cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Counter-streaming flows in a giant quiet-Sun filament observed in the extreme ultraviolet
Creators: name: Diercke, A.
name: Kuckein, C.
name: Verma, M.
name: Denker, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A giant solar filament was visible on the solar surface from 2011 Nov. 8-23. The filament stretched over more than half a solar diameter. Multiwavelength data from the SDO instrument AIA (171, 193, 304, and 211Å) were used to examine counter-streaming flows within the spine of the filament. H$α$ images from the Kanzelhöhe Solar Observatory provided context information. We apply local correlation tracking (LCT) to a two-hour time series on 2011 Nov. 16 of the AIA images to derive horizontal flow velocities of the filament. To enhance the contrast of the AIA images, noise adaptive fuzzy equalization is employed, which allows us to identify and quantify counter-streaming flows in the filament. We detect counter-streaming flows in the filament, which are visible in the time-lapse movies in all examined AIA wavelength bands. In the time-lapse movies we see that these persistent flows lasted for at least two hours. Furthermore, by applying LCT to the images we clearly determine counter-streaming flows in time series of 171 and 193Å images. In the 304Å wavelength band, we only see minor indications for counter-streaming flows with LCT, while in the 211Å wavelength band the counter-streaming flows are not detectable. The average horizontal flows reach mean flow speeds of 0.5 km/s. The highest horizontal flow speeds are identified in the 171Å band with flow speeds of up to 2.5 km/s. The results are averaged over a time series of 90 min. Because the LCT sampling window has finite width, a spatial degradation cannot be avoided leading to lower estimates of the flow velocities as compared to feature tracking or Doppler measurements. The counter-streaming flows cover about 15-20% of the whole area of the EUV filament channel and are located in the central part of the spine. In conclusion, we confirm the omnipresence of counter-streaming flows also in giant quiet-Sun filaments.
description: 11 pages, 8 figures, 1 online movie
Estimation of the Evolutionary Spectra with Application to Stationarity Test
Creators: name: Xiang, Yu
name: Ding, Jie
name: Tarokh, Vahid
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: In this work, we propose a new inference procedure for understanding non-stationary processes, under the framework of evolutionary spectra developed by Priestley. Among various frameworks of modeling non-stationary processes, the distinguishing feature of the evolutionary spectra is its focus on the physical meaning of frequency. The classical estimate of the evolutionary spectral density is based on a double-window technique consisting of a short-time Fourier transform and a smoothing. However, smoothing is known to suffer from the so-called bias leakage problem. By incorporating Thomson's multitaper method that was originally designed for stationary processes, we propose an improved estimate of the evolutionary spectral density, and analyze its bias/variance/resolution tradeoff. As an application of the new estimate, we further propose a non-parametric rank-based stationarity test, and provide various experimental studies.
description: To appear in IEEE Transactions on Signal Processing. A short version of this work appeared in ICASSP 2018
Radiative Symmetry Breaking and the Top Quark Mass in Local Supersymmetry
Creators: name: Leontaris, G. K.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Exact low energy expressions are derived for the top-squark and higgs masses, taking into account radiative contributions due to a heavy top quark. Their masses are expressed as analytic functions of $m_{1/2}$, $m_{3/2}$, $m_t$ and $sinβ$. Constraints from the radiative symmetry breaking mechanism are used then, to put lower bounds on the top-quark mass $m_t$. In particular, when $m_{3/2}\gg m_{1/2}$, we obtain the bound $m_t \ge 150sinβGeV$, while in the case of $m_{3/2}\equiv 0$, we obtain $m_t \ge 80sinβGeV$.
description: (Latex file, 8 pages, No figures) Ioannina preprint, July 1993, IOA.295/93
Blood Donation Practice And Associated Factors Among Health Care Professionals At Somali Sudanese Hospital,2024
Creators: name: Fa'izo, Hassan Salad
Publisher: name: Zenodo
Year: 2025
Subjects: Blood Donation
Practice And Associated
Factors Among Health Care
Professionals At
Somali Sudanese Hospital

description: Abstract

Blood donation is a critical aspect of healthcare, ensuring the availability of life-saving blood supplies for patients in need. However, the level of participation among healthcare professionals in blood donation remains a significant concern. This study examines blood donation practices and associated factors among healthcare professionals at Somali Sudanese Hospital in Mogadishu, Somalia. The research focuses on assessing healthcare professionals' knowledge, attitudes, and practices related to voluntary blood donation, as well as identifying barriers that affect their willingness to donate.

