دورية أكاديمية
Conceptual design of BabyIAXO, the intermediate stage towards the International Axion Observatory
| العنوان: | Conceptual design of BabyIAXO, the intermediate stage towards the International Axion Observatory |
|---|---|
| المؤلفون: | Abeln, A., Altenmüller, K., Arguedas Cuendis, S., Armengaud, E., Attié, D., Aune, S., Basso, S., Bergé, L., Biasuzzi, B., Borges de Sousa, P.T. C., Brun, P., Bykovskiy, N., Calvet, D., Carmona, J.M., Castel, J.F., Cebrián, S., Chernov, V., Christensen, F.E., Civitani, M.M., Cogollos, C., Dafní, T., Derbin, A., Desch, K., Díez, D., Dinter, M., Döbrich, B., Drachnev, I., Dudarev, A., Dumoulin, L., Ferreira, D.D. M., Ferrer-Ribas, E., Fleck, I., Galán, J., Gascón, D., Gastaldo, L., Giannotti, M., Giomataris, Y., Giuliani, A., Gninenko, S., Golm, J., Golubev, N., Hagge, L., Hahn, J., Hailey, C.J., Hengstler, D., Henriksen, P.L., Houdy, T., Iglesias-Marzoa, R., Iguaz, F.J., Irastorza, I.G., Iñiguez, C., Jakovčić, K., Kaminski, J., Kanoute, B., Karstensen, S., Kravchuk, L., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Loidl, M., Lomskaya, I., López-Alegre, G., Lubsandorzhiev, B., Ludwig, K., Luzón, G., Malbrunot, C., Margalejo, C., Marin-Franch, A., Marnieros, S., Marutzky, F., Mauricio, J., Menesguen, Y., Mentink, M., Mertens, S., Mescia, F., Miralda-Escudé, J., Mirallas, H., Mols, J.P., Muratova, V., Navick, X.F., Nones, C., Notari, A., Nozik, A., Obis, L., Oriol, C., Orsini, F., Ortiz de Solórzano, A., Oster, S., Pais da Silva, H.P., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Pérez, O., Picatoste, E., Pivovaroff, M.J., Poda, D.V., Redondo, J., Ringwald, A., Rodrigues, M., Rueda-Teruel, F., Rueda-Teruel, S., Ruiz-Choliz, E., Ruz, J., Saemann, E.O., Salvado, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Segui, L., Tavecchio, F., ten Kate, H.H. J., Tkachev, I., Troitsky, S., Unger, D., Unzhakov, E., Ushakov, N., Vogel, J.K., Voronin, D., Weltman, A., Werthenbach, U., Wuensch, W., Yanes-Díaz, A. |
| المساهمون: | Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Synchrotron SOLEIL (SSOLEIL), Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), IAXO, ANR-19-CE31-0024,DALPS,Déteteurs pour la recherche des particules "axion-like"(2019) |
| المصدر: | JHEP ; https://hal.science/hal-02999568Test ; JHEP, 2021, 05, pp.137. ⟨10.1007/JHEP05(2021)137⟩ |
| بيانات النشر: | HAL CCSD |
| سنة النشر: | 2021 |
| مصطلحات موضوعية: | Beyond Standard Model, Dark matter, CP violation, Other experiments, axion: solar, axion: dark matter, IAXO, optics, axion-like particles, sensitivity, detector: design, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], envir, phil |
| الوصف: | International audience ; This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles (ALPs), produced in the Sun, with unprecedented sensitivity. BabyIAXO is conceived to test all IAXO subsystems (magnet, optics and detectors) at a relevant scale for the final system and thus serve as prototype for IAXO, but at the same time as a fully-fledged helioscope with relevant physics reach itself, and with potential for discovery. The BabyIAXO magnet will feature two 10 m long, 70 cm diameter bores, and will host two detection lines (optics and detector) of dimensions similar to the final ones foreseen for IAXO. BabyIAXO will detect or reject solar axions or ALPs with axion-photon couplings down to g$_{aγ}$ ∼ 1.5 × 10$^{−11}$ GeV$^{−1}$, and masses up to m$_{a}$ ∼ 0.25 eV. BabyIAXO will offer additional opportunities for axion research in view of IAXO, like the development of precision x-ray detectors to identify particular spectral features in the solar axion spectrum, and the implementation of radiofrequency-cavity-based axion dark matter setups.[graphic not available: see fulltext] |
| نوع الوثيقة: | article in journal/newspaper |
| اللغة: | English |
| العلاقة: | https://hal.science/hal-02999568Test |
| الإتاحة: | https://doi.org/10.1007/JHEP05Test(2021)137 https://hal.science/hal-02999568Test |
| حقوق: | undefined |
| رقم الانضمام: | edsbas.DC5D0D90 |
| قاعدة البيانات: | BASE |
| الوصف غير متاح. |