cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Structure formation during phase transitions in strongly interacting matter
Creators: name: Voskresensky, D. N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A broad range of problems associated with phase transitions in systems characterized by the strong interaction between particles and with formation of structures is reviewed. A general phenomenological mean-field model is constructed describing phase transitions of the first and the second order to the $k_0=0$ and $\vec{k}_0\neq 0$ states. Due to fluctuations, the phase transition to the state $\vec{k}_0\neq 0$ is the transition of the first order. Various specific features of the phase transitions to the state $\vec{k}_0\neq 0$ are considered such as the anisotropic spectrum of excitations, a possibility of the formation of various structures including running and standing waves, three-axis structures, chiral waves, pasta phases, etc. A formal transition to hydrodynamical variables is performed. Then focus is made on description of the dynamics of the order parameter at the phase transitions to the states with $\vec{k}_0= 0$ and $\vec{k}_0\neq 0$. Next the non-ideal hydrodynamical description of the phase transitions of the liquid-gas type in nuclear systems is performed. Quasiperiodic structures are developed. Next, pion condensation phase transition to the $\vec{k}_0\neq 0$ state in dense, cold or warm nuclear matter is considered and then the high temperature -- small baryon chemical potential system is studied, when baryons become completely blurred and light bosons, e.g., pions, may condense either in $\vec{k}_0= 0$ or $\vec{k}_0\neq 0$ states. Then, for scalar collective modes phenomena of the Pomeranchuk instability and the Bose condensation in $\vec{k}_0= 0$ or $\vec{k}_0\neq 0$ states are studied. Next, possibility of the condensation of Bose excitations in the $\vec{k}_0\neq 0$ state in moving media is considered. Then Bose-Einstein condensation of pions at dynamically fixed number of particles is studied and specific non-equilibrium effects are demonstrated on an example.
description: 110pages, 13 figures
"slhaTab08.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 31
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
The Morphology and Dynamics of Jet-Driven Supernova Remnants: the Case of W49B
Creators: name: Gonzalez-Casanova, Diego F.
name: De Colle, Fabio
name: Ramirez-Ruiz, Enrico
name: Lopez, Laura A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The circumstellar medium (CSM) of a massive star is modified by its winds before a supernova (SN) explosion occurs, and thus the evolution of the resulting supernova remnant (SNR) is influenced by both the geometry of the explosion as well as the complex structure of the CSM. Motivated by recent work suggesting the SNR W49B was a jet-driven SN expanding in a complex CSM, we explore how the dynamics and the metal distributions in a jet-driven explosion are modified by the interaction with the surrounding environment. In particular, we perform hydrodynamical calculations to study the dynamics and explosive nucleosynthesis of a jet-driven SN triggered by the collapse of a 25 solar masses Wolf-Rayet star and its subsequent interaction with the CSM up to several hundred years following the explosion. We find that although the CSM has small-scale effects on the structure of the SNR, the overall morphology and abundance patterns are reflective of the initial asymmetry of the SN explosion. Thus, we predict that jet-driven SNRs, such as W49B, should be identifiable based on morphology and abundance patterns at ages up to several hundred years, even if they expand into a complex CSM environment.
description: 5 pages, 5 figures, submitted to ApJL
A Method for Calculating Collision Probability Between Space Objects
Creators: name: Xu, Xiaoli
name: Xiong, Yongqing
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A method is developed to calculate collision probability in this paper. Based on the encounter geometric features of space objects, it is reasonable to separate the radial orbital motions from that in the cross section for most encounter events in near circular orbit. Therefore, the collision probability caused by orbit altitude difference in the radial direction and the collision probability caused by arrival time difference in the cross section are calculated respectively. The net collision probability is expressed as an explicit expression by multiplying the above two components. Numerical cases are applied to test this method by comparing the results with the general method. The results indicate that this method is valid for most near circular orbital encounter events.
description: 9 pages, 6 figures, accepted for publication in RAA
Supplemental figures from Linking deep-time subduction history to modern day expressions of dynamic topography
Creators: name: Calvelage, Christopher
name: Wu, Jonny
name: Colli, Lorenzo
name: Lin, Yi-An
name: Zheng, Yingcai
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 3706
subject: Geophysics
subject: FOS: Earth and related environmental sciences

description: This file contains supplemental figures that support the main text.
Magnetic signature of vertically migrating aggregations in the ocean
Creators: name: Fu, Matt K.
name: Dabiri, John O.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The transport of heat and solutes by vertically migrating aggregations of plankton has long been explored as a potentially important source of ocean mixing. However, direct evidence of enhanced mixing due to these migrations remains challenging to obtain and inconclusive. These shortcomings are due to the limitations of current measurement techniques, i.e., velocimetry techniques, which require a priori knowledge of the precise aggregation location and typically trigger animal avoidance behavior from introducing instrumentation into the migration. Here we develop a new approach to overcome these longstanding limitations by leveraging advancements in modern magnetometry to detect the flow-induced magnetic fields that naturally arise from seawater as it moves through the Earth's geomagnetic field. We derive quantitative predictions showing that these flow-induced magnetic fields in the vicinity of migrating aggregations have a strength proportional to the integrated fluid transport due to the migration. Importantly these magnetic signatures are potentially detectable remotely at a significant distance far from the aggregation and region of moving fluid with emerging quantum-enhanced magnetometry techniques such as Nitrogen-Vacancy centers in diamond. These results provide a new, testable framework for quantifying the significance of fluid transport in the ocean due to swimming organisms that may finally resolve a scientific debate with potentially enormous implications for our understanding of ocean dynamics and climate change.
Amylolactobacillus amylophilus AMYLOPHILUS 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Amylolactobacillus
Amylolactobacillus amylophilus

description: DESCRIPTIONOF AMYLOLACTOBACILLUS AMYLOPHILUS COMB. NOV.
Amylolactobacillus amylophilus (a.my.lo’phi.lus. Gr. neut. n. amylon starch; Gr. masc. adj. philos loving; N.L. masc. adj. amylophilus starch-loving).
Basonym: Lactobacillus amylophilus Nakamura and Crowell 1981, 216 VP (Effective publication: Nakamura and Crowell 1979, 539).
A. amylophilus strainsferment starch to L(+)-lactic acid, they also metabolise fructose, galactose, glucose, mannose and maltose [111]. The genome size is 1.56 Mbp. The mol% G+C content of DNA is 43.6 [111].
Isolated from swine waste-corn fermentation, corn-starch processing industrial wastes and kocho (Ensete ventricosum) bread.
Thetypestrainis ATCC 49845 T =LMG 6900 T =DSM 20533 T =CCUG 30137 T =CIP 102988 T =IFO (now NBRC) 15881 T =JCM 1125 T =NCAIM B.01457 T =NRRL B-4437 T =NRRL B-4476 T.
Genome sequence accession number: AYYS00000000.
16S rRNA gene accession number: M58806.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2801, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
"param_card.SM.GG.2stepWZ.dat" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the 2Step signal in Figure 6b
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Minimal physical constraints on the angular distributions of two-body boson decays
Creators: name: Faccioli, Pietro
name: Lourenco, Carlos
name: Seixas, Joao
name: Woehri, Hermine
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The angular distribution of the two-body decay of a boson of unknown properties is strongly constrained by angular momentum conservation and rotation invariance, as well as by the nature of the detected decay particles and of the colliding ones. Knowing the border between the "physical" and "unphysical" parameter domains defined by these "minimal constraints" (excluding specific hypotheses on what is still subject of measurement) is a useful ingredient in the experimental determinations of angular distributions and can provide model-independent criteria for spin characterizations. In particular, analysing the angular decay distribution with the general parametrization for the J = 2 case can provide a model-independent discrimination between the J = 0 and J = 2 hypotheses for a particle produced by two real gluons and decaying into two real photons.
