bluuebunny/crossref_metadata_2025_split huggingface dataset:
ANALISIS BREAK EVEN SEBAGAI ALAT PERENCANA LABA: KASUS PADA TOKO PUTRA PASTI MANDIRI CIKAMPEK KARAWANG
Authors: Hari Sandi Santi Pertiwi pertiwi 
Published: December 2019

Abstrak
Tujuan sebuah perusahaan adalah untuk memperoleh keuntungan atau laba yang dapat di pergunakan untuk kelangsungan hidup. Mendapatkan keuntungan atau laba dan besar kecilnya laba sering menjadi ukuran kesuksesan suatu manajemen. Hal tersebut didukung oleh kemampuan manajemen di dalam melihat kemungkinan dan kesempatan dimasa yang akan datang.
Cikampek terdapat perkampungan yang penduduknya merupakan pengrajin boneka, Kampung boneka tersebut terletak di Cikampek utara tepatnya di Desa Mekar sari dan lebih dikenal sebagai Kampung baru (Kamba). Lokasi kampung boneka ini tidak jauh dari Stasiun Cikampek, Di kampung tersebut terdapat kurang lebih 50 rumah yang memproduksi boneka dan setiap rumah rata-rata terdapat 5 hingga 10 pekerja yang membuat boneka. (Kompasiana, 21/11/2011). Usaha ini dimulai dari taun 1980. Berkembang pesatnya industri boneka mendukung berkembangnya usaha dalam pemenuhan bahan baku pembuatan usaha tersebut, salah satu usaha yang menjalani pemenuhan bahan baku pembuatan boneka, topi dan lain-lain adalah Usaha dangang Putra Pasti Mandiri (PPM). Usaha ini merupakan usaha keluarga yang di dirikan pada tahun 1998, berikut merupakan laba yang diperoleh selama tiga tahun terakhir.
Volume penjualan di mana penghasilannya (revenue) tepat sama besarnya dengan biaya totalnya, sehingga perusahaan tidak mendapatkan keuntungan atau menderita kerugian dinamakan Break Even Point (Bambang Riyanto, 2010 : 360). Rumusan untuk menghitung BEP = titik impas
Penelitian ini bertujuan untuk mengetahui gambaran keseluruhan Break Even toko PPM melalui biaya tetap, biaya variable, dan volume penjulan, sehingga bisa menetukan penjulan minimum agar tidak mengalami kerugian dan menentukan perencanaan laba yang akan di capai oleh pemilik Toko. Metode pada penelitian ini menggunakan pendekatan expost facto karena variabel yang diteliti tidak dikenai suatu tindakan, perlakuan atau manipulasi, melainkan hanya meneliti dan mengungkapkan faktor-faktor yang diteliti berdasarkan keadaan yang sudah ada.
Kata Kunci : Break Even, total fixes cost, total variable cost, sales, perencana laba
ANALISIS PENGARUH KUALITAS PELAYANAN TERHADAP KEPUASAN MAHASISWA UNIVERSITAS BUANA PERJUANGAN KARAWANG
Authors: MM Wanta 
Published: December 2019

