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researcher

Liang Gao

77 papers hereh-index 3610.5k citations97 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author10
  • middle author48
  • last author16

Across the 74 of 77 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.CO27
  • astro-ph18
  • astro-ph.HE2
same name
  • Liang Gao — 20 papers, h 17
  • Liang Gao — 9 papers, h 8
  • Liang Gao — 7 papers, h 4
  • Liang Gao — 7 papers, h 4
  • Liang Gao — 6 papers, h 2
  • Liang Gao — 6 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032026
most citedSimulating the joint evolution of quasars, galaxies and their large-scale distribution

5.1k citations · 13.5k across the 77 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005★ 685 cited

The age dependence of halo clustering

Liang Gao, Volker Springel, Simon D. M. White

We use a very large simulation of the concordance LCDM cosmogony to study the clustering of dark matter haloes. For haloes less massive than about 1e13Msun/h, the amplitude of the…

astro-ph2005★ 5.1k cited

Simulating the joint evolution of quasars, galaxies and their large-scale distribution

Volker Springel, Simon D. M. White, Adrian Jenkins +14

The cold dark matter model has become the leading theoretical paradigm for the formation of structure in the Universe. Together with the theory of cosmic inflation, this model make…

astro-ph2005★ 68 cited

The First Generation of Star-Forming Haloes

Darren Reed, Richard Bower, Carlos S. Frenk +4

We model gas cooling in high-resolution N-body simulations in order to investigate the formation of the first generation of stars. We follow a region of a LCDM universe especially…

astro-ph2005★ 117 cited

Early structure in LCDM

Liang Gao, Simon D. M. White, Adrian Jenkins +2

We use a novel technique to simulate the growth of the most massive progenitor of a protocluster region from redshift z~80, when its mass was about 10 Msun until the present day. O…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.