Gravitational Faraday rotation in a weak gravitational field

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 69, Issue 8, 2004, Pages 4-

  Sereno, Mauro ^a,b  

^a UNIVERSITY OF NAPLES FEDERICO II   (Italy)

^b INFN SEZIONE DI NAPOLI   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 2442715081     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.087501     Document Type: Article

References (22)

1. C. Misner, K.S. Thorne, and J.A. Wheeler, Gravitation (Freeman, San Francisco, 1973).
2. A.O. Petters, H. Levine, and J. Wambsganss, Singularity Theory and Gravitational Lensing (Birkhäuser, Boston, 2001).
3. P. Schneider, J.J. Ehlers, and E.E. Falco, Gravitational Lenses (Springer, Berlin, 1992).
4. T. Piran and P.N. Safier, Nature (London) 318, 271 (1985).
5. G.B. Skrotskii, Dokl. Akad. Nauk SSSR 114, 73 (1957).
6. S.M. Rytov, C. R. (Dokl.) Acad. Sci. URSS 18, 263 (1938).
7. N.L. Balazs, Phys. Rev. 110, 236 (1958).
8. J. Plebanski, Phys. Rev. 118, 1396 (1960).
9. B.B. Godfrey, Phys. Rev. D 1, 2721 (1970).
10. F.S.O. Su and R.L. Mallett, Astrophys. J. 238, 1111 (1980).
11. P.A. Connors, T. Piran, and R.F. Stark, Astrophys. J. 235, 224 (1980).
12. S. Kopeikin and B. Mashoon, Phys. Rev. D 65, 064025 (2002).
13. H. Ishihara, M. Takahashi, and A. Tomimatsu, Phys. Rev. D 38, 472 (1988).
14. M. Nouri-Zonoz, Phys. Rev. D 60, 024013 (1999).
15. L.D. Landau and E.M. Lifshits, Teoria dei Campi (Editori Riuniti, Roma, 1985).
16. B. Mashoon, Phys. Rev. D 11, 2679 (1975).
17. M. Sereno, Phys. Rev. D 67, 064007 (2003).
18. I. Ciufolini, S. Kopeikin, B. Mashoon, and F. Ricci, Phys. Lett. A 308, 101 (2003).
19. M. Sereno, in preparation.
20. A.D. Biggs, I.W.A. Browne, P. Helbig, L.V.E. Koopmans, P.N. Wilkinson, and R.A. Perley, Mon. Not. R. Astron. Soc. 304, 349 (1999).
21. Latin indices run from 1 to 3, whereas Greek indices run from 0 to 3.
22. The controvariant components of spatial three-vectors are equal to the spatial components of the corresponding four-vectors. Operations on such three-vectors are defined in the three-dimensional space with metric (Formula presented)