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Hydrostatic equilibrium and Tsallis’ equilibrium for self-gravitating systems
Published 2005-09-01Subjects: Get full text
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The hydrostatic equilibrium and its implications on the mechanical properties of planets
Published 1974-06-01“…Under the hypothesis of hydrostatic equilibrium the planets of the solar system are represented on the plane (J"2, w2 a?…”
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The principal moments of inertia calculated with the hydrostatic equilibrium figure of the Earth
Published 2017-05-01Subjects: Get full text
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Hydrostatic equilibrium configurations of neutron stars in a non-minimal geometry-matter coupling theory of gravity
Published 2020-05-01“…Abstract In this work we analyze hydrostatic equilibrium configurations of neutron stars in a non-minimal geometry-matter coupling (GMC) theory of gravity. …”
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Stability of the 3D incompressible MHD equations with horizontal dissipation in periodic domain
Published 2021-08-01Subjects: Get full text
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Method of construction of three-dimensional mass distribution of hydrostatically introduced ellipsoidal planet
Published 2019-10-01Subjects: Get full text
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A low-Mach Roe-type solver for the Euler equations allowing for gravity source terms *
Published 2017-01-01“…In order to perform simulations of low Mach number flow in presence of gravity the technique from [23] is found insufficient as it is unable to cope with the presence of a hydrostatic equilibrium. Instead, a new modification of the diffusion matrix in the context of Roe-type schemes is suggested. …”
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Probing the evolution of galaxy clusters using SZ effect and non-thermal emission: First results from A1413
Published 2024-01-01“…Calibrating mass from intracluster medium observables such as the Sunyaev-Zel’dovich (SZ) effect is subject to uncertainty and biases because of the hydrostatic equilibrium assumption. On the other hand, merging cluster systems have been shown to exhibit radio emission which implies a link with disturbances from hydrostatic equilibrium. …”
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Brief communication: Time step dependence (and fixes) in Stokes simulations of calving ice shelves
Published 2020-09-01“…This can be especially problematic for models of calving glaciers, where rapid changes in geometry cause configurations that suddenly depart from hydrostatic equilibrium and lead to inaccurate estimates of the stress field. …”
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A comprehensive discussion for the identification of cracking points in f(R) theories of gravity
Published 2023-08-01“…In this context, we developed the hydrostatic equilibrium equation for spherically symmetric spacetime with anisotropic matter configuration and subsequently employed the Krori Barua technique. …”
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Development of local density perturbation technique to identify cracking points in f(R, T) gravity
Published 2023-09-01“…To achieve this, we developed the hydrostatic equilibrium equation for spherically symmetric spacetime with anisotropic matter configuration and subsequently applied the Krori–Barua spacetime coefficient. …”
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Reply to A. G. C. A. Meesters et al.'s comment on "Biotic pump of atmospheric moisture as driver of the hydrological cycle on land"
Published 2009-07-01“…This disturbs hydrostatic equilibrium and makes air circulate under the action of the recently described evaporative force. …”
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Averaged water potentials in soil water and groundwater, and their connection to menisci in soil pores, field-scale flow phenomena, and simple groundwater flows
Published 2011-05-01“…Others hypothesized a direct connection at hydrostatic equilibrium between the average matric potential of a subsurface body of water and the average pressure drop over the menisci in the soil pores. …”
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Disk formation and structure*
Published 2015-01-01“…We also summarise the structure of such a disk as it results from hydrostatic equilibrium and viscous accretion.…”
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A machine learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel’dovich maps with The Three Hundred clusters
Published 2024-01-01“…We verify the capabilities of our model by comparing it with the hydrostatic equilibrium technique, showing that it accurately recovers total mass profiles without any bias.…”
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A New Hydrodynamic Spherical Accretion Exact Solution and Its Quasi-spherical Perturbations
Published 2023-01-01“…This change allows for simple power-law solutions on the density and infall velocity fields, ranging from a cold empty freefall condition where pressure tends to zero, to a hot hydrostatic equilibrium limit with no infall velocity. As in the case of the Bondi solution, a maximum accretion rate appears. …”
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Short note: Intraterrestial stresses caused by the decreasing spin angular momentum of the Earth
Published 2003-05-01“…The departures of the planet’s actual shape and structure from the ideal shape and structure as required by hydrostatic equilibrium may be a source of potential energy for intraterrestial and, ultimately, crustal unrest.…”
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