Axion search with BabyIAXO in view of IAXO

Javier Galan; A. Abeln; K. Altenmüller; S. Arguedas Cuendis; E. Armengaud; D. Attié; S. Aune; S. Basso; L. Bergé; B. Biasuzzi; P. T. C. Borges De Sousa; P. Brun; N. Bykovskiy; D. Calvet; J. M. Carmona; J. F. Castel; S. Cebrian; V. Chernov; F. E. Christensen; M.M. Civitani; C. Cogollos; T. Dafni; A. Derbin; K. Desch; D. Díez; M. Dinter; B. Dobrich; I. Drachnev; A. Dudarev; L. Dumoulin; D. D. M. Ferreira; E. Ferrer-Ribas; I. Fleck; D. Gascon; L. Gastaldo; M. Giannotti; Y. Giomataris; A. Giuliani; S. Gninenko; J. Golm; N. Golubev; L. Hagge; J. Hahn; C. J. Hailey; D. Hengstler; P. L. Henriksen; R. Iglesias-Marzoa; F. J. Iguaz-Gutierrez; I. G. Irastorza; C. Iñiguez; K. Jakovčić; J. Kaminski; B. Kanoute; S. Karstensen; L. Kravchuk; B. Lakić; T. Lasserre; P. Laurent; O. Limousin; A. Lindner; M. Loidl; I. Lomskaya; G. López-Alegre; B. Lubsandorzhiev; K. Ludwig; G. Luzon; C. Malbrunot; C. Margalejo; A. Marin-Franch; S. Marnieros; F. Marutzky; J. Mauricio; Y. Menesguen; M. Mentink; F. Mescia; J. Miralda-Escudé; H. Mirallas; J. P. Mols; V. Muratova; X. F. Navick; C. Nones; A. Notari; A. Nozik; L. Obis; C. Oriol; F. Orsini; A. Ortiz de Solórzano; S. Oster; H. P. Pais Da Silva; V. Pantuev; T. Papaevangelou; G. Pareschi; K. Perez; O. Pérez; E. Picatoste; M. J. Pivovaroff; D. V. Poda; J. Redondo; A. Ringwald; M. R.D. Rodrigues; F. Rueda-Teruel; S. Rueda-Teruel; E. Ruiz-Choliz; J. Ruz; E. O. Saemann; J. Salvado; T. Schiffer; S. Schmidt; U. Schneekloth; M. Schott; L. Segui; F. Tavecchio; H. H. J. ten Kate; I. Tkachev; S. Troitsky; D. Unger; E. Unzhakov; N. Ushakov; J. K. Vogel; D. Voronin; A. Weltman; U. Werthenbach; W. Wuensch; A. Yanes-Díaz

doi:10.22323/1.390.0631

Axion search with BabyIAXO in view of IAXO

Javier Galan, A. Abeln, K. Altenmüller, S. Arguedas Cuendis, E. Armengaud, D. Attié, S. Aune, S. Basso, L. Bergé, B. Biasuzzi, P. T. C. Borges De Sousa, P. Brun, N. Bykovskiy, D. Calvet, J. M. Carmona, J. F. Castel, S. Cebrian, V. Chernov, F. E. Christensen, M.M. CivitaniC. Cogollos, T. Dafni, A. Derbin, K. Desch, D. Díez, M. Dinter, B. Dobrich, I. Drachnev, A. Dudarev, L. Dumoulin, D. D. M. Ferreira, E. Ferrer-Ribas, I. Fleck, D. Gascon, L. Gastaldo, M. Giannotti, Y. Giomataris, A. Giuliani, S. Gninenko, J. Golm, N. Golubev, L. Hagge, J. Hahn, C. J. Hailey, D. Hengstler, P. L. Henriksen, R. Iglesias-Marzoa, F. J. Iguaz-Gutierrez, I. G. Irastorza, C. Iñiguez, K. Jakovčić, J. Kaminski, B. Kanoute, S. Karstensen, L. Kravchuk, B. Lakić, T. Lasserre, P. Laurent, O. Limousin, A. Lindner, M. Loidl, I. Lomskaya, G. López-Alegre, B. Lubsandorzhiev, K. Ludwig, G. Luzon, C. Malbrunot, C. Margalejo, A. Marin-Franch, S. Marnieros, F. Marutzky, J. Mauricio, Y. Menesguen, M. Mentink, F. Mescia, J. Miralda-Escudé, H. Mirallas, J. P. Mols, V. Muratova, X. F. Navick, C. Nones, A. Notari, A. Nozik, L. Obis, C. Oriol, F. Orsini, A. Ortiz de Solórzano, S. Oster, H. P. Pais Da Silva, V. Pantuev, T. Papaevangelou, G. Pareschi, K. Perez, O. Pérez, E. Picatoste, M. J. Pivovaroff, D. V. Poda, J. Redondo, A. Ringwald, M. R.D. Rodrigues, F. Rueda-Teruel, S. Rueda-Teruel, E. Ruiz-Choliz, J. Ruz, E. O. Saemann, J. Salvado, T. Schiffer, S. Schmidt, U. Schneekloth, M. Schott, L. Segui, F. Tavecchio, H. H. J. ten Kate, I. Tkachev, S. Troitsky, D. Unger, E. Unzhakov, N. Ushakov, J. K. Vogel, D. Voronin, A. Weltman, U. Werthenbach, W. Wuensch, A. Yanes-Díaz

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Abstract

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun’s core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to background ratio of about 5 orders of magnitude higher than CAST. Recently the IAXO collaboration has proposed and intermediate experimental stage, BabyIAXO, conceived to test all IAXO subsystems (magnet, optics, detectors and sun-tracking systems) at a relevant scale for the final system and thus serve as pathfinder for IAXO but at the same time as a fully-fledged helioscope with record and relevant physics reach in itself with potential for discovery. BabyIAXO was endorsed by the Physics Review committee of DESY last May 2019. Here we will review the status and prospects of BabyIAXO and its potential to probe the most physics motivated regions of the axion & ALPs parameter space.

Original language	English
Title of host publication	Proceedings of 40th International Conference on High Energy physics (ICHEP2020)
Number of pages	6
Volume	390
Publisher	Proceedings of Science
Publication date	2021
Article number	631
DOIs	https://doi.org/10.22323/1.390.0631
Publication status	Published - 2021
Event	40th International Conference on High Energy Physics - Virtual conference, Prague, Czech Republic Duration: 28 Jul 2020 → 6 Aug 2020

Conference

Conference	40th International Conference on High Energy Physics
Location	Virtual conference
Country/Territory	Czech Republic
City	Prague
Period	28/07/2020 → 06/08/2020

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10.22323/1.390.0631Licence: CC BY-NC-ND

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Galan, J., 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., Cebrian, S., Chernov, V., Christensen, F. E., ... Yanes-Díaz, A. (2021). Axion search with BabyIAXO in view of IAXO. In Proceedings of 40th International Conference on High Energy physics (ICHEP2020) (Vol. 390). Article 631 Proceedings of Science. https://doi.org/10.22323/1.390.0631

@inproceedings{33fc9b94607f45f98a3636191c4ccc20,

title = "Axion search with BabyIAXO in view of IAXO",

abstract = "Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun{\textquoteright}s core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to background ratio of about 5 orders of magnitude higher than CAST. Recently the IAXO collaboration has proposed and intermediate experimental stage, BabyIAXO, conceived to test all IAXO subsystems (magnet, optics, detectors and sun-tracking systems) at a relevant scale for the final system and thus serve as pathfinder for IAXO but at the same time as a fully-fledged helioscope with record and relevant physics reach in itself with potential for discovery. BabyIAXO was endorsed by the Physics Review committee of DESY last May 2019. Here we will review the status and prospects of BabyIAXO and its potential to probe the most physics motivated regions of the axion & ALPs parameter space.",

