Results 21 to 30 of about 258,357 (262)

In-Lab Shallow-Water Simulations of Gaseous Discs for Astrophysical Fluid Dynamics [PDF]

open access: bronze, 2012
G. P. Chernikov   +4 more
openalex   +2 more sources

Entropy-conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations [PDF]

open access: yesAstrophysical Journal Supplement Series, 2021
We compare the performance of energy-based and entropy-conserving schemes for modeling nonthermal energy components, such as unresolved turbulence and cosmic rays, using idealized fluid dynamics tests and isolated galaxy simulations.
V. Semenov, A. Kravtsov, B. Diemer
semanticscholar   +1 more source

Analytical results for binary dynamics at the first post-Newtonian order in Einstein-Cartan theory with the Weyssenhoff fluid [PDF]

open access: yesPhysical Review D, 2023
The quantum spin effects inside matter can be modeled via the Weyssenhoff fluid, which permits to unearth a formal analogy between general relativity and Einstein-Cartan theory at the first post-Newtonian order.
Vittorio De Falco, E. Battista
semanticscholar   +1 more source

Non-linear dynamics of hydrodynamic tori as a model of oscillations and bending waves in astrophysical discs [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
Understanding oscillations and waves in astrophysical fluid bodies helps to elucidate their observed variability and the underlying physical mechanisms.
Callum W. Fairbairn, G. Ogilvie
semanticscholar   +1 more source

Tidally Forced Planetary Waves in the Tachocline of Solar-like Stars

open access: yesThe Astrophysical Journal, 2023
Can atmospheric waves in planet-hosting solar-like stars substantially resonate to tidal forcing, perhaps at a level of impacting the space weather or even being dynamo-relevant?
Gerrit M. Horstmann   +4 more
doaj   +1 more source

Formulating the r-mode Problem for Slowly Rotating Neutron Stars

open access: yesThe Astrophysical Journal, 2023
We revisit the problem of inertial r-modes in stratified stars, drawing on a more precise description of the composition stratification in a mature neutron star.
Nils Andersson, Fabian Gittins
doaj   +1 more source

How the growth of ice depends on the fluid dynamics underneath

open access: yesProceedings of the National Academy of Sciences of the United States of America, 2021
Significance Landscapes, resulting from ice–water interactions coupled with solidification/melting, are ubiquitous in nature, yet most previous studies have not considered the rich fluid dynamics induced by water density anomaly underneath the moving ice
Ziqi Wang   +3 more
semanticscholar   +1 more source

On Secular Gravitational Instability in Vertically Stratified Disks

open access: yesThe Astrophysical Journal, 2023
Secular gravitational instability (GI) is one promising mechanism for explaining planetesimal formation. Previous studies of secular GI utilized a razor-thin disk model and derived the growth condition in terms of vertically integrated physical values ...
Ryosuke T. Tominaga   +2 more
doaj   +1 more source

SPROUT: A Moving-mesh Hydro Code Using a Uniformly Expanding Cartesian Grid

open access: yesThe Astrophysical Journal Supplement Series, 2023
We present the publicly available moving-mesh hydrodynamics code Sprout . Sprout solves the equations of ideal hydrodynamics on an expanding Cartesian mesh.
Soham Mandal, Paul C. Duffell
doaj   +1 more source

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