cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Inverse Magnetic Catalysis in the Soft-Wall Model of AdS/QCD
Creators: name: Li, Danning
name: Huang, Mei
name: Yang, Yi
name: Yuan, Pei-Hung
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Magnetic effects on chiral phase transition have been investigated in a modified soft-wall AdS/QCD model, in which the dilaton field is taken to be negative at the ultraviolet region and positive at the infrared region as in Phys.Rev.D93(2016),101901 and JHEP1604(2016)036. The magnetic field is introduced into the background geometry by solving the Einstein-Maxwell system. After embedding the magnetized background geometry into the modified soft-wall model, the magnetic field dependent behavior of chiral condensate is worked out numerically. It is found that, in the chiral limit, the chiral phase transition remains as a second order at finite magnetic field $B$, while the symmetry restoration temperature and chiral condensate decrease with the increasing of magnetic field in small $B$ region. When including finite quark mass effect, the phase transition turns to be a crossover one, and the transition temperature still decreases with increasing magnetic field $B$ when $B$ is not very large. In this sense, inverse magnetic catalysis effect is observed in this modified soft-wall AdS/QCD model.
description: 18 pages, 6 figures, regular article
Weyl Representation of the Canonical Commutation Relations Algebras in a Krein Space
Creators: name: Mnatsakanova, M. N.
name: Salinsky, S. G.
name: Vernov, Yu. S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the present article the existence of the Weyl representation for the canonical commutation relations algebras was proved in a Krein space.
description: 9 pages
Wrapped and Stacked: ‘Smart Contracts’ and the Interaction of Natural and Formal Language
Creators: name: Allen, J. G.
Publisher: name: Humboldt-Universität zu Berlin
Year: 2018
Subjects: subject: 340 Recht

