cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
What About Model Data - Best Practices for Preservation & Replicability One-Pager
Creators: name: Mayernik, Matthew
name: Mullendore, Gretchen
name: Schuster, Douglas
Publisher: name: ESIP
Year: 2020
Subjects: subject: Atmospheric Sciences
subject: FOS: Earth and related environmental sciences
subject: Climate Science
subject: 40199 Atmospheric Sciences not elsewhere classified
subject: 49999 Earth Sciences not elsewhere classified
subject: Environmental Science
subject: Geophysics
subject: Hydrology
subject: 40107 Meteorology
subject: Oceanography
subject: 40503 Physical Oceanography

description: This document provides a brief overview of the EarthCube Research Coordination Network project, "What about model data?" Determining Best Practices for Preservation and Replicability.
Scissors resonance in the quasi-continuum of Th, Pa and U isotopes
Creators: name: Guttormsen, M.
name: Bernstein, L. A.
name: Görgen, A.
name: Jurado, B.
name: Siem, S.
name: Aiche, M.
name: Ducasse, Q.
name: Giacoppo, F.
name: Gunsing, F.
name: Hagen, T. W.
name: Larsen, A. C.
name: Lebois, M.
name: Leniau, B.
name: Renstrøm, T.
name: Rose, S. J.
name: Tornyi, T. G.
name: Tveten, G. M.
name: Wiedeking, M.
name: Wilson, J. N.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The gamma-ray strength function in the quasi-continuum has been measured for 231-233Th, 232,233Pa and 237-239U using the Oslo method. All eight nuclei show a pronounced increase in gamma strength at omega_SR approx 2.4 MeV, which is interpreted as the low-energy M1 scissors resonance (SR). The total strength is found to be B_SR = 9-11 mu_N^2 when integrated over the 1 - 4 MeV gamma-energy region. The SR displays a double-hump structure that is theoretically not understood. Our results are compared with data from (gamma, gamma') experiments and theoretical sum-rule estimates for a nuclear rigid-body moment of inertia.
description: 11 pages, 9 figures
title: Cycloadditions of Azulene at High Pressure
Creators: name: Klärner, Frank-Gerrit
name: Dogan, Barbara
name: Roth, Wolfgang R.
name: Hafner, Klaus
Publisher: name: Wiley
Year: 2023

description: Reaction of dimethyl acetylenedicarboxylate 2a with azulene 1 (boiling tetralin, 207.6 °C) leads to the heptalene-dicarboxylic acid dimethyl ester 7a[¹].
Companilactobacillus alimentarius PARALIMENTARIUS 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
Companilactobacillus
Companilactobacillus alimentarius

description: DESCRIPTIONOF COMPANILACTOBACILLUS ALIMENTARIUS COMB. NOV.
Companilactobacillus alimentarius (a.li.men.ta'ri.us. L. masc. adj. alimentarius related to food).
Basonym: Lactobacillus alimentarius (ex Reuter 1970) Reuter 1983a, 672 VP
Growth is observed between 15 and 37°C and with pentoses, hexoses and disaccharides as carbon sources [115]. The genome size is 2.34 Mbp. The mol% G+C content of DNA is 35.4.
Isolated as spoilage organisms from marinated fish products, as fermentation organismsin fermented sausages, as spoilage organism in ready-to-eat meats. Astrain of the species had been usedas biopreservatives culture [116]. It occurs inassociation with Fructilactobacillus sanfranciscensis intype Isourdoughs [114] and was isolated in other plant fermentations.
Thetypestrainis R13 T =ATCC 29643 T =CCUG 30672 T =CIP 102986 T =DSM 20249 T =JCM 1095 T =LMG 9187 T.
Genome sequence accession number: AZDQ00000000.
16S RNA gene sequence accession number: M58804.
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 2803, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Orientation Dependence of the Critical Magnetic Field for Multiferroic BiFeO$_3$
Creators: name: Fishman, Randy S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Multiferroic BiFeO3 undergoes a transition from a distorted spiral phase to a G-type antiferromagnet above a critical field H_c that depends on the orientation m of the field. We show that H_c(m) has a maximum when oriented along a cubic diagonal parallel to the electric polarization P and a minimum in the equatorial plane normal to P when two magnetic domains with the highest critical fields are degenerate. The measured critical field along a cubic axis is about 19 T but H_c is predicted to vary by as much as 2.5 T above and below this value. The orientational dependence of H_c(m) is more complex than indicated by earlier work, which did not consider the competition between magnetic domains.
description: 4 pages, 3 figures
Local Statistics of Immiscible and Incompressible Two-Phