Miracle-dz/UniFAR-FTUs huggingface dataset:
The Fourier Copula: Theory & Applications

This paper introduces a new parametric copula family based on Fourier expansions and flexible enough to describe arbitrary dependence structures. We derive its various properties and show that it can be fit efficiently by the Fast Fourier Transform. We overcome the Fourier series' assumption of periodicity by using a pseudo-copula and demonstrate the resulting model's superiority in applications like financial risk management. The concept of "discordant tail dependence" is introduced along with a Fourier-Clayton mixture copula. The Fourier-Clayton copula allows for some measure of tail dependence and also reduces the dimensionality of the Fourier copula's parameter space. The distinguishing feature of this new family of copulas is its ability to transform a flexible nonparametric density estimate into a robust parametric model. (A version of this paper was awarded the Thomas T. Hoopes Prize by Harvard University and the Allyn A. Young Prize by the Harvard University Department of Economics.)
Applications of cavitation dynamics in a three fluid system

In this thesis a numerical method is developed for modelling multiple bubbles with axis-symmetric geometry, in a domain of three ﬂuids separated by two ﬂuid-ﬂuid interfaces. The density ratios across these interfaces can vary allowing simulations of bubble inter-action with rigid boundaries, free surfaces and any density ratio values between these two extremes. The inclusion of buoyancy and surface tension into the simulations allow for a wide array of possible models, including investigations into explosion bubbles and biomedical applications. The evolution of the bubble is analysed in various scenarios right through to the toroidal stage of bubble collapse. The numerical simulations are conducted using the boundary integral method with vortex ring calculations for modelling the bubble transition from the simply connected bubble to the doubly connected toroidal phase. The numerical method is then compared with numerical and experimental data from other work to verify the validity of the model. The results show good agreement with past numerical results for spherical bubble oscillations and rigid boundary collapse. The veriﬁed model is then used to simulate a multitude of scenarios to investigate two bubble interaction with applications to mixing. A range of parameters are investigated and results are given for an optimal mixing approach. The introduction of a curved density interface is explored to determine the eﬀect it has on bubble collapse. The curved interface collapse is then adapted to consider bubble collapse near a cell wall.
Application of Deep Convolutional Neural Networks in the Diagnosis of Osteoporosis

The aim of this study was to assess the possibility of using deep convolutional neural networks (DCNNs) to develop an effective method for diagnosing osteoporosis based on CT images of the spine. The research material included the CT images of L1 spongy tissue belonging to 100 patients (50 healthy and 50 diagnosed with osteoporosis). Six pre-trained DCNN architectures with different topological depths (VGG16, VGG19, MobileNetV2, Xception, ResNet50, and InceptionResNetV2) were used in the study. The best results were obtained for the VGG16 model characterised by the lowest topological depth (ACC = 95%, TPR = 96%, and TNR = 94%). A specific challenge during the study was the relatively small (for deep learning) number of observations (400 images). This problem was solved using DCNN models pre-trained on a large dataset and a data augmentation technique. The obtained results allow us to conclude that the transfer learning technique yields satisfactory results during the construction of deep models for the diagnosis of osteoporosis based on small datasets of CT images of the spine.
Inside-out Planet Formation. IV. Pebble Evolution and Planet Formation Timescales

