Miracle-dz/UniFAR-FTUs huggingface dataset:
Overlaps with arbitrary two-site states in the XXZ spin chain

We present a conjectured exact formula for overlaps between the Bethe states of the spin-1/2 XXZ chain and generic two-site states. The result takes the same form as in the previously known cases: it involves the same ratio of two Gaudin-like determinants, and a product of single-particle overlap functions, which can be fixed using a combination of the quench action and quantum transfer matrix methods. Our conjecture is confirmed by numerical data from exact diagonalization. For one-site states, the formula is found to be correct even in chains with odd length. It is also pointed out that the ratio of the Gaudin-like determinants plays a crucial role in the overlap sum rule: it guarantees that in the thermodynamic limit there remains no term in the quench action.
Entanglement versus quantum degree of polarization

In this article we make a comparison between the behavior of entanglement and quantum degree of polarization for a special class of states of the radiation field, namely the Bell-type diagonal mixed states. For the three-photon mixed states we have plotted the concurrence and the Chernoff quantum degree of polarization in terms of the parameter, which defines the state. We find the the entanglement and the quantum degree of polarization are incomparable measures.
ON THE MODULATION OF RR LYRAE STARS IN THE GLOBULAR CLUSTER M3

New, extended time-series photometry of M3 RR Lyrae stars has revealed that 4 of the 10 double-mode stars show large-amplitude Blazhko modulation of both radial modes. The first, detailed analysis of the peculiar behavior of the unique, Blazhko RRd stars is given. While the P1/P0 period ratio is normal, and the overtone mode is dominant in the other RRd stars of the cluster, the period ratio is anomalous and the fundamental mode has a larger (or similar) mean amplitude than the overtone has in Blazhko RRd stars. The modulations of the fundamental and overtone modes are synchronized only in one of the Blazhko RRd stars. No evidence of any connection between the modulations of the modes in the other three stars is found. The Blazhko modulation accounts, at least partly, for the previously reported amplitude and period changes of these stars. Contrary to the ∼50% Blazhko statistics of RRab and RRd stars, Blazhko modulation occurs only in 10% of the overtone variables in M3. Four of the five Blazhko RRc stars are bright, evolved objects, and one has a period and brightness similar to those of Blazhko RRd stars. The regions of the instability strip with high and low occurrence rates of the Blazhko modulation overlap with the regions populated by first- and second-generation stars according to theoretical and observational studies, raising up the possibility that the Blazhko modulation occurs preferentially in first-generation RR Lyrae stars.
Vitamin B 12 uptake by intestinal microorganisms : mechanism and relevance to syndromes of intestinal bacterial overgrowth

This work was presented in part at a meeting of the American Federation for Clinical Research, Washington, D. C. 13 December 1969; an Abstract has been published in 1970 Gastroenterology. 58:1042. Received for publication 27 July 1970 and in revised form 16 November 1970. Km for human intrinsic factor (0.38 X 10"1M). Competition between bacteria and intrinsic factor for vitamin Bn may be inferred from the similarity of these constants. These observations suggest that a variety of enteric and nonenteric organisms, not requiring exogenous B,2, may play a role in the pathogenesis of the vitamin B,2 malabsorption found in the intestinal bacterial overgrowth syndromes.
Spectral photonic lattices with complex long-range coupling

We suggest and experimentally realize a spectral photonic lattice - a signal can hop between discrete frequency channels, driven by nonlinear interaction with stronger pump lasers. By controlling the complex envelope and frequency separations of multiple pumps, it is possible to introduce non- local hopping and to break time-reversal symmetry, which opens up new possibilities for photonic quantum simulation. As two examples, we observe a spectral quantum walk and demonstrate the discrete Talbot effect in the spectral domain, where we find novel instances containing asymmetry and periodicities not possible in spatial lattices.
Prevalence and treatment of venous thromboembolism in patients with solid tumors

