cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
การจัดการสิ่งแวดล้อมและการวางแผนกลยุทธ์ทางการตลาดจากมุมมองของผู้รับบริการ (4C) กรณีศึกษา กลุ่มโรงแรมที่เป็นมิตรกับสิ่งแวดล้อมในเขตกรุงเทพมหานคร
Creators: name: ระชานนท์ ทวีผล
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย
Year: 2567
Subjects: การจัดการสิ่งแวดล้อม
การวางแผนการตลาดจากมุมมองผู้รับบริการ
โรงแรมที่เป็นมิตรกับสิ่งแวดล้อม

description: วารสารวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย, 19, 68, 52
Constraints on planet X/Nemesis from Solar System's inner dynamics
Creators: name: Iorio, Lorenzo
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We put full 3D constraints on a putative planet X by using the dynamics of the inner planets of the solar system. In particular, we compute the mimium distance of X as a function of its heliocentric latitude and longitude for different values of its mass.
description: LaTex, MNRAS macros. 12 pages, 4 figures, 3 tables. To appear in Monthly Notices of the Royal Astronomical Society (MNRAS). Some typos fixed
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ² Ð»ÐµÑÐ½ÑÑ ÑÐ³Ð¾Ð´ Ð±ÑÑÑÐ½Ð¸ÐºÐ¸ Ð¸ ÐºÐ»ÑÐºÐ²Ñ Ð¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð² ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿Ð°ÑÑÐ¸Ð»ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¨ÐµÐ²ÑÐµÐ½ÐºÐ¾, ÐÐ½Ð¶ÐµÐ»Ð¸ÐºÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¾Ð±Ð¾Ð³Ð°ÑÐµÐ½Ð½ÑÐµ Ð¿Ð¸ÑÐµÐ²ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ
ÐºÐ»ÑÐºÐ²ÐµÐ½Ð½ÑÐ¹ Ð¶Ð¾Ð¼
Ð±ÑÑÑÐ½Ð¸ÑÐ½ÑÐ¹ Ð¶Ð¾Ð¼
Ð¿Ð°ÑÑÐ¸Ð»ÑÐ½ÑÐµ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ
Ð²ÑÐ¾ÑÐ¸ÑÐ½ÑÐµ Ð±Ð¸Ð¾ÑÐµÑÑÑÑÑ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ² Ð»ÐµÑÐ½ÑÑ ÑÐ³Ð¾Ð´ Ð±ÑÑÑÐ½Ð¸ÐºÐ¸ Ð¸ ÐºÐ»ÑÐºÐ²Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¸Ñ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐµÑÐµÐ¿ÑÑÑÐ°Ñ Ð¿Ð°ÑÑÐ¸Ð»ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÐ°Ð²Ð° Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð² ÑÐµÐ»ÑÐ½ÑÑ ÑÐ³Ð¾Ð´Ð°Ñ Ð¸ ÑÐ³Ð¾Ð´Ð½Ð¾Ð¼ Ð¶Ð¾Ð¼Ðµ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ»Ðµ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¾ÐºÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ ÑÐ¾ÑÑÐ°Ð½Ð½Ð¾ÑÑÐ¸ Ð² Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½Ð¾Ð¼ ÑÐ³Ð¾Ð´Ð½Ð¾Ð¼ Ð¶Ð¾Ð¼Ðµ Ð¿ÑÐ¸ ÑÐ¾Ð»Ð¾Ð´Ð¸Ð»ÑÐ½Ð¾Ð¼ ÑÑÐ°Ð½ÐµÐ½Ð¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ñ Ð² Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð² ÐÐÐ Â«ÐÐÐ¡Ð¢Ð ÐÐÐÐÂ» ÑÐµÑÐµÐ¿ÑÑÑÑ Ð¿Ð°ÑÑÐ¸Ð»ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹ Ñ Ð´Ð¾Ð±Ð°Ð²ÐºÐ°Ð¼Ð¸ ÑÐ³Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¶Ð¾Ð¼Ð° Ð±ÑÑÑÐ½Ð¸ÐºÐ¸ Ð¸ ÐºÐ»ÑÐºÐ²Ñ - Ð·ÐµÑÐ¸ÑÐ° "Ð¯Ð³Ð¾Ð´Ð½Ð°Ñ Ð¿Ð¾Ð»ÑÐ½Ð°", Ð¿Ð°ÑÑÐ¸Ð»Ñ Ð´Ð¸ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Â«Ð¯Ð³Ð¾Ð´Ð½Ð°ÑÂ» Ð¸ Â«ÐÐµÐ»ÐµÐ²ÑÐºÐ°ÑÂ» Ñ ÑÐ³Ð¾Ð´Ð½Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ»Ð¾Ð¹ÐºÐ¾Ð¹, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° Ð¿Ð¸ÑÐµÐ²Ð°Ñ ÑÐµÐ½Ð½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. ÐÐ¾Ð»ÑÑÐµÐ½Ñ ÑÐ¼Ð¿Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¸ÑÐ»Ð¾Ñ Ð¸ ÑÐµÐ½Ð¾Ð»ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð² Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½Ð¾Ð¼ ÑÐ³Ð¾Ð´Ð½Ð¾Ð¼ Ð¶Ð¾Ð¼Ðµ Ð¿ÑÐ¸ ÑÐ¾Ð»Ð¾Ð´Ð¸Ð»ÑÐ½Ð¾Ð¼ ÑÑÐ°Ð½ÐµÐ½Ð¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÐºÐ¸Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿Ð¾ÑÐµÑÐµÐ¹ ÑÐ¸ÑÐ¾Ð¼Ð¸ÐºÑÐ¾Ð½ÑÑÑÐ¸ÐµÐ½ÑÐ¾Ð².
ปัจจัยที่มีความสัมพันธ์ต่อการจัดการขยะพลาสติกของประชาชนในเขตเทศบาลเมืองมหาสารคาม จังหวัดมหาสารคาม
Creators: name: รัชชานันท์ ศรีสุภักดิ์
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย
Year: 2567
Subjects: การจัดการขยะพลาสติก
ขยะพลาสติก
ประชาชน

