cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of A fluorescence-based high-throughput screening method for cytokinin translocation mutants
Creators: name: Mengyuan Zhang
name: Bingli Ding
name: Jiangzhe Zhao
name: Penghong Zhang
name: Yujia Li
name: Guodong Yang
name: Zhang, Kewei
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Construction of ARR5::eGFP reporter vector. The promoter of Arabidopsis RR5 was cloned and constructed into the plant expression vector (RCS2) to drive free GFP expressing. The map was prepared by SnapGene
Data from: Cranial anatomy of the mekosuchine crocodylian Trilophosuchus rackhami Willis, 1993
Creators: name: Ristevski, Jorgo
name: Weisbecker, Vera
name: Scanlon, John D.
name: Price, Gilbert J.
name: Salisbury, Steven W.
Publisher: name: Zenodo
Year: 2022
Subjects: Trilophosuchus
Mekosuchinae
Crocodylia
Mekosuchini
Longirostres

description: One of the best-preserved crocodylian fossil specimens from the Cenozoic of Australia is the holotype of the mekosuchine Trilophosuchus rackhami, from the middle Miocene (13.56 ± 0.67 Ma) Ringtail Site at Riversleigh, northwestern Queensland. Although lacking most of the snout, the holotype skull of T. rackhami (QMF16856) has an exceptionally well-preserved cranium. Micro-CT scanning of the holotype has allowed for all the preserved cranial bones to be digitally disarticulated, facilitating an unprecedented insight into the cranial anatomy of not just T. rackhami, but any mekosuchine. Trilophosuchus rackhami was a small-bodied crocodylian and one of the most morphologically distinct mekosuchines, characterized by a unique combination of cranial characteristics several of which are exclusive to the species. Fossil material that is definitively referrable to the species T. rackhami is currently known solely from the middle Miocene Ringtail Site. However, an isolated parietal from Hiatus Site at Riversleigh demonstrates that Trilophosuchus also occurred during the late Oligocene (~25 Ma), extending the range of the genus by more than ten million years. The new description of T. rackhami also allowed for a reevaluation of its phylogenetic relationships. Our results reaffirm the placement of T. rackhami as a member of Mekosuchinae within the subclade Mekosuchini. In all analyses, Mekosuchinae was consistently found to be monophyletic and part of the larger crocodylian clade Longirostres. However, the assignment of Mekosuchinae as a subset of Crocodylidae is brought into question, suggesting that the status of Mekosuchinae as a subfamily should be reconsidered.
Optical pumping and relaxation of atomic population in assorted conditions
Creators: name: Pradhan, Swarupananda
name: Chowdhury, Saptarshi Roy
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: The precise control and knowledge over the atomic dynamics is central to the advancement of quantum technology. The different experimental conditions namely, atoms in a vacuum, an anti-relaxation coated and a buffer gas filled atomic cell provides complementary platform for such investigations. The extent of changes in optical pumping, velocity changing collision and hyperfine changing collision rates associated with these conditions are discussed. There is a phenomenal change in the optical density by a factor of >25 times in presence of a control field in buffer gas environment. In contrary to earlier reports, we found confinement induced enhanced optical pumping as the mechanism behind the observed transparency in buffer gas cell. The feeble interplay of radiation trapping under specific conditions are pointed out. The diffusive velocity of atoms is measured to be ~25+-12 m/s and <= 8+-4 m/s for anti-relaxation coated and buffer gas filled cell respectively. The studies will have useful application in measurements of relaxation rates, quantum memory, quantum repeaters and atomic devices.
description: 9 pages, 8 Figures
A Spectral Analysis of the Nonlinear Schroedinger Equation in the Co-Exploding Frame
Creators: name: Chapman, S. J.
name: Kavousanakis, M. E.
name: Charalampidis, E. G.
name: Kevrekidis, I. G.
name: Kevrekidis, P. G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: The nonlinear Schroedinger model is a prototypical dispersive wave equation that features finite time blowup, either for supercritical exponents (for fixed dimension) or for supercritical dimensions (for fixed nonlinearity exponent). Upon identifying the self-similar solutions in the so-called "co-exploding frame", a dynamical systems analysis of their stability is natural, yet is complicated by the mixed Hamiltonian-dissipative character of the relevant frame. In the present work, we study the spectral picture of the relevant linearized problem. We examine the point spectrum of 3 eigenvalue pairs associated with translation, $U(1)$ and conformal invariances, as well as the continuous spectrum. We find that two eigenvalues become positive, yet are attributed to symmetries and are thus not associated with instabilities. In addition to a vanishing eigenvalue, 3 more are found to be negative and real, while the continuous spectrum is nearly vertical and on the left-half (spectral) plane. Finally, the subtle effects of the boundaries are also assessed and their role in the observed weak eigenvalue oscillations is clarified.