author = "Javier Galan and A. Abeln and K. Altenm{\"u}ller and {Arguedas Cuendis}, S. and E. Armengaud and D. Atti{\'e} and S. Aune and S. Basso and L. Berg{\'e} and B. Biasuzzi and {Borges De Sousa}, {P. T. C.} and P. Brun and N. Bykovskiy and D. Calvet and Carmona, {J. M.} and Castel, {J. F.} and S. Cebrian and V. Chernov and Christensen, {F. E.} and M.M. Civitani and C. Cogollos and T. Dafni and A. Derbin and K. Desch and D. D{\'i}ez and M. Dinter and B. Dobrich and I. Drachnev and A. Dudarev and L. Dumoulin and Ferreira, {D. D. M.} and E. Ferrer-Ribas and I. Fleck and D. Gascon and L. Gastaldo and M. Giannotti and Y. Giomataris and A. Giuliani and S. Gninenko and J. Golm and N. Golubev and L. Hagge and J. Hahn and Hailey, {C. J.} and D. Hengstler and Henriksen, {P. L.} and R. Iglesias-Marzoa and Iguaz-Gutierrez, {F. J.} and Irastorza, {I. G.} and C. I{\~n}iguez and K. Jakov{\v c}i{\'c} and J. Kaminski and B. Kanoute and S. Karstensen and L. Kravchuk and B. Laki{\'c} and T. Lasserre and P. Laurent and O. Limousin and A. Lindner and M. Loidl and I. Lomskaya and G. L{\'o}pez-Alegre and B. Lubsandorzhiev and K. Ludwig and G. Luzon and C. Malbrunot and C. Margalejo and A. Marin-Franch and S. Marnieros and F. Marutzky and J. Mauricio and Y. Menesguen and M. Mentink and F. Mescia and J. Miralda-Escud{\'e} and H. Mirallas and Mols, {J. P.} and V. Muratova and Navick, {X. F.} and C. Nones and A. Notari and A. Nozik and L. Obis and C. Oriol and F. Orsini and {Ortiz de Sol{\'o}rzano}, A. and S. Oster and {Pais Da Silva}, {H. P.} and V. Pantuev and T. Papaevangelou and G. Pareschi and K. Perez and O. P{\'e}rez and E. Picatoste and Pivovaroff, {M. J.} and Poda, {D. V.} and J. Redondo and A. Ringwald and Rodrigues, {M. R.D.} and F. Rueda-Teruel and S. Rueda-Teruel and E. Ruiz-Choliz and J. Ruz and Saemann, {E. O.} and J. Salvado and T. Schiffer and S. Schmidt and U. Schneekloth and M. Schott and L. Segui and F. Tavecchio and {ten Kate}, {H. H. J.} and I. Tkachev and S. Troitsky and D. Unger and E. Unzhakov and N. Ushakov and Vogel, {J. K.} and D. Voronin and A. Weltman and U. Werthenbach and W. Wuensch and A. Yanes-D{\'i}az",

year = "2021",

doi = "10.22323/1.390.0631",

language = "English",

volume = "390",

booktitle = "Proceedings of 40th International Conference on High Energy physics (ICHEP2020)",

publisher = "Proceedings of Science",

note = "40th International Conference on High Energy Physics , ICHEP 2020 ; Conference date: 28-07-2020 Through 06-08-2020",

