Observation of sub-relativistic collisionless shock generation and breakout dynamics

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-rela...

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Main Authors: Yafeng Bai, Dongdong Zhang, Yushan Zeng, Jiakang Mao, Liwei Song, Ye Tian, Ruxin Li
Format: Article
Language:English
Published: Nature Portfolio 2025-04-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-025-58867-3
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author Yafeng Bai
Dongdong Zhang
Yushan Zeng
Jiakang Mao
Liwei Song
Ye Tian
Ruxin Li
author_facet Yafeng Bai
Dongdong Zhang
Yushan Zeng
Jiakang Mao
Liwei Song
Ye Tian
Ruxin Li
author_sort Yafeng Bai
collection DOAJ
description 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.
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institution Kabale University
issn 2041-1723
language English
publishDate 2025-04-01
publisher Nature Portfolio
record_format Article
series Nature Communications
spelling doaj-art-c2a29af08a034ed9a5bc0c97101351052025-08-20T03:52:24ZengNature PortfolioNature Communications2041-17232025-04-011611810.1038/s41467-025-58867-3Observation of sub-relativistic collisionless shock generation and breakout dynamicsYafeng Bai0Dongdong Zhang1Yushan Zeng2Jiakang Mao3Liwei Song4Ye Tian5Ruxin Li6State Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesState Key Laboratory of Ultra-intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of SciencesAbstract 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.https://doi.org/10.1038/s41467-025-58867-3
spellingShingle Yafeng Bai
Dongdong Zhang
Yushan Zeng
Jiakang Mao
Liwei Song
Ye Tian
Ruxin Li
Observation of sub-relativistic collisionless shock generation and breakout dynamics
Nature Communications
title Observation of sub-relativistic collisionless shock generation and breakout dynamics
title_full Observation of sub-relativistic collisionless shock generation and breakout dynamics
title_fullStr Observation of sub-relativistic collisionless shock generation and breakout dynamics
title_full_unstemmed Observation of sub-relativistic collisionless shock generation and breakout dynamics
title_short Observation of sub-relativistic collisionless shock generation and breakout dynamics
title_sort observation of sub relativistic collisionless shock generation and breakout dynamics
url https://doi.org/10.1038/s41467-025-58867-3
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