A Critical Assessment of Solutions to the Galaxy Diversity Problem
Creators: name: Zentner, Aidan
name: Dandavate, Siddharth
name: Slone, Oren
name: Lisanti, Mariangela
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Galactic rotation curves exhibit a diverse range of inner slopes. Observational data indicates that explaining this diversity may require a mechanism that correlates a galaxy's surface brightness with the central-most region of its dark matter halo. In this work, we compare several concrete models that capture the relevant physics required to explain the galaxy diversity problem. We focus specifically on a Self-Interacting Dark Matter (SIDM) model with an isothermal core and two Cold Dark Matter (CDM) models with/without baryonic feedback. In contrast to the CDM case, the SIDM model can lead to the formation of an isothermal core in the halo, and is also mostly insensitive to baryonic feedback processes, which act on longer time-scales. Using rotation curves from 90 galaxies in the Spitzer Photometry and Accurate Rotation Curves (SPARC) catalog, we perform a comprehensive model comparison that addresses issues of statistical methodology from prior works. The best-fit halo models that we recover are consistent with standard CDM concentration-mass and abundance matching relations. We find that both the SIDM and feedback-affected CDM models are better than a CDM model with no feedback in explaining the rotation curves of low and high surface brightness galaxies in the sample. However, when compared to each other, there is no strong statistical preference for either the SIDM or the feedback-affected CDM halo model as the source of galaxy diversity in the SPARC catalog.
description: JCAP accepted version
A Late-Time Radio Flare following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh
Creators: name: Sfaradi, I.
name: Horesh, A.
name: Fender, R.
name: Green, D. A.
name: Williams, D. R. A.
name: Bright, J.
name: Schulze, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report here radio follow-up observations of the optical Tidal Disruption Event (TDE) AT 2019azh. Previously reported X-ray observations of this TDE showed variability at early times and a dramatic increase in luminosity, by a factor of $\sim 10$, about 8 months after optical discovery. The X-ray emission is mainly dominated by intermediate hard--soft X-rays and is exceptionally soft around the X-ray peak, which is $L_X \sim 10^{43} \rm \, erg \, s^{-1}$. The high cadence $15.5$ GHz observations reported here show an early rise in radio emission followed by an approximately constant light curve, and a late-time flare. This flare starts roughly at the time of the observed X-ray peak luminosity and reaches its peak about $110$ days after the peak in the X-ray, and a year after optical discovery. The radio flare peaks at $νL_ν \sim 10^{38} \rm \, erg \, s^{-1}$, a factor of two higher than the emission preceding the flare. In light of the late-time radio and X-ray flares, and the X-ray spectral evolution, we speculate a possible transition in the accretion state of this TDE, similar to the observed behavior in black hole X-ray binaries. We compare the radio properties of AT 2019azh to other known TDEs, and focus on the similarities to the late time radio flare of the TDE ASASSN-15oi.
description: 10 pages, 5 figures. Accepted for publication in ApJ
Numerical Model Of Harmonic Hall Voltage Detection For Spintronic Devices
Creators: name: Ziętek, Sławomir
name: Mojsiejuk, Jakub
name: Grochot, Krzysztof
name: Łazarski, Stanisław
name: Skowroński, Witold
name: Stobiecki, Tomasz
Publisher: name: arXiv
Year: 2022
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We present a numerical macrospin model for harmonic voltage detection in multilayer spintronic devices. The core of the computational backend is based on the Landau-Lifshitz-Gilbert-Slonczewski equation, which combines high performance with satisfactory, for large-scale applications, agreement with the experimental results. We compare the simulations with the experimental findings in Ta/CoFeB bilayer system for angular- and magnetic field-dependent resistance measurements, electrically detected magnetisation dynamics, and harmonic Hall voltage detection. Using simulated scans of the selected system parameters such as the polar angle $θ$, magnetisation saturation ($μ_\textrm{0}M_\textrm{s}$) or uniaxial magnetic anisotropy ($K_\textrm{u}$) we show the resultant changes in the harmonic Hall voltage, demonstrating the dominating influence of the $μ_\textrm{0}M_\textrm{s}$ on the first and second harmonics. In the spin-diode ferromagnetic resonance (SD-FMR) technique resonance method the ($μ_\textrm{0}M_\textrm{s}$, $K_\textrm{u}$) parameter space may be optimised numerically to obtain a set of viable curves that fit the experimental data.
description: 9 pages, 9 figures
"More minds are brought to bear on a problem": Methods of Interaction and Collaboration within Digital Humanities research
Creators: name: Siemens, Lynne
name: Cunningham, Richard
name: Duff, Wendy
name: Warwick, Claire
Publisher: name: HSSCommons
Year: 2022
Subjects: Digital humanities

description:
Digital project teams are by definition comprised of people with various skills, disciplines, and content knowledge. Collaboration within these teams is undertaken by librarians, academics, undergraduate and graduate students, research assistants, computer programmers and developers, content experts, and other individuals. While this diversity of people, skills and perspectives creates benefits for the teams, at the same time, it creates a series of challenges which must be minimized to ensure project success. Drawing upon interview and survey data, this paper explores the benefits, challenges, and patterns of interaction associated with these types of project teams. It will conclude with a series of recommendations focused on harnessing the advantages while minimizing the challenges.