description: This publication is with permission of the rights owner freely accessible due to an Alliance licence and a national licence (funded by the DFG, German Research Foundation) respectively.
description: This article explores ‘smart contracts’ from first principles: What they are, whether they are properly called ‘contracts’, and what issues they raise for national contract law. A ‘smart’ contract purports to record contractual promises in language which is both intelligible to human beings and (ultimately) executable by machines. The formalisation of contracting language that this entails is, I argue, the most important aspect for lawyers—just as important as the automation of contractual performance. Rather than taking a doctrinal approach focused on the presence of traditional indicia of contract formation, I examine the nature of contracts as legal entities created by words and documents. In most cases, smart contracts will be ‘wrapped in paper’ and nested in a national legal system. Borrowing from the idiom of computer science, I introduce the term ‘contract stack’ to highlight the complex nature of contracts as legal entities incorporating different ‘layers’, including speech acts by the parties in both natural and formal languages as well as mandatory legal rules. It is the interactions within this contract stack that will be most important to the development of contract law doctrines appropriate to smart contracts. To illustrate my points, I explore a few issues that smart contracts might raise for English contract law. I touch on the questions of illegality, jurisdiction, and evidence, but my focus in this paper is on exploring issues in contract law proper. This contribution should be helpful not only to lawyers attempting to understand smart contracts, but to those involved in coding smart contracts—and writing the languages used to code them.
A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
Creators: name: Pascucci, I.
name: Testi, L.
name: Herczeg, G. J.
name: Long, F.
name: Manara, C. F.
name: Hendler, N.
name: Mulders, G. D.
name: Krijt, S.
name: Ciesla, F.
name: Henning, Th.
name: Mohanty, S.
name: Drabek-Maunder, E.
name: Apai, D.
name: Szucs, L.
name: Sacco, G.
name: Olofsson, J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The disk mass is among the most important input parameter for every planet formation model to determine the number and masses of the planets that can form. We present an ALMA 887micron survey of the disk population around objects from 2 to 0.03Msun in the nearby 2Myr-old Chamaeleon I star-forming region. We detect thermal dust emission from 66 out of 93 disks, spatially resolve 34 of them, and identify two disks with large dust cavities of about 45AU in radius. Assuming isothermal and optically thin emission, we convert the 887micron flux densities into dust disk masses, hereafter Mdust. We find that the Mdust-Mstar relation is steeper than linear with power law indices 1.3-1.9, where the range reflects two extremes of the possible relation between the average dust temperature and stellar luminosity. By re-analyzing all millimeter data available for nearby regions in a self-consistent way, we show that the 1-3 Myr-old regions of Taurus, Lupus, and Chamaeleon I share the same Mdust-Mstar relation, while the 10Myr-old Upper Sco association has a steeper relation. Theoretical models of grain growth, drift, and fragmentation reproduce this trend and suggest that disks are in the fragmentation-limited regime. In this regime millimeter grains will be located closer in around lower-mass stars, a prediction that can be tested with deeper and higher spatial resolution ALMA observations.
description: ApJ, in press
Evaluation of toroidal torque by non-resonant magnetic perturbations in tokamaks for resonant transport regimes using a Hamiltonian approach
Creators: name: Albert, Christopher G.
name: Heyn, Martin F.
name: Kapper, Gernot
name: Kasilov, Sergei V.
name: Kernbichler, Winfried
name: Martitsch, Andreas F.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Toroidal torque generated by neoclassical viscosity caused by external non-resonant, non-axisymmetric perturbations has a significant influence on toroidal plasma rotation in tokamaks. In this article, a derivation for the expressions of toroidal torque and radial transport in resonant regimes is provided within quasilinear theory in canonical action-angle variables. The proposed approach treats all low-collisional quasilinear resonant NTV regimes including superbanana plateau and drift-orbit resonances in a unified way and allows for magnetic drift in all regimes. It is valid for perturbations on toroidally symmetric flux surfaces of the unperturbed equilibrium without specific assumptions on geometry or aspect ratio. The resulting expressions are shown to match existing analytical results in the large aspect ratio limit. Numerical results from the newly developed code NEO-RT are compared to calculations by the quasilinear version of the code NEO-2 at low collisionalities. The importance of the magnetic shear term in the magnetic drift frequency and a significant effect of the magnetic drift on drift-orbit resonances are demonstrated.
Chiral spiral induced by a strong magnetic field
