Super-harmonic injection locking of nano-contact spin-torque vortex oscillators
Super-harmonic injection locking of single nano-contact (NC) spin-torque vortex oscillators (STVOs) subject to a small microwave current has been explored. Frequency locking was observed up to the fourth harmonic of the STVO fundamental frequency \(f_{0}\) in microwave magneto-electronic measurement...
Saved in:
Published in | arXiv.org |
---|---|
Main Authors | , , , , , , |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
15.04.2016
|
Subjects | |
Online Access | Get full text |
ISSN | 2331-8422 |
DOI | 10.48550/arxiv.1604.04462 |
Cover
Summary: | Super-harmonic injection locking of single nano-contact (NC) spin-torque vortex oscillators (STVOs) subject to a small microwave current has been explored. Frequency locking was observed up to the fourth harmonic of the STVO fundamental frequency \(f_{0}\) in microwave magneto-electronic measurements. The large frequency tunability of the STVO with respect to \(f_{0}\) allowed the device to be locked to multiple sub-harmonics of the microwave frequency \(f_{RF}\), or to the same sub-harmonic over a wide range of \(f_{RF}\) by tuning the DC current. In general, analysis of the locking range, linewidth, and amplitude showed that the locking efficiency decreased as the harmonic number increased, as expected for harmonic synchronization of a non-linear oscillator. Time-resolved scanning Kerr microscopy (TRSKM) revealed significant differences in the spatial character of the magnetization dynamics of states locked to the fundamental and harmonic frequencies, suggesting significant differences in the core trajectories within the same device. Super-harmonic injection locking of a NC-STVO may open up possibilities for devices such as nanoscale frequency dividers, while differences in the core trajectory may allow mutual synchronisation to be achieved in multi-oscillator networks by tuning the spatial character of the dynamics within shared magnetic layers. |
---|---|
Bibliography: | SourceType-Working Papers-1 ObjectType-Working Paper/Pre-Print-1 content type line 50 |
ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.1604.04462 |