bluuebunny/crossref_metadata_2025_split huggingface dataset:
SISTEM AKUNTANSI PEMBELIAN KREDIT PADA PT. GLOBAL MULTIPARTS
Authors: Fera Lufhidarani Pranita  , Wulandari Suhanda  
Published: July 2024

In general, in a company, having purchase transactions is useful for procuring merchandise. Having goods available for sale will generate profits for the company. This research aims to find out: What is the accounting system for credit purchases at PT. Global Multiparts, how is the internal control in the credit purchase accounting system at PT. Global Multiparts, what is the internal control system at PT. Global Multiparts has been running well and correctly, what are the healthy practices at PT. Global Multiparts To obtain data and information in preparing research on the accounting review of credit purchases of merchandise required in this research, the author conducted research on research and theoretical foundations as a guide so that the research focus is in accordance with the facts in the field. The research results show that the implementation of Credit Purchase Systems and Procedures at PT. Global Multiparts is running well, but there are still shortcomings such as related functions that are still not separated.
State and Trends of Reproduction of the Population and Labor Resources in the Region
Authors: Кутаев Ш.К. , Кутаева Р.А. 
Published: July 2024

Актуальность исследуемых вопросов обусловлена тем, что численность населения и трудовых ресурсов выступают важнейшими составляющими социально-экономического развития страны и регионов. Состав трудовых ресурсов, их количество и качество во многом коррелируют с проводимой в государстве соответствующей политикой. Наличие актуальных сведений и учет современных тенденций в данной сфере может послужить основой для совершенствования государственной политики регионального развития.
The relevance of the studied issues is due to the fact that the population and labor resources are the most important components of the socio-economic development of the country and regions. The composition of labor resources, their quantity and quality in many respects correlate with the corresponding policy in the state. The availability of up-to-date information and consideration of current trends in this area can serve as a basis for improving the state policy of regional development.
Tunable UV ∼ IR frequency comb generation via high-order sideband generation
Authors: Kim Jeail , Kang Hwihyeon , Elu Ugaitz , Kim Dasol , Haberstroh Florian , Sidiropoulos Themistoklis , Steinle Tobias , Baudisch Matthias , Ortmann Lisa , Landsman Alexandra S. , Biegert Jens , Chacón Alexis , Kim Dong Eon 
Published: July 2024

Abstract
We propose the generation of a widely tunable UV-to-IR frequency comb by high-order sideband generation (HSB) spectrum emitted from semiconductors. In our theoretical simulations, we demonstrate the high-order sideband signals of two series (2m

Ω
seed

+ (2n + 1)

ω
driver

,

and (2m + 1)

Ω
seed

+ 2

n

ω
driver

), where m and n are integers of a seed pulse and a driver laser frequency, respectively. The simulations also reveal the intensity of HSB scale with the driver laser power, both perturbatively and non-perturbatively. We find that the harmonic position and spacing of the high-order sideband emission can be controlled by varying the seed pulse and driver photon energies. In the experiment, we applied a visible (

ℏ

Ω
seed

= 3.1 eV, ∼400 nm) seed pulse and mid-infrared (MIR,

ℏ
ω

driver

= 0.4 eV, 3.1 μm) driver pulses to ZnSe target. Our experimental observations confirmed the UV (4.7 eV, 263 nm and 3.9 eV, 317 nm) HSB generation.
Konsumsi Ikan Gabus Mempercepat Penyembuhan Luka Pasca Bedah Caesar di RSAU Jakarta
Authors: Alfisyah Miladiah  , Luluk Eka Meylawati  , Siti Rochanah  , Muhamad Iqbal  
Published: July 2024

