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Relevant bibliographies by topics / Physics. Sub-grid Physics

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Journal articles

Academic literature on the topic 'Physics. Sub-grid Physics'

Author: Grafiati

Published: 22 February 2023

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Journal articles on the topic "Physics. Sub-grid Physics"

1

Algoso, Anne Kurtz, Georgia Richardson, and Peter Woods. "Sub-grid Numerical Techniques for First Principles Physics Based Tools." Procedia Engineering 58 (2013): 433–44. http://dx.doi.org/10.1016/j.proeng.2013.05.050.

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2

Gibson, B. K., K. Pilkington, C. B. Brook, G. S. Stinson, and J. Bailin. "Constraining sub-grid physics with high-redshift spatially-resolved metallicity distributions." Astronomy & Astrophysics 554 (June 2013): A47. http://dx.doi.org/10.1051/0004-6361/201321239.

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3

Negri, A., and M. Volonteri. "Black hole feeding and feedback: the physics inside the ‘sub-grid’." Monthly Notices of the Royal Astronomical Society 467, no. 3 (2017): 3475–92. http://dx.doi.org/10.1093/mnras/stx362.

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4

Nuñez-Castiñeyra, A., E. Nezri, J. Devriendt, and R. Teyssier. "Cosmological simulations of the same spiral galaxy: the impact of baryonic physics." Monthly Notices of the Royal Astronomical Society 501, no. 1 (2020): 62–77. http://dx.doi.org/10.1093/mnras/staa3233.

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ABSTRACT The interplay of star formation (SF) and supernova (SN) feedback in galaxy formation is a key element for understanding galaxy evolution. Since these processes occur at small scales, it is necessary to have sub-grid models that recover their evolution and environmental effects at the scales reached by cosmological simulations. In this work, we present the results of the Mochima simulation, where we simulate the same spiral galaxy inhabiting a Milky Way (MW) size halo in a cosmological environment changing the sub-grid models for SN feedback and SF. We test combinations of the Schmidt

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5

Bing Deng, Xiao, and Siwei Dong. "Sub-Grid modelling based on vorticity-stretching." Journal of Physics: Conference Series 1522 (April 2020): 012021. http://dx.doi.org/10.1088/1742-6596/1522/1/012021.

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6

Shutts, Glenn, Thomas Allen, and Judith Berner. "Stochastic parametrization of multiscale processes using a dual-grid approach." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 366, no. 1875 (2008): 2623–39. http://dx.doi.org/10.1098/rsta.2008.0035.

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Some speculative proposals are made for extending current stochastic sub-gridscale parametrization methods using the techniques adopted from the field of computer graphics and flow visualization. The idea is to emulate sub-filter-scale physical process organization and time evolution on a fine grid and couple the implied coarse-grained tendencies with a forecast model. A two-way interaction is envisaged so that fine-grid physics (e.g. deep convective clouds) responds to forecast model fields. The fine-grid model may be as simple as a two-dimensional cellular automaton or as computationally dem

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7

WU, CHUI-JIE, and HUI GUAN. "LATTICE BOLTZMANN DYNAMICS AND DYNAMICAL SYSTEM SUB-GRID MODELS." Modern Physics Letters B 23, no. 03 (2009): 349–52. http://dx.doi.org/10.1142/s0217984909018370.

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The dynamics sub-grid scale (SGS) models and the dynamical system SGS model are introduced into the lattice Boltzmann method (LBM), and applied to numerical simulation of turbulent cavity flows. The results are compared with those of direct numerical simulation of turbulence and Smagorinsky SGS model. A new average method of eliminating the inherent unphysical oscillation of LBM is also given.

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8

Labarre, V., B. Dubrulle, and D. Paillard. "Sub-grid modelling for a diffusive lattice gas." Journal of Physics A: Mathematical and Theoretical 53, no. 40 (2020): 405006. http://dx.doi.org/10.1088/1751-8121/aba577.

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9

Sun, Mengxue, Ruixin Gao, Yuhui Ji, Xin Long, Changzhi Yao, and Fan Wu. "Inside-wind-farm/Wind-farm-grid sub-synchronous oscillation characteristics analysis in grid-connected system of multiple DFIGs." Journal of Physics: Conference Series 2076, no. 1 (2021): 012116. http://dx.doi.org/10.1088/1742-6596/2076/1/012116.

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Abstract Aiming at the sub-synchronous oscillation (SSO) problem of the grid-connected system of multiple DFIGs, most of the existing theoretical studies take the entire wind farm as a single-machine model, the stand-alone model cannot reflect the inside-wind-farm oscillation mode produced by the interactions among DFIGs in the wind farm. Therefore, this paper takes the equivalent value of DFIG-based wind farm to three DFIGs, establishes a mathematical model of the grid-connected system of three DFIGs, and studies the sub-synchronous oscillation modes existing in the system through eigenvalue

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10

Oliva, G. André, and R. Kuiper. "Modeling disk fragmentation and multiplicity in massive star formation." Astronomy & Astrophysics 644 (November 27, 2020): A41. http://dx.doi.org/10.1051/0004-6361/202038103.

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Context. There is growing evidence that massive stars grow by disk accretion in a similar way to their low-mass counterparts. Early in evolution, these disks can achieve masses that are comparable to the current stellar mass, and therefore the forming disks are highly susceptible to gravitational fragmentation. Aims. We investigate the formation and early evolution of an accretion disk around a forming massive protostar, focussing on its fragmentation physics. To this end, we follow the collapse of a molecular cloud of gas and dust, the formation of a massive protostar, the formation of its ci

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