bluuebunny/crossref_metadata_2025_split huggingface dataset:
USE OF A NEW METHODOLOGY TO ASSESS THE STRUCTURE OF WATER AND WATER-CONTAINING SYSTEMS
Authors: Сидоренко Галина Николаевна , Лаптев Борис Иннокентьевич , Горленко Николай Петрович , Антошкин Леонид Владимирович 
Published: October 2024

В работе использована новая методика для оценки структуры воды и водосодержащих систем с включением измерительной ячейки или ее эквивалентной схемы параллельно с индуктивностью в колебательный контур генератора синусоидальных колебаний. В опытах с дистиллированной водой и при увеличении концентрации растворов хлорида натрия до 10М на кривых амплитуды генератора синусоидальных колебаний выявлено наличие двух минимумов при частотах 28-32 кГц и 106-117 кГц, а при дальнейшем возрастании концентрации растворов oт 10 М до 10 М эти минимумы отсутствуют. Сделано предположение, что наличие этих минимумов обусловлено присутствием в воде двух структурных образований, которые изменяются относительно дискретно при повышении концентрации раствора хлорида натрия. Полученные в работе данные могут быть использованы для дальнейшего изучения механизмов изменений структуры, других свойств воды и водосодержащих систем при внешних воздействиях, а также для оценки влияния этих изменений на различные технологические процессы и процессы, протекающие в живых системах.
A new technique for evaluating the structure of water and water-containing systems with the inclusion of a measuring cell or its equivalent circuit in parallel with an inductance in the oscillating circuit of a sinusoidal oscillator generator is used in this work. In experiments with distilled water and at increasing the concentration of sodium chloride solutions up to 10-4 M, the presence of two minima at frequencies 28-32 kHz and 106-117 kHz was revealed on the amplitude curves of the sinusoidal oscillator, and at further increasing the concentration of solutions from 10-3 M to 10-1 M these minima are absent. An assumption is made that the presence of these minima is due to the presence of two structural formations in water, which change relatively discretely with increasing concentration of sodium chloride solution. The data obtained in this work can be used for further study of the mechanisms of changes in the structure and other properties of water and water-containing systems under external influences, as well as for evaluating the influence of these changes on various technological processes and processes occurring in living systems.
La Socioformación y el Trabajo Colaborativo un Avance en el Proceso Enseñanza Aprendizaje
Authors: Hernández Jiménez Alfredo 
Published: October 2024

Introducción: El trabajo colaborativo se puede expresar desde el punto de vista del aprendizaje basado en el planteamiento de un problema en un entorno virtual, aprender colaborativamente, es la adquisición de destrezas y actitudes, esto es el resultado de la interacción adecuada del grupo, cabe hacer mención que el trabajo colaborativo-aprendizaje está motivado por los cambios constantes que se identifican en la sociedad y por una nueva visión que se presentan con las relaciones tecnología-educación y tecnología-sociedad. Objetivo: conocer como la sociedad del conocimiento es una alternativa para que el conocimiento se convierta en una herramienta central en el propio beneficio de la sociedad en general. La (UNESCO), ha preponderado los atributos especiales a tomar en cuenta en la educación del siglo XXI, estos atributos o premisas se deberían de tomar en cuenta por los gobiernos a nivel mundial mediante un sistema educativo donde se dé prioridad a aspecto importantes como: aprender a aprender, aprender a hacer, aprender a ser y aprender a trabajar mediante la formación de equipos formados por tres o cuatro elementos como máximo. Metodología: se desarrolló una investigación de tipo descriptiva en base a un análisis de revistas indexadas que hablaran exclusivamente del trabajo colaborativo. Resultados: el trabajo colaborativo es la estrategia que se debería de aplicar en el proceso enseñanza-aprendizaje. Conclusiones: Los diferentes escenarios que presenta la sociedad actual hacen que se tenga la necesidad de poner en práctica nuevos recursos de enseñanza aprendizaje.
Hacia una Justicia Equitativa: Desafíos y Avances en la Lucha Contra la Violencia de Género en Bolivia
Authors: Peralta Moya Cameron Marcela 
Published: October 2024

