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20082023
most citedEnzo: An Adaptive Mesh Refinement Code for Astrophysics

869 citations · 3.5k across the 55 of their papers we have counts for

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Showing astro-ph.COShow all

14 papers · 1 filter

astro-ph.CO2019★ 2 cited

Revisiting Ryskin's Model of Cosmic Acceleration

Zhiqi Huang, Han Gao, Haoting Xu

Cosmic backreaction as an additional source of the expansion of the universe has been a debate topic since the discovery of cosmic acceleration. The major concern is whether the se…

astro-ph.CO2019★ 1 cited

Forecasting Cosmological Bias due to Local Gravitational Redshift

Haoting Xu, Zhiqi Huang, Na Zhang +1

When photons from distant galaxies and stars pass through our neighboring environment, the wavelengths of the photons would be shifted by our local gravitational potential. This lo…

astro-ph.CO2018★ 7 cited

Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State

Haoting Xu, Zhiqi Huang, Zhenjie Liu +1

The cosmic spatial curvature parameter is constrained, primarily by cosmic microwave background (CMB) data, to be very small. Observations of the cosmic distance ladder and t…

astro-ph.CO2017★ 11 cited

Fully Coupled Simulation of Cosmic Reionization. III. Stochastic Early Reionization by the Smallest Galaxies

Michael L Norman, Pengfei Chen, John H Wise +1

Previously we identified a new class of early galaxy that we estimate contributes up to 30\% of the ionizing photons responsible for reionization. These are low mass halos in the r…

astro-ph.CO2015★ 6 cited

Cluster magnetic fields through the study of polarized radio halos in the SKA era

F. Govoni, M. Murgia, H. Xu +17

Galaxy clusters are unique laboratories to investigate turbulent fluid motions and large scale magnetic fields. Synchrotron radio halos at the center of merging galaxy clusters pro…

astro-ph.CO2014★ 32 cited

Spatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early Universe

Kyungjin Ahn, Hao Xu, Michael L. Norman +2

We present our prediction for the local 21 cm differential brightness temperature () from a set of strongly clustered sources of Population III (Pop III) and II (Pop II) ob…