We discuss the general models with one time-like extra dimension and parallel 3-branes on the space-time $M^4 \times M^1$. We also construct the general brane models or networks with $n$ space-like and $m$ time-like extra dimensions and with constant cosmological constant on the space-time $M^4\times (M^1)^{n+m}$, and point out that there exist two kinds of models with zero cosmological constant. For static solutions, we have to introduce time-like and space-like extra dimensions to obtain the models with zero cosmological constant. For non-static solutions, we can obtain the models with only space-like extra dimension(s) and zero cosmological constant. We also give two simplest models explicitly
Some time ago Dvali, Gabadadze and Senjanovic (hep-ph/9910207) discussed brane world scenarios with ...
We derive the analogue of the vanishing of the cosmological constant in 3+1 dimensions, T_0^0 = 0, i...
We consider a model with two parallel (positive tension) 3-branes separated by a distance $L$ in 5-d...
AbstractWe construct an intersecting brane configuration in six-dimensional space with one extra spa...
If the fifth dimension is one-dimensional connected manifold, up to diffeomorphic, the only possible...
I present the main features of the brane cosmology scenario, according to which our universe is a se...
AbstractSome time ago Dvali, Gabadadze and Senjanović hep-ph/9910207 discussed brane world scenarios...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
Brane-Universe model embedded in 6-dimensional space-time with the signature (2+4) is considered. A ...
We argue that the cosmological constant problem can be solved in a braneworld model with infinite-vo...
A simple model of the brane-world cosmology has been proposed, which is characterized by four parame...
We study cosmological braneworld models with a single timelike extra dimension. Such models admit th...
We derive the effective cosmological equations for a non-$\mathbb{Z}_2$ symmetric codimension one br...
We consider Randall-Sundrum model with localized gravity, replacing the extra compact space-like dim...
The possibility of neutral, brane-like solutions in a higher dimensional setting is discussed. In pa...
Some time ago Dvali, Gabadadze and Senjanovic (hep-ph/9910207) discussed brane world scenarios with ...
We derive the analogue of the vanishing of the cosmological constant in 3+1 dimensions, T_0^0 = 0, i...
We consider a model with two parallel (positive tension) 3-branes separated by a distance $L$ in 5-d...
AbstractWe construct an intersecting brane configuration in six-dimensional space with one extra spa...
If the fifth dimension is one-dimensional connected manifold, up to diffeomorphic, the only possible...
I present the main features of the brane cosmology scenario, according to which our universe is a se...
AbstractSome time ago Dvali, Gabadadze and Senjanović hep-ph/9910207 discussed brane world scenarios...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
Brane-Universe model embedded in 6-dimensional space-time with the signature (2+4) is considered. A ...
We argue that the cosmological constant problem can be solved in a braneworld model with infinite-vo...
A simple model of the brane-world cosmology has been proposed, which is characterized by four parame...
We study cosmological braneworld models with a single timelike extra dimension. Such models admit th...
We derive the effective cosmological equations for a non-$\mathbb{Z}_2$ symmetric codimension one br...
We consider Randall-Sundrum model with localized gravity, replacing the extra compact space-like dim...
The possibility of neutral, brane-like solutions in a higher dimensional setting is discussed. In pa...
Some time ago Dvali, Gabadadze and Senjanovic (hep-ph/9910207) discussed brane world scenarios with ...
We derive the analogue of the vanishing of the cosmological constant in 3+1 dimensions, T_0^0 = 0, i...
We consider a model with two parallel (positive tension) 3-branes separated by a distance $L$ in 5-d...