cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A singlet doublet dark matter model with radiative neutrino masses
Creators: name: Esch, S.
name: Klasen, M.
name: Yaguna, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a detailed study of a combined singlet-doublet scalar and singlet-doublet fermion model for dark matter. These models have only been studied separately in the past. We show that their combination allows for the radiative generation of neutrino masses, but that it also implies the existence of lepton-flavour violating (LFV) processes. We first analyse the dark matter, neutrino mass and LFV aspects separately. We then perform two random scans for scalar dark matter imposing Higgs mass, relic density and neutrino mass constraints, one over the full parameter space, the other over regions where scalar-fermion coannihilations become important. In the first case, a large part of the new parameter space is excluded by LFV, and the remaining models will be probed by XENONnT. In the second case, direct detection cross sections are generally too small, but a substantial part of the viable models will be tested by future LFV experiments. Possible constraints from the LHC are also discussed.
description: 27 pages, 18 figures, 2 tables
Helix spirorbis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix spirorbis

description: Helix spirorbis [spec. nov.]
H. testa utrinque concava plana albida, anfractibus quinque teretibus.
Fn. svec. 1305.
Habitat in Europae Lacubus, magnitudine Sem. Anethi.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 770, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A new species of Pila (Gastropoda: Ampullariidae) from Mizoram, India
Creators: name: Sil, Maitreya
name: Basak, Reshma
name: Karanth, K. Praveen
name: Aravind, Neelavara Ananthram
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Family Ampullariidae consists of 11 genera of freshwater snails distributed pan-tropically in the Old and the New World. One of the ampullarid genera, Pila, is distributed in Africa and Asia and consists of 28 species. Here we describe the sixth member of the genus Pila from India. Pila mizoramensis n. sp. was collected from the Northeast Indian state of Mizoram. We adopted an integrative taxonomic approach to describe this species. First, a multilocus phylogeny of the genus was built to determine its placement in the tree. Then we used pairwise distance in the cytochrome oxidase I gene to compare its divergence from its congeners. Finally morphometric data was used to show that this hill stream species of Pila does not overlap with other hill stream species in morphometric space. The morphology of the species is also discussed in detail. With the advent of molecular tools in taxonomy a plethora of new species have been described from India in the last few decades. We add this newest member of genus Pila to the growing list.ZooBank registration: http://www.zoobank.org/urn:urn:lsid:zoobank.org:pub:0ED40557-4595-49E5-99A6-8A684C5D6AB3
Additional file 6: of Viral and metabolic controls on high rates of microbial sulfur and carbon cycling in wetland ecosystems
Creators: name: Martins, Paula Dalcin
name: Danczak, Robert
name: Roux, Simon
name: Frank, Jeroen
name: Borton, Mikayla
name: Wolfe, Richard
name: Burris, Marie
name: Wilkins, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: 60506 Virology
subject: Computational Biology

description: Figure S3. dsrA phylogenetic affiliation and abundance per sample. The RAxML tree was constructed using 162 amino acid sequences. The gene affiliation was inferred from the best BLASTP hit. For the heat map, the dsrA-containing contig RPKM values were used as input. The statistical significance of hierarchical clustering branches is indicated by green stars (pvclust, approximately unbiased pâ
Helix contorta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix contorta

description: Helix contorta [spec. nov.]
H. testa subumbilicata plana utrinque aequali, apertura lineari arcuata.
Fn. svec. 1309.
Habitat in Europae stagnis supra plantas.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 770, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Feedbacks from the metabolic network to the genetic network reveal regulatory modules in E. coli and B. subtilis
Creators: name: Kumar, Santhust
name: Mahajan, Saurabh
name: Jain, Sanjay
Publisher: name: arXiv
Year: 2018
Subjects: subject: Molecular Networks (q-bio.MN)
subject: FOS: Biological sciences

description: The genetic regulatory network (GRN) plays a key role in controlling the response of the cell to changes in the environment. Although the structure of GRNs has been the subject of many studies, their large scale structure in the light of feedbacks from the metabolic network (MN) has received relatively little attention. Here we study the causal structure of the GRNs, namely the chain of influence of one component on the other, taking into account feedback from the MN. First we consider the GRNs of E. coli and B. subtilis without feedback from MN and illustrate their causal structure. Next we augment the GRNs with feedback from their respective MNs by including (a) links from genes coding for enzymes to metabolites produced or consumed in reactions catalyzed by those enzymes and (b) links from metabolites to genes coding for transcription factors whose transcriptional activity the metabolites alter by binding to them. We find that the inclusion of feedback from MN into GRN significantly affects its causal structure, in particular the number of levels and relative positions of nodes in the hierarchy, and the number and size of the strongly connected components (SCCs). We then study the functional significance of the SCCs. For this we identify condition specific feedbacks from the MN into the GRN by retaining only those enzymes that are essential for growth in specific environmental conditions simulated via the technique of flux balance analysis (FBA). We find that the SCCs of the GRN augmented by these feedbacks can be ascribed specific functional roles in the organism. Our algorithmic approach thus reveals relatively autonomous subsystems with specific functionality, or regulatory modules in the organism. This automated approach could be useful in identifying biologically relevant modules in other organisms for which network data is available, but whose biology is less well studied.
