Miracle-dz/UniFAR-FTUs huggingface dataset:
Public Space Behaviors and Intentions: The Role of Gender through the Window of Culture, Case of Kerman

Urban public spaces are the spatial nexus of social interactions, activities, and expressions. Society manifests itself within these spaces through different lenses such as cultures and norms. The framework and restrictions related to gender-based behavior play a central role in the discourse about inclusivity and equity in urban public spaces when viewed through these lenses. There is, however, a gap in the literature that addresses how culture and gender influence public space behaviors and intentions within a traditional and modern cultural framework. The current study tests whether culture correlates with public space behavior on a neighborhood scale. A comparative study was conducted between two distinct neighborhoods in the city of Kerman, Iran. The two cases were selected due to their significant differences in how women use and interact with urban space. The effects of gender differences and perceived constraints on how residents manifest their behavior in public spaces were investigated. The study further investigated whether gender has a significant relationship with the level of appropriateness of certain public space behaviors and the intention to pursue them. The findings indicate significant cultural differences in both behavioral practice and behavioral intentions among the respondents. Furthermore, in traditional neighborhoods, the findings support significant gender-dependent differences in public space behavior, even though this gap is not apparent regarding intentions toward public space behaviors. The findings show a significantly greater disparity between traditional and modern districts in women’s perceived behavioral restrictions on personal expression.
Ultra-diffuse galaxies in the Auriga simulations

We investigate the formation of ultra-diffuse galaxies (UDGs) using the Auriga high-resolution cosmological magnetohydrodynamical simulations of Milky Way–sized galaxies. We identify a sample of 92 UDGs in the simulations that match a wide range of observables such as sizes, central surface brightness, Sérsic indices, colours, spatial distribution, and abundance. Auriga UDGs have dynamical masses similar to normal dwarfs. In the field, the key to their origin is a strong correlation present in low-mass dark matter haloes between galaxy size and halo spin parameter. Field UDGs form in dark matter haloes with larger spins compared to normal dwarfs in the field, in agreement with previous semi-analytical models. Satellite UDGs, on the other hand, have two different origins: ${\sim}55{{\ \rm per\ cent}}$ of them formed as field UDGs before they were accreted; the remaining ${\sim}45{{\ \rm per\ cent}}$ were normal field dwarfs that subsequently turned into UDGs as a result of tidal interactions.
Comparison of Surgical Outcomes between Single-Use and Reusable Flexible Ureteroscopes for Renal Stone Management: A Systematic Review and Meta-Analysis

Background and Objectives: Disposable flexible ureteroscopes have been widely used because of their cost-effectiveness and higher sterility potential compared with reusable flexible ureteroscopes. This study aimed to compare the surgical outcomes and complication rates in patients who undergo reusable or disposable flexible ureteroscopic stone surgeries (fURS) for urinary stone disease. Materials and Methods: A systematic review and meta-analysis were conducted under the Preferred Reporting Items for Systematic Reviews and Meta-Analyses (PRISMA) guideline. This systematic review was registered with PROSPERO (CRD42022331291). Clinical trials comparing reusable and disposable fURS for stone disease were found from PubMed, EMBASE, Cochrane Library, and the Web of Science up to March 2022. Participants were patients with upper urinary tract stones; the interventions were reusable or disposable fURS. Outcomes, including stone-free rate, operation time, length of hospital stay, and complication rate, were compared for analysis. Results: Overall, 111 studies were identified, but after removing duplicate studies, 75 studies remained. Thirty-two of these studies were excluded. Of the 43 screened studies, 11 met the eligibility criteria. There was no difference in the stone-free rate (SFR) between disposable and reusable fURS (p = 0.14; OR = 1.36; 95% CI, 0.9 to 2.04). For operation time, no difference was identified between reusable and disposable fURS groups (p = 0.12; MD = −5.31; 95% CI, −12.08 to 1.46). For hospital stay, there was also no difference between the two groups (p = 0.61; MD = −0.03; 95% CI, −0.17 to 0.10). There was no significant difference in complication rate between the two groups (p = 0.85; OR = 0.95; 95% CI, 0.56 to 1.61). Conclusions: There were no differences in the SFR, operation time, length of hospital stay, and complication rate between reusable and disposable fURS. Disposable fURS may be a comparable alternative to reusable fURS.
Berkeley 94 and Berkeley 96: Two Young Clusters with Different Dynamical Evolution

