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Title: Physics potential of the International Axion Observatory (IAXO)

Abstract

We report on the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO) . Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as g ~ 10 –12 GeV –1, or to electrons g ae~10 –13, IAXO has the potential to find the QCD axion in the 1 meV~1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. Similarly, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous "transparency" of the Universe to gamma-rays, 2) the observed soft X-ray excess from galaxy clusters or 3) some inflationary models. Furthermore, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums.

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org.:
USDOE; European Research Council (ERC)
Contributing Org.:
[IAXO collaboration]
OSTI Identifier:
1547283
Grant/Contract Number:  
[AC02-76SF00515]
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Cosmology and Astroparticle Physics
Additional Journal Information:
[ Journal Volume: 2019; Journal Issue: 06]; Journal ID: ISSN 1475-7516
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Armengaud, E., Attié, D., Basso, S., Brun, P., Bykovskiy, N., Carmona, J. M., Castel, J. F., Cebrián, S., Cicoli, M., Civitani, M., Cogollos, C., Conlon, J. P., Costa, D., Dafni, T., Daido, R., Derbin, A. V., Descalle, M. A., Desch, K., Dratchnev, I. S., Döbrich, B., Dudarev, A., Ferrer-Ribas, E., Fleck, I., Galán, J., Galanti, G., Garrido, L., Gascon, D., Gastaldo, L., Germani, C., Ghisellini, G., Giannotti, M., Giomataris, I., Gninenko, S., Golubev, N., Graciani, R., Irastorza, I. G., Jakovčić, K., Kaminski, J., Krčmar, M., Krieger, C., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Lomskaya, I., Lubsandorzhiev, B., Luzón, G., Marsh, M. C. D., Margalejo, C., Mescia, F., Meyer, M., Miralda-Escudé, J., Mirallas, H., Muratova, V. N., Navick, X. F., Nones, C., Notari, A., Nozik, A., de Solórzano, A. Ortiz, Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Picatoste, E., Pivovaroff, M. J., Redondo, J., Ringwald, A., Roncadelli, M., Ruiz-Chóliz, E., Ruz, J., Saikawa, K., Salvadó, J., Samperiz, M. P., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Silva, H., Tagliaferri, G., Takahashi, F., Tavecchio, F., Kate, H. ten, Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J. K., Weinsheimer, C., Weltman, A., and Yin, W. Physics potential of the International Axion Observatory (IAXO). United States: N. p., 2019. Web. doi:10.1088/1475-7516/2019/06/047.
Armengaud, E., Attié, D., Basso, S., Brun, P., Bykovskiy, N., Carmona, J. M., Castel, J. F., Cebrián, S., Cicoli, M., Civitani, M., Cogollos, C., Conlon, J. P., Costa, D., Dafni, T., Daido, R., Derbin, A. V., Descalle, M. A., Desch, K., Dratchnev, I. S., Döbrich, B., Dudarev, A., Ferrer-Ribas, E., Fleck, I., Galán, J., Galanti, G., Garrido, L., Gascon, D., Gastaldo, L., Germani, C., Ghisellini, G., Giannotti, M., Giomataris, I., Gninenko, S., Golubev, N., Graciani, R., Irastorza, I. G., Jakovčić, K., Kaminski, J., Krčmar, M., Krieger, C., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Lomskaya, I., Lubsandorzhiev, B., Luzón, G., Marsh, M. C. D., Margalejo, C., Mescia, F., Meyer, M., Miralda-Escudé, J., Mirallas, H., Muratova, V. N., Navick, X. F., Nones, C., Notari, A., Nozik, A., de Solórzano, A. Ortiz, Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Picatoste, E., Pivovaroff, M. J., Redondo, J., Ringwald, A., Roncadelli, M., Ruiz-Chóliz, E., Ruz, J., Saikawa, K., Salvadó, J., Samperiz, M. P., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Silva, H., Tagliaferri, G., Takahashi, F., Tavecchio, F., Kate, H. ten, Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J. K., Weinsheimer, C., Weltman, A., & Yin, W. Physics potential of the International Axion Observatory (IAXO). United States. doi:10.1088/1475-7516/2019/06/047.
