cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The flow and evolution of ice-sucrose crystal mushes
Creators: name: Gilbert, Andrew
name: Oppong, Felix
name: Farr, Robert
Publisher: name: arXiv
Year: 2016
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We study the rheology of suspensions of ice crystals at moderate to high volume fractions in a sucrose solution in which they are partially soluble; a model system for a wide class of crystal mushes or slurries. Under step changes in shear rate, the viscosity changes to a new `relaxed' value over several minutes, in a manner well fitted by a single exponential. The behavior of the relaxed viscosity is power-law shear thinning with shear rate, with an exponent of $-1.76 \pm 0.25$, so that shear stress falls with increasing shear rate. On longer timescales, the crystals ripen (leading to a falling viscosity) so that the mean radius increases with time to the power $0.14 \pm 0.07$. We speculate that this unusually small exponent is due to the interaction of classical ripening dynamics with abrasion or breakup under flow. We compare the rheological behavior to mechanistic models based on flow-induced aggregation and breakup of crystal clusters, finding that the exponents can be predicted from liquid phase sintering and breakup by brittle fracture.
description: 15 pages, 16 figures
Role of nuclear physics in oscillations of magnetars
Creators: name: Nandi, Rana
name: Char, Prasanta
name: Chatterjee, Debarati
name: Bandyopadhyay, Debades
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Strong magnetic fields have important effects on the crustal properties of magnetars. Here we study the magneto-elastic oscillations of magnetars taking into consideration the effect of strong magnetic fields on the crustal composition (magnetised crust). We calculate global magneto-elastic (GME) modes as well as modes confined to the crust (CME) only. The composition of the crust directly affects its shear modulus which we calculate using three different nucleon-nucleon interactions: SLy4, SkM and Sk272. The shear modulus of the crust is found to be enhanced in strong magnetic fields $\geq 10^{17}$ G for all those Skyrme interactions. It is noted that the shear modulus of the crust for the SLy4 interaction is much higher than those of the SkM and Sk272 interactions in presence of magnetic fields or not. Though we do not find any appreciable change in frequencies of fundamental GME and CME modes with and without magnetised crusts, frequencies of first overtones of CME modes are significantly affected in strong magnetic fields $\geq 10^{17}$ G. However, this feature is not observed in frequencies of first overtones of GME modes. As in earlier studies, it is also noted that the effects of crusts on frequencies of both types of maneto-elastic modes disappear when the magnetic field reaches the critical field ($B > 4 \times 10^{15}$ G). Frequencies of GME and CME modes calculated with magnetised crusts based on all three nucleon-nucleon interactions, stellar models and magnetic fields, are compared with frequencies of observed quasi-periodic oscillations (QPOS) in SGR 1806-20 and SGR1900+14. As in earlier studies, this comparison indicates that GME modes are essential to explain all the frequencies as CME modes can explain only the higher frequencies.
description: 28 pages, 8 figures, accepted for publication in PRC. arXiv admin note: substantial text overlap with arXiv:1207.3247
A nonlinear structural subgrid-scale closure for compressible MHD Part II: a priori comparison on turbulence simulation data
Creators: name: Grete, P.
name: Vlaykov, D. G.
name: Schmidt, W.
name: Schleicher, D. R. G.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Computational Physics (physics.comp-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Even though compressible plasma turbulence is encountered in many astrophysical phenomena, its effect is often not well understood. Furthermore, direct numerical simulations are typically not able to reach the extreme parameters of these processes. For this reason, large-eddy simulations (LES), which only simulate large and intermediate scales directly, are employed. The smallest, unresolved scales and the interactions between small and large scales are introduced by means of a subgrid-scale (SGS) model. We propose and verify a new set of nonlinear SGS closures for future application as an SGS model in LES of compressible magnetohydrodynamics (MHD). We use 15 simulations (without explicit SGS model) of forced, isotropic, homogeneous turbulence with varying sonic Mach number $\mathrm{M_s} = 0.2$ to $20$ as reference data for the most extensive \textit{a priori} tests performed so far in literature. In these tests we explicitly filter the reference data and compare the performance of the new closures against the most widely tested closures. These include eddy-viscosity and scale-similarity type closures with different normalizations. Performance indicators are correlations with the turbulent energy and cross-helicty flux, the average SGS dissipation, the topological structure and the ability to reproduce the correct magnitude and direction of the SGS vectors. We find that only the new nonlinear closures exhibit consistently high correlations (median value \textgreater$0.8$) with the data over the entire parameter space and outperform the other closures in all tests. Moreover, we show that these results are independent of resolution and chosen filter scale. Additionally, the new closures are effectively coefficient-free with a deviation of less than $20\%$.