description: 15 figures
Infrared spectroscopy of lunar core 73001: Upper limit on hydration in a lunar sample with no history of exposure to terrestrial water vapor
Creators: name: Lucey, Paul
name: Sun, Lingzhi
name: Flom, Abigail
Publisher: name: Zenodo
Year: 2024

description: This dataset includes spectra file of Apollo core sample 73001 before and after venting the curational cabinet.
MOESM11 of Regulatory T cells and M2 macrophages present diverse prognostic value in gastric cancer patients with different clinicopathologic characteristics and chemotherapy strategies
Creators: name: Liu, Xu
name: Xu, Danhua
name: Huang, Chen
name: Guo, Yixian
name: Wang, Shuchang
name: Zhu, Chunchao
name: Xu, Jia
name: Zhang, Zizhen
name: Shen, Yanying
name: Zhao, Wenyi
name: Zhao, Gang
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Additional file 11: Table S6. Univariable and multivariable analysis in different chemotherapy strategies of IIâ III gastric cancer.
Additional file 4: of A framework for assessing local transmission risk of imported malaria cases
Creators: name: Lei, Lei
name: Richards, Jack
name: Li, Zhi-Hong
name: Gong, Yan-Feng
name: Zhang, Shao-Zai
name: Xiao, Ning
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: The indexes for the two rounds of the Delphi process (DOCX 15 kb)
The Convergence Radius of the Chiral Expansion in the Dyson-Schwinger Approach
Creators: name: Meissner, Th.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We determine the convergence radius $m_{conv}$ for the expansion in the current quark mass using the Dyson-Schwinger (DS) equation of QCD in the rainbow approximation. Within a Gaussian form for the gluon propagator $D_{μν} ({\bf p}) \sim δ_{μν} χ^2 e^{- {{p^2} \over Δ}}$ we find that $m_{conv}$ increases with decreasing width $Δ$ and increasing strength $χ^2$. For those values of $χ^2$ and $Δ$, which provide the best known description of low energy hadronic phenomena, $m_{conv}$ lies around $2 Λ_{QCD}$, which is big enough, that the chiral expansion in the strange sector converges. Our analysis also explains the rather low value of $m_{conv} \approx 50 \dots 80 \ {\text MeV}$ in the Nambu--Jona-Lasinio model, which as itself can be regarded as a special case of the rainbow DS models, where the gluon propagator is a constant in momentum space.
description: 12 pages (REVTEX) + 4 postscript figures (uuencoded tar-compressed), DOE/ER/40561-140INT94-00-01
Helix cornu arietis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix cornu arietis

description: Helix cornu arietis [spec. nov.]
H. testa umbilicata planiuscula, apertura ovali.
List. conch. t. 136. f. 40. Cochlea marina compressa.
Argenv. conch. t. 11. f. E.
Klein. ostr. t. 1. f. 7.
Habitat in O. Europaeo.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Comment about the vanishing of the vacuum energy in the Wess-Zumino model
Creators: name: Barvinsky, Andrei O.
name: Kamenshchik, Alexander Yu.
name: Vardanyan, Tereza
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We check the cancellation of the vacuum energy in the Wess-Zumino model at the two-loop order in the component field formalisms with and without auxiliary fields. We show that in both cases the vacuum energy is equal to zero. However, in the formalism where the auxiliary fields are excluded, the vanishing of the vacuum energy arises due to the cancellation between the potential and kinetic energies, while in the formalism with the auxiliary fields, both terms vanish separately.
description: 13 pages
Next-to-Next-to-Leading Order QCD Analysis of DIS Structure Functions
Creators: name: Kotikov, A. V.
name: Krivokhizhin, V. G.
name: Parente, G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is performed for the first time a next-to-next-to-leading order analysis of deep inelastic structure functions $F_2$ and $F_L$ using the recently determined first moments of the non-singlet anomalous dimensions and the corresponding Wilson coefficients. {}From a comparison to BCDMS data we found a slight decrease in the energy scale of perturbative QCD with respect to the next-to-leading order analysis, which brings the scale closer to the value predicted from a scheme invariant approach.
description: Latex 12 pages, 2 figures available on request, preprint UCI-TR/94-4
A new species of Pila (Gastropoda: Ampullariidae) from Mizoram, India
Creators: name: Sil, Maiterya
name: Basak, Reshma
name: Karanth, K. Praveen
name: Aravind, Neelavara Ananthram
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Family Ampullariidae consists of 11 genera of freshwater snails distributed pan-tropically in the Old and the New World. One of the ampullarid genera, Pila, is distributed in Africa and Asia and consists of 28 species. Here we describe the sixth member of the genus Pila from India. Pila mizoramensis n. sp. was collected from the Northeast Indian state of Mizoram. We adopted an integrative taxonomic approach to describe this species. First, a multilocus phylogeny of the genus was built to determine its placement in the tree. Then we used pairwise distance in the cytochrome oxidase I gene to compare its divergence from its congeners. Finally morphometric data was used to show that this hill stream species of Pila does not overlap with other hill stream species in morphometric space. The morphology of the species is also discussed in detail. With the advent of molecular tools in taxonomy a plethora of new species have been described from India in the last few decades. We add this newest member of genus Pila to the growing list.ZooBank registration: http://www.zoobank.org/urn:urn:lsid:zoobank.org:pub:0ED40557-4595-49E5-99A6-8A684C5D6AB3
Submillimeter-selected galaxies
Creators: name: Blain, Andrew W.
name: Smail, Ian
name: Ivison, Rob
name: Kneib, Jean-Paul
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first generation of submillimeter(submm)-wave surveys are being carried out using the 450/850-micron SCUBA camera at the JCMT on Mauna Kea. These surveys are potentially sensitive to galaxies at very high redshift, and the galaxies that have been detected so far appear to contribute the greater fraction of the mm/submm-wave background radiation intensity measured by COBE. In order to understand this new population of galaxies, individual examples must be studied in detail across many wavebands; in particular their redshifts must be determined. We discuss the potential selection effects at work in submm-wave surveys and describe the spectral energy distributions of galaxies selected or luminous in the submm waveband. We also describe the general procedure for, and emphasize the difficulty of, identifying optical counterparts to submm-selected galaxies. Finally, we summarize what is known about the redshifts of these galaxies and the source of their luminosity.
description: 12 pages, 1 two-panel figure, 3 one-panel figures, uses paspconf.sty. To appear in `The Hy-redshift universe', eds A. Bunker & W. van Breughel
Highly Automated Learning for Improved Active Safety of Vulnerable Road Users
Creators: name: Bieshaar, Maarten
name: Reitberger, Günther
name: Kreß, Viktor
name: Zernetsch, Stefan
name: Doll, Konrad
name: Fuchs, Erich
name: Sick, Bernhard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Highly automated driving requires precise models of traffic participants. Many state of the art models are currently based on machine learning techniques. Among others, the required amount of labeled data is one major challenge. An autonomous learning process addressing this problem is proposed. The initial models are iteratively refined in three steps: (1) detection and context identification, (2) novelty detection and active learning and (3) online model adaption.
description: 4 pages, 1 figure
Helix hispida Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix hispida

description: Helix hispida [spec. nov.]
H. testa umbilicata convexa hispida diaphana, anfractibus quinis, apertura subrotundo-lunata.
Fn. svec. 1296.
Habitat in Svecia; terrestris.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Some Explorations in Holomorphy
Creators: name: Dine, M.
name: Shirman, Y.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In supersymmetric theories, one can obtain striking results and insights by exploiting the fact that the superpotential and the gauge coupling function are holomorphic functions of the model parameters. The precise meaning of this holomorphy is subtle, and has been explained most clearly by Shifman and Vainshtein, who have stressed the role of the Wilsonian effective action. In this note, we elaborate on the Shifman-Vainshtein program, applying it to examples in grand unification, supersymmetric QCD and string theory. We stress that among the ``model parameters" are the cutoffs used to define the Wilsonian action itself, and that generically these must be defined in a field-dependent manner to obtain holomorphic results.
