Tracking and coupled dark energy as seen by the Wilkinson Microwave Anisotropy Probe
By Luca Amendola, C. Quercellini. 2003
204 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/2e52fe70a10f7e155ca865dc41d53fc3dd3932f8
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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- Catherine Heymans
- Lavinia Heisenberg
- H. Hoekstra
- Luca Amendola
- Tomi Koivisto
- Stephen A. Appleby
- Thomas D. Kitching
- Richard J. Massey
Citations in the corpus
- WMAP constraints on low redshift evolution of dark energy (2004, methodology): “The results we obtain are consistent with similar analysis in other papers (Amendola & Quercellini 2003; Jimenez 2003; Jimenez et al. 2003; Padmanabhan & Choudhury 2003; Alam et al. 2004a,b; Bassett 2004; Bassett et al. 2004; Corasaniti et al. 2004; Choudhury & Padmanabhan 2004; Daly & Djorgovski…”
- Cosmology and Fundamental Physics with the Euclid Satellite (2012, methodology): “06 (at 95% CL for a constant coupling and an exponential potential) [152, 62, 47, 59], or possibly more [720, 711] if neutrinos are taken into account or for more realistic timedependent choices of the coupling.”