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An accurate solar axions ray-tracing response of BabyIAXO

Fuente: arXiv

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Bibliographische Detailangaben
Hauptverfasser:	Ahyoune, S., Altenmueller, K., Antolin, I., Basso, S., Brun, P., Candon, F. R., Castel, J. F., Cebrian, S., Chouhan, D., Della Ceca, R., Cervera-Cortes, M., Chernov, V., Civitani, M. M., Cogollos, C., Costa, E., Cotroneo, V., Dafni, T., Derbin, A., Desch, K., Diaz-Martin, M. C., Diaz-Morcillo, A., Diez-Ibanez, D., Pardos, C. Diez, Dinter, M., Doebrich, B., Drachnev, I., Dudarev, A., Ezquerro, A., Fabiani, S., Ferrer-Ribas, E., Finelli, F., Fleck, I., Galan, J., Galanti, G., Galaverni, M., Garcia, J. A., Garcia-Barcelo, J. M., Gastaldo, L., Giannotti, M., Giganon, A., Goblin, C., Goyal, N., Gu, Y., Hagge, L., Helary, L., Hengstler, D., Heuchel, D., Hoof, S., Iglesias-Marzoa, R., Iguaz, F. J., Iniguez, C., Irastorza, I. G., Jakovcic, K., Kaefer, D., Kaminski, J., Karstensen, S., Law, M., Lindner, A., Loidl, M., Loiseau, C., Lopez-Alegre, G., Lozano-Guerrero, A., Lubsandorzhiev, B., Luzon, G., Manthos, I., Margalejo, C., Marin-Franch, A., Marques, J., Marutzky, F., Menneglier, C., Mentink, M., Mertens, S., Miralda-Escude, J., Mirallas, H., Muleri, F., Muratova, V., Navarro-Madrid, J. R., Navick, X. F., Nikolopoulos, K., Notari, A., Nozik, A., Obis, L., Ortiz-de-Solorzano, A., O'Shea, T., von Oy, J., Pareschi, G., Papaevangelou, T., Perez, K., Perez, O., Picatoste, E., Pivovaroff, M. J., Porron, J., Puyuelo, M. J., Quintana, A., Redondo, J., Reuther, D., Ringwald, A., Rodrigues, M., Rubini, A., Rueda-Teruel, S., Rueda-Teruel, F., Ruiz-Choliz, E., Ruz, J., Schaffran, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schoenfeld, L., Schott, M., Segui, L., Singh, U. R., Soffitta, P., Spiga, D., Stern, M., Straniero, O., Tavecchio, F., Unzhakov, E., Ushakov, N. A., Vecchi, G., Vogel, J. K., Voronin, D. M., Ward, R., Weltman, A., Wiesinger, C., Wolf, R., Yanes-Diaz, A., Yu, Y.
Format:	Preprint
Veröffentlicht:	2024
Schlagworte:	High Energy Physics - Experiment Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Computational Physics Data Analysis, Statistics and Probability
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author	Ahyoune, S. Altenmueller, K. Antolin, I. Basso, S. Brun, P. Candon, F. R. Castel, J. F. Cebrian, S. Chouhan, D. Della Ceca, R. Cervera-Cortes, M. Chernov, V. Civitani, M. M. Cogollos, C. Costa, E. Cotroneo, V. Dafni, T. Derbin, A. Desch, K. Diaz-Martin, M. C. Diaz-Morcillo, A. Diez-Ibanez, D. Pardos, C. Diez Dinter, M. Doebrich, B. Drachnev, I. Dudarev, A. Ezquerro, A. Fabiani, S. Ferrer-Ribas, E. Finelli, F. Fleck, I. Galan, J. Galanti, G. Galaverni, M. Garcia, J. A. Garcia-Barcelo, J. M. Gastaldo, L. Giannotti, M. Giganon, A. Goblin, C. Goyal, N. Gu, Y. Hagge, L. Helary, L. Hengstler, D. Heuchel, D. Hoof, S. Iglesias-Marzoa, R. Iguaz, F. J. Iniguez, C. Irastorza, I. G. Jakovcic, K. Kaefer, D. Kaminski, J. Karstensen, S. Law, M. Lindner, A. Loidl, M. Loiseau, C. Lopez-Alegre, G. Lozano-Guerrero, A. Lubsandorzhiev, B. Luzon, G. Manthos, I. Margalejo, C. Marin-Franch, A. Marques, J. Marutzky, F. Menneglier, C. Mentink, M. Mertens, S. Miralda-Escude, J. Mirallas, H. Muleri, F. Muratova, V. Navarro-Madrid, J. R. Navick, X. F. Nikolopoulos, K. Notari, A. Nozik, A. Obis, L. Ortiz-de-Solorzano, A. O'Shea, T. von Oy, J. Pareschi, G. Papaevangelou, T. Perez, K. Perez, O. Picatoste, E. Pivovaroff, M. J. Porron, J. Puyuelo, M. J. Quintana, A. Redondo, J. Reuther, D. Ringwald, A. Rodrigues, M. Rubini, A. Rueda-Teruel, S. Rueda-Teruel, F. Ruiz-Choliz, E. Ruz, J. Schaffran, J. Schiffer, T. Schmidt, S. Schneekloth, U. Schoenfeld, L. Schott, M. Segui, L. Singh, U. R. Soffitta, P. Spiga, D. Stern, M. Straniero, O. Tavecchio, F. Unzhakov, E. Ushakov, N. A. Vecchi, G. Vogel, J. K. Voronin, D. M. Ward, R. Weltman, A. Wiesinger, C. Wolf, R. Yanes-Diaz, A. Yu, Y.