ABSTRAK Penelitian ini bertujuan untuk mengetahui pengaruh kualitas pelayanan terhadap kepuasan mahasiswa Universitas Buana Perjuangan Karawang. Penelitian ini menggunakan metode koefisien korelasi yang bertujuan untuk mengetahui tingkat hubungan antar variabel. Nilai korelasi secara parsial antara fasilitas akademik dengan kepuasan mahasiswa sebesar 0,503, mempunyai tingkat hubungan sedang dan positif atau searah. Nilai korelasi antara fasilitas akademik dengan kepuasan mahasiswa dengan variabel kontrol layanan akademik, praktikum dan proses akademik sebesar 0,072, mempunyai tingkat hubungan sangat rendah dan positif atau searah. Nilai korelasi secara parsial antara layanan akademik dengan kepuasan mahasiswa sebesar 0,655, mempunyai tingkat hubungan kuat dan positif atau searah. Nilai korelasi antara layanan akademik dengan kepuasan mahasiswa dengan variabel kontrol fasilitas akademik, praktikum dan proses akademik sebesar 0,307, mempunyai tingkat hubungan rendah dan positif atau searah. Nilai korelasi antara praktikum dengan kepuasan mahasiswa secara parsial sebesar 0,625, mempunyai tingkat hubungan kuat dan positif atau searah. Nilai korelasi antara praktikum dengan kepuasan mahasiswa dengan variabel kontrol fasilitas akademik, layanan akademik dan proses akademik sebesar 0,192, mempunyai tingkat hubungan sangat rendah dan positif atau searah. Nilai korelasi antara proses akademik dengan kepuasan mahasiswa secara parsial sebesar 0,583, mempunyai tingkat hubungan sedang dan positif atau searah. nilai korelasi antara proses akademik dengan kepuasan mahasiswa dengan variabel kontrol fasilitas akademik, layanan akademik dan praktikum sebesar 0,205, mempunyai tingkat hubungan rendah dan positif atau searah. Hasil analisis regresi analisis kualitas pelayanan terhadap kepuasan mahasiswa diperoleh nilai koefisien korelasi (R) sebesar 0,724 atau R>0, artinya bahwa terdapat hubungan kuat (0,600 â€“ 0,799 = kuat) antara kualitas pelayanan (fasilitas akademik, layanan akademik, praktikum dan proses akademik) dengan kepuasan mahasiswa. Nilai koefisien
determinasi (R Square atau R2) sebesar 0,524 atau 52,40%, Nilai tersebut menunjukan kemampuan variabel kualitas pelayanan (fasilitas akademik, layanan akademik, praktikum dan proses akademik) menjelaskan variansi pada variabel kepuasan mahasiswa sebesar 52,40% dan sisanya sebesar 47,60% dipengaruhi oleh faktor lain (e) yang tidak diikutsertakan dalam penelitian ini. Faktor lain tersebut seperti komunikasi, budaya organisasi, prestasi akademik dan lain-lain.

Kata kunci: Kualitas Pelayanan, Kepuasan Mahasiswa
Perencanaan Karir Mahasiswa Setelah Wisuda Pascasarjana
Authors: Nasution Helsa 
Published: December 2019

Setiap orang pada umumnya memerlukan lapangan kerja untuk bekerja serta hasil dengan pekerjaan yang dijabatnya terutama pada mahasiswa setelah wisuda pascasarjana. Untuk itu, seseorang harus mempersiapkan perencanaan karirnya demi untuk mencapai karir yang sesuai dengan bakat, minat dan kemampuan terutama bidang kejuruannya. Namun, kenyataan dilapangan masih ada mahasiswa setelah wisuda pascasarjana cemas dan khawatir untuk karirnya nanti. Faktor yang mempengaruhi perencanaan karir adalah kemampuan (abilities), minat (interest) dan prestasi (achievement). Penghambat seseorang dalam berkarir ialah tidak mempersiapkan dan perencanaan karirnya serta tidak memanfaatkan kesempatan yang ada. Berdasarkan hasil penelitian bahwasanya perencanaan karir informan yaitu kuliah pascasarjana, PPK (Pendidikan Profesi Konselor), Perencanaan lainnya adalah menjalin relasi, kemampuan menguasai bahasa Inggris. Kendala informan dalam mewujudkan karirnya ialah keinginan informan untuk berkarir hanya di Provinsi Riau tanah kelahiran informan. Dapat disimpulkan bahwasanya ada hambatan dalam perencanaan karir setelah wisuda pascasarjana dan masih ada kekhawatiran dalam mewujudkan karirnya nanti.
ISLAM DAN SOLIDARITAS SOSIAL: PERKEMBANGAN MASYARAKAT ISLAM PERIODE MADINAH
Authors: Yakub Muhammad 
Published: December 2019

