We investigate Big-Bang nucleosynthesis in the Brans-Dicke model with a variable cosmological term (BDA) for the coupling constant ω=10^4. The model parameters are constrained from comparison between the resulting abundance of ^4He, D and ^7Li and the observed ones. Furthermore, we examine the magnitude redshift (m-z) relation for the BDA with and without another constant cosmological term in a flat universe. Observational data of Type Ia Supernovae (SNIa) are used in the redshift range 0.01<z<2. It is found that BDA is inconsistent with the present accelerating universe but the model with a constant cosmological term with the value 0.7 can explain the SNIa data. The model parameters are insensitive to the m-z relation
p. 3301-3306In previous papers, a cosmological model with constant rate particle creation and vacuum...
The High-z Supernova Search Team has discovered and observed eight new supernovae in the redshift in...
International audienceAmong the various possibilities to probe the theory behind the recent accelera...
We investigate observational constraints on the Brans-Dicke cosmological model using observational d...
The five-dimensional Brans-Dicke theory naturally provides two scalar fields by the Killing reductio...
We investigate the big-bang nucleosynthesis in a Brans-Dicke model with a varying Λ term using the...
In this paper we summarise the constraints that low-redshift data—such as supernovae Ia (SN Ia), ba...
International audienceContext. The cosmological concordance model (ΛCDM) is the current standard mod...
We use the generalized Brans-Dicke theory, in which the Pauli metric is identified to be the physica...
The fate of the Universe, infinite expansion or a big crunch , can be determined by measuring the r...
International audienceWe study different one-parametric models of type Ia Supernova magnitude evolut...
International audienceContext. The cosmological concordance model (ΛCDM) matches the cosmological ob...
The Brans-Dicke (BD) theory is the simplest Scalar-Tensor theory of gravity, which can be considered...
In this paper, we have examined the viability of the Bianchi type-V universe in Brans-Dicke (BD) the...
p. 3301-3306In previous papers, a cosmological model with constant rate particle creation and vacuum...
The High-z Supernova Search Team has discovered and observed eight new supernovae in the redshift in...
International audienceAmong the various possibilities to probe the theory behind the recent accelera...
We investigate observational constraints on the Brans-Dicke cosmological model using observational d...
The five-dimensional Brans-Dicke theory naturally provides two scalar fields by the Killing reductio...
We investigate the big-bang nucleosynthesis in a Brans-Dicke model with a varying Λ term using the...
In this paper we summarise the constraints that low-redshift data—such as supernovae Ia (SN Ia), ba...
International audienceContext. The cosmological concordance model (ΛCDM) is the current standard mod...
We use the generalized Brans-Dicke theory, in which the Pauli metric is identified to be the physica...
The fate of the Universe, infinite expansion or a big crunch , can be determined by measuring the r...
International audienceWe study different one-parametric models of type Ia Supernova magnitude evolut...
International audienceContext. The cosmological concordance model (ΛCDM) matches the cosmological ob...
The Brans-Dicke (BD) theory is the simplest Scalar-Tensor theory of gravity, which can be considered...
In this paper, we have examined the viability of the Bianchi type-V universe in Brans-Dicke (BD) the...
p. 3301-3306In previous papers, a cosmological model with constant rate particle creation and vacuum...
The High-z Supernova Search Team has discovered and observed eight new supernovae in the redshift in...
International audienceAmong the various possibilities to probe the theory behind the recent accelera...