El artículo aborda la persistencia de la violencia de género en Bolivia y el éxito de la Ley 348. Si bien fue promulgada en 2013 para proteger a las mujeres, su ejecución coercitiva fue criticada por algunos problemas estructurales y operativos y por la falta de recursos y capacitación judicial adecuada. Esta investigación es un primer paso para revelar los retrocesos y avances en la aplicación práctica de la Ley 348 y, de esta manera, mejorar las políticas públicas y las estrategias judiciales para una protección efectiva de las víctimas. Adicionalmente, abordamos el concepto de violencia de género en Bolivia y señalamos que se trata de un problema multidimensional. La violencia puede tomar la forma física, psicológica, sexual, económica y a veces derivar en el feminicidio. Las relaciones desiguales de poder entre hombres y mujeres, la dependencia económica y los bajos niveles educativos también son factores que aumentan el riesgo de ser objeto de violencia. El artículo también sitúa la violencia de género en el contexto más amplio de las sociedades latinoamericanas y bolivianas, enfatizando que es un problema trivial y profundamente arraigado en las sociedades patriarcales. En Bolivia, la moderación para prevenir y poner fin a este abuso es muy conmovedora, incluso en presencia de leyes y reglamentos. La historia y evolución de las leyes en Bolivia, incluida la Ley 348 y la Ley 1173, se han visto convulsionadas con los pasos y articulaciones como la seguridad de las mujeres, pero siguen empantanadas con problemas como la falta de conciencia, la trivialización criminal y la escasa preparación y respuesta de las autoridades. El texto defiende reformas pertinentes en la Ley No 348 con el fin de acercar la justicia equitativa; especificándolas como el rediseño de la ley con el objetivo de abordar con mayor precisión la violencia y mejorar la capacitación de los operadores de justicia
Emotional Intelligence in Insurance Leaders For Managing Business Communication with Generation Z
Authors: Dwiastuti Winda , Basir Yulinda , Febrianno Boer Rino 
Published: October 2024

Modern business landscape, including the insurance industry, demands effective leadership to navigate the complex interpersonal dynamics, especially when working with Gen Z as the newest generation that enters the workplace. Gen Z employees, with their unique expectations and communication styles, seek leaders who offer transparency, authenticity, and emotional connection. This study explores the significant role of emotional intelligence (EI) in achieving leadership success within insurance companies. Emotional intelligence is increasingly recognized as a key factor in leadership effectiveness, influencing how leaders build relationships, make strategic decisions, and inspire their teams. Given the competitive nature of the insurance industry and its technological advancements, leaders must adeptly manage a multigenerational workforce and adapt to new challenges. This qualitative research explores how insurance leaders utilize EI to engage Generation Z, who prioritize diversity, collaboration, and flexible leadership. By understanding Generation Z's unique communication preferences, emotionally intelligent leaders enhance organizational performance and employee satisfaction. Drawing on current literature and interviews with leaders from an insurance company in Indonesia, this study finds that leaders with high emotional intelligence significantly boost employee engagement, satisfaction, and productivity. The findings emphasize the importance of integrating emotional intelligence into leadership practices to ensure resilience and competitiveness in the market, benefiting organizations by bridging generational gaps and empowering Gen Z employees.
ШКАЛЫ PIRO И SAPS ДЛЯ ПРОГНОЗА ИСХОДА ЗАБОЛЕВАНИЯ У КОШЕК
Authors: Лаптев Сергей , Павлович Василий 
Published: October 2024

Надежное прогнозирование сепсиса является важной клинической проблемой в медицине и ветеринарии из-за высокой заболеваемости и смертности от осложнений сепсиса. Изучая этиологию септических осложнений при панлейкопении кошек, мы адаптировали диагностические шкалы PIRO и SAPS, предложенные для оценки прогноза сепсиса в клинической ветеринарии. Многоэтапная оценка клинического состояния животных позволяет выявить животных с повышенным риском осложнений на ранних стадиях септического процесса и прогнозировать его летальность, правильно оценить состояние животного и оптимизировать терапевтическую стратегию для септических животных. Прогноз исхода септических осложнений при панлейкопении кошек был основан на изучении историй болезни 10 кошек с диагнозом панлейкопения, зарегистрированных при поступлении животных в стационар. Подтверждение вирусного заболевания основывалось на клинических признаках болезни - апатии, рвоте, диарее, морфологическом и биохимическом анализах крови, положительном ПЦР-тесте на вирус панлейкопении кошек. Исследование проводилось на кафедре эпизоотологии и организации ветеринарного дела Московской государственной академии ветеринарной медицины и биотехнологии – МВА имени К. И. Скрябина. Статистическую значимость прогноза оценивали с помощью корреляционно-регрессионного анализа показателей в связке (Баллы PIRO–Исход заболевания; Баллы SAPS–Исход заболевания; Баллы PIRO–Баллы SAPS). Рассчитанные параметры прогностической модели исхода заболевания у кошек с диагнозом панлейкопения на 86,1% объясняют достоверную зависимость от количества баллов по шкале PIRO при первичном обследовании животных. Достоверная зависимость баллов по шкале SAPS при первичном исследовании составляла 42,3%, которая увеличилась до 58,1% на 3-й день заболевания. Повышение достоверности прогноза в последующие дни заболевания позволяет использовать данные шкалы SAPS для модификации тактики и стратегии лечения.
ҚЫЛШЫҚ ЖҮНДІ ҚҰЙРЫҚТЫ ҚОЙЛАРДЫҢ СЕЛЕКЦИЯЛЫҚ БЕЛГІЛЕРІНІҢ ГЕНЕТИКАЛЫҚ ПАРАМЕТРЛЕРІ
Authors: Муканова Ляззат , Садықұлов Тулеухан , Малмаков Нурлан , Адылканова Шолпан , Койшибаев Азамат 
Published: October 2024