<p>Solidaritas sosial hanya mampu dibangun dalam konsep kepemimpinan yang matang. Nabi Muhammad sebagai seorang pemimpin mampu menyatukan seluruh elemen masyarakat Madinah dan menjadikan Madinah menjadi kota yang memiliki tatanan sosial yang sangat baik. Ini ditunjukkan dari isi Piagam Madinah yang menjunjung tinggi nilai-nilai kebersamaan, tanggung jawab sosial, toleransi dan juga sikap saling menghormati. Karakter masyarakat Madinah telah tercipta dengan akhlak yang luhur dan sikap toleransi yang tinggi telah terjaga dengan baik ditengah-tengah masyarakat Madinah yang heterogen dan pluralistik. Tetapi, tidak terlepas juga Rasulullah mendapatkan gangguan baik dari kaum Yahudi, munafik dan kaum kafir Quraisy. Hijrah telah menjadi tolak ukur awal eksistensi umat Islam dalam menyampaikan pesan-pesan kedamaian dimulai dari kota Madinah.</p>
PERAN PEMBERDAYAAN KESEJAHTERAAN KELUARGA DALAM PEMBERDAYAAN WANITA DI DESA SIMATAHARI KECAMATAN KOTA PINANG KABUPATEN LABUHANBATU SELATAN
Authors: Harahap Jam'ah , Rizal Fahrul 
Published: December 2019

<p>Penelitian ini bertujuan untuk mengetahui bagaimana pemberdayaan kesejahteraan keluarga (PKK) dalam hal pemberdayaan life skill, bagaimana pemberdayaan kesejahteraan keluarga (PKK) dalam hal pembinaan rohani, dan bagaimana pemberdayaan kesejahteraan keluarga (PKK) dalam pemberdayaan kesehatan, serta mengetahui hasil dari pemberdayaan yang telah diterapkan kepada para anggota PKK. Penelitian ini termasuk jenis penelitian lapangan yaitu peneliti untuk memperoleh data lapangan (data primer) yang bersifat deskriptif kualitatif. Metode yang digunakan adalah wawancara, observasi dan dokumentasi. Peneliti ini dilakukan di Desa Simatahari Kecamatan Kota Pinang Kabupaten Labuhanbatu Selatan. Hasil penelitian yaitu (1) pemberdayaan kesejahteraan keluarga dalam hal pemberdayaan life skill dengan memberikan modal berupa peralatan keterampilan, dan mengadakan pelatihan kepada anggota pemberdayaan kesejahteraan keluarga. (2) pemberdayaan kesejahteraan keluarga dalam hal pembinaan rohani yaitu mengadakan pengajian rutin dan yasinan akbar. (3) pemberdayaan kesejahteraan keluarga dalam hal pemberdayaan kesehatan yaitu mengadakan posyandu setiap bulannya)</p>
Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae
Authors: Bauer Evan B. , White Christopher J. , Bildsten Lars 
Published: December 2019

Abstract
Some binary systems composed of a white dwarf (WD) and a hot subdwarf (sdB) helium star will make contact within the helium burning lifetime of the sdB star. The accreted helium on the WD inevitably undergoes a thermonuclear instability, causing a detonation that is expected to transition into the WD core and lead to a thermonuclear supernova (SN) while the donor orbits nearby with high velocity. Motivated by the recent discovery of fast moving objects that occupy unusual locations on the HR diagram, we explore the impact of the thermonuclear SNe on the donors in this specific double detonation scenario. We use MESA to model the binary up to the moment of detonation, then 3D Athena++ to model the hydrodynamic interaction of the SN ejecta with the donor star, calculating the amount of mass that is stripped and the entropy deposited in the deep stellar interior by the strong shock that traverses it. We show that these donor remnants are ejected with velocities primarily set by their orbital speeds: 700–900 km s−1. We model the long-term thermal evolution of remnants by introducing the shock entropy into MESA models. In response to this entropy change, donor remnants expand and brighten for timescales ranging from 106 to 108 yr, giving ample time for these runaway stars to be observed in their inflated state before they leave the galaxy. Even after surface layers are stripped, some donors retain enough mass to resume core helium burning and further delay fading for more than 108 yr.
Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1
Authors: Kim Jinhyub , Jee M. James , Perlmutter Saul , Hayden Brian , Rubin David , Huang Xiaosheng , Aldering Greg , Ko Jongwan 
Published: December 2019