Cancer-associated venous thromboembolism (VTE) has exhibited a rising incidence rate. Research focusing on cancer-associated VTE and current anticoagulation therapy strategies is limited. The present study aimed to investigate the prevalence, characteristics and anticoagulation therapy strategies of cancer-associated VTE. The study was performed on patients with major solid tumors who were admitted to The First Affiliated Hospital of Guangxi Medical University (Nanning, China) between January 2020 and December 2020. The medical records of the patients' demographic characteristics, disease and treatment were extracted from the medical record data system and reviewed. The prevalence of cancer-associated VTE was calculated, followed by statistical analysis. Patients who received anticoagulation therapy for cancer-associated VTE were followed up for 1 year. The characteristics and efficacy of anticoagulation therapy strategies were compared and analyzed. A total of 4,926 patients with major solid tumors (mean age, 55.86±11.97 years) were included in the analysis, of which 117 (2.4%; 117/4,926) were diagnosed with cancer-associated VTE. Patients with pancreatic cancer exhibited the highest prevalence of VTE (10.2%; 5/49), followed by patients with ovarian cancer (5.8%; 9/156) and lung cancer (3.3; 73/2,237). Multivariate analysis identified hypertension comorbidity [odds ratio (OR), 1.661; 95% CI, 1.031-2.674; P=0.037)] and cancer stage (OR, 1.266; 95% CI, 1.079-1.486; P=0.004) as independent risk factors for cancer-associated VTE. Deep vein thrombosis (DVT) of the lower extremity accounted for 62.0%; 62/100) of all DVTs. Moreover, pulmonary embolism (PE) with lower extremity DVT accounted for 53.5% (23/43) of all PE cases. The majority of cancer-associated VTE cases (63.2%; 74/117) developed 30 days before or after a cancer diagnosis. In addition, cancer-associated VTE was dominated by symptomatic VTE (59.8%; 70/117). Only 74.4% (87/117) of patients with VTE received anticoagulant treatment, with a median duration of 79 days. The most common anticoagulant treatment strategies were heparin during hospitalization and direct oral anticoagulants (rivaroxaban) after discharge. The anticoagulants associated with bleeding events were rivaroxaban (4.2%; 3/72) and enoxaparin (1.9%; 1/54). In total, 62.1% (36/58) of the patients received anticoagulant treatment for <90 days. In conclusion, the results indicated that the prevalence of cancer-associated VTE is common and exhibits numerous characteristics. Rivaroxaban has been widely used in cancer-associated VTE treatment. However, compliance with long-term anticoagulant treatment is not adequate at present, while the efficacy and safety of rivaroxaban must be evaluated to improve long-term medication monitoring and follow-up among patients with cancer-associated VTE.
Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectors

Earth-based gravitational-wave detectors will be limited by quantum noise in a large part of their spectrum. The most promising technique to achieve a broadband reduction of such noise is the injection of a frequency-dependent squeezed vacuum state from the output port of the detector, with the squeeze angle rotated by the reflection off a Fabry-Perot filter cavity. One of the most important parameters limiting the squeezing performance is represented by the optical losses of the filter cavity. We report here the operation of a 300 m filter cavity prototype installed at the National Astronomical Observatory of Japan. The cavity is designed to obtain a rotation of the squeeze angle below 100 Hz. After achieving the resonance of the cavity with a multiwavelength technique, the round trip losses have been measured to be between 50 and 90 ppm. This result demonstrates that with realistic assumptions on the input squeeze factor and the other optical losses, a quantum noise reduction of at least 4 dB in the frequency region dominated by radiation pressure can be achieved.
Image Quantization Towards Data Reduction: Robustness Analysis for SLAM Methods On Embedded Platforms

Embedded simultaneous localization and mapping (SLAM) aims at providing real-time performances with restrictive hardware resources of advanced perception functions. Localization methods based on visible cameras include image processing functions that require frame memory management. This work reduces the dynamic range of input frame and evaluates the accuracy and robustness of real-time SLAM algorithms with quantified frames. We show that the input data can be reduced up to 62% and 75% while maintaining a similar trajectory error lower than 0.15m compared to full precision input images.
Reconciling MOND and dark matter