We have performed multiband UBVRcIcJHKs photometry of two young clusters located at large Galactocentric distances in the direction of the Perseus spiral arm. The obtained distances and colour excesses amount to 3.9+-0.11 kpc, E(B-V)=0.62+-0.05 for Berkeley 94, and 4.3+-0.15 kpc, E(B-V)=0.58+-0.06 for Berkeley 96. The respective ages, as measured from the comparison of the upper colour-magnitude diagrams to model isochrones, amount to LogAge(yr)=7.5+-0.07, and 7.0+-0.07, respectively. A sequence of optical PMS members is proposed in both clusters. In addition, samples of objects showing (H-Ks) excess are found. Part of these are suggested to be PMS cluster members of lower mass than the optical candidates. The spatial distribution of these sources, the comparison to galactic models and to the expected number of contaminating distant red galaxies, and the spectral energy distribution in particular cases support this suggestion. According to the results from numerical simulations, the spatial distributions of members in different mass ranges are interpreted as suggesting different initial conditions and evolutionary dynamical paths for the clusters. Berkeley 94 would have formed under supervirial conditions, and followed the so-called warm collapse model in its evolution, whereas Berkeley 96 would have formed with a subvirial structure, and would have evolved following a cold collapse path. Both processes would be able to reproduce the suggested degree of mass segregation and their spatial distribution by mass range. Finally, the mass distributions of the clusters, from the most massive stars down to PMS stars around 1.3 Msun, are calculated. An acceptable general agreement with the Salpeter IMF slope is found.
Barriers to adoption of industry 4.0 and sustainability: a case study with SMEs

ABSTRACT The concepts of sustainable supply chains and Industry 4.0 are progressively getting attention in different domains. Companies have started developing and implementing these practices in their business models. However, several challenges influence the adoption of sustainability and Industry 4.0 (I4.0) in small and medium-sized enterprises (SMEs). This study aimed (i) to identify the adoption barriers of sustainability and I4.0 and (ii) to establish the interrelationship among these barriers for SMEs. An extensive literature search supported by interviews with supply chain practitioners from three SMEs identified 12 critical barriers to adoption. The barriers are then ranked using ‘Interpretive Structural Modeling’. The results suggest that the ‘lack of resources’ and the ‘lack of employee’s competence/expertise’ are the most influencing barriers. Changing government regulations on the allocation of capital and financial incentives for SMEs to encourage training and skills development programs could promote sustainable supply chains and practices. The study also reflects short-, medium- and long-term planning strategies for supply chain practitioners for adoption of sustainability and I4.0 in SMEs.
Assessing Mental Health Among Thai University Students: A Cross-Sectional Study

Even before the COVID-19 pandemic, experts warned of the increasing rate of mental well-being issues among university students. The pandemic impacted the university-age populations, which studies have found to be particularly at risk for COVID-related stress, anxiety, and depression. There is cause for concern, particularly in countries such as Thailand that have relatively underdeveloped mental health systems and greater stigmatization of psychopathology. As a step toward addressing this concern, this study assessed student well-being at a Thai university (N = 367) using three online survey instruments: the EPOCH Measure of Adolescent Well-being, the Subjective Happiness Scale (SHS), and the Satisfaction with Life Scale (SWLS). Participants’ scores on all three scales were relatively low compared to the results of previous studies conducted in Thailand and internationally. Based on these results, the authors call for further investigation and interventions to address the growing need for the cultivation of well-being among university students in Thailand.
Theoretical and practical aspects of team teaching