Ikan gabus merupakan ikan air tawar yang banyak manfaat yaitu asam amino non-esensial yang dikandungnya sangat penting dalam penyembuhan luka pada manusia. Ikan gabus banyak dikonsumsi oleh orang pasca operasi untuk membantu pemulihan luka operasi. Penelitian deskriptif mengidentifikasi manfaat ikan gabus dalam membantu penyembuhan luka operasi pasca melahirkan caesar. Penelitian ini dilakukan pada dua orang pasca persalinan caesar. Pasien 1 konsumsi ikan gabus sedangkan pasien 2 tidak mengkonsumsi ikan gabus. Penelitian ini menggunakan metode wawancara, observasi, dan pemeriksaan fisik. Alat ukur yang digunakan yaitu lembar observasi luka operasi dengan REEDA (Redness, Edema, Ecchymosis, Discharge, Approximation) dan skala nyeri. Ikan gabus dikonsumsi pasien satu kali sehari selama 4 hari di RSAU Jakarta. Hasil: Pasien 1 skor REEDA yaitu 1, skala nyeri 1, sedangkan pasien 2 yaitu skor REEDA adalah 2 dan skala nyeri 2. Kesimpulan: Konsumsi Ikan gabus baik dalam mempercepat penyembuhan luka terutama pada ibu pasca melahirkan caesar sehingga baik ditambahkan dalam konsumsi harian pasca operasi caesar.

Cork fish is a freshwater fish that has many benefits, namely the non-essential amino acids it contains are very important in wound healing in humans. Cork fish is widely consumed by people after surgery to help the recovery of surgical wounds. Descriptive research identifies the benefits of cork fish in helping wound healing after cesarean delivery. This study was conducted on two people after cesarean delivery. Patient 1 consumed cork fish while patient 2 did not consume cork fish. This study used interview, observation, and physical examination methods. The measuring instruments used were a surgical wound observation sheet with REEDA (Redness, Edema, Ecchymosis, Discharge, Approximation) and a pain scale. Cork fish was consumed by patients once a day for 4 days at RSAU Jakarta. Results: Patient 1 REEDA score is 1, pain scale is 1, while patient 2 is REEDA score is 2 and pain scale is 2. Conclusion: Consumption of cork fish is good in accelerating wound healing, especially in mothers after cesarean delivery so it is good to be added to daily consumption after cesarean section.
Size adaptation: Do you know it when you see it?
Authors: Yousif Sami R. , Clarke Sam 
Published: July 2024

AbstractThe visual system adapts to a wide range of visual features, from lower-level features like color and motion to higher-level features like causality and, perhaps, number. According to some, adaptation is a strictly perceptual phenomenon, such that the presence of adaptation licenses the claim that a feature is truly perceptual in nature. Given the theoretical importance of claims about adaptation, then, it is important to understand exactly when the visual system does and does not exhibit adaptation. Here, we take as a case study one specific kind of adaptation: visual adaptation to size. Supported by evidence from four experiments, we argue that, despite robust effects of size adaptation in the lab, (1) size adaptation effects are phenomenologically underwhelming (in some cases, hardly appreciable at all), (2) some effects of size adaptation appear contradictory, and difficult to explain given current theories of size adaptation, and (3) prior studies on size adaptation may have failed to isolate size as the adapted dimension. Ultimately, we argue that while there is evidence to license the claim that size adaptation is genuine, size adaptation is a puzzling and poorly understood phenomenon.
Semantic meaning enhances feature-binding but not quantity or precision of locations in visual working memory
Authors: Sahar Tomer , Gronau Nurit , Makovski Tal 
Published: July 2024

AbstractRecent studies showed that real-world items are better remembered in visual working memory (VWM) than visually similar stimuli that are stripped of their semantic meaning. However, the exact nature of this advantage remains unclear. We used meaningful and meaningless stimuli in a location-reproduction VWM task. Employing a mixture-modeling analysis, we examined whether semantic meaning enables more item locations to be remembered, whether it improves the precision of the locations stored in memory, or whether it improves binding between the specific items and their locations. Participants were presented with streams of four (Experiments 1 & 2) or six (Experiment 3) real-world items, or their scrambled, meaningless counterparts. Each item was presented at a unique location, and the task was to reproduce one item’s location. Overall, location memory was consistently better for real-world items compared with their scrambled counterparts. Furthermore, the results revealed that participants were less likely to make swap errors for the meaningful items, but there was no effect of conceptual meaning on the guess rate or the precision of the report. In line with previous findings, these results indicate that conceptual meaning enhances VWM for arbitrary stimulus properties such as item location, and this improvement is primarily due to a more efficient identity-location binding rather than an increase in the quantity or quality (precision) of the locations held in memory.
Filaments of the Slime Mold Cosmic Web and How They Affect Galaxy Evolution
Authors: Hasan Farhanul , Burchett Joseph N. , Hellinger Douglas , Elek Oskar , Nagai Daisuke , Faber S. M. , Primack Joel R. , Koo David C. , Mandelker Nir , Woo Joanna 
Published: July 2024