author_facet	Ahyoune, S. Altenmueller, K. Antolin, I. Basso, S. Brun, P. Candon, F. R. Castel, J. F. Cebrian, S. Chouhan, D. Della Ceca, R. Cervera-Cortes, M. Chernov, V. Civitani, M. M. Cogollos, C. Costa, E. Cotroneo, V. Dafni, T. Derbin, A. Desch, K. Diaz-Martin, M. C. Diaz-Morcillo, A. Diez-Ibanez, D. Pardos, C. Diez Dinter, M. Doebrich, B. Drachnev, I. Dudarev, A. Ezquerro, A. Fabiani, S. Ferrer-Ribas, E. Finelli, F. Fleck, I. Galan, J. Galanti, G. Galaverni, M. Garcia, J. A. Garcia-Barcelo, J. M. Gastaldo, L. Giannotti, M. Giganon, A. Goblin, C. Goyal, N. Gu, Y. Hagge, L. Helary, L. Hengstler, D. Heuchel, D. Hoof, S. Iglesias-Marzoa, R. Iguaz, F. J. Iniguez, C. Irastorza, I. G. Jakovcic, K. Kaefer, D. Kaminski, J. Karstensen, S. Law, M. Lindner, A. Loidl, M. Loiseau, C. Lopez-Alegre, G. Lozano-Guerrero, A. Lubsandorzhiev, B. Luzon, G. Manthos, I. Margalejo, C. Marin-Franch, A. Marques, J. Marutzky, F. Menneglier, C. Mentink, M. Mertens, S. Miralda-Escude, J. Mirallas, H. Muleri, F. Muratova, V. Navarro-Madrid, J. R. Navick, X. F. Nikolopoulos, K. Notari, A. Nozik, A. Obis, L. Ortiz-de-Solorzano, A. O'Shea, T. von Oy, J. Pareschi, G. Papaevangelou, T. Perez, K. Perez, O. Picatoste, E. Pivovaroff, M. J. Porron, J. Puyuelo, M. J. Quintana, A. Redondo, J. Reuther, D. Ringwald, A. Rodrigues, M. Rubini, A. Rueda-Teruel, S. Rueda-Teruel, F. Ruiz-Choliz, E. Ruz, J. Schaffran, J. Schiffer, T. Schmidt, S. Schneekloth, U. Schoenfeld, L. Schott, M. Segui, L. Singh, U. R. Soffitta, P. Spiga, D. Stern, M. Straniero, O. Tavecchio, F. Unzhakov, E. Ushakov, N. A. Vecchi, G. Vogel, J. K. Voronin, D. M. Ward, R. Weltman, A. Wiesinger, C. Wolf, R. Yanes-Diaz, A. Yu, Y.
