Observation of sub-relativistic collisionless shock generation and breakout dynamics

Relativistic collisionless shocks, which are ubiquitous in the cosmos, play a significant role in various astrophysical phenomena such as gamma-ray bursts, PeVatrons, and supernova shock breakouts. Here we present a demonstration using a compact femtosecond laser system to generate sub-relativistic collisionless shocks (0.03c) under astrophysically relevant conditions. We attribute the shock formation to a rapidly growing Weibel instability in a precisely tuning low-density preplasma environment, which resembles the interstellar media near an astrophysical central engine. Owing to this Weibel instability, a 5000 Tesla magnetic field is developed within 2.7 ps, leading to the collisionless shock formation and subsequent breakout at the preplasma boundaries. This platform enables direct investigation of astrophysics related to relativistic collisionless shocks. The achieved parameters bridge the gap between astrophysical observations and controlled laboratory experiments, offering unprecedented opportunities to validate cosmic shock models.

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Publication Details

Journal
Nature Communications
Published
2025-04-28
DOI
https://doi.org/10.1038/s41467-025-58867-3
Citations
5
Primary Topic
Laser-Plasma Interactions and Diagnostics
Type
article
Field-Weighted Citation Impact
9.35

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article

Observation of sub-relativistic collisionless shock generation and breakout dynamics

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5 citations
Nature Communications
Laser-Plasma Interactions and Diagnostics
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article

Observation of sub-relativistic collisionless shock generation and breakout dynamics

Yafeng Bai, Ye Tian, Ruxin Li, Liwei Song, Yushan Zeng, Dongdong Zhang, J. Mao
article en
5 citations

Abstract

Relativistic collisionless shocks, which are ubiquitous in the cosmos, play a significant role in various astrophysical phenomena such as gamma-ray bursts, PeVatrons, and supernova shock breakouts. Here we present a demonstration using a compact femtosecond laser system to generate sub-relativistic collisionless shocks (0.03c) under astrophysically relevant conditions. We attribute the shock formation to a rapidly growing Weibel instability in a precisely tuning low-density preplasma environment, which resembles the interstellar media near an astrophysical central engine. Owing to this Weibel instability, a 5000 Tesla magnetic field is developed within 2.7 ps, leading to the collisionless shock formation and subsequent breakout at the preplasma boundaries. This platform enables direct investigation of astrophysics related to relativistic collisionless shocks. The achieved parameters bridge the gap between astrophysical observations and controlled laboratory experiments, offering unprecedented opportunities to validate cosmic shock models.

Nature CommunicationsVol. 16(1)
Shanghai Zhangjiang Laboratory (CN), Shanghai Institute of Optics and Fine Mechanics (CN), University of Chinese Academy of Sciences (CN)
Natural Science Foundation of Shanghai, National Natural Science Foundation of China, Chinese Academy of Sciences, Youth Innovation Promotion Association of the Chinese Academy of Sciences, Chinese Academy of Sciences, Shanghai Branch, Youth Innovation Promotion Association
Climate action
Openalex Percentile: Top 3%
Laser-Plasma Interactions and Diagnostics
9.35
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