzzetti, M., Hanretty, C., Leum, G., Rosenberg, L. J, Rybka, G., Sinnis, J., Clarke, John, Siddiqi, I., Khatiwada, R., Carosi, G., Du, N., Robertson, N., Duffy, L. D., Boutan, C., Oblath, N. S., Taubman, M. S., Yang, J., Lentz, E., Daw, E. J., Perry, M. G., Bartram, C., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Nitta, T.
We investigate reentrant and dielectric loaded cavities for the purpose of extending the range of axion cavity haloscopes to lower masses, below the range where the Axion Dark Matter eXperiment (ADMX) has already searched. Reentrant and dielectric lo
Externí odkaz:
http://arxiv.org/abs/2303.07116
Autor:
Bartram, C., Braine, T., Cervantes, R., Crisosto, N., Du, N., Leum, G., Mohapatra, P., Nitta, T., Rosenberg, L. J, Rybka, G., Yang, J., Clarke, John, Siddiqi, I., Agrawal, A., Dixit, A. V., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Hoof, S., Lentz, E., Khatiwada, R., Carosi, G., Cisneros, C., Robertson, N., Woollett, N., Duffy, L. D., Boutan, C., Jones, M., LaRoque, B. H., Oblath, N. S., Taubman, M. S., Daw, E. J., Perry, M. G., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K., Goryachev, M., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E.
Publikováno v:
Rev. Sci. Instrum., 94, 044703, 2023
We present a new exclusion bound of axion-like particle dark matter with axion-photon couplings above $\mathrm{10^{-13}}$ $\mathrm{GeV^{-1}}$ over the frequency range 4796.7--4799.5 MHz, corresponding to a narrow range of axion masses centered around
Externí odkaz:
http://arxiv.org/abs/2110.10262
Autor:
ADMX Collaboration, Bartram, C., Braine, T., Burns, E., Cervantes, R., Crisosto, N., Du, N., Korandla, H., Leum, G., Mohapatra, P., Nitta, T., Rosenberg, L. J, Rybka, G., Yang, J., Clarke, John, Siddiqi, I., Agrawal, A., Dixit, A. V., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Lentz, E., Khatiwada, R., Carosi, G., Robertson, N., Woollett, N., Duffy, L. D., Boutan, C., Jones, M., LaRoque, B. H., Oblath, N. S., Taubman, M. S., Daw, E. J., Perry, M. G., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Goryachev, M., McAllister, B. T., Quiskamp, A., Thomson, C., Tobar, M. E.
Publikováno v:
Phys. Rev. Lett. 127, 261803 (2021)
We report the results from a haloscope search for axion dark matter in the $3.3\text{-}4.2~{\mu}$eV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the KSVZ model.
Externí odkaz:
http://arxiv.org/abs/2110.06096
Autor:
ADMX Collaboration, Bartram, C., Braine, T., Cervantes, R., Crisosto, N., Du, N., Leum, G., Rosenberg, L. J, Rybka, G., Yang, J., Bowring, D., Chou, A. S., Khatiwada, R., Sonnenschein, A., Wester, W., Carosi, G., Woollett, N., Duffy, L. D., Goryachev, M., McAllister, B., Tobar, M. E., Boutan, C., Jones, M., Laroque, B. H., Oblath, N. S., Taubman, M. S., Clarke, John, Dove, A., Eddins, A., O'Kelley, S. R., Nawaz, S., Siddiqi, I., Stevenson, N., Agrawal, A., Dixit, A. V., Gleason, J. R., Jois, S., Sikivie, P., Solomon, J. A., Sullivan, N. S., Tanner, D. B., Lentz, E., Daw, E. J., Perry, M. G., Buckley, J. H., Harrington, P. M., Henriksen, E. A., Murch, K. W.
Publikováno v:
Phys. Rev. D 103, 032002 (2021)
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 $\mu$eV, corresponding to the frequency range 680--790 MHz. Using an axion haloscope consisting of a microwave cavity i
Externí odkaz:
http://arxiv.org/abs/2010.06183
Autor:
Khatiwada, R., Bowring, D., Chou, A. S., Sonnenschein, A., Wester, W., Mitchell, D. V., Braine, T., Bartram, C., Cervantes, R., Crisosto, N., Du, N., Kimes, S., Rosenberg, L. J, Rybka, G., Yang, J., Will, D., Carosi, G., Woollett, N., Durham, S., Duffy, L. D., Bradley, R., Boutan, C., Jones, M., LaRoque, B. H., Oblath, N. S., Taubman, M. S., Tedeschi, J., Clarke, John, Dove, A., Eddins, A., Hashim, A., O'Kelley, S. R., Nawaz, S., Siddiqi, I., Stevenson, N., Agrawal, A., Dixit, A. V., Gleason, J. R., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Solomon, J. A., Lentz, E., Daw, E. J., Perry, M. G., Buckley, J. H., Harrington, P. M., Henriksen, E. A., Murch, K. W., Hilton, G. C.
Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the $2.66$ to $3.1$ $\mu$eV mass range with Dine-Fischler-Srednicki-Z
Externí odkaz:
http://arxiv.org/abs/2010.00169
Autor:
Braine, T., Cervantes, R., Crisosto, N., Du, N., Kimes, S., Rosenberg, L. J, Rybka, G., Yang, J., Bowring, D., Chou, A. S., Khatiwada, R., Sonnenschein, A., Wester, W., Carosi, G., Woollett, N., Duffy, L. D., Bradley, R., Boutan, C., Jones, M., LaRoque, B. H., Oblath, N. S., Taubman, M. S., Clarke, J., Dove, A., Eddins, A., O'Kelley, S. R., Nawaz, S., Siddiqi, I., Stevenson, N., Agrawal, A., Dixit, A. V., Gleason, J. R., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Lentz, E., Daw, E. J., Buckley, J. H., Harrington, P. M., Henriksen, E. A., Murch, K. W.
Publikováno v:
Phys. Rev. Lett. 124, 101303 (2020)
This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range $2.81$-$3.31$ ${\mu}eV$. This search excludes the full range of axion-photon coupling values predicted in benchmark models of the invisible
Externí odkaz:
http://arxiv.org/abs/1910.08638