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Past singularities in phantom theories

Published online by Cambridge University Press:  30 September 2008

L. Fernández-Jambrina*
Affiliation:
E.T.S.I. Navales, Universidad Politécnica de Madrid, Arco de la Victoria s/n, 28040 Madrid, Spain
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Abstract

FLRW models filled with just dark energy are shown to have a finite past, since causal geodesics cannot be extended beyond a certain proper time. It is shown that curvature measured along causal geodesics becomes infinity on travelling to the past, though curvature scalars tend to zero. Furthermore the time measured by free-falling observers from coincidence time to Big Rip is shown to be as short as wished by increasing their linear momentum.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

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References

Barrow, J.D., 2004, Class. Quant. Grav., 21, L79 CrossRef
Caldwell, R.R., 2002, Phys. Lett., B. 545, 23
Cattoën, C., & Visser, M., 2005, Class. Quant. Grav., 22, 4913 CrossRef
Fernández-Jambrina, L., 2007, Phys. Lett. B, 656, 9 CrossRef
Fernández-Jambrina, L., & Lazkoz, R., 2004, Phys. Rev. D, 70, 121503(R) CrossRef
Fernández-Jambrina, L., & Lazkoz, R., 2006, Phys. Rev. D, 74, 064030 CrossRef
Hawking, S.W., & Ellis, G.F.R., The Large Scale Structure of Space-time (Cambridge University Press)
Królak, A., 1986, Class. Quant. Grav., 3, 267 CrossRef
Nojiri, S., Odintsov, S.D., & Tsujikawa, S., 2005, Phys. Rev. D, 71, 063004 CrossRef
Padmanabhan, T., 2005, Curr. Sci., 88, 1057
Tipler, F.J., 1977, Phys. Lett., A, 64, 8