Search Results - "Klypin, A."
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Dark Matter Halos in the Standard Cosmological Model: Results from the Bolshoi Simulation
Published in The Astrophysical journal (20-10-2011)“…Lambda Cold Dark Matter ( Delta *LCDM) is now the standard theory of structure formation in the universe. We present the first results from the new Bolshoi…”
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The Uchuu simulations: Data Release 1 and dark matter halo concentrations
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT We introduce the Uchuu suite of large high-resolution cosmological N-body simulations. The largest simulation, named Uchuu, consists of 2.1 trillion…”
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Response of Dark Matter Halos to Condensation of Baryons: Cosmological Simulations and Improved Adiabatic Contraction Model
Published in The Astrophysical journal (20-11-2004)“…The cooling of gas in the centers of dark matter halos is expected to lead to a more concentrated dark matter distribution. The response of dark matter to the…”
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The Anisotropic Distribution of Galactic Satellites
Published in The Astrophysical journal (10-08-2005)“…We present a study of the spatial distribution of dwarf satellites (or subhalos) in galactic dark matter halos using dissipationless cosmological simulations…”
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The Tumultuous Lives of Galactic Dwarfs and the Missing Satellites Problem
Published in The Astrophysical journal (10-07-2004)“…Hierarchical cold dark matter (CDM) models predict that Milky Way-sized halos contain several hundred dense low-mass dark matter satellites (the substructure),…”
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The MultiDark Database: Release of the Bolshoi and MultiDark cosmological simulations
Published in Astronomische Nachrichten (01-08-2013)“…We present the online MultiDark Database – a Virtual Observatory‐oriented, relational database for hosting various cos‐mological simulations. The data is…”
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The Dark Side of the Halo Occupation Distribution
Published in The Astrophysical journal (01-07-2004)“…We analyze the halo occupation distribution (HOD) and two-point correlation function of galaxy-size dark matter halos using high-resolution dissipationless…”
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The velocity shear tensor: tracer of halo alignment
Published in Monthly notices of the Royal Astronomical Society (01-01-2013)“…The alignment of dark matter (DM) haloes and the surrounding large-scale structure (LSS) is examined in the context of the cosmic web. Halo spin, shape and the…”
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Resonances in barred galaxies
Published in Monthly notices of the Royal Astronomical Society (11-08-2007)“…The inner parts of many spiral galaxies are dominated by bars. These are strong non-axisymmetric features which significantly affect orbits of stars and dark…”
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A dynamical classification of the cosmic web
Published in Monthly notices of the Royal Astronomical Society (01-07-2009)“…In this paper, we propose a new dynamical classification of the cosmic web. Each point in space is classified in one of four possible web types: voids, sheets,…”
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The Uchuu–SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
Published in Monthly notices of the Royal Astronomical Society (15-02-2024)“…ABSTRACT We present the data release of the Uchuu–SDSS galaxies: a set of 32 high-fidelity galaxy light-cones constructed from the large Uchuu 2.1 trillion…”
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The virialized mass of dark matter haloes
Published in Monthly notices of the Royal Astronomical Society (01-09-2008)“…Virial mass is used as an estimator for the mass of a dark matter halo. However, the commonly used constant overdensity criterion does not reflect the…”
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Profiles of dark haloes: evolution, scatter and environment
Published in Monthly notices of the Royal Astronomical Society (01-03-2001)“…We study dark matter halo density profiles in a high-resolution N-body simulation of a ΛCDM cosmology. Our statistical sample contains ∼5000 haloes in the…”
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Probing galaxy assembly bias with LRG weak lensing observations
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…Abstract In Montero-Dorta et al., we show that luminous red galaxies (LRGs) from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) at z ∼ 0.55 can be…”
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A Universal Angular Momentum Profile for Galactic Halos
Published in The Astrophysical journal (01-07-2001)Get full text
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A semi-analytical perspective on massive galaxies at z ∼ 0.55
Published in Monthly notices of the Royal Astronomical Society (11-06-2019)“…ABSTRACT The most massive and luminous galaxies in the Universe serve as powerful probes to study the formation of structure, the assembly of mass, and…”
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The Origin of Angular Momentum in Dark Matter Halos
Published in The Astrophysical journal (20-12-2002)Get full text
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Dark matter annihilation in the milky way galaxy: effects of baryonic compression
Published in Physical review letters (10-12-2004)“…If the dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric particles, the central region of our Galaxy…”
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How Far Do They Go? The Outer Structure of Galactic Dark Matter Halos
Published in The Astrophysical journal (10-07-2006)“…We study the density profiles of collapsed galaxy-size dark matter halos with masses 10 super(11) to 5 x 10 super(12) M sub( )focusing mostly on the halo outer…”
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Bars and Cold Dark Matter Halos
Published in The Astrophysical journal (20-06-2006)“…The central part of a dark matter halo reacts to the presence and evolution of a bar. Not only does the halo absorb angular momentum from the disk, it can also…”
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