description: (26 pages and 2 figures as one uuencoded PostScript file) SCIPP 94/11. Important references added; typos corrected
Additional file 6: of Targeted next-generation sequencing identifies clinically relevant somatic mutations in a large cohort of inflammatory breast cancer
Creators: name: Liang, Xu
name: Vacher, Sophie
name: Anais Boulai
name: Bernard, Virginie
name: Baulande, Sylvain
name: Mylene Bohec
name: BiĂ¨Che, Ivan
name: Lerebours, Florence
name: CĂŠline Callens
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Hematology
subject: Plant Biology

description: Figure S4. MFS curves stratified by PIK3CA mutation in three subgroups of IBC patients. (a) Kaplan-Meier estimates of MFS according to PIK3CA mutations in patients of the HRâ subgroup, (b) Kaplan-Meier estimates of MFS according to PIK3CA mutations in patients of the HER2+ subgroup, (c) Kaplan-Meier estimates of MFS according to PIK3CA mutations in patients of the HR+ subgroup. (PDF 42 kb)
Depolarization of Pulsar Radio Emission
Creators: name: Lyutikov, Maxim
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that intensity dependent depolarization of single pulses (e.g., Xiluoris et al. 1994) may be due to the nonlinear decay of the "upper" ordinary mode into an unpolarized extraordinary mode and a backward propagating wave. The decay occurs in the innermost parts of the pulsar magnetosphere for obliquely propagating O waves.
description: 6 pages, 1 postscript figure
Pseudo Dirac Neutrinos in Seesaw Model
Creators: name: Dutta, Gautam
name: Joshipura, Anjan S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Specific class of textures for the Dirac and Majorana mass matrices in the seesaw model leading to a pair of almost degenerate neutrinos is discussed. These textures can be obtained by imposing a horizontal $U(1)$ symmetry. A specific model is discussed in which: (1) All three neutrino masses are similar in magnitude and could lie around eV providing hot component of the dark matter in the universe. (2) Two of these are highly degenerate and their ${\hbox{(mass)}}^2$ difference could solve the solar neutrino problem through large angle MSW solution. (3) The electron neutrino mass may be observable through Kurie plot as well as through search of the neutrinoless double beta decay.
description: PRL-Th-94/13 (LATEX File)
Integrability, Duality and Sigma Models
Creators: name: Fateev, V. A.
name: Litvinov, A. V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We introduce and study conformal field theories specified by $W-$algebras commuting with certain set of screening charges. These CFT's possess perturbations which define integrable QFT's. We establish that these QFT's have local and non-local Integrals of Motion and admit the perturbation theory in the weak coupling region. We construct factorized scattering theory which is consistent with non-local Integrals of Motion and perturbation theory. In the strong coupling limit the $S-$matrix of this QFT tends to the scattering matrix of the $O(N)$ sigma model. The perturbation theory, Bethe anzatz technique, renormalization group approach and methods of conformal field theory are applied to show, that the constructed QFT's are dual to integrable deformation of $O(N)$ sigma-models.
The core density of dark matter halos: a critical challenge to the Lambda-CDM paradigm?
Creators: name: Navarro, Julio F.
name: Steinmetz, Matthias
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the central mass concentration of Cold Dark Matter halos found in cosmological N-body simulations with constraints derived from the Milky Way disk dynamics and from the Tully-Fisher relation. For currently favored values of the cosmological parameters ($Ω_0 \sim 0.3$; $Λ_0=1-Ω_0 \sim 0.7$; $h \sim 0.7$; COBE- and cluster abundance-normalized $σ_8$; Big-Bang nucleosynthesis $Ω_b$), we find that halos with circular velocities comparable to the rotation speed of the Galaxy have typically {\it three times} more dark matter inside the solar circle than inferred from observations of Galactic dynamics. Such high central concentrations of dark matter on the scale of galaxy disks also imply that stellar mass-to-light ratios much lower than expected from population synthesis models must be assumed in order to reproduce the zero-point of the Tully-Fisher relation. Indeed, even under the extreme assumption that {\it all} baryons in a dark halo are turned into stars, disks with conventional $I$-band stellar mass-to-light ratios ($M/L_I \sim 2 \pm 1 (M/L_I)_{\odot}$) are about two magnitudes fainter than observed at a given rotation speed. We examine several modifications to the $Λ$CDM model that may account for these discrepancies and conclude that agreement can only be accomplished at the expense of renouncing other major successes of the model. Reproducing the observed properties of disk galaxies thus appears to demand substantial revision to the currently most successful model of structure formation.