"slhaTab07.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 30
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
The Berry dipole photovoltaic demon and the thermodynamics of photo-current generation within the optical gap of metals
Creators: name: Shi, Li-kun
name: Matsyshyn, Oles
name: Song, Justin C. W.
name: Villadiego, Inti Sodemann
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We dismantle the previously held misconception that it is impossible for bulk rectification mechanisms to induce a net DC electric current when the frequency of the impinging radiation lies within the optical gap of a metal in the limit of small carrier relaxation rates. We argue that generically such in-gap rectification mechanisms are irreversible and accompanied by a continuous exchange of energy with a heat bath and must also be necessarily accompanied by a small but finite absorption of radiation in order to guarantee the positivity of the net entropy production and abide by the second law of thermodynamics. We show, however, that the intra-band non-linear Hall effect arising from the Berry curvature is a special kind of in-gap rectification mechanism that behaves as a ``photo-voltaic demon'', namely it can operate as an ideal reversible and dissipationless conveyor of energy between the radiation and an external circuit. Its reversible nature allows for an interesting mode of operation as an amplifier of circularly polarized light, whose efficiency can approach 100%, and which could be technologically promising especially in the infrared frequency range.
description: 16 pages, 6 figures
Lasiopodomys brandtii
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Lasiopodomys
Lasiopodomys brandtii

description: Lasiopodomys brandtii (Radde, 1861). Melanges Biol. Acad. St. Petersbourg, 3:683. TYPE LOCALITY: Russia, NE Mongolia, near Tarei-Nor. DISTRIBUTION: Mongolia and adjacent Transbaikalia, Russia, and the Chinese provinces of E Nei Mongol, Heilungkiang, Jilin, and Hebei. SYNONYMS: aga, hangaicus, warringtoni.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 515, DOI: 10.5281/zenodo.7353098
Neutrino Flavor Conversion, Advection, and Collisions: Towards the Full Solution
Creators: name: Shalgar, Shashank
name: Tamborra, Irene
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: At high densities in compact astrophysical sources, the coherent forward scattering of neutrinos onto each other is responsible for making the flavor evolution non-linear. Under the assumption of spherical symmetry, we present the first simulations tracking flavor transformation in the presence of neutrino-neutrino forward scattering, neutral and charged current collisions with the matter background, as well as neutrino advection. We find that, although flavor equipartition could be one of the solutions, it is not a generic outcome, as often postulated in the literature. Intriguingly, the strong interplay between flavor conversion, collisions, and advection leads to a spread of flavor conversion across the neutrino angular distributions and neighboring spatial regions. Our simulations show that slow and fast flavor transformation can occur simultaneously. In the light of this, looking for crossings in the electron neutrino lepton number as a diagnostic tool of the occurrence of flavor transformation in the high-density regime is a limiting method.
description: 15 pages, 11 figures. Revtex4-1, 2-column format. Version accepted in Phys. Rev. D
"SameSignThreeLepton2017.cxx" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: pseudocode illustrating the event and object selections for all the signal regions
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Website
Creators: name: Barrio, Maria
name: Rambæk, Ida
Publisher: name: Zenodo
Year: 2022
Subjects: Water recycling and reuse
Circular economy
Environment, resources and sustainability
Sustainability transition
Symbiosis between industry and water utilities

description: The project website has been established for presentation and dissemination of the project and its deliverables. The address is www.wider-uptake.eu.
