bluuebunny/crossref_metadata_2025_split huggingface dataset:
ТЕРМІНОЛОГІЧНА СУТНІСТЬ ТА РІВНІ ДЕРЕГУЛЮВАННЯ ЕКОНОМІКИ
Authors: Chechetova-Terashvily Т. М. 
Published: December 2015

Дерегулювання є одним із пріоритетних напрямів реформування державного управління економікою країни, що пожвавлює її соціально-економічний розвиток. У статті досліджено підходи до визначення термінологічної сутності поняття «дерегулювання» з виокремленням об’єктів даного процесу. В якості об’єктів дерегулювання можуть виступати: економічні відносини, ринкові відносини, різні сфери суспільних відносин, підприємницька діяльність тощо. Аналіз категоріального апарату дерегулювання дозволив виявити взаємопов’язаність та співвідношення понять дерегулювання, лібералізація, децентралізація, приватизація та дебюрократизація. Визначено рівні дерегулювання: мікрорівень, що передбачає зменшення ступеня втручання держави у підприємницьку діяльність; мезорівень - пов'язаний з наданням більших свобод регіональним органам влади, а також зменшення втручання держави на галузевому рівні; макрорівень, що передбачає зменшення присутності держави у таких сферах, як податкова, соціальна, бюджетна та ін.
ПІДХОДИ ДО РОЗКРИТТЯ СУТНОСТІ ФІНАНСОВОЇ БЕЗПЕКИ БАНКІВСЬКОГО СЕКТОРУ НАЦІОНАЛЬНОЇ ЕКОНОМІКИ
Authors: Vovchenko R. S. 
Published: December 2015

В статті доведено актуальність і значущість питання забезпечення фінансової безпеки банківського сектору економіки України, що зумовлює необхідність адекватного теоретичного осмислення і розробки практичного інструментарію її забезпечення в нашій країні. Розглянуті підходи до визначення сутності фінансової безпеки банківського сектору національної економіки. Висвітлена багатоаспектність тлумачення в економічній літературі понять «безпека банківського сектору», «економічна безпека банківського сектору». Наведено авторське бачення сутності фінансової безпеки банківського сектору національної економіки.
ПРИНЦИП ЗБАЛАНСОВАНОСТІ У ЗАБЕЗПЕЧЕННІ РЕЗУЛЬТАТИВНОСТІ ГОСПОДАРСЬКОЇ ДІЯЛЬНОСТІ ПІДПРИЄМСТВА
Authors: Trukhachova К. V. 
Published: December 2015

В статті розглянуто принцип збалансованості з позиції забезпечення результативності, через співвідношення основних управлінських підходів із характеристиками господарської діяльності підприємства. Виділені основні факторами зовнішнього і внутрішнього середовища, що мають найбільший вплив на господарську діяльність підприємства. Наведені приклади впливу зовнішніх і внутрішніх факторів на господарську діяльність підприємства. Визначено управління, як інструмент узгодження цілей і результатів з процесами господарської діяльності через можливості, які спрямовані на досягнення цілей, що передбачає аналіз проблем результативності і розуміння причин їх існування, а також формування зразків результативності у кожному конкретному періоді діяльності. Запропоновано загальний комплекс елементів узгодження, основаних на внутрішніх економічних, виробничо-технологічних, структурних та ринкових можливостях забезпечення результативності господарської діяльності підприємства.
Analysing the problems of science teachers that they encounter while teaching physics education
Authors: Demir Cihat 
Published: December 2015

Even though physical science is very important in our daily lives, it is insufficiently understood by students. In order for students to get a better physical education, the teachers who have given physics lesson should first eliminated the problems that they face during the teaching process. The aim of this survey is to specify the matters encountered by science teachers during the teaching of physics and to provide them with solutions. The study group consisted of 50 science teachers who worked in Diyarbakır and Batman over the period of 2014 - 2015. This research is a descriptive study carried out by content analysis. In this study, semi-structured interview have been used along with qualitative research methods. According to the research findings, the top problems that the physics teachers encountered in physics lesson while processing the topics were laboratory problems. Some solutions have been introduced for science teachers in order to help them provide a better physics education. Keywords: science teacher, physics education.
Table of Contents
Authors: Contents Table of 
Published: December 2015

<p>From the Editors</p><p><em>Huseyin Uzunboylu, Cigdem Hursen</em></p><p> </p><p>Analysing the problems of science teachers that they encounter while teaching physics education</p><p><em>Cihat Demir, Burhan Sincar, Rıdvan Çelik</em></p><p><em>296-304</em></p><p> </p><p>An investigation into the impact of reflective teaching on EFL learners’ autonomy and intrinsic motivation</p><p><em>Parisa Abdolrezapour, Elahe Fallah</em></p><p><em>305-315</em></p><p><em> </em></p><p>Awareness of consequence of high school students on loss of bio-diversity</p><p><em>Nazım Kaşot, Serap Özbaş</em></p><p><em>316-325</em></p><p><em> </em></p><p>Research on historical environments in elementary schools’ social sciences textbooks taught in Northern Cyprus</p><p><em>Nazım Kaşot, Mete Özsezer</em></p><p><em>326-337</em></p><p><em> </em></p><p>Metacognitive awareness and math anxiety in gifted students</p><p><em>Hakan Sarıcam, Üzeyir Ogurlu</em></p><p><em>338-348</em></p>
Seed Source May Determine Field‐Specific Germination and Emergence: The Source by Planting Environment Interaction
Authors: Espeland Erin K. , Perkins Lora B. , Horning Matthew E. , Johnson Richard C. 
Published: December 2015

ABSTRACTFarm environmental conditions and management practices can result in within‐cultivar differences in seed quality and lead to transgenerational plasticity (farm‐specific effects on offspring, or TGP) that affect germination and emergence in transplant fields. We used three perennial bunchgrasses, [green needlegrass (Nassella viridula) ‘Lodorm’, slender wheatgrass (Elymus trachycaulus) ‘Pryor’, and bluebunch wheatgrass (Pseudoregneria spicata) prevariety registered germplasm P‐7] to determine if seeds exhibited TGP. We also determined if TGP was affected by the interaction between production farms and planting environments (farm × environment interaction, or context‐dependent TGP), using four laboratory temperature regimes to test germination response and four field environments to test emergence response in 2013. We stored seeds in four different environments for 10 mo before repeating the experiment to test if recent seed storage conditions mitigated TGP. Context‐dependent TGP affected emergence for Pryor and Lodorm both years, however, only Pryor exhibited context‐dependent TGP for germination in 2013. Sources with low germination and emergence in the field were less likely to exhibit context‐dependent TGP. Some transplant fields did not show differences among sources, but in other transplant fields, emergence increased as much as 24% depending on farm source. The effect of recent seed storage conditions, significant only for Pryor, was opposite for germination and emergence, with room‐temperature stored seeds exhibiting the highest emergence and lowest germination. Context‐dependent TGP in emergence could not be predicted by our coarse information regarding seed production environments and storage conditions or by germination in the lab. Nonetheless, context‐dependent TGP significantly determined emergence in two of the three study species. Mechanisms underlying this phenomenon need further study to understand potential benefits and pitfalls for producers and seed buyers.
Soil Organic Carbon Stocks in Deep Soils at a Watershed Scale on the Chinese Loess Plateau
Authors: Wang Yunqiang , Han Xiangwei , Jin Zhao , Zhang Chencheng , Fang Linchuan 
Published: December 2015