description: 17 pages, 10 figures, 2 tables; to be published in Physics of Plasmas
Off-centred dark matter halo leading to strong central disc lopsidedness
Creators: name: Prasad, Chaitanya
name: Jog, Chanda J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: There is increasing evidence now from simulations and observations that the centre of dark matter halo in a Milky Way type galaxy could be off-centred by a few 100 pc w.r.t. the galactic disc. We study the effect of such an offset halo on the orbits and kinematics in the central few kpc of the disc. The equations of motion in the disc plane can be written in terms of the disc and halo potentials when these two are concentric and a perturbation term due to the offset halo. This perturbation potential shows an m=1 azimuthal variation, or is lopsided, and its magnitude increases at small radii. On solving these equations, we find that the perturbed orbit shows a large deviation of ~ 40 % in radius at R = 1.5 kpc, and also strong kinematical lopsidedness. Thus even a small halo offset of 350 pc can induce surprisingly strong spatial and kinematical lopsidedness in the central region within ~ 3 kpc radius. Further, the disc would remain lopsided for several Gyr, as long as the halo offset lasts. This would have important implications for the dynamical evolution of this region.
description: 6 pages, 6 figures, Submitted to MNRAS
Partial autocorrelation parameterization for subset autoregression
Creators: name: McLeod, A. Ian
name: Zhang, Ying
Publisher: name: arXiv
Year: 2016
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62M10, 91B84

description: A new version of the partial autocorrelation plot and a new family of subset autoregressive models are introduced. A comprehensive approach to model identification, estimation and diagnostic checking is developed for these models. These models are better suited to efficient model building of high-order autoregressions with long time series. Several illustrative examples are given.
description: 28 pages, 3 figures, 3 tables
A bound on the averaged spectral shift function and a lower bound on the density of states for random Schrödinger operators on $\mathbb{R}^d$
Creators: name: Dietlein, Adrian
name: Gebert, Martin
name: Hislop, Peter D.
name: Klein, Abel
name: Müller, Peter
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We obtain a bound on the expectation of the spectral shift function for alloy-type random Schrödinger operators on $\mathbb{R}^d$ in the region of localisation, corresponding to a change from Dirichlet to Neumann boundary conditions along the boundary of a finite volume. The bound scales with the area of the surface where the boundary conditions are changed. As an application of our bound on the spectral shift function, we prove a reverse Wegner inequality for finite-volume Schrödinger operators in the region of localisation with a constant locally uniform in the energy. The application requires that the single-site distribution of the independent and identically distributed random variables has a Lebesgue density that is also bounded away from zero. The reverse Wegner inequality implies a strictly positive, locally uniform lower bound on the density of states for these continuum random Schrödinger operators.
Host Galaxy Dispersion Measure of Fast Radio Burst
Creators: name: Wang, Xinxin
name: Yu, Ye-Zhao
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Fast radio bursts are a class of transient radio sources that are thought to originate from extragalactic sources since their dispersion measure greatly exceeds the highest dispersion measure that the Milky Way interstellar medium can provide. Host Galaxies of twenty-two fast radio bursts have already been identified. In this paper, the dispersion measurement of these fast radio bursts produced by the Milky Way interstellar medium, and the intergalactic medium is obtained through known physical models to yield the host galaxy dispersion measure. It is observed that the host galaxy dispersion measure increases with its redshift value. We also obtained that the host galaxy dispersion measure has different distribution between repeaters and non-repeaters. It is noted that the reason for the divergence of the host galaxy dispersion measures should be accounted for by the difference in their local environment.
description: 11 pages, 5 figures, accepted for publication in American Research Journal of Physics
KAM for beating solutions of the quintic NLS
Creators: name: Haus, Emanuele
name: Procesi, Michela
Publisher: name: arXiv
Year: 2016
Subjects: subject: Analysis of PDEs (math.AP)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 37K55

description: We consider the nonlinear Schrödinger equation of degree five on the circle $\mathbb{S}^1 = \mathbb{R}/2π$. We prove the existence of quasi-periodic solutions which bifurcate from "resonant" solutions (studied in [14]) of the system obtained by truncating the Hamiltonian after one step of Birkhoff normal form, exhibiting recurrent exchange of energy between some Fourier modes. The existence of these quasi-periodic solutions is a purely nonlinear effect.
description: 32 pages, 1 figure
X-ray and Rotational Luminosity Correlation and Magnetic Heating of the Radio Pulsars
Creators: name: Shibata, S.