Using a cross-sectional study design, data was collected through structured questionnaires administered to healthcare professionals at the hospital. The findings indicate that while most healthcare professionals recognize the importance of blood donation, the actual practice remains low due to various barriers, including fear of anemia, lack of time, and limited access to donation facilities. Socio-demographic factors such as age, gender, and occupation also influence blood donation practices among healthcare workers.

The study underscores the need for targeted interventions to improve voluntary blood donation among healthcare professionals. Recommendations include implementing awareness campaigns, providing incentives for donors, and ensuring easy access to donation centers within healthcare institutions. These findings provide valuable insights for policymakers, hospital administrators, and public health officials
A new species and new distribution records of Zercon C. L. Koch from Iran (Acari: Zerconidae)
Creators: name: Mohammadreza Kavianpour
name: Karaca, Mehmet
name: Karimpour, Younes
name: Raşit Urhan
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: A new species of the family Zerconidae, Zercon persicus sp. n., is described based on female and male morphological characters. It was collected in West Azarbaijan province (northwestern Iran). Idiosomal chaetotaxy, poroidotaxy and related notations are illustrated. The similarities and differences between the related species within the genus are discussed. Records of some other Zercon species from the province are given for the first time. http://www.zoobank.org/urn:lsid:zoobank.org:pub:3D1122C7-2B86-40D2-974E-EE69035A2413
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0130
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0130, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
Entanglement Hamiltonian of Interacting Fermionic Models
Creators: name: Toldin, Francesco Parisen
name: Assaad, Fakher F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Recent numerical advances in the field of strongly correlated electron systems allow the calculation of the entanglement spectrum and entropies for interacting fermionic systems. An explicit determination of the entanglement (modular) Hamiltonian has proven to be a considerably more difficult problem, and only a few results are available. We introduce a technique to directly determine the entanglement Hamiltonian of interacting fermionic models by means of auxiliary field quantum Monte Carlo simulations. We implement our method on the one-dimensional Hubbard chain partitioned into two segments and on the Hubbard two-leg ladder partitioned into two chains. In both cases, we study the evolution of the entanglement Hamiltonian as a function of the physical temperature.
description: 9 pages, 5 figures including Supplemental Material; v2: new refs; v3: 10 pages, 5 figures including Supplemental Material, improved exposition, new refs; published version
Additional file 1: of Utilising network pharmacology to explore the underlying mechanism of Wumei Pill in treating pancreatic neoplasms
Creators: name: Wan, Yuxiang
name: Xu, Lin
name: Liu, Zeyu
name: Yang, Ming
name: Jiang, Xin
name: Zhang, Qiaoli
name: Huang, Jinchang
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Computational Biology

description: Table S1. Active ingredients and ADME parameters of Wumei Pill (DOCX 890 kb)
Micromaser line broadening without photon exchange
Creators: name: Henkel, Carsten
Publisher: name: arXiv
Year: 2007
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We perform a calculation of the linewidth of a micromaser, using the master equation and the quantum regression approach. A `dephasing' contribution is identified from pumping processes that conserve the photon number and do not appear in the photon statistics. We work out examples for a single-atom maser with a precisely controlled coupling and for a laser where the interaction time is broadly distributed. In the latter case, we also assess the convergence of a recently developed uniform Lindblad approximation to the master equation; it is relatively slow.
description: 8 pages, proceedings of Central European Workshop on Quantum Optics (Palermo Jun 07)
Indole-3-Acetic Acid induced oxidative stress in model host Galleria mellonella L. (Lepidoptera: Pyralidae) and its endoparasitoid Pimpla turionellae (L.) (Hymenoptera: Ichneumonidae)
Creators: name: Özyılmaz, D
name: Özbek, R
name: Altuntaş, H
name: Uçkan, F
Publisher: name: Invertebrate Survival Journal
Year: 2019

description: Investigation of the antioxidant and oxidative effects of dietary indole-3-acetic acid (IAA), a plant growth regulator, on pest Galleria mellonella L. (Lepidoptera: Pyralidae) and its endoparasitoid Pimpla turionellae (L.) (Hymenoptera: Ichneumonidae) was aimed in this study. Different doses of dietary IAA (50-10,000 ppm) caused an increase in lipid peroxidation in the hemolymph of the host, G. mellonella (L.) and its endoparasitoid P. turionellae (L.). When compared to the control, higher doses of dietary IAA decreased CAT, SOD and GST enzymes’ activities in G. mellonella. At higher IAA doses, the activity of SOD enzyme in the hemolymph of P. turionellae significantly decreased while CAT enzyme activity showed no significant change when compared to the control. Additionally, GST activity in the endoparasitoid larval hemolymph significantly increased at 500 and 1000 ppm IAA doses. These findings indicate that incorporating IAA in the diet of model host G. mellonella larvae leads to oxidative stress and, also negatively affects the survivability of both the host and its endoparasitoid.
description: Invertebrate Survival Journal, Vol 16 No 1 (2019)
Inference Duality as a Basis for Sensitivity Analysis
Creators: name: Hooker, John N.
Publisher: name: Carnegie Mellon University
Year: 1967
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: The constraint programming community has recently begun to address certain types of optimization problems. These problems tend to be discrete or to have discrete elements. Although sensitivity analysis is well developed for continuous problems, progress in this area for discrete problems has been limited. This paper proposes a general approach to sensitivity analysis that applies to both continuous and discrete problems. In the continuous case, particularly in linear programming, sensitivity analysis can be obtained by solving a dual problem. One way to broaden this result is to generalize the classical idea of a dual to that of an ldquoinference dual,rdquo which can be defined for any optimization problem. To solve the inference dual is to obtain a proof of the optimal value of the problem. Sensitivity analysis can be interpreted as an analysis of the role of each constraint in this proof. This paper shows that traditional sensitivity analysis for linear programming is a special case of this approach. It also illustrates how the approach can work out in a discrete problem by applying it to 0-1 linear programming (linear pseudo-boolean optimization).
Inefficiencies from Metropolitan Political and Fiscal Decentralization: Failures of Tiebout Competition
Creators: name: Calabrese, Stephen
name: Epple, Dennis
name: Romano, Richard
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: We examine theoretically and quantitatively the welfare effects of decentralized (Tiebout) provision of local public goods as compared to uniform centralized provision. We show that inefficiencies associated with property taxation offset the potential welfare gains from matching provision to preferences under decentralized provision. We identify an externality in community choice as the major source of inefficiency: Poorer households crowd the suburbs while avoiding taxes by consuming little housing. Our quantitative findings are based on a variety of estimates including an estimated model of the Boston Metropolitan Area.
Mechanical, optoelectronic and transport properties of single-layer Ca2N and Sr2N electrides
Creators: name: Mortazavi, Bohayra
name: Berdiyorov, Golibjon R
name: Shahrokhi, Masoud
name: Rabczuk, Timon
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Electride materials offer attractive physical properties due to their loosely bound electrons. Ca2N, an electride in the two-dimensional (2D) form was successfully recently synthesized. We conducted extensive first-principles calculations to explore the mechanical, electronic, optical and transport response of single-layer and free-standing Ca2N and Sr2N electrides to external strain. We show that Ca2N and Sr2N sheets present isotropic elastic properties with positive Poisson's ratios, however, they yield around 50% higher tensile strength along the zigzag direction as compared with armchair. We also showed that the strain has negligible effect on the conductivity of the materials; the current in the system reduces by less than 32% for the structure under ultimate uniaxial strain along the armchair direction. Compressive strain always increases the electronic transport in the systems due to stronger overlap of the atomic orbitals. Our results show that the optical spectra are anisotropic for light polarization parallel and perpendicular to the plane. Interband transition contributions along in-plane polarization are not negligible, by considering this effect the optical properties of Ca2N and Sr2N sheets in the low frequency regime significantly changed. The insight provided by this study can be useful for the future application of Ca2N and Sr2N in nanodevices.
description: arXiv admin note: text overlap with arXiv:1703.06786
Evidence for D0-D0bar mixing using the CDF II Detector
Creators: name: CDF Collaboration
name: Aaltonen, T.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We measure the time dependence of the ratio of decay rates for the rare decay D0->K+pi- to the Cabibbo-favored decay D0->K-pi+. We use a signal of 12.7 x10^3 D0->K+pi decays with proper decay times between 0.75 and 10 mean D0 lifetimes. The data sample was recorded with the CDF II detector at the Fermilab Tevatron and corresponds to an integrated luminosity of 1.5 fb-1 of p-pbar collisions at sqrt(s) = 1.96 TeV. We search for D0-D0bar mixing and measure the mixing parameters to be Rd = (3.04 +/- 0.55) x10^{-3}, y' = (8.5 +/- 7.6) x10^{-3}, and x'^2 = (-0.12 +/- 0.35) x10^{-3}. We report Bayesian probability contours in the x'^2-y' plane and find that the data are inconsistent with the no-mixing hypothesis with a probability equivalent to 3.8 Gaussian standard deviations.
description: 7 pages, 4 figures, submitted to Phys. Rev. Lett
The Hawking temperature of expanding cosmological black holes
Creators: name: Faraoni, Valerio
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In the context of a debate on the correct expression of the Hawking temperature of an expanding cosmological black hole, we show that the correct expression in terms of the Hawking-Hayward quasi-local energy m of the hole is T=1/(8πm(t)). This expression holds for comoving black holes and agrees with a recent proposal by Saida, Harada, and Maeda.
description: 5 latex pages, to appear in Phys. Rev. D. Some references added
Main conclusions of the self-assessment made in participant HEIs on gender equity in STEM fields
Creators: name: Harmoinen, S.
name: Heikkinen, M.
name: Pascual, J.
name: Mena, J. J.
Publisher: name: Zenodo
Year: 2019
Subjects: Women, Science, CBHE, EU, gender, STEM, W-STEM

description: Presentation of the main conclusions of the self-assessment at the W-STEM International Leadership Summit, held in Cartagena de Indias, Colombia on November 25-26th, 2019. This was made within the W-STEM ERASMUS + Capacity-building in Higher Education European Project (Ref. 598923-EPP-1-2018-1-ES-EPPKA2-CBHE-JP).
description: W-STEM (Building the future of Latin America: engaging women into STEM) is a project funded under European Union ERASMUS + Capacity-building in Higher Education Programme (598923-EPP-1-2018-1-ES-EPPKA2-CBHE-JP). The European Commission support for the production of this publication does not constitute an endorsement of the contents which reflects the views only of the authors, and the Commission cannot be held responsi­ble for any use which may be made of the information contained therein.
Higgscitement: Cosmological Dynamics of Fine Tuning
Creators: name: Amin, Mustafa A.
name: Fan, JiJi
name: Lozanov, Kaloian D.
name: Reece, Matthew
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Higgs potential appears to be fine-tuned, hence very sensitive to values of other scalar fields that couple to the Higgs. We show that this feature can lead to a new epoch in the early universe featuring violent dynamics coupling the Higgs to a scalar modulus. The oscillating modulus drives tachyonic Higgs particle production. We find a simple parametric understanding of when this process can lead to rapid modulus fragmentation, resulting in gravitational wave production. A nontrivial equation-of-state arising from the nonlinear dynamics also affects the time elapsed from inflation to the CMB, influencing fits of inflationary models. Supersymmetric theories automatically contain useful ingredients for this picture.
description: v2: 8 pages + 14 pages of appendices, 10 figures. Clarified and expanded discussion, more numerical simulations and evidence, references added. Accepted by Phys Rev D
Event shape criteria for single-lepton top signals
Creators: name: Barger, V.
name: Ohnemus, J.
name: Phillips, R. J. N.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Single-lepton plus jets signals from $t\bar t$ production at hadron colliders generally give more spherically symmetrical events than the principal backgrounds from $W$ production. We show that sphericity and aplanarity criteria, applied to lepton plus neutrino plus four jet final states at the Fermilab Tevatron $p\bar p$ collider, help to discriminate; they can be used either to validate an eventual top signal or simply to reduce background. An alternative circularity criterion in the transverse plane is less successful.
description: Standard Latex file, 8 pages. 3 figures, encoded using "uufiles", also submitted to hep-ph; uncompressed PS files or hardcopies available upon request. MAD/PH/777
Inducing Optimal Scheduling with Selfish Users
Creators: name: Enders, Paul
name: Anshul  Gandhi
name: Varun  Gupta
name: Debo, Laurens
name: Harchol-Balter, Mor
name: Wolf, Alan
Publisher: name: Carnegie Mellon University
Year: 2003
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: It is well known that scheduling jobs according to the Shortest-Remaining-Processing-Time (SRPT) policy is optimal for minimizing mean response time in a single-server system with online arrivals. Unfortunately, SRPT scheduling requires users to reveal their job size (service requirement), which is not always realistic. This may be because some users are informed, but selfish (or rational): they know their job size but are willing to lie about it if that is to their advantage. Alternatively, users may be uninformed { they may genuinely not know their size. Complicating matters further, the system administrator may not be able to differentiate between users of these two types. This adds significant complications to the management of such systems, as threats that are credible to force informed users to reveal their size may be unfair to uninformed users. This situation is common in supercomputing environments, for example. To cope with such a situation we develop a novel approach for inducing the informed users into self- scheduling themselves according to (an approximation of) SRPT while not, unfairly, penalizing the uninformed users.We achieve this by defining a game that users play, applying priority-boosting tokens to portions of their job. For the informed users, we characterize the features of a unique equilibrium self-scheduling policy. We prove that the equilibrium policy is a dominant strategy, i.e. no user has any incentive to follow any other strategy, regardless of other users' behavior. We show that the optimal strategy of uninformed users is highly complex and may lead to multiple, potentially unstable, equilibria. Then, via queueing-theoretic analysis, we evaluate the effectiveness of our game as a function of job size variability, load, and other system parameters. We find that our game results in a near approximation of SRPT scheduling for informed users when the appropriate number of tokens (which we can determine) is distributed.
(Re-)Konstruktion der Lübecker Aegyptiaca – Didaktische Perspektiven auf gegenständliche Quellen in der Ägyptologie
Creators: name: Wagenknecht, Nina
Publisher: name: Zenodo
Year: 2021
Subjects: Egyptology
aegyptiaca
digitalisation
objects
museum communication

description: Im Rahmen des Dissertationsvorhabens wird ein Online-Vermittlungskonzept für die nicht physisch ausgestellten Aegyptiaca der Völkerkundesammlung der Lübecker Museen erarbeitet. Die methodischen Schritte der Analyse teilen sich in Identifizierung von Ausstellungsthema und Zielgruppe, die fachwissenschaftliche Sachanalyse und die didaktische Analyse der thematisch ausgewählten Objekte. Diese Form der Aufbereitung vermittelt die Objekte als historische Zeugnisse zur „Konstruktion“ von Geschichte.
Supergravity Coupled to Chiral Matter at One Loop
Creators: name: Gaillard, \Mary K.
name: Jain, Vidyut
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extend earlier calculations of the one-loop contributions to the effective bose Lagrangian in supergravity coupled to chiral matter. We evaluate all logarithmically divergent contributions for arbitrary background scalar fields and space-time metric. We show that, with a judicious choice of gauge fixing and of the definition of the action expansion, much of the result can be absorbed into a redefinition of the metric and a renormalization of the Kähler potential. Most of the remaining terms depend on the curvature of the Kähler metric. Further simplification occurs in models obtained from superstrings in which the Kähler Riemann tensor is covariantly constant.
description: 33 pages, LBL-34457, UCB-PTH-93-22
Individualizing Pay Allocations Under Secret and Open Pay Systems
Creators: name: Goodman, Paul S.
name: Friedman, Abraham
Publisher: name: Carnegie Mellon University
Year: 2012
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: Although wages and salaries represent a substantial cost of doing business, there are surprisingly few studies concerning how managers make wage and salary decisions. This research is designed to increase our understanding of the salary allocation decision and it should have both theoretical and practical implications.
Docker Image and Source Code of MISH
Creators: name: Cao, Clinton
name: Panichella, Annibale
name: Verwer, Sicco
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 461201
subject: Automated software engineering
classificationCode: 461208
subject: Software testing, verification and validation

description: This page contains the Docker image that you can use to run MISH on EvoMaster. All dependencies are already installed. We also included a ZIP of the MISH's source code. Importing image in DockerPlease import the docker image by first going to the location of "mish.tar" and then executing the following command:cat mish.tar | docker import - mish/mish load --input mish.tar (see https://docs.docker.com/reference/cli/docker/image/import/)Starting the Docker imageThen start the docker image using the following command:docker run -it mish/mish:latest /bin/bashOnce the container has been started navigate to /home/EvoMaster/.Running MISH and EvoMasterYou can now run MISH by executing the following command:./mish/scripts/run_experiment.sh MISH BUDGET with_500_faults APPLICATIONReplace BUDGET with the desired search budget and replace APPLICATION with the app you would like to run. Note that the search budget is defined in minutes! Names of applications are all in small letters. If you would like to run OCVN, then you would need to use "ocvn-rest" as the name. Please note that OCVN starts a docker container. In theory, it should be okay to start a docker container in docker but we have not tested this option! Furthermore, we have not installed Docker in the docker image.As an example, we show how to run MISH on CatWatch for 60 minutes:./mish/scripts/run_experiment.sh MISH 60 with_500_faults_test catwatchViewing the Source CodeThere are two options for how one can view and inspect MISH's source code:The first option is to attach VS Code to the running docker container of MISH (see https://code.visualstudio.com/docs/devcontainers/attach-container)The second option is to download the included ZIP file (EvoMaster.zip) and extract all the files. Once the files have been extracted, the source code can be viewed and inspected using an IDE (e.g., IntelliJ)
Pulsar Searches with the SKA
Creators: name: Levin, L.
name: Armour, W.
name: Baffa, C.
name: Barr, E.
name: Cooper, S.
name: Eatough, R.
name: Ensor, A.
name: Giani, E.
name: Karastergiou, A.
name: Karuppusamy, R.