Core Ideas:SOC stocks under three land uses were measured to a soil depth of 500 cm.SOC stocks in the 0‐200 cm soil layer were significantly the lowest under shrubland.Significantly higher SOC stocks occurred in the loamy than in the sandy soils.Land use, soil texture, and water significantly affected SOC stock to depths of 500 cm.A considerable amount of SOC is stored in deep soils on the Chinese Loess Plateau.An accurate evaluation of soil organic C (SOC) stocks is important to C management and to understanding fully the role of soils in the C cycle. However, SOC stocks in deep soils and the factors that affect them have been largely ignored. We measured SOC stocks and other soil properties to a depth of 500 cm (n= 73) under three land uses in the Lao Ye Man Qu watershed on the Chinese Loess Plateau. Similar patterns in the vertical distributions of SOC stocks were found under cropland, grassland, and shrubland. However, for the 0‐ to 200‐cm soil layer, SOC stocks were significantly lower under shrubland than under either cropland or grassland. The SOC stocks under cropland, grassland, and shrubland in the 0‐ to 100‐cm layer were 2.64 ± 0.67, 2.50 ± 0.69, and 1.99 ± 0.22 kg m−2, respectively; in the 0‐ to 500‐cm layer they were 8.34 ± 2.26, 8.37 ± 2.01, and 7.26 ± 1.00 kg m−2, respectively. Significantly higher SOC stocks occurred in loamy than sandy soils (P< 0.01), and they were lower at the mid than at the upper and lower slope positions. However, SOC stocks were similar in sunlit and shaded soils. Pearson correlation analysis indicated that land use, soil texture, and soil water content significantly affected SOC stocks in each 100‐cm soil layer to a depth of 500 cm. Effects of topographic features and pH varied with increasing depth. A considerable amount of SOC was stored in deep soils, indicating the SOC content dependence on time and depth. This information is essential for evaluating C fluxes, estimating C stocks, and for managing the C cycles in regions around the world with deep soils.
Limitations and Potential of Spectral Subtractions in Fourier‐Transform Infrared Spectroscopy of Soil Samples
Authors: Margenot Andrew J. , Calderón Francisco J. , Parikh Sanjai J. 
Published: December 2015

Core Ideas
Spectral subtractions are a tool for improving FTIR spectroscopy.
Minor components of soil spectra such as SOM can be resolved by subtracting interfering backgrounds (e.g., minerals).
Limitations to spectral subtractions are specific to both FTIR spectroscopy and soils.
There is strong potential to improve accuracy and applications of subtractions in soil spectra.
Soil science research is increasingly applying Fourier transform infrared (FTIR) spectroscopy for analysis of soil organic matter (SOM). However, the compositional complexity of soils and the dominance of the mineral component can limit spectroscopic resolution of SOM and other minor components. The use of spectral subtraction is an established technique for isolating specific components of multicomponent spectra, and as such is a powerful tool to improve and expand the potential of spectroscopy of soil samples. To maximize the utility of spectral subtraction and avoid its misuse, consideration must be given to the general and soil‐specific limitations of FTIR spectroscopy and subtractions, as well as specific experimental objectives. This review summarizes the history of subtractions in FTIR spectroscopy of soil samples, identifies and qualifies misconceptions and limitations on its use, and highlights trade‐offs, recent developments, and future directions on the potential of spectral subtractions to improve and expand FTIR applications in soil science.
A spectrophotometric method for the determination Co-EDTA complexes
Authors: Paraneeiswaran Arunachalam , Shukla Sudhir K , Sathyaseelan V.S. , Rao Toleti Subba 
Published: December 2015

