Abstract
The response of a magnetic fluid microdrop to a rotating magnetic field is studied for the first time. An unexpected shape instability is observed, leading to the formation of a spiny starfish shape that slowly corotates with the field. A simple model accounts for (i) the stability range of an oblate ellipsoidal shape that is a precursor to the starfish, (ii) the rotational frequency which is substantially lower than that of the applied magnetic field, and (iii) a lateral peak instability that is responsible for growth of the spiny arms of the starfish.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.