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19972005
most citedMinihalo photoevaporation during cosmic reionization: evaporation times and photon consumption rates

154 citations · 162 across the 6 of their papers we have counts for

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17 papers · 1 filter

astro-ph20052 cited

Ionization fronts and their interaction with density fluctuations: implications for reionization

Ilian T. Iliev, Paul R. Shapiro, Evan Scannapieco +4

The propagation of cosmological ionization fronts (I-fronts) during reionization is strongly influenced by small-scale structure. Here we summarize our recent attemps to understand…

astro-ph20044 cited

The Equilibrium Structure of CDM Halos

Paul R. Shapiro, Ilian T. Iliev, Hugo Martel +2

Dark-matter halos are the scaffolding around which galaxies and clusters are built. They form when the gravitational instability of primordial density fluctuations causes regions w…

astro-ph2004154 cited

Minihalo photoevaporation during cosmic reionization: evaporation times and photon consumption rates

Ilian T. Iliev, Paul R. Shapiro, Alejandro C. Raga

The weak, R-type ionization fronts (I-fronts) which swept across the intergalactic medium (IGM) during the reionization of the universe often found their paths blocked by cosmologi…

astro-ph20032 cited

Gravitational Lensing by CDM Halos: Singular versus Nonsingular Profiles

Hugo Martel, Paul R. Shapiro

The gravitational lensing properties of cosmological halos depend upon the mass distribution within each halo. The description of halos as nonsingular, truncated isothermal spheres…

astro-ph2003

Density Profiles of Dark Halos from their Mass Accretion Histories

Marcelo A. Alvarez, Kyungjin Ahn, Paul R. Shapiro

We use the universal mass accretion history recently reported for simulations of halo formation in the cold dark matter model (CDM) to analyze the formation and growth of a single…

astro-ph2002

Gravitational lensing by the truncated isothermal sphere model for cosmological halos. I. Individual lens properties

Hugo Martel, Paul R. Shapiro

The gravitational lensing properties of cosmological halos depend upon the mass distribution within each halo. The description of halos as nonsingular, truncated isothermal spheres…