description: accepted for publication in The Astrophysical Journal
Leptonic Flavor Violations in the Presence of an Extra Z
Creators: name: Dutta, Gautam
name: Vijaykumar, K. B.
name: Joshipura, Anjan S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Gauged extensions [$SU(2)_L\otimes U(1)_Y\otimes U(1)_X$] of the standard $SU(2)_L\otimes U(1)_Y$ model obtained without extending the fermion content of the model are studied. Models that are possible when $U(1)_X$ is identified with some combination of the family lepton numbers are systematically classified. Most of these contain flavor violations in the leptonic sector. These flavor violations are correlated to the mixing of the $U(1)_X$ gauge boson $Z'$ with the ordinary $Z$ in the models considered here. Detailed phenomenological implications of a typical model are discussed. Constraints on the $Z'$ mass and the $Z$-$Z'$ mixing following from ({\em i}) the observations at LEP, ({\em ii}) rare processes like $Z\rightarrow eτ$ and ({\em iii}) flavor violating $τ$ decays are presented. It is found that the constraints coming from the LEP allows the rare processes like $τ\rightarrow eee $ at the level of the present limits on its branching ratio. Thus the future search could either improve on the existing LEP limits or would find such flavor violating decays.
description: (LATEX File, Two figures not included)
Helix ampullacea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix ampullacea

description: Helix ampullacea [spec. nov.]
H. testa subumbilicata subrotunda glabra, anfractibus supra ventricosioribus, umbilico obtecto, apertura o- vato-oblonga.
Rumph. mus. t. 27. f. Q.
Gvalt. test. t. 1. f. R.
Habitat in Asia; terrestris.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and its Consequences
Creators: name: Marietta, Evonne
name: Burrows, Adam
name: Fryxell, Bruce
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: One method of discriminating between the many Type Ia progenitor scenarios is by searching for contaminating hydrogen and helium stripped from the companion star. We present several high-resolution 2-D numerical simulations of the impact of a Type Ia supernova explosion with hydrogen-rich main sequence, subgiant, and red giant companions. The binary parameters were chosen to represent several classes of single-degenerate Type Ia progenitor models that have been suggested in the literature. We use realistic stellar models and supernova debris profiles to represent each binary system. For each scenario, we explore the hydrodynamics of the supernova-secondary interaction, calculate the amount of stellar material stripped from the secondary and the kick delivered by the impact, and construct the velocity and solid angle distributions of the stripped material. After the impact, the main sequence star is puffed up, much like a pre-main sequence star. The subgiant companion behaves similarly. The secondary will not be contaminated by much supernova debris from the initial impact, but it may accrete low-velocity iron-group elements (or oxygen and silicon if the ejecta is radially mixed) at late times. A He pre-white dwarf will be left behind after a supernova explosion with a red giant companion.
description: 58 text pages, LaTeX, 32 figures (24 BW-postscript plus 8 color-.gif); better versions of the 8 color figures and mpeg movies to be found at ftp://www.astrophysics.arizona.edu/pub/marietta; submitted to ApJ
Additional file 1: of QTL mapping and genome-wide association study reveal two novel loci associated with green flesh color in cucumber
Creators: name: Bo, Kailiang
name: Wei, Shuang
name: Wang, Weiping
name: Miao, Han
name: Dong, Shaoyun
name: Zhang, Shengping
name: Gu, Xingfang
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S1. Flesh color of five groups in the F2 population. Figure S2. Flesh color of five groups in the backcross population. a Flesh color distribution in BC1P1 population (P1 is the green flesh parent 9110Gt). b Flesh color distribution in BC1P2 population (P2 is the white flesh parent PI183967). Figure S3. Violin and box plots depicting phenotypic distribution of flesh color, flesh extract color and flesh chlorophyll content in SY2017W experiment. a Violin and box plots depicting flesh color. b Violin and box plots depicting flesh extract color. c Violin and box plots depicting flesh chlorophyll content. Figure S4. Linkage map constructed using a 234 F2 population in SY2016W experiment. Figure S5. Linkage map constructed using a 125 F2 population in BJ2017F experiment. Table S1. Summary of populations used for phenotypic data collection, QTL mapping and GWAS analysis. Table S2. Statistics of two linkage maps. Table S3. Information of markers mapped with 234 9110GtĂ PI183967 F2 population. Table S4. Information of markers mapped with 125 9110GtĂ PI183967 F2 population. Table S5. Information of the CG lines used in this study. (PDF 663 kb)
Ensuring referential integrity under causal consistency
Creators: name: Shapiro, Marc
name: Bieniusa, Annette
name: Zeller, Peter
name: Petri, Gustavo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences

description: Referential integrity (RI) is an important correctness property of a shared, distributed object storage system. It is sometimes thought that enforcing RI requires a strong form of consistency. In this paper, we argue that causal consistency suffices to maintain RI. We support this argument with pseudocode for a reference CRDT data type that maintains RI under causal consistency. QuickCheck has not found any errors in the model.
