Experimental confirmation of the standard magnetorotational instability mechanism with a spring-mass analogue
Autor: | Hantao Ji, Eric G. Blackman, Kyle Caspary, Erik P. Gilson, Derek M. H. Hung |
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Jazyk: | angličtina |
Rok vydání: | 2019 |
Předmět: |
Angular momentum
General Physics and Astronomy FOS: Physical sciences lcsh:Astrophysics Kinetic energy 01 natural sciences Magnetorotational instability 0103 physical sciences lcsh:QB460-466 010306 general physics 010303 astronomy & astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Solar and Stellar Astrophysics (astro-ph.SR) Physics High Energy Astrophysical Phenomena (astro-ph.HE) Fluid Dynamics (physics.flu-dyn) Fluid mechanics Mechanics Plasma Physics - Fluid Dynamics Accretion (astrophysics) lcsh:QC1-999 Magnetic field Stars Astrophysics - Solar and Stellar Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics Astrophysics - High Energy Astrophysical Phenomena lcsh:Physics |
Zdroj: | Communications Physics, Vol 2, Iss 1, Pp 1-7 (2019) |
ISSN: | 2399-3650 |
DOI: | 10.1038/s42005-018-0103-7 |
Popis: | The Magnetorotational Instability (MRI) has long been considered a plausibly ubiquitous mechanism to destabilize otherwise stable Keplerian flows to support radially outward transport of angular momentum. Such an efficient transport process would allow fast accretion in astrophysical objects such as stars and black holes to release copious kinetic energy that powers many of the most luminous sources in the universe. But the standard MRI under a purely vertical magnetic field has heretofore never been directly measured despite numerous efforts over more than a decade. Here we report an unambiguous laboratory demonstration of the spring-mass analogue to the standard MRI by comparing motion of a spring-tethered ball within different rotating flows. The experiment corroborates the theory: efficient outward angular momentum transport manifests only for cases with a weak spring in quasi-Keperian flow. Our experimental method accomplishes this in a new way, thereby connecting solid and fluid mechanics to plasma astrophysics. Comment: 7 pages; 4 figures; accepted by Communications Physics |
Databáze: | OpenAIRE |
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