First results of the CAST-RADES haloscope search for axions at 34.67 μeV

Autor: A. Álvarez Melcón, S. Arguedas Cuendis, J. Baier, K. Barth, H. Bräuninger, S. Calatroni, G. Cantatore, F. Caspers, J. F. Castel, S. A. Cetin, C. Cogollos, T. Dafni, M. Davenport, A. Dermenev, K. Desch, A. Díaz-Morcillo, B. Döbrich, H. Fischer, W. Funk, J. D. Gallego, J. M. García Barceló, A. Gardikiotis, J. G. Garza, B. Gimeno, S. Gninenko, J. Golm, M. D. Hasinoff, D. H. H. Hoffmann, I. G. Irastorza, K. Jakovčić, J. Kaminski, M. Karuza, B. Lakić, J. M. Laurent, A. J. Lozano-Guerrero, G. Luzón, C. Malbrunot, M. Maroudas, J. Miralda-Escudé, H. Mirallas, L. Miceli, P. Navarro, A. Ozbey, K. Özbozduman, C. Peña Garay, M. J. Pivovaroff, J. Redondo, J. Ruz, E. Ruiz Chóliz, S. Schmidt, M. Schumann, Y. K. Semertzidis, S. K. Solanki, L. Stewart, I. Tsagris, T. Vafeiadis, J. K. Vogel, E. Widmann, W. Wuensch, K. Zioutas

Publikováno v: Journal of High Energy Physics, Vol 2021, Iss 10, Pp 1-16 (2021)

Abstract 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 μeV mass range. A radio frequency cavity consisting

Externí odkaz: https://doaj.org/article/b4da561013ce4e3f99effa6ac702d493

First Results on the Search for Chameleons with the KWISP Detector at CAST

Autor: C. Krieger, Sami K. Solanki, K. Barth, B. Döbrich, S. Neff, Michael J. Pivovaroff, J. Castel, A. Belov, I. Tsagris, E. Ruiz Chóliz, Marc Schumann, A. Ozbey, A. V. Dermenev, A. Bayirli, L. Stewart, S. C. Yildiz, J. Ruz, J. G. Garza, L. Miceli, Serkant Ali Cetin, S. Arguedas Cuendis, T. Dafni, Giovanni Cantatore, J. M. Laurent, F.J. Iguaz, T. Vafeiadis, J. M. Carmona, Klaus Kurt Desch, I. G. Irastorza, M. Maroudas, M. D. Hasinoff, S. N. Gninenko, Biljana Lakić, I. Ortega, H. Bräuninger, M. Vretenar, Konstantin Zioutas, Søren Schmidt, Marin Karuza, Sebastian Baum, Julia Vogel, G. Luzón, A. Gardikiotis, Yannis K. Semertzidis, J. Baier, M. Davenport, Krešimir Jakovčić, M. Rosu, H. Fischer, Wolfgang Funk, J. A. García, Dieter Hoffmann, J. Kaminski

Publikováno v: Zaguán. Repositorio Digital de la Universidad de Zaragoza
instname
Physics of the Dark Universe
Zaguán: Repositorio Digital de la Universidad de Zaragoza
Universidad de Zaragoza

We report on a first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter. These dark energy candidates could be produced in the Sun and stream unimpeded to Earth. The KW

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f786cd67016d87b390dfb967c80b1a7e
http://cds.cern.ch/record/2677617

