Zobrazeno 1 - 10
of 853
pro vyhledávání: '"Lewis, S M"'
Autor:
HAYSTAC Collaboration, Bai, Xiran, Jewell, M. J., Echevers, J. M., van Bibber, K., Cahn, S. B., Droster, A., Esmat, Maryam H., Ghosh, Sumita, Graham, Eleanor, Jackson, H., Laffan, Claire, Lamoreaux, S. K., Leder, A. F., Lehnert, K. W., Lewis, S. M., Maruyama, R. H., Nath, R. D., Rapidis, N. M., Ruddy, E. P., Silva-Feaver, M., Simanovskaia, M., Singh, Sukhman, Speller, D. H., Zacarias, Sabrina, Zhu, Yuqi
This Letter reports new results from the HAYSTAC experiment's search for dark matter axions in our galactic halo. It represents the widest search to date that utilizes squeezing to realize sub-quantum limited noise. The new results cover 1.71 $\mu$eV
Externí odkaz:
http://arxiv.org/abs/2409.08998
Autor:
HAYSTAC Collaboration, Jewell, M. J., Leder, A. F., Backes, K. M., Bai, Xiran, van Bibber, K., Brubaker, B. M., Cahn, S. B., Droster, A., Esmat, Maryam H., Ghosh, Sumita, Graham, Eleanor, Hilton, Gene C., Jackson, H., Laffan, Claire, Lamoreaux, S. K., Lehnert, K. W., Lewis, S. M., Malnou, M., Maruyama, R. H., Palken, D. A., Rapidis, N. M., Ruddy, E. P., Simanovskaia, M., Singh, Sukhman, Speller, D. H., Vale, Leila R., Wang, H., Zhu, Yuqi
A search for dark matter axions with masses $>10 \mu eV/c^{2}$ has been performed using the HAYSTAC experiment's squeezed state receiver to achieve sub-quantum limited noise. This report includes details of the design and operation of the experiment
Externí odkaz:
http://arxiv.org/abs/2301.09721
Autor:
Adams, C. B., Aggarwal, N., Agrawal, A., Balafendiev, R., Bartram, C., Baryakhtar, M., Bekker, H., Belov, P., Berggren, K. K., Berlin, A., Boutan, C., Bowring, D., Budker, D., Caldwell, A., Carenza, P., Carosi, G., Cervantes, R., Chakrabarty, S. S., Chaudhuri, S., Chen, T. Y., Cheong, S., Chou, A., Co, R. T., Conrad, J., Croon, D., D'Agnolo, R. T., Demarteau, M., DePorzio, N., Descalle, M., Desch, K., Di Luzio, L., Diaz-Morcillo, A., Dona, K., Drachnev, I. S., Droster, A., Du, N., Dunne, K., Döbrich, B., Ellis, S. A. R., Essig, R., Fan, J., Foster, J. W., Fry, J. T., Rosso, A. Gallo, Barceló, J. M. García, Irastorza, I. G., Gardner, S., Geraci, A. A., Ghosh, S., Giaccone, B., Giannotti, M., Gimeno, B., Grin, D., Grote, H., Guzzetti, M., Awida, M. H., Henning, R., Hoof, S., Hoshino, G., Irsic, V., Irwin, K. D., Jackson, H., Kimball, D. F. Jackson, Jaeckel, J., Jakovcic, K., Jewell, M. J., Kagan, M., Kahn, Y., Khatiwada, R., Knirck, S., Kovachy, T., Krueger, P., Kuenstner, S. E., Kurinsky, N. A., Leane, R. K., Leder, A. F., Lee, C., Lehnert, K. W., Lentz, E. W., Lewis, S. M., Liu, J., Lynn, M., Majorovits, B., Marsh, D. J. E., Maruyama, R. H., McAllister, B. T., Millar, A. J., Miller, D. W., Mitchell, J., Morampudi, S., Mueller, G., Nagaitsev, S., Nardi, E., Noroozian, O., O'Hare, C. A. J., Oblath, N. S., Ouellet, J. L., Pappas, K. M. W., Peiris, H. V., Perez, K., Phipps, A., Pivovaroff, M. J., Quílez, P., Rapidis, N. M., Robles, V. H., Rogers, K. K., Rudolph, J., Ruz, J., Rybka, G., Safdari, M., Safdi, B. R., Safronova, M. S., Salemi, C. P., Schuster, P., Schwartzman, A., Shu, J., Simanovskaia, M., Singh, J., Singh, S., Sinha, K., Sinnis, J. T., Siodlaczek, M., Smith, M. S., Snow, W. M., Sokolov, A. V., Sonnenschein, A., Speller, D. H., Stadnik, Y. V., Sun, C., Sushkov, A. O., Tait, T. M. P., Takhistov, V., Tanner, D. B., Tavecchio, F., Temples, D. J., Thomas, J. H., Tobar, M. E., Toro, N., Tsai, Y. -D., van Assendelft, E. C., van Bibber, K., Vandegar, M., Visinelli, L., Vitagliano, E., Vogel, J. K., Wang, Z., Wickenbrock, A., Winslow, L., Withington, S., Wooten, M., Yang, J., Young, B. A., Yu, F., Zhou, K., Zhou, T.
Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white p
Externí odkaz:
http://arxiv.org/abs/2203.14923
Autor:
Antypas, D., Banerjee, A., Bartram, C., Baryakhtar, M., Betz, J., Bollinger, J. J., Boutan, C., Bowring, D., Budker, D., Carney, D., Carosi, G., Chaudhuri, S., Cheong, S., Chou, A., Chowdhury, M. D., Co, R. T., López-Urrutia, J. R. Crespo, Demarteau, M., DePorzio, N., Derbin, A. V., Deshpande, T., Di Luzio, L., Diaz-Morcillo, A., Doyle, J. M., Drlica-Wagner, A., Droster, A., Du, N., Döbrich, B., Eby, J., Essig, R., Farren, G. S., Figueroa, N. L., Fry, J. T., Gardner, S., Geraci, A. A., Ghalsasi, A., Ghosh, S., Giannotti, M., Gimeno, B., Griffin, S. M., Grin, D., Grote, H., Gundlach, J. H., Guzzetti, M., Hanneke, D., Harnik, R., Henning, R., Irsic, V., Jackson, H., Kimball, D. F. Jackson, Jaeckel, J., Kagan, M., Kedar, D., Khatiwada, R., Knirck, S., Kolkowitz, S., Kovachy, T., Kuenstner, S. E., Lasner, Z., Leder, A. F., Lehnert, R., Leibrandt, D. R., Lentz, E., Lewis, S. M., Liu, Z., Manley, J., Maruyama, R. H., Millar, A. J., Muratova, V. N., Musoke, N., Nagaitsev, S., Noroozian, O., O'Hare, C. A. J., Ouellet, J. L., Pappas, K. M. W., Peik, E., Perez, G., Phipps, A., Rapidis, N. M., Robinson, J. M., Robles, V. H., Rogers, K. K., Rudolph, J., Rybka, G., Safdari, M., Safronova, M. S., Salemi, C. P., Schmidt, P. O., Schumm, T., Schwartzman, A., Shu, J., Simanovskaia, M., Singh, J., Singh, S., Smith, M. S., Snow, W. M., Stadnik, Y. V., Sun, C., Sushkov, A. O., Tait, T. M. P., Takhistov, V., Tanner, D. B., Temples, D. J., Thirolf, P. G., Thomas, J. H., Tobar, M. E., Tretiak, O., Tsai, Y. -D., Tyson, J. A., Vandegar, M., Vermeulen, S., Visinelli, L., Vitagliano, E., Wang, Z., Wilson, D. J., Winslow, L., Withington, S., Wooten, M., Yang, J., Ye, J., Young, B. A., Yu, F., Zaheer, M. H., Zelevinsky, T., Zhao, Y., Zhou, K.
The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. Transformative advances in quantum technologies have led to a plethora of new high-precision
Externí odkaz:
http://arxiv.org/abs/2203.14915
A plasma haloscope has recently been proposed as a feasible approach to extend the search for dark matter axions above 10 GHz ($\sim$ 40 $\mu$eV), whereby the microwave cavity in a conventional axion haloscope is supplanted by a wire array metamateri
Externí odkaz:
http://arxiv.org/abs/2203.13945
Autor:
Backes, K. M., Palken, D. A., Kenany, S. Al, Brubaker, B. M., Cahn, S. B., Droster, A., Hilton, Gene C., Ghosh, Sumita, Jackson, H., Lamoreaux, S. K., Leder, A. F., Lehnert, K. W., Lewis, S. M., Malnou, M., Maruyama, R. H., Rapidis, N. M., Simanovskaia, M., Singh, Sukhman, Speller, D. H., Urdinaran, I., Vale, Leila R., van Assendelft, E. C., van Bibber, K., Wang, H.
In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a new parti
Externí odkaz:
http://arxiv.org/abs/2008.01853
Autor:
Palken, D. A., Brubaker, B. M., Malnou, M., Kenany, S. Al, Backes, K. M., Cahn, S. B., Gurevich, Y. V., Lamoreaux, S. K., Lewis, S. M., Maruyama, R. H., Rapidis, N. M., Root, J. R., Simanovskaia, M., Shokair, T. M., Singh, Sukhman, Speller, D. H., Urdinaran, I., van Bibber, K., Zhong, L., Lehnert, K. W.
Publikováno v:
Phys. Rev. D 101, 123011 (2020)
In experiments searching for axionic dark matter, the use of the standard threshold-based data analysis discards valuable information. We present a Bayesian analysis framework that builds on an existing processing protocol to extract more information
Externí odkaz:
http://arxiv.org/abs/2003.08510
Autor:
Zhong, L., Kenany, S. Al, Backes, K. M., Brubaker, B. M., Cahn, S. B., Carosi, G., Gurevich, Y. V., Kindel, W. F., Lamoreaux, S. K., Lehnert, K. W., Lewis, S. M., Malnou, M., Maruyama, R. H., Palken, D. A., Rapidis, N. M., Root, J. R., Simanovskaia, M., Shokair, T. M., Speller, D. H., Urdinaran, I., van Bibber, K. A.
Publikováno v:
Phys. Rev. D 97, 092001 (2018)
We report on the results from a search for dark matter axions with the HAYSTAC experiment using a microwave cavity detector at frequencies between 5.6-5.8$\, \rm Ghz$. We exclude axion models with two photon coupling $g_{a\gamma\gamma}\,\gtrsim\,2\ti
Externí odkaz:
http://arxiv.org/abs/1803.03690
Design and Operational Experience of a Microwave Cavity Axion Detector for the 20-100 micro-eV Range
Autor:
Kenany, S. Al, Anil, M. A., Backes, K. M., Brubaker, B. M., Cahn, S. B., Carosi, G., Gurevich, Y. V., Kindel, W. F., Lamoreaux, S. K., Lehnert, K. W., Lewis, S. M., Malnou, M., Palken, D. A., Rapidis, N. M., Root, J. R., Simanovskaia, M., Shokair, T. M., Urdinaran, I., van Bibber, K. A., Zhong, L.
We describe a dark matter axion detector designed, constructed, and operated both as an innovation platform for new cavity and amplifier technologies and as a data pathfinder in the $5 - 25$ GHz range ($\sim20-100\: \mu$eV). The platform is small but
Externí odkaz:
http://arxiv.org/abs/1611.07123