Abstract
We present a novel approach for identifying cosmic web filaments within the DisPerSE structure identification framework, using cosmic density field estimates from the Monte Carlo Physarum Machine (MCPM), inspired by the slime mold organism. We apply our method to the IllustrisTNG (TNG100) cosmological simulations and investigate the impact of filaments on galaxies. The MCPM density field is superior to the Delaunay tessellation field estimator in tracing the true underlying matter distribution and allows filaments to be identified with higher fidelity, finding more low-prominence/diffuse filaments. Using our new filament catalogs, we find that ≳90% of galaxies are located within ∼1.5 Mpc of a filamentary spine, with little change in the median star formation activity with distance to the nearest filament. Instead, we uncover a differential effect of the local filament line density, Σfil (MCPM)—the total MCPM overdensity per unit length along a filament segment—on galaxy formation: most galaxies are quenched and gas-poor near high-line density filaments at z ≤ 1. At earlier times, the filamentary environment appears to have no effect on galactic gas supply and quenching. At z = 0, quenching in

log
(

M
*

/

M
⊙

)
≳
10.5

galaxies is mainly driven by mass, while lower-mass galaxies are significantly affected by the filament line density. Satellites are far more susceptible to filaments than centrals. The local environments of massive halos are not sufficient to account for the effect of filament line density on gas removal and quenching. Our new approach holds great promise for observationally identifying filaments from galaxy surveys such as SDSS and DESI.
Closed-form Expressions for Multiscatter Dark Matter Capture Rates
Authors: Ilie Cosmin 
Published: July 2024

Abstract
Any astrophysical object can, in principle, serve as a probe of the interaction between dark matter (DM) and regular baryonic matter. This method is based on the potential observable consequences annihilations of captured DM have on the surface temperature of the object itself. In a series of previous papers we developed and validated simple analytic approximations for the total capture rates of DM valid in four distinct regions of the DM–nucleon scattering cross section (σ) versus DM particle mass (m

X
) parameter space. In this work, we summarize those previous results and extend them significantly by deriving a completely general closed-form solution for the total capture rate of DM in the multiscatter regime. Moreover, we demonstrate the existence of a region in the σ versus m

X
parameter space where the constraining power of any astrophysical object heated by annihilations of captured DM is lost. This corresponds to a maximal temperature (T
crit) any astrophysical object can have, such that it can still serve as a DM probe. Any object with observed temperature T
obs > T
crit loses its DM constraining power. We provide analytic formulae that can be used to estimate T
crit for any object.
Study of Dust Impact Signals around Mars Using MAVEN/LPW Observations
Authors: Ijaz Samia , Vaverka Jakub , Šafránková Jana , Němeček Zdeněk 
Published: July 2024

Abstract
This study investigates short (millisecond) pulses detected by the Langmuir Probe and Waves instrument on board the Mars Atmosphere and Volatile Evolution spacecraft. We present a statistical analysis of 360,000 medium-frequency burst electric field waveforms recorded in 2015; the study aims to identify and analyze the characteristics of these transient pulses. An automatic routine is used to detect waveforms with rapid fluctuations in the electric field data; this comprises over 12,000 events in the dipole and nearly 5000 in the monopole configurations. Our findings reveal that most of the pulses in monopole configuration are likely the result of interference rather than dust impacts. Our analysis mainly focuses on dipole observations, which predominantly consist of bipolar events typically associated with dust impacts. These events are mainly detected in the Martian ionosphere, where the spacecraft is negatively charged. Fewer events are recorded when the spacecraft is positively charged, with a maximum at an altitude of 1200 km. The low detection rate of dust impact signals outside the ionosphere suggests that the planet is the most probable source of these dust particles. However, the physical processes by which dust grains are lifted from the surface of the planet to high altitudes are not clear, and thus a possibility that the signals observed might not be generated by dust impacts remains for further investigation.
Quasi-stars as a Means of Rapid Black Hole Growth in the Early Universe
Authors: Coughlin Eric R. , Begelman Mitchell C. 
Published: July 2024