Ауылшаруашылық малдарының жеке генетикасының маңызды мәселелерінің бірі-экономикалық пайдалы селекциялық белгілер арасындағы байланысты орнату. Сонымен қатар, байланыстардың мөлшері мен бағыты белгінің сипатына, селекцияның қарқындылығына және малдардың генотипіне байланысты болады. Осы тұрғыдан алғанда, еділбай қой тұқымының саулығын гиссар қойының қошқарымен шағылыстыру арқылы алынған бірінші ұрпақтардың селекциялық белгілерінің генетикалық параметрлерін зерттеудің маңызы зор және де бұл осы жұмыстың өзекті мәселесі болып саналады. Генетикалық-математикалық әдіс мал популяциясындағы, табынындағы селекциялық үрдісті талдау жасауға мүмкіндік береді, сонымен бірге белгілерге және малдардың өнімділік қасиетіне генотиптің және қоршаған ортаның әсері бағаланады. Ауыл шаруашылығындағы селекция нәтижелерін тұқым қуалаушылық (һ2), белгілердің қайталануы (rb), селекциялық белгілердің өзара байланысы (r), селекциялық дифференциал (SD), регрессия (R), селекциялық тиімділік (SE) сияқты параметрлер арқылы анықталады.
«Байсерке Агро» ОҒӨО мал шаруашылығының әр түрлі генотипті қылшық жүнді құйрықты қойларының генотиптік өзгергіштігі белгілерінің арасын және өзара байланысын анықтауға бағытталған ізденістер қазіргі селекцияда үлкен өзектілікке ие және ғылыми-практикалық маңызы бар, өйткені зерттеу нәтижелерін қолдану малдарды бағалауға қажетті уақытты қысқартуға, оның қарқынын айтарлықтай жеделдетуге көмектеседі.
Formation of WNL Stars in the MW and LMC Based on the k − ω Model
Authors: Si Jijuan , Li Zhi , Li Yan 
Published: October 2024

Abstract
We adopt a set of second-order differential equations (k − ω model) to handle core convective overshooting in massive stars, simulate the evolution of nitrogen sequence Wolf–Rayet (WNL) stars with different metallicities and initial masses, both rotating and nonrotating models, and compare the results with the classical overshooting model. The results indicate that, under the same initial conditions, the k − ω model generally produces larger convective cores and wider overshooting regions, thereby increasing the mass ranges and extending the lifetimes of WNL stars, as well as the likelihood of forming WNL stars. The masses and lifetimes of WNL stars both increase with higher metallicities and initial masses. Under higher-metallicity conditions, the two overshooting schemes significantly differ in their impacts on the lifetimes of WNL stars, but are insignificant in the mass ranges of the WNL stars. Rotation may drive the formation of WNL stars in low-mass, metal-poor counterparts, with this effect being more pronounced in the overshooting model. The surface nitrogen of metal-rich WNL stars formed during the main-sequence phase is likely primarily from the CN cycle, while it may come from both the CN and NO cycles for relatively metal-poor counterparts. Our model can effectively explain the distribution of WNL stars in the Milky Way, but appears to have inadequacies in explaining the WNL stars in the LMC.
Microphysical Prescriptions for Parameterized Water Cloud Formation on Ultra-cool Substellar Objects
Authors: Mang James , Morley Caroline V. , Robinson Tyler D. , Gao Peter 
Published: October 2024

