Formula for Entropy Solutions of the 1D Pressureless Euler–Poisson System: Well-Posedness of Entropy Solutions and the Asymptotic Behavior

We consider the Cauchy problem for the one-dimensional pressureless Euler–Poisson system, which describes dust stars with density being a finite Radon measure. For this Cauchy problem, we introduce three generalized potentials to establish a representation formula for entropy solutions, and prove the uniqueness of entropy solutions via the variational principle and the method of generalized characteristics. Furthermore, we employ this newly derived formula to analyze the asymptotic behavior of entropy solutions: For the initial data $$(\rho_0,u_0)$$ with finite Radon measure density $$\rho_0\,({\not\equiv 0})$$ and bounded velocity $$u_0$$ , we prove that the entropy solutions always decay to a single $$\delta$$ -shock by showing that any two $$\delta$$ -shocks must coincide with each other outside a finite time interval; in particular, it is interesting that, for the initial density with a nonempty compact support, the entropy solution will turn into a $$\delta$$ -shock wave in finite time, after which this $$\delta$$ -shock wave will propagate linearly despite the characteristics in general are parabolas.

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Publication Details

Journal
Proceedings of the Steklov Institute of Mathematics
Published
2025-09-01
DOI
https://doi.org/10.1134/s0081543825601236
Primary Topic
Navier-Stokes equation solutions
Type
article
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article

Formula for Entropy Solutions of the 1D Pressureless Euler–Poisson System: Well-Posedness of Entropy Solutions and the Asymptotic Behavior

Feimin Huang, Guirong Tang, Gaowei Cao
Proceedings of the Steklov Institute of Mathematics
Navier-Stokes equation solutions
article

Formula for Entropy Solutions of the 1D Pressureless Euler–Poisson System: Well-Posedness of Entropy Solutions and the Asymptotic Behavior

Feimin Huang, Guirong Tang, Gaowei Cao
article en

Abstract

We consider the Cauchy problem for the one-dimensional pressureless Euler–Poisson system, which describes dust stars with density being a finite Radon measure. For this Cauchy problem, we introduce three generalized potentials to establish a representation formula for entropy solutions, and prove the uniqueness of entropy solutions via the variational principle and the method of generalized characteristics. Furthermore, we employ this newly derived formula to analyze the asymptotic behavior of entropy solutions: For the initial data $$(\rho_0,u_0)$$ with finite Radon measure density $$\rho_0\,({\not\equiv 0})$$ and bounded velocity $$u_0$$ , we prove that the entropy solutions always decay to a single $$\delta$$ -shock by showing that any two $$\delta$$ -shocks must coincide with each other outside a finite time interval; in particular, it is interesting that, for the initial density with a nonempty compact support, the entropy solution will turn into a $$\delta$$ -shock wave in finite time, after which this $$\delta$$ -shock wave will propagate linearly despite the characteristics in general are parabolas.

Proceedings of the Steklov Institute of MathematicsVol. 330(1)
Chinese Academy of Sciences (CN), Wuhan Institute of Physics and Mathematics (CN), Academy of Mathematics and Systems Science (CN), University of Chinese Academy of Sciences (CN)
Openalex Percentile: Top 19%
Navier-Stokes equation solutions
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