"slhaTab06.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 29
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Finding $r$-II sibling stars in the Milky Way with the Greedy Optimistic Clustering algorithm
Creators: name: Hattori, Kohei
name: Okuno, Akifumi
name: Roederer, Ian U.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: $R$-process enhanced stars with [Eu/Fe]$\geq+0.7$ (so-called $r$-II stars) are believed to have formed in an extremely neutron-rich environment in which a rare astrophysical event (e.g., a neutron star merger) occurred. This scenario is supported by the existence of an ultra-faint dwarf galaxy, Reticulum~II, where most of the stars are highly enhanced in $r$-process elements. In this scenario, some small fraction of dwarf galaxies around the Milky Way were $r$ enhanced. When each $r$-enhanced dwarf galaxy accreted to the Milky Way, it deposited many $r$-II stars in the Galactic halo with similar orbital actions. To search for the remnants of the $r$-enhanced systems, we analyzed the distribution of the orbital actions of $N=161$ $r$-II stars in the Solar neighborhood by using the Gaia EDR3 data. Since the observational uncertainty is not negligible, we applied a newly-developed {\it greedy optimistic clustering method} to the orbital actions of our sample stars. We found six clusters of $r$-II stars that have similar orbits and chemistry, one of which is a new discovery. Given the apparent phase-mixed orbits of the member stars, we interpret that these clusters are good candidates for remnants of completely disrupted $r$-enhanced dwarf galaxies that merged with the ancient Milky Way.
description: Main text 21 pages, References 3 pages, Appendix 16 pages. 11 figures. 3 tables. ApJ accepted. (See arXiv:2204.08205 for the algorithm of our method.)
Order-by-disorder and magnetic field response in Heisenberg-Kitaev model on a hyperhoneycomb lattice
Creators: name: Lee, SungBin
name: Lee, Eric Kin-Ho
name: Paramekanti, Arun
name: Kim, Yong Baek
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the finite temperature phase diagram of the Heisenberg-Kitaev model on a three dimensional hyperhoneycomb lattice. Using semiclassical analysis and classical Monte-Carlo simulations, we investigate quantum and thermal order-by-disorder, as well as the magnetic ordering temperature. We find the parameter regime where quantum and thermal fluctuations favor different magnetic orders, which leads to an additional finite temperature phase transition within the ordered phase. This transition, however, occurs at a relatively low temperature and the entropic effects may dominate most of the finite temperature region below the ordering temperature. In addition, we explore the magnetization process in the presence of a magnetic field and discover spin-flop transitions which are sensitive to the applied-field direction. We discuss implications of our results for future experiments on a hyperhoneycomb lattice system such as the recently discovered β-Li2IrO3.
description: 11 pages, 10 figures
A search for compact object companions to high mass function single-lined spectroscopic binaries in Gaia DR3
Creators: name: Jayasinghe, T.
name: Rowan, D. M.
name: Thompson, Todd A.
name: Kochanek, C. S.
name: Stanek, K. Z.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Gaia DR3 provides >181, 000 radial velocity solutions for single-lined spectroscopic binaries (SB1s) which can be used to search for non-interacting compact object+star binary candidates by selecting systems with large mass functions. We selected 234 such systems and identified 114 systems with good RV solutions in DR3. We used light curves from ASAS-SN and TESS to identify and remove 31 eclipsing binaries to produce a catalog of 80 compact object+star candidates, including 38 ellipsoidal variables. The positions of these candidates on Gaia and 2MASS CMDs suggest that many of these systems are binaries with luminous companions. We compared the periods and eccentricities of detached eclipsing binaries in Gaia DR3 and ASAS-SN, and found that ~11% and ~60% of the binaries had different periods and eccentricities. We also compared RV solutions for 311 binaries in both Gaia DR3 and the Ninth Catalog of Spectroscopic Binary Orbits (SB9), and found similar results. We do not identify any strong candidates for non-interacting compact object+star binaries.
description: 15 pages, 10 figures. Submitted to MNRAS
Binary Cepheids: Separations and Mass Ratios in $5\,M_\odot$ Binaries
Creators: name: Evans, Nancy Remage
name: Bond, Howard E.
name: Schaefer, Gail H.
name: Mason, Brian D.
