Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Barceló, J. M."'
Autor:
Ahyoune, S., Melcón, A. Álvarez, Cuendis, S. Arguedas, Calatroni, S., Cogollos, C., Díaz-Morcillo, A., Döbrich, B., Gallego, J. D., García-Barceló, J. M., Gimeno, B., Golm, J., Granados, X., Gutierrez, J., Herwig, L., Irastorza, I. G., Lamas, N., Lozano-Guerrero, A., Millar, W. L., Malbrunot, C., Miralda-Escudé, J., Navarro, P., Navarro-Madrid, J. R., Puig, T., Siodlaczek, M., Telles, G. T., Wuensch, W.
We describe the results of a haloscope axion search performed with an 11.7 T dipole magnet at CERN. The search used a custom-made radio-frequency cavity coated with high-temperature superconducting tape. A set of 27 h of data at a resonant frequency
Externí odkaz:
http://arxiv.org/abs/2403.07790
Haloscopes, microwave resonant cavities utilized in detecting dark matter axions within powerful static magnetic fields, are pivotal in modern astrophysical research. This paper delves into the realm of cylindrical geometries, investigating technique
Externí odkaz:
http://arxiv.org/abs/2309.13199
Autor:
Ahyoune, S., Melcón, A. Álvarez, Cuendis, S. Arguedas, Calatroni, S., Cogollos, C., Devlin, J., Díaz-Morcillo, A., Díez-Ibáñez, D., Döbrich, B., Galindo, J., Gallego, J. D., García-Barceló, J. M., Gimeno, B., Golm, J., Gu, Y., Herwig, L., Irastorza, I. G., Lozano-Guerrero, A. J., Malbrunot, C., Miralda-Escudé, J., Monzó-Cabrera, J., Navarro, P., Navarro-Madrid, J. R., Redondo, J., Reina-Valero, J., Schmieden, K., Schneemann, T., Siodlaczek, M., Ulmer, S., Wuensch, W.
In the near future BabyIAXO will be the most powerful axion helioscope, relying on a custom-made magnet of two bores of 70 cm diameter and 10 m long, with a total available magnetic volume of more than 7 m$^3$. In this document, we propose and descri
Externí odkaz:
http://arxiv.org/abs/2306.17243
Autor:
García-Barceló, J. M., Melcón, A. Álvarez, Díaz-Morcillo, A., Gimeno, B., Lozano-Guerrero, A. J., Monzo-Cabrera, J., Navarro-Madrid, J. R., Navarro, P.
Haloscopes are resonant cavities that serve as detectors of dark matter axions when they are immersed in a strong static magnetic field. In order to increase the volume and improve its introduction within dipole or solenoid magnets for axion searches
Externí odkaz:
http://arxiv.org/abs/2302.10569
Autor:
Barceló, J. M. García, Melcón, A. Álvarez, Cuendis, S. Arguedas, Díaz-Morcillo, A., Gimeno, B., Kanareykin, A., Lozano-Guerrero, A. J., Navarro, P., Wuensch, W.
Tuning is an essential requirement for the search of dark matter axions employing haloscopes since its mass is not known yet to the scientific community. At the present day, most haloscope tuning systems are based on mechanical devices which can lead
Externí odkaz:
http://arxiv.org/abs/2204.11919
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:
Díaz-Morcillo, A., Barceló, J. M. García, Lozano-Guerrero, A. J., Navarro, P., Gimeno, B., Cuendis, S. Arguedas, Melcón, A. Álvarez, Cogollos, C., Calatroni, S., Döbrich, B., Gallego, J. D., Golm, J., Irastorza, I. G., Malbrunot, C., Miralda-Escudé, Jordi, Garay, C. Peña, Redondo, J., Wuensch, W.
Publikováno v:
Universe 2022, 8, 5
Within the increasing interest in the dark matter axion detection through haloscopes, in which different international groups are currently involved, the RADES group was established in 2016 with the goal of developing very sensitive detection systems
Externí odkaz:
http://arxiv.org/abs/2111.14510
Autor:
Golm, J., Cuendis, S. Arguedas, Calatroni, S., Cogollos, C., Döbrich, B., Gallego, J. D., Barceló, J. M. García, Granados, X., Gutierrez, J., Irastorza, I. G., Koettig, T., Lamas, N., Liberadzka-Porret, J., Malbrunot, C., Millar, W. L., Navarro, P., Carlos, C. Pereira, Puig, T., Rosaz, G. J., Siodlaczek, M., Telles, G., Wuensch, W.
Publikováno v:
IEEE Transactions on Applied Superconductivity 2022
The axion is a hypothetical particle which is a candidate for cold dark matter. Haloscope experiments directly search for these particles in strong magnetic fields with RF cavities as detectors. The Relic Axion Detector Exploratory Setup (RADES) at C
Externí odkaz:
http://arxiv.org/abs/2110.01296
Autor:
Navarro, P., Gimeno, Benito, Melcon, A. Alvarez, Cuendis, S. Arguedas, Cogollos, C., Diaz-Morcillo, A., Gallego, J. D., Barcelo, J. M. Garcia, Golm, J., Irastorza, I. G., Guerrero, A. J. Lozano, Garay, C. Penya
Publikováno v:
Physics of the Dark Universe 36 (2022) 101001
The electromagnetic coupling axion-photon in a microwave cavity is revisited with the Boundary Integral - Resonant Mode Expansion (BI-RME) 3D technique. Such full-wave modal technique has been applied for the rigorous analysis of the excitation of a
Externí odkaz:
http://arxiv.org/abs/2107.03137
Autor:
Melcón, A. Álvarez, Cuendis, S. Arguedas, Baier, J., Barth, K., Bräuniger, H., Calatroni, S., Cantatore, G., Caspers, F., Castel, J. F, Cetin, S. A., Cogollos, C., Dafni, T., Davenport, M., Dermenev, A., Desch, K., Díaz-Morcillo, A., Döbrich, B., Fischer, H., Funk, W., Gallego, J. D, Barceló, J. M García, Gardikiotis, A., Garza, J., Gimeno, B., Gninenko, S., Golm, J., Hasinoff, M., Hoffmann, D. H. H., Irastorza, I. G., Jakovčić, K., Kaminski, J., Karuza, M., Lakić, B., Laurent, J. M, Lozano-Guerrero, A., Luzón, G., Malbrunot, C., Maroudas, M., Miralda-Escudé, J., Mirallas, H., Miceli, L., Navarro, P., Ozbey, A., Özbozduman, K., Garay, C. Peña, Pivovaroff, M., Redondo, J., Ruz, J., Chóliz, E. Ruiz, Schmidt, S., Schumann, M., Semertzidis, Y., Solanki, S. K, Stewart, L., Tsagris, I., Vogel, T. Vafeiadis J. K., Widmann, E., Wuensch, W., Zioutas, K.
Publikováno v:
J. High Energ. Phys. 2021, 75 (2021)
We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67$\mu$eV mass range. A radio frequency cavity consisting of 5 s
Externí odkaz:
http://arxiv.org/abs/2104.13798