Results 81 to 90 of about 427,202 (211)
Shock‐heated Gas in the Large‐Scale Structure of the Universe [PDF]
HyeSung Kang +7 more
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Two-dimensional simulation of the gravitational system dynamics and formation of the large-scale structure of the Universe [PDF]
А. G. Doroshkevich +5 more
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Emulating Power Spectra for Prereconstructed and Postreconstructed Galaxy Samples
The small-scale linear information in galaxy samples typically lost during nonlinear growth can be restored to a certain level by the density field reconstruction, which has been demonstrated for improving the precision of the baryon acoustic oscillation
Yuting Wang +12 more
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Large Scale Structure of the Universe: Theoretical Problems [PDF]
E. Saar
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Across scales in our Universe: Gravitational Waves and the Large-Scale Structure
Henrique Rubira, Thomas Konstandin
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We investigated the alignment between the angular momenta of galaxy groups and the spines of their associated cosmic filaments. Our results demonstrate a significant tendency for these two orientations to be perpendicular, indicating that the rotation of
Yu Rong, Peng Wang, Xiao-xiao Tang
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Reconstructing the mass density, velocity, and tidal (MTV) fields of dark matter from galaxy surveys is essential for advancing our understanding of the large-scale structure of the Universe.
Feng Shi +12 more
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Cosmic Tidal Reconstruction in Redshift Space
Gravitational coupling between large- and small-scale density perturbations leads to anisotropic distortions to local small-scale matter fluctuations. Such local anisotropic distortions can be used to reconstruct large-scale matter distribution, known as
Shi-Hui Zang +3 more
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Halo Asymmetry in the Modeling of Galaxy Clustering
Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter halos can be approximated by the Navarro–Frenk–White (NFW) spherically symmetric profile.
Anna Durkalec +2 more
doaj +1 more source
Equal-time consistency relations in the large-scale structure of the universe [PDF]
A. Kehagias, H Perrier, A. Riotto
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