Creators: name: Abuki, H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the modification of the chiral phase structure of QCD due to an external magnetic field. We first demonstrate how the effect of magnetic field can systematically be incorporated into a generalized Ginzburg-Landau framework. We then analyze the phase structure in the vicinity of the chiral critical point. In the chiral limit, the effect is found to be so drastic that it totally washes the tricritical point out of the phase diagram, bringing the continent for the chiral spiral. This is the case no matter how small is the intensity of the magnetic field. On the other hand, the current quark mass protects the chiral critical point from a weak magnetic field. However the critical point will eventually be covered by the chiral spiral phase as the magnetic field grows.
description: 6 pages, 6 eps figures. Presented at QCD@Work 2016: International Workshop on QCD - Theory and Experiment, June 27-30, Martina-Franca (Italy)
Einasto Profiles and the Dark Matter Power Spectrum
Creators: name: Ludlow, Aaron D.
name: Angulo, Raul E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the mass accretion histories (MAHs) and density profiles of dark matter halos using N-body simulations of self-similar gravitational clustering from scale-free power spectra, $P(k)\propto k^n$. We pay particular attention to the density profile curvature, which we characterize using the shape parameter, $α$, of an Einasto profile. In agreement with previous findings our results suggest that, despite vast differences in their MAHs, the density profiles of virialized halos are remarkably alike. Nonetheless, clear departures from self-similarity are evident: for a given spectral index, $α$ increases slightly but systematically with "peak height", $ν\equivδ_{sc}/σ(M,z)$, regardless of mass or redshift. More importantly, however, the "$α-ν$" relation depends on $n$: the steeper the initial power spectrum, the more gradual the curvature of both the mean MAHs and mean density profiles. These results are consistent with previous findings connecting the shapes of halo mass profiles and MAHs and imply that dark matter halos are not structurally self-similar but, through the merger history, retain a memory of the linear density field from which they form.
description: MNRAS letters, accepted
Abundance trend with condensation temperature for stars with different Galactic birth places
Creators: name: Adibekyan, V.
name: Delgado-Mena, E.
name: Figueira, P.
name: Sousa, S. G.
name: Santos, N. C.
name: Hernandez, J. I. Gonzalez
name: Minchev, I.
name: Faria, J. P.
name: Israelian, G.
name: Harutyunyan, G.
name: Suarez-Andres, L.
name: Hakobyan, A. A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: During the past decade, several studies reported a correlation between chemical abundances of stars and condensation temperature (also known as Tc trend). However, the real astrophysical nature of this correlation is still debated. The main goal of this work is to explore the possible dependence of the Tc trend on stellar Galactocentric distances, Rmean. We used high-quality spectra of about 40 stars observed with the HARPS and UVES spectrographs to derive precise stellar parameters, chemical abundances, and stellar ages. A differential line-by-line analysis was applied to achieve the highest possible precision in the chemical abundances. We confirm previous results that [X/Fe] abundance ratios depend on stellar age and that for a given age, some elements also show a dependence on Rmean. When using the whole sample of stars, we observe a weak hint that the Tc trend depends on Rmean. The observed dependence is very complex and disappears when only stars with similar ages are considered. To conclude on the possible dependence of the Tc trend on the formation place of stars, a larger sample of stars with very similar atmospheric parameters and stellar ages observed at different Galactocentric distances is needed
description: Accepted by A&A
Non-Abelian Vortex in Four Dimensions as a Critical Superstring
Creators: name: Shifman, M.
name: Yung, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss recent progress in describing a certain non-Abelian vortex string as a critical superstring on a conifold and clarify some subtle points. This particular solitonic vortex is supported in four-dimensional N=2 supersymmetric QCD with the U(2) gauge group, N_f=4 quark flavors and the Fayet-Iliopoulos term. Under certain conditions the non-Abelian vortex can become infinitely thin and can be interpreted as a critical ten-dimensional superstring. In addition to four translational moduli the non-Abelian vortex under consideration carries six orientational and size moduli. The vortex moduli dynamics are described by a two-dimensional sigma model with the target space {R}^4\times Y_6 where Y_6 is a non-compact Calabi-Yau conifold. The closed string states which emerge in four dimensions (4D) are identified with hadrons of 4D bulk N=2 QCD. It turns out that most of the states arising from the ten-dimensional graviton spectrum are non-dynamical in 4D. A single dynamical massless hypermultiplet associated with the deformation of the complex structure of the conifold is found. It is interpreted as a monopole-monopole baryon of the 4D theory (at strong coupling).
description: 9 pages, Invited contribution to JETP Letters. arXiv admin note: substantial text overlap with arXiv:1605.01472, arXiv:1605.08433 v2: minor textual changes
Die Chemie Pilotanlage der FHNW Muttenz
Creators: name: Zogg, Andreas
name: Asprion, Jonas
Publisher: name: My University
Year: 2023
Subjects: subject: Safety
subject: Prozesssicherheit
subject: Scale Down Reactor
subject: Miniplant 4.0
subject: Scale Down Reaktor
subject: 540 - Chemie