Abstract
JWST observations demonstrate that supermassive black holes (SMBHs) exist by redshifts z ≳ 10, providing further evidence for “direct collapse” black hole (BH) formation, whereby massive (∼103–5
M
⊙) SMBH seeds are generated within a few million years as a byproduct of the rapid inflow of gas into the centers of protogalaxies. Here we analyze the intermediate “quasi-star” phase that accompanies some direct-collapse models, during which a natal BH accretes mass from and energetically sustains (through accretion) an overlying gaseous envelope. We argue that previous estimates of the maximum BH mass that can be reached during this stage, ∼1% of the total quasi-star mass, are unphysical, and arise from underestimating the efficiency with which energy can be transported outward from regions close to the BH. We construct new quasi-star models that consist of an inner, “saturated convection” region (which conforms to a convection-dominated accretion flow near the BH) matched to an outer, adiabatic envelope. These solutions exist up to a BH mass of ∼60% of the total quasi-star mass, at which point the adiabatic envelope contains only 2% of the mass (with the remaining ∼38% in the saturated-convection region), and this upper limit is reached within a time of 20–40 Myr. We conclude that quasi-stars remain a viable route for producing SMBHs at large redshifts, which is consistent with recent JWST observations.
Debiasing with Diffusion: Probabilistic Reconstruction of Dark Matter Fields from Galaxies with CAMELS
Authors: Ono Victoria , Park Core Francisco , Mudur Nayantara , Ni Yueying , Cuesta-Lazaro Carolina , Villaescusa-Navarro Francisco 
Published: July 2024

Abstract
Galaxies are biased tracers of the underlying cosmic web, which is dominated by dark matter (DM) components that cannot be directly observed. Galaxy formation simulations can be used to study the relationship between DM density fields and galaxy distributions. However, this relationship can be sensitive to assumptions in cosmology and astrophysical processes embedded in galaxy formation models, which remain uncertain in many aspects. In this work, we develop a diffusion generative model to reconstruct DM fields from galaxies. The diffusion model is trained on the CAMELS simulation suite that contains thousands of state-of-the-art galaxy formation simulations with varying cosmological parameters and subgrid astrophysics. We demonstrate that the diffusion model can predict the unbiased posterior distribution of the underlying DM fields from the given stellar density fields while being able to marginalize over uncertainties in cosmological and astrophysical models. Interestingly, the model generalizes to simulation volumes ≈500 times larger than those it was trained on and across different galaxy formation models. The code for reproducing these results can be found at https://github.com/victoriaono/variational-diffusion-cdm
✎.
Evolution of the Secondary Electron Spectrum during Cosmic-Ray Discharge in the Universe
Authors: Ohira Yutaka 
Published: July 2024

Abstract
We recently found that streaming cosmic rays (CRs) induce a resistive electric field that can accelerate secondary electrons produced by CR ionization. In this work, we study the evolution of the energy spectrum of secondary electrons by numerically solving the one-dimensional Boltzmann equation and Ohm’s law. We show that the accelerated secondary electrons further ionize a gas, that is, an electron avalanche occurs, resulting in increased ionization and excitation of the gas. Although the resistive electric field becomes weaker than the one before the CR discharge, the weak resistive electric field weakly accelerates the secondary electrons. The quasi-steady state is almost independent of the initial resistive electric field but depends on the electron fraction in the gas. The resistive electric field in the quasi-steady state is larger for the higher electron fraction, which makes the number of secondary electrons that can ionize the gas larger, resulting in a higher ionization rate. The CR discharge could explain the high ionization rate that is observed in some molecular clouds.
Discovery of Giant Radio Sources from TGSS Alternative Data Release 1: Radio, Optical, and Infrared Properties
Authors: Bhukta Netai , Manik Souvik , Pal Sabyasachi , Mondal Sushanta K. 
Published: July 2024