name: Watanabe, E.
name: Yatsu, Y.
name: Enoto, T.
name: Bamba, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Previous works have suggested a correlation between the X-ray luminosity Lx and the rotational luminosity Lrot of the radio pulsars.However, none of the obtained regression lines are statistically acceptable due to large scatters. We construct a statistical model which has an intrinsic Lx-Lrot relation and reproduces the observed Lx distribution about it by using a Monte Carlo simulator, which takes into account the effects obscuring the intrinsic relation,i.e., the anisotropy of radiation, additional heating, uncertainty in distance and detection limit of the instruments. From the ATNF pulsar catalog we collect 57 `ordinary radio pulsars' with significant detection and 42 with upper limits.The sample does not include the high-magnetic field pulsars (>10^{13} G), which are separately analyzed. We obtain a statistically acceptable relation Lx (0.5 - 10 keV)= 10^{31.69} (Lrot / L_0)^{c_1} with c_1 = 1.03 \pm 0.27 and L_0 =10^{35.38}. The distribution about the obtained Lx-Lrot relation is reproduced well by the simulator. Pulsars with abnormally high Lx fall into two types: one is the soft gamma-ray pulsars, and the other is thermally bright pulsars in comparison with the standard cooling curve. On the other hand, pulsars showing low Lx are found to have dim pulsar wind nebulae. We argue that there is an unknown mechanism that governs both the magnetospheric emission and the pulsar wind nebulae, and it might involve the production rate of electron-positron pairs. The high-field pulsars form a distinctive population other than the ordinary pulsars due to their excess luminosities.
description: 17 pages, 11 figures, to be published in ApJ
Co-Salient Object Detection with Semantic-Level Consensus Extraction and Dispersion
Creators: name: Xu, Peiran
name: Mu, Yadong
Publisher: name: arXiv
Year: 2023
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Given a group of images, co-salient object detection (CoSOD) aims to highlight the common salient object in each image. There are two factors closely related to the success of this task, namely consensus extraction, and the dispersion of consensus to each image. Most previous works represent the group consensus using local features, while we instead utilize a hierarchical Transformer module for extracting semantic-level consensus. Therefore, it can obtain a more comprehensive representation of the common object category, and exclude interference from other objects that share local similarities with the target object. In addition, we propose a Transformer-based dispersion module that takes into account the variation of the co-salient object in different scenes. It distributes the consensus to the image feature maps in an image-specific way while making full use of interactions within the group. These two modules are integrated with a ViT encoder and an FPN-like decoder to form an end-to-end trainable network, without additional branch and auxiliary loss. The proposed method is evaluated on three commonly used CoSOD datasets and achieves state-of-the-art performance.
description: Accepted by ACM MM 2023
TYC 8241 2652 1 and the case of the disappearing disk: no smoking gun yet
Creators: name: Günther, Hans Moritz
name: Kraus, Stefan
name: Melis, Carl
name: Curé, Michel
name: Harries, Tim
name: Ireland, Michael
name: Kanaan, Samer
name: Poppenhaeger, Katja
name: Rizzuto, Aaron
name: Rodriguez, David
name: Schneider, Christian P.
name: Sitko, Michael
name: Weigelt, Gerd
name: Willson, Matthew
name: Wolk, Scott
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: TYC 8241 2652 1 is a young star that showed a strong mid-infrared (mid-IR, 8-25 mu) excess in all observations before 2008 consistent with a dusty disk. Between 2008 and 2010 the mid-IR luminosity of this system dropped dramatically by at least a factor of 30 suggesting a loss of dust mass of an order of magnitude or more. We aim to constrain possible models including removal of disk material by stellar activity processes, the presence of a binary companion, or other explanations suggested in the literature. We present new X-ray observations, optical spectroscopy, near-IR interferometry, and mid-IR photometry of this system to constrain its parameters and further explore the cause of the dust mass loss. In X-rays TYC 8241 2652 1 has all properties expected from a young star: Its luminosity is in the saturation regime and the abundance pattern shows enhancement of O/Fe. The photospheric Ha line is filled with a weak emission feature, indicating chromospheric activity consistent with the observed level of coronal emission. Interferometry does not detect a companion and sets upper limits on the companion mass of 0.2, 0.35, 0.1 and 0.05 M_sun at projected physical separations of 0.1-4 AU,4-5 AU, 5-10 AU, and 10-30 AU, respectively (assuming a distance of 120.9 pc). Our mid-IR measurements, the first of the system since 2012, are consistent with the depleted dust level seen after 2009. The new data confirms that stellar activity is unlikely to destroy the dust in the disk and shows that scenarios where either TYC 8241 2652 1 heats the disk of a binary companion or a potential companion heats the disk of TYC 8241 2652 1 are unlikely.
