Klaus Barth, Alexander Belov, Berta Beltran, Heinrich Bräuninger, José Manuel Carmona, Juan I. Collar, Theopisti Dafni, Martyn Davenport, Luigi Di Lella, Christos Eleftheriadis, Jakob Englhauser, George Fanourakis, Ester Ferrer-Ribas, Horst Fischer, Jürgen Franz, Peter Friedrich, Javier Galán, J. A. García, Theodoros Geralis, Ioanis Giomataris, Sergei Gninenko, Héctor Gómez, Michael D. Hasinoff, Fritz-Herbert Heinsius, Dieter H. H. Hoffmann, Igor Garcia Irastorza, Joachim Jacoby, Kresimir Jakovčić, Donghwa Kang, Kay Königsmann, Rainer Kotthaus, Konstantinos Kousouris, Milica Krčmar, M. Kuster, Biljana Lakić, Anastasios Liolios, Ante Ljubičić, Gerhard Lutz, Gloria Luzón, David W. Miller, Thomas Papaevangelou, Mike J. Pivovaroff, Georg Raffelt, Javier Redondo, Hans Riege, A. Rodríguez, Jaime Ruz, Ilias Savvidis, Yannis Semertzidis, Laura Stewart, Karl van Bibber, Joaquin D. Vieira, José A. Villar, Julia K. Vogel, Louis Walckiers, Konstantin Zioutas
- In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axiorecombination, the "BCA processes." Based on a new calculation of this flux, including for the first time axio-recombination, we derive limits on the axion-electron Yukawa coupling gae and axion-photon interaction strength ga using the CAST phase-I data (vacuum phase). For ma <~ 10 meV/c2 we find ga gae < 8.1 × 10−23 GeV−1 at 95% CL. We stress that a next-generation axion helioscope such as the proposed IAXO could push this sensitivity into a range beyond stellar energy-loss limits and test the hypothesis that white-dwarf cooling is dominated by axion emission.
Metadaten| Verfasserangaben: | Klaus Barth, Alexander Belov, Berta Beltran, Heinrich Bräuninger, José Manuel Carmona, Juan I. Collar, Theopisti Dafni, Martyn Davenport, Luigi Di Lella, Christos EleftheriadisORCiD, Jakob Englhauser, George Fanourakis, Ester Ferrer-Ribas, Horst Fischer, Jürgen Franz, Peter Friedrich, Javier Galán, J. A. García, Theodoros Geralis, Ioanis Giomataris, Sergei Gninenko, Héctor Gómez, Michael D. Hasinoff, Fritz-Herbert HeinsiusORCiDGND, Dieter H. H. HoffmannORCiDGND, Igor Garcia Irastorza, Joachim JacobyGND, Kresimir Jakovčić, Donghwa KangORCiDGND, Kay Königsmann, Rainer Kotthaus, Konstantinos Kousouris, Milica Krčmar, M. Kuster, Biljana Lakić, Anastasios Liolios, Ante Ljubičić, Gerhard Lutz, Gloria Luzón, David W. Miller, Thomas Papaevangelou, Mike J. Pivovaroff, Georg Raffelt, Javier Redondo, Hans Riege, A. Rodríguez, Jaime Ruz, Ilias Savvidis, Yannis Semertzidis, Laura Stewart, Karl van Bibber, Joaquin D. Vieira, José A. Villar, Julia K. Vogel, Louis Walckiers, Konstantin Zioutas |
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| URN: | urn:nbn:de:hebis:30:3-259158 |
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| DOI: | https://doi.org/10.1088/1475-7516/2013/05/010 |
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| ISSN: | 1475-7516 |
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| ArXiv-Id: | http://arxiv.org/abs/1302.6283 |
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| Titel des übergeordneten Werkes (Englisch): | Journal of cosmology and astroparticle physics |
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| Verlag: | IOP |
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| Verlagsort: | London |
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| Dokumentart: | Wissenschaftlicher Artikel |
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| Sprache: | Englisch |
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| Datum der Veröffentlichung (online): | 09.05.2013 |
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| Datum der Erstveröffentlichung: | 09.05.2013 |
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| Veröffentlichende Institution: | Universitätsbibliothek Johann Christian Senckenberg |
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| Datum der Freischaltung: | 14.06.2013 |
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| Freies Schlagwort / Tag: | axions; dark matter experiments; solar physics; white and brown dwarfs |
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| Jahrgang: | 2013 |
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| Ausgabe / Heft: | 5 |
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| Seitenzahl: | 17 |
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| Bemerkung: | c 2013 IOP Publishing Ltd and Sissa Medialab srl. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
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| HeBIS-PPN: | 347115691 |
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| Institute: | Physik / Physik |
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| DDC-Klassifikation: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
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| PACS-Klassifikation: | 10.00.00 THE PHYSICS OF ELEMENTARY PARTICLES AND FIELDS (for experimental methods and instrumentation for elementary-particle physics, see section 29) / 14.00.00 Properties of specific particles / 14.80.-j Other particles (including hypothetical) / 14.80.Mz Axions and other Nambu-Goldstone bosons (Majorons, familons, etc.) |
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| 90.00.00 GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS (for more detailed headings, see the Geophysics Appendix) / 97.00.00 Stars (for relativistic stars, see 04.40.Dg in general relativity and gravitation) / 97.10.-q Stellar characteristics and properties (see also section 26 Nuclear astrophysics) / 97.10.Ld Magnetic and electric fields; polarization of starlight |
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| 90.00.00 GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS (for more detailed headings, see the Geophysics Appendix) / 97.00.00 Stars (for relativistic stars, see 04.40.Dg in general relativity and gravitation) / 97.10.-q Stellar characteristics and properties (see also section 26 Nuclear astrophysics) / 97.10.Me Mass loss and stellar winds |
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| 90.00.00 GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS (for more detailed headings, see the Geophysics Appendix) / 97.00.00 Stars (for relativistic stars, see 04.40.Dg in general relativity and gravitation) / 97.20.-w Normal stars (by class): general or individual / 97.20.Rp Faint blue stars (including blue stragglers), white dwarfs, degenerate stars, nuclei of planetary nebulae (for planetary nebulae, see 98.38.Ly or 98.58.Li) |
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| Sammlungen: | Universitätspublikationen |
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| Lizenz (Deutsch): |  Creative Commons - Namensnennung 3.0 |
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