name: Karovska, Margarita
name: Tingle, Evan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Deriving the distribution of binary parameters for a particular class of stars over the full range of orbital separations usually requires the combination of results from many different observing techniques (radial velocities, interferometry, astrometry, photometry, direct imaging), each with selection biases. However, Cepheids---cool, evolved stars of $\sim$$5\, M_\odot$---are a special case because ultraviolet spectra will immediately reveal any companion star hotter than early type A, {\it regardless of the orbital separation}. We have used {\it International Ultraviolet Explorer} (\IUE) UV spectra of a complete sample of all 76 Cepheids brighter than V=8 to create a list of {\it all 18} Cepheids with companions more massive than $2.0\, M_\odot$. Orbital periods of many of these binaries are available from radial-velocity studies, or can be estimated for longer-period systems from detected velocity variability. In an imaging survey with the {\it Hubble Space Telescope} Wide Field Camera 3, we resolved three of the companions (those of $η$ Aql, S Nor, and V659 Cen), allowing us to make estimates of the periods out to the long-period end of the distribution. Combining these separations with orbital data in the literature, we derive an unbiased distribution of binary separations, orbital periods, and mass ratios. The distribution of orbital periods shows that the $5\, M_\odot$ binaries have systematically shorter periods than do $1\, M_\odot$ stars. Our data also suggest that the distribution of mass ratios depends both on binary separation and system multiplicity. The distribution of mass ratios as a function of orbital separation, however, does not depend on whether a system is a binary or a triple.
description: accepted in AJ
Lasiopodomys fuscus
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Lasiopodomys
Lasiopodomys fuscus

description: Lasiopodomys fuscus (Büchner, 1889). Wiss. Res. Przewalski Cent.-Asien Reisen, Zool., I:(Säuget.), p. 125. TYPE LOCALITY: China, Qinghai Prov., "Dy-Tschju River (upper reaches of Yellow and Blue Rivers), approximately 34°N, 93°E " (as given by Ellerman and Morrison-Scott, 1951:682). DISTRIBUTION: Recorded from Qinghai Prov.; extent of range unresolved. COMMENTS: Included in Pitymys leucurus by Ellerman and Morrison-Scott (1951) and Corbet (1978c), but separated as a species and placed in Lasiopodomys by Zheng and Wang (1980).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 516, DOI: 10.5281/zenodo.7353098
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Zheng Chang-lin and Wang Sung. 1980. [On the taxonomic status of Pitymys leucurus Blyth.] Acta Zootaxonomica Sinica, 5: 106 - 112 (in Chinese)."]}
"slhaTab10.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 33
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Modeling early-universe energy injection with Dense Neural Networks
Creators: name: Sun, Yitian
name: Slatyer, Tracy R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We show that Dense Neural Networks can be used to accurately model the cooling of high-energy particles in the early universe, in the context of the public code package DarkHistory. DarkHistory self-consistently computes the temperature and ionization history of the early universe in the presence of exotic energy injections, such as might arise from the annihilation or decay of dark matter. The original version of DarkHistory uses large pre-computed transfer function tables to evolve photon and electron spectra in redshift steps, which require a significant amount of memory and storage space. We present a light version of DarkHistory that makes use of simple Dense Neural Networks to store and interpolate the transfer functions, which performs well on small computers without heavy memory or storage usage. This method anticipates future expansion with additional parametric dependence in the transfer functions without requiring exponentially larger data tables.