The paper deals with the theory of team teaching and related terms. This theoretical background leads us to implementation of the team teaching approach during the EPTE (European Primary Teacher Education) teaching in the Pedagogy and Didactics module through English language as a mean of instruction. We adopted action research and case study as a qualitative research design. The purpose of the research was the reflection of participated teachers on important aspects of the team teaching practice (e.g., necessary time for planning lessons, collaboration, solving issues, as well as evaluation, etc.). The students’ attitude towards team teaching was positive and it was their first experience. We formulate several advantages, disadvantages, as well as implications for teacher practice. it. of conception of team for me as a What should I do I on team
New Evidence on National Culture and Corporate Financing: Does Institutional Quality Matter?

The purpose of this paper is twofold. First, to examine the dynamic impact of national culture on corporate financing in the context of seven Asian countries using a two-step GMM model, and second, to assess the moderating role of institutional quality on the relationship between culture and corporate financing. To achieve these objectives, a unique sample of seven Asian countries from the period of 2002 to 2018 was employed. The empirical results reveal that firms operating in countries that encourage individualism, masculinity, and uncertainty avoidance tend to use higher leverage in their operations. Individualism encourages autonomy in decision making and managers from such cultures engage in more risky decisions, while masculinity focuses on competition and suggests that males have a higher tendency for risk preference than females when undertaking financial decisions. In addition, firms from high uncertainty avoidance societies are more driven to engage in the use of leverage to obtain benefits via tax saving, whereas firms in higher power distance countries are less reliant on leverage. Our findings are consistent with our expectations, as well as supporting the existing literature on the issue. Further, the positive culture–leverage nexus is significantly and positively moderated by institutional quality. The findings are robust to alternative procedures (i.e., alternative proxies for culture and corporate financing, reduced sample size, and alternative estimation model), contribute to the existing literature, and have implications for potential policymakers.
A SHOCK FRONT IN THE MERGING GALAXY CLUSTER A754: X-RAY AND RADIO OBSERVATIONS

We present new Chandra X-ray and Giant Metrewave Radio Telescope (GMRT) radio observations of the nearby merging galaxy cluster A754. Our X-ray data confirm the presence of a shock front by obtaining the first direct measurement of a gas–temperature jump across the X-ray brightness edge previously seen in the imaging data. A754 is only the fourth galaxy cluster with confirmed merger shock fronts, and it has the weakest shock of those, with a Mach number, M = 1.57+0.16−0.12. In our new GMRT observation at 330 MHz, we find that the previously known centrally located radio halo extends eastward to the position of the shock. The X-ray shock front also coincides with the position of a radio relic previously observed at 74 MHz. The radio spectrum of the post-shock region, using our radio data and the earlier results at 74 MHz and 1.4 GHz, is very steep. We argue that acceleration of electrons at the shock front directly from thermal to ultrarelativistic energies is problematic due to energy arguments, while reacceleration of pre-existing relativistic electrons is more plausible.
Anomalously slow spin dynamics and short-range correlations in the quantum spin ice systems Yb 2 Ti 2 O 7 and Yb 2 SN 2 O 7

We report a positive muon spin relaxation and rotation (\muSR) study of the quantum spin ice materials Yb2Ti2O7 and Yb2Sn2O7 focusing on the low field response. In agreement with earlier reports, data recorded in small longitudinal fields evidence anomalously slow spin dynamics in the microsecond range below the temperature T_c at which the specific heat displays an intense peak, namely T_c = 0.24 K and 0.15 K, respectively, for the two systems. We found that slow dynamics extends above T_c up to at least 0.7 K for both compounds. The conventional dynamical Gaussian Kubo-Toyabe model describes the \muSR spectra recorded above T_c. At lower temperatures a published analytical extension of the Gaussian Kubo-Toyabe model provides a good description, consistent with the existence of short-range magnetic correlations. While the physical response of the two systems is qualitatively the same, Yb2Ti2O7 exhibits a much larger local magnetic susceptibility than Yb2Sn2O7 below T_c. Considering previously reported ac susceptibility, neutron scattering and \muSR results, we suggest the existence of anomalously slow spin dynamics to be a common physical property of pyrochlore magnetic materials. The possibility of molecular spin substructures to be associated to the slow dynamics and therefore the short-range correlations is mentioned. The slow spin dynamics observed under field does not exclude the presence of much faster dynamics detected in extremely low or zero field.
Second order gyrokinetic theory for particle-in-cell codes

