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Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory

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. Baby...

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Published in:arXiv.org 2021-03
Main Authors: Altenmüller, K, S Arguedas Cuendis, Armengaud, E, Attié, D, Basso, S, Bergé, L, P T C Borges De Sousa, Brun, P, Bykovskiy, N, Calvet, D, Carmona, J M, Castel, J F, Cebrián, S, Chernov, V, Christensen, F E, Civitani, M M, Cogollos, C, Derbin, A, Desch, K, Díez, D, Dinter, M, Döbrich, B, Drachnev, I, Dudarev, A, Dumoulin, L, Ferrer-Ribas, E, Fleck, I, Galán, J, Gascón, D, Giomataris, Y, Giuliani, A, Golm, J, Golubev, N, Hagge, L, Hahn, J, Hailey, C J, Hengstler, D, Houdy, T, Iglesias-Marzoa, R, Iguaz, F J, Irastorza, I G, Iñiguez, C, Jakovcic, K, Kaminski, J, Karstensen, S, Lasserre, T, Laurent, P, Lindner, A, Loidl, M, Lomskaya, I, López-Alegre, G, Ludwig, K, Luzón, G, Margalejo, C, Marin-Franch, A, Marnieros, S, Marutzky, F, Mauricio, J, Mentink, M, Mertens, S, Mescia, F, Miralda-Escudé, J, Mirallas, H, Mols, J P, Muratova, V, Nones, C, Notari, A, Obis, L, Oriol, C, Orsini, F, Ortiz de Solórzano, A, H P Pais Da Silva, 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, Ruiz-Choliz, E, Saemann, E O, Salvado, J, Schiffer, T, Schmidt, S, Schneekloth, U, Schott, M, H H J ten Kate, Tkachev, I, Troitsky, S, Unger, D, Unzhakov, E, Ushakov, N, Vogel, J K, Weltman, A, Yanes-Díaz, A
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creator Altenmüller, K
S Arguedas Cuendis
Armengaud, E
Attié, D
Basso, S
Bergé, L
P T C Borges De Sousa
Brun, P
Bykovskiy, N
Calvet, D
Carmona, J M
Castel, J F
Cebrián, S
Chernov, V
Christensen, F E
Civitani, M M
Cogollos, C
Derbin, A
Desch, K
Díez, D
Dinter, M
Döbrich, B
Drachnev, I
Dudarev, A
Dumoulin, L
Ferrer-Ribas, E
Fleck, I
Galán, J
Gascón, D
Giomataris, Y
Giuliani, A
Golm, J
Golubev, N
Hagge, L
Hahn, J
Hailey, C J
Hengstler, D
Houdy, T
Iglesias-Marzoa, R
Iguaz, F J
Irastorza, I G
Iñiguez, C
Jakovcic, K
Kaminski, J
Karstensen, S
Lasserre, T
Laurent, P
Lindner, A
Loidl, M
Lomskaya, I
López-Alegre, G
Ludwig, K
Luzón, G
Margalejo, C
Marin-Franch, A
Marnieros, S
Marutzky, F
Mauricio, J
Mentink, M
Mertens, S
Mescia, F
Miralda-Escudé, J
Mirallas, H
Mols, J P
Muratova, V
Nones, C
Notari, A
Obis, L
Oriol, C
Orsini, F
Ortiz de Solórzano, A
H P Pais Da Silva
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
Ruiz-Choliz, E
Saemann, E O
Salvado, J
Schiffer, T
Schmidt, S
Schneekloth, U
Schott, M
H H J ten Kate
Tkachev, I
Troitsky, S
Unger, D
Unzhakov, E
Ushakov, N
Vogel, J K
Weltman, A
Yanes-Díaz, A
description 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 \(g_{a\gamma} \sim 1.5 \times 10^{-11}\) GeV\(^{-1}\), and masses up to \(m_a\sim 0.25\) 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.