Helix pomatia Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix pomatia

description: Helix pomatia [spec. nov.]
H. testa umbilicata subovata obtusa decolori, apertura subrotundo-lunata.
Fn. svec. 1293.
Gesn. aqv. 255.
Aldr. exsangu. 389.
List. angl. 111. t. 2. f. 1.
Swamm. bibl. t. 4. f. 2.
Gvalt. test. t. 1. f. A.
Argenv. conch. t. 32. f. 1.
Habitat in Angliae, Galliae nemoribus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Aspects of the Mass Distribution of Interstellar Dust Grains in the Solar System from In-Situ Measurements
Creators: name: Landgraf, M.
name: Baggaley, W. J.
name: Grün, E.
name: Krüger, H.
name: Linkert, G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The in-situ detection of interstellar dust grains in the Solar System by the dust instruments on-board the Ulysses and Galileo spacecraft as well as the recent measurements of hyperbolic radar meteors give information on the properties of the interstellar solid particle population in the solar vicinity. Especially the distribution of grain masses is indicative of growth and destruction mechanisms that govern the grain evolution in the interstellar medium. The mass of an impacting dust grain is derived from its impact velocity and the amount of plasma generated by the impact. Because the initial velocity and the dynamics of interstellar particles in the Solar System are well known, we use an approximated theoretical instead of the measured impact velocity to derive the mass of interstellar grains from the Ulysses and Galileo in-situ data. The revised mass distributions are steeper and thus contain less large grains than the ones that use measured impact velocities, but large grains still contribute significantly to the overall mass of the detected grains. The flux of interstellar grains with masses $> 10^{-14} {\rm kg}$ is determined to be $1\cdot 10^{-6} {\rm m}^{-2} {\rm s}^{-1}$. The comparison of radar data with the extrapolation of the Ulysses and Galileo mass distribution indicates that the very large ($m > 10^{-10} {\rm kg}$) hyperbolic meteoroids detected by the radar are not kinematically related to the interstellar dust population detected by the spacecraft.
description: 14 pages, 11 figures, to appear in JGR
Moments of inertia of neutron stars in relativistic mean field theory: the role of the isovector scalar channel
Creators: name: Qian, Zhuang
name: Xing, Ruo Yu
name: Sun, Bao Yuan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: With the inclusion of the isovector scalar channel in the meson-nucleon couplings, taking DD-ME$δ$ as an effective interaction, the moments of inertia of neutron stars possessing various stellar masses are studied within the density dependent relativistic mean field (RMF) theory. The isovector scalar channel contributes to the softening of the neutron-star matter equation of state (EOS) and therefore the reduction of the maximum mass and radius of neutron stars. Smaller values of the total moment of inertia $I$ and the crustal moment of inertia $Δ{I}$ are then obtained in DD-ME$δ$ via numerical procedure in comparison with those in other selected RMF functionals. In addition, the involvement of the isovector scalar channel lowers the thickness of the neutron star crust and its mass fraction as well. The sensitivity to both the crustal mass and stellar radius causes the crustal moment of inertia to be more obviously reduced than the total one, eventually leading to a suppression on the fraction of crustal moment of inertia $Δ{I}/I$ in DD-ME$δ$. The results indicate the crustal moment of inertia as a more sensitive probe of the neutron-star matter EOS than the total one, and demonstrate that the isovector scalar meson-nucleon couplings in the RMF theory could exert influence over the physics of pulsar glitches.
description: 7 pages, 5 figures, 1 table, to be published in SCIENCE CHINA Physics, Mechanics & Astronomy
Additional file 10: of Dysregulation and prognostic potential of 5-methylcytosine (5mC), 5-hydroxymethylcytosine (5hmC), 5-formylcytosine (5fC), and 5-carboxylcytosine (5caC) levels in prostate cancer
Creators: name: Storebjerg, Tine
name: Strand, Siri
name: Høyer, Søren
name: Anne-Sofie Lynnerup
name: Borre, Michael
name: Ørntoft, Torben
name: Sørensen, Karina
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Table S1D. Clinical characteristics for PC patients represented on the TMA. Data for RP patients for whom a 5caC score could be evaluated in malignant cores. Four PC specimens had unknown ERG status. (DOCX 15 kb)
Helix glauca Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix glauca

description: Helix glauca [spec. nov.]
