Non-linear dynamics of the Richtmyer-Meshkov instability in supernovae

Snezhana I. Abarzhi; Marcus Herrmann

doi:10.1007/s10509-005-3975-4

Non-linear dynamics of the Richtmyer-Meshkov instability in supernovae

Snezhana I. Abarzhi, Marcus Herrmann

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.

Original language	English (US)
Pages (from-to)	379-383
Number of pages	5
Journal	Astrophysics and Space Science
Volume	298
Issue number	1-2
DOIs	https://doi.org/10.1007/s10509-005-3975-4
State	Published - Jun 1 2005
Externally published	Yes

Keywords

Non-local
Richtmyer-Meshkov
Singularities
Supernovae

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/s10509-005-3975-4

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title = "Non-linear dynamics of the Richtmyer-Meshkov instability in supernovae",

abstract = "We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.",

keywords = "Non-local, Richtmyer-Meshkov, Singularities, Supernovae",

author = "Abarzhi, {Snezhana I.} and Marcus Herrmann",

year = "2005",

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doi = "10.1007/s10509-005-3975-4",

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T1 - Non-linear dynamics of the Richtmyer-Meshkov instability in supernovae

AU - Abarzhi, Snezhana I.

AU - Herrmann, Marcus

PY - 2005/6/1

Y1 - 2005/6/1

N2 - We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.

AB - We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.

KW - Non-local

KW - Richtmyer-Meshkov

KW - Singularities

KW - Supernovae

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DO - 10.1007/s10509-005-3975-4

M3 - Article

AN - SCOPUS:21644478780

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SP - 379

EP - 383

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1-2

ER -

Non-linear dynamics of the Richtmyer-Meshkov instability in supernovae

Abstract

Keywords

ASJC Scopus subject areas

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