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K</creatorcontrib><creatorcontrib>Weltman, A</creatorcontrib><creatorcontrib>Yanes-Díaz, A</creatorcontrib><title>Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory</title><title>arXiv.org</title><description>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 \(g_{a\gamma} \sim 1.5 \times 10^{-11}\) GeV\(^{-1}\), and masses up to \(m_a\sim 0.25\) 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.</description><subject>Conceptual design</subject><subject>Couplings</subject><subject>Dark matter</subject><subject>Observatories</subject><subject>Radio frequency</subject><subject>Subsystems</subject><subject>X ray 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20210304</creationdate><title>Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory</title><author>Altenmüller, K ; S Arguedas Cuendis ; Armengaud, E ; Attié, D ; Basso, S ; Bergé, L ; P T C Borges De Sousa ; Brun, P ; Bykovskiy, N ; Calvet, D ; Carmona, J M ; Castel, J F ; Cebrián, S ; Chernov, V ; Christensen, F E ; Civitani, M M ; Cogollos, C ; Derbin, A ; Desch, K ; Díez, D ; Dinter, M ; Döbrich, B ; Drachnev, I ; Dudarev, A ; Dumoulin, L ; Ferrer-Ribas, E ; Fleck, I ; Galán, J ; Gascón, D ; Giomataris, Y ; Giuliani, A ; Golm, J ; Golubev, N ; Hagge, L ; Hahn, J ; Hailey, C J ; Hengstler, D ; Houdy, T ; Iglesias-Marzoa, R ; Iguaz, F J ; Irastorza, I G ; Iñiguez, C ; Jakovcic, K ; Kaminski, J ; Karstensen, S ; Lasserre, T ; Laurent, P ; Lindner, A ; Loidl, M ; Lomskaya, I ; López-Alegre, G ; Ludwig, K ; Luzón, G ; Margalejo, C ; Marin-Franch, A ; Marnieros, S ; Marutzky, F ; Mauricio, J ; Mentink, M ; Mertens, S ; Mescia, F ; Miralda-Escudé, J ; Mirallas, H ; Mols, J P ; Muratova, V ; Nones, C ; Notari, A ; Obis, L ; Oriol, C ; Orsini, F ; Ortiz de Solórzano, A ; H P Pais Da Silva ; 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 ; Ruiz-Choliz, E ; Saemann, E O ; Salvado, J ; Schiffer, T ; Schmidt, S ; Schneekloth, U ; Schott, M ; H H J ten Kate ; Tkachev, I ; Troitsky, S ; Unger, D ; Unzhakov, E ; Ushakov, N ; Vogel, J K ; Weltman, A ; Yanes-Díaz, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_24542416373</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Conceptual design</topic><topic>Couplings</topic><topic>Dark matter</topic><topic>Observatories</topic><topic>Radio frequency</topic><topic>Subsystems</topic><topic>X ray detectors</topic><toplevel>online_resources</toplevel><creatorcontrib>Altenmüller, K</creatorcontrib><creatorcontrib>S Arguedas Cuendis</creatorcontrib><creatorcontrib>Armengaud, E</creatorcontrib><creatorcontrib>Attié, D</creatorcontrib><creatorcontrib>Basso, S</creatorcontrib><creatorcontrib>Bergé, L</creatorcontrib><creatorcontrib>P T C Borges De Sousa</creatorcontrib><creatorcontrib>Brun, P</creatorcontrib><creatorcontrib>Bykovskiy, N</creatorcontrib><creatorcontrib>Calvet, D</creatorcontrib><creatorcontrib>Carmona, J M</creatorcontrib><creatorcontrib>Castel, J 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Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Altenmüller, K</au><au>S Arguedas Cuendis</au><au>Armengaud, E</au><au>Attié, D</au><au>Basso, S</au><au>Bergé, L</au><au>P T C Borges De Sousa</au><au>Brun, P</au><au>Bykovskiy, N</au><au>Calvet, D</au><au>Carmona, J M</au><au>Castel, J F</au><au>Cebrián, S</au><au>Chernov, V</au><au>Christensen, F E</au><au>Civitani, M M</au><au>Cogollos, C</au><au>Derbin, A</au><au>Desch, K</au><au>Díez, D</au><au>Dinter, M</au><au>Döbrich, B</au><au>Drachnev, I</au><au>Dudarev, A</au><au>Dumoulin, L</au><au>Ferrer-Ribas, E</au><au>Fleck, I</au><au>Galán, J</au><au>Gascón, D</au><au>Giomataris, Y</au><au>Giuliani, A</au><au>Golm, J</au><au>Golubev, N</au><au>Hagge, L</au><au>Hahn, J</au><au>Hailey, C J</au><au>Hengstler, D</au><au>Houdy, T</au><au>Iglesias-Marzoa, R</au><au>Iguaz, F J</au><au>Irastorza, I G</au><au>Iñiguez, C</au><au>Jakovcic, K</au><au>Kaminski, J</au><au>Karstensen, S</au><au>Lasserre, T</au><au>Laurent, P</au><au>Lindner, A</au><au>Loidl, M</au><au>Lomskaya, I</au><au>López-Alegre, G</au><au>Ludwig, K</au><au>Luzón, G</au><au>Margalejo, C</au><au>Marin-Franch, A</au><au>Marnieros, S</au><au>Marutzky, F</au><au>Mauricio, J</au><au>Mentink, M</au><au>Mertens, S</au><au>Mescia, F</au><au>Miralda-Escudé, J</au><au>Mirallas, H</au><au>Mols, J P</au><au>Muratova, V</au><au>Nones, C</au><au>Notari, A</au><au>Obis, L</au><au>Oriol, C</au><au>Orsini, F</au><au>Ortiz de Solórzano, A</au><au>H P Pais Da Silva</au><au>Pantuev, V</au><au>Papaevangelou, T</au><au>Pareschi, G</au><au>Perez, K</au><au>Pérez, O</au><au>Picatoste, E</au><au>Pivovaroff, M J</au><au>Poda, D V</au><au>Redondo, J</au><au>Ringwald, A</au><au>Rodrigues, M</au><au>Rueda-Teruel, F</au><au>Ruiz-Choliz, E</au><au>Saemann, E O</au><au>Salvado, J</au><au>Schiffer, T</au><au>Schmidt, S</au><au>Schneekloth, U</au><au>Schott, M</au><au>H H J ten Kate</au><au>Tkachev, I</au><au>Troitsky, S</au><au>Unger, D</au><au>Unzhakov, E</au><au>Ushakov, N</au><au>Vogel, J K</au><au>Weltman, A</au><au>Yanes-Díaz, A</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory</atitle><jtitle>arXiv.org</jtitle><date>2021-03-04</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>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 \(g_{a\gamma} \sim 1.5 \times 10^{-11}\) GeV\(^{-1}\), and masses up to \(m_a\sim 0.25\) 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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Conceptual design
Couplings
Dark matter
Observatories
Radio frequency
Subsystems
X ray detectors
title Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory
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