name: Keith, M.
name: Kramer, M.
name: Lyon, R.
name: Mackintosh, M.
name: Mickaliger, M.
name: van Nieuwpoort, R
name: Pearson, M.
name: Prabu, T.
name: Roy, J.
name: Sinnen, O.
name: Spitler, L.
name: Spreeuw, H.
name: Stappers, B. W.
name: van Straten, W.
name: Williams, C.
name: Wang, H.
name: Wiesner, K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Square Kilometre Array will be an amazing instrument for pulsar astronomy. While the full SKA will be sensitive enough to detect all pulsars in the Galaxy visible from Earth, already with SKA1, pulsar searches will discover enough pulsars to increase the currently known population by a factor of four, no doubt including a range of amazing unknown sources. Real time processing is needed to deal with the 60 PB of pulsar search data collected per day, using a signal processing pipeline required to perform more than 10 POps. Here we present the suggested design of the pulsar search engine for the SKA and discuss challenges and solutions to the pulsar search venture.
description: 4 pages, 1 figure. To be published in Proceedings of IAU Symposium 337: Pulsar Astrophysics - The Next 50 Years
Increasing the Efficiency and Effectiveness of Environmental Decisions: Benefit-Cost Analysis and Effluent Fees A Critical Review
Creators: name: Lave, Lester B
name: Gruenspecht, Howard
Publisher: name: Carnegie Mellon University
Year: 1973
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: The objective of this critical review is to evaluate and summarize the literature on economic tools used to improve environmental decision making. Environmental decisions are complicated by pervasive uncertainty, and the lack of consensus on goals and on tradeoffs, such as air versus water pollution and versus loss of coal mining jobs. Five decision frameworks are used by regulatory agencies to simplify decision making. Congress’ choice of a decision framework designates the amount of data and analysis that will be required and the range and depth of social values that must be considered. Economic incentives have worked well for phasing out lead in gasoline, for increasing recycling and for reducing the volume of municipal solid waste. Congress has mandated incentives for acid rain and CFCs, and several countries have implemented carbon taxes to abate greenhouse gas emissions. Economic tools have become more central to the analysis and implementation of environmental policies; their role should continue to increase. We conclude that economic tools are extremely valuable, although their application is difficult.
Thermal D-brane boundary states from type IIB Green-Schwarz superstring in pp-wave background
Creators: name: Vancea, Ion V.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct the thermal boundary states from the type IIB Green-Schwarz superstring in {\em pp}-wave background in the light-cone gauge. The superstring is treated in the canonical ensemble and in the TFD formalism which is appropriate to discuss quantum systems in the canonical quantization. The thermal boundary states are obtained by thermalizing the total boundary states which are the boundary states of the total system that is composed by the superstring modes and the corresponding thermal reservoir modes. That analysis is similar to the one in the flat spacetime case \cite{ivv12}. However, there are some subtleties concerning the construction of the total string which are discussed. Next, we compute the entropy of thermal boundary state which is defined as the expectation value of the superstring entropy operator in the thermal boundary state.
description: References added. Minor typos corrected. 24 pages, LATeX file
Spontaneous CP violation in the Supersymmetric Higgs Sector
Creators: name: Babu, K. S.
name: Barr, S. M.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Spontaneous CP--violation in the minimal supersymmetric standard model with a gauge singlet and a cubic superpotential is examined. Although the tree--level Higgs potential conserves CP, it is shown that with the inclusion of the one--loop top--quark radiative effects, CP may be broken spontaneously. The CP--violating minimum requires two neutral $(h_1,h_2)$ and one charged $(H^\pm)$ Higgs--bosons to be relatively light with $m_{h_1}+m_{h_2} \stackrel{_
description: 14 pages (Plain LaTeX, 2 figures availbale on request), BA-93-42
Inconsistent Behavior in Lottery Choice Experiments
Creators: name: F. T. Dolbear
name: Lave, Lester B.
Publisher: name: Carnegie Mellon University
Year: 1965
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: College students made choices in binary lottery situations involving small amounts of money-payoffs ranged from $2.50 to -$1.00. Each of 52 subjects made 150 choices. Any of a number of choice models might be used to describe the outcome of such an experiment. However, no simple model (based on expected utility maximization) is capable of explaining all choices (of a particular subject)-there are always some inconsistent choices. The experiment was designed to isolate factors affecting inconsistency. Such research is aimed at improving the predictive ability of choice models by reducing the stochastic error. A choice model based on expected utility maximization was developed. The model was designed to maximize the internal consistency of each subject's choices. In all cases, some choices were found to be inconsistent with the model. Grouping the data in various ways, four factors hypothesized to affect inconsistency were tested: difference in dispersion of the payoffs, signs of the payoffs, order of the choice situation, and small changes in wealth. Applying classical statistical techniques, inconsistency was found to be related to the first three of these factors. Some implications of these results for expected utility models of choice are presented.
