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If axions or axion-like particles exist and are detected, they will not only extend the standard model of particle physics but will also open a new way to probe their sources.
1904
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2015
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2015
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S. Basu, “The Solar Metallicity Problem: What is the Solution?,” in “Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology,” Proceedings of Astronomical Society of the Pacific Conference Series, 2009
2009
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2010
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2011
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2012
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2012
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C. Blancard, P. Cossé and G. Faussurier, “Solar Mixture Opacity Calculations Using Detailed Configuration and Level Accounting Treatments.” Astrophysical Journal 745
2012
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I. G. Irastorza et al
2013
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2016
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2016
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2017
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2017
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2017
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2017
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2017
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2017
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2018
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2018
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S. Kempf, A. Fleischmann, L. Gastaldo and C. Enss, “Physics and Applications of Metallic Magnetic Calorimeters,” J Low Temp Phys 193
2018
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2018
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S. Vagnozzi, “New solar metallicity measurements,” Atoms 7
2019
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J. Jaeckel and L. J. Thormaehlen, “Distinguishing Axion Models with IAXO,” JCAP 1903
2019
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2019
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