description: 12 pages, 10 figures. Code at https://github.com/hongwanliu/DarkHistory . Data files at https://doi.org/10.5281/zenodo.6819281
Supplementary information from Divergent age-related changes in parasite infection occur independently of behaviour and demography in a wild ungulate
Creators: name: Albery, Gregory F
name: Hasik, Adam
name: Morris, Sean
name: Morris, Alison
name: Kenyon, Fiona
name: McBean, David
name: Pemberton, Josephine
name: Nussey, Dan
name: Firth, Josh A
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310901
subject: Animal behaviour

description: Supplementary Information Ageing-Infection Paper February 2024.docx
Pre main sequence: Accretion & Outflows
Creators: name: Schneider, P. Christian
name: Günther, H. Moritz
name: Ustamujic, Sabina
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Low-mass pre-main sequence (PMS) stars are strong X-ray sources, because they possess hot corona like their older main-sequence counterparts. Unique to young stars, however, are X-rays from accretion and outflows, and both processes are of pivotal importance for star and planet formation. We describe how X-ray data provide important insight into the physics of accretion and outflows. First, mass accreted from a circumstellar disk onto the stellar surface reaches velocities up to a few hundred km/s, fast enough to generate soft X-rays in the post-shock region of the accretion shock. X-ray observations together with laboratory experiments and numerical simulations show that the accretion geometry is complex in young stars. Specifically, the center of the accretion column is likely surrounded by material shielding the inner flow from view but itself also hot enough to emit X-rays. Second, X-rays are observed in two locations of protostellar jets: an inner stationary emission component probably related to outflow collimation and outer components, which evolve withing years and are likely related to working surfaces where the shock travels through the jet. Jet-powered X-rays appear to trace the fastest jet component and provide novel information on jet launching in young stars. We conclude that X-ray data will continue to be highly important for understanding star and planet formation, because they directly probe the origin of many emission features studied in other wavelength regimes. In addition, future X-ray missions will improve sensitivity and spectral resolution to probe key model parameters (e.g. velocities) in large samples of PMS stars.
description: Invited chapter for the "Handbook of X-ray and Gamma-ray Astrophysics" (Eds. C. Bambi and A. Santangelo, Springer Nature, 2022), accepted (34 pages, 11 figures)
Physics with Trapped Charged Particles
Creators: name: Knoop, Martina
name: Madsen, Niels
name: Thompson, Richard C.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Ion traps, which were first introduced in the late 1950s and early 1960s, have established themselves as indispensable tools in many areas of physics, chemistry and technology. This chapter gives a brief survey of the operating principles and development of ion traps, together with a short description of how ions are loaded and detected. This is followed by a brief account of some of the current applications of ion traps.
"param_card.SM.GG.ttn1.dat" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the off-shell gtt signal in Figure 7a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
IEA Wind Task 43 on Wind Energy Digitalization: Task Launch Overview
Creators: name: Fields, M Jason
name: Hahn, Berthold
name: Farren, Des
Publisher: name: Zenodo
Year: 2019
Subjects: Digitalization
Wind Energy
Wind Energy Digitalization
Energy Yield Assessment
Wind Resource Assessment
Operations and maintenance

description: This presentation discusses the definition, opportunities and challenges of wind energy digitalization. It also presents the organization and management of International Energy Agency Task 43 on Wind Energy Digitalization.
