Abstract
Extending a technique developed for static fields by Janiset al. [10] to the nonstatic fields two exact solutions in the case of Einstein-Rosen metric for the interacting electromagnetic and zero mass scalar fields have been obtained.
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References
Datta Majumdar, S.: Phys. Rev.72, 390 (1947).
Misra, M., Radhakrishna, L.: Proc. Nat. Inst. Sci. India, Part A,28, 632 (1962).
Harrison, B. K.: Phys. Rev.138 B, 488 (1965).
Buchdahl, H.: Quart. J. Maths.5, 116 (1954).
Buchdahl, H.: Aust. J. Phys.9, 13 (1956).
Buchdahl, H.: Nuovo Cimento Ser. X,5, 1083 (1957).
Buchdahl, H.: Phys. Rev.115, 1325 (1959).
Bandyopadhyay, G.: J. Math. Mech.12, 655 (1963).
Rao, J. R., Tiwari, R. N.: Communicated for publication.
Janis, A. I., Robinson, D. C., Winicour, J.: Phys. Rev.186, 1729 (1969).
Rao, J. R., Roy, A. R., Tiwari, R. N.: Ann. Phys.69, 473 (1972).
Levi-Civita, T.: R. C. Acad. Lincei,28i, 101 (1919).
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Roy, A.R., Datta, C.R. Time dependent axially symmetric solutions of the Einstein-Maxwell-Yukawa fields. Commun.Math. Phys. 29, 285–292 (1973). https://doi.org/10.1007/BF01646131
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DOI: https://doi.org/10.1007/BF01646131