Abstract
An exact solution of Einstein’s equations is interpreted as describing the gravitational field of a tachyon in a de Sitter universe. Switching off the cosmological constant yields the gravitational field of a tachyon in flat spacetime background.
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O M P Bilaniuk, V K Deshpande and E C G Sudarshan,Am. J. Phys. 30 718 (1962)
M E Arons and E C G Sudarshan,Phys. Rev. 173 1622 (1968)
O M P Bilaniuk and E C G Sudarshan,Phys. Today 5 43 (1969)
J Dhar and E C G Sudarshan,Phys. Rev. 174 1808 (1968)
G Fienberg,Phys. Rev. 159, 1089 (1967)
E Recami,Riv. Nuovo Cimento 9 1 (1986)
J V Narlikar and E C G Sudarshan,Mon. Not. R. Astron. Soc. 175 105 (1976)
J V Narlikar and S V Dhurandhar,Pramana — J. Phys. 6 388 (1976)
S V Dhurandhar,Phys. Rev. D19 2310 (1979)
P C Vaidya,Curr. Sci. 40 651 (1971)
X Chongming, W Xuejun and H Zhum,Gen. Relativ. Gravit. 19 1203 (1987)
R L Mallet,Phys. Rev. D31 416 (1985)
R L Mallet,Phys. Lett. A126 226 (1988)
A Patino and H Rago,Phys. Lett. A121 329 (1987)
D Vick,Lett. Nuovo Cimento 44 127 (1985)
C Xu, C L Shen and X Wu,Phys. Lett. A130 1 (1988)
R Resnick,Introduction to special relativity (Wiley Eastern, New Delhi) p. 84
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Virbhadra, K.S. Gravitational field of a tachyon in a de Sitter universe. Pramana - J Phys 40, 273–275 (1993). https://doi.org/10.1007/BF02845846
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DOI: https://doi.org/10.1007/BF02845846