Search for solar axions via axion-photon coupling with the Majorana Demonstrator

التفاصيل البيبلوغرافية
العنوان: Search for solar axions via axion-photon coupling with the Majorana Demonstrator
المؤلفون: Arnquist, I. J., Avignone III, F. T., Barabash, A. S., Barton, C. J., Bhimani, K. H., Blalock, E., Bos, B., Busch, M., Buuck, M., Caldwell, T. S., Chan, Y-D., Christofferson, C. D., Chu, P. -H., Clark, M. L., Cuesta, C., Detwiler, J. A., Efremenko, Yu., Ejiri, H., Elliott, S. R., Giovanetti, G. K., Green, M. P., Gruszko, J., Guinn, I. S., Guiseppe, V. E., Haufe, C. R., Henning, R., Aguilar, D. Hervas, Hoppe, E. W., Hostiuc, A., Kidd, M. F., Kim, I., Kouzes, R. T., Lannen V, T. E., Li, A., Lopez, A. M., López-Castaño, J. M., Martin, E. L., Martin, R. D., Massarczyk, R., Meijer, S. J., Oli, T. K., Othman, G., Paudel, L. S., Pettus, W., Poon, A. W. P., Radford, D. C., Reine, A. L., Rielage, K., Ruof, N. W., Schaper, D. C., Tedeschi, D., Varner, R. L., Vasilyev, S., Wilkerson, J. F., Wiseman, C., Xu, W., Yu, C. -H., Zhu, B. X.
المصدر: Physical Review Letters 129, 081803 (2022)
سنة النشر: 2022
المجموعة: High Energy Physics - Experiment
Nuclear Experiment
مصطلحات موضوعية: Nuclear Experiment, High Energy Physics - Experiment
الوصف: Axions were originally proposed to explain the strong-CP problem in QCD. Through the axion-photon coupling, the Sun could be a major source of axions, which could be measured in solid state detection experiments with enhancements due to coherent Primakoff-Bragg scattering. The Majorana Demonstrator experiment has searched for solar axions with a set of $^{76}$Ge-enriched high purity germanium detectors using a 33 kg-yr exposure collected between Jan. 2017 and Nov. 2019. A temporal-energy analysis gives a new limit on the axion-photon coupling as $g_{a\gamma}<1.45\times 10^{-9}$ GeV$^{-1}$ (95% C.I.) for axions with mass up to 100 eV/$c^2$. This improves laboratory-based limits between about 1 eV/$c^2$ and 100 eV/$c^2$.
Comment: Minor updates to match published version
نوع الوثيقة: Working Paper
DOI: 10.1103/PhysRevLett.129.081803
URL الوصول: http://arxiv.org/abs/2206.05789
رقم الانضمام: edsarx.2206.05789
قاعدة البيانات: arXiv
الوصف
DOI:10.1103/PhysRevLett.129.081803