A precise quantification of Co(II)EDTA complex is required to develop bioremediation approaches for Co(III)EDTA complex that is generated in various industrial processes. It is cumbersome to quantify Co(II)EDTA in a mixture of Co(II)EDTAand Co(III)EDTAby normal UV-visible spectrophotometric methods as both the complexes absorb significantly at 490 nm, which is the λ max of Co(II)EDTA. Whereas other sophisticated techniques such as gas chromatography, atomic absorption spectrophotometer, inductively coupled plasma-atomic emission spectroscopy can measure individual species of Co(II)EDTA or Co(III)EDTA when present alone but are ineffective to measure the Co(II)EDTAprecisely when it is mixed with Co(III)EDTA. Hence, an attempt has been made to develop a spectrophotometric method for its quantification. This paper describes the development of a simple and economic dual wavelength spectrophotometric method for the determination of Co(II)EDTAin a mixture of Co(II)EDTA and Co(III)EDTA complexes. The wavelength pair, 490-580 nm was optimized for the measurement of absorbance for this dual wavelength method of determination of Co(II)EDTA in the presence of Co(III)EDTA. Int J Appl Sci Biotechnol, Vol 3(4): 584-587
RESOLVING IONIZATION AND METALLICITY ON PARSEC SCALES ACROSS MRK 71 WITH HST-WFC3
Authors: James Bethan L. , Auger Matthew , Aloisi Alessandra , Calzetti Daniela , Kewley Lisa 
Published: December 2015

ABSTRACT
Blue compact dwarf (BCD) galaxies in the nearby universe provide a means for studying feedback mechanisms and star formation processes in low-metallicity environments in great detail. Owing to their vicinity, these local analogs to primordial young galaxies are well suited for high-resolution studies that are unfeasible for high-redshift galaxies. Here we present Hubble Space Telescope Wide Field Camera 3 observations of one such BCD, Mrk 71, one of the most powerful local starbursts known, in the light of [O ii], He ii, Hβ, [O iii], Hα, and [S ii]. At D ≃ 3.44 Mpc, this extensive suite of emission-line images enables us to explore the chemical and physical conditions of Mrk 71 on ∼2 pc scales. We use emission-line diagnostics to distinguish ionization mechanisms on a pixel-by-pixel basis and show that despite the previously reported hypersonic gas and superbubble blowout, the gas in Mrk 71 is photoionized, with no sign of shock-excited emission. He ii emission line images are used to identify up to six Wolf-Rayet stars, three of which lie on the edge of a blowout region. Using strong-line metallicity diagnostics, we present the first “metallicity image” of a galaxy, revealing chemical inhomogeneity on scales of <50 pc. We additionally demonstrate that while chemical structure can be lost at large scales, metallicity diagnostics can break down on spatial scales smaller than an H ii region. This study highlights not only the benefits of high-resolution spatially resolved observations in assessing the effects of feedback mechanisms but also the potential limitations when employing emission-line diagnostics; these results are particularly relevant as we enter the era of extremely large telescopes.
THE SENSITIVITY OF CORE-COLLAPSE SUPERNOVAE TO NUCLEAR ELECTRON CAPTURE
Authors: Sullivan Chris , O’Connor Evan , Zegers Remco G. T. , Grubb Thomas , Austin Sam M. 
Published: December 2015

ABSTRACT
A weak-rate library aimed at investigating the sensitivity of astrophysical environments to variations of electron-capture rates on medium-heavy nuclei has been developed. With this library, the sensitivity of the core-collapse and early post-bounce phases of core-collapse supernovae to nuclear electron capture is examined. The rates are adjusted by factors consistent with uncertainties indicated by comparing theoretical rates to those deduced from charge-exchange and β-decay measurements. To ensure a model-independent assessment, sensitivity studies across a comprehensive set of progenitors and equations of state are performed. We find a +16/−4% range in the mass of the inner core at shock formation and a ±20% range of peak

luminosity during the deleptonization burst. These ranges are five times as large as those seen from a separate progenitor study, where we evaluate the sensitivity of these parameters to 32 presupernova models. Additionally, the simulations are found to be more sensitive to a reduction in electron-capture rates than an enhancement, and specifically to the reduction in rates for neutron-rich nuclei near the N = 50 closed neutron shell. As measurements for medium-heavy (