description: accepted by A&A
Controls and Interfaces
Creators: name: King, Q.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Reliable powering of accelerator magnets requires reliable power converters and controls, able to meet the powering specifications in the long term. In this paper, some of the issues that will challenge a power converter controls engineer are discussed.
description: 16 pages, contribution to the 2014 CAS - CERN Accelerator School: Power Converters, Baden, Switzerland, 7-14 May 2014
An Incentive-Compatible Scheme for Electricity Cooperatives: An Axiomatic Approach
Creators: name: Ehsanfar, Abbas
name: Heydari, Babak
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computer Science and Game Theory (cs.GT)
subject: Systems and Control (eess.SY)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper introduces a new scheme for autonomous electricity cooperatives, called predictive cooperative (PCP), which aggregates commercial and residential electricity consumers and participates in the electricity market on behalf of its members. An axiomatic approach is proposed to calculate the day-ahead bid and to disaggregate the collective cost among participating consumers. The resulting formulation is shown to keep the members incentivized to both participate in the cooperative and remain truthful in reporting their expected loads. The scheme is implemented using PJM (world's largest wholesale electricity market) real-time and day-ahead price data for 2015 and a collection of residential and commercial load profiles. The model performance of this framework is compared to that of real-time pricing (RTP) scheme, in which wholesale market prices are directly applied to individual consumers. The results show truthful load announcement by consumers, reduction in electricity price variation for all consumers, and comparative benefits for participants.
description: 9 pages
Big Data Caching for Networking: Moving from Cloud to Edge
Creators: name: Zeydan, Engin
name: Baştuğ, Ejder
name: Bennis, Mehdi
name: Kader, Manhal Abdel
name: Karatepe, Alper
name: Er, Ahmet Salih
name: Debbah, Mérouane
Publisher: name: arXiv
Year: 2016
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: In order to cope with the relentless data tsunami in $5G$ wireless networks, current approaches such as acquiring new spectrum, deploying more base stations (BSs) and increasing nodes in mobile packet core networks are becoming ineffective in terms of scalability, cost and flexibility. In this regard, context-aware $5$G networks with edge/cloud computing and exploitation of \emph{big data} analytics can yield significant gains to mobile operators. In this article, proactive content caching in $5$G wireless networks is investigated in which a big data-enabled architecture is proposed. In this practical architecture, vast amount of data is harnessed for content popularity estimation and strategic contents are cached at the BSs to achieve higher users' satisfaction and backhaul offloading. To validate the proposed solution, we consider a real-world case study where several hours of mobile data traffic is collected from a major telecom operator in Turkey and a big data-enabled analysis is carried out leveraging tools from machine learning. Based on the available information and storage capacity, numerical studies show that several gains are achieved both in terms of users' satisfaction and backhaul offloading. For example, in the case of $16$ BSs with $30\%$ of content ratings and $13$ Gbyte of storage size ($78\%$ of total library size), proactive caching yields $100\%$ of users' satisfaction and offloads $98\%$ of the backhaul.
description: accepted for publication in IEEE Communications Magazine, Special Issue on Communications, Caching, and Computing for Content-Centric Mobile Networks
Experimental Status of Supersymmetry after the LHC Run-I
Creators: name: Autermann, Christian
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The ATLAS and CMS experiments at the Large Hadron Collider (LHC) at CERN have searched for signals of new physics, in particular for supersymmetry. The data collected until 2012 at center-of-mass energies of 7 and 8 TeV and integrated luminosities of 5 fb^-1 and 20 fb^-1, respectively, agree with the expectation from standard model processes. Constraints on supersymmetry have been calculated and interpreted in different models. Limits on supersymmetry particle masses at the TeV scale have been derived and interpreted generally in the context of simplified model spectra. The constrained minimal supersymmetric standard model is disfavored by the experimental results. Natural supersymmetry scenarios with low supersymmetry particle masses remain possible in multiple regions, for example in those with compressed spectra, that are difficult to access experimentally. The upgraded LHC operating at 13 TeV is gaining sensitivity to the remaining unexplored SUSY parameter space.