Social Knowledge Creation In Action: Activities in The Electronic Textual Cultures Lab
Creators: name: Khatib, Randa
name: Arbuckle, Alyssa
name: Siemens, Ray
Publisher: name: HSSCommons
Year: 2021
Subjects: Digital Humanities

description:
Digital environments now serve as the primary network for academic and non-academic modes of communication, research practices, and knowledge dissemination. This shift has resulted in greater ease of pursuing collaborative modes of engagement. Social knowledge creation, citizen scholarship, interdisciplinary collaborations, and university-community partnerships have become more common and more visible. Engaging with such transformations in knowledge creation has been a significant research focus for the Electronic Textual Cultures Lab (ETCL) at the University of Victoria. This presentation will detail the intellectual foundations of social knowledge creation, as well as the major initiatives undertaken by the ETCL to pursue and enact this research. The ETCL explores these topics via on-campus activities as well as three substantial environmental scans: Social Knowledge Creation: Three Annotated Bibliographies” (Arbuckle, Belojevic, Hiebert, Siemens, et al., 2014), “An Annotated Bibliography on Social Knowledge Creation” (Arbuckle, Belojevic, El Hajj, El Khatib, Seatter, Siemens, et al., 2018), and “Open Social Scholarship Annotated Bibliography” (El-Hajj, El Khatib, Leibel, Seatter, et al., under development). The annotated bibliographies bring together myriad perspectives on how collaborative knowledge creation and engagement practices have been carried out, historically as well as currently. This work suggests how elements of academia might be reimagined in order to effectively integrate collaborative, interdisciplinary, public-minded praxis. Building on field touchstones like Kathleen Fitzpatrick’s Planned Obsolescence (2011) and John Willinsky’s The Access Principle (2006), this work proposes that collaboration-driven academic practices in a new media context can create a more critical work environment that integrates creative options for publishing and disseminating research.
Random Processes with High Variance Produce Scale Free Networks
Creators: name: Johnston, Josh
name: Andersen, Tim
Publisher: name: arXiv
Year: 2022
Subjects: subject: Discrete Mathematics (cs.DM)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Real-world networks tend to be scale free, having heavy-tailed degree distributions with more hubs than predicted by classical random graph generation methods. Preferential attachment and growth are the most commonly accepted mechanisms leading to these networks and are incorporated in the Barabási-Albert (BA) model. We provide an alternative model using a randomly stopped linking process inspired by a generalized Central Limit Theorem (CLT) for geometric distributions with widely varying parameters. The common characteristic of both the BA model and our randomly stopped linking model is the mixture of widely varying geometric distributions, suggesting the critical characteristic of scale free networks is high variance, not growth or preferential attachment. The limitation of classical random graph models is low variance in parameters, while scale free networks are the natural, expected result of real-world variance.
description: Submitted to Physica A. 13 pages, 1 figure
Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
Creators: name: Esposito, Matteo
name: Iršič, Vid
name: Costanzi, Matteo
name: Borgani, Stefano
name: Saro, Alexandro
name: Viel, Matteo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present an analysis aimed at combining cosmological constraints from number counts of galaxy clusters identified through the Sunyaev-Zeldovich effect, obtained with the South Pole Telescope (SPT), and from Lyman-$α$ spectra obtained with the MIKE/HIRES and X-shooter spectrographs. The SPT cluster analysis relies on mass calibration based on weak lensing measurements, while the Lyman-$α$ analysis is built over a suite of hydrodynamical simulations for the extraction of mock spectra. The resulting constraints exhibit a tension ($\sim 3.3σ$) between the low $σ_8$ values preferred by the low-redshift cluster data, $σ_8=0.74 ^{+0.03}_{-0.04}$, and the higher one preferred by the high-redshift Lyman-$α$ data, $σ_8=0.91 ^{+0.03}_{-0.03}$. We present a detailed analysis in order to understand the origin of this tension and, in particular, to establish whether it arises from systematic uncertainties related to the assumptions underlying the analyses of cluster counts and/or Lyman-$α$ forest. We found this tension to be robust with respect to the choice of modeling of the IGM, even when including possible systematics from unaccounted sub-Damped Lyman-$α$ (DLA) and Lyman-limit systems (LLS) in the Lyman-$α$ data. We conclude that to solve this tension from the SPT side would require a large bias on the cluster mass estimate, or from the Lyman-$α$ side large unaccounted errors on the Lyman-$α$ mean fluxes, respectively. Our results have important implications for future analyses based on cluster number counts from future large photometric surveys (e.g. Euclid and LSST) and on larger samples of high-redshift quasar spectra (e.g. DESI and WEAVE surveys). If confirmed at the much higher statistical significance reachable by such surveys, this tension could represent a significant challenge for the standard $Λ$CDM paradigm.
