You need not be afraid of phantom energy
By P. Gonzalez-diaz. 2003
204 citations recorded by the source corpus.
The author thanks Mariam Bouhmadi and Carmen L. Sigu¨enza for useful conversations. This work was supported by MCYT under Research Project No. BMF2002-03758.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/1dffd959ac550ed9989f4f0ef4bf2923e21a1795
How researchers see this paper
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In Astronomy and Astrophysics
- Emmanuel N. Saridakis
- Francisco S. N. Lobo
- H. K. Jassal
- J. Bagla
- Thanu Padmanabhan
- Tiberiu Harko
- Salvatore Capozziello
- Sergei D. Odintsov
In Nuclear and High Energy Physics
- Emmanuel N. Saridakis
- H. K. Jassal
- J. Bagla
- Francisco S. N. Lobo
- Thanu Padmanabhan
- Salvatore Capozziello
- Sergei D. Odintsov
- Tiberiu Harko
In Statistical and Nonlinear Physics
- Emmanuel N. Saridakis
- Thanu Padmanabhan
- Francisco S. N. Lobo
- H. K. Jassal
- J. Bagla
- T.Padmanabhan
- R. Cai
- Li-Ming Cao
Citations in the corpus
- Phantom energy traversable wormholes (2005, background): “However, it has been shown that in certain models the presence of phantom energy does not lead to the above-mentioned doomsday [19, 20, 21, 22, 23, 24].”
- WMAP constraints on low redshift evolution of dark energy (2004, background): “…& Lazkoz 2004; Gorini et al. 2004), phantom fields (Caldwell 2002; Carroll et al. 2003; Dabrowski et al. 2003; Frampton 2003; Gibbons 2003b; Gonzalez-Diaz 2003b; Hao E-mail: hkj@mri.ernet.in (HKJ); jasjeet@mri.ernet.in (JSB); nabhan@iucaa.ernet.in (TP) & Li 2003a,b; Nojiri & Odinstov 2003;…”