Dynamic instabilities of microwaves generated with optoelectronic oscillators

3 pages.-- OCIS codes: 120.3940, 190.3100, 350.4010.-- Final full-text version of the paper available at: http://dx.doi.org/10.1364/OL.32.002571.We introduce a time-domain model to study the dynamics of optoelectronic oscillators. We show that, due to the interaction between nonlinearity and time delay, the envelope amplitude of ultrapure microwaves generated by optoelectronic oscillators can turn unstable when the gain is increased beyond a given critical value. Our analytical predictions are confirmed by numerical simulations and experiments.Y. K. C. acknowledges a research grant from the Govern de les Illes Balears. Financial support from EC project PICASSO IST-2005-34551, MEC (Spain) and FEDER project TEC2006-1009/MIC (PhoDECC) is also acknowledged

Application of the optical fiber to generation and measurement of low phase noise microwaves

International audienceThe optical delay line proved to be a method to measure the phase noise of microwave oscillators with high sensitivity. The delay, inherently, turns frequency fluctuations into phase fluctuations. Hence, a mixer is used to compare the phase of the oscillator signal to a delayed copy, from which we measure the oscillator phase noise. This article reports on the progress in this type of instruments in our laboratory. For practical reasons, the delay is implemented with an optical-fiber channel, either at 1.3 or 1.55 µm wavelength, modulated in intensity. The laser Relative Intensity Noise (RIN) turns out to be a critical parameter because it converts the RIN into near DC noise through the mixer offset sensitivity to power. The best semiconductor lasers we can find show a RIN of about -155 dB/Hz. Additionally, in our experience the simple microwave photodiodes are to be preferred to the photodiodes with integrated transconductance amplifier because of the lower noise. This seems to be a technical issue, rather than a general property. Thus, we used a separate amplifier, based on SiGe technology for lowest flicker. The optical fiber is temperature stabilized by an Aluminum mass and a sub-milliKelvin electronic control. Other components, like the Mach Zehnder intensity modulator, seem to be less critical for noise. A single channel version was realized and tested with a microwave synthesizer and with a sapphire whispering gallery oscillator at 10 GHz carrier frequency. Using a 2 km delay line (Τ=10 µs) the measured 1/f3 noise is b-3 = -12 dB.rad²/Hz, which matches the a-priori knowledge of the oscillator 1/f3 noise. This means that the instrument sensitivity is higher than this value, thus it is sufficient to measure a room-temperature sapphire oscillator without need of correlation. At higher Fourier frequencies, the instrument background noise is of -145 dBrad²/Hz at 10 kHz off the carrier. Unfortunately, with other source types (eg, a synthesizer) the background noise can be higher because of the effect of am noise. Another test of the noise floor consists of shortening the optical delay to a negligible value. In this way, the oscillator noise is rejected. Unfortunately, this is only a qualitative test because it hides the noise of the optical fiber, due to Rayleigh scattering and other optical phenomena. The background noise is reduced proportionally to 1/√m, where m is the number of averaged spectra, by correlation and averaging on two fully independent channels that measure the same oscillator. Using 2 km optical fibers and averaging on 200 spectra, the background noise is of -110 dBrad²/Hz at 100 Hz off the carrier, and of -160 dBrad²/Hz at 10 kHz. Re-using the parts of the two-channel system, we assemble single-channel system with matched 10 µs optical delays at the two inputs of the mixer, which rejects the noise of the oscillator. The 1/f noise measured in this condition, b-1 = -113 dBrad²/Hz referred to one channel, is the background noise of the system without correlation, which includes amplifiers, detector and optical fiber

Optical mini-disk resonator integrated into a compact optoelectronic oscillator

Original de l'article en libre accès sur le site d'Acta Polonica Physica A http://przyrbwn.icm.edu.pl/APP/SPIS/a116-4.html au lien suivant: http://przyrbwn.icm.edu.pl/APP/PDF/116/a116z465.pdfInternational audienceThis work consists in the design, fabrication and characterization of mini-disk MgF2 resonators for integration into optoelectronic oscillator and first experimental results of implementation in microwave free spectral range oscillator with taper coupling optoelectronic oscillator

Optical disk resonator with microwave free spectral range for optoelectronic oscillator

International audienceWe report on MgF2 optical whispering gallery mode resonators, intended to operate in an optoelectronic microwave oscillator. We describe the definition of the physical and geometrical properties of the disk shape resonator, the fabrication process, and finally the mechanical and optical characterization obtained with the first fabricated devices. For the MgF2 disk, an optical quality factor of Q = 3.2 × 10^8 was measured at the telecoms wavelength lambda = 1.55 μm, and with a coupling performed through a tapered fiber