Abstract
We present a detailed high-resolution weak-lensing study of SPT-CL J2106-5844 at z = 1.132, claimed to be the most massive system discovered at z > 1 in the South Pole Telescope Sunyaev–Zel’dovich survey. Based on the deep imaging data from the Advanced Camera for Surveys and Wide Field Camera 3 on board the Hubble Space Telescope, we find that the cluster mass distribution is asymmetric, composed of a main clump and a subclump ∼640 kpc west thereof. The central clump is further resolved into two smaller northwestern and southeastern substructures separated by ∼150 kpc. We show that this rather complex mass distribution is more consistent with the cluster galaxy distribution than a unimodal distribution as previously presented. The northwestern substructure coincides with the brightest cluster galaxy and the X-ray peak while the southeastern one agrees with the location of the peak in number density. These morphological features and the comparison with the X-ray emission suggest that the cluster might be a merging system. We estimate the virial mass of the cluster to be

, where the second error bar is the systematic uncertainty. Our result confirms that the cluster SPT-CL J2106-5844 is indeed the most massive cluster at z > 1 known to date. We demonstrate the robustness of this mass estimate by performing a number of tests with different assumptions on the centroids, mass–concentration relations, and sample variance.
Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85
Authors: Casey Caitlin M. , Zavala Jorge A. , Aravena Manuel , Béthermin Matthieu , Caputi Karina I. , Champagne Jaclyn B. , Clements David L. , Cunha Elisabete da , Drew Patrick , Finkelstein Steven L. , Hayward Christopher C. , Kartaltepe Jeyhan S. , Knudsen Kirsten , Koekemoer Anton M. , Magdis Georgios E. , Man Allison , Manning Sinclaire M. , Scoville Nick Z. , Sheth Kartik , Spilker Justin , Staguhn Johannes , Talia Margherita , Taniguchi Yoshiaki , Toft Sune , Treister Ezequiel , Yun Min 
Published: December 2019

Abstract
We present a physical characterization of MM J100026.36+021527.9 (a.k.a. “Mambo-9”), a dusty star-forming galaxy (DSFG) at z = 5.850 ± 0.001. This is the highest-redshift unlensed DSFG (and fourth most distant overall) found to date and is the first source identified in a new 2 mm blank-field map in the COSMOS field. Though identified in prior samples of DSFGs at 850 μm to 1.2 mm with unknown redshift, the detection at 2 mm prompted further follow-up as it indicated a much higher probability that the source was likely to sit at z > 4. Deep observations from the Atacama Large Millimeter and submillimeter Array (ALMA) presented here confirm the redshift through the secure detection of 12CO(J = 6→5) and p-H2O (21,1 → 20,2). Mambo-9 is composed of a pair of galaxies separated by 6 kpc with corresponding star formation rates of 590 M
⊙ yr−1 and 220 M
⊙ yr−1, total molecular hydrogen gas mass of (1.7 ± 0.4) × 1011
M
⊙, dust mass of (1.3 ± 0.3) × 109
M
⊙, and stellar mass of (

) × 109
M
⊙. The total halo mass, (3.3 ± 0.8) × 1012
M
⊙, is predicted to exceed 1015
M
⊙ by z = 0. The system is undergoing a merger-driven starburst that will increase the stellar mass of the system tenfold in τ
depl = 40−80 Myr, converting its large molecular gas reservoir (gas fraction of

) into stars. Mambo-9 evaded firm spectroscopic identification for a decade, following a pattern that has emerged for some of the highest-redshift DSFGs found. And yet, the systematic identification of unlensed DSFGs like Mambo-9 is key to measuring the global contribution of obscured star formation to the star formation rate density at z ≳ 4, the formation of the first massive galaxies, and the formation of interstellar dust at early times (≲1 Gyr).
Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
Authors: An Sung-Ho , Kim Juhan , Moon Jun-Sung , Yoon Suk-Jin 
Published: December 2019