description: Der Verein Miniplant 4.0 entwickelt im Process Technology Center an der FHNW neuartige Chemie-Pilotanlagen im Miniplant-Massstab. Der zentrale Scale-Down-Reaktor dient der präzisen Prozessentwicklung im Rührkessel. Insbesondere werden darin die lokalen thermischen Verhältnisse des Produktionsreaktors durch den Einsatz eines speziell designten Wärmetauschers exakt nachgebildet. Damit wird den Studenten und lokalen Unternehmen ein neuartiges Entwicklungswerkzeug zur Verfügung gestellt, welches einen schnelleren und präziseren Scale-Up von Produktionsverfahren direkt aus dem Labormassstab in den Produktionsreaktor erlaubt. Herr Prof. Dr. Andreas Zogg von der FHNW in Muttenz zeigt Ihnen den aktuellen Status der Anlage und die vielseitigen Schulungs- und Forschungsmöglichkeiten. Unterstützt wird er durch Herrn Dr. Jonas Asprion von der Firma Tool-Temp AG, welche die Kommerzialisierung der Temperierlösungen für Reaktormantel und Wärmetauscher anstrebt.
Flow-Through Porous Silicon Membranes for Real-Time Label-Free Biosensing
Creators: name: Zhao, Yiliang
name: Gaur, Girija
name: Retterer, Scott T.
name: Laibinis, Paul E.
name: Weiss, Sharon M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A flow-through sensing platform based on open-ended porous silicon (PSi) microcavity membranes that are compatible with integration in on-chip sensor arrays is demonstrated. Due to the high aspect ratio of PSi nanopores, the performance of closed-ended PSi sensors is limited by infiltration challenges and slow sensor responses when detecting large molecules such as proteins and nucleic acids. In order to improve molecule transport efficiency and reduce sensor response time, open-ended PSi nanopore membranes were used in a flow-through sensing scheme, allowing analyte solutions to pass through the nanopores. The molecular binding kinetics in these PSi membranes were compared through experiments and simulation with those from closed-ended PSi films of comparable thickness in a conventional flow-over sensing scheme. The flow-through PSi membrane resulted in a six-fold improvement in sensor response time when detecting a high molecular weight analyte (streptavidin) versus in the flow-over PSi approach. This work demonstrates the possibility of integrating multiple flow-through PSi sensor membranes within parallel microarrays for rapid and multiplexed label-free biosensing.
description: 8 pages, 8 figures and 9 pages of supporting information
The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3
Creators: name: Vulcani, Benedetta
name: Treu, Tommaso
name: Schmidt, Kasper B.
name: Morishita, Takahiro
name: Dressler, Alan
name: Poggianti, Bianca M.
name: Abramson, Louis
name: Bradač, Marusa
name: Brammer, Gabriel B.
name: Hoag, Austin
name: Malkan, Matthew
name: Pentericci, Laura
name: Trenti, Michele
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Exploiting the slitless spectroscopy taken as part of the Grism Lens-Amplified Survey from Space (GLASS), we present an extended analysis of the spatial distribution of star formation in 76 galaxies in 10 clusters at 0.3< z <0.7. We use 85 foreground and background galaxies in the same redshift range as a field sample. The samples are well matched in stellar mass (10^8-10^11 M_sun) and star formation rate (0.5-50 M_sun/yr). We visually classify galaxies in terms of broad-band morphology, Halpha morphology and likely physical process acting on the galaxy. Most Halpha emitters have a spiral morphology (41+/-8% in clusters, 51+/-8% in the field), followed by mergers/interactions (28+/-8%, 31+/-7%, respectively) and early-type galaxies (remarkably as high as 29+/-8% in clusters and 15+/-6% in the field). A diversity of Halpha morphologies is detected, suggesting a diversity of physical processes. In clusters, 30+/-8% of the galaxies present a regular morphology, mostly consistent with star formation diffused uniformly across the stellar population (mostly in the disk component, when present). The second most common morphology (28+/-8%) is asymmetric/jellyfish, consistent with ram pressure stripping or other non-gravitational processes in 18+/-8% of the cases. Ram pressure stripping appears significantly less prominent in the field (2+/-2%), where the most common morphology/mechanism appears to be consistent with minor gas rich mergers or clump accretion. This work demonstrates that while environment specific mechanisms affect galaxy evolution at this redshift, they are diverse and their effects subtle. A full understanding of this complexity requires larger samples and detailed and spatially resolved physical models.
description: ApJ in press (22 pages, 21 figures)
Time-dependent density-functional description of nuclear dynamics
Creators: name: Nakatsukasa, Takashi
name: Matsuyanagi, Kenichi
name: Matsuo, Masayuki
name: Yabana, Kazuhiro
Publisher: name: arXiv
Year: 2016
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present the basic concepts and recent developments in the time-dependent density functional theory (TDDFT) for describing nuclear dynamics at low energy. The symmetry breaking is inherent in nuclear energy density functionals (EDFs), which provides a practical description of important correlations at the ground state. Properties of elementary modes of excitation are strongly influenced by the symmetry breaking and can be studied with TDDFT. In particular, a number of recent developments in the linear response calculation have demonstrated their usefulness in description of collective modes of excitation in nuclei. Unrestricted real-time calculations have also become available in recent years, with new developments for quantitative description of nuclear collision phenomena. There are, however, limitations in the real-time approach; for instance, it cannot describe the many-body quantum tunneling. Thus, we treat the quantum fluctuations associated with slow collective motions assuming that time evolution of densities are determined by a few collective coordinates and momenta. The concept of collective submanifold is introduced in the phase space associated with the TDDFT and used to quantize the collective dynamics. Selected applications are presented to demonstrate the usefulness and quality of the new approaches. Finally, conceptual differences between nuclear and electronic TDDFT are discussed, with some recent applications to studies of electron dynamics in the linear response and under a strong laser field.
description: 57 pages, 15 figures, Review article
Non-thermal radiation from a pulsar wind interacting with an inhomogeneous stellar wind
Creators: name: de la Cita, Víctor M.
name: Bosch-Ramon, Valentí
name: Paredes-Fortuny, Xavier
name: Khangulyan, Dmitry
name: Perucho, Manel
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Binaries hosting a massive star and a non-accreting pulsar are powerful non-thermal emitters due to the interaction of the pulsar and the stellar wind. The winds of massive stars are thought to be inhomogeneous, which could have an impact on the non-thermal emission. We study numerically the impact of the presence of inhomogeneities or clumps in the stellar wind on the high-energy non-thermal radiation of high-mass binaries hosting a non-accreting pulsar. We compute the trajectories and physical properties of the streamlines in the shocked pulsar wind without clumps, with a small clump, and with a large one. This information is used to compute the synchrotron and inverse Compton emission from the non-thermal populations, accounting also for the effect of gamma-ray absorption through pair creation. A specific study is done for PSR B1259-63/LS2883. When stellar wind clumps perturb the two-wind interaction region, the associated non-thermal radiation in the X-ray band,of synchrotron origin, and in the GeV-TeV band, of inverse Compton origin, is affected by several effects: (i) strong changes in the the plasma velocity direction that result in Doppler boosting factor variations, (ii) strengthening of the magnetic field that mainly enhances the synchrotron radiation, (iii) strengthening of the pulsar wind kinetic energy dissipation at the shock, potentially available for particle acceleration, and (iv) changes in the rate of adiabatic losses that affect the lower energy part of the non-thermal particle population. The radiation above 100 GeV detected, presumably, during the post-periastron crossing of the Be star disc in PSR B1259-63/LS2883, can be roughly reproduced assuming that the crossing of the disc is modeled as the encounter with a large inhomogeneity.
description: 13 pages, 12 figures, submitted to A&A
REINFORCEMENT OF PROFESSIONAL LEARNING COMMUNITY PROCESS FOR PROFESSIONAL ETHICS DEVELOPMENT OF STUDENT TEACHERS BY INFORMATION TECHNOLOGY SYSTEM
Creators: name: Thidawan UNKONG
Publisher: name: PSAKU International Journal of Interdisciplinary Research
Year: 2023
Subjects: Professional Learning Community Development
Student Teacher Internship
Teacher Ethics