Abstract
Giant radio sources (GRSs) are the single largest astrophysical objects known in the Universe that have grown to megaparsec scales (≥0.7 Mpc). GRSs are much rarer compared with normal-sized radio galaxies. Still, the reason for the formation of their gigantic sizes is under debate. We systematically search for GRSs from the TIFR Giant Metrewave Radio Telescope Sky Survey Alternative Data Release 1 at 150 MHz. We have newly identified 34 GRSs from this study. We have also studied the multiwavelength properties (radio, optical, and infrared) of these GRSs. We have used the likelihood ratio method to identify highly reliable multiwavelength counterparts of GRSs from Pan-STARRS (optical) and Wide-field Infrared Survey Explorer (mid-IR) data. We have classified GRSs based on their accretion mode of the central black holes using optical and mid-IR data. For all sources, we also discuss the principal characteristic parameters (redshift distribution, angular and projected linear size, total integrated radio flux density, spectral index, and radio power). We show the radio evolution track and the location of the GRSs in the P–D diagram. Using a radio–optical luminosity diagram, we identify GRSs in the Fanaroff–Riley classification. Only two GRGs in our sample reside close to the centers of galaxy clusters.
Accompagner vers l’apprentissage d’une langue et d’un métier
Authors: Labbé-Riou Stéphanie 
Published: July 2024

Les centres de formation d’apprentis en France accueillent de plus en plus d’apprentis plurilingues. Leur souhait est d’apprendre un métier et une langue dans un but d’insertion socioprofessionnelle. Des équipes pédagogiques proposent de les accompagner en créant un dispositif particulier : contribuer à l’apprentissage d’un métier et d’une langue par la voie de la formation professionnelle en Centre de Formation d’Apprentis (CFA). Nous présenterons le cas d’un dispositif en CFA qui se propose de favoriser l’échange entre enseignants de langue et de pratique professionnelle. La situation est complexe, elle demande un réel travail de concertation car de nombreux apprentis découvrent les codes de la scolarité en arrivant au CFA. La démarche de l’enseignement du « Français sur Objectif Spécifique » et de recherches en « Français à Visée Professionnelle » peuvent permettre de proposer des supports adaptés.
Les « types de phrases » en grammaire : une nécessité didactique ?
Authors: Kuyumcuyan Annie 
Published: July 2024

« Grammaire n° 1 en langue française » selon un dépliant publicitaire, la Grammaire méthodique du français de M. Riegel, J.-C. Pellat & R. Rioul a acquis droit de cité dans le paysage universitaire français, au terme de sa huitième réédition depuis la première intervenue en 1994. Les qualités indiscutables de l’ouvrage n’empêchent cependant pas de s’interroger sur la pertinence et l’efficacité de ses définitions de la phrase et des types de phrase pour le public étudiant auquel elle s’adresse en premier lieu.
Définition des objets grammaticaux dans les grammaires de référence et de formation
Authors: Kalinowska Irène-Marie 
Published: July 2024

Les grammaires de référence et de formation destinées aux (futurs) enseignants ont pour double mission de transformer les connaissances préexistantes et de permettre la diffusion des savoirs renouvelés parmi les publics scolaires. Ces deux objectifs, difficiles à concilier, se résument souvent en une alternative : une grammaire critique vs une grammaire enseignable. Les énoncés définitoires sont le lieu discursif où se mesurent ces deux aspects. L’analyse des scénarios définitoires dans un corpus amène à dégager plusieurs instructions d’écriture pour les grammaires à venir.
Enseignement du verbe dans des manuels de FLES : critiques et alternatives
Authors: Ulma Dominique , Lequeux Dorine , Merkusheva Maria , Texier Lauriane 
Published: July 2024

Il est communément admis que, tôt ou tard, en classe de Français langue étrangère et/ou seconde (FLES), on se heurte à (de) la grammaire, et le domaine du verbe en est un flagrant témoignage : dès les premières leçons, il faut apprendre à conjuguer. La question n’est pas de savoir s’il faut enseigner la grammaire, mais laquelle, et comment, pour quels publics. Les modèles linguistiques et didactiques à disposition des enseignants de FLES sont-ils adaptés à des apprenants faiblement scolarisés ou grammatisés ? L’article examine plusieurs points de crispation spécifiques au verbe dans trois manuels de FLES en usage auprès de ces publics, et analyse leur mise en œuvre dans une perspective critique et alternative.