Observations of galaxies suggest a one-to-one analytic relation between the inferred gravity of dark matter at any radius and the enclosed baryonic mass, a relation summarized by Milgrom's law of modified Newtonian dynamics (MOND). However, present-day covariant versions of MOND usually require some additional fields contributing to the geometry, as well as an additional hot dark matter component to explain cluster dynamics and cosmology. Here, we envisage a slightly more mundane explanation, suggesting that dark matter does exist but is the source of MOND-like phenomenology in galaxies. We assume a canonical action for dark matter, but also add an interaction term between baryonic matter, gravity, and dark matter, such that standard matter effectively obeys the MOND field equation in galaxies. We show that even the simplest realization of the framework leads to a model which reproduces some phenomenological predictions of cold dark matter (CDM) and MOND at those scales where these are most successful. We also devise a more general form of the interaction term, introducing the medium density as a new order parameter. This allows for new physical effects which should be amenable to observational tests in the near future. Hence, this very general framework, which can be furthermore related to a generalized scalar-tensor theory, opens the way to a possible unification of the successes of CDM and MOND at different scales.
Three twin neutrinos: Evidence from LSND and MiniBooNE

We construct a neutrino model of three twin neutrinos in light of the neutrino appearance excesses at LSND and MiniBooNE. The model, which includes a twin parity, naturally predicts identical lepton Yukawa structures in the Standard Model and the twin sectors. As a result, a universal mixing angle controls all three twin neutrino couplings to the Standard Model charged leptons. This mixing angle is predicted to be the ratio of the electroweak scale over the composite scale of the Higgs boson and has the right order of magnitude to fit the data. The heavy twin neutrinos decay within the experimental lengths into active neutrinos plus a long-lived Majoron and can provide a good fit, at around $4\sigma$ confidence level, to the LSND and MiniBooNE appearance data while simultaneously satisfying the disappearance constraints. For the Majorana neutrino case, the fact that neutrinos have a larger scattering cross section than anti-neutrinos provides a natural explanation to MiniBooNE's observation of a larger anti-neutrino appearance excess.
Halo dust detection around NGC 891

Observations of edge-on galaxies allow us to investigate the vertical extent and properties of dust, gas and stellar distributions. NGC 891 has been studied for decades and represents one of the best studied cases of an edge-on galaxy. We use deep PACS data together with IRAC, MIPS and SPIRE data to study the vertical extent of dust emission around NGC 891. We also test the presence of a more extended, thick dust component. By performing a convolution of an intrinsic vertical profile emission with each instrument PSF and comparing it with observations we derived the scaleheight of a thin and thick dust disc component. For all wavelengths considered the emission is best fit with the sum of a thin and a thick dust component. The scaleheight of both dust components shows a gradient passing from 70 $\mu$m to 250 $\mu$m. This could be due to a drop in dust heating (and thus dust temperature) with the distance from the plane, or to a sizable contribution ($\sim 15 - 80%$) of an unresolved thin disc of hotter dust to the observed surface brightness at shorter wavelengths. The scaleheight of the thick dust component, using observations from 70 $\mu$m to 250 $\mu$m has been estimated to be $(1.44\pm 0.12)$ kpc, consistent with previous estimates (extinction and scattering in optical bands and MIR emission). The amount of dust mass at distances larger than $\sim 2$ kpc from the midplane represents $2 - 3.3$ % of the total galactic dust mass and the relative abundance of small grains with respect to large grains is almost halved comparing to that in the midplane. The paucity of small grains high above the midplane might indicate that dust is hit by interstellar shocks or galactic fountains and entrained together with gas. The halo dust component is likely to be embedded in an atomic / molecular gas and heated by a thick stellar disc.
Eclipsing binary stars with a δ Scuti component