description: PSAKU International Journal of Interdisciplinary Research, 12, 1, 30-42
Aithal P. S. NEP 2020 SWAYAM PDP Certificate 2023
Creators: name: Aithal P., S.
Publisher: name: Zenodo
Year: 2023
Subjects: Certificate

description: PDP Certificate of NEP 2020 Training. Participated in and successfully completed the Professional Development Programme on ‘Implementation of NEP­2020 for University and College Teachers’ held from 12-­20, June, 2023 and obtained 'A+' Grade. INDIRA GANDHI NATIONAL OPEN UNIVERSITY, Staff Training and Research Institute of Distance Education New Delhi 110068 UGC­ Approved Short ­Term Professional Development Programme Under Pandit Madan Mohan Malaviya National Mission on Teachers and Teaching
การจัดการโลจิสติกส์และโซ่อุปทาน เพื่อสร้างความได้เปรียบทางการแข่งขันและ เพื่อผลการดำเนินงานของเกษตรกรสินค้าเกษตรใบเตยหอม
Creators: name: สุดารัตน์ พิมลรัตนกานต์
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: การจัดการโลจิสติกส์และโซ่อุปทาน
ความได้เปรียบทางการแข่งขัน
ผลการดำเนินงานของเกษตรกร

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 15-30
องค์ประกอบประสิทธิภาพโลจิสติกส์ของผู้ให้บริการโลจิสติกส์เดลิเวอรี่
Creators: name: ศรีศรินทร์ นรเศรษฐโสภณ
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: ประสิทธิภาพโลจิสติกส์
โลจิสติกส์เดลิเวอรี่
องค์ประกอบเชิงยืนยัน

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 31-48
BICEP3 performance overview and planned Keck Array upgrade
Creators: name: Grayson, J. A.
name: Ade, P. A. R.
name: Ahmed, Z.
name: Alexander, K. D.
name: Amiri, M.
name: Barkats, D.
name: Benton, S. J.
name: Bischoff, C. A.
name: Bock, J. J.
name: Boenish, H.
name: Bowens-Rubin, R.
name: Buder, I.
name: Bullock, E.
name: Buza, V.
name: Connors, J.
name: Filippini, J. P.
name: Fliescher, S.
name: Halpern, M.
name: Harrison, S.
name: Hilton, G. C.
name: Hristov, V. V.
name: Hui, H.
name: Irwin, K. D.
name: Kang, J.
name: Karkare, K. S.
name: Karpel, E.
name: Kefeli, S.
name: Kernasovskiy, S. A.
name: Kovac, J. M.
name: Kuo, C. L.
name: Leitch, E. M.
name: Lueker, M.
name: Megerian, K. G.
name: Monticue, V.
name: Namikawa, T.
name: Netterfield, C. B.
name: Nguyen, H. T.
name: O'Brient, R.
name: Ogburn, R. W.
name: Pryke, C.
name: Reintsema, C. D.
name: Richter, S.
name: Schwarz, R.
name: Sorensen, C.
name: Sheehy, C. D.
name: Staniszewski, Z. K.
name: Steinbach, B.
name: Teply, G. P.
name: Thompson, K. L.
name: Tolan, J. E.
name: Tucker, C.
name: Turner, A. D.
name: Vieregg, A. G.
name: Wandui, A.
name: Weber, A. C.
name: Wiebe, D. V.
name: Willmert, J.
name: Wu, W. L. K.
name: Yoon, K. W.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: BICEP3 is a 520 mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in BICEP2 and the Keck Array. The increased per-receiver optical throughput compared to BICEP2/Keck Array, due to both its faster f/1.7 optics and the larger aperture, more than doubles the combined mapping speed of the BICEP/Keck program. The BICEP3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, BICEP3-class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.
description: 17 pages, 6 figures. To be published in Proc. SPIE. Presented at SPIE Astronomical Telescopes and Instrumentation Conference 9914: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, June 2016
ปัจจัยที่มีอิทธิพลต่อความตั้งใจใช้บริการโรงแรม AI ของนักท่องเที่ยวชาวไทยตามลักษณะส่วนบุคคล
Creators: name: ฉัตยาพร เสมอใจ
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: ความตั้งใจใช้บริการ
โรงแรมAI
สถานการณ์ปกติใหม่
นักท่องเที่ยว

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 49-61
ปัจจัยที่ส่งผลต่อความภักดีในการซื้อเสื้อผ้าแฟชั่นผ่านการแพร่ภาพสด บนแอปพลิเคชัน Facebook ของผู้บริโภควัยทำงานในเขตกรุงเทพมหานคร
Creators: name: บุญญาพร ศรีประเสริฐ
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: ส่วนประสมทางการตลาดออนไลน์
ความภักดี
การแพร่ภาพสดบนแอปพลิเคชันFacebook

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 62-77
External US pressure on Japan's policy reform in the case of large-scale retail store law
Creators: name: Terada, Takashi
Publisher: name: Canberra, ACT : The Australian National University
Year: 1993
Subjects: subject: Japan. Large-Scale Retail Store Law
subject: Stores, Retail Japan
subject: Japan Commercial policy
subject: Japan Commerce United States
subject: United States Commerce Japan

description: The Structural Impediments Initiative (SII) talks held from September 1989 to July 1990 represented the first attempt by Japan and the United States to harmonise their domestic problems in international trade negotiations. These bilateral talks were also the first of their kind to delve into a comprehensive review of domestic laws and intrinsic business practices. In this sense, the SII talks may be seen as a preamble to mutual arrangements by domestic economies of their respective institutions and practices. This is likely to feature more prominently in the field of international relations, as seen recently in the European Community (EC) and the North American Free Trade Agreement (NAFTA). In this context, as the United States and Japan are the two largest and most technologically advanced economies in the world, accounting for more than 40 per cent of the world total gross national product, it is significant that they started harmonising their domestic rules through the SII talks, which are examined in this thesis.
อิทธิพลของทุนทางจิตวิทยาเชิงบวกและการมีใจบริการที่มีต่อคุณภาพ การบริการของผู้ให้บริการจัดส่งแบบส่งถึงที่ในจังหวัดเชียงราย
Creators: name: ปองสุข ศรีชัย
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: ทุนทางจิตวิทยาเชิงบวก
ใจบริการ
คุณภาพการบริการ
การจัดส่งแบบส่งถึงที่