description: 14 pages, 8 figures
Additional file 2 of A fluorescence-based high-throughput screening method for cytokinin translocation mutants
Creators: name: Mengyuan Zhang
name: Bingli Ding
name: Jiangzhe Zhao
name: Penghong Zhang
name: Yujia Li
name: Guodong Yang
name: Zhang, Kewei
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 2: Figure S2. The growth conditions were optimized for mutant screening. a Seedlings of ARR5::eGFP Col-4 and ARR5::eGFP abcg14 showed discriminating phenotypes in culture sucrose at 1%, 2% and 3%. The effects of long day (LD, 16-h light/8-h dark) and all light (AL, 24-h light) growth regimes on root growth of ARR5::eGFP abcg14 were demonstrated. Scale bar, 3 mm. b Root lengths of ARR5::eGFP Col-4 and ARR5::eGFP abcg14 at 6-DAG. Data are mean ± SD (n = 6, biological replicates); Asterisks indicate significant differences compared to ARR5::eGFP Col-4 (**P
Anomalous convective transport of the tokamak edge plasma, caused by the inhomogeneous ion cyclotron parametric turbulence
Creators: name: Mikhailenko, V. S.
name: Mikhailenko, V. V.
name: Lee, Hae June
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: In this paper, we develop the kinetic and hydrodynamic theories of the convective mesoscale flows driven by the spatially inhomogeneous electrostatic ion cyclotron parametric microturbulence in the pedestal plasma with a sheared poloidal flow. The developed kinetic theory predicts the generation of the sheared poloidal convective flow, and of the radial compressed flow with radial flow velocity gradient. The developed hydrodynamic theory of the convective flows reveals the radial compressed convective flow as the dominant factor in the formation of the steep pedestal density profile with density gradient exponentially growing with time. This gradient density growth is limited by the formation of the radial oscillating with time ion outflow of pedestal plasma to scrape-off layer.
description: 25
Alabama: An Index to the State Official Sources of Agricultural Statistics
Creators: name: Olcott, Margaret T.
name: Olcott, Margaret T.
Publisher: name: Unknown
Year: 1926
Subjects: Crop Production/Industries
Demand and Price Analysis
Labor and Human Capital
Livestock Production/Industries

description: Excerpts from the report: At the meeting of the Agricultural Libraries Section of the American Library Association in July, 1925, it was proposed that the Library of the U. S. Department of Agriculture, cooperating with the agricultural librarians of the country, issue a series of source books of state agricultural statistics to meet the increasing demand for indexes in this field. In accordance with this suggestion the library of the Bureau of Agricultural Economics has compiled this index to the sources of the state official agricultural statistics of Alabama. State official sources of agricultural statistics have been indexed insofar as these sources were available in the Library of the U. S. Department of Agriculture. That is to say the publications in this library issued by official agencies of the state of Alabama, such as the Department of Agriculture and Industries, the Alabama Polytechnic Institute and the Agricultural Experiment Station were examined. In addition to such official sources the publications of the following associations have been examined: Alabama Livestock Association, Alabama State Agricultural Society, Alabama State Horticultural Society.
title: Histories of Postwar Architecture, Issue 0 (2017)
title: Issue 0 (2017)
titleType: AlternativeTitle
Creators: name: Histories Of Postwar Architecture
Publisher: name: Histories of Postwar Architecture
Year: 2017

description: Editorial
Waiting for the Site to Show Up. Henry Luce Makes Frank Lloyd Wright America’s Greatest Architect
Eduardo Torroja. 1949 Strategy to Industrialise Housing in Post-World War II
Fearless Forms: The Fluid Creations of Joaquim Cardozo
Belonging as a Corporate Ideal: Nathaniel A. Owings of Skidmore, Owings & Merrill writes The Spaces in Between (1973)
Organic or functional?
Modernism
Anonymous as a Theme of Discontinuity in the Culture of Italian Architecture between the First and Second Halves of the 20th Century
Questions That History Cannot Answer. Three Positions from 1981
(Re)Search Towards Exhibiting Architecture
Tra architettura, paesaggio e grandi capolavori: la “via” bolognese per un metodo interdisciplinare
La mostra Beton alla Kunsthalle di Vienna
The SAAL Process. Architecture and Partecipation 1974-1976, Serralves, Porto, 2015
Modernism
Optical detection of long electron spin transport lengths in a monolayer semiconductor
Creators: name: Ren, Lei
name: Lombez, Laurent
name: Robert, Cedric
name: Beret, Dorian
name: Lagarde, Delphine
name: Urbaszek, Bernhard
name: Renucci, Pierre
name: Taniguchi, Takashi
name: Watanabe, Kenji
name: Crooker, Scott A.
name: Marie, Xavier
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Using a spatially-resolved optical pump-probe experiment, we measure the lateral transport of spin/valley polarized electrons over very long distances (tens of micrometers) in a single WSe2 monolayer. By locally pumping the Fermi sea of 2D electrons to a high degree of spin/valley polarization (up to 75%) using circularly-polarized light, the lateral diffusion of the electron polarization can be mapped out via the photoluminescence induced by a spatially-separated and linearly-polarized probe laser. Up to 25% spin-valley polarization is observed at pump-probe separations up to 20 microns. Characteristic spin/valley diffusion lengths of 18 +/- 3 um are revealed at low temperatures. The dependence on temperature, pump helicity, pump intensity, and electron density highlight the key roles played by spin relaxation time and pumping efficiency on polarized electron transport in monolayer semiconductors possessing spin-valley locking.
