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most citedThermally Induced Density Perturbations in the Inflation Era

391 citations · 2.6k across the 103 of their papers we have counts for

collaborators

103 papers

astro-ph.CO2013★ 23 cited

Turbulence in the Inter-galactic Medium: Solenoidal and Dilatational Motions, and the Impact of Numerical Viscosity

Weishan Zhu, Long-Long Feng, Yinhua Xia +3

We use a suite of cosmological hydrodynamic simulations, run by two fixed grid codes, to investigate the properties of solenoidal and dilatational motions of the intergalactic medi…

astro-ph.CO2011★ 6 cited

Time-Dependent Behavior of Lyman Photon Transfer in High Redshift Optically Thick Medium

Wen Xu, Xiang-Ping Wu, Li-Zhi Fang

With Monte Carlo simulation method, we investigate the time dependent behavior of Ly photon transfer in optically thick medium of the concordance CDM universe. At high redshi…

astro-ph.CO2011★ 5 cited

Effect of Dust on Lyman-alpha Photon Transfer in Optically Thick Halo

Yang Yang, Ishani Roy, Chi-Wang Shu +1

We investigate the effects of dust on Lyα photons emergent from an optically thick medium by solving the integro-differential equation of the radiative transfer of resonant photons…

astro-ph.CO2011★ 1 cited

Intermittence of the Map of Kinetic Sunyaev-Zel'dovich Effect and Turbulence of IGM

Weishan Zhu, Long-Long Feng, Li-Zhi Fang

We investigate the possibility of detecting the turbulent state of the IGM with the kinetic Sunyaev-Zel'dovich (kSZ) effect. Being sensitive to the divergence-free component of the…

astro-ph.CO2011★ 21 cited

Dynamical Effect of the Turbulence of IGM on the Baryon Fraction Distribution

Zhu Weishan, Feng Long-Long, Fang Li-Zhi

We investigate the dynamical effect of the turbulence in baryonic intergalactic medium (IGM) on the baryon fraction distribution. In the fully developed nonlinear regime, the IGM w…

astro-ph.CO2010★ 5 cited

Statistical and dynamical decoupling of the IGM from Dark Matter

Li-Zhi Fang, Weishan Zhu

The mean mass densities of cosmic dark matter is larger than that of baryonic matter by a factor of about 5 in the CDM universe. Therefore, the gravity on large scales should be…