Systems with tightly packed inner planets (STIPs) are very common. Chatterjee & Tan proposed Inside-out Planet Formation (IOPF), an in situ formation theory, to explain these planets. IOPF involves sequential planet formation from pebble-rich rings that are fed from the outer disk and trapped at the pressure maximum associated with the dead zone inner boundary (DZIB). Planet masses are set by their ability to open a gap and cause the DZIB to retreat outwards. We present models for the disk density and temperature structures that are relevant to the conditions of IOPF. For a wide range of DZIB conditions, we evaluate the gap-opening masses of planets in these disks that are expected to lead to the truncation of pebble accretion onto the forming planet. We then consider the evolution of dust and pebbles in the disk, estimating that pebbles typically grow to sizes of a few centimeters during their radial drift from several tens of astronomical units to the inner, ≲1 au scale disk. A large fraction of the accretion flux of solids is expected to be in such pebbles. This allows us to estimate the timescales for individual planet formation and the entire planetary system formation in the IOPF scenario. We find that to produce realistic STIPs within reasonable timescales similar to disk lifetimes requires disk accretion rates of ∼10−9 M⊙ yr−1 and relatively low viscosity conditions in the DZIB region, i.e., a Shakura–Sunyaev parameter of α ∼ 10−4.
Lectures on Nonlinear Hyperbolic Differential Equations

In this introductory textbook, a revised and extended version of well-known lectures by L. Hormander from 1986, four chapters are devoted to weak solutions of systems of conservation laws. Apart from that the book only studies classical solutions. Two chapters concern the existence of global solutions or estimates of the lifespan for solutions of nonlinear perturbations of the wave or Klein-Gordon equation with small initial data. Four chapters are devoted to microanalysis of the singularities of the solutions. This part assumes some familiarity with pseudodifferential operators which are standard in the theory of linear differential operators, but the extension to the more exotic classes of opertors needed in the nonlinear theory is presented in complete detail.
Calculation of an Improved Stiffness Index Using Decomposed Radial Pulse and Digital Volume Pulse Signals

The stiffness index (SI) is used to estimate cardiovascular risk in humans. In this study, we developed a refined SI for determining arterial stiffness based on the decomposed radial pulse and digital volume pulse (DVP) waveforms. In total, 40 mature asymptomatic subjects (20 male and 20 female, 42 to 76 years of age) and 40 subjects with type 2 diabetes mellitus (T2DM) (23 male and 17 female, 35 to 78 years of age) were enrolled in this study. We measured subjects’ radial pulse at the wrist and their DVP at the fingertip, and then implemented ensemble empirical mode decomposition (EEMD) to derive the orthogonal intrinsic mode functions (IMFs). An improved SI (SInew) was calculated by dividing the body height by the mean transit time between the first IMF5 peak and the IMF6 trough. Another traditional index, pulse wave velocity (PWVfinger), was also included for comparison. For the PWVfinger index, the subjects with T2DM presented significantly higher SInew values measured according to the radial pulse (SInew-RP) and DVP signals (SInew-DVP). Using a one-way analysis of variance, we found no statistically significant difference between SInew-RP and PWVfinger when applied to the same test subjects. Binary logistic regression analysis showed that a high SInew-RP value was the most significant risk factor for developing T2DM (SInew-RP odds ratio 3.17, 95% CI 1.53–6.57; SInew-DVP odds ratio 2.85, 95% CI 1.27–6.40). Our refined stiffness index could provide significant information regarding the decomposed radial pulse and digital volume pulse signals in assessments of arterial stiffness.
Diabetes Mellitus Is Still a Strong Predictor of Periprocedural Outcomes of Primary Percutaneous Coronary Interventions in Patients Presenting with ST-Segment Elevation Myocardial Infarction (from the ORPKI Polish National Registry)

The impact of diabetes mellitus (DM) on outcomes of patients with ST-segment elevation myocardial infarction (STEMI) undergoing primary percutaneous coronary intervention (PCI) was confirmed by several studies. However, it is unclear whether this effect is still present in large groups of unselected patients undergoing up-to-date treatment. Thus, we sought to assess the impact of DM on periprocedural outcomes of primary PCI in STEMI using data from the Polish National Registry of PCI. Data on 150,782 STEMI patients undergoing primary PCI were collected. Of them, 26,360 (17.5%) patients had DM. Patients with DM were higher-risk individuals who experienced longer reperfusion delays and were less likely to have closed infarct-related artery at baseline (TIMI 0 + 1 flow: 73.2% vs. 72.0%; p < 0.0001) and achieve optimal reperfusion after PCI (TIMI 3 flow: 91.8% vs. 88.5%; p < 0.0001). The periprocedural mortality (1.1% vs. 1.9%; p < 0.0001) was higher in patients with DM and DM was identified as an independent predictor of periprocedural death. In conclusion, despite continuous progress in STEMI treatment, DM remains a strong predictor of periprocedural mortality. However, this detrimental effect of DM may be partially explained by the overall higher risk profile of diabetic patients.
Evidence for a new even-denominator fractional quantum Hall state in graphene