) and neutron-rich nuclei are sparse, and because accurate theoretical models that account for nuclear structure considerations of individual nuclei are not readily available, rates for these nuclei may be overestimated. If more accurate estimates confirm this, results from this study indicate that significant changes to the core-collapse trajectory are expected. For this reason, experimental and theoretical efforts should focus on this region of the nuclear chart.
FORMATION OF THE DOUBLE NEUTRON STAR SYSTEM PSR J1930–1852
Authors: Shao Yong , Li Xiang-Dong 
Published: December 2015

ABSTRACT
The spin period (185 ms) and period derivative (

) of the recently discovered double neutron star (DNS) system PSR J1930–1852 indicate that the pulsar was mildly recycled through the process of Roche-lobe overflow. This system has the longest orbital period (45 days) of the known DNS systems, and can be formed from a helium star-NS binary if the initial mass of the helium star was

otherwise, the helium star would never fill its Roche-lobe. At the moment of the supernova explosion, the mass of the helium star was

. We find that the probability distribution of the velocity kick imparted to the new-born neutron star has a maximum at about

(and a tail up to

), indicating that this NS probably received a low kick velocity at birth.
AN M DWARF COMPANION AND ITS INDUCED SPIRAL ARMS IN THE HD 100453 PROTOPLANETARY DISK
Authors: Dong (董若冰) Ruobing , Zhu (朱照寰) Zhaohuan , Fung (馮澤之) Jeffrey , Rafikov Roman , Chiang (蔣詒曾) Eugene , Wagner Kevin 
Published: December 2015

ABSTRACT
Recent VLT/SPHERE near-infrared imaging observations revealed two spiral arms with a near m = 2 rotational symmetry in the protoplanetary disk around the ∼1.7 M
⊙ Herbig star HD 100453. A ∼0.3 M
⊙ M dwarf companion, HD 100453 B, was also identified at a projected separation of 120 AU from the primary. In this Letter, we carry out hydrodynamic and radiative transfer simulations to examine the scattered light morphology of the HD 100453 disk as perturbed by the companion on a circular and coplanar orbit. We find that the companion truncates the disk at ∼45 AU in scattered light images, and excites two spiral arms in the remaining (circumprimary) disk with a near m = 2 rotational symmetry. Both the truncated disk size and the morphology of the spirals are in excellent agreement with the SPHERE observations at Y, J, H, and K1-bands, suggesting that the M dwarf companion is indeed responsible for the observed double-spiral-arm pattern. Our model suggests that the disk is close to face on (inclination angle ∼5°), and that the entire disk-companion system rotates counterclockwise on the sky. The HD 100453 observations, along with our modeling work, demonstrate that double spiral arm patterns in near-infrared scattered light images can be generically produced by companions, and support future observations to identify the companions responsible for the arms observed in the MWC 758 and SAO 206462 systems.
AN EXCESS OF MID-INFRARED EMISSION FROM THE TYPE Iax SN 2014dt
Authors: Fox Ori D. , Johansson Joel , Kasliwal Mansi , Andrews Jennifer , Bally John , Bond Howard E. , Boyer Martha L. , Gehrz R. D. , Helou George , Hsiao E. Y. , Masci Frank J. , Parthasarathy M. , Smith Nathan , Tinyanont Samaporn , Dyk Schuyler D. Van 
Published: December 2015

ABSTRACT
Supernovae Type Iax (SNe Iax) are less energetic and less luminous than typical thermonuclear explosions. A suggested explanation for the observed characteristics of this subclass is a binary progenitor system consisting of a CO white dwarf primary accreting from a helium star companion. A single-degenerate explosion channel might be expected to result in a dense circumstellar medium (CSM), although no evidence for such a CSM has yet been observed for this subclass. Here we present recent Spitzer observations of the SN Iax 2014dt obtained by the SPIRITS program nearly one year post-explosion that reveal a strong mid-IR excess over the expected fluxes of more normal SNe Ia. This excess is consistent with 10−5

