- Letter
- Open Access
Geometric optics in the presence of axionlike particles in curved spacetime
Phys. Rev. D 103, L081306 – Published 27 April, 2021
DOI: https://doi.org/10.1103/PhysRevD.103.L081306
Abstract
We present a concise derivation of geometric optics in the presence of axionic fields in a curved spacetime. Whenever light can be described via geometric optics (the eikonal approximation), the only difference to the situation without axionic field is the phenomenon of achromatic birefringence. Consequently, redshift of light and distance estimates based on propagating light rays, as well as shear and magnification due to gravitational lensing are not affected by the interaction of light with an axionic field.
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References (27)
- J. Ipser and P. Sikivie, Phys. Rev. Lett. 50, 925 (1983).
- F. W. Stecker and Q. Shafi, Phys. Rev. Lett. 50, 928 (1983).
- J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. 120B, 127 (1983).
- L. F. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
- M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
- P. Sikivie and Q. Yang, Phys. Rev. Lett. 103, 111301 (2009).
- J. E. Kim and G. Carosi, Rev. Mod. Phys. 82, 557 (2010); 91, 049902(E) (2019).
- G. Sigl and P. Trivedi, arXiv:1811.07873.
- T. Fujita, R. Tazaki, and K. Toma, Phys. Rev. Lett. 122, 191101 (2019).
- M. M. Ivanov, Y. Y. Kovalev, M. L. Lister, A. G. Panin, A. B. Pushkarev, T. Savolainen, and S. V. Troitsky, J. Cosmol. Astropart. Phys. 02 (2019) 059.
- S. Chigusa, T. Moroi, and K. Nakayama, Phys. Lett. B 803, 135288 (2020).
- Y. Chen, J. Shu, X. Xue, Q. Yuan, and Y. Zhao, Phys. Rev. Lett. 124, 061102 (2020).
- A. Basu, J. Goswami, D. J. Schwarz, and Y. Urakawa, arXiv:2007.01440.
- L. D. Landau and E. M. Lifshitz, Klassische Feldtheorie, Lehrbuch der Theoretischen Physik, Band 2 (Akademie-Verlag, Berlin, 1987).
- I. I. Tkachev, Phys. Lett. B 191, 41 (1987).
- A. Caputo, M. Regis, M. Taoso, and S. J. Witte, J. Cosmol. Astropart. Phys. 03 (2019) 027.
- A. Arza and P. Sikivie, Phys. Rev. Lett. 123, 131804 (2019).
- D. G. Levkov, A. G. Panin, and I. I. Tkachev, Phys. Rev. D 102, 023501 (2020).
- D. Harari and P. Sikivie, Phys. Lett. B 289, 67 (1992).
- D. Blas, A. Caputo, M. M. Ivanov, and L. Sberna, Phys. Dark Universe 27, 100428 (2020).
- M. A. Fedderke, P. W. Graham, and S. Rajendran, Phys. Rev. D 100, 015040 (2019).
- I. M. H. Etherington, Philos. Mag. 15, 761 (1933).
- R. Sachs, Proc. R. Soc. Ser. A 264, 309 (1961).
Note that for , the last term in Eq. (8) would actually be of order ; therefore, our approximation does not capture the resonant case. For flat spacetimes, a similar ansatz has been worked out in Ref. [18].
- J. I. McDonald and L. B. Ventura, Phys. Rev. D 101, 123503 (2020).
- C. L. Carilli and G. B. Taylor, Annu. Rev. Astron. Astrophys. 40, 319 (2002).
- T. Akahori and D. Ryu, Astrophys. J. 723, 476 (2010).