A remarkable development in the field of the fractional quantum Hall effect has been the proposal that the 5/2 state observed in the Landau level with orbital index $n = 1$ of two-dimensional electrons in a GaAs quantum well originates from a chiral $p$-wave paired state of composite fermions which are topological bound states of electrons and quantized vortices. This state is theoretically described by a "Pfaffian" wave function or its hole partner called the anti-Pfaffian whose excitations are neither fermions nor bosons but Majorana quasiparticles obeying non-Abelian braid statistics. This has inspired innovative ideas on fault-tolerant topological quantum computation and has also instigated a quest for other states with exotic quasiparticles. Here we report experiments on monolayer graphene that show clear evidence for unexpected even-denominator fractional quantum Hall physics in the $n = 3$ Landau level. We numerically investigate the known candidate states for even-denominator fractional quantum Hall effect, including the Pfaffian, the particle-hole symmetric Pfaffian, the 221-parton, and several valley / spin singlet states, and conclude that, among these, the 221-parton state is the most plausible candidate to explain the experimentally observed state. Like the Pfaffian, this state is also believed to harbour quasi-particles with non-Abelian braid statistics.
A new application of the fixed-points theory for the control of kinetic energy of a continuous structure

The fixed-points theory was originally used to determine the optimum tuning and damping ratios of a vibration neutraliser that may flatten the frequency response function (FRF) of a simple structure. Although the theory has also been used for the control of vibration of a continuous structure, applications have been limited only to point control. In this paper, a new application of the theory is discussed, which is for the global control of vibration of a continuous structure. The theory is used to determine the optimum tuning and damping ratios of the vibration neutraliser that flatten the global response of the structure. Kinetic energy is used as a measure of the structure's global response, and the application is demonstrated on undamped and damped simply supported beams. It is found that by using these optimum values, it is possible to remove the effects of the dominant mode leaving only the effect of the residual modes in the global behaviour. This shows that the theory can also be used to reduce the vibration of a continuous structure at all points instead of at a particular point only, such as in the conventional application.
Effects of Dietary Carbohydrate Level on the Growth and Conversion Efficiency of the Indian Major Carp Fingerling, Labeo rohita (Ham.): A Preliminary Study

Effect of varying levels of dietary carbohydrate on the growth and conversion efficiency of fingerling Labeo rohita (Ham.) have been reported. During the 6-week feeding trial, a linear growth pattern (ANOVA P<0.01) was noted. The level of carbohydrate that produced maximum growth and the best feed efficiency was 30%, corresponding to an energy to protein ratio of 8.83 kcal-g-1 protein. Beyond the above level of carbohydrate incorporation in the diet, various growth parameters of fish seemed negatively affected (P<0.01).
Energy consumption for Shortcuts To Adiabaticity

Shortcuts to adiabaticity let a system reach the results of a slow adiabatic process in a shorter time. We propose to quantify the "energy cost" of the shortcut by the energy consumption of the system enlarged by including the control device. A mechanical model where the dynamics of the system and control device can be explicitly described illustrates that a broad range of possible values for the consumption are possible, including zero (above the adiabatic energy increment) when friction is negligible and the energy given away as negative power is stored and recovered by perfect regenerative braking.
Social Learning in Cluster Organizations and Accumulation of Technological Capability

