English

Solar Kaluza-Klein axion search with NEWS-G

High Energy Physics - Experiment 2022-01-11 v2 Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics

Abstract

Kaluza-Klein (KK) axions appear in theories with extra dimensions as higher mass, significantly shorter lifetime, excitations of the Peccei-Quinn axion. When produced in the Sun, they would remain gravitationally trapped in the solar system, and their decay to a pair of photons could provide an explanation of the solar corona heating problem. A low-density detector would discriminate such a signal from the background, by identifying the separation of the interaction point of the two photons. The NEWS-G collaboration uses large volume Spherical Proportional Counters, gas-filled metallic spheres with a spherical anode in their centre. After observation of a single axionlike event in a 42 day long run with the SEDINE detector, a 90%90\% C.L. upper limit of gaγγ<8.991013GeV1g_{a\gamma\gamma}<8.99\cdot10^{-13}\,GeV^{-1} is set on the axion-photon coupling for a KK axion density on Earth of na=4.071013m3n_{a}=4.07\cdot10^{13}\,m^{-3} and two extra dimensions of size R=1eV1R = 1\,eV^{-1}.

Keywords

Cite

@article{arxiv.2109.03562,
  title  = {Solar Kaluza-Klein axion search with NEWS-G},
  author = {G collaboration and Q. Arnaud and L. Balogh and C. Beaufort and A. Brossard and J. -F. Caron and M. Chapellier and J. -M. Coquillat and E. C. Corcoran and S. Crawford and A. Dastgheibi-Fard and Y. Deng and K. Dering and D. Durnford and C. Garrah and G. Gerbier and I. Giomataris and G. Giroux and P. Gorel and M. Gros and P. Gros and O. Guillaudin and E. W. Hoppe and I. Katsioulas and F. Kelly and P. Knights and S. Langrock and P. Lautridou and R. D. Martin and J. -P. Mols and J. -F. Muraz and T. Neep and K. Nikolopoulos and P. O'Brien and M. -C. Piro and D. Santos and G. Savvidis and I. Savvidis and F. A. Vazquez de Sola Fernandez and M. Vidal and R. Ward and M. Zampaolo},
  journal= {arXiv preprint arXiv:2109.03562},
  year   = {2022}
}

Comments

19 pages, 11 figures. Updated with additional details requested during review for publication in PRD and mild relaxation of final constraint