Power Converters for Accelerators
Creators: name: Visintini, R.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Particle accelerators use a great variety of power converters for energizing their sub-systems; while the total number of power converters usually depends on the size of the accelerator or combination of accelerators (including the experimental setup), the characteristics of power converters depend on their loads and on the particle physics requirements: this paper aims to provide an overview of the magnet power converters in use in several facilities worldwide.
description: 30 pages, contribution to the 2014 CAS - CERN Accelerator School: Power Converters, Baden, Switzerland, 7-14 May 2014
Exploiting Depth from Single Monocular Images for Object Detection and Semantic Segmentation
Creators: name: Cao, Yuanzhouhan
name: Shen, Chunhua
name: Shen, Heng Tao
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Augmenting RGB data with measured depth has been shown to improve the performance of a range of tasks in computer vision including object detection and semantic segmentation. Although depth sensors such as the Microsoft Kinect have facilitated easy acquisition of such depth information, the vast majority of images used in vision tasks do not contain depth information. In this paper, we show that augmenting RGB images with estimated depth can also improve the accuracy of both object detection and semantic segmentation. Specifically, we first exploit the recent success of depth estimation from monocular images and learn a deep depth estimation model. Then we learn deep depth features from the estimated depth and combine with RGB features for object detection and semantic segmentation. Additionally, we propose an RGB-D semantic segmentation method which applies a multi-task training scheme: semantic label prediction and depth value regression. We test our methods on several datasets and demonstrate that incorporating information from estimated depth improves the performance of object detection and semantic segmentation remarkably.
description: 14 pages. Accepted to IEEE T. Image Processing
Astro-COLIBRI: An Advanced Platform for Real-Time Multi-Messenger Astrophysics
Creators: name: Schüssler, Fabian
name: de Lavergne, Mathieu de Bony
name: Alkan, Atilla Kaan
name: Mourier, Jayson
name: Reichherzer, Patrick
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Observations of transient phenomena like Gamma-Ray Bursts (GRBs), Fast Radio Bursts (FRBs), stellar flares and explosions (novae and supernovae), combined with the detection of novel cosmic messengers like high-energy neutrinos and gravitational waves has revolutionized astrophysics over the last years. The discovery potential of both ulti-messenger and multi-wavelength follow-up observations as well as serendipitous observations could be maximized with a novel tool which allows for quickly acquiring an overview over relevant information associated with each new detection. Here we present Astro-COLIBRI, a novel and comprehensive platform for this challenge. Astro-COLIBRI's architecture comprises a public RESTful API, real-time databases, a cloud-based alert system and a website as well as apps for iOS and Android as clients for users. Astro-COLIBRI evaluates incoming messages of astronomical observations from all available alert streams in real time, filters them by user specified criteria and puts them into their MWL and MM context. The clients provide a graphical representation with an easy to grasp summary of the relevant data to allow for the fast identification of interesting phenomena, provides an assessment of observing conditions at a large selection of observatories around the world, and much more. Here the key features of Astro-COLIBRI are presented. We outline the architecture, summarize the used data resources, and provide examples for applications and use cases. Focussing on the high-energy domain, we'll discuss the use of the platform in searches for high-energy gamma-ray counterparts to high-energy neutrinos, gamma-ray bursts and gravitational waves.
description: Proceedings 38th International Cosmic Ray Conference (ICRC2023)
Quantum frequency conversion and strong coupling of photonic modes using four-wave mixing in integrated microresonators
Creators: name: Vernon, Z.
name: Liscidini, M.
name: Sipe, J. E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Single photon-level quantum frequency conversion has recently been demonstrated using silicon nitride microring resonators. The resonance enhancement offered by such systems enables high-efficiency translation of quantum states of light across wide frequency ranges at sub-watt pump powers. Using a quantum-mechanical Hamiltonian formalism, we present a detailed theoretical analysis of the conversion dynamics in these systems, and show that they are capable of converting single- and multi-photon quantum states. Analytic formulas for the conversion efficiency, spectral conversion probability density, and pump power requirements are derived which are in good agreement with previous theoretical and experimental results. We show that with only modest improvement to the state of the art, efficiencies exceeding 95% are achievable using less than 100 mW of pump power. At the critical driving strength that yields maximum conversion efficiency, the spectral conversion probability density is shown to exhibit a flat-topped peak, indicating a range of insensitivity to the spectrum of a single photon input. Two alternate theoretical approaches are presented to study the conversion dynamics: a dressed mode approach that yields a better intuitive picture of the conversion process, and a study of the temporal dynamics of the participating modes in the resonator, which uncovers a regime of Rabi-like coherent oscillations of single photons between two different frequency modes. This oscillatory regime arises from the strong coupling of distinct frequency modes mediated by coherent pumps.
