Laboratory Observation of Radiative Shock Deceleration and Application to SN 1987A

被引:6
|
作者
Michel, Th [1 ]
Albertazzi, B. [1 ]
Mabey, P. [1 ]
Rigon, G. [1 ]
Lefevre, F. [1 ]
Some, L. Van Box [2 ]
Barroso, P. [3 ]
Egashira, S. [4 ]
Kumar, R. [4 ]
Michaut, C. [5 ]
Ota, M. [4 ]
Ozaki, N. [4 ,6 ]
Sakawa, Y. [4 ]
Sano, T. [4 ]
Falize, E. [2 ]
Koenig, M. [1 ,6 ]
机构
[1] Sorbonne Univ, Ecole Polytech, Inst Polytech Paris, LULI CNRS, F-91128 Palaiseau, France
[2] CEA, DAM, DIF, F-91297 Arpajon, France
[3] PSL Res Univ, GEPI, Observ Paris, CNRS, 61 Ave Observ, F-75014 Paris, France
[4] Osaka Univ, Inst Laser Engn, Suita, Osaka 5650871, Japan
[5] Univ Cote dAzur, Observ Cote dAzur, CNRS, Lab Lagrange, Bd Observ,CS 34229, F-06304 Nice 4, France
[6] Osaka Univ, Grad Sch Engn, Osaka 5650871, Japan
来源
ASTROPHYSICAL JOURNAL | 2020年 / 888卷 / 01期
关键词
Laboratory astrophysics; Experimental techniques; Shocks; HOT-SPOTS; REMNANT;
D O I
10.3847/1538-4357/ab5956
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The first laboratory evidence of a radiative shock (RS) decelerating during its free expansion phase in an optically thick medium is presented. A shock is generated in a multilayer solid target under the irradiation of a high-power laser at the GEKKO XII laser facility. The rear surface of the target is connected to a gas cell filled with Xe. Upon breakout, an RS, characterized by low Boltzmann number Bo MUCH LESS-THAN 1 and Mihalas number R 10, is generated. Experimental results reveal that radiative losses through the radiative precursor cause the shock to lose energy and decelerate. A model is developed that describes the shock propagation as a function of time. The model is in agreement with both numerical simulations and experimental results. These results have tremendous consequences for astrophysical systems, such as SN 1987A, where radiative deceleration may play a role in the formation of the observed hotspots in the circumstellar ring.
引用
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页数:5
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