H. testa umbilicata subrotunda acuminata, labro marginato, apertura ovali.
Habitat ..
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
LIBERTAD Y ESTÁNDARES EN LA CORREGULACIÓN
Creators: name: Suing, Abel
Publisher: name: Zenodo
Year: 2021
Subjects: LIbertad de expresión
Regulación
Medios de comunicación
autorregulación
Derecho
comunicación
Ecuador

description: Publicación en la sección de opinión del diario digital hora 32 https://hora32.com.ec/ que se edita en Loja (Ecuador)
Additional file 4 of DUB1 suppresses Hippo signaling by modulating TAZ protein expression in gastric cancer
Creators: name: Wang, Dehai
name: Li, Zhongbo
name: Li, Xin
name: Yan, Cheng
name: Yang, Huijie
name: Zhuang, Ting
name: Wang, Xiao
name: Zang, Yifeng
name: Liu, Ziping
name: Wang, Tianshi
name: Jiang, Rixia
name: Su, Peng
name: Zhu, Jian
name: Ding, Yinlu
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 4.
Additional file 5: of Targeted next-generation sequencing identifies clinically relevant somatic mutations in a large cohort of inflammatory breast cancer
Creators: name: Liang, Xu
name: Vacher, Sophie
name: Anais Boulai
name: Bernard, Virginie
name: Baulande, Sylvain
name: Mylene Bohec
name: BiĂ¨Che, Ivan
name: Lerebours, Florence
name: CĂŠline Callens
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Figure S3. DNA copy number alterations in the IBC cohort. The genes with DNA copy number alterations are grouped along the x axis, the percentage of samples with DNA copy number alterations shown on the y axis, DNA amplifications are indicated by black bars above the x axis, and DNA deletions are indicated by gray bars below the x axis. (PDF 164 kb)
A large local rotational speed for the Galaxy found from proper-motions: Implications for the mass of the Milky-Way
Creators: name: Méndez, René A.
name: Platais, Imants
name: Girard, Terrence M.
name: Kozhurina-Platais, Vera
name: van~Altena, William F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Predictions from a Galactic Structure and Kinematic model are compared to the absolute proper-motions of about 30,000 randomly selected stars with $9 < B_{\rm J} \le 19$ derived from the Southern Proper-Motion Program (SPM) toward the South Galactic Pole. The absolute nature of the SPM proper-motions allow us to measure not only the relative motion of the Sun with respect to the local disk, but also, and most importantly, the overall state of rotation of the local disk with respect to galaxies. The SPM data are best fit by models having a solar peculiar motion of +5 km~s$^{-1}$ in the V-component (pointing in the direction of Galactic rotation), a large LSR speed of 270 km~s$^{-1}$, and a disk velocity ellipsoid that points towards the Galactic center. We stress, however, that these results rest crucially on the assumptions of both axisymmetry and equilibrium dynamics. The absolute proper-motions in the U-component indicate a solar peculiar motion of $11.0 \pm 1.5$ km~s$^{-1}$, with no need for a local expansion or contraction term. The implications of the large LSR speed are discussed in terms of gravitational mass of the Galaxy inferred from the most recent and accurate determination for the proper-motion of the LMC. We find that our derived value for the LSR is consistent both with the mass of the Galaxy inferred from the motion of the Clouds ($3 - 4 \times 10^{12} M_\odot$ to $\sim 50$ kpc), as well as the timing argument, based on the binary motion of M31 and the Milky Way, and Leo I and the Milky Way ($\ge 1.2 \times 10^{12} M_\odot$ to $\sim 200$ kpc).
description: 7 pages (AAS Latex macro v4.0), 2 B&W postscript figures, accepted for publication on ApJ, Letters section
Additional file 1 of The relations among worry, meta-worry, intolerance of uncertainty and attentional bias for threat in men at high risk for generalized anxiety disorder: a network analysis
Creators: name: Ren, Lei
name: Yang, Zhou
name: Wang, Yidi
name: Cui, Long-Biao
name: Jin, Yinchuan
name: Ma, Zhujing
name: Zhang, Qintao
name: Wu, Zhongying
name: Wang, Hua-Ning
name: Yang, Qun
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Additional file 1 : Figure S1. Bootstrapped difference test for edge weights. Figure S2. Bootstrapped difference test for node expected influences.
