AbstractWe point out that extended gravity theories, the Lagrangian of which is an arbitrary function of scalar curvature R, are equivalent to a class of the scalar-tensor theories of gravity. The corresponding gravity theory is ω=0 Brans–Dicke gravity with a potential for the Brans–Dicke scalar field, which is not compatible with solar system experiments if the field is very light: the case when such modifications become important recently
AbstractWe point out that extended gravity theories, the Lagrangian of which is an arbitrary functio...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
AbstractWe consider class of modified f(R) gravities with the effective cosmological constant epoch ...
We review the main properties of the recently proposed the Geometric Scalar Gravity (GSG), emphasizi...
The dynamical equivalence between modified and scalar-tensor gravity theories is revisited and it is...
We explore differences between scalar field, and scalar density solutions by using Robertson-Walker ...
We study minimal realistic scalar-tensor model of dilatonic gravity with Brance-Dicke factor $\omega...
Large extra dimensions provide interesting extensions of our parameter space for gravitational theor...
We study the cosmological constraints on the variation of Newton’s constant and on post-Newtonian p...
We generalize the well-known analogies between m^2 \phi^2 and R + R^2 theories to include the selfin...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
AbstractWe point out that extended gravity theories, the Lagrangian of which is an arbitrary functio...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
AbstractWe consider class of modified f(R) gravities with the effective cosmological constant epoch ...
We review the main properties of the recently proposed the Geometric Scalar Gravity (GSG), emphasizi...
The dynamical equivalence between modified and scalar-tensor gravity theories is revisited and it is...
We explore differences between scalar field, and scalar density solutions by using Robertson-Walker ...
We study minimal realistic scalar-tensor model of dilatonic gravity with Brance-Dicke factor $\omega...
Large extra dimensions provide interesting extensions of our parameter space for gravitational theor...
We study the cosmological constraints on the variation of Newton’s constant and on post-Newtonian p...
We generalize the well-known analogies between m^2 \phi^2 and R + R^2 theories to include the selfin...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
AbstractWe point out that extended gravity theories, the Lagrangian of which is an arbitrary functio...
5 pages, reference added, version accepted in PRLInternational audienceWe introduce a new class of s...
AbstractWe consider class of modified f(R) gravities with the effective cosmological constant epoch ...