Self/anti-self charge conjugate states in the helicity basis
Creators: name: Dvoeglazov, Valeriy V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: General Physics (physics.gen-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct self/anti-self charge conjugate (Majorana-like) states for the (1/2,0)+(0,1/2) representation of the Lorentz group, and their analogs for higher spins within the quantum field theory. The problem of the basis rotations and that of the selection of phases in the Dirac-like and Majorana-like field operators are considered. The discrete symmetries properties (P, C, T) are studied. Particular attention has been paid to the question of (anti)commutation of the Charge conjugation operator and the Parity in the helicity basis. Dynamical equations have also been presented. In the (1/2,0)+(0,1/2) representation they obey the Dirac-like equation with eight components, which has been first introduced by Markov. Thus, the Fock space for corresponding quantum fields is doubled (as shown by Ziino). The chirality and the helicity for Dirac and Majorana states have been discussed. PACS: 11.30.Cp, 11.30.Er, 11.30.Ly Keywords: Lorentz Group, Neutral Particles, Helicity Basis
description: 4 pp. To be published in the AIP Proceedings. Talks given at the MG13, July 2012, Stockholm, Sweden; LC2012, July 2012, Krakow, Poland; IX Mexican School DGFM-SMF, Dec. 2012, Puerta Vallarta, Mexico. Also presented at the LV Congreso Nacional de Fisica, Oct. 2012, Morelia, Mexico; slightly different version in Acta Phys. Polon. Suppl. 6 (2013), pp. 65-70
Lasiopodomys mandarinus
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Lasiopodomys
Lasiopodomys mandarinus

description: Lasiopodomys mandarinus (Milne-Edwards, 1871). Rech. Hist. Nat. Mammifères, p. 129. TYPE LOCALITY: China, Shanxi (Shansi), probably near Saratsi. DISTRIBUTION: C and NE China (Nei Mongolia, Hebei, Shaanxi, Shanxi, Jiangsu, Anhui, Heilongjiang); N Mongolia; Transbaikal region and E and SE Siberia of Russia; Korea; limits of range uncertain. SYNONYMS: faeceus, jeholensis, johannes, kishidai, pullus, vinogradovi.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 516, DOI: 10.5281/zenodo.7353098
"slhaTab12.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 35
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Lemmiscus Thomas 1912
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Lemmiscus

description: Lemmiscus Thomas, 1912. Ann. Mag. Nat. Hist., ser. 8, 9:401. TYPE SPECIES: Arvicola curtata Cope, 1868. COMMENTS: Named as a subgenus of Lagurus to segregate New World sagebrush voles from Old World steppe voles. Davis (1939) underscored the morphological separation between New and Old World forms and raised Lemmiscus to a genus, a view supported by Carleton's (1981) study of gastric anatomy. Subsequent faunal studies and checklists have variously listed Lemmiscus as a genus (Carleton and Musser, 1984; Gromov and Polyakov, 1977) or as a subgenus of Lagurus (Hall, 1981; Honacki et al., 1982). Certain morphological traits associate Lemmiscus with Microtus (Carleton, 1981; Davis, 1939), but chromosomal banding patterns provide little resolution of its phylogenetic affinity (Modi, 1987).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 516, DOI: 10.5281/zenodo.7353098
description: {"references": ["Davis, W. B. 1939. The Recent mammals of Idaho. Caldwell, Idaho, The Caxton Printers, Ltd., 400 pp.", "Carleton, M. D., and G. G. Musser. 1984. Muroid rodents. Pp. 289 - 379, in Orders and families of Recent mammals of the world (S. Anderson and J. K. Jones, Jr., eds.). John Wiley and Sons, New York, 686 pp.", "Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian).", "Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90.", "Honacki, J. H., K. E. Kinman and J. W. Koeppl (eds.). 1982. Mammal species of the world, a taxonomic and geographic reference. Allen Press, Inc. and The Association of Systematics Collections, Lawrence, Kansas, 694 pp.", "Carleton, M. D. 1981. A survey of gross stomach morphology in Microtinae (Rodentia, Muroidea). Zeitschrift fur Saugetierkunde, 46: 93 - 108.", "Modi, W. S. 1987. Phylogenetic analyses of chromosomal banding patterns among the Nearctic Arvicolidae (Mammalia: Rodentia). Systematic Zoology, 36: 109 - 136."]}
The Past, Present and Future of Cybernetics and Systems Research
Creators: name: Gershenson, Carlos
name: Csermely, Peter
name: Erdi, Peter
name: Knyazeva, Helena
name: Laszlo, Alexander
Publisher: name: arXiv
Year: 2013
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: Cybernetics and Systems Research (CSR) were developed in the mid-twentieth century, offering the possibility of describing and comparing different phenomena using the same language. The concepts which originated in CSR have spread to practically all disciplines, many now used within the scientific study of complex systems. CSR has the potential to contribute to the solution of relevant problems, but the path towards this goal is not straightforward. This paper summarizes the ideas presented by the authors during a round table in 2012 on the past, present and future of CSR.
description: 10 pages