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Origin of linewidth broadening? Frequency fluctuations!

Why is the linewidth broadened ? Phasenoise is the parameter that any engineer will ask you to provide in order to evaluate the performance and to define possible applications for an oscillator. From theory [Kim, Slavin], phase noise is a major contribution to linewidth broadening and linewidth is thus a good first indicator for phase noise performance. The phase φ and frequency ƒare directly related by 2πƒ=dφ/dt, so phase and frequency noise are as well. Hence, if the frequency of the oscillator fluctuates, evidently the linewidth will be enlarged.
How to measure frequency fluctuations ? A first approach to understand the origin of linewidth broadening and of phase noise is to demonstrate that the frequency is not constant, but fluctuates in time. This can already be seen when studying the emission peak on a spectrum analyzer and reducing the number of averages and the scan time [1]. Subsequent registrations of the signal will show that the centre frequency changes from one scan to the next. How can we better demonstrate this ? Fluctuations are stochastic processes and thus require time resolved experiments. So, instead of using a spectrum analyzer we need a fast single shot oscilloscope of sufficient vertical resolution [1, 2].
Evidence of frequency fluctuations in Magnetic Tunnel Junction Oscillators (Hitachi) :

 

 

 

fig2

Timescale of frequency fluctuations

From the spectrogram one would estimate a fluctuation time of a few tens of nanoseconds. However this timescale is related to the analysis technique. In fact frequency fluctuations exist on all timescales (ms to ns) and are indeed better described by a white noise. This has been demonstrated in further experiments by our group [3] when extracting phase and amplitude noise (see the corresponding section on Phase and Amplitude Noise).
SPINTEC Publications

[1] D. Houssemeddine, PhD Thesis September 2009, http://tel.archives-ouvertes.fr

[2] Phys. Rev. Lett. 102, 257202 (2009), D. Houssameddine et al.

[3] Appl. Phys. Lett. 97, 182507 (2010), M. Quinsat et al.
Main contributors:

 

References

 

[Kim] Phys. Rev. Lett. 100, 017207 (2008), J.-V. Kim et al;

[Slavin] IEEE Trans. Magn. 45, 1875 (2009), A. N. Slavin et al;

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