description: 14 pages, 7 figures
Putting it into Practice
Creators: name: Burnet, J-P
Publisher: name: arXiv
Year: 2016
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: This paper presents the latest trends in the powering of particle accelerators. A series of solutions is proposed for responding to the challenges of high performance machines. This paper covers the domains of magnetic field uncertainty, power converter control, and energy saving. This list is not exhaustive, but it does correspond to the latest innovations in the field of powering particle accelerators.
description: 13 pages, contribution to the 2014 CAS - CERN Accelerator School: Power Converters, Baden, Switzerland, 7-14 May 2014
Growth and Characterization of Iron Scandium Sulfide (FeSc2S4)
Creators: name: Morey, Jennifer R.
name: Plumb, Kemp W.
name: Pasco, Chris M.
name: McQueen, Tyrel M.
name: Koohpayeh, Seyed M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Here we report successful growth of mm scale single crystals of stoichiometric FeSc2S4. Single crystal X-ray diffraction yields a cubic structure, spacegroup Fd-3m, with a=10.5097(2) angstroms at T=110(2) K consistent with previous literature on polycrystallin samples. Models fit to the data reveal no detectable antisite mixing or deviations from the ideal stoichiometry. Heat capacity and dc magnetization measurements on the single crystals match those of high quality powder specimens. The novel traveling solvent growth method presented in this work opens the door to studies requiring sizable single crystals of the candidate spin-orbital liquid FeSc2S4.
description: Journal of Crystal Growth (2016)
Exponential parameterization of neutrino mixing matrix with account for CP-violation data
Creators: name: Zhukovsky, K.
name: Murilio, F. M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The exponential parameterization of Pontecorvo-Maki-Nakagawa-Sakata mixing matrix for neutrino is discussed. The exponential form allows easy factorization and separate analysis of the CP-violating and Majorana terms. Based upon the recent experimental data on the neutrino mixing, the values for the exponential parameterization matrix for neutrinos are determined. The matrix entries for the pure rotational part in charge of the mixing without CP-violation are derived. The complementarity hypothesis for quarks and neutrinos is demonstrated. The comparison of the results, based on most recent and on old data is held. The CP-violating parameter value is estimated, based on the so far imprecise experimental indications, regarding CP-violation for neutrinos. The unitarity of the exponential parameterisation and the CP-violating term transform is confirmed. The transform of the neutrino mass state vector by the exponential matrix with account for CP-violation is shown.
Photohadronic scenario in interpreting the February-March 2014 flare of 1ES 1011+496
Creators: name: Sahu, Sarira
name: de León, Alberto Rosales
name: Miranda, Luis Salvador
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The extraordinary multi-TeV flare from 1ES 1011 +496 during February-March 2014 was observed by MAGIC telescopes for 17 nights and the average spectrum of the whole period has a non-trivial shape. We have used the photohadronic model and a template EBL model to explain the average spectrum which fits well to the flare data. The spectral index $α$ is the only free parameter in our model. We have also shown that the non-trivial nature of the spectrum is due to the change in the behavior of the optical depth above $\sim 600$ GeV $γ$-ray energy accompanied with the high SSC flux.
description: 11 pages, 3 figures, LaTeX
Requirements for Power Converters
Creators: name: Burnet, J. -P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: This paper introduces the requirements for power converters needed for particle accelerators. It describes the role of power converters and the challenges and constraints when powering magnets. The different circuit layouts are presented as well as the operating cycles. The power converter control and high precision definition are also introduced. This paper lists the key circuit parameters to be taken into consideration to properly specify a power converter that can be compiled in a functional specification.