Abstract
We present a statistical analysis of the flybys of dark matter halos compared to mergers, using cosmological N-body simulations. We mainly focus on gravitationally interacting target halos with mass of 1010.8–1013.0
h
−1
M
⊙, and their neighbors are counted only when the mass ratio is 1:3–3:1 and the distance is less than the sum of the virial radii of target and neighbor. The neighbors are divided into the flyby or merger samples if the pair’s total energy is greater or smaller, respectively, than the capture criterion with consideration of dynamical friction. The main results are as follows: (a) the flyby fraction increases by up to a factor of 50 with decreasing halo mass and by up to a factor of 400 with increasing large-scale density, while the merger fraction does not show any significant dependencies on these two parameters; (b) the redshift evolution of the flyby fraction is twofold, increasing with redshift at 0 < z < 1 and remaining constant at z > 1, while the merger fraction increases monotonically with redshift at z = 0 ∼ 4; (c) Multiple interactions with two or more neighbors are on average flyby-dominated, and their fraction has a mass and environment dependence similar to that for the flyby fraction; and (d) Given that flybys substantially outnumber mergers toward z = 0 (by a factor of five) and the multiple interactions are flyby-dominated, the flyby’s contribution to galactic evolution is stronger than ever at the present epoch, especially for less massive halos and in the higher density environment. We propose a scenario that connects the evolution of the flyby and merger fractions to the hierarchical structure formation process.
Chiral Effective Field Theory Description of Neutrino Nucleon–Nucleon Bremsstrahlung in Supernova Matter
Authors: Guo Gang , Martínez-Pinedo Gabriel 
Published: December 2019

Abstract
We revisit the rates of neutrino pair emission and absorption from nucleon–nucleon bremsstrahlung in supernova matter using the T-matrix formalism in the long-wavelength limit. Based on two-body potentials of chiral effective field theory (χEFT), we solve the Lippmann–Schwinger equation for the T-matrix including non-diagonal contributions. We consider final-state Pauli blocking and hence our calculations are valid for nucleons with an arbitrary degree of degeneracy. We also explore the in-medium effects on the T-matrix and find that they are relatively small for supernova matter. We compare our results with one-pion exchange rates, commonly used in supernova simulations, and calculations using an effective on-shell diagonal T-matrix from measured phase shifts. We estimate that multiple-scattering effects and correlations due to the random phase approximation introduce small corrections on top of the T-matrix results at subsaturation densities. A numerical table of the structure function is provided that can be used in supernova simulations.
Fine-scale Explosive Energy Release at Sites of Prospective Magnetic Flux Cancellation in the Core of the Solar Active Region Observed by Hi-C 2.1, IRIS, and SDO
Authors: Tiwari Sanjiv K. , Panesar Navdeep K. , Moore Ronald L. , Pontieu Bart De , Winebarger Amy R. , Golub Leon , Savage Sabrina L. , Rachmeler Laurel A. , Kobayashi Ken , Testa Paola , Warren Harry P. , Brooks David H. , Cirtain Jonathan W. , McKenzie David E. , Morton Richard J. , Peter Hardi , Walsh Robert W. 
Published: December 2019

Abstract
The second Hi-C flight (Hi-C 2.1) provided unprecedentedly high spatial and temporal resolution (∼250 km, 4.4 s) coronal EUV images of Fe ix/x emission at 172 Å of AR 12712 on 2018 May 29, during 18:56:21–19:01:56 UT. Three morphologically different types (I: dot-like; II: loop-like; III: surge/jet-like) of fine-scale sudden-brightening events (tiny microflares) are seen within and at the ends of an arch filament system in the core of the AR. Although type Is (not reported before) resemble IRIS bombs (in size, and brightness with respect to surroundings), our dot-like events are apparently much hotter and shorter in span (70 s). We complement the 5 minute duration Hi-C 2.1 data with SDO/HMI magnetograms, SDO/AIA EUV images, and IRIS UV spectra and slit-jaw images to examine, at the sites of these events, brightenings and flows in the transition region and corona and evolution of magnetic flux in the photosphere. Most, if not all, of the events are seated at sites of opposite-polarity magnetic flux convergence (sometimes driven by adjacent flux emergence), implying likely flux cancellation at the microflare’s polarity inversion line. In the IRIS spectra and images, we find confirming evidence of field-aligned outflow from brightenings at the ends of loops of the arch filament system. In types I and II the explosion is confined, while in type III the explosion is ejective and drives jet-like outflow. The light curves from Hi-C, AIA, and IRIS peak nearly simultaneously for many of these events, and none of the events display a systematic cooling sequence as seen in typical coronal flares, suggesting that these tiny brightening events have chromospheric/transition region origin.
Getters in silicon
Authors: Kharchenko Vyacheslav A. 
Published: December 2019