The purpose of the paper is to present how members of cluster organizations perceive their role in the accumulation of technological capability through social learning. The paper presents the results of a qualitative study of four cluster organizations. The theoretical foundation of the study are the communities of practice and the organizational inertia theories. The study indicates that the dynamics of technological capability of cluster organizations’ companies varies regarding three identified communities of practice, namely Participants, Cooperators and Locomotives. The so-called Dead souls (not included in any of the identified communities of practice) did not accumulate technological capability, while the companies classified as Participants increased their technological capability through social learning in cluster organizations provided that the cluster organizations offered comparatively high benefits. Those members of cluster organizations, identified as Cooperators and Locomotives, exhibited relatively high initial technological capability and increased it when the benefits received through social learning in cluster organizations were aligned with their technological trajectories. The study adds to the underdeveloped knowledge of cluster organizations by examining their role in enabling social learning that helps cluster firms accumulate technological capability.
ALMA polarization observations of the particle accelerators in the hotspot of the radio galaxy 3C 445

We present Atacama Large Millimeter Array (ALMA) polarization observations at 97.5 GHz of the southern hot spot of the radio galaxy 3C 445. The hot spot structure is dominated by two bright components enshrouded by diffuse emission. Both components show fractional polarization between 30 and 40 per cent, suggesting the presence of shocks. The polarized emission of the western component has a displacement of about 0.5 kpc outward with respect to the total intensity emission, and may trace the surface of a front shock. Strong polarization is observed in a thin strip marking the ridge of the hot spot structure visible from radio to optical. No significant polarization is detected in the diffuse emission between the main components, suggesting a highly disordered magnetic field likely produced by turbulence and instabilities in the downstream region that may be at the origin of the extended optical emission observed in this hot spot. The polarization properties support a scenario in which a combination of both multiple and intermittent shock fronts due to jet dithering, and spatially distributed stochastic second-order Fermi acceleration processes are present in the hot spot complex.
ANTITHROMBOTIC ACTIVITY OF A SYNTHETIC HEPARIN PENTASACCHARIDE IN A RABBIT STASIS THROMBOSIS MODEL USING DIFFERENT THROMBOGENIC CHALLENGES

The synthetic pentasccharide, representing the critical sequence required in heparin for binding to antithrombin III, provides a unique tool to study the question of whether an agent solely capable of inhibiting factor Xa but devoid of anti-factor Ila activity in vitro, has the capacity to produce an antithrombotic effect in vivo. We have previously demonstrated in a rabbit stasis thrombosis model using a human serum challenge, a significant antithrombotic effect of the pentasaccharide (Walenga et al., Thromb Res 43:243, 1986). To extend and confirm these studies, four modifications of the stasis thrombosis model were developed using more specified induction sites of thrombosis. The following thrombogenic challenges were selected: monkey brain thromboplastin, an activated prothrombin complex concentrate, a non-activated prothrombin complex concentrate administered simultaneously with Russell's viper venom, and factor Xa. Dose-dependent antithrombotic responses were obtained in all four systems with ED50 values between 25-43 ug/kg for pentasaccharide as compared to 16-47 ug/kg for heparin. Complete inhibition of induced thrombosis was obtained in all four systems for pentasaccharide. Ex vivo analysis revealed expected anti-factor Xa levels but no anti-factor IIa activity. It was also shown that pentasaccharide in the rabbit was capable of inhibiting the generation of thrombin without directly inhibiting formed thrombin. It is concluded that an oligosaccharide with high anti-factor Xa activity, devoid of anti-factor Ila activity, is capable of inhibiting thrombosis induced in rabbit stasis models, but that higher dosages than heparin are required for this effect-in terms of anti-factor Xa activity.
The emergence of smart service ecosystems—The role of socio‐technical antecedents and affordances