title: Histories of Postwar Architecture, Vol 1, No 1 (2017)
title: Histories of the Futures
titleType: AlternativeTitle
Creators: name: Histories Of Postwar Architecture
Publisher: name: Histories of Postwar Architecture
Year: 2017

description: The Cybernetic Hypothesis & Architecture
Jumbo Architecture
The Image as Reaction.  Nuclear Painting and Architecture, Italy 1951-1958
The Urban Core in Japan (1930s-1950s): From Plans for the Colonies to the Mainland
Attualità dell’Antologia di edifici moderni in Milano di Piero Bottoni
Yona Friedman. Mobile Architecture, People’s Architecture  Review of The Exhibition Curated by Gong Yan and Elena Motisi
Between Science Fiction and Social Sciences: The “Dark Side” of American Cities
Editorial
Empirical investigation of the acceptance of the automated shuttle bus in Stolberg
Creators: name: Beckmann, Sönke
name: Zadek, Hartmut
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 2022
Subjects: subject: Automated shuttle buses
subject: Future mobility concepts
subject: 620

description: Automated shuttle buses are one of the future mobility concepts. As part of the AS-NaSA project, an automated shuttle bus was tested in Stolberg (Germany, Saxony-Anhalt) in 2021. Besides the use, the acceptance of such systems is very important. In addition to the users, however, the residents who live along a pilot route of an automated shuttle bus are also affected. For this reason, a household survey on the acceptance of automated shuttle buses in Stolberg is being conducted in 2022. A questionnaire based on the "Unified Theory of Acceptance and Use of Technology" model was created and every household in Stolberg received two questionnaires. The results show that the current mobility situation and public transport connections in Stolberg needs improvement. Automated shuttle buses are a possibility for the future, but the use of rail has the most support.
Pair-density-wave superconductor from doping Haldane chain and rung-singlet ladder
Creators: name: Zhang, Ya-Hui
name: Vishwanath, Ashvin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the numerical discovery of a pair-density-wave (PDW) superconductor from doping either (i) a spin-one Haldane chain or (ii) a two-leg ladder in the rung singlet phase in which the doped charges occupy a single leg. We model these systems using a generalized Kondo model. The itinerant electrons are correlated and described by the $t-J$ model, and are further coupled to a spin $1/2$ Heisenberg model through the Kondo coupling $J_K$. When the density of electrons $x$ is one, the Mott insulator is in a Haldane phase or in a rung singlet phase depending on whether $J_K$ is negative or positive. Upon doping, a pair-density-wave with $\mathbf Q=π$ can emerge for both signs of $J_K$. In the $J_K \rightarrow -\infty$ limit, the model reduces to the recently proposed type II t-J model and we observes a continuous transition between the PDW superconductor and an unconventional Luttinger liquid phase with doping. We also identify a composite order parameter for the superconductor, which can be understood as a Cooper pair formed by two nearby fermionic spin-polarons. Our model and the predicted PDW phase can be experimentally realized by doping S=1 chains formed by Ni$^{2+}$ in a solid state system or a two-leg ladder of fermionic cold atoms with a potential bias between legs, which preferentially dopes carriers into a single leg.
description: 5+19 pages; 4+16 figures
Detecting Beyond the Standard Model Interactions of Solar Neutrinos in Low-Threshold Dark Matter Detectors
Creators: name: Schwemberger, Thomas
name: Yu, Tien-Tien
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: As low-threshold dark matter detectors advance in development, they will become sensitive to recoils from solar neutrinos which opens up the possibility to explore neutrino properties. We predict the enhancement of the event rate of solar neutrino scattering from Beyond the Standard Model interactions in low-threshold DM detectors, with a focus on silicon, germanium, gallium arsenide, xenon, and argon-based detectors. We consider a set of general neutrino interactions, which fall into five categories: the neutrino magnetic moment as well as interactions mediated by four types of mediators (scalar, pseudoscalar, vector, and axial vector), and consider coupling these mediators to either quarks or electrons. Using these predictions, we place constraints on the mass and couplings of each mediator and the neutrino magnetic moment from current low-threshold detectors like SENSEI, Edelweiss, and SuperCDMS, as well as projections relevant for future experiments such as DAMIC-M, Oscura, Darwin, and ARGO. We find that such low-threshold detectors can improve current constraints by up to two orders of magnitude for vector mediators and one order of magnitude for scalar mediators.
description: 39 pages, 20 figures, 3 tables, v2: figures updated for viewer compatibility, minor typos corrected, references added
Electric field screening in pair discharges and generation of pulsar radio emission
Creators: name: Tolman, Elizabeth A.
name: Philippov, Alexander A.