The main idea of the gyrokinetic dynamical reduction consists in a systematical removal of the fast scale motion (the gyromotion) from the dynamics of the plasma, resulting in a considerable simplification and a significant gain of computational time. The gyrokinetic Maxwell–Vlasov equations are nowadays implemented in for modeling (both laboratory and astrophysical) strongly magnetized plasmas. Different versions of the reduced set of equations exist, depending on the construction of the gyrokinetic reduction procedure and the approximations performed in the derivation. The purpose of this article is to explicitly show the connection between the general second order gyrokinetic Maxwell–Vlasov system issued from the modern gyrokinetic theory and the model currently implemented in the global electromagnetic Particle-in-Cell code ORB5. Necessary information about the modern gyrokinetic formalism is given together with the consistent derivation of the gyrokinetic Maxwell–Vlasov equations from first principle.
Influence of marketing innovation on the performance of coffee cooperatives in Kenya

The purpose of the study was to assess the influence of marketing innovation on the performance of coffee cooperatives in Kenya. A descriptive research design was applied. The target population of this study was 525 coffee cooperative societies in Kenya registered with the Commissioner for Cooperatives and licensed by AFFA (Coffee Directorate) as of 30th of October 2016. The sample size was 227 respondents. Structured questionnaires were used to collect primary data from the selected respondents. The results revealed that marketing innovation and performance are positive and significantly related (? =0.674, p=0.001). This implied that significant changes in product design and packaging led to a positive change in the performance of coffee cooperatives. The study affirms that to improve performance by targeting the customers, constant improvements in how the company promotes its new products to capture the attention of new customers is a key aspect to be considered. The study recommends the management employ skills in developing clear operating procedures to run the business successfully, coordinate different areas of the business to achieve results and the ability and design jobs to suit staff capabilities and interests.
Spherically symmetric Einstein–Maxwell theory and loop quantum gravity corrections

Effects of inverse triad corrections and (point) holonomy corrections, occurring in loop quantum gravity, are considered on the properties of Reissner–Nordström black holes. The version of inverse triad corrections with unmodified constraint algebra reveals the possibility of occurrence of three horizons (over a finite range of mass) and also shows a mass threshold beyond which the inner horizon disappears. For the version with modified constraint algebra, coordinate transformations are no longer a good symmetry. The covariance property of spacetime is regained by using a quantum notion of mapping from phase space to spacetime. The resulting quantum effects in both versions of these corrections can be associated with renormalization of either mass, charge or wavefunction. In neither of the versions, Newton’s constant is renormalized. (Point) Holonomy corrections are shown to preclude the undeformed version of constraint algebra as also a static solution, though time-independent solutions exist. A possible reason for difficulty in constructing a covariant metric for these corrections is highlighted. Furthermore, the deformed algebra with holonomy corrections is shown to imply signature change.
Physiomechanical and Surface Characteristics of 3D-Printed Zirconia: An In Vitro Study

