Laboratorial radiative shocks with multiple parameters and first quantifying verifications to core-collapse supernovae

We present experiments to reproduce the characteristics of core-collapse supernovae with different stellar masses and initial explosion energies in the laboratory. In the experiments, shocks are driven in 1.2 atm and 1.9 atm xenon gas by laser with energy from 1600J to 2800J on the SGIII prototype l...

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Hauptverfasser: Zhang, Lu, Zheng, Jianhua, Yang, Zhenghua, Song, Tianming, Zhang, Shuai, Liu, Tong, Wei, Yunfeng, Kuang, Longyu, Longfei Jing, Lin, Zhiwei, Li, Liling, Li, Hang, Zheng, Jinhua, Yang, Pin, Zhang, Yuxue, Zhang, Zhiyu, Zhao, Yang, He, Zhibing, Li, Ping, Yang, Dong, Yang, Jiamin, Zhao, Zongqing, Ding, Yongkun
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container_title arXiv.org
container_volume
creator Zhang, Lu
Zheng, Jianhua
Yang, Zhenghua
Song, Tianming
Zhang, Shuai
Liu, Tong
Wei, Yunfeng
Kuang, Longyu
Longfei Jing
Lin, Zhiwei
Li, Liling
Li, Hang
Zheng, Jinhua
Yang, Pin
Zhang, Yuxue
Zhang, Zhiyu
Zhao, Yang
He, Zhibing
Li, Ping
Yang, Dong
Yang, Jiamin
Zhao, Zongqing
Ding, Yongkun
description We present experiments to reproduce the characteristics of core-collapse supernovae with different stellar masses and initial explosion energies in the laboratory. In the experiments, shocks are driven in 1.2 atm and 1.9 atm xenon gas by laser with energy from 1600J to 2800J on the SGIII prototype laser facility. The average shock velocities and shocked densities are obtained from experiments. Experimental results reveal that higher laser energy and lower Xe gas density led to higher shock velocity, and lower Xe gas initial density has a higher compression. Modeling of the experiments using the 2D radiation hydrodynamic codes Icefire shows excellent agreement with the experimental results and gives the temperature. These results will contribute to time-domain astrophysical systems, such as gravitational supernovae, where a strong radiative shock propagates outward from the center of the star after the core collapses.
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subjects Compressive strength
Gas density
Gravitational collapse
Lasers
Supernovae
Xenon
title Laboratorial radiative shocks with multiple parameters and first quantifying verifications to core-collapse supernovae
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