Gettering of rapidly diffusing metallic impurities and structural defects in silicon which is the main material for IC fabrication, high-power high-voltage devices and neutron doped silicon has been studied. Structural defect based getters and gas phase getters based on chlorine containing compounds have been analyzed. Formation of structural defect based getters requires producing intrinsic sources of dislocation generation and precipitate/dislocation agglomerate formation. We show that dislocations are generated at microcrack mouths and form a low-mobility dislocation network at inactive wafer sides. In the latter case the defects are generated in the wafer region adjacent to the active layer of the electronic component. The generation of intrinsic getters is based on the decomposition of the supersaturated oxygen solid solution in silicon which favors the formation of a complex defect system in silicon that consists of various precipitate/dislocation agglomerates. Stacking faults also form, i.e., oxide precipitates with Frank’s dislocation loop clouds. Two intrinsic getter formation methods have been considered: one is related to oxygen impurity drain from the wafer surface region and the other implies accurate control of vacancy distribution over wafer thickness. We have analyzed the effect of getters as defect structures on the reduction of the mechanical stress required for dislocation generation onset which may eventually determine the mechanical strength of silicon wafers.
The mechanism of impurity and defect gettering by gas phase medium with chlorine-containing compound additions has been considered. We show that silicon atom interaction with chlorine in the surface wafer region at high temperatures may cause the formation of vacancies which may penetrate to the specimen bulk with some probability. This leads to the case ∆Сv &gt; 0 and ∆Ci ≤ 0, which changes the composition and density of the microdefects. Examples have been given for practical use of heat treatment of silicon wafers in a chlorine-containing atmosphere during oxide film application with the aim to dissolve microdefects, drain rapidly diffusing impurities from crystal bulk and prevent the formation of generation/recombination centers during device fabrication and silicon neutron doping.
Les apports de la « psychologie du contrôle » à la recherche en contrôle de gestion
Authors: Ancelin-Bourguignon Annick , Giraud Françoise 
Published: December 2019

Cet article recense les concepts de « psychologie du contrôle » qui peuvent expliquer les aspects cognitifs du pouvoir d’agir des managers impliqués dans les processus de contractualisation et d’évaluation des performances du contrôle de gestion, ainsi que les rares travaux de recherche en contrôle de gestion qui ont jusqu’à présent mobilisé ces concepts. Nous montrons comment ces concepts permettent d’enrichir le cadre conceptuel du contrôle de gestion et de tracer de nombreuses nouvelles pistes de recherche dans le domaine.
Langue et (bi)sexualité
Authors: Hinze Hélène 
Published: December 2019

Dès l’origine, la (bi)sexualité infantile surcharge les mots de la langue de son énergie érotique hallucinatoire. Cette énergie pulsionnelle entre en conflit avec la langue d’usage qui tente de la contenir et prétend la dompter. À travers trois illustrations : les constructions syntaxiques, la traduction de la Gradiva de Jensen et un exemple clinique, l’auteur examine ces conflits et leurs effets.
Décorporation et perte de la bisexualité commune : lorsque l’enfant paraît
Authors: Suarez-Labat Hélène 
Published: December 2019

L’auteure propose un double questionnement : quelles sont les expressions de l’ancrage de la bisexualité de l’enfant qui conduisent à la construction de la différenciation des espaces psychiques ; quels sont les effets chez les parents des mouvements de décorporation de l’enfant du corps maternel vers les identifications paternelles ? Comment les parents aménagent-ils l’économie de la perte d’une bisexualité commune ? Le contre-transfert de l’analyste permet-il de mesurer les effets de cette perte ? Deux vignettes cliniques illustrent ces questions.