Avalanches and subaqueous debris flows are two cases of a wide range of natural hazards that have been previously modeled with non-Newtonian fluid mechanics approximating the interplay of forces associated with gravity flows of granular and solid–liquid mixtures. The complex behaviors of such flows at unsteady flow initiation (i.e., destruction of structural jamming) and flow stalling (restructuralization) imply that the representative viscosity–stress relationships should include hysteresis: there is no reason to expect the timescale of microstructure destruction is the same as the timescale of restructuralization. The non-Newtonian Herschel–Bulkley relationship that has been previously used in such models implies complete revers...
This paper proposes a computational approach to debris flow model. In recent years, the theoretical...
Classical depth-integrated smoothed particle hydrodynamics (SPH) models for avalanches are extended ...
International audienceThis work focuses on the use of thin-layer models for simulating fast gravitat...
© Author(s) 2018. This work is distributed under the Creative Commons Attribution 3.0 License. Avala...
Some forms of mud flows and debris flows exhibit a non-Newtonian thixotropic behaviour, and this stu...
In this contribution, I present a historical account of debris flow modelling leading to the state o...
AbstractSince 1989 models to route debris flows and avalanches for hazards mitigation have been cons...
Abstract: A new mathematical model developed to predict behavior of debris flows and avalanches also...
Some forms of mud flows and debris flows exhibit a non-Newtonian thixotropic behaviour, and this stu...
Observational and experimental evidence suggests that it is important to explicitly account for the ...
Debris flows and debris avalanches are complex, gravity-driven currents of rock, water and sediments...
Background: Rock avalanches are flow-like landslides that can travel at extremely r...
This work presents the thermodynamically consistent development of a scaled, depth-integrated model ...
Abstract. Rock avalanches, debris flows, and related phenomena consist of grain-fluid mixtures that ...
International audienceThe main goal of these notes is to present several depth-averaged models with ...
This paper proposes a computational approach to debris flow model. In recent years, the theoretical...
Classical depth-integrated smoothed particle hydrodynamics (SPH) models for avalanches are extended ...
International audienceThis work focuses on the use of thin-layer models for simulating fast gravitat...
© Author(s) 2018. This work is distributed under the Creative Commons Attribution 3.0 License. Avala...
Some forms of mud flows and debris flows exhibit a non-Newtonian thixotropic behaviour, and this stu...
In this contribution, I present a historical account of debris flow modelling leading to the state o...
AbstractSince 1989 models to route debris flows and avalanches for hazards mitigation have been cons...
Abstract: A new mathematical model developed to predict behavior of debris flows and avalanches also...
Some forms of mud flows and debris flows exhibit a non-Newtonian thixotropic behaviour, and this stu...
Observational and experimental evidence suggests that it is important to explicitly account for the ...
Debris flows and debris avalanches are complex, gravity-driven currents of rock, water and sediments...
Background: Rock avalanches are flow-like landslides that can travel at extremely r...
This work presents the thermodynamically consistent development of a scaled, depth-integrated model ...
Abstract. Rock avalanches, debris flows, and related phenomena consist of grain-fluid mixtures that ...
International audienceThe main goal of these notes is to present several depth-averaged models with ...
This paper proposes a computational approach to debris flow model. In recent years, the theoretical...
Classical depth-integrated smoothed particle hydrodynamics (SPH) models for avalanches are extended ...
International audienceThis work focuses on the use of thin-layer models for simulating fast gravitat...