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19922026
most citedHeavy quarkonium: progress, puzzles, and opportunities

1.8k citations

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51 papers · 1 filter

astro-ph2008★ 108 cited

Deconfinement phase transition in hybrid neutron stars from the Brueckner theory with three-body forces and a quark model with chiral mass scaling

G. X. Peng, A. Li, U. Lombardo

We study the properties of strange quark matter in equilibrium with normal nuclear matter. Instead of using the conventional bag model in quark sector, we achieve the confinement b…

astro-ph2008★ 126 cited

Observational constraints on the dark energy and dark matter mutual coupling

Chang Feng, Bin Wang, Elcio Abdalla +1

We examine different phenomenological interaction models for Dark Energy and Dark Matter by performing statistical joint analysis with observational data arising from the 182 Gold…

astro-ph2007★ 181 cited

Testing the viability of the interacting holographic dark energy model by using combined observational constraints

Chang Feng, Bin Wang, Yungui Gong +1

Using the data coming from the new 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy…

astro-ph2006★ 215 cited

Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy

Xin Zhang

When taking the holographic principle into account, the vacuum energy will acquire dynamical property that its equation of state is evolving. The current available observational da…

astro-ph2006★ 126 cited

Two-Field Quintom Models in the w-w' Plane

Zong-Kuan Guo, Yun-Song Piao, Xinmin Zhang +1

The w-w' plane, defined by the equation of state parameter for the dark energy and its derivative with respect to the logarithm of the scale factor, is useful to the study of class…

astro-ph2006★ 15 cited

Noncommutative chaotic inflation and WMAP three year results

Xin Zhang, Feng-Quan Wu

Noncommutative inflation is based upon the consideration of some effects of the space-time uncertainty principle motivated by ideas from string/M theory. The CMB anisotropies may c…

astro-ph2006★ 16 cited

Uncertainty on determining the dark energy equation of state due to the spatial curvature

Zhuo-Yi Huang, Bin Wang, Ru-Keng Su

We have studied the uncertainty on the determination of the dark energy equation of state due to a non-vanishing spatial curvature by considering some fundamental observables. We d…

astro-ph2006★ 63 cited

Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations

Zong-Kuan Guo, Zong-Hong Zhu, J. S. Alcaniz +1

Although there is mounting observational evidence that the expansion of our universe is undergoing a late-time acceleration, the mechanism for this acceleration is yet unknown. In…

astro-ph2006★ 85 cited

Modified equation of state, scalar field, and bulk viscosity in Friedmann universe

J. Ren, X. H. Meng

A generalized dynamical equation for the scale factor of the universe is proposed to describe the cosmological evolution, of which the CDM model is a special case. It also provi…

astro-ph2006★ 59 cited

Towards Determination of the Initial Flavor Composition of Ultrahigh-energy Neutrino Fluxes with Neutrino Telescopes

Zhi-zhong Xing, Shun Zhou

We propose a simple but useful parametrization of the flavor composition of ultrahigh-energy neutrino fluxes produced from distant astrophysical sources: $ϕ^{}_e : ϕ^{}_μ: ϕ^{}_τ=…

astro-ph2006★ 48 cited

Is PSR B0943+10 a low-mass quark star?

Y. L. Yue, X. H. Cui, R. X. Xu

A recent X-ray observation has shown that the radio pulsar PSR B0943+10, with clear drifting subpulses, has a much smaller polar cap area than that of conventional pulsars with mas…

astro-ph2006★ 125 cited

A Tracker Solution for a Holographic Dark Energy Model

Hui Li, Zong-kuan Guo, Yuan-zhong Zhang

We investigate a kind of holographic dark energy model with the future event horizon the IR cutoff and the equation of state -1. In this model, the constraint on the equation of st…

astro-ph2005

Dark Energy: relating the evolution of the universe from the past to the future

Zhuo-Yi Huang, Bin Wang, Rong-Gen Cai +1

Using the evolution history of the universe, one can make constraint on the parameter space of dynamic dark energy models. We discuss two different parameterized dark energy models…

astro-ph2005★ 133 cited

Bulk viscous cosmology: statefinder and entropy

M. Hu, Xin He Meng

The statefinder diagnostic pair is adopted to differentiate viscous cosmology models and it is found that the trajectories of these viscous cosmology models on the statefinder pair…

astro-ph2005★ 183 cited

Cosmological model with viscosity media (dark fluid) described by an effective equation of state

J. Ren, Xin He Meng

A generally parameterized equation of state (EOS) is investigated in the cosmological evolution with bulk viscosity media modelled as dark fluid, which can be regarded as a unifica…

astro-ph2005★ 179 cited

Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters

Zhe Chang, Feng-Quan Wu, Xin Zhang

We use the Chandra measurements of the X-ray gas mass fraction of 26 rich clusters released by Allen et al. to perform constraints on the holographic dark energy model. The constra…

astro-ph2005★ 446 cited

Constraints on holographic dark energy from type Ia supernova observations

Xin Zhang, Feng-Quan Wu

In this paper, we use the type Ia supernovae data to constrain the holographic dark energy model proposed by Li. We also apply a cosmic age test to this analysis. We consider in th…

astro-ph2005★ 125 cited

Cosmology with a Variable Chaplygin Gas

Zong-Kuan Guo, Yuan-Zhong Zhang

We consider a new generalized Chaplygin gas model that includes the original Chaplygin gas model as a special case. In such a model the generalized Chaplygin gas evolves as from du…

astro-ph2005★ 138 cited

Parametrization of Quintessence and Its Potential

Zong-Kuan Guo, Nobuyoshi Ohta, Yuan-Zhong Zhang

We develop a theoretical method of constructing the quintessence potential directly from the effective equation of state function , which describes the properties of the dark…

astro-ph2004★ 151 cited

Cosmological Evolution of Interacting Phantom Energy with Dark Matter

Zong-Kuan Guo, Rong-Gen Cai, Yuan-Zhong Zhang

We investigate the cosmological evolution of an interacting phantom energy model in which the phantom field has interaction with the dark matter. We discuss the existence and stabi…

astro-ph2004★ 126 cited

Interacting Phantom Energy

Zong-Kuan Guo, Yuan-Zhong Zhang

We investigate the role of a suitable interaction between a matter fluid and a phantom field for the coincidence problem. There exists a stationary scaling solution which is a stab…

astro-ph2004★ 195 cited

New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter

Xin Zhang, Feng-Quan Wu, Jingfei Zhang

We propose in this paper a new model for describing the unification of dark energy and dark matter. This new model is a further generalization of the generalized Chaplygin gas (GCG…

astro-ph2004★ 804 cited

Cosmological Evolution of a Quintom Model of Dark Energy

Zong-Kuan Guo, Yun-Song Piao, Xinmin Zhang +1

We investigate in this paper the cosmological evolution of a dark energy model with two scalar fields where one of the scalar has canonical kinetic energy and another scalar has ne…

astro-ph2004★ 217 cited

Can vacuum decay in our Universe?

Peng Wang, Xin-He Meng

We take a phenomenological approach to study the cosmological evolution of decaying vacuum cosmology (CDM) based on a simple assumption about the form of the modified matter…