description: วารสารวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย, 19, 68, 64
Additional file 1 of A reduced level of the long non-coding RNA SNHG8 activates the NF-kappaB pathway by releasing functional HIF-1alpha in a hypoxic inflammatory microenvironment
Creators: name: Wang, Chenxin
name: Yang, Qiaolin
name: Han, Yineng
name: Liu, Hao
name: Wang, Yue
name: Huang, Yiping
name: Zheng, Yunfei
name: Li, Weiran
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. The sequence of siRNAs and primers used in the study.
X-ray Isophotes in a Rapidly Rotating Elliptical Galaxy: Evidence of Inflowing Gas
Creators: name: Brighenti, Fabrizio
name: Mathews, William G.
name: Humphrey, Philip J.
name: Buote, David A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We describe two-dimensional gasdynamical computations of the X-ray emitting gas in the rotating elliptical galaxy NGC 4649 that indicate an inflow of about one solar mass per year at every radius. Such a large instantaneous inflow cannot have persisted over a Hubble time. The central constant-entropy temperature peak recently observed in the innermost 150 parsecs is explained by compressive heating as gas flows toward the central massive black hole. Since the cooling time of this gas is only a few million years, NGC 4649 provides the most acutely concentrated known example of the cooling flow problem in which the time-integrated apparent mass that has flowed into the galactic core exceeds the total mass observed there. This paradox can be resolved by intermittent outflows of energy or mass driven by accretion energy released near the black hole. Inflowing gas is also required at intermediate kpc radii to explain the ellipticity of X-ray isophotes due to spin-up by mass ejected by stars that rotate with the galaxy and to explain local density and temperature profiles. We provide evidence that many luminous elliptical galaxies undergo similar inflow spin-up. A small turbulent viscosity is required in NGC 4649 to avoid forming large X-ray luminous disks that are not observed, but the turbulent pressure is small and does not interfere with mass determinations that assume hydrostatic equilibrium.
description: 21 pages, 9 figures, accepted for publication by ApJ
การวางแผนทางการเงินเพื่อสร้างความมั่นคงในวัยเกษียณอายุของบุคลากรในมหาวิทยาลัยราชภัฏเลย
Creators: name: จิราวดี กำยาน
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย
Year: 2567
Subjects: การวางแผนทางการเงิน
การเงินส่วนบุคคล
ความมั่นคงทางการเงินในวัยเกษียณอายุ

description: วารสารวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย, 19, 68, 72
The impact of charter carriers on scheduled operations
Creators: name: Feldstein, Sidney
Publisher: name: University of British Columbia
Year: 2011

description: The charter market of the airline industry has progressively grown from an insignificant segment in international traffic to a relatively significant one during the last decade. What affect has the growth of the international charter market had on scheduled operations? The scheduled operators state that charters divert a substantial amount of passenger traffic away from them thereby jeopardizing their cross-subsidization system. On the other hand, charter operators claim that not only do they serve an entirely different market segment of demand for air travel thereby causing no diversion but that they in fact generate additional business for the airline industry as a whole. The purpose of this paper then, is to attempt to determine the impact, if any, that charter carriers may have on scheduled operations. A number of hypotheses were developed which, when investigated, would indicate whether or not charter flights divert passengers away from scheduled flights. Data to test these hypotheses were obtained from questionnaires distributed, during the summer of 1970, to trans-Atlantic passengers on charter and scheduled flights. The sample size consisted of 182 charter passengers and 100 scheduled passengers. The general conclusion was that charter and scheduled passengers have different demographic characteristics. This implies that charter carriers may serve a different market segment of demand for international air travel. However, when the charter passengers, notwithstanding their demographic characteristics, were asked if they would still take this trip to Europe, either now or in the near future, if they had to fly on a scheduled airliner and pay the regular fare, almost fifty percent responded in the affirmative. Therefore, it appears that, over the trans-Atlantic route, charter carriers divert a substantial amount of passenger traffic away from scheduled carriers.
การพัฒนาระบบแจ้งเตือนการใช้บริการการซ่อมบำรุงโสตทัศนูปกรณ์ออนไลน์ คณะวิทยาการจัดการ มหาวิทยาลัยราชภัฏเลย
Creators: name: ประสิทธิ์ฏิชัย ชัยยันต์
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย
Year: 2567
Subjects: การพัฒนาระบบ
การแจ้งเตือน
ระบบออนไลน์