name: Timokhin, Andrey N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Pulsar radio emission may be generated in pair discharges which fill the pulsar magnetosphere with plasma as an accelerating electric field is screened by freshly created pairs. In this Letter we develop a simplified analytic theory for the screening of the electric field in these pair discharges and use it to estimate total radio luminosity and spectrum. The discharge has three stages. First, the electric field is screened for the first time and starts to oscillate. Next, a nonlinear phase occurs. In this phase, the amplitude of the electric field experiences strong damping because the field dramatically changes the momenta of newly created pairs. This strong damping ceases, and the system enters a final linear phase, when the electric field can no longer dramatically change pair momenta. Applied to pulsars, this theory may explain several aspects of radio emission, including the observed luminosity, $L_{\rm{rad}} \sim 10^{28} \rm{erg} \, \rm{s}^{-1}$, and the observed spectrum, $S_ω\sim ω^{-1.4 \pm 1.0} $.
description: Updated to accepted version
Additional file 3 of A fluorescence-based high-throughput screening method for cytokinin translocation mutants
Creators: name: Mengyuan Zhang
name: Bingli Ding
name: Jiangzhe Zhao
name: Penghong Zhang
name: Yujia Li
name: Guodong Yang
name: Zhang, Kewei
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 3: Figure S3. Morphological phenotypes of rs1 to rs12. a The rosette leaves of rs mutants at 25-DAG. Scale bar,1 cm; b GFP signal in the roots of rs mutants at 6-DAG. White triangles pointing to the elevated GFP signal in mutants. DAG, days after germination
Measurement of atmospheric muon angular distribution using a portable setup of liquid scintillator bars
Creators: name: Sogarwal, Hariom
name: Shukla, Prashant
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Measurements of cosmogenic particles at various locations and altitudes are becoming increasingly important in view of worldwide interests in rare signals for search of new physics. In this work, we report measurement of muon zenith angle distributions and integrated flux using a portable setup of four one-meter long liquid scintillator bars. Each scintillator bar is read out from both sides via photomultiplier tubes followed by an 8-channel Digitizer. We exploit energy deposition and excellent timing of scintillators to construct two dimensional tracks and hence angles of charged particles. We use liquid scintillators since they have an added advantage of pulse shape discrimination (PSD) which can be used for detecting muon induced particles. The energy deposition, time window of event and PSD cuts are used to reduce the random as well as correlated backgrounds. In addition, we propose three track quality parameters which are applied to obtain a clean muon spectrum. The zenith angle measurement is performed upto $60^\circ$. With our improved analysis, we demonstrate that a setup of 3 bars can also be used for quicker and precise measurements. The vertical muon flux measured is $66.70 \pm 0.36 \pm 1.50$ $/m^2/sr/s$ with $n=2.10 \pm 0.05 \pm 0.25 $ in $\cos^n θ$ at the location of Mumbai, India ($19^{\circ}$N, $72.9^{\circ}$E) at Sea level with a muon momentum above $255$ MeV/$c$. The muon flux has dependence on various factors, the most prominents are latitudes, altitudes and momentum cut of muon so that portable setup like this can be a boon for such measurements at various locations.
description: 30 pages, 24 figures
The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
Creators: name: Mahony, Constance
name: Dvornik, Andrej
name: Mead, Alexander
name: Heymans, Catherine
name: Asgari, Marika
name: Hildebrandt, Hendrik
name: Miyatake, Hironao
name: Nishimichi, Takahiro
name: Reischke, Robert
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We determine the error introduced in a joint halo model analysis of galaxy-galaxy lensing and galaxy clustering observables when adopting the standard approximation of linear halo bias. Considering the Kilo-Degree Survey, we forecast that ignoring the non-linear halo bias would result in up to 5$σ$ offsets in the recovered cosmological parameters describing structure growth, $S_8$, and the matter density parameter, $Ω_{\mathrm{m}}$. We include the scales $10^{-1.3}
description: v2: Version accepted in MNRAS. Minor clarifications and added robustness test, conclusions unchanged
Additional file 1 of Creation of Golden Gate constructs for gene doctoring
Creators: name: Thomson, Nicholas M.
name: Chuanzhen Zhang
name: Trampari, Eleftheria
name: Pallen, Mark J.
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Supplementary Figures 1 and 2 as referenced in the manuscript.
An isolated mass gap black hole or neutron star detected with astrometric microlensing
Creators: name: Lam, Casey Y.
name: Lu, Jessica R.
name: Udalski, Andrzej
name: Bond, Ian
name: Bennett, David P.
name: Skowron, Jan
name: Mroz, Przemek
name: Poleski, Radek
name: Sumi, Takahiro
name: Szymanski, Michal K.
name: Kozlowski, Szymon
name: Pietrukowicz, Pawel
name: Soszynski, Igor
name: Ulaczyk, Krzysztof
name: Wyrzykowski, Lukasz
name: Miyazaki, Shota
name: Suzuki, Daisuke
name: Koshimoto, Naoki
name: Rattenbury, Nicholas J.
name: Hosek, Matthew W.