Applications of the optical fiber to the generation and to the measurement of low-phase-noise microwave signals

The optical fiber used as a microwave delay line exhibits high stability and low noise and makes accessible a long delay (>100 microseconds) in a wide bandwidth (about 40 GHz, limited by the optronic components). Hence, it finds applications as the frequency reference in microwave oscillators and as the reference discriminator for the measurement of phase noise. The fiber is suitable to measure the oscillator stability with a sensitivity of parts in 1E-12. Enhanced sensitivity is obtained with two independent delay lines, after correlating and averaging. Short-term stability of parts in 1E-12 is achieved inserting the delay line in an oscillator. The frequency can be set in steps multiple of the inverse delay, which is in the 10-100 kHz region. This article adds to the available references a considerable amount of engineering and practical knowledge, the understanding of 1/f noise, calibration, the analysis of the cross-spectrum technique to reduce the instrument background, the phase-noise model of the oscillator, and the experimental test of the oscillator model.Comment: 23 pages, 13 figures, 41 reference

Quasi-linear Masking to Protect Kyber against both SCA and FIA

The recent technological advances in Post-Quantum Cryptography (PQC) rise the questions of robust implementations of new asymmetric cryptographic primitives in today’s technology. This is the case for the lattice-based CRYSTALS-Kyber algorithm which has been selected as the first NIST standard for Public Key Encryption (PKE) and Key Encapsulation Mechanisms (KEM). We have notably to make sure the Kyber implementation is resilient against physical attacks like Side-Channel Analysis (SCA) and Fault Injection Attacks (FIA). To reach this goal, we propose to use the masking countermeasure, more precisely the generic Direct Sum Masking method (DSM). By taking inspiration of a previous paper on AES, we extend the method to finite fields of characteristic prime other than 2 and even-length codes. In particular, we investigated its application to Keccak, which is the hash-based function used in Kyber. We also provided the first masked implementation of Kyber providing both SCA and FIA resilience while not requiring any conversion between different masking methods

Hot Carrier Solar Cell: From Simulation to Devices

International audienceSingle junction III-V heterostructures based devices could overtake the Shockley-Queisser limit if thermalisation of photogenerated carriers can be strongly limited as in the hot carrier solar cell concept. Previous modelling and experiments have shown the interest of Multiple Quantum Wells heterostructures in the antimonide system and the importance of very thin structures. In this paper we report new data on the thermalisation rates in antimonide and phosphide heterostructures measured at ambient temperature. For the first time electrical control of hot carrier population is performed on hot carrier heterostructures device

Dominant-negative mutations in human IL6ST underlie hyper-IgE syndrome

Autosomal dominant hyper-IgE syndrome (AD-HIES) is typically caused by dominant-negative (DN) STAT3 mutations. Patients suffer from cold staphylococcal lesions and mucocutaneous candidiasis, severe allergy, and skeletal abnormalities. We report 12 patients from 8 unrelated kindreds with AD-HIES due to DN IL6ST mutations. We identified seven different truncating mutations, one of which was recurrent. The mutant alleles encode GP130 receptors bearing the transmembrane domain but lacking both the recycling motif and all four STAT3-recruiting tyrosine residues. Upon overexpression, the mutant proteins accumulate at the cell surface and are loss of function and DN for cellular responses to IL-6, IL-11, LIF, and OSM. Moreover, the patients’ heterozygous leukocytes and fibroblasts respond poorly to IL-6 and IL-11. Consistently, patients with STAT3 and IL6ST mutations display infectious and allergic manifestations of IL-6R deficiency, and some of the skeletal abnormalities of IL-11R deficiency. DN STAT3 and IL6ST mutations thus appear to underlie clinical phenocopies through impairment of the IL-6 and IL-11 response pathways

Reception Test of Petals for the End Cap TEC+ of the CMS Silicon Strip Tracker

The silicon strip tracker of the CMS experiment has been completed and was inserted into the CMS detector in late 2007. The largest sub system of the tracker are its end caps, comprising two large end caps (TEC) each containing 3200 silicon strip modules. To ease construction, the end caps feature a modular design: groups of about 20 silicon modules are placed on sub-assemblies called petals and these self-contained elements are then mounted onto the TEC support structures. Each end cap consists of 144 such petals, which were built and fully qualified by several institutes across Europe. Fro