description: วารสารวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย, 19, 68, 82
Insights into the room temperature magnetism of ZnO/Co3O4 mixtures
Creators: name: Martin-Gonzalez, M. S.
name: Fernandez, J. F.
name: Rubio-Marcos, F.
name: Lorite, I.
name: Costa-Kramer, J. L.
name: Quesada, A.
name: Banares, M. A.
name: Fierro, J. L. G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The origin of room temperature (RT) ferromagneticlike behavior in ZnO-based diluted magnetic semiconductors is still an unclear topic. The present work concentrates on the appearance of RT magnetic moments in just mixed ZnO/Co3O4 mixtures without thermal treatment. In this study, it is shown that the magnetism seems to be related to surface reduction of the Co3O4 nanoparticles, in which, an antiferromagnetic Co3O4 nanoparticle (core) is surrounded by a CoO-like shell. This singular superficial magnetism has also been found in other mixtures with semiconductors such as TiO2 and insulators such as Al2O3.
Volume comparison for hypersurfaces in Lorentzian manifolds and singularity theorems
Creators: name: Treude, Jan-Hendrik
name: Grant, James D. E.
Publisher: name: Universität Regensburg
Year: 2012
Subjects: subject: Lorentzian geometry, comparison theorems, singularity theorems
subject: 510 Mathematik
subject: 53C23
subject: 53C80

description: We develop area and volume comparison theorems for the evolution of spacelike, acausal, causally complete hypersurfaces in Lorentzian manifolds, where one has a lower bound on the Ricci tensor along timelike curves, and an upper bound on the mean curvature of the hypersurface. Using these results, we give a new proof of Hawking's singularity theorem.
Una introducción a las analíticas de datos educativos
Creators: name: García-Peñalvo, F. J.
Publisher: name: Zenodo
Year: 2021
Subjects: Cooperación Internacional; Innovación Social; Analíticas de Aprendizaje

description: La conferencia “Una introducción a las analíticas de datos educativos” tuvo lugar el 18 de noviembre de 2021 dentro de este Laboratorio Social, como propuesta de mejora del proceso educativo siempre que las analíticas se incluyan de forma transparente en el ecosistema tecnológico de aprendizaje y en el diseño del aprendizaje, pero preservando el comportamiento ético y la privacidad de los actores implicados.
A model of the emergence and evolution of integrated worldviews
Creators: name: Gabora, Liane
name: Aerts, Diederik
Publisher: name: arXiv
Year: 2010
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: It is proposed that the ability of humans to flourish in diverse environments and evolve complex cultures reflects the following two underlying cognitive transitions. The transition from the coarse-grained associative memory of Homo habilis to the fine-grained memory of Homo erectus enabled limited representational redescription of perceptually similar episodes, abstraction, and analytic thought, the last of which is modeled as the formation of states and of lattices of properties and contexts for concepts. The transition to the modern mind of Homo sapiens is proposed to have resulted from onset of the capacity to spontaneously and temporarily shift to an associative mode of thought conducive to interaction amongst seemingly disparate concepts, modeled as the forging of conjunctions resulting in states of entanglement. The fruits of associative thought became ingredients for analytic thought, and vice versa. The ratio of associative pathways to concepts surpassed a percolation threshold resulting in the emergence of a self-modifying, integrated internal model of the world, or worldview.
ปัจจัยสิ่งแวดล้อมในองค์กรที่มีผลต่อระดับความเครียดของเจ้าหน้าที่ส่วนสารวัตรทหาร กองพันทหารสารวัตร สำนักกองบัญชาการ กองบัญชาการกองทัพไทย
Creators: name: ชนนีนาถ สุวรรณมณี
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย
Year: 2567
Subjects: ปัจจัยส่วนบุคคล
สิ่งแวดล้อมในองค์กร
ความเครียด