of newly formed dust, which would be the first time that newly formed dust has been observed to form in a Type Ia. The excess, however, is also consistent with a dusty CSM that was likely formed in pre-explosion mass-loss, thereby suggesting a single degenerate progenitor system. Compared to other SNe Ia that show significant shock interaction (SNe Ia-CSM) and interacting core-collapse events (SNe IIn), this dust shell in SN 2014dt is less massive. We consider the implications that such a pre-existing dust shell has for the progenitor system, including a binary system with a mass donor that is a red giant, a red supergiant, or an asymptotic giant branch star.
Le déterminisme entre sciences et philosophie
Authors: Henry Julie 
Published: December 2015

La pensée spinoziste semble allier deux dimensions incompatibles l’une avec l’autre : l’extension du déterminisme des corps aux esprits (les idées s’enchaînant de façon tout aussi nécessaire que les actions), et une visée éthique fondamentale (excluant de réduire les actions humaines à de simples comportements). Ce n’est alors qu’en l’étudiant en lien étroit avec cette exigence éthique forte, que nous serons à même de caractériser le déterminisme spinoziste dans sa spécificité, à savoir un déterminisme non réductionniste et sans fatalisme. Ainsi, c’est en incarnant de manière singulière le déterminisme naturel que les hommes pourront s’inscrire dans un certain devenir éthique, par le biais d’une modification de leur complexion affective, qui déterminera d’autres désirs et donc d’autres tendances d’action à l’avenir. En effet, c’est parce que les hommes sont des corps suffisamment complexes pour pouvoir être affectés différemment dans le temps qu’ils ont la possibilité d’entreprendre un cheminement éthique. L’éthique spinoziste pourra alors être comprise comme étant naturelle – au sens de ce qui ne requiert pas la possibilité de s’abstraire du déterminisme naturel, par exemple grâce à un libre arbitre –, sans être pour autant qualifiée de par nature – au sens de ce qui adviendrait spontanément, sans investissement personnel et sans effort dans le temps. Le déterministe spinoziste a donc une dimension temporelle irréductible : il consiste en retour en la possibilité d’une explication rétrospective (condition de tout changement possible), mais sans force prédictive (impliquant dès lors un certain tâtonnement affectif dans la recherche d’une certaine existence éthique).
Le déterminisme entre sciences et philosophie
Authors: Wolfe Charles T. 
Published: December 2015

Au chapitre XXI du 2 e Livre de son Essai concernant l’entendement humain , intitulé « Du Pouvoir », Locke propose une critique radicale du libre arbitre (« free will ») dans son acception traditionnelle. Il s’agit du chapitre le plus long de l’ Essai , et de l’un des plus difficiles, car Locke l’a retravaillé lors des quatre éditions successives, sans tout à fait se soucier de la cohérence entre les éléments présents dans la 1 re édition et ses ajouts conceptuels ultérieurs. Mon but est de montrer qu’il existe bel et bien une cohérence dans l’approche lockienne de la liberté, en tant qu’elle articule une forme de « compatibilisme » – c’est-à-dire la position selon laquelle le libre arbitre et le déterminisme sont compatibles. Mais la position de Locke vacille entre une reconnaissance du déterminisme (selon la dimension hédoniste de son argument) et un retrait face à ce constat (selon ce qu’il appelle la « suspension du désir »). Cette indécision, ou en tout cas cette coexistence précaire de deux visions de l’action et de la motivation, sera critiquée par le disciple préféré de Locke, le déiste Anthony Collins, dans son Enquête philosophique sur la liberté humaine (1717). Je suggérerai en conclusion que Locke a défini un espace conceptuel dans lequel le déterminisme et la reconnaissance de la spécificité de l’univers mental peuvent coexister, mais que Collins en a tiré un système plus conséquent, fondé en grande partie sur l’idée de « clôture causale ».