The cern axion solar telescope (CAST): an update

Autor: J. M. Carmona, Thomas Papaevangelou, S. Aune, A. Liolios, M.L. Sarsa, A. Ortiz de Solórzano, Y. Semertzidis, J. Engelhauser, José Villar, R. Kotthaus, F. T. Avignone, B. Beltrán, Milica Krčmar, J. P. Robert, Dieter H. H. Hoffmann, R. J. Creswick, J. Morales, Louis Walckiers, M. Delattre, A. Placci, W. Serber, A. Nikolaidis, Markus Kuster, K. Barth, G. Luzón, V. Arsov, D. Kang, A. Delbart, J. Franz, R. Hartmann, Ante Ljubičić, Efrain J. Ferrer, Georg G. Raffelt, Joachim Jacoby, Perikles Rammos, H. Bräuninger, F. H. Heinsius, J. N. Joux, Georgios Fanourakis, T. Geralis, A. Lippitsch, T. Aune, I. Giomataris, H. Fischer, C. Eleftheriadis, J. I. Collar, N. Golubev, E. Chesi, C. Lasseur, B. Vullierme, R. Deoliveira, M. Mutterer, M. D. Hasinoff, T. Dafni, S. Cebrián, H. A. Farach, Joaquin Vieira, A. Belov, G. Cipolla, I. G. Irastorza, M. Davenport, Gerhard Lutz, S. N. Gninenko, S. Dedousis, C. Schill, J. Ruz, Peter Friedrich, F. Formenti, Konstantin Zioutas, S. Andriamonje, K. Königsmann, A. Morales, Biljana Lakić, L. DiLella

Publikováno v: Nuclear Physics B - Proceedings Supplements. 138:41-44

The CERN Axion Solar Telescope (CAST), a 10 meter long LHC, 9 Tesla, test magnet is mounted on a moving platform that tracks the sun about 1.5 hours during sunrise, again during sunset. It moves ±8 0 vertically and ±40 0 horizontally. It has been t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::1a7179fe74759f2f0e5e23dca8d1ac74
https://doi.org/10.1016/j.nuclphysbps.2004.11.008

The Coronal Diagnostic Spectrometer for the solar and heliospheric observatory

Autor: R. A. Harrison, E. C. Sawyer, M. K. Carter, A. M. Cruise, R. M. Cutler, A. Fludra, R. W. Hayes, B. J. Kent, J. Lang, D. J. Parker, J. Payne, C. D. Pike, S. C. Peskett, A. G. Richards, J. L. Gulhane, K. Norman, A. A. Breeveld, E. R. Breeveld, K. F. Al Janabi, A. J. Mccalden, J. H. Parkinson, D. G. Self, P. D. Thomas, A. I. Poland, R. J. Thomas, W. T. Thompson, O. Kjeldseth-Moe, P. Brekke, J. Karud, P. Maltby, B. Aschenbach, H. Bräuninger, M. Kühne, J. Hollandt, O. H. W. Siegmund, M. C. E. Huber, A. H. Gabriel, H. E. Mason, B. J. I. Bromage

Publikováno v: Solar Physics. 162:233-290

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::0742f103831be4bf7f951cbce21a3bc5
https://doi.org/10.1007/bf00733431

Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope with (3)He Buffer Gas

Autor: M, Arik, S, Aune, K, Barth, A, Belov, S, Borghi, H, Bräuninger, G, Cantatore, J M, Carmona, S A, Cetin, J I, Collar, T, Dafni, M, Davenport, C, Eleftheriadis, N, Elias, C, Ezer, G, Fanourakis, E, Ferrer-Ribas, P, Friedrich, J, Galán, J A, García, A, Gardikiotis, E N, Gazis, T, Geralis, I, Giomataris, S, Gninenko, H, Gómez, E, Gruber, T, Guthörl, R, Hartmann, F, Haug, M D, Hasinoff, D H H, Hoffmann, F J, Iguaz, I G, Irastorza, J, Jacoby, K, Jakovčić, M, Karuza, K, Königsmann, R, Kotthaus, M, Krčmar, M, Kuster, B, Lakić, J M, Laurent, A, Liolios, A, Ljubičić, V, Lozza, G, Lutz, G, Luzón, J, Morales, T, Niinikoski, A, Nordt, T, Papaevangelou, M J, Pivovaroff, G, Raffelt, T, Rashba, H, Riege, A, Rodríguez, M, Rosu, J, Ruz, I, Savvidis, P S, Silva, S K, Solanki, L, Stewart, A, Tomás, M, Tsagri, K, van Bibber, T, Vafeiadis, J A, Villar, J K, Vogel, S C, Yildiz, K, Zioutas

The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=pmid_dedup__::effec1b3f3ef9b0f2b9aa57a11e0da8d
https://hdl.handle.net/11368/2489536