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 78-92
Choose your own adventure: Mapping out interweaving plant stress response pathways
Creators: name: Tee, Estee
Publisher: name: The Australian National University
Year: 2020

description: The sessile nature of a plant has placed an evolutionary pressure on them to develop a highly sophisticated network of signals that encode perception, response and adaptation to a dynamic range of stressors. When a plant experiences drought stress, a number of molecular and physiological processes occur. This includes the production of the retrograde chloroplast-to-nucleus stress signal 3'phosphoadenosine 5'phosphate (PAP), which upregulates the transcription of stress-responsive genes. The initiation of reactive oxygen species (ROS) and stomatal closure signalling pathways occur in parallel. However, the functional role of chloroplasts and specifically PAP-mediated signalling has remained largely enigmatic as to their intersecting role of the two. Thus in my PhD, I tackled these three intertwining pathways that occur in response to stress: retrograde signalling, ROS signalling and stomatal closure signalling. I investigate how PAP affects ROS homeostasis, signalling thresholds, the 'biphasic ROS wave' and the resulting physiological consequences. Here I present evidence how ROS induces signalling cascades, as well as being part of the pathway that propagates signals. As an exemplar proof of concept, I use the guard cell model to show how PAP influences this network of information. Gatekeepers of gas exchange, guard cells mediate stomatal closure as a short-term physiological response that plants utilise to prevent water loss. I show that exogenous application of PAP leads to rapid stomatal closure to a similar extent as the guard cell regulatory hormone abscisic acid (ABA). Significantly, genetic analyses and biochemical manipulation experiments indicate that PAP signalling can supplement the canonical ABA-mediated signalling pathway in guard cells. PAP signalling in stomatal closure includes a dynamic interaction with secondary messengers (including ROS), ion flux induction, and the utilisation of chloroplastic mechanisms separate to ABA signalling. PAP signalling can act at least in part by up-regulating a number of novel calcium protein kinases. My thesis presents evidence of the chloroplast signal PAP having a function role as a molecular signal in response to stress. While we can measure outcomes of drought stress, the complexity of what happens for such responses to occur is an example of how the journey is just as important as the ending.
Development and application of an effective and robust flood inundation model
Creators: name: Teng, Jin
Publisher: name: The Australian National University
Year: 2020

description: Flood inundation models are the best available tools to study and predict flooding. They provide critical information for integrated water resources management. Most of the existing models simulate water movements by solving fluid dynamics equations and are data intensive and computationally costly. Effective and robust flood inundation modelling remains a significant and challenging research subject in hydrology and hydraulics, especially in applications that require inundation assessment for large floodplains, over a long time period, or require multiple simulations. This PhD research focused on the development and application of a simple conceptual flood inundation model that can be used for rapid and accurate assessment of inundation in large floodplains. The major contributions of this thesis are listed below. 1. The literature review provides guidance for selecting the most suitable method/model for solving practical flood related problems, taking into account the specific outputs required for the modelling purpose, the data available and computational demands. 2. The TVD (Teng-Vaze-Dutta) model uses high resolution DEM to derive floodplain storages and connectivity between them at different river stages. It has the advantage of low computational cost and can efficiently estimate the maximum or final flood extent in most conditions. Improvements to the model structure were made to overcome its inherent limitations by implementing mass conservation, reach connectivity and maintaining water balance on the floodplain. These new modules improved model accuracy in areas with hydrologically complex topography, without compromising the model efficiency. 3. The TVD model was coupled with the Australian Water Resource Assessment River System (AWRA-R) model, which is operational in the Australian Bureau of Meteorology for continental scale water accounting. Linking with the TVD model improved accounting for overbank flux and storage, recharge to the groundwater system, and substantially reduced the unaccounted volume. 4. An innovative Floodplain Ecological Response Model (FERM) was developed and coupled with the latest version of the TVD model to support holistic environmental water management. The coupled model provides flood dynamics and quantitative ecological responses and helps water managers to balance benefits and costs and considering environmental and social impacts; 5. Finally, future climate projections were explored so that they can be used as input to investigate climate change impacts on flooding. Two studies that will lead to the future research were carried out to evaluate datasets and assess method to produce climate projections.
พฤติกรรมนักท่องเที่ยวกลุ่ม Generation Z ในเขตกรุงเทพมหานครและปริมณฑล
Creators: name: สมรศรี คำตรง
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: พฤติกรรมนักท่องเที่ยว
กลุ่มเจเนอเรชั่นซี
กรุงเทพมหานครและปริมณฑล