description: วารสารวิจัยและพัฒนา มหาวิทยาลัยราชภัฏเลย, 19, 68, 94
Interplay of Rare Earth and Iron magnetism in RFeAsO with R = La, Ce, Pr, and Sm: A muon spin relaxation study and symmetry analysis
Creators: name: Maeter, H.
name: Luetkens, H.
name: Pashkevich, Yu. G.
name: Kwadrin, A.
name: Khasanov, R.
name: Amato, A.
name: Gusev, A. A.
name: Lamonova, K. V.
name: Chervinskii, D. A.
name: Klingeler, R.
name: Hess, C.
name: Behr, G.
name: Buechner, B.
name: Klauss, H. -H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report zero field muon spin relaxation (muSR) measurements on RFeAsO with R = La, Ce, Pr, and Sm. We study the interaction of the FeAs and R (rare earth) electronic systems in the non superconducting magnetically ordered parent compounds of RFeAsO{1-x}Fx superconductors via a detailed comparison of the local hyperfine fields at the muon site with available Moessbauer spectroscopy and neutron scattering data. These studies provide microscopic evidence of long range commensurate magnetic Fe order with the Fe moments not varying by more than 15 % within the series RFeAsO with R = La, Ce, Pr, and Sm. At low temperatures, long range R magnetic order is also observed. Different combined Fe and R magnetic structures are proposed for all compounds using the muon site in the crystal structure obtained by electronic potential calculations. Our data point to a strong effect of R order on the iron subsystem in the case of different symmetry of Fe and R order parameters resulting in a Fe spin reorientation in the R ordered phase in PrFeAsO. Our symmetry analysis proves the absence of collinear Fe--R Heisenberg interactions in RFeAsO. A strong Fe--Ce coupling due to non--Heisenberg anisotropic exchange is found in CeFeAsO which results in a large staggered Ce magnetization induced by the magnetically ordered Fe sublattice far above T_N{Ce}. Finally, we argue that the magnetic R--Fe interaction is probably not crucial for the observed enhanced superconductivity in RFeAsO{1-x}Fx with a magnetic R ion.
description: 21 pages, 12 figures, text modified, citations updated, accepted for publication in Physical Review B
First-principles thermal equation of state and thermoelasticity of hcp Fe at high pressures
Creators: name: Sha, Xianwei
name: Cohen, R. E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate the equation of state and elastic properties of hcp iron at high pressures and high temperatures using first principles linear response linear-muffin-tin-orbital method in the generalized-gradient approximation. We calculate the Helmholtz free energy as a function of volume, temperature, and volume-conserving strains, including the electronic excitation contributions from band structures and lattice vibrational contributions from quasi-harmonic lattice dynamics. We perform detailed investigations on the behavior of elastic moduli and equation of state properties as functions of temperature and pressure, including the pressure-volume equation of state, bulk modulus, the thermal expansion coefficient, the Gruneisen ratio, and the shock Hugoniot. Detailed comparison has been made with available experimental measurements and theoretical predictions.
description: 33 pages, 12 figures
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð±Ð¸Ð¾Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð² Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð°ÑÑÐµÐ½ÑÐ¸ÑÐ½ÑÑ Ð¼ÑÑÐ½ÑÑ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¶, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ¸Ð¾Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÑ
ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð±Ð¸Ð¾Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÐºÐ¾Ð»Ð»Ð°Ð³ÐµÐ½Ð¾Ð²ÑÐµ Ð¾Ð±Ð¾Ð»Ð¾ÑÐºÐ¸
Ð±Ð°ÐºÑÐµÑÐ¸Ð¾ÑÐ¸Ð½Ñ
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð²Ð¾Ð·ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÑÐ°ÑÐ¸Ð½Ð½Ð¾Ð¹ ÑÐµÑÐµÐ¿ÑÑÑÑ ÐºÐ¾Ð»Ð±Ð°ÑÐ¾Ðº Â«ÐÐ¸Ð¾Ð½ÑÐºÐ¸ÐµÂ» Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÐºÑÐ»Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð±Ð¸Ð¾Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÐºÐ¾Ð»Ð»Ð°Ð³ÐµÐ½Ð¾Ð²ÑÑ Ð¾Ð±Ð¾Ð»Ð¾ÑÐµÐº Ñ Ð±Ð°ÑÑÐµÑÐ½ÑÐ¼Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼Ð¸, Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð»ÐµÐ½Ð¸Ñ ÑÑÐ¾ÐºÐ¾Ð² ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð±Ð°ÑÐ¾Ðº. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð»Ð»Ð°Ð³ÐµÐ½Ð¾Ð²ÑÑ Ð¾Ð±Ð¾Ð»Ð¾ÑÐµÐº Ð¿ÑÐµÐ¿Ð°ÑÐ°ÑÐ°Ð¼Ð¸ Bactoferm SM, Fermarom R4 Ð¸ B3, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¼Ð¸ ÑÐ¸Ð¼Ð±Ð¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÑÐ»ÑÑÑÑÑ Ð¼Ð¸ÐºÑÐ¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ñ Ð±Ð°ÐºÑÐµÑÐ¸Ð¾ÑÐ¸Ð½Ð¾Ð³ÐµÐ½Ð½ÑÐ¼Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼Ð¸ Ð¿Ð¾ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ðº ÑÐ°Ð½Ð¸ÑÐ°ÑÐ½Ð¾-Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¼Ð¸ÐºÑÐ¾ÑÐ»Ð¾ÑÐµ Ð¼ÑÑÐ½ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð².
Analysis of the Vibrational Mode Spectrum of a Linear Chain with Spatially Exponential Properties
Creators: name: Michelitsch, Thomas
name: Maugin, Gérard A.
name: Nowakowski, Andrzej. F.
name: Nicolleau, Franck C. G. A
Publisher: name: arXiv
Year: 2009
Subjects: subject: Spectral Theory (math.SP)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Mathematical Physics (math-ph)
subject: Classical Physics (physics.class-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We deduce the dynamic frequency-domain-lattice Green's function of a linear chain with properties (masses and next-neighbor spring constants) of exponential spatial dependence. We analyze the system as discrete chain as well as the continuous limiting case which represents an elastic 1D exponentially graded material. The discrete model yields closed form expressions for the $N \times N$ Green's function for an arbitrary number $N=2,..,\infty$ of particles of the chain. Utilizing this Green's function yields an explicit expression for the vibrational mode density. Despite of its simplicity the model reflects some characteristics of the dynamics of a 1D exponentially graded elastic material. As a special case the well-known expressions for the Green's function and oscillator density of the homogeneous linear chain are contained in the model. The width of the frequency band is determined by the grading parameter which characterizes the exponential spatial dependence of the properties. In the limiting case of large grading parameter, the frequency band is localized around a single finite frequency where the band width tends to zero inversely with the grading parameter. In the continuum limit the discrete Green's function recovers the Green's function of the continuous equation of motion which takes in the time domain the form of a Klein-Gordon equation.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð»Ð¸Ð¾ÑÐ¸Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¼ÑÐ»ÑÑÐ¸ÑÐµÑÐ¼ÐµÐ½ÑÐ½ÑÑ Ð·Ð°ÐºÐ²Ð°ÑÐ¾Ðº Ð½Ð° ÑÐ¾ÑÑÐ°Ð² Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¼Ð¾Ð»Ð¾ÑÐ½Ð¾Ð¹ ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¸Ð½ÐºÐ¸Ð½, ÐÐ¸ÐºÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¼ÑÐ»ÑÑÐ¸ÑÐµÑÐ¼ÐµÐ½ÑÐ½ÑÐµ Ð·Ð°ÐºÐ²Ð°ÑÐºÐ¸
Ð¼Ð¾Ð»Ð¾ÑÐ½Ð°Ñ ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐ°
Ð¿Ð»Ð¾Ð´Ð¾Ð¾Ð²Ð¾ÑÐ½ÑÐµ Ð½Ð°Ð¿Ð¸ÑÐºÐ¸
ÑÐ¼ÑÐ·Ð¸