The $H_0$ Tension in Non-flat QCDM Cosmology
Creators: name: Miao, Haitao
name: Huang, Zhiqi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences
subject: J.2
subject: 83F05

description: The recent local measurement of Hubble constant leads to a more than $3σ$ tension with Planck + $Λ$CDM (Riess {\it et al} 2018). In this article we study the $H_0$ tension in non-flat QCDM cosmology, where Q stands for a minimally coupled and slowly-or-moderately rolling quintessence field $ϕ$ with a smooth potential $V(ϕ)$. By generalizing the QCDM one-parameter and three-parameter parametrizations in Huang {\it et al} 2011 to non-flat universe and using the latest cosmological data, we find that the $H_0$ tension remains above $3.2σ$ level for this class of model.
description: 8 pages, 6 figures
Docker Image and Source Code of MISH
Creators: name: Cao, Clinton
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 461201
subject: Automated software engineering
classificationCode: 461208
subject: Software testing, verification and validation

description: This page contains the Docker image that you can use to run MISH on EvoMaster. All dependencies are already installed. We also included a ZIP of the MISH's source code. Importing image in DockerPlease import the docker image by first going to the location of "mish.tar" and then executing the following command:cat mish.tar | docker import - mish/mish load --input mish.tar (see https://docs.docker.com/reference/cli/docker/image/import/)Starting the Docker imageThen start the docker image using the following command:docker run -it mish/mish:latest /bin/bashOnce the container has been started navigate to /home/EvoMaster/.Running MISH and EvoMasterYou can now run MISH by executing the following command:./mish/scripts/run_experiment.sh MISH BUDGET with_500_faults APPLICATIONReplace BUDGET with the desired search budget and replace APPLICATION with the app you would like to run. Note that the search budget is defined in minutes! Names of applications are all in small letters. If you would like to run OCVN, then you would need to use "ocvn-rest" as the name. Please note that OCVN starts a docker container. In theory, it should be okay to start a docker container in docker but we have not tested this option! Furthermore, we have not installed Docker in the docker image.As an example, we show how to run MISH on CatWatch for 60 minutes:./mish/scripts/run_experiment.sh MISH 60 with_500_faults_test catwatchViewing the Source CodeThere are two options for how one can view and inspect MISH's source code:The first option is to attach VS Code to the running docker container of MISH (see https://code.visualstudio.com/docs/devcontainers/attach-container)The second option is to download the included ZIP file (EvoMaster.zip) and extract all the files. Once the files have been extracted, the source code can be viewed and inspected using an IDE (e.g., IntelliJ)
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 439
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 439, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 439, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Chasing Lambda
Creators: name: Kurek, Aleksandra
name: Szydlowski, Marek
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent astronomical observations of SNIa, CMB, as well as BAO in the Sloan Digital Sky Survey, suggest that the current Universe has entered a stage of an accelerated expansion with the transition redshift at $z \simeq 0.5$. While the simplest candidates to explain this fact is cosmological constant/vacuum energy, there exists a serious problem of coincidence. In theoretical cosmology we can find many possible approaches alleviating this problem by applying new physics or other conception of dark energy. We consider state of art candidates for the description of accelerating Universe in the framework of the Bayesian model selection. We point out advantages as well as troubles of this approach. We find that the combination of four data bases gives a stringent posterior probability of the $Λ$CDM model which is 74%. This fact is a quantitative exemplification of a turmoil in modern cosmology over the $Λ$ problem.
description: Talk presented at the "A Century of Cosmology - Past, Present and Future" conference, S.Servolo(Venice), Italy, August 27-31 2007. To be published in Il Nuovo Cimento
Vertices for Iwahori-Hecke algebras and the Dipper-Du conjecture
Creators: name: Whitley, James R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 20C30 (Primary), 20C08, 16G99 (Secondary)

description: Let $\mathscr{H}_n$ denote the Iwahori-Hecke algebra corresponding to the symmetric group $\mathfrak{S}_n$. We set up a Green correspondence for bimodules of these Hecke algebras, and a Brauer correspondence between their blocks. We examine Specht modules for $\mathscr{H}_n$ and compute the vertices of certain Specht modules, before using this to give a classification of the vertices of blocks of $\mathscr{H}_n$ in any characteristic. Finally, we apply this classification to resolve the Dipper-Du conjecture about the structure of vertices of indecomposable $\mathscr{H}_n$-modules.