contents	BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large magnet that is pointing to the sun. The resulting X-rays are focused by appropriate X-ray optics and detected by sensitive low-background detectors placed at the focal spot. The aim of this article is to provide an accurate quantitative description of the different components (such as the magnet, optics, and X-ray detectors) involved in the detection of axions. Our efforts have focused on developing robust and integrated software tools to model these helioscope components, enabling future assessments of modifications or upgrades to any part of the IAXO axion helioscope and evaluating the potential impact on the experiment's sensitivity. In this manuscript, we demonstrate the application of these tools by presenting a precise signal calculation and response analysis of BabyIAXO's sensitivity to the axion-photon coupling. Though focusing on the Primakoff solar flux component, our virtual helioscope model can be used to test different production mechanisms, allowing for direct comparisons within a unified framework.
format	Preprint
id	arxiv_https___arxiv_org_abs_2411_13915
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	An accurate solar axions ray-tracing response of BabyIAXO Ahyoune, S. Altenmueller, K. Antolin, I. Basso, S. Brun, P. Candon, F. R. Castel, J. F. Cebrian, S. Chouhan, D. Della Ceca, R. Cervera-Cortes, M. Chernov, V. Civitani, M. M. Cogollos, C. Costa, E. Cotroneo, V. Dafni, T. Derbin, A. Desch, K. Diaz-Martin, M. C. Diaz-Morcillo, A. Diez-Ibanez, D. Pardos, C. Diez Dinter, M. Doebrich, B. Drachnev, I. Dudarev, A. Ezquerro, A. Fabiani, S. Ferrer-Ribas, E. Finelli, F. Fleck, I. Galan, J. Galanti, G. Galaverni, M. Garcia, J. A. Garcia-Barcelo, J. M. Gastaldo, L. Giannotti, M. Giganon, A. Goblin, C. Goyal, N. Gu, Y. Hagge, L. Helary, L. Hengstler, D. Heuchel, D. Hoof, S. Iglesias-Marzoa, R. Iguaz, F. J. Iniguez, C. Irastorza, I. G. Jakovcic, K. Kaefer, D. Kaminski, J. Karstensen, S. Law, M. Lindner, A. Loidl, M. Loiseau, C. Lopez-Alegre, G. Lozano-Guerrero, A. Lubsandorzhiev, B. Luzon, G. Manthos, I. Margalejo, C. Marin-Franch, A. Marques, J. Marutzky, F. Menneglier, C. Mentink, M. Mertens, S. Miralda-Escude, J. Mirallas, H. Muleri, F. Muratova, V. Navarro-Madrid, J. R. Navick, X. F. Nikolopoulos, K. Notari, A. Nozik, A. Obis, L. Ortiz-de-Solorzano, A. O'Shea, T. von Oy, J. Pareschi, G. Papaevangelou, T. Perez, K. Perez, O. Picatoste, E. Pivovaroff, M. J. Porron, J. Puyuelo, M. J. Quintana, A. Redondo, J. Reuther, D. Ringwald, A. Rodrigues, M. Rubini, A. Rueda-Teruel, S. Rueda-Teruel, F. Ruiz-Choliz, E. Ruz, J. Schaffran, J. Schiffer, T. Schmidt, S. Schneekloth, U. Schoenfeld, L. Schott, M. Segui, L. Singh, U. R. Soffitta, P. Spiga, D. Stern, M. Straniero, O. Tavecchio, F. Unzhakov, E. Ushakov, N. A. Vecchi, G. Vogel, J. K. Voronin, D. M. Ward, R. Weltman, A. Wiesinger, C. Wolf, R. Yanes-Diaz, A. Yu, Y. High Energy Physics - Experiment Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Computational Physics Data Analysis, Statistics and Probability BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large magnet that is pointing to the sun. The resulting X-rays are focused by appropriate X-ray optics and detected by sensitive low-background detectors placed at the focal spot. The aim of this article is to provide an accurate quantitative description of the different components (such as the magnet, optics, and X-ray detectors) involved in the detection of axions. Our efforts have focused on developing robust and integrated software tools to model these helioscope components, enabling future assessments of modifications or upgrades to any part of the IAXO axion helioscope and evaluating the potential impact on the experiment's sensitivity. In this manuscript, we demonstrate the application of these tools by presenting a precise signal calculation and response analysis of BabyIAXO's sensitivity to the axion-photon coupling. Though focusing on the Primakoff solar flux component, our virtual helioscope model can be used to test different production mechanisms, allowing for direct comparisons within a unified framework.
title	An accurate solar axions ray-tracing response of BabyIAXO
topic	High Energy Physics - Experiment Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Computational Physics Data Analysis, Statistics and Probability
url	https://arxiv.org/abs/2411.13915