Similarity Properties and Scaling Laws of Radiation Hydrodynamic Flows in Laboratory Astrophysics

TL;DR

This paper develops a comprehensive framework using Lie-group theory to analyze and establish scaling laws for radiation hydrodynamic flows in laboratory astrophysics, enabling experimental exploration of astrophysical phenomena.

Contribution

It introduces a systematic Lie-group based method to derive scaling laws across different radiating regimes in laboratory astrophysics, unifying recent advances and identifying new similarity concepts.

Findings

Complete analysis of radiating regimes using Lie-group formalism

Unified scaling laws for optically thin and thick regimes

Demonstrates experimental feasibility of astrophysical phenomena simulation

Abstract

The spectacular recent development of modern high-energy density laboratory facilities which concentrate more and more energy in millimetric volumes allows the astrophysical community to reproduce and to explore, in millimeter-scale targets and during very short times, astrophysical phenomena where radiation and matter are strongly coupled. The astrophysical relevance of these experiments can be checked from the similarity properties and especially scaling laws establishment, which constitutes the keystone of laboratory astrophysics. From the radiating optically thin regime to the so-called optically thick radiative pressure regime, we present in this paper, for the first time, a complete analysis of the main radiating regimes that we encountered in laboratory astrophysics with the same formalism based on the Lie-group theory. The use of the Lie group method appears as systematic which allows to construct easily and orderly the scaling laws of a given problem. This powerful tool permits to unify the recent major advances on scaling laws and to identify new similarity concepts that we discuss in this paper and which opens important applications for the present and the future laboratory astrophysics experiments. All these results enable to demonstrate theoretically that astrophysical phenomena in such radiating regimes can be explored experimentally thanks to powerful facilities. Consequently the results presented here are a fundamental tool for the high-energy density laboratory astrophysics community in order to quantify the astrophysics relevance and justify laser experiments. Moreover, relying on the Lie-group theory, this paper constitutes the starting point of any analysis of the self-similar dynamics of radiating fluids.