name: Abe, Fumio
name: Barry, Richard
name: Bhattacharya, Aparna
name: Fukui, Akihiko
name: Fujii, Hirosane
name: Hirao, Yuki
name: Itow, Yoshitaka
name: Kirikawa, Rintaro
name: Kondo, Iona
name: Matsubara, Yutaka
name: Matsumoto, Sho
name: Muraki, Yasushi
name: Olmschenk, Greg
name: Ranc, Clement
name: Okamura, Arisa
name: Satoh, Yuki
name: Silva, Stela Ishitani
name: Toda, Taiga
name: Tristram, Paul J.
name: Vandorou, Aikaterini
name: Yama, Hibiki
name: Abrams, Natasha S.
name: Agarwal, Shrihan
name: Rose, Sam
name: Terry, Sean K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the analysis of five black hole candidates identified from gravitational microlensing surveys. Hubble Space Telescope astrometric data and densely sampled lightcurves from ground-based microlensing surveys are fit with a single-source, single-lens microlensing model in order to measure the mass and luminosity of each lens and determine if it is a black hole. One of the five targets (OGLE-2011-BLG-0462/MOA-2011-BLG-191 or OB110462 for short) shows a significant $>1$ mas coherent astrometric shift, little to no lens flux, and has an inferred lens mass of 1.6 - 4.4 $M_\odot$. This makes OB110462 the first definitive discovery of a compact object through astrometric microlensing and it is most likely either a neutron star or a low-mass black hole. This compact object lens is relatively nearby (0.70-1.92 kpc) and has a slow transverse motion of $<$30 km/s. OB110462 shows significant tension between models well-fit to photometry vs. astrometry, making it currently difficult to distinguish between a neutron star and a black hole. Additional observations and modeling with more complex system geometries, such as binary sources are needed to resolve the puzzling nature of this object. For the remaining four candidates, the lens masses are $<2 M_\odot$ and they are unlikely to be black holes; two of the four are likely white dwarfs or neutron stars. We compare the full sample of five candidates to theoretical expectations on the number of black holes in the Milky Way ($\sim 10^8$) and find reasonable agreement given the small sample size.
description: Accepted to ApJ Letters, with corresponding ApJ Supplement. 10 page Letter (6 figures, 2 tables) + 51 page Supplement (27 figures, 20 tables, 9 appendices). Some minor updates from the refereeing process, but no change to main conclusions
Annex C Information Sheet 1.07 Use Of Non-Contaminated Water
Creators: name: European Food Safety Authority Panel On Plant Health
Publisher: name: Zenodo
Year: 2018
Subjects: subject: Pest control
subject: Pest management
subject: Quarantine pest
subject: Effectiveness
subject: http://id.agrisemantics.org/gacs/C587

description: Annex C Information sheet 1.07

Use of non-contaminated water

This information sheet is part of Annex C (Standardised checklist of risk reduction options) supporting document to the draft Guidance of the EFSA Plant Health Panel on quantitative pest risk assessment under public consultation (http://www.efsa.europa.eu/en/consultations/call/180212-0)

Chemical and physical treatment of water to eliminate waterborne microorganisms. The measures addressed in this information sheet are: chemical treatments (e.g. chlorine, chlorine dioxide, ozone) ; physical treatments (e.g. membrane filters, ultraviolet radiation, heat); ecological treatments (e.g. slow sand filtration).
description: Contact email: ALPHA@efsa.europa.eu
Influence of protostellar jets and HII regions on the formation and evolution of stellar clusters
Creators: name: Verliat, Antoine
name: Hennebelle, Patrick
name: González, Marta
name: Lee, Yueh-Ning
name: Geen, Sam
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Understanding the conditions in which stars and stellar clusters form is of great importance. In particular the role that stellar feedback may have is still hampered by large uncertainties. Aims. We investigate the role played by ionising radiation and protostellar outflows during the formation and evolution of a stellar cluster. To self-consistently take into account gas accretion, we start with clumps of tens of parsecs in size. Methods. Using an adaptive mesh refinement code, we run magneto-hydrodynamical numerical simulations aiming at describing the collapse of massive clumps with either no stellar feedback or taking into account ionising radiation and/or protostellar jets. Results. Stellar feedback substantially modifies the protostellar cluster properties, in several ways. We confirm that protostellar outflows reduce the star formation rate by a factor of a few, although the outflows do not stop accretion and likely enough do not modify the final cluster mass. On the other hand, ionising radiation, once sufficiently massive stars have formed, efficiently expels the remaining gas and reduces the final cluster mass by a factor of several. We found that while HII radiation and jets barely change the distribution of high density gas, the latter increases, at a few places, the dense gas velocity dispersion again by a factor of several. As we are starting from a relatively large scale, we found that the clusters whose mass and size are respectively on the order of a few 1000 M and a fraction of parsec, present a significant level of rotation. Moreover we found that the sink particles which mimic the stars themselves, tend to have rotation axis aligned with the cluster large scale rotation. Finally, computing the classical Q parameter used to quantify stellar cluster structure, we infer that when jets are included in the calculation, [...]