Abstract
Water must condense into ice clouds in the coldest brown dwarfs and exoplanets. When they form, these icy clouds change the emergent spectra, temperature structure, and albedo of the substellar atmosphere. The properties of clouds are governed by complex microphysics but these complexities are often not captured by the simpler parameterized cloud models used in climate models or retrieval models. Here, we combine microphysical cloud modeling and 1D climate modeling to incorporate insights from microphysical models into a self-consistent, parameterized cloud model. Using the 1D Community Aerosol and Radiation Model for Atmospheres (CARMA), we generate microphysical water clouds and compare their properties with those from the widely used EddySed cloud model for a grid of Y dwarfs. We find that the mass of water condensate in our CARMA water clouds is significantly limited by available condensation nuclei; in models without additional seed particles for clouds added, the atmosphere becomes supersaturated. We incorporate water latent heat release in the convective and radiative parts of the atmosphere and find no significant impact on water-ice cloud formation for typical gas giant compositions. Our analysis reveals the CARMA cloud profiles have a gradual decrease in opacity of approximately 4% per bar below the cloud base. Incorporating this gradual cloud base falloff and a variable f
sed parameter allows spectra generated from the parameterized Eddysed model to better match those of the microphysical CARMA model. This work provides recommendations for efficiently generating microphysically informed water clouds for future models of cold substellar objects with H/He atmospheres.
High-energy Neutrinos from Late-time Jets of Gamma-Ray Bursts Seeded with Cocoon Photons
Authors: Matsui Riki , Kimura Shigeo S. , Hamidani Hamid 
Published: October 2024

Abstract
In gamma-ray bursts (GRBs), ∼100–1000 s after the prompt emission, afterglow observations have consistently shown X-ray excesses detected in the form of flares (in long GRBs) or extended emission (in short GRBs). These observations are interpreted as emissions from jets launched by late central engine activity. However, the characteristics of these late-time jets, particularly the dissipation radius (r
diss), Lorentz factor (Γ), and cosmic-ray loading factor (ξ

p
), remain unknown despite their importance. Here, in order to understand the properties of the late-time jets with future multimessenger observations, we estimate the detectability of neutrinos associated with late-time emissions for a wide range of r
diss and Γ, assuming ξ

p
= 10. We take into account external seed photons from the cocoon around the jets, which can enhance the neutrino production through photohadronic interaction in the jet dissipation region. Our results are still consistent with the upper limit obtained by IceCube. Our calculations indicate a promising prospect for neutrino detection with IceCube-Gen2 through the stacking of ∼1000–2000 events, for a wide range of r
diss and Γ. We found that setting an optimal energy threshold of 10 TeV can significantly reduce noise without negatively affecting neutrino detection. Furthermore, even in the case of nondetection, we show that meaningful constraints on the characteristics of the late-time jets can be obtained.
Nucleosynthesis Contribution of Neutrino-dominated Accretion Flows to the Solar Neighborhood
Authors: Qi Yan-Qing , Liu Tong , Sun Mouyuan , Cai Zhen-Yi 
Published: October 2024

Abstract
The elemental abundances of stars reflect the complex enrichment history of the Galaxy. To explore and explain the metal enrichment history of the cosmic environment near our solar system, we study the evolution of 56Fe abundance over time and [Mg/Fe] versus [Fe/H] evolution in the solar neighborhood. Core-collapse supernovae make the dominant contribution in the early stages, while Type Ia supernovae (SNe Ia) have a delayed and dominant impact in the later stages. In this work, we consider the nucleosynthesis contribution of neutrino-dominated accretion flows (NDAFs) formed at the end of the lives of massive stars. The results show that the [Fe/H] gradually increases over time and eventually reaches [Fe/H] = 0 and above, reproducing the chemical enrichment process in the solar neighborhood. Before the onset of SNe Ia, the ratio of 56Fe mass to the total gas mass increases by a factor of at most ∼1.44 when NDAFs are taken into account. We find that by including NDAF in our models, the agreement with the observed metallicity distribution of metal-poor stars in the solar neighborhood (<1 kpc) is improved while not significantly altering the location of the metallicity peak. This inclusion can also reproduce the observed evolutionary change of [Mg/Fe] at [Fe/H] ∼ −1.22, bringing the ratio to match the solar abundance. Our results provide an extensive understanding of metallicity evolution in solar environments by highlighting the nucleosynthesis contribution of NDAF outflows in the solar neighborhood.
High-quality Extragalactic Legacy-field Monitoring (HELM) with DECam: Project Overview and First Data Release
Authors: Zhuang 庄 Ming-Yang 明阳 , Yang Qian , Shen Yue , Adamów Monika , Friedel Douglas N. , Gruendl R. A. , Stone Zachary , Li Junyao , Liu Xin , Martini Paul , Abbott Timothy M. C. , Anderson Scott F. , Assef Roberto J. , Bauer Franz E. , Bielby Richard , Brandt W. N. , Burke Colin J. , Casares Jorge , Chen Yu-Ching , De Rosa Gisella , Drlica-Wagner Alex , Dwelly Tom , Eltvedt Alice , Fonseca Alvarez Gloria , Fu 傅 Jianyang 健洋 , Fuentes Cesar , Graham Melissa L. , Grier Catherine J. , Golovich Nathan , Hall Patrick B. , Hartigan Patrick , Horne Keith , Koekemoer Anton M. , Krumpe Mirko , Li Jennifer I. , Lidman Chris , Malik Umang , Mangian Amelia , Merloni Andrea , Ricci Claudio , Salvato Mara , Sharp Rob , Trilling David E. , Tucker Brad E. , Wen Di , Wideman Zachary , Xue Yongquan , Yu Zhefu , Zucker Catherine 
Published: October 2024

