arXiv subjects

Rui Luo

Publications and source records attributed to Rui Luo.

118 records · Page 7Linked to original sources

arXiv2018

Semi-nonlinear nanophotonic waveguides for highly efficient second-harmonic generation

Quadratic optical parametric processes form the foundation for a variety of applications related to classical and quantum frequency conversion, which have attracted significant interest recently in on-chip implementation. These processes rely on phase matching among the interacting guided modes, and refractive index engineering has been a primary approach for this purpose. Unfortunately, the modal phase matching approaches developed so far only produce parametric generation with fairly low efficiencies, due to the intrinsic modal mismatch of spatial symmetries. Here we propose a universal design and operation principle for highly efficient optical parametric generation on integrated photonic platforms. By introducing spatial symmetry breaking into the optical nonlinearity of the device, we are able to dramatically enhance the nonlinear parametric interaction to realize an extremely high efficiency. We employ this approach to design and fabricate a heterogeneous titanium oxide/lithium niobate nanophotonic waveguide that is able to offer second-harmonic generation with a theoretical conversion efficiency as high as 2900% W$^{-1}$cm$^{-2}$, which enables us to experimentally achieve a conversion efficiency of 36.0% W$^{-1}$ in a waveguide only 2.35 mm long, corresponding to a recorded normalized efficiency of 650% W$^{-1}$cm$^{-2}$ that is significantly beyond the reach of conventional modal phase matching approaches. Unlike nonlinearity domain engineering that is material selective, the proposed operation principle can be flexibly applied to any other on-chip quadratic nonlinear platform to support ultra-highly efficient optical parametric interactions, thus opening up a great avenue towards extreme nonlinear and quantum optics with great potentials for broad applications in energy efficient nonlinear and quantum photonic signal processing.

physics.optics↗

arXiv2018

On the normalised FRB luminosity function

Thirty-three fast radio bursts (FRBs) had been detected by March 2018. Although the sample size is still limited, meaningful statistical studies can already be carried out. The normalised luminosity function places important constraints on the intrinsic power output, sheds light on the origin(s) of FRBs, and can guide future observations. In this paper, we measure the normalised luminosity function of FRBs. Using Bayesian statistics, we can naturally account for a variety of factors such as receiver noise temperature, bandwidth, and source selection criteria. We can also include astronomical systematics, such as host galaxy dispersion measure, FRB local dispersion measure, galaxy evolution, geometric projection effects, and Galactic halo contribution. Assuming a Schechter luminosity function, we show that the isotropic luminosities of FRBs have a power-law distribution that covers approximately three orders of magnitude, with a power-law index ranging from $-1.8$ to $-1.2$ and a cut off $\sim 2\times 10^{44}\,\rm erg\,s^{-1}$. By using different galaxy models and well-established Bayesian marginalisation techniques, we show that our conclusions are robust against unknowns, such as the electron densities in the Milky Way halo and the FRB environment, host galaxy morphology, and telescope beam response.

astro-ph.HE↗

arXiv2018

High-Q two-dimensional lithium niobate photonic crystal slab nanoresonators

Lithium niobate (LN), known as "silicon of photonics," exhibits outstanding material characteristics with great potential for broad applications. Enhancing light-matter interaction in the nanoscopic scale would result in intriguing device characteristics that enable revealing new physical phenomena and realizing novel functionalities inaccessible by conventional means. High-Q two dimensional (2D) photonic crystal (PhC) slab nanoresonators are particularly suitable for this purpose, which, however, remains open challenge to be realized on the lithium niobate platform. Here we take an important step towards this direction, demonstrating 2D LN PhC slab nanoresonators with optical Q as high as $3.51 \times 10^5$, about three orders of magnitude higher than other 2D LN PhC structures reported to date. The high optical quality, tight mode confinement, together with pure polarization characteristics of the devices enable us to reveal peculiar anisotropy of photorefraction quenching and unique anisotropic thermo-optic nonlinear response, which have never been reported before. They also allow us to observe third harmonic generation for the first time in on-chip LN nanophotonic devices, and strong orientation-dependent generation of second harmonic. The demonstrated high-Q 2D LN PhC nanoresonators not only offer an excellent device platform for the exploration of extreme nonlinear and quantum optics at single-photon and few-photon level, but also open up a great avenue towards future development of large-scale integrated LN photonic circuits for energy efficient nonlinear photonic and electro-optic signal processing.

physics.optics↗

arXiv2018

Highly-tunable efficient second-harmonic generation in a lithium niobate nanophotonic waveguide

Highly-tunable coherent light generation is crucial for many important photonic applications. Second-harmonic generation (SHG) is a dominant approach for this purpose, which, however, exhibits a trade-off between the conversion efficiency and the wavelength tunability in a conventional nonlinear platform. Recent development of the integrated lithium niobate (LN) technology makes it possible to achieve a large wavelength tuning while maintaining a high conversion efficiency. Here we report on-chip SHG that simultaneously achieves a large tunability and a high conversion efficiency inside a single device. We utilize the unique strong thermo-optic birefringence of LN to achieve flexible temperature tuning of type-I inter-modal phase matching. We experimentally demonstrate spectral tuning with a tuning slope of 0.84 nm/K for a telecom-band pump, and a nonlinear conversion efficiency of 4.7% W$^{-1}$, in a LN nanophotonic waveguide only 8~mm long. Our device shows great promise for efficient on-chip wavelength conversion to produce highly-tunable coherent visible light for broad applications, while taking advantage of the mature and cost-effective telecom laser technology.

physics.optics↗

arXiv2017

FRB 121102: a star quake-induced repeater?