description: 31 pages, v2 Minor corrections and corrected statement of Theorem 5.9
Detection of an intergalactic meteor particle with the 6-m telescope
Creators: name: Afanasiev, V. L.
name: Kalenichenko, V. V.
name: Karachentsev, I. D.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: On July 28, 2006 the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences recorded the spectrum of a faint meteor. We confidently identify the lines of FeI and MgI, OI, NI and molecular-nitrogen N_2 bands. The entry velocity of the meteor body into the Earth's atmosphere estimated from radial velocity is equal to 300 km/s. The body was several tens of a millimeter in size, like chondrules in carbon chondrites. The radiant of the meteor trajectory coincides with the sky position of the apex of the motion of the Solar system toward the centroid of the Local Group of galaxies. Observations of faint sporadic meteors with FAVOR TV CCD camera confirmed the radiant at a higher than 96% confidence level. We conclude that this meteor particle is likely to be of extragalactic origin. The following important questions remain open: (1) How metal-rich dust particles came to be in the extragalactic space? (2) Why are the sizes of extragalactic particles larger by two orders of magnitude (and their masses greater by six orders of magnitude) than common interstellar dust grains in our Galaxy? (3) If extragalactic dust surrounds galaxies in the form of dust (or gas-and-dust) aureoles, can such formations now be observed using other observational techniques (IR observations aboard Spitzer satellite, etc.)? (4) If inhomogeneous extragalactic dust medium with the parameters mentioned above actually exists, does it show up in the form of irregularities on the cosmic microwave background (WMAP etc.)?
description: 9 pages, 6 EPS figures
Equilibrium chemistry down to 100 K - Impact of silicates and phyllosilicates on carbon/oxygen ratio
Creators: name: Woitke, P.
name: Helling, Ch.
name: Hunter, G. H.
name: Millard, J. D.
name: Turner, G. E.
name: Worters, M.
name: Blecic, J.
name: Stock, J. W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We introduce a fast and versatile computer code, GGchem, to determine the chemical composition of gases in thermo-chemical equilibrium down to 100 K, with or without equilibrium condensation. We review the data for molecular equilibrium constants, kp(T), from several sources and discuss which functional fits are most suitable for low temperatures. We benchmark our results against another chemical equilibrium code. We collect Gibbs free energies, dG(T), for about 200 solid and liquid species from the NIST-JANAF database and the geophysical database SUPCRTBL. We discuss the condensation sequence of the elements with solar abundances in phase equilibrium down to 100 K. Once the major magnesium silicates Mg2SiO4[s] and MgSiO3[s] have formed, the dust/gas mass ratio jumps to a value of about 0.0045 which is significantly lower than the often assumed value of 0.01. Silicate condensation is found to increase the carbon/oxygen ratio (C/O) in the gas from its solar value of ~0.55 up to ~0.71, and, by the additional intake of water and hydroxyl into the solid matrix, the formation of phyllosilicates at temperatures below ~400 K increases the gaseous C/O further to about 0.83. Metallic tungsten (W) is the first condensate found to become thermodynamically stable around 1600 - 2200 K (depending on pressure), several hundreds of Kelvin before subsequent materials like zirconium dioxide (ZrO2) or corundum (Al2O3) can condense. We briefly discuss whether tungsten, despite its low abundance of ~2.E-7 times the silicon abundance, could provide the first seed particles for astrophysical dust formation. The GGchem code is publicly available at https://github.com/pw31/GGchem.
description: accepted by A&A, 18 pages plus 16 pages appendix, 16 figures, and 5 long tables
Improving the Management of Environmental Health
Creators: name: Lave, Lester B.
Publisher: name: Carnegie Mellon University
Year: 1971
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: Environmental health regulation has been developed on the premise that both problems and solutions are obvious, requiring only attention and commitment. The result has been impossible legislative goals and frenetic, unfocused agency efforts to deal with too many issues. Preventing all environmental health problems is impossible and not the best approach; instead, attention ought to be shifted toward reacting quickly to problems before irreversible, severe health damage has occurred. Rather than having regulatory agencies attempt to manage all problems, they should be focused on exemplifying goals and productive approaches, and on handling a few major issues. Regulatory agencies should be managing the nonregulatory institutions to ensure that they are effective in dealing with the myriad issues that the agencies will never be able to handle. The inherent limitations of federal regulatory agencies must be recognized to restructure environmental health management to be more effective in lowering risks while being efficient, administratively simple, and more equitable.