As physical products are increasingly augmented with digital technology, manufacturing firms have become part of the development of so‐called smart products and smart services. As such, manufacturing firms are challenged by new market participants and ecosystem partners, particularly from the software development industry, and by the dynamic nature of business relationships. While the academic literature on the distinctive characteristics of ecosystems, particularly digital ecosystems, is rich, the effect of smart service ecosystems' emergence on the foundation of smart products remains uncertain. This study reports on case study research based on 47 semi‐structured interviews with four companies that participate in an industrial smart service ecosystem. Taking an affordance‐theoretic perspective, we uncover the antecedents of and the process of emergent smart service ecosystems. We find that smart service ecosystems have three socio‐technical antecedents: a shared worldview, structural flexibility and integrity, and architecture of participation. We explain the emergence of smart service ecosystems as the result of specialisation in shared affordances and integration of idiosyncratic affordances into collective affordances. We derive seven propositions regarding the emergence of smart services, outline opportunities for further research, and present practical guidelines for manufacturing firms.
Awareness and Use of Remote Access to Electronic Resources by Postgraduate Students in a University

Abstract Off-campus access provides seamless and reliable access to licensed resources of libraries to multiple users, anywhere and anytime simultanously. Using a purposive sampling design, one hundred and forty-two postgraduate students were selected during information literacy training sessions to participate in this study. This study used a structured questionnaire as the data collection instrument. The study results revealed that the students are aware of the remote access facility. Many respondents were accessing the off-campus access facility from their homes and offices. Some recommendations were made to encourage the use of the remote access facility.
The Search for Spatial Extension in High-latitude Sources Detected by the Fermi Large Area Telescope

We present a search for spatial extension in high-latitude ( ) sources in recent Fermi point source catalogs. The result is the Fermi High-Latitude Extended Sources Catalog, which provides source extensions (or upper limits thereof) and likelihood profiles for a suite of tested source morphologies. We find 24 extended sources, 19 of which were not previously characterized as extended. These include sources that are potentially associated with supernova remnants and star-forming regions. We also found extended γ-ray emission in the vicinity of the Cen A radio lobes and—at GeV energies for the first time—spatially coincident with the radio emission of the SNR CTA 1, as well as from the Crab Nebula. We also searched for halos around active galactic nuclei, which are predicted from electromagnetic cascades induced by the e+e− pairs that are deflected in intergalactic magnetic fields. These pairs are produced when γ-rays interact with background radiation fields. We do not find evidence for extension in individual sources or in stacked source samples. This enables us to place limits on the flux of the extended source components, which are then used to constrain the intergalactic magnetic field to be stronger than 3 × 10−16 G for a coherence length λ ≳ 10 kpc, even when conservative assumptions on the source duty cycle are made. This improves previous limits by several orders of magnitude.
V1369 Cen High-resolution Panchromatic Late Nebular Spectra in the Context of a Unified Picture for Nova Ejecta

Nova Cen 2013 (V1369 Cen) is the fourth bright nova observed panchromatically through high-resolution UV+optical multiepoch spectroscopy. It is also the nova with the richest set of spectra (in terms of both data quality and number of epochs) thanks to its exceptional brightness. Here, we use the late nebular spectra taken between day ∼250 and day ∼837 after outburst to derive the physical, geometrical, and kinematical properties of the nova. We compare the results with those determined for the other panchromatic studies in this series: T Pyx, V339 Del (nova Del 2013), and V959 Mon (nova Mon 2012). From this we conclude that in all these novae the ejecta geometry and phenomenology can be consistently explained by clumpy gas expelled during a single, brief ejection episode and in ballistic expansion, and not by a wind. For V1369 Cen the ejecta mass (∼1 × 10−4 M⊙) and filling factor (0.1 ≤ f ≤ 0.2) are consistent with those of classical novae but larger (by at least an order of magnitude) than those of T Pyx and the recurrent novae. V1369 Cen has an anomalously high (relative to solar) N/C ratio that is beyond the range currently predicted for a CO nova, and the Ne emission line strengths are dissimilar to those of typical ONe or CO white dwarfs.