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 93-107
On the origin of the near-infrared emission from the neutron-star low-mass X-ray binary GX 9+1
Creators: name: Berg, Maureen van den
name: Homan, Jeroen
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We have determined an improved position for the luminous persistent neutron-star low-mass X-ray binary and atoll source GX 9+1 from archival Chandra X-ray Observatory data. The new position significantly differs from a previously published Chandra position for this source. Based on the revised X-ray position we have identified a new near-infrared (NIR) counterpart to GX 9+1 in Ks-band images obtained with the PANIC and FourStar cameras on the Magellan Baade Telescope. NIR spectra of this Ks=16.5+-0.1 mag star taken with the FIRE spectrograph on the Baade Telescope show a strong Br-gamma emission line, which is a clear signature that we discovered the true NIR counterpart to GX 9+1. The mass donor in GX 9+1 cannot be a late-type giant, as such a star would be brighter than the estimated absolute Ks magnitude of the NIR counterpart. The slope of the dereddened NIR spectrum is poorly constrained due to uncertainties in the column density N_H and NIR extinction. Considering the source's distance and X-ray luminosity, we argue that N_H likely lies near the high end of the previously suggested range. If this is indeed the case, the NIR spectrum is consistent with thermal emission from a heated accretion disk, possibly with a contribution from the secondary. In this respect, GX 9+1 is similar to other bright atolls and the Z sources whose NIR spectra do not show the slope that is expected for a dominant contribution from optically thin synchrotron emission from the inner regions of a jet.
description: Accepted for publication in ApJ
ความสัมพันธ์ระหว่างคุณภาพการบริการกับความภักดีของผู้ใช้บริการ บริษัท สยามกลการอุตสาหกรรม จำกัด จังหวัดระยอง
Creators: name: จันทรา นามทอง
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: คุณภาพบริการ
ความสัมพันธ์
ความภักดี

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 108-121
Buckled Graphene for Efficient Energy Harvest, Storage, and Conversion
Creators: name: Jiang, Jin-Wu
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Buckling is one of the most common phenomena in atomic-thick layered structures like graphene. While the buckling phenomenon usually causes disaster for most nano-devices, we illustrate one positive application of the buckled graphene for energy harvest, storage, and conversion. More specifically, we perform molecular dynamical simulations to show that the buckled graphene can be used to collect the wasted mechanical energy and store the energy in the form of internal knotting potential. Through strain engineering, the knotting potential can be converted into useful kinetic (thermal) energy that is highly concentrated at the free edges of the buckled graphene. The present study demonstrates potential applications of the buckled graphene for converting the dispersed wasted mechanical energy into the concentrated useful kinetic (thermal) energy.
description: Nanotechnology, accepted
การบริหารงบประมาณของสถานศึกษา ในสังกัดองค์การบริหารส่วนจังหวัดนนทบุรี
Creators: name: จิดานันท์ สวนคล้าย
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: การบริหารงบประมาณ
องค์การบริหารส่วนจังหวัดนนทบุรี
ผู้บริหารสถานศึกษา

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 122-139
Anomaly indicators for time-reversal symmetric topological orders
Creators: name: Wang, Chenjie
name: Levin, Michael
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Some time-reversal symmetric topological orders are anomalous in that they cannot be realized in strictly two-dimensions without breaking time reversal symmetry; instead, they can only be realized on the surface of certain three-dimensional systems. We propose two quantities, which we call {\it anomaly indicators}, that can detect if a time-reversal symmetric topological order is anomalous in this sense. Both anomaly indicators are expressed in terms of the quantum dimensions, topological spins, and time-reversal properties of the anyons in the given topological order. The first indicator, $η_2$, applies to bosonic systems while the second indicator, $η_f$, applies to fermionic systems in the DIII class. We conjecture that $η_2$, together with a previously known indicator $η_1$, can detect the two known $\mathbb Z_2$ anomalies in the bosonic case, while $η_f$ can detect the $\mathbb Z_{16}$ anomaly in the fermionic case.
description: 11 pages
มุมมองต่อความหลากหลายของภาษาอังกฤษกับการใช้ภาษาอังกฤษในฐานะภาษากลาง ในบริบทปัจจุบันของไทย
Creators: name: แบร์ พิตต์พันธุ์
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: diversity of English
English as a lingua franca
current use of English in Thailand
English teaching and learning in Thailand