Abstract
High-quality Extragalactic Legacy-field Monitoring (HELM) is a long-term observing program that photometrically monitors several well-studied extragalactic legacy fields with the Dark Energy Camera (DECam) imager on the CTIO 4 m Blanco telescope. Since 2019 February, HELM has been monitoring regions within COSMOS, XMM-LSS, CDF-S, S-CVZ, ELAIS-S1, and SDSS Stripe 82 with few-day cadences in the (u)gri(z) bands, over a collective sky area of ∼38 deg2. The main science goal of HELM is to provide high-quality optical light curves for a large sample of active galactic nuclei (AGNs), and to build decades-long time baselines when combining past and future optical light curves in these legacy fields. These optical images and light curves will facilitate the measurements of AGN reverberation mapping lags, as well as studies of AGN variability and its dependencies on accretion properties. In addition, the time-resolved and coadded DECam photometry will enable a broad range of science applications from galaxy evolution to time-domain science. We describe the design and implementation of the program and present the first data release that includes source catalogs and the first ∼3.5 yr of light curves during 2019A–2022A.
A new species of the genus Humboldtiana (Gastropoda, Stylommatophora, Xanthonychidae) from Sierra de Penjamo, Guanajuato, Mexico
Authors: Mejía Omar , López Benjamín 
Published: October 2024

Mexican terrestrial malacofauna is highly diverse, but poorly studied. The genus Humboldtiana includes near to 60 species, most with insular distributions on single mountains from South Texas (USA) to entral Mexico.
Humboldtiana dugesi sp. nov. is described from the state of Guanajuato, Mexico. This new species represents the first one described for the state and is diagnosed by the following combination of characters that allow distinguishing for other species included in the genus, a protoconch with growth lines and granulated microsculpture, a globose penis that bears a stout verge that covers half of the penis cavity and a long flagellum that is four times longer than the combined length of the penis and epiphallus.
Avec la Pietà de Villeneuve-lès-Avignon. Performance et réception d’une œuvre intermédiale
Authors: Lieutaghi Clara 
Published: October 2024

L’article prend pour objet d’étude la Pietà de Villeneuve-lès-Avignon (v. 1455) en proposant une interprétation de son dispositif représentationnel. L’intermédialité observée au sein du retable construit sa performance et se trouve à l’origine de la réponse dévotionnelle des fidèles. Aborder certaines des copies et variantes de la Pietà autorise également une meilleure compréhension des transformations apportées au dispositif initial à l’occasion de ces reprises.
A Cabinet of Religious Curiosities
Authors: Nellis Steff 
Published: October 2024

En 1723, les premiers volumes de la série en sept livres, Cérémonies et coutumes religieuses de tous les peuples du monde (1723-1737), sont publiés à Amsterdam par le Huguenot exilé Jean Frédéric Bernard. Somptueusement illustrée de plus de 250 gravures par le célèbre graveur parisien, également exilé, Bernard Picart, la série Cérémonies offre une perspective révolutionnaire sur les religions du monde en comparant à parts égales cérémonies, coutumes et rituels. Des recherches antérieures ont montré que le corpus d’illustrations de Picart doit être considéré comme une « source et cible de l’agentivité sociale », pour le dire avec les mots de Gell. En conséquence, les illustrations imprimées de Picart peuvent être vues comme des outils pour susciter des émotions et exiger l’intervention active du spectateur par le biais de diverses stratégies visuelles. Dans cet article, je souhaite approfondir notre compréhension des moyens par lesquels les représentations des cérémonies religieuses de Picart ont agi comme une force de changement en examinant les différentes manières dont il a cherché à atteindre son objectif. En plus des travaux universitaires antérieurs qui ont mis en avant l’utilisation par Picart de la méthode comparative (Hunt et al., 2010), de la « con‑visualisation » des images (Von Wyss-Giacosa, 2019) et de la « dés‑orientation du soi » (Tarantino, 2021), je suggère que sa stratégie artistique doit également beaucoup à l’utilisation de la théâtralité comme dispositif rhétorique visuel et performatif pour diffuser le savoir.