The objective of this study is to examine the physiomechanical and surface properties of 3D-printed zirconia in comparison to milled zirconia. A total of 80 disc-shaped (14 × 1.5 ± 0.2 mm) specimens (20 milled and 60 3D-printed (at three different orientations; horizontal, vertical, and tilted)) were manufactured from 3-mol% yttria-stabilized tetragonal zirconia. Five specimens per group were evaluated for crystalline phase, grain size, density, porosity, surface roughness, wettability, microhardness, and SEM analysis of the surface. Biaxial flexural strength (BFS) was measured (n = 15) followed by Weibull analysis and SEM of fractured surfaces. Statistical analysis was performed using one-way ANOVA and Tukey’s post hoc test at α = 0.05. All groups showed a predominant tetragonal phase, with a 450 nm average grain size. There was no significant difference between groups with regards to density, porosity, and microhardness (p > 0.05). The tilted group had the highest surface roughness (0.688 ± 0.080 µm), significantly different from the milled (p = 0.012). The horizontal group presented the highest contact angle (89.11 ± 5.22°), significantly different from the milled and tilted (p > 0.05). The BFS of the milled group (1507.27 ± 340.10 MPa) was significantly higher than all other groups (p < 0.01), while vertical and tilted had a similar BFS that was significantly lower than horizontal (p < 0.005). The highest and lowest Weibull modulus were seen with tilted and milled, respectively. Physical properties of all groups were comparable. The surface roughness of the tilted group was higher than milled. The horizontal group had the highest hydrophobicity. Printing orientations influenced the flexural strength of 3D-printed zirconia. Clinical implications: This study demonstrates how the printing orientation affects the physiomechanical characteristics of printed zirconia.
Evolution of dust and molecular hydrogen in the Magellanic System

We investigate the evolution of the interstellar medium (ISM) in self-consistent, chemodynamical simulations of the Magellanic Clouds (MCs) during their recent (z<0.3) past. An explicit modelling of dust and molecular hydrogen lifecycles enables the comparison of our models against the observed properties of the ISM, including elemental depletion from the gas-phase. Combining this model with a tidal-dominated paradigm for the formation for the Magellanic Stream and Bridge, we reproduce the age-metallicity relations, long gas depletion timescales, and presently observed dust and molecular hydrogen masses of the MCs to within their respective uncertainties. We find that these models' enrichment depends sensitively on the processing of dust within the ISM and the dynamical influence of external tides/stellar bars. The ratio of characteristic dust destruction timescales in our SMC and LMC models, a governing parameter of our models' evolution, is consistent with estimates based on observed supernova (SN) rates. Our reference MC models tend to exhibit the disputed universal dust-to-metal ratio, which we argue stems from the adoption of high SNe II condensation efficiencies. Our models are the first to reproduce the one-tenth solar metallicity of the Stream/Leading Arm following tidal stripping of the SMC; the hypothesis that the LMC contributes a metal-rich filament to the Stream, as implied by recent kinematic and abundance analyses, is also appraised in this study.
An Empirical Study of Determinants of Pay-for-Performance in PPP Procurement

Pay-for-performance is important in procuring Public–Private Partnership projects to which existing research has not paid enough attention. We took 884 ecological construction and environmental protection PPP projects (eco-environmental PPPs) as a sample and used the fuzzy-set qualitative comparative analysis method to discuss the links among technological, organizational, and environment in pay-for-performance procurement based on technology–organization–environment frameworks. We found the following: (1) A single condition alone does not constitute a necessary condition for the high-level pay-for-performance of PPP projects. The multiple concurrencies of technology, organization, and environmental conditions form three configurations that drive the pay-for-performance of PPPs with the same effect. (2) The existence of attention distribution and institutional regulation are crucial for optimizing pay-for-performance. To improve pay-for-performance, local governments should combine their own conditions to strengthen the synergy of technology, organization, and environmental conditions. In addition, the leader’s attention distribution and institutional regulation should be taken seriously. The contributions of this study are twofold: (1) Theoretically, this study provides new evidence of the determinants of pay-for-performance in PPP procurement, complementing empirical studies on the factors facilitating its implementation. (2) In practice, it provides a specific path for the government to improve the performance of eco-environmental PPPs.