Efficient Highly Subsonic Turbulent Dynamo and Growth of Primordial Magnetic Fields

Author:

Achikanath Chirakkara Radhika,Federrath ChristophORCID,Trivedi Pranjal,Banerjee RobiORCID

Funder

Australian National University

Universität Hamburg

Australian Research Council

Deutsche Forschungsgemeinschaft

U.S. Department of Energy

University of Chicago

Australia-Germany Joint Research Cooperation Scheme

Leibniz Rechenzentrum

Gauss Centre for Supercomputing

GCS Large-scale

Australian National Computational Infrastructure

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Cited by 18 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Amplification and Saturation of Turbulent Magnetic Fields in Collapsing Primordial Gas Clouds;The Astrophysical Journal;2024-02-01

2. The dual role of outflows in quenching satellites of low-mass hosts: NGC 3109;Monthly Notices of the Royal Astronomical Society;2024-01-04

3. Critical magnetic Reynolds number of the turbulent dynamo in collisionless plasmas;Monthly Notices of the Royal Astronomical Society;2023-12-22

4. Role of magnetic pressure forces in fluctuation dynamo saturation;Monthly Notices of the Royal Astronomical Society;2023-11-09

5. Vorticity and magnetic dynamo from subsonic expansion waves;Astronomy & Astrophysics;2023-09

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