Hao Xu

researcher ORCID ID = 0000-0003-4084-9925

Hao Xu is …
instance of (P31):
humanQ5

External links are
P496ORCID iD0000-0003-4084-9925
P1053ResearcherIDB-8734-2014
P1153Scopus author ID55493766100

P69educated atUniversity of Hong KongQ15568
Sun Yat-sen UniversityQ178972
University of California, San DiegoQ622664
P108employerSan Diego Supercomputer CenterQ3947008
Los Alamos National LaboratoryQ379848
University of California, San DiegoQ622664
P106occupationresearcherQ1650915

Reverse relations

author (P50)
Q60735176Comparing numerical methods for isothermal magnetized supersonic turbulence
Q59713361Comparisons of cosmological magnetohydrodynamic galaxy cluster simulations to radio observations
Q59713390Cosmological adaptive mesh refinement magnetohydrodynamics with Enzo
Q59713354Cosmological magnetohydrodynamic simulations of galaxy cluster radio relics: insights and warnings for observations
Q59713393Evolution and distribution of magnetic fields from active galactic nuclei in galaxy clusters. I. The effect of injection energy and redshift
Q59713382Evolution and distribution of magnetic fields from active galactic nuclei in galaxy clusters. II. The effects of cluster size and dynamical state
Q59713446Formation of X-Ray Cavities by the Magnetically Dominated Jet-Lobe System in a Galaxy Cluster
Q59713357Magnetohydrodynamic turbulence and cosmic-ray reacceleration in galaxy clusters
Q58922853Supermassive population III supernovae and the birth of the first quasars
Q59713465The Biermann Battery in Cosmological MHD Simulations of Population III Star Formation
Q59713374The two states of star-forming clouds
Q59713425Turbulence and dynamo in galaxy cluster medium: implications on the origin of cluster magnetic fields

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