description: 14 pages, contribution to the 2014 CAS - CERN Accelerator School: Power Converters, Baden, Switzerland, 7-14 May 2014
Trois Quintetti pour deux Violons, deux Altos et Basse
Creators: name: Wranitzky, Paul
Publisher: name: Imbault
Year: 1790

description: Stimmen: Viol. I & II, Viola I & II, Bass
description: Nr. I: B-Dur ; Nr. II: D-Dur ; Nr. III: G-Dur
description: [Bd.] 1 Livre de Quintetti
description: composés par Paul Wranizki
description: Auch bei J. André : Offenbach erschienen [1792, mit Pl.-Nr. 450], dort als Oeuvre 18, Livre 1 bezeichnet
description: Alter Umschlag mit handschriftl. Incipits
Aria à 9  con più Stromenti : "Scherza il nocchier tal ora"
Scherza il nocchier talora
Creators: name: Wagenseil, Georg Christoph
name: Metastasio, Pietro
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Sopran [Alceste] (canto) + Bassinstrument ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola (viola) ; Bassinstrument (basso) ; Oboe I (oboe primo) ; Oboe II (oboe secondo) ; Horn I (corno primo) ; Horn II (corno secondo)
description: Del Signore Wagenseil ; [Text von Pietro Metastasio]
description: Aus der Oper "Demetrio"
description: Der Name auf der Singstimme bezieht sich auf der Sopran-Kastrat Giovanni Manzuoli, der bei den Aufführungen in Mailand 1760 mitgewirkt hat
description: Italienisch
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Aria à 8 Con più Stromentÿ : Aria : "Dal Suo gentil Sembiante"
Dal suo gentil sembiante
Creators: name: Wagenseil, Georg Christoph
name: Metastasio, Pietro
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Sopran [Alceste] (canto) + Bassinstrument ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola (viola) ; Bassinstrument (basso) ; Fagott oder Violoncello (fagotto, o sia violoncello obligato) ; Horn I (corno primo) ; Horn I (im Altschlüssel notiert) (corno primo in alto viola) ; Horn II (corno secondo) ; Horn II (im Altschlüssel notiert) (corno secondo in alto viola)
description: Del Signore Wagenseil ; [Text von Pietro Metastasio]
description: Aus der Oper "Demetrio"
description: Der Name auf der Singstimme bezieht sich auf der Sopran-Kastrat Giovanni Manzuoli, der bei den Aufführungen in Mailand 1760 mitgewirkt hat
description: Italienisch
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Aria à 5 (in Discante) Con piu Stromenty : "Non sò frenare il pianto"
Non sò frenare il pianto
Creators: name: Wagenseil, Georg Christoph
name: Metastasio, Pietro
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Sopran [Alceste] (canto) + Bassinstrument ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola (viola) ; Bassinstrument (basso)
description: Del Signore Wagenseil ; [Text von Pietro Metastasio]
description: Aus der Oper "Demetrio"
description: Der Name auf der Singstimme bezieht sich auf der Sopran-Kastrat Giovanni Manzuoli, der bei den Aufführungen in Mailand 1760 mitgewirkt hat
description: Italienisch
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Aria à 9 (in Discante) Con più Stromentÿ : Aria : "Quel labro adorato"
Quel labro adorato
Creators: name: Wagenseil, Georg Christoph
name: Metastasio, Pietro
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Sopran [Alceste] (canto) + Bassinstrument ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola (viola) ; Bassinstrument (basso) ; Flöte I (flutta prima) ; Flöte II (flutta seconda) ; Horn I (corno primo) ; Horn I (im Altschlüssel notiert) (corno primo in alto viola) ; Horn II (corno secondo) ; Horn II (im Altschlüssel notiert) (corno secondo in alto viola)
description: del Signore Wagenseil ; [Text von Pietro Metastasio]
description: Aus der Oper "Demetrio"
description: Der Name auf der Singstimme bezieht sich auf den Sopran-Kastraten Giovanni Manzuoli, der bei den Aufführungen in Mailand 1760 mitgewirkt hat
description: Italienisch
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Six Quatuors pour deux Violons, Alto et Basse : Œuvre 16
Creators: name: Wranitzky, Paul
Publisher: name: [Imbault]
Year: 2023

description: Stimmen: Viol. I & II, Viola, Bass
description: Vorhanden: 2. Partie. Nr. IV: F-Dur ; Nr. V: c-moll ; Nr. VI: D-Dur
description: composés par Paul Wranizki
description: Verlagsangabe fehlt auf Titelblatt; stattdessen Vertriebsangabe "Chez tous les Marchands de Musique"
description: Alter Umschlag mit handschriftl. Incipits
Sinphonia Concertanti à 12 [B-Dur]
Sinfonia Concertante à 10 Stromenti
Sinfonie concertante
Creators: name: Stamitz, Carl
Publisher: name: [s.n.]
