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19942023
most citedAccelerating Universes with Scaling Dark Matter

2.5k citations · 8.6k across the 62 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

gr-qc2006★ 708 cited

Conditions for the cosmological viability of f(R) dark energy models

Luca Amendola, Radouane Gannouji, David Polarski +1

We derive the conditions under which dark energy models whose Lagrangian densities f are written in terms of the Ricci scalar R are cosmologically viable. We show that the cosmolog…

astro-ph2006★ 161 cited

Pointer states for primordial fluctuations in inflationary cosmology

C. Kiefer, I. Lohmar, D. Polarski +1

Primordial fluctuations in inflationary cosmology acquire classical properties through decoherence when their wavelengths become larger than the Hubble scale. Although decoherence…

astro-ph2006★ 220 cited

Scalar-Tensor Models of Normal and Phantom Dark Energy

Radouane Gannouji, David Polarski, Andre Ranquet +1

We consider the viability of dark energy (DE) models in the framework of the scalar-tensor theory of gravity, including the possibility to have a phantom DE at small redshifts …

astro-ph2006★ 12 cited

Dark Energy: Beyond General Relativity?

David Polarski

6 pages; Subm. to AIP Conf. Proceedings

astro-ph2006★ 111 cited

Power-laws f(R) theories are cosmologically unacceptable

Luca Amendola, David Polarski, Shinji Tsujikawa

In a recent paper [1] (PRL 98,131302,2007) we have shown that f(R)=R + mu R^{n} modified gravity dark energy models are not cosmologically viable because during the matter era that…

astro-ph2006★ 539 cited

Are f(R) dark energy models cosmologically viable ?

Luca Amendola, David Polarski, Shinji Tsujikawa

All modified gravity theories are conformally identical to models of quintessence in which matter is coupled to dark energy with a strong coupling. This coupling induces a c…