Armengaud, E., Attié, D., Basso, S., Brun, P., Bykovskiy, N., Carmona, J. M., Castel, J. F., Cebrián, S., Cicoli, M., Civitani, M., Cogollos, C., Conlon, J. P., Costa, D., Dafni, T., Daido, R., Derbin, A. V., Descalle, M. A., Desch, K., Dratchnev, I. S., Döbrich, B., Dudarev, A., Ferrer-Ribas, E., Fleck, I., Galán, J., Galanti, G., Garrido, L., Gascon, D., Gastaldo, L., Germani, C., Ghisellini, G., Giannotti, M., Giomataris, I., Gninenko, S., Golubev, N., Graciani, R., Irastorza, I. G., Jakovčić, K., Kaminski, J., Krčmar, M., Krieger, C., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Lomskaya, I., Lubsandorzhiev, B., Luzón, G., Marsh, M. C. D., Margalejo, C., Mescia, F., Meyer, M., Miralda-Escudé, J., Mirallas, H., Muratova, V. N., Navick, X. F., Nones, C., Notari, A., Nozik, A., de Solórzano, A. Ortiz, Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Picatoste, E., Pivovaroff, M. J., Redondo, J., Ringwald, A., Roncadelli, M., Ruiz-Chóliz, E., Ruz, J., Saikawa, K., Salvadó, J., Samperiz, M. P., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Silva, H., Tagliaferri, G., Takahashi, F., Tavecchio, F., Kate, H. ten, Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J. K., Weinsheimer, C., Weltman, A., and Yin, W. Mon . "Physics potential of the International Axion Observatory (IAXO)". United States. doi:10.1088/1475-7516/2019/06/047.
@article{osti_1547283,
title = {Physics potential of the International Axion Observatory (IAXO)},
author = {Armengaud, E. and Attié, D. and Basso, S. and Brun, P. and Bykovskiy, N. and Carmona, J. M. and Castel, J. F. and Cebrián, S. and Cicoli, M. and Civitani, M. and Cogollos, C. and Conlon, J. P. and Costa, D. and Dafni, T. and Daido, R. and Derbin, A. V. and Descalle, M. A. and Desch, K. and Dratchnev, I. S. and Döbrich, B. and Dudarev, A. and Ferrer-Ribas, E. and Fleck, I. and Galán, J. and Galanti, G. and Garrido, L. and Gascon, D. and Gastaldo, L. and Germani, C. and Ghisellini, G. and Giannotti, M. and Giomataris, I. and Gninenko, S. and Golubev, N. and Graciani, R. and Irastorza, I. G. and Jakovčić, K. and Kaminski, J. and Krčmar, M. and Krieger, C. and Lakić, B. and Lasserre, T. and Laurent, P. and Limousin, O. and Lindner, A. and Lomskaya, I. and Lubsandorzhiev, B. and Luzón, G. and Marsh, M. C. D. and Margalejo, C. and Mescia, F. and Meyer, M. and Miralda-Escudé, J. and Mirallas, H. and Muratova, V. N. and Navick, X. F. and Nones, C. and Notari, A. and Nozik, A. and de Solórzano, A. Ortiz and Pantuev, V. and Papaevangelou, T. and Pareschi, G. and Perez, K. and Picatoste, E. and Pivovaroff, M. J. and Redondo, J. and Ringwald, A. and Roncadelli, M. and Ruiz-Chóliz, E. and Ruz, J. and Saikawa, K. and Salvadó, J. and Samperiz, M. P. and Schiffer, T. and Schmidt, S. and Schneekloth, U. and Schott, M. and Silva, H. and Tagliaferri, G. and Takahashi, F. and Tavecchio, F. and Kate, H. ten and Tkachev, I. and Troitsky, S. and Unzhakov, E. and Vedrine, P. and Vogel, J. K. and Weinsheimer, C. and Weltman, A. and Yin, W.},
abstractNote = {We report on the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO) . Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as gaγ~ 10–12 GeV–1, or to electrons gae~10–13, IAXO has the potential to find the QCD axion in the 1 meV~1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. Similarly, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous "transparency" of the Universe to gamma-rays, 2) the observed soft X-ray excess from galaxy clusters or 3) some inflationary models. Furthermore, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums.},
doi = {10.1088/1475-7516/2019/06/047},
journal = {Journal of Cosmology and Astroparticle Physics},
number = [06],
volume = [2019],
place = {United States},
year = {2019},
month = {6}
}

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