The BATSE Gamma-Ray Burst Spectral Catalog. I. High Time Resolution Spectroscopy of Bright Bursts using High Energy Resolution Data
Creators: name: Preece, R. D.
name: Briggs, M. S.
name: Mallozzi, R. S.
name: Pendleton, G. N.
name: Paciesas, W. S.
name: Band, D. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is the first in a series of gamma-ray burst spectroscopy catalogs from the Burst And Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory, each covering a different aspect of burst phenomenology. In this paper, we present time-sequences of spectral fit parameters for 156 bursts selected for either their high peak flux or fluence. All bursts have at least eight spectra in excess of 45 sigma above background and span burst durations from 1.66 to 278 s. Individual spectral accumulations are typically 128 ms long at the peak of the brightest events, but can be as short as 16 ms, depending on the type of data selected. We have used mostly high energy resolution data from the Large Area Detectors, covering an energy range of typically 28 - 1800 keV. The spectral model chosen is from a small empirically-determined set of functions, such as the well-known `GRB' function, that best fits the time-averaged burst spectra. Thus, there are generally three spectral shape parameters available for each of the 5500 total spectra: a low-energy power-law index, a characteristic break energy and possibly a high-energy power-law index. We present the distributions of the observed sets of these parameters and comment on their implications. The complete set of data that accompanies this paper is necessarily large, and thus is archived electronically at: http://www.journals.uchicago.edu/ApJ/journal/.
description: Accepted for publication: ApJS, 125. 38 pages, 9 figures; supplementary electronic archive to be published by ApJ; available from lead author upon request
Thermal rectification in a double quantum dots system with polaron effect
Creators: name: Tang, Gaomin
name: Zhang, Lei
name: Wang, Jian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate the rectification of heat current carried by electrons through a double quantum dot (DQD) system under a temperature bias. The DQD can be realized by molecules such as suspended carbon nanotube and be described by the Anderson-Holstein model in presence of electron-phonon interaction. Strong electron-phonon interaction can lead to formation of polaronic states in which electronic states are dressed by phonon cloud. Dressed tunneling approximation (DTA), which is nonperturbative in dealing with strong electron-phonon interaction, is employed to obtain the heat current expression. In DTA, self-energies are dressed by phonon cloud operator and are temperature dependent. The temperature dependency of imaginary part of dressed retarded self-energy gives rise to the asymmetry of the system and is the necessary condition of thermal rectification. On top of this, one can either tune DQD effective energy levels such that $|\barε_1|\neq |\barε_2|$ or have asymmetric dot-lead couplings to achieve thermal rectification. We numerically find that increasing electron-phonon coupling and reducing inter dot coupling can both improve thermal rectification effect, while the electronic heat current is reduced.
description: 8 pages, 5 figures
Spectral Stability of Inviscid Roll Waves
Creators: name: Johnson, Mathew A.
name: Noble, Pascal
name: Rodrigues, L. Miguel
name: Yang, Zhao
name: Zumbrun, Kevin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We carry out a systematic analytical and numerical study of spectral stability of discontinuous roll wave solutions of the inviscid Saint Venant equations, based on a periodic Evans-Lopatinski determinant analogous to the periodic Evans function of Gardner in the (smooth) viscous case, obtaining a complete spectral stability diagram useful in hydraulic engineering and related applications. In particular, we obtain an explicit low-frequency stability boundary, which, moreover, matches closely with its (numerically-determined) counterpart in the viscous case. This is seen to be related to but not implied by the associated formal first-order Whitham modulation equations.
description: 45 pages, 11 figures
Helix citrina Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix citrina

description: Helix citrina [spec. nov.]
H. testa umbilicata convexa obtusa flavescens: fascia fusca.
Gvalt. test. t. 1. f. D.
Argenv. conch. t. 32. f. 10.
Habitat in Jamaica australi; terrestris.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 771, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Generalized Heisenberg algebra and (non linear) pseudo-bosons
Creators: name: Bagarello, Fabio
name: Curado, Evaldo M. F.
name: Gazeau, Jean-Pierre
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose a deformed version of the generalized Heisenberg algebra by using techniques borrowed from the theory of pseudo-bosons. In particular, this analysis is relevant when non self-adjoint Hamiltonians are needed to describe a given physical system. We also discuss relations with nonlinear pseudo-bosons. Several examples are discussed.
description: Accepted in Journal of Physics A