}

Galan, J, Abeln, A, Altenmüller, K, Arguedas Cuendis, S, Armengaud, E, Attié, D, Aune, S, Basso, S, Bergé, L, Biasuzzi, B, Borges De Sousa, PTC, Brun, P, Bykovskiy, N, Calvet, D, Carmona, JM, Castel, JF, Cebrian, S, Chernov, V, Christensen, FE, Civitani, MM, Cogollos, C, Dafni, T, Derbin, A, Desch, K, Díez, D, Dinter, M, Dobrich, B, Drachnev, I, Dudarev, A, Dumoulin, L, Ferreira, DDM, Ferrer-Ribas, E, Fleck, I, Gascon, D, Gastaldo, L, Giannotti, M, Giomataris, Y, Giuliani, A, Gninenko, S, Golm, J, Golubev, N, Hagge, L, Hahn, J, Hailey, CJ, Hengstler, D, Henriksen, PL, Iglesias-Marzoa, R, Iguaz-Gutierrez, FJ, Irastorza, IG, 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, Luzon, G, Malbrunot, C, Margalejo, C, Marin-Franch, A, Marnieros, S, Marutzky, F, Mauricio, J, Menesguen, Y, Mentink, M, Mescia, F, Miralda-Escudé, J, Mirallas, H, Mols, JP, Muratova, V, Navick, XF, Nones, C, Notari, A, Nozik, A, Obis, L, Oriol, C, Orsini, F, Ortiz de Solórzano, A, Oster, S, Pais Da Silva, HP, Pantuev, V, Papaevangelou, T, Pareschi, G, Perez, K, Pérez, O, Picatoste, E, Pivovaroff, MJ, Poda, DV, Redondo, J, Ringwald, A, Rodrigues, MRD, Rueda-Teruel, F, Rueda-Teruel, S, Ruiz-Choliz, E, Ruz, J, Saemann, EO, Salvado, J, Schiffer, T, Schmidt, S, Schneekloth, U, Schott, M, Segui, L, Tavecchio, F, ten Kate, HHJ, Tkachev, I, Troitsky, S, Unger, D, Unzhakov, E, Ushakov, N, Vogel, JK, Voronin, D, Weltman, A, Werthenbach, U, Wuensch, W & Yanes-Díaz, A 2021, Axion search with BabyIAXO in view of IAXO. in Proceedings of 40th International Conference on High Energy physics (ICHEP2020). vol. 390, 631, Proceedings of Science, 40th International Conference on High Energy Physics , Prague, Czech Republic, 28/07/2020. https://doi.org/10.22323/1.390.0631

TY - GEN

T1 - Axion search with BabyIAXO in view of IAXO

AU - Galan, Javier

AU - Abeln, A.

AU - Altenmüller, K.

AU - Arguedas Cuendis, S.

AU - Armengaud, E.

AU - Attié, D.

AU - Aune, S.

AU - Basso, S.

AU - Bergé, L.

AU - Biasuzzi, B.

AU - Borges De Sousa, P. T. C.

AU - Brun, P.

AU - Bykovskiy, N.

AU - Calvet, D.

AU - Carmona, J. M.

AU - Castel, J. F.

AU - Cebrian, S.

AU - Chernov, V.

AU - Christensen, F. E.

AU - Civitani, M.M.

AU - Cogollos, C.

AU - Dafni, T.

AU - Derbin, A.

AU - Desch, K.

AU - Díez, D.

AU - Dinter, M.

AU - Dobrich, B.

AU - Drachnev, I.

AU - Dudarev, A.

AU - Dumoulin, L.

AU - Ferreira, D. D. M.

AU - Ferrer-Ribas, E.

AU - Fleck, I.

AU - Gascon, D.

AU - Gastaldo, L.

AU - Giannotti, M.

AU - Giomataris, Y.

AU - Giuliani, A.

AU - Gninenko, S.

AU - Golm, J.

AU - Golubev, N.

AU - Hagge, L.

AU - Hahn, J.

AU - Hailey, C. J.

AU - Hengstler, D.

AU - Henriksen, P. L.

AU - Iglesias-Marzoa, R.

AU - Iguaz-Gutierrez, F. J.

AU - Irastorza, I. G.

AU - Iñiguez, C.

AU - Jakovčić, K.

AU - Kaminski, J.

AU - Kanoute, B.

AU - Karstensen, S.

