Modelling of planetary accretion and core-mantle structure formation
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Publication:6633656
DOI10.1088/1751-8121/AD75D9MaRDI QIDQ6633656
Ulisse Stefanelli, Tomáş Roubíçek
Publication date: 6 November 2024
Published in: Journal of Physics A: Mathematical and Theoretical (Search for Journal in Brave)
planetsviscoelastic fluidstransport equationsself-gravitationtwo-component flowNavier-Stokes-Fourier-Poisson system
Planetary atmospheres (85A20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- Title not available (Why is that?)
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- Title not available (Why is that?)
- Title not available (Why is that?)
- The mathematics and mechanics of biological growth
- A thermo-mechanically coupled theory for fluid permeation in elastomeric materials: application to thermally responsive gels
- A theory for species migration in a finitely strained solid with application to polymer network swelling
- Mass transport in morphogenetic processes: a second gradient theory for volumetric growth and material remodeling
- The state of deformation in earthlike self-gravitating objects
- On global motions of a compressible barotropic and self-gravitating gas with density-dependent viscosities
- Allgemeine Kontinuumstheorie der Versetzungen und Eigenspannungen
- Tractions, balances, and boundary conditions for nonsimple materials with application to liquid flow at small-length scales
- Elastic materials with couple-stresses
- Thermomechanics of volumetric growth in uniform bodies
- On the dynamics of gaseous stars
- Global in time weak solutions for compressible barotropic self-gravitating fluids
- Micro-structure in linear elasticity
- Mathematical characterization and identification of remodeling, growth, aging and morphogenesis
- Some Open Problems in Elasticity
- Multipolar viscous fluids
- Global invertibility of Sobolev functions and the interpenetration of matter
- Principles of Continuum Mechanics
- Mathematics of Open Fluid Systems
- Viscoelastic Cahn–Hilliard models for tumor growth
- Thermodynamics of viscoelastic solids, its Eulerian formulation, and existence of weak solutions
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