Eclipsing binaries with a $\delta$ Sct component are powerful tools to derive the fundamental parameters and probe the internal structure of stars. In this study, spectral analysis of 6 primary $\delta$ Sct components in eclipsing binaries has been performed. Values of $T_{\rm eff}$, $v \sin i$, and metallicity for the stars have been derived from medium-resolution spectroscopy. Additionally, a revised list of $\delta$ Sct stars in eclipsing binaries is presented. In this list, we have only given the $\delta$ Sct stars in eclipsing binaries to show the effects of the secondary components and tidal-locking on the pulsations of primary $\delta$ Sct components. The stellar pulsation, atmospheric and fundamental parameters (e.g., mass, radius) of 92 $\delta$ Sct stars in eclipsing binaries have been gathered. Comparison of the properties of single and eclipsing binary member $\delta$ Sct stars has been made. We find that single $\delta$ Sct stars pulsate in longer periods and with higher amplitudes than the primary $\delta$ Sct components in eclipsing binaries. The $v \sin i$ of $\delta$ Sct components is found to be significantly lower than that of single $\delta$ Sct stars. Relationships between the pulsation periods, amplitudes, and stellar parameters in our list have been examined. Significant correlations between the pulsation periods and the orbital periods, $T_{\rm eff}$, $\log g$, radius, mass ratio, $v \sin i$, and the filling factor have been found.
Cloud and Edge Computing for Smart Management of Power Electronic Converter Fleets: A Key Connective Fabric to Enable the Green Transition

The increasing grid penetration of renewable energy generation, energy storage, and controllable electronic loads [e.g., electric vehicle (EV) chargers, motor drives, and electrolyzers) is making power electronic converters (PECs)—their controllable grid connection interfaces—omnipresent. Therefore, fleets of PECs are becoming key players not only in coordinating the generation and storage but also in unlocking the potential for flexibility within each load. In this article, we discuss how cloud-based platforms and edge devices can allow for interfacing PECs and advanced control algorithms. We present seven different study cases using our own developed cloud-based platform that demonstrate the smart coordination of PECs in a variety of prototypes and real-world solutions. Moreover, the capabilities of cloud and edge computing are highlighted throughout the article at large, effectively characterizing cloud-based control of fleets of PECs as an essential part of the future energy sector.
Integrated Design and Assessment for Indoor Heating, Ventilation and Air-Conditioning in Hot Summer and Cold Winter Area: A Case Study in China

Integrated design of the heating, ventilation and air-conditioning (HVAC) is indispensable to green design because the increasing demand for HVAC systems has led to the diversification of indoor terminals for residential buildings, either focusing on energy efficiency or specializing in creating comfortable indoor environments, and they have different impacts on architectural and engineering design. The paper discussed the assessment-based integration design of the HVAC system, and by introducing case experiences, the whole process of the collaboration between architects and engineers was explored. Various methods were used in the research. The analytic hierarchy process (AHP) was employed to develop the assessment structure and calculate weightings; employing fuzzy comprehensive evaluation (FCE), the social performances of HVAC systems were subjectively evaluated; simulation technology was used to calculate the energy performances; the final results were ranked by the order of preference by similarity to ideal solution (TOPSIS). The research perspective of the collaboration between architects and engineers contributed to the existing literature. Besides, different indoor terminals were analyzed from the two disciplines; an assessment tool (ATI) was conducted and could be referred to; the current green building rating tools were analyzed, and suggestions were proposed to promote the integrated design.
Effects of Parent Role Modeling Behaviors in Correlation to Child Overweight and Obesity in Preschool-aged Children

EFFECTS OF PARENT ROLE MODELING BEHAVIORS IN CORRELATION TO CHILD OVERWEIGHT AND OBESITY IN PRESCHOOL-AGED CHILDREN NICOLE VAN HEEK 2018 OBJECTIVE: Parents have been proven to shape their children’s health through their growing years. Extensive research has been done on the correlation between adolescent’s health status and parent’s role modeling behaviors. However, little research has been done in preschool-aged children. Therefore, the purpose of this study was to determine if parenting style with food and meal behaviors was associated with body mass index (BMI) and weight status in preschool-aged children (3-5 years). METHODS: This study is a part of South Dakota State University’s iGrow Readers study. For this study, a total of 229 child/parent dyads participated from 14 recruited daycare centers across the Midwest. All heights and weights were recorded at pre-, post-, and follow-up data collection points. At pre-assessment, parents were given the Parent Survey, which contained information regarding their demographic and nutrition lifestyle. RESULTS: A total of 194 parents completed section I, which contained information regarding nutrition-related parent role modeling behaviors, in the Parent Survey. The average child age was 3.6 years. Characteristics of parents included predominantly mothers (83.5%) with an average age of 34.27 years with an Associate’s/Bachelor’s degree (51.2%) making over $60,00 a year (76.1%). No significance was found between
Probing the qudit depolarizing channel

