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Dark Energy and Fate of the Universe     Dark Energy  Fate  Universe  negative redshifts       font style='font-size:12px;'> 2012/2/21
We explore the ultimate fate of the Universe by using a divergence-free parametrization for dark energy $w(z)=w_0+w_a({\ln (2+z)\over 1+z}-\ln2)$. Unlike the CPL parametrization, this parametrization ...
The geometric characteristics of the universe     cosmology       font style='font-size:12px;'> 2011/9/26
A new kinematics cosmological model that base on
Diversity in the Phoenix Universe     Diversity  Phoenix Universe       font style='font-size:12px;'> 2011/10/17
It has recently been argued by Copeland et al. that in eleven dimensions two orbifold planes can collide and bounce in a regular way, even when the bulk metric is perturbed away from Milne spacetime t...
Who discovered the expanding universe?     discovered  expanding universe       font style='font-size:12px;'> 2011/10/18
Who discovered the expanding universe? Was it Hubble, or Lemaitre, or was it just the end result of a long series of investigations? In this article we summarise the main steps and contributions that ...
Do baryons trace dark matter in the early universe?     baryons trace  matter  early universe       font style='font-size:12px;'> 2011/9/30
Baryon-density perturbations of large amplitude may exist if they are compensated by dark-matter perturbations so that the total density remains unchanged. Big-bang nucleosynthesis and galaxy clusters...
We discuss two versions of the conformal scenario for generating scalar cosmological perturbations: a spectator version with a scalar field conformally coupled to gravity and carrying negligible energ...
We investigate the general properties of expanding cosmological models which generate scale-invariant curvature perturbations in the presence of a variable speed of sound. We show that in an expanding...
We make detailed theoretical predictions for the assembly properties of the Local Group (LG) in the standard LambdaCDM cosmological model. We use three cosmological N-body dark matter simulations from...
The main purpose of this paper is to explicitly verify the consistency of the energy-momentum and angular momentum tensor of the gravitational field established in the Hamiltonian structure of the Tel...
This paper is devoted to study the gravitational charged perfect fluid collapse in the Friedmann universe models with cosmological constant. For this purpose, we assume that the electromagnetic field ...
Geometry of the quantum universe     causal dynamical triangulation         font style='font-size:12px;'> 2010/3/19
A universe much like the (Euclidean) de Sitter space-time appears as background geometry in the causal dynamical triangulation (CDT) regularization of quantum gravity. We study the geometry of such un...
The Holographic Universe     Holographic Universe  quantum field theory       font style='font-size:12px;'> 2010/3/19
We present a holographic description of four-dimensional single-scalar inflationary universes in terms of a three-dimensional quantum field theory. The holographic description correctly reproduces sta...
EMIRUsing GRBs to probe the high redshift Universe     high redshift Universe  EMIR       font style='font-size:12px;'> 2009/6/12
EMIRUsing GRBs to probe the high redshift Universe
Luminous Blue Variables in the local universe     Luminous Blue Variables  local universe       font style='font-size:12px;'> 2009/6/12
Luminous Blue Variables in the local universe
Reionization of the universe and the photoevaporation of cosmological minihalos。

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