AU - Kravchuk, L.

AU - Lakić, B.

AU - Lasserre, T.

AU - Laurent, P.

AU - Limousin, O.

AU - Lindner, A.

AU - Loidl, M.

AU - Lomskaya, I.

AU - López-Alegre, G.

AU - Lubsandorzhiev, B.

AU - Ludwig, K.

AU - Luzon, G.

AU - Malbrunot, C.

AU - Margalejo, C.

AU - Marin-Franch, A.

AU - Marnieros, S.

AU - Marutzky, F.

AU - Mauricio, J.

AU - Menesguen, Y.

AU - Mentink, M.

AU - Mescia, F.

AU - Miralda-Escudé, J.

AU - Mirallas, H.

AU - Mols, J. P.

AU - Muratova, V.

AU - Navick, X. F.

AU - Nones, C.

AU - Notari, A.

AU - Nozik, A.

AU - Obis, L.

AU - Oriol, C.

AU - Orsini, F.

AU - Ortiz de Solórzano, A.

AU - Oster, S.

AU - Pais Da Silva, H. P.

AU - Pantuev, V.

AU - Papaevangelou, T.

AU - Pareschi, G.

AU - Perez, K.

AU - Pérez, O.

AU - Picatoste, E.

AU - Pivovaroff, M. J.

AU - Poda, D. V.

AU - Redondo, J.

AU - Ringwald, A.

AU - Rodrigues, M. R.D.

AU - Rueda-Teruel, F.

AU - Rueda-Teruel, S.

AU - Ruiz-Choliz, E.

AU - Ruz, J.

AU - Saemann, E. O.

AU - Salvado, J.

AU - Schiffer, T.

AU - Schmidt, S.

AU - Schneekloth, U.

AU - Schott, M.

AU - Segui, L.

AU - Tavecchio, F.

AU - ten Kate, H. H. J.

AU - Tkachev, I.

AU - Troitsky, S.

AU - Unger, D.

AU - Unzhakov, E.

AU - Ushakov, N.

AU - Vogel, J. K.

AU - Voronin, D.

AU - Weltman, A.

AU - Werthenbach, U.

AU - Wuensch, W.

AU - Yanes-Díaz, A.

PY - 2021

Y1 - 2021

N2 - Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun’s core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to background ratio of about 5 orders of magnitude higher than CAST. Recently the IAXO collaboration has proposed and intermediate experimental stage, BabyIAXO, conceived to test all IAXO subsystems (magnet, optics, detectors and sun-tracking systems) at a relevant scale for the final system and thus serve as pathfinder for IAXO but at the same time as a fully-fledged helioscope with record and relevant physics reach in itself with potential for discovery. BabyIAXO was endorsed by the Physics Review committee of DESY last May 2019. Here we will review the status and prospects of BabyIAXO and its potential to probe the most physics motivated regions of the axion & ALPs parameter space.

AB - Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun’s core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to background ratio of about 5 orders of magnitude higher than CAST. Recently the IAXO collaboration has proposed and intermediate experimental stage, BabyIAXO, conceived to test all IAXO subsystems (magnet, optics, detectors and sun-tracking systems) at a relevant scale for the final system and thus serve as pathfinder for IAXO but at the same time as a fully-fledged helioscope with record and relevant physics reach in itself with potential for discovery. BabyIAXO was endorsed by the Physics Review committee of DESY last May 2019. Here we will review the status and prospects of BabyIAXO and its potential to probe the most physics motivated regions of the axion & ALPs parameter space.

U2 - 10.22323/1.390.0631

DO - 10.22323/1.390.0631

M3 - Article in proceedings

VL - 390

BT - Proceedings of 40th International Conference on High Energy physics (ICHEP2020)

PB - Proceedings of Science

T2 - 40th International Conference on High Energy Physics

Y2 - 28 July 2020 through 6 August 2020

ER -

Axion search with BabyIAXO in view of IAXO

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