Physics potential of the International Axion Observatory (IAXO)

We review 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...

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Detalles Bibliográficos
Autores principales: 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., Ortiz de Solórzano, A., 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., ten Kate, H., Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J.K., Weinsheimer, C., Weltman, A., Yin, W.
Lenguaje:eng
Publicado: 2019
Materias:
hep-ex
Particle Physics - Experiment
hep-ph
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2019/06/047
http://cds.cern.ch/record/2672353
_version_ 1780962454952476672
author 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.
Ortiz de Solórzano, A.
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.
ten Kate, H.
Tkachev, I.
Troitsky, S.
Unzhakov, E.
Vedrine, P.
Vogel, J.K.
Weinsheimer, C.
Weltman, A.
Yin, W.
author_facet 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.
Ortiz de Solórzano, A.
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.
ten Kate, H.
Tkachev, I.
Troitsky, S.
Unzhakov, E.
Vedrine, P.
Vogel, J.K.
Weinsheimer, C.
Weltman, A.
Yin, W.
author_sort Armengaud, E.
collection CERN
description We review 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. At the same time, 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. In addition, 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.
id cern-2672353
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-26723532022-07-28T07:21:53Zdoi:10.1088/1475-7516/2019/06/047http://cds.cern.ch/record/2672353engArmengaud, 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.Ortiz de Solórzano, A.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.ten Kate, H.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)hep-exParticle Physics - Experimenthep-phParticle Physics - PhenomenologyWe review 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. At the same time, 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. In addition, 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.We review 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 $g_{a\gamma}\sim 10^{-12}$ GeV$^{-1}$, or to electrons $g_{ae}\sim$10$^{-13}$, IAXO has the potential to find the QCD axion in the 1 meV$\sim$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. At the same time, 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. In addition, 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.arXiv:1904.09155oai:cds.cern.ch:26723532019-04-19
spellingShingle hep-ex
Particle Physics - Experiment
hep-ph
Particle Physics - Phenomenology
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.
Ortiz de Solórzano, A.
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.
ten Kate, H.
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)
title Physics potential of the International Axion Observatory (IAXO)
title_full Physics potential of the International Axion Observatory (IAXO)
title_fullStr Physics potential of the International Axion Observatory (IAXO)
title_full_unstemmed Physics potential of the International Axion Observatory (IAXO)
title_short Physics potential of the International Axion Observatory (IAXO)
title_sort physics potential of the international axion observatory (iaxo)
topic hep-ex
Particle Physics - Experiment
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/1475-7516/2019/06/047
http://cds.cern.ch/record/2672353
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