We constrain proposed phenomenological models for a vacuum energy which decays with the expansion of the universe from considerations of standard big bang nucleosynthesis. Several such models which attempt to solve the cosmological age problem are disfavored or even ruled out
The primordial nucleosynthesis and pulsar timing noise constraints on cosmic-string gravitational ra...
Next year we will celebrate 100 years of the cosmological term, Λ, in Einstein's gravitational field...
AbstractA cosmology with the growing cosmological term is considered. If there is no exchange of ene...
International audienceAmong the various possibilities to probe the theory behind the recent accelera...
Abstract: The possibility of a slow cosmic evolution of fundamental "constants" of Nature ...
In the standard hot big bang model, the expansion of the early universe is given by the Friedmann eq...
The prevailing constant Λ-G cosmological model agrees with observational evidence including the obse...
We critically review several recent approaches to solving the two cosmological constant problems. Th...
We put bounds on the variation of the value of the fine structure constant elements up to $^7$Li. We...
The currently available values and confidence limits for $\Omega_{\mathrm{m0}}$, H0 and globular cl...
This paper is devoted to investigate the implications of Einstein-Aether and modified Hořava–Lifshit...
We study the role of the cosmological constant in different theories with finite space- time. The co...
The Hubble expansion of galaxies, the $2.73\dK$ blackbody radiation background and the cosmic abunda...
The primordial nucleosynthesis and pulsar timing noise constraints on cosmic-string gravitational ra...
Next year we will celebrate 100 years of the cosmological term, Λ, in Einstein's gravitational field...
AbstractA cosmology with the growing cosmological term is considered. If there is no exchange of ene...
International audienceAmong the various possibilities to probe the theory behind the recent accelera...
Abstract: The possibility of a slow cosmic evolution of fundamental "constants" of Nature ...
In the standard hot big bang model, the expansion of the early universe is given by the Friedmann eq...
The prevailing constant Λ-G cosmological model agrees with observational evidence including the obse...
We critically review several recent approaches to solving the two cosmological constant problems. Th...
We put bounds on the variation of the value of the fine structure constant elements up to $^7$Li. We...
The currently available values and confidence limits for $\Omega_{\mathrm{m0}}$, H0 and globular cl...
This paper is devoted to investigate the implications of Einstein-Aether and modified Hořava–Lifshit...
We study the role of the cosmological constant in different theories with finite space- time. The co...
The Hubble expansion of galaxies, the $2.73\dK$ blackbody radiation background and the cosmic abunda...
The primordial nucleosynthesis and pulsar timing noise constraints on cosmic-string gravitational ra...
Next year we will celebrate 100 years of the cosmological term, Λ, in Einstein's gravitational field...
AbstractA cosmology with the growing cosmological term is considered. If there is no exchange of ene...