In-Lab Shallow-Water Simulations of Gaseous Discs for Astrophysical Fluid Dynamics [PDF]
G. P. Chernikov +4 more
openalex +2 more sources
Entropy-conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations [PDF]
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]
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]
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
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
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
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
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
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