Since its initial discovery, the Fast radio burst (FRB) FRB 121102 has been found to be repeating with millisecond-duration pulses. Very recently, 15 new bursts were detected by the Green Bank Telescope (GBT) during its continous monitoring observations. In this letter, we show that the burst energy distribution has a power law form which is very similar to the Gutenberg-Richter law of earthquakes. In addition, the waiting time of the burst has a Gaussian distribution, which is also a distinctive feature of earthquakes. These findings suggest that the repeating FRB pulses may originate from the starquakes of a pulsar. Noting that the soft gamma-ray repeaters (SGRs) also exhibit such distributions, the FRB could be powered by some mechanism associated with the SGRs, including crustal acitivity of a magnetar, solidification-induced stresss of a young strangeon star, and oscillation-drivern magnetic activities of a slowly rotating pulsar. These conjectures could be tested with more repeating samples.

astro-ph.HE↗

arXiv2017

High-quality lithium niobate photonic crystal nanocavities

Lithium niobate (LN) exhibits unique material characteristics that have found many important applications. Scaling LN devices down to a nanoscopic scale can dramatically enhance light-matter interaction that would enable nonlinear and quantum photonic functionalities beyond the reach of conventional means. However, developing LN-based nanophotonic devices turns out to be nontrivial. Although significant efforts have been devoted in recent years, LN photonic crystal structures developed to date exhibit fairly low quality. Here we demonstrate LN photonic crystal nanobeam resonators with optical Q as high as 10^5, more than two orders of magnitude higher than other LN nanocavities reported to date. The high optical quality together with tight mode confinement leads to extremely strong nonlinear photorefractive effect, with a resonance tuning rate of 0.64 GHz/aJ, or equivalently 84 MHz/photon, three orders of magnitude greater than other LN resonators. In particular, we observed intriguing quenching of photorefraction that has never been reported before. The devices also exhibit strong optomechanical coupling with gigahertz nanomechanical mode with a significant f*Q product of 1.47*10^12 Hz. The demonstration of high-Q LN photonic crystal nanoresonators paves a crucial step towards LN nanophotonics that could integrate the outstanding material properties with versatile nanoscale device engineering for diverse intriguing functionalities.

physics.optics↗

arXiv2017

Large host-galaxy dispersion measure of fast radio bursts

Fast radio bursts (FRBs) have excessive dispersion measures (DMs) and an all-sky distribution, which point toward an extragalactic or even a cosmological origin. We develop a method to extract the mean host galaxy DM ($\left\langle{\rm DM_{HG,loc}}\right\rangle$) and the characterized luminosity ($L$) of FRBs using the observed DM-Flux data, based on the assumption of a narrow luminosity distribution. Applying Bayesian inference to the data of 21 FRBs, we derive a relatively large mean host DM, i.e. $\left\langle{\rm DM_{HG,loc}}\right\rangle \sim 270~\rm{pc~cm^{-3}}$ with a large dispersion. A relatively large ${\rm DM_{HG}}$ of FRBs is also supported by the millisecond scattering times of some FRBs and the relatively small redshift $z=0.19273$ of FRB 121102 (which gives ${\rm DM_{HG,loc}} \sim 210 ~\rm{pc~cm^{-3}}$). The large host galaxy DM may be contributed by the ISM or a near-source plasma in the host galaxy. If it is contributed by the ISM, the type of the FRB host galaxies would not be Milky Way (MW)-like, consistent with the detected host of FRB 121102. We also discuss the possibility of having a near-source supernova remnant (SNR), pulsar wind nebula (PWN) or HII region that gives a significant contribution to the observed ${\rm DM_{HG}}$.

astro-ph.HE↗

arXiv2016

Learning text representation using recurrent convolutional neural network with highway layers

Recently, the rapid development of word embedding and neural networks has brought new inspiration to various NLP and IR tasks. In this paper, we describe a staged hybrid model combining Recurrent Convolutional Neural Networks (RCNN) with highway layers. The highway network module is incorporated in the middle takes the output of the bi-directional Recurrent Neural Network (Bi-RNN) module in the first stage and provides the Convolutional Neural Network (CNN) module in the last stage with the input. The experiment shows that our model outperforms common neural network models (CNN, RNN, Bi-RNN) on a sentiment analysis task. Besides, the analysis of how sequence length influences the RCNN with highway layers shows that our model could learn good representation for the long text.

cs.CL↗

arXiv2015

Multicolor Bound Soliton Molecule

We show a new class of bound soliton molecule that exists in a parametrically driven nonlinear optical cavity with appropriate dispersion characteristics. The composed solitons exhibit distinctive colors but coincide in time and share a common phase, bound together via strong inter-soliton four-wave mixing and Cherenkov radiation. The multicolor bound soliton molecule shows intriguing spectral locking characteristics and remarkable capability of spectrum management to tailor soliton frequencies, which may open up a great avenue towards versatile generation and manipulation of multi-octave spanning phase-locked Kerr frequency combs, with great potential for applications in frequency metrology, optical frequency synthesis, and spectroscopy.

physics.optics↗

arXiv2005

An approximate solution for solar and supernova neutrino oscillation in matter

By using Laplace transformation we developed an approximate solution to describe neutrino oscillation probabilities in arbitrary density matter. We show that this approximation solution is valid when matter potential V satisfy $V< Δm^2/2E$ and $\int VL<1$, where $L$ is the length of the neutrino oscillation . Thus, the formula is useful for propagation of the solar or supernova neutrinos with terrestrial matter effect.

hep-ph↗