For the quantum depolarizing channel with any finite dimension, we compare three schemes for channel identification: unentangled probes, probes maximally entangled with an external ancilla, and maximally entangled probe pairs. This comparison includes cases where the ancilla is itself depolarizing and where the probe is circulated back through the channel before measurement. Compared on the basis of (quantum Fisher) information gained per channel use, we find broadly that entanglement with an ancilla dominates the other two schemes, but only if entanglement is cheap relative to the cost per channel use and only if the external ancilla is well shielded from depolarization. We arrive at these results by a relatively simple analytical means. A separate, more complicated analysis for partially entangled probes shows for the qudit depolarizing channel that any amount of probe entanglement is advantageous and that the greatest advantage comes with maximal entanglement.
Polaritonic frequency-comb generation and breather propagation in a negative-index metamaterial with a cold four-level atomic medium

We develop a concept for a waveguide that exploits spatial control of nonlinear surface-polaritonic waves. Our scheme includes an optical cavity with four-level $\text{N}$-type atoms in a lossless dielectric placed above a negative-index metamaterial layer. We propose exciting a polaritonic Akhmediev breather at a certain position of the interface between the atomic medium and the metamaterial by modifying laser-field intensities and detunings. Furthermore, we propose generating position-dependent polaritonic frequency combs by engineering widths of the electromagnetically induced transparency window commensurate with the surface-polaritonic modulation instability. Therefore, this waveguide acts as a high-speed polaritonic modulator and position-dependent frequency-comb generator, which can be applied to compact photonic chips.
CONTEMPORANEOUS XMM-NEWTON INVESTIGATION OF A GIANT X-RAY FLARE AND QUIESCENT STATE FROM A COOL M-CLASS DWARF IN THE LOCAL CAVITY

We report the serendipitous detection of a giant X-ray flare from the source 2XMM J043527.2−144301 during an XMM-Newton observation of the high latitude molecular cloud MBM20. The source has not been previously studied at any wavelength. The X-ray flux increases by a factor of more than 52 from quiescent state to peak of flare. A 2MASS counterpart has been identified (2MASS J04352724−1443017), and near-infrared colors reveal a spectral type of M8–M8.5 and a distance of (67 ± 13) pc, placing the source in front of MBM20. Spectral analysis and source luminosity are also consistent with this conclusion. The measured distance makes this object the most distant source (by about a factor of four) at this spectral type detected in X-rays. The X-ray flare was characterized by a peak X-ray luminosity of ∼8.2 × 1028 erg s−1 and integrated X-ray energy of ∼2.3 × 1032 erg. The flare emission has been characterized with a two-temperature model with temperatures of ∼10 and 46 MK (0.82 and 4.0 keV) and is dominated by the higher temperature component.
SILCC-Zoom: The early impact of ionizing radiation on forming molecular clouds

As part of the SILCC-ZOOM project we present our first sub-parsec resolution radiation-hydrodynamic simulations of two molecular clouds self-consistently forming from a turbulent, multi-phase ISM. The clouds have similar initial masses of few 10$^4$ M$_{\odot}$, escape velocities of ~5 km s$^{-1}$, and a similar initial energy budget. We follow the formation of star clusters with a sink based model and the impact of radiation from individual massive stars with the tree-based radiation transfer module TreeRay. Photo-ionizing radiation is coupled to a chemical network to follow gas heating, cooling and molecule formation and dissociation. For the first 3 Myr of cloud evolution we find that the overall star formation effciency is considerably reduced by a factor of ~4 to global cloud values of < 10 % as the mass accretion of sinks that host massive stars is terminated after <1 Myr. Despite the low effciency, star formation is triggered across the clouds. Therefore, a much larger region of the cloud is affected by radiation and the clouds begin to disperse. The time scale on which the clouds are dispersed sensitively depends on the cloud substructure and in particular on the amount of gas at high visual extinction. The damage of radiation done to the highly shielded cloud (MC1) is delayed. We also show that the radiation input can sustain the thermal and kinetic energy of the clouds at a constant level. Our results strongly support the importance of ionizing radiation from massive stars for explaining the low observed star formation effciency of molecular clouds