2005
DOI: 10.1090/s0033-569x-05-00961-8
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Delta-shock wave type solution of hyperbolic systems of conservation laws

Abstract: Abstract. For two classes of hyperbolic systems of conservation laws new definitions of a δ-shock wave type solution are introduced. These two definitions give natural generalizations of the classical definition of the weak solutions. It is relevant to the notion of δ-shocks. The weak asymptotics method developed by the authors is used to describe the propagation of δ-shock waves to the three types of systems of conservation laws and derive the corresponding Rankine-Hugoniot conditions for δ-shocks.

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Cited by 143 publications
(151 citation statements)
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“…The convolution in (18) is justified by the fact (12) is a state law and, as such, is physically valid only in space regions larger than those in which the basic conservation laws (10,11) are valid. An explanation is needed to justify the convolution in (18). The formulas (15,16) state that the conservation laws of mass and momentum are valid in the cells of length .…”
Section: Approximate Solutions To the System Of Isothermal Gases And mentioning
confidence: 99%
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“…The convolution in (18) is justified by the fact (12) is a state law and, as such, is physically valid only in space regions larger than those in which the basic conservation laws (10,11) are valid. An explanation is needed to justify the convolution in (18). The formulas (15,16) state that the conservation laws of mass and momentum are valid in the cells of length .…”
Section: Approximate Solutions To the System Of Isothermal Gases And mentioning
confidence: 99%
“…The formulas (15,16) state that the conservation laws of mass and momentum are valid in the cells of length . These conservation laws are known to hold at a very small scale close to the molecular scale; maybe can be of the order of magnitude of 10 −8 m. On the other hand, the state law p = Kρ is valid only at the order of magnitude of the measurement apparatus and in absence of strong irregularities such as shock waves, or a slight extrapolation at smaller order, maybe at a magnitude not smaller than 10 −3 m represented in (18) by α in the convolution. This is the theoretical reason for which this convolution and α , 0 < α < 1, are introduced.…”
Section: Approximate Solutions To the System Of Isothermal Gases And mentioning
confidence: 99%
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