Email this article 
Light-shining-through-wall cavity setups for probing alps
- Authors: Salnikov D.1,2, Satunin P.1,2, Fitkevich M.1,3, Kirpichnikov D.V1
-
Affiliations:
- Institute for Nuclear Research of the Russian Academy of Sciences
- Lomonosov Moscow State University
- Moscow Institute of Physics and Technology
- Issue: Vol 117, No 11-12 (6) (2023)
- Pages: 892-893
- Section: Articles
- URL: https://cardiosomatics.ru/0370-274X/article/view/663153
- DOI: https://doi.org/10.31857/S1234567823120030
- EDN: https://elibrary.ru/EUTEAX
- ID: 663153
Cite item
Open Access
Access granted
Subscription or Fee Access
Abstract
We discuss the aspects of axion-like-particles searches with Light-Shining-through-Wall experimental setups consisted of two radio-frequency cavities. We compare the efficiencies of four setups which involve the cavity pump modes and external magnetic fields. Additionally, we discuss the sensitivity dependence both on the relative position of two cylindrical cavities and on their radius-to-length ratio.
About the authors
D. Salnikov
Institute for Nuclear Research of the Russian Academy of Sciences; Lomonosov Moscow State University
Email: letters@kapitza.ras.ru
P. Satunin
Institute for Nuclear Research of the Russian Academy of Sciences; Lomonosov Moscow State University
Email: letters@kapitza.ras.ru
M. Fitkevich
Institute for Nuclear Research of the Russian Academy of Sciences; Moscow Institute of Physics and Technology
Email: letters@kapitza.ras.ru
D. V Kirpichnikov
Institute for Nuclear Research of the Russian Academy of Sciences
Author for correspondence.
Email: letters@kapitza.ras.ru
References
- R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38, 1440 (1977).
- P. Svrcek and E. Witten, JHEP 06, 051 (2006), hepth/0605206.
- J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. B 120, 127 (1983).
- L. F. Abbott and P. Sikivie, Phys. Lett. B 120, 133 (1983).
- M. Dine and W. Fischler, Phys. Lett. B 120, 137 (1983).
- V. Anastassopoulos, S. Aune, K. Barth et al. (CAST collaboration), Nature Phys. 13, 584 (2017); 1705.02290.
- I. G. Irastorza and J. Redondo, Prog. Part. Nucl. Phys. 102, 89 (2018); 1801.08127.
- P. Sikivie, Phys. Rev. Lett. 51, 1415 (1983), Erratum: Phys. Rev. Lett. 52, 695 (1984).
- A. A. Anselm, Yad. Fiz. 42, 1480 (1985).
- F. Hoogeveen, Phys. Lett. B 288, 195 (1992).
- K. Ehret, M. Frede, S. Ghazaryan et al. (Collaboration), Phys. Lett. B 689, 149 (2010); 1004.1313.
- M. Betz, F. Caspers, M. Gasior, M. Thumm, and S. W. Rieger, Phys. Rev. D 88, 075014 (2013), 1310.8098.
- M. Ortiz, J. Gleason, H. Grote et al. (Collaboration), Phys. Dark Univ. 35, 100968 (2022); 2009.14294.
- A. Berlin, S. Belomestnykh, D. Blas et al. (Collaboration), (2022), 2203.12714.
- C. Gao and R. Harnik, JHEP 07, 053 (2021), 2011.01350.
- D. Salnikov, P. Satunin, D. V. Kirpichnikov, and M. Fitkevich, JHEP 03, 143 (2021); 2011.12871.
Supplementary files