Additional file 4 of A fluorescence-based high-throughput screening method for cytokinin translocation mutants
Creators: name: Mengyuan Zhang
name: Bingli Ding
name: Jiangzhe Zhao
name: Penghong Zhang
name: Yujia Li
name: Guodong Yang
name: Zhang, Kewei
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 4: Table S1. Primers used in this study
Deeply Learned Preselection of Higgs Dijet Decays at Future Lepton Colliders
Creators: name: Chigusa, So
name: Li, Shu
name: Nakai, Yuichiro
name: Zhang, Wenxing
name: Zhang, Yufei
name: Zheng, Jiaming
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Future electron-positron colliders will play a leading role in the precision measurement of Higgs boson couplings which is one of the central interests in particle physics. Aiming at maximizing the performance to measure the Higgs couplings to the bottom, charm and strange quarks, we develop machine learning methods to improve the selection of events with a Higgs decaying to dijets. Our methods are based on the Boosted Decision Tree (BDT), Fully-Connected Neural Network (FCNN) and Convolutional Neural Network (CNN). We find that the BDT and FCNN-based algorithms outperform the conventional cut-based method. With our improved selection of Higgs decaying to dijet events using the FCNN, the charm quark signal strength is measured with a $16\%$ error, which is roughly a factor of two better than the $34\%$ precision obtained by the cut-based analysis. Also, the strange quark signal strength is constrained as $μ_{ss} \lesssim 35$ at the $95\%$ C.L. with the FCNN, which is to be compared with $μ_{ss} \lesssim 70$ obtained by the cut-based method.
Additional file 1 of Lure, retain, and catch malaria mosquitoes. How heat and humidity improve odour-baited trap performance
Creators: name: Cribellier, Antoine
name: Spitzen, Jeroen
name: Fairbairn, Henry
name: Geer, Cedric Van De
name: Leeuwen, Johan L. Van
name: Muijres, Florian T.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional file 1: Supplementary figures S1–S15, and legends of the supplementary datasets S1–S3 and the table S1.
Magnetization dynamics affected by phonon pumping
Creators: name: Schlitz, Richard
name: Siegl, Luise
name: Sato, Takuma
name: Yu, Weichao
name: Bauer, Gerrit E. W.
name: Huebl, Hans
name: Goennenwein, Sebastian T. B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: "Pumping" of phonons by a dynamic magnetization promises to extend the range and functionality of magnonic devices. We explore the impact of phonon pumping on room-temperature ferromagnetic resonance (FMR) spectra of bilayers of thin yttrium iron garnet (YIG) films on thick gadolinium gallium garnet substrates over a wide frequency range. At low frequencies the Kittel mode hybridizes coherently with standing ultrasound waves of a bulk acoustic resonator to form magnon polarons that induce rapid oscillations of the magnetic susceptibility, as reported before. At higher frequencies, the phonon resonances overlap, merging into a conventional FMR line, but with an increased line width. The frequency dependence of the increased line broadening follows the predictions from phonon pumping theory in the thick substrate limit. In addition, we find substantial magnon-phonon coupling of a perpendicular standing spin wave (PSSW) mode. This evidences the importance of the mode overlap between the acoustic and magnetic modes, and provides a route towards engineering the magnetoelastic mode coupling.
description: 6 pages, 3 figures
FLUKA cross sections for cosmic-ray interactions with the DRAGON2 code
Creators: name: Luque, Pedro de la Torre
name: Mazziotta, Mario Nicola
name: Ferrari, Alfredo
name: Loparco, Francesco
name: Sala, Paola
name: Serini, Davide
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Secondary particles produced in spallation reactions of cosmic rays with the interstellar gas provide valuable information that allow us to investigate the injection and transport of charged particles in the Galaxy. A good understanding of the cross sections of production of these particles is crucial to correctly interpret our models, although the existing experimental data is very scarce and uncertain. We have developed a new set of cross sections, both inelastic and inclusive, computed with the {\tt FLUKA} Monte Carlo nuclear code and tested its compatibility with CR data. Inelastic and inclusive cross sections have been compared to the most up-to-date data and parameterisations finding a general good agreement. Then, these cross sections have been implemented in the {\tt DRAGON2} code to characterize the spectra of CR nuclei up to $Z=26$ and the secondary-to-primary ratios of B, Be and Li. Interestingly, we find that the FLUKA cross sections allow us to predict an energy-dependence of the B, Be and Li flux ratios which is compatible with AMS-02 data and to reproduce simultaneously these flux ratios with a scaling lower than $20\%$. Finally, we implement the cross sections of production of gamma rays, calculated with {\tt FLUKA}, in the {\tt Gammasky} code and compute diffuse gamma-ray sky maps and the local HI emissivity spectrum, finding a very good agreement with Fermi Large Area Telescope data.
description: 28 pages, 12 figures, 3 tables
Editorial
Creators: name: Antonucci, Micaela
name: Ascari, Stefano
name: Cassani Simonetti, Matteo
name: Ciccarelli, Lorenzo
name: Formia, Elena
name: Lampariello, Beatrice
name: Nannini, Sofia
name: Rosellini, Anna
name: Sintini, Matteo
name: Tolic, Ines
Publisher: name: Histories of Postwar Architecture
Year: 2017

description: Histories of Postwar Architecture, Issue 0 (2017)