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð¼Ð±Ð¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð»Ð¸Ð¾ÑÐ¸Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð·Ð°ÐºÐ²Ð°ÑÐ¾Ðº Ð¿ÑÑÐ¼Ð¾Ð³Ð¾ Ð²Ð½ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«Christian HansenÂ» (ÐÐ°Ð½Ð¸Ñ), ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ Ð´Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÐ¼ÐµÑÐ°Ð½Ñ, ÑÐ²Ð¾ÑÐ¾Ð³Ð°, ÑÐ²ÐµÑÐ´ÑÑ ÑÑÑÑÐ¶Ð½ÑÑ Ð¸ Ð¼ÑÐ³ÐºÐ¸Ñ ÑÑÑÐ¾Ð², ÐºÐ¸ÑÐ»Ð¾Ð¼Ð¾Ð»Ð¾ÑÐ½ÑÑ Ð½Ð°Ð¿Ð¸ÑÐºÐ¾Ð². ÐÐ¾Ð»ÑÑÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð·Ð°ÐºÐ²Ð°ÑÐ¾Ðº Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ²Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐ¸, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾ÑÐ»Ðµ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ³ÑÑÑÐºÐ°. ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð·Ð°ÐºÐ²Ð°ÑÐ¾Ðº Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐ¸ Ñ ÑÐ»ÑÑÑÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼Ð¸ Ð¸ ÐµÐµ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ ÑÑÑÐºÑÐ¾Ð²ÑÑ Ð¸ Ð¾Ð²Ð¾ÑÐ½ÑÑ Ð½Ð°Ð¿Ð¸ÑÐºÐ¾Ð² ÑÐ¼ÑÐ·Ð¸.
Geometrodynamics of Spinning Light
Creators: name: Bliokh, K. Y.
name: Niv, A.
name: Kleiner, V.
name: Hasman, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Optics (physics.optics)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The semiclassical evolution of spinning particles has recently been re-examined in condensed matter physics, high energy physics, and optics, resulting in the prediction of the intrinsic spin Hall effect associated with the Berry phase. A fundamental nature of this effect is related to the spin-orbit interaction and topological monopoles. Here we report a unified theory and a direct observation of two mutual phenomena: a spin-dependent deflection (the spin Hall effect) of photons and the precession of the Stokes vector along the coiled ray trajectory of classical geometrical optics. Our measurements are in perfect agreement with theoretical predictions, thereby verifying the dynamical action of the topological Berry-phase monopole in the evolution of light. These results may have promising applications in nano-optics and can be immediately extrapolated to the evolution of massless particles in a variety of physical systems.
description: 18 pages, 4 figures, to appear in Nature Photonics
Phase-Locked Starbirth_ Observational Evidence of Structured Resonance in Stellar Formation
Creators: name: Bostick, Devin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Stellar Formation
subject: Gravitational Waves
subject: Dark matter
subject: Dark Energy
subject: General Relativity
subject: Quantum Mechanics
subject: Black Hole Physics
subject: Resonance Fields
subject: Wavelet Analysis
subject: Tensor Field Mapping
subject: Resonance Intelligence
subject: Non-Stochastic Computation
subject: Structured Emergence
subject: Prime Harmonics
subject: Chirality
subject: Coherence Fields
subject: Field-Based Computing
subject: Resonance-Based Algorithms

description: Main Paper w/Empirical Tests

Abstract:

NASA’s James Webb Space Telescope captured the formation of a star in unprecedented detail, revealing coherent outflows, disk structures, and jet dynamics. Traditional models explain these through gravitational collapse and magnetic fields. This paper proposes an alternative interpretation using the CODES framework (Chirality of Dynamic Emergent Systems): that star formation is not a random accretion process, but a deterministic coherence event—a phase-lock between chirality, prime harmonics, and structured resonance. We show how each element of the JWST image maps directly onto key principles in CODES, and provide falsifiable predictions for resonance signatures in future observations.
title: ÐÐ¸Ð¾Ð½Ð°Ð½Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
Creators: name: ÐÐ¾Ð¿Ð¾Ð²Ð°, ÐÐ°ÑÐ¸ÑÐ°
name: ÐÑÐ¾Ð½Ð¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÐÐ°Ð½Ð¾ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 19.04.01 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð±Ð¸Ð¾Ð½Ð°Ð½Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 19.03.01 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÑÐ½Ð¾Ð²Ñ Ð±Ð¸Ð¾Ð½Ð°Ð½Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â».
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title: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ "Ð¥Ð¸Ð¼Ð¸Ñ Ð¸ ÑÐ¸Ð½ÑÐµÐ· Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ²"
title: Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸: 19.04.01 "ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ" ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ (ÑÑÐµÐ¿ÐµÐ½Ñ) Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ° - Ð¼Ð°Ð³Ð¸ÑÑÑ ; ÑÐ¾ÑÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ - Ð¾ÑÐ½Ð°Ñ, Ð·Ð°Ð¾ÑÐ½Ð°Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿Ð¾Ð²Ð°, ÐÐ°ÑÐ¸ÑÐ°
name: ÐÐ¾ÑÐºÐ°ÐµÐ²Ð°, ÐÐ²Ð³ÐµÐ½Ð¸Ñ
name: ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¸Ð½ÑÐµÐ·
ÐÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÐµ Ð²ÐµÑÐµÑÑÐ²Ð°

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 19.04.01 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¥Ð¸Ð¼Ð¸Ñ Ð¸ ÑÐ¸Ð½ÑÐµÐ· Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ²Â» Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ.
ÐÐµÑÐµÑÐ¸ÑÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¸Ð»Ð° Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð² Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ¸Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¸Ð½ÑÐµÐ·Ð° Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÑÐµÐ¼Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ°ÐºÑÐ¸Ð¹ Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð½Ð¸ÑÑÐ¾Ð±ÐµÐ½Ð·Ð¾Ð»Ð°; Ð¾- Ð¸ Ð¿-Ð½Ð¸ÑÑÐ¾ÑÐ»Ð¾ÑÐ±ÐµÐ½Ð·Ð¾Ð»Ð°; Ð°Ð½Ð¸Ð»Ð¸Ð½Ð°; ÑÐ¸ÐºÐ»Ð¾Ð³ÐµÐºÑÐµÐ½Ð°; Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð°Ð±Ð¸ÐµÑÐ¸Ð½Ð¾Ð²Ð¾Ð¹ ÐºÐ¸ÑÐ»Ð¾ÑÑ Ð¸Ð· ÑÐ°Ð»Ð»Ð¾Ð²Ð¾Ð¹ ÐºÐ°Ð½Ð¸ÑÐ¾Ð»Ð¸; 1,3- Ð¸ 1,6-Ð´Ð¸Ð½Ð¸ÑÑÐ¾ÐºÐ°ÑÐ±Ð°Ð·Ð¾Ð»Ð°; 1,3- Ð¸ 1,6-Ð´Ð¸Ð°Ð¼Ð¸Ð½Ð¾-ÐºÐ°ÑÐ±Ð°Ð·Ð¾Ð»Ð° Ð¸ Ð´Ð¸Ð°Ð·Ð¾ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¸Ð°Ð¼Ð¸Ð½Ð¾ÐºÐ°ÑÐ±Ð°Ð·Ð¾Ð»Ð¾Ð².
ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð².
Black lives matter in research and higher education too!
Creators: name: Association, Marie Curie Alumni
Publisher: name: Zenodo
Year: 2020

description: See PDF below for full statement. Web: https://www.mariecuriealumni.eu ; This statement is released under a CC BY license. Please reference this statement using http://doi.org/10.5281/zenodo.3984824 Link to all MCAA statements: https://zenodo.org/communities/mcaa/
Poisson-Lie T-dual sigma models on supermanifolds
Creators: name: Eghbali, A.
name: Rezaei-Aghdam, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate Poisson-Lie symmetry for T-dual sigma models on supermanifolds in general and on Lie supergroups in particular. We show that the integrability condition on this super Poisson-Lie symmetry is equivalent to the super Jacobi identities of the Lie super-bialgebras. As examples we consider models related to four dimensional Lie super-bialgebras $((2A1,1 + 2A)^1, D10_p=1/2)$ and $((2A1,1 + 2A)^1, I)$. Then generally it is shown that for Abelian case (g, I) the super Poisson-Lie T-duality transforms the role of fermionic (bosonic) fields in the model to bosonic (fermionic) fields on the dual model and vice versa.
description: 13 pages, Revised and accepted for publication in JHEP
Counterexamples to the sonic criterion
Creators: name: Elling, Volker
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 76L05; 76H05