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 140-152
title: The Pontic lyra in contemporary Greece
Creators: name: Tsahourides, Matthaios
Publisher: name: Goldsmiths, University of London
Year: 2007

description: This thesis examines the performance techniques for playing the Politic lyra, a vertically-held bottle-shaped bowed lute which is the main instrument of the Poetic Greeks. The objectives of the research were to identify the ways in which the traditional performance techniques for the Lyra have been extended in the past, especially in the work of Gogos Petrides, and to explore the possibilities of extending these further in order to enable the lyra player to effectively perform styles and repertoires from outside Greece, with particular reference to the music of Afghanistan. A detailed discussion of changes in performance practices required the use of a broad range of contextualising material, enabling the author to position his work in the context of modern Greece. The thesis begins with a historical overview and provides background information about the culture and history of the Pontic settlements on the Black Sea coast of what is modern Turkey, up to the population exchanges of 1922. It provides a detailed organological study of the instrument and looks into its history, concluding it has a European/Byzantine rather than a Middle Eastern origin. The author also discusses the traditional and the contemporary performance techniques of the Pontic Lyra and describes his own experience as both performer and ethnographer during extended periods of fieldwork. The DVD and CD included in the thesis are of major importance as they provide a key role in demonstrating and illustrating the author's core research methods, findings and outcomes. The author's work was `mirrored' in an unassessed recital given at the end of the research. Chapter 1 provides a historical overview of the culture of the Pontic Greeks. Chapter 2 describes the morphology of the Pontic lyra and discusses its origins. Chapter 3 discusses the traditional and the contemporary performance techniques for the lyra; the author also describes his own learning experience within the context of a musical family. Chapter 4 considers three traditional genres of lyra music, the extended techniques attributed to Gogos Petrides, which have been further developed by the author. Chapter 5 recounts fieldwork carried out in Greece with six well-established Pontic musicians, who have much to say about the influence of Gogos Petrides. Chapter 6 explains how, through making a study of Afghan music as played on the dutar and rubab, the has adapted pre-existing and devised new techniques for playing the Afghan repertoire on the Pontic lyra. Chapter 7 summarises the research carried out, while an Appendix describes the preparations made for the recital which is part of the examination process. This thesis is accompanied by a CD and a DVD illustrating aspects of the research.
A JWST investigation of the evolution of the bar fraction at 1
Creators: name: Le Conte, Zoe
Publisher: name: Zenodo
Year: 2023
Subjects: Bar fraction
High redshift

description: Disc galaxies are thought to undergo two essential evolutionary phases: firstly, an unstable merging period, followed by internal secular evolution, thought to commence at z ≈ 1 and driven by the redistribution of angular momentum by a stellar bar. Therefore, the observed fraction of barred galaxies as a function of redshift provides crucial information on the onset and importance of secular evolution. However, it is well known that the fraction of bars in disc galaxies is underestimated by rest-frame optical and UV images because these wavelengths trace the younger stellar population. In contrast, stellar bars typically contain older stellar populations, which are more favourably imaged in the rest-frame near-infrared. The launch of JWST has provided us with the unique opportunity to study massive disc galaxies at higher redshifts with improved sensitivity and spatial resolution and at longer wavelengths than with HST. We will present a study of the bar fraction in the redshift range of 1 < z < 3 with imaging data from both JWST and HST. Stellar bars are significantly more apparent in the redder JWST NIRCam images than in the HST WFC3 images. Our results show that stellar bars exist already at z ≈ 2.5, which suggests that the secondary evolution phase could have begun only ≈ 2 Gyr after the Big Bang. Therefore, this calls for a review of our theories about when internal secular evolution began.
เทคนิคหลอกสมองให้เปลี่ยนตัวเองเป็นคนใหม่
Creators: name: วรสิริ ธรรมประดิษฐ์
Publisher: name: Southeast Bangkok University
Year: 2023
Subjects: สมอง;จิตวิทยา;การเปลี่ยนตัวเอง

description: วารสารวิชาการเซาธ์อีสท์บางกอก(สาขามนุษยศาสตร์และสังคมศาสตร์), 9, 1, 153-156
Sharygin triangles and elliptic curves
Creators: name: Netay, I. V.
name: Savvateev, A. V.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: The paper is devoted to the description of family of scalene triangles for which the triangle formed by the intersection points of bisectors with opposite sides is isosceles. We call them Sharygin triangles. It turns out that they are parametrized by an open subset of an elliptic curve. Also we prove that there are infinitely many non-similar integer Sharygin triangles.
description: 20 pages, 5 figures
Limits of applicability of the quasilinear approximation to the electrostatic wave-plasma interaction
Creators: name: Zacharegkas, Georgios
name: Isliker, Heinz
name: Vlahos, Loukas
Publisher: name: arXiv
Year: 2016
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The limitation of the Quasilinear Theory (QLT) to describe the diffusion of electrons and ions in velocity space when interacting with a spectrum of large amplitude electrostatic Langmuir, Upper and Lower hybrid waves, is analyzed. We analytically and numerically estimate the threshold for the amplitude of the waves above which the QLT breaks down, using a test particle code. The evolution of the velocity distribution, the velocity-space diffusion coefficients, the driven current, and the heating of the particles are investigated, for the interaction with small and large amplitude electrostatic waves, i.e. in both regimes, there where QLT is valid and there where it clearly breaks down.
description: 21 pages, 14 figures, accepted at Physics of Plasmas (2016)