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2
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0039092608
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D. Bensimon, L. Kadanoff, S. Liang, B.I. Shraiman, and C. Tang, Rev. Mod. Phys. 58, 977 (1986).
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(1986)
Rev. Mod. Phys.
, vol.58
, pp. 977
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Bensimon, D.1
Kadanoff, L.2
Liang, S.3
Shraiman, B.I.4
Tang, C.5
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6
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85036155802
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J.S. Langer Chance and Matter, edited by J. Souletie, J. Vannimenus, and R. Stora, Les Houches (North-Holland, Amsterdam, 1987)
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J.S. Langer Chance and Matter, edited by J. Souletie, J. Vannimenus, and R. Stora, Les Houches (North-Holland, Amsterdam, 1987).
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7
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85036248052
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P. Pelcé, Dynamics of Curved Fronts, Perspectives in Physics (Academic Press, New York, 1988)
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P. Pelcé, Dynamics of Curved Fronts, Perspectives in Physics (Academic Press, New York, 1988).
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17
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0000772856
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R. Combescot, T. Dombre, V. Hakim, Y. Pomeau, and A. Pumir, Phys. Rev. Lett. 56, 2036 (1986).
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(1986)
Phys. Rev. Lett.
, vol.56
, pp. 2036
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Combescot, R.1
Dombre, T.2
Hakim, V.3
Pomeau, Y.4
Pumir, A.5
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37
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85036134619
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For interfaces symmetric with respect to the central axis of the channel our formulation also describes periodic boundary conditions, that is, an infinite array of fingers
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For interfaces symmetric with respect to the central axis of the channel our formulation also describes periodic boundary conditions, that is, an infinite array of fingers.
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38
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85036248976
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This region can move differently from the (Formula presented) (zero) once the second inner region discussed below has impacted the unit disk. We do not consider this possibility here
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This region can move differently from the (Formula presented) (zero) once the second inner region discussed below has impacted the unit disk. We do not consider this possibility here.
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39
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85036254879
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Although the daughter singularity is said to impact the unit disk when (Formula presented) the singularities comprising the cluster do not actually impinge upon the unit disk. However, at (Formula presented) the singularities are close enough to influence the interface shape, in the sense that (Formula presented)
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Although the daughter singularity is said to impact the unit disk when (Formula presented) the singularities comprising the cluster do not actually impinge upon the unit disk. However, at (Formula presented) the singularities are close enough to influence the interface shape, in the sense that (Formula presented)
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40
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85036407526
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The steady state with (Formula presented) is unstable to tip splitting modes, although specifying the initial value problem in the extended complex plane precludes the presence of noise needed to activate the instability
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The steady state with (Formula presented) is unstable to tip splitting modes, although specifying the initial value problem in the extended complex plane precludes the presence of noise needed to activate the instability.
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41
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85036406537
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It is noted that the (Formula presented) interfacial profile and the projection profile do differ significantly in small scale features. This is another indication of the difficulties in using zero-surface-tension solutions to describe, even qualitatively, the finite surface tension dynamics
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It is noted that the (Formula presented) interfacial profile and the projection profile do differ significantly in small scale features. This is another indication of the difficulties in using zero-surface-tension solutions to describe, even qualitatively, the finite surface tension dynamics.
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