description: We consider self-similar (pseudo-steady) shock reflection at an oblique wall. There are three parameters: wall corner angle, Mach number, angle of incident shock. Ever since Ernst Mach discovered the irregular reflection named after him, it has been an open problem to predict precisely for what parameters the reflection is regular. Three conflicting proposals, the detachment, sonic and von Neumann criteria, have been studied extensively without a clear result. We demonstrate that the sonic criterion is not correct. We consider polytropic potential flow and prove that there is an open nonempty set of parameters that admit a global regular reflection with a reflected shock that is \emph{transonic}. We also provide a clear physical reason: the flow type (sub- or supersonic) is not decisive; instead the reflected shock type (weak or strong) determines whether structural perturbations decay towards the reflection point.
title: ÐÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÑÑÑÑ Ð¸ Ð³Ð¾ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð£ÐÐ¡Ð 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â»
titleType: Subtitle
Creators: name: ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
name: Ð¡Ð¼Ð¾Ð»ÐµÐ½ÑÐµÐ²Ð°, ÐÐ»Ð»Ð°
name: ÐÐ»Ð¸ÑÐµÐµÐ²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: Ð¤ÐµÐ´Ð¸Ð½Ð¸ÑÐ¸Ð½Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: Ð¡ÐµÐ²Ð°ÑÑÑÑÐ½Ð¾Ð²Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°ÑÐµÑÑÐ²Ð°
Ð¿Ð¸ÑÐµÐ²Ð¾Ðµ ÑÑÑÑÐµ
Ð³Ð¾ÑÐ¾Ð²Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ
ÐºÑÐ»Ð¸Ð½Ð°ÑÐ½ÑÐµ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÑÑÑÑ Ð¸ Ð³Ð¾ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸Â» Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð£ÐÐ¡Ð 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â» / Ð°Ð²ÑÐ¾ÑÑ: Ð®. Ð. ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð. Ð. Ð¡Ð¼Ð¾Ð»ÐµÐ½ÑÐµÐ²Ð°, Ð¡. Ð. ÐÐ»Ð¸ÑÐµÐµÐ²Ð°, Ð. Ð®. Ð¤ÐµÐ´Ð¸Ð½Ð¸ÑÐ¸Ð½Ð°, Ð. Ð. Ð¡ÐµÐ²Ð°ÑÑÑÑÐ½Ð¾Ð²Ð° â Ð¡ÐÐ±ÐÐ£, 2020. â 35 Ñ.

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Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÑÐ½ÑÐµ ÑÐµÐ¼Ñ, ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÑÑÑÐºÑÑÑÐµ, ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾Ð± Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°ÑÐ¸ÑÑ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
ÐÑÐ°Ð²Ð¸Ð»Ð° Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð·Ð°Ð¿Ð¸ÑÐºÐ¸ Ð¸ Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð·Ð°ÑÐ¸ÑÑ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÐÐ¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¡ÐÐ±ÐÐ£.
Pulsars as Fantastic Objects and Probes
Creators: name: Han, J. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Pulsars are fantastic objects, which show the extreme states of matters and plasma physics not understood yet. Pulsars can be used as probes for the detection of interstellar medium and even the gravitational waves. Here I review the basic facts of pulsars which should attract students to choose pulsar studies as their future projects.
description: Invited Lecture on the "First Kodai-Trieste Workshop on Plasma Astrophysics", Kodaikanal Obs, India. Aug.27-Sept.7th, 2007. In: "Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes". Get a copy from: http://www.springerlink.com/content/978-1-4020-8867-4
Properties of thin yttrium oxide dielectric films.
Creators: name: Riemann, Ernest B.
Publisher: name: University of British Columbia
Year: 2011

description: A study has been made of the properties of thin yttrium oxide dielectric films prepared by the electron beam evaporation of high purity Y₂O₃ powder. Films deposited on freshly cleaved NaCl crystals and on polished n-type silicon were examined in the electron microscope. The specimens were found to be polycrystalline, with a crystal size of the order of 100 Å. The structure was found to be essentially the same as found for bulk Y₂O₃. D.C. conduction measurements were made on films of various thicknesses. The characteristics were found to be bulk-limited, with the conductivity decreasing at lower pressures. An activation energy of 0.6 eV was found. The conduction mechanism was believed to be Poole-Frenkel emission of electrons from donor centers into the Y₂O₃ conduction band. The donor centers were believed to be interstitial yttrium atoms rather than oxygen vacancies because of the pressure dependence observed in conductivity. Step response measurements were made, and the results explained on the basis of a loss peak with a most probable relaxation time of 200 seconds. The relaxation of oxygen atoms dissolved in the anion defective Y₂O₃ lattice was assumed to be the mechanism. The results of step response and A.C. bridge loss measurements indicated that different relaxation mechanisms are dominant in different frequency ranges. Internal photoemission measurements were made on Al-Y₂O₃-Al sandwiches. The energy barrier between the electrodes was found to be trapezoidal, with barrier heights of 3.14 and 3.72 eV.
Determinants of Environmental, Social, and Governance Performance in Nigeria
Creators: name: Nnadi, Okechukwu
name: Yahaya, Onipe Adabenege
Publisher: name: Zenodo
Year: 2024
Subjects: audit firms
audit committees
earnings quality
Nigeria

description: This study examines whether audit firms and audit committees contribute to enhancing earnings quality in publicly listed companies. It investigates how the index of audit firms (derived from size, opinion, independence, tenure, quality, and rotation) and audit committees (derived from independence, financial expertise, size, meetings, and gender) impact the accuracy and reliability of reported earnings. An empirical approach is employed using a sample of publicly listed companies over five years. The study utilizes a quantitative methodology, conducting regression analyses to evaluate the relationship between audit firm quality, audit committee characteristics, and earnings quality, as measured by accruals-based metrics and earnings restatements. The results suggest that higher-quality audit firms, particularly the Big 4, and more independent and financially expert audit committees are associated with improved earnings quality. The findings show that these factors reduce earnings manipulation, enhance transparency, and foster higher levels of financial reporting reliability. The study is limited by its focus on publicly listed companies, which may not generalize to private firms or those in non-regulated markets. Additionally, the study is restricted to a specific geographical region, limiting cross-country comparisons. For practitioners, the results highlight the importance of choosing reputable audit firms and ensuring audit committees are composed of independent, financially knowledgeable members to enhance financial reporting quality. The research contributes to greater trust in financial markets by demonstrating that robust governance mechanisms, such as high-quality audits and audit committees, play a vital role in protecting investors' interests and promoting corporate transparency. The study provides evidence that supports strengthening regulatory policies concerning audit firm qualifications and the composition of audit committees to improve corporate governance and protect shareholders. This paper adds value to the existing literature by providing empirical evidence on the combined effect of audit firms and audit committees on earnings quality, offering insights into their complementary roles in enhancing the integrity of financial reporting.
Formation Process of the Circumstellar Disk: Long-term Simulations in the Main Accretion Phase of Star Formation
Creators: name: Machida, Masahiro N.
name: Inutsuka, Shu-ichiro
name: Matsumoto, Tomoaki
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The formation and evolution of the circumstellar disk in unmagnetized molecular clouds is investigated using three-dimensional hydrodynamic simulations from the prestellar core until the end of the main accretion phase. In collapsing clouds, the first (adiabatic) core with a size of ~10AU forms prior to the formation of the protostar. At its formation, the first core has a thick disk-like structure, and is mainly supported by the thermal pressure. After the protostar formation, it decreases the thickness gradually, and becomes supported by the centrifugal force. We found that the first core is a precursor of the circumstellar disk. This indicates that the circumstellar disk is formed before the protostar formation with a size of ~10AU, which means that no protoplanetary disk smaller than <10AU exists. Reflecting the thermodynamics of the collapsing gas, at the protostar formation epoch, the circumstellar disk has a mass of ~0.01-0.1 solar mass, while the protostar has a mass of ~10^-3 solar mass. Thus, just after the protostar formation, the circumstellar disk is about 10-100 times more massive than the protostar. Even in the main accretion phase that lasts for ~10^5yr, the circumstellar disk mass dominates the protostellar mass. Such a massive disk is unstable to gravitational instability, and tends to show fragmentation. Our calculations indicate that the planet or brown-dwarf mass object may form in the circumstellar disk in the main accretion phase. In addition, the mass accretion rate onto the protostar shows strong time variability that is caused by the perturbation of proto-planets and/or the spiral arms in the circumstellar disk. Such variability provides a useful signature for detecting the planet-sized companion in the circumstellar disk around very young protostars.
description: 32 pages, 11 figures, Submitted to ApJ. For high resolution figures see http://www2-tap.scphys.kyoto-u.ac.jp/~machidam/astro-ph/CircumstellarDisk.pdf
title: ÐÐ°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Â«ÐÐ¸ÑÐµÐ²Ð°Ñ Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ»
title: Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° ÑÐºÑÑÐ¿Ð½ÐµÐ½Ð½Ð¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â»
titleType: Subtitle
Creators: name: ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
name: ÐÐ²Ð°Ð½ÑÐµÐ½ÐºÐ¾, ÐÐ»ÑÐ³Ð°
name: Ð¡ÐµÐ²Ð°ÑÑÑÑÐ½Ð¾Ð²Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
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description: ÐÐ°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Â«ÐÐ¸ÑÐµÐ²Ð°Ñ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐºÑÑÐ¿Ð½ÐµÐ½Ð½Ð¾Ð¹ Ð³ÑÑÐ¿Ð¿Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â».
Ð¦ÐµÐ»ÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼Ð° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÑÐ¼ÐµÐ½Ð¸Ð¹ Ð¸ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð¿ÑÐ¾ÑÐµÐºÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸ ÑÑÐ°Ð½ÐµÐ½Ð¸Ð¸ Ð¿Ð¸ÑÐµÐ²Ð¾Ð³Ð¾ ÑÑÑÑÑ Ð¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÐ°ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ, Ð¾ÐºÐ°Ð·Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¿ÑÐ¸ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ¸ÑÐµÐ²Ð°Ñ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ».
ÐÐ¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ°Ð¶Ð´Ð¾Ð¹ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼Ð° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ: ÑÐµÐ¼Ñ, ÑÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ, Ð·Ð°Ð´Ð°Ð½Ð¸Ñ, Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ, Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÑÐµÑÐ°.
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Correlated electrons in Fe-As compounds: a quantum chemical perspective
Creators: name: Hozoi, L.
name: Fulde, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: State-of-the-art quantum chemical methods are applied to the study of the multiorbital correlated electronic structure of a Fe-As compound, the recently discovered LiFeAs. Our calculations predict a high-spin, S=2, ground-state configuration for the Fe ions, which shows that the on-site Coulomb interactions are substantial. Also, orbital degeneracy in the (xz,yz) sector and a three-quarter filling of these levels suggest the presence of strong fluctuations and are compatible with a low metallic conductivity in the normal state. The lowest electron-removal states have As 4p character, in analogy to the ligand hole states in p-type cuprate superconductors.
title: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¸ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 19.06.01 "ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸"
titleType: Subtitle
Creators: name: ÐÐ°Ð·Ð°ÑÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
name: ÐÐ²Ð°Ð½ÑÐµÐ½ÐºÐ¾, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
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