Year: 1760

description: Stimmen:Violine principale I (violino principale primo) ; Violine principale II (violino principale secondo) ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola I + II (due viola prima & seconda) ; Violoncello (violoncello/violon) + Kontrabass (contra basso) ; Bassinstrument [=Cello] (basso) (2 Ex.) ; Flöte I (flauto primo) ; Flöte II (flauto secondo) ; Solotrompete (clarino solo in b) ; Horn I (corno primo in dis) ; Horn II (corno secondo in dis) ; Umschlag
description: Del Signore Carlo Stammitz
description: Verschieden von UBH kr XII 30 und UBH kr XII 58
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Six Simphonies à grand Orghestre
Creators: name: Vaňhal, Jan Křtitel
name: Rosetti, Antonio
name: Sterkel, Johann Franz Xaver
name: Haydn, Joseph
name: Touchemoulin, Joseph
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo) ; Viola I (alto viola prima) ; Viola II (alto viola seconda) (nur in den Sinfonien 2, 5 und 6) ; Bassinstrument (basso) ; Flöte I (flauto primo) ; Flöte II (flauto secondo) ; Horn I (corno primo) ; Horn II (corno secondo)
description: Del Signore Wanhall
description: Nr. 4 ist 1947 im Druck erschienen, hg. v. F. Kneusslin. Standort: UBH kk XVII 3066
description: Nr. 6 ist 1933 in der Edition Bernoulli im Druck erschienen. Standort: UBH kk XVII 189
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Trio [G-Dur] : Per il Violino, [Flauto ove Oboe & Basso]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine (violino) ; Flöte oder Oboe (flaute travers ô oboè) ; Bassinstrument (basso)
description: Del Signore [?]
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Concerto à 6 [D-Dur]
Concerto à Più Istrumenti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine principale (violino principale) ; Violine I (violino primo obligato) ; Violine II (violino secondo obligato) ; Viola (viola obligato) ; Bassinstrument (basso obligato) ; Orgel oder Bassinstrument ripieno (organo o vero basso di ripieno)
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Duetto à Flauto Trauersiera Prima & Seconda [G-Dur]
Sonata à Due Trauersiere Soli
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Flöte I (traversiera prima) ; Flöte II (trauersiera seconda)
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Trio à Violino Primo, Secondo & Basso [B-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo) ; Bassinstrument (basso)
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Trio à flauto Traverso Prima, Seconda et Basso [B-Dur]
Sonata à Due Trauersiera è Basso
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Flöte I (trauersiera prima) ; Flöte II (trauersiera seconda) ; Bassinstrument (basso)
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
Concerto à 5 [A-Dur] : Violino principale, Violino Primo, Violino Secondo, Viola, Basso
Creators: name: Reichenauer, Johann Anton
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine principale (violino principale) ; Violine I (violino primo) ; Violine II (violino secondo) ; Viola (viola) ; Bassinstrument (basso)
description: [Johann Anton Reichenauer?]
description: Anfang und Schluss jedes Satzes entsprechen genau dem Johann Anton Reichenauer zugeschriebenen Konzert in G-Dur aus der Dresdner Hofkapelle (Sächsische Landesbibliothek - Staats- und Universitätsbibliothek, Mus.2494-O-3), nicht aber die Mittelteile
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
[20 kurze Tanzstücke]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo) ; Bassinstrument (basso)
description: 16 nummerierte und 4 nicht nummerierte Stücke
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl
Duetto [C-Dur] : a due Violini ô Flauti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Flöte I oder Violine I (flauto ove violino primo) ; Flöte II oder Violine II (secondo)
description: Verzeichnung=Description=Inventaire März 2023 HAN-Katalogisierungsregeln jpl
[Konzert? in C-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo d'accompagnamento) ; Violine II (violino secondo d'accompagnamento) ; Viola I (alto viola prima) ; Viola II (alto viola seconda) ; Bassinstrument (basso) ; Oboe I (oboe primo) ; Oboe II (oboe secondo) ; Horn I (corno primo in C) ; Horn II (corno secondo in C)
description: Ein Satz eines unbekannten Werkes. Möglicherweise fehlen Stimmen für ein oder mehrere Soloinstrumente.
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl
Duetto [C-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo)
description: Besitzvermerk: Pierre Vischer de Bâle
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl
Concerto à 6 [Es-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine principale I (violino principale primo) ; Violine principale II (violino principale secondo) ; Violine I (violino primo obligato) ; Violine II (violino secondo obligato) ; Viola (viola obligata) ; Violoncello (violoncello obligato)
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl
Unterlagen zu den Protokollen der Sitzungen des Verwaltungsrats VI
Creators: name: Hero
Publisher: name: [s.n.]
Year: 1973

description: Enthält: Breda - Culina Fünfjahresplan, Ideenskizze zu einer Kapitalerhöhung, Technische Investitionsbudgets, Orientierung über das Geschäftsjahr, Mittelfristiger Finanzplan der Herogruppe etc.
description: Darin: Verzeichnis
description: Deutsch
Duetto [F-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo)
description: Besitzvermerk: Pierre Vischer
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl
Duetto [As-Dur]
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1760

description: Stimmen: Violine I (violino primo) ; Violine II (violino secondo)
description: Besitzvermerk: Pierre Vischer
description: Verzeichnung=Description=Inventaire April 2023 HAN-Katalogisierungsregeln jpl