Results 181 to 190 of about 135,634 (231)
Nonlinear flow characteristics of cement grout in fractures with varying geometries. [PDF]
Sci RepLi X, Zhao W, Zhang J, Ma Y, Chen L.
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Computational methods for inertial microfluidics: recent advances and future perspectives. [PDF]
Microsyst NanoengLauricella G +6 more
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Hemodynamic response to stent-induced aneurysm deformation in patient-specific internal carotid artery cases: A computational study. [PDF]
Sci RepRajhi W +7 more
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2003
In this chapter, we shall present a wide variety of intellectually delectable recipes involving velocity- and position-dependent forces. The resulting Newtonian equations of motion will be either linear or nonlinear ordinary differential equations (ODEs).
Richard H. Enns, George C. McGuire
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In this chapter, we shall present a wide variety of intellectually delectable recipes involving velocity- and position-dependent forces. The resulting Newtonian equations of motion will be either linear or nonlinear ordinary differential equations (ODEs).
Richard H. Enns, George C. McGuire
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Dynamics of Non-Newtonian Droplets
Physical Review Letters, 2007We study the impact and subsequent retraction dynamics of aqueous liquid droplets upon high-speed impact on hydrophobic surfaces. Often a spectacular "rebound" of the droplet can be observed: after the impact and expansion, the drop retracts rapidly, leading to ejection of part of the material from the surface. We show how non-Newtonian flow properties
Bartolo, D. +3 more
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Dynamic wetting with viscous Newtonian and non-Newtonian fluids
Journal of Physics: Condensed Matter, 2009We examine various aspects of dynamic wetting with viscous Newtonian and non-Newtonian fluids. Rather than concentrating on the mechanisms that relieve the classic contact line stress singularity, we focus on the behavior in the wedge flow near the contact line which has the dominant influence on wetting with these fluids.
Y, Wei, E, Rame, L M, Walker, S, Garoff
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American Journal of Physics, 2009
This paper describes a world in which Newton’s first and second laws hold, but Newton’s third law takes the form that the forces between any two objects are equal in magnitude and direction. The dynamics for such a system exhibit curious and unfamiliar features including chaos for two bodies in two spatial dimensions.
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This paper describes a world in which Newton’s first and second laws hold, but Newton’s third law takes the form that the forces between any two objects are equal in magnitude and direction. The dynamics for such a system exhibit curious and unfamiliar features including chaos for two bodies in two spatial dimensions.
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Dynamics in Newtonian-Riemannian space-time (IV)
Applied Mathematics and Mechanics, 2000zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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