Results 11 to 20 of about 17,923,772 (307)
Direct N-body simulations [PDF]
Journal of Computational and Applied Mathematics, 1999 32 pages, 13 figures, in press in Riffert, H., Werner K. (eds), Computational Astrophysics, The Journal of Computational and Applied Mathematics (JCAM), Elsevier Press, Amsterdam ...
Spurzem, Rainer, Rainer Spurzem
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Relativistic N-body simulations with massive neutrinos [PDF]
Journal of Cosmology and Astroparticle Physics, 2017 26 pages + appendix, 17 figures; v2: minor revision, published version; code available at https://github.com/gevolution-code/gevolution-1 ...
Adamek, Julian +2 more
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TimThuering/N-Body-Simulation: Version 1.1
, 2023 <p>SYCL code for n-body simulations with the naive algorithm and the Barnes-Hut algorithm</p ...
Marcel Breyer, Tim Thüring
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Investigating rotation in young massive clusters by means of hydrodynamical and direct N-body simulations [PDF]
, 2022 One of the main open questions of star formation is the process of star clusters aggregation. In my thesis I investigate the kinematical features of embedded star clusters through hydrodynamical and N-body simulations.
Di Carlo, Ugo Niccolò
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The complexity of N-body simulation [PDF]
, 1993 The n-body simulation problem is stated as follows: Given initial positions and velocities of n particles that have pair-wise force interactions, simulate the movement of these particles so as to determine the positions of the particles at a future time.
John H. Reif, Stephen R. Tate
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Revisiting Vainshtein Screening for fast N-body simulations [PDF]
, 2023 We revisit a method to incorporate the Vainshtein screening mechanism in N-body simulations proposed by R. Scoccimarro in~\cite{Scoccimarro:2009eu}. We further extend this method to cover a subset of Horndeski theories that evade the bound on the speed ...
Koyama, K. +5 more
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The Astrophysical Journal, 2023 We investigate the influence of Toomre’s Q parameter on the bar-forming dynamics of the Maclaurin disk using N -body simulations. According to Toomre’s criterion, the local velocity dispersion parametrized by Q ≥ 1 is required to suppress the local ...
T. Worrakitpoonpon
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On Distributed Gravitational N-Body Simulations
CoRR, 2022 The N-body problem is a classic problem involving a system of N discrete bodies mutually interacting in a dynamical system. At any moment in time there are N*(N - 1)/2 such interactions occurring. This scaling as N^2 leads to computational difficulties where simulations range from tens of thousands of bodies to many millions.
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Collisional Growth and Fragmentation of Dust Aggregates. II. Mass Distribution of Icy Fragments
The Astrophysical Journal, 2023 By performing N -body simulations, we investigated the fundamental processes of collisions between dust aggregates composed of submicron-sized icy dust monomers.
Yukihiko Hasegawa +4 more
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Halo modelling in chameleon theories [PDF]
, 2014 We analyse modelling techniques for the large-scale structure formed in scalar-tensor theories of constant Brans-Dicke parameter which match the concordance model background expansion history and produce a chameleon suppression of the gravitational ...
Lombriser, Lucas +5 more
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