Results 271 to 280 of about 442,368 (316)
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The Open Journal of Astrophysics
Observational and/or astrophysical systematics modulating the observed number of luminous tracers can constitute a major limitation in the cosmological exploitation of surveys of the large scale structure of the universe.
C. Hern'andez-Monteagudo +20 more
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Observational and/or astrophysical systematics modulating the observed number of luminous tracers can constitute a major limitation in the cosmological exploitation of surveys of the large scale structure of the universe.
C. Hern'andez-Monteagudo +20 more
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Large scale structure of the universe
Space Science Reviews, 1995The current situation with the cosmological model and fundamental constants is briefly reviewed. Here, we concentrate on evolutionary effects of large-scale structure formation, in particular, the relationship with the quasar distribution and dynamics is discussed.
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Physics of the Dark Universe, 2023
We characterize the peculiar velocity field of the local large-scale structure reconstructed from the $2M++$ survey, by treating it as a fluid, extracting the divergence via different approximations over a range pf averaged scales.
Erick Pastén, S. Gálvez, V. Cárdenas
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We characterize the peculiar velocity field of the local large-scale structure reconstructed from the $2M++$ survey, by treating it as a fluid, extracting the divergence via different approximations over a range pf averaged scales.
Erick Pastén, S. Gálvez, V. Cárdenas
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Large Scale Structure of the Universe
2016The universe is full of stars. But how are all the stars distributed? Are they all huddled together, like freezing people around a fire? Or are they sprinkled evenly, as raisins in bread? The short answer is: both! The longer answer is surprisingly complex.
Benjamin Bahr +2 more
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Large-Scale Structure of the Universe
2019By naked eye, we can easily detect only three galaxies: the Andromeda galaxy in the northern sky, and the Large and Small Magellanic Clouds in the southern sky. Pictures taken via large telescopes contain millions of galaxies, and it is estimated that there are hundreds of billions of faint galaxies all over the sky.
Pekka Teerikorpi +5 more
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Detection of supernova magnitude fluctuations induced by large-scale structure
The Open Journal of AstrophysicsThe peculiar velocities of supernovae and their host galaxies are correlated with the large-scale structure of the Universe, and can be used to constrain the growth rate of structure and test the cosmological model.
Andrew Nguyen +58 more
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Large-scale-structure observables in general relativity validated at second order
Journal of Cosmology and Astroparticle PhysicsWe present a second-order calculation of relativistic large-scale-structure observables in cosmological perturbation theory, specifically the “cosmic rulers and clock”, which are the building-blocks of any other large-scale-structure observable ...
Antoine Villey +4 more
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Impact of light sterile neutrinos on cosmological large scale structure
Journal of Cosmology and Astroparticle PhysicsSterile neutrinos with masses on the eV scale are promising candidates to account for the origin of neutrino mass and the reactor neutrino anomalies. The mixing between sterile and active neutrinos in the early universe could result in a large abundance ...
Rui Hu +3 more
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The large-scale structure of the Universe
European Review, 1997The study of the distribution of matter in the Universe is at the forefront of modern astronomy, and stimulates numerous research programmes both in theory, observation and experiment. The distribution of galaxies has a cell-like structure resulting from the alternation of sheets and voids with the topological properties of a ‘sponge’.
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Spherical simulations of large‐scale structure of the Universe
Astronomische Nachrichten, 1985AbstractWe consider a spherical‐smmetric perturbation in an initially homogeneous dust filled universe within the frame‐work of the Bondi‐Tolman solution. The decoupling of the perturbed region from the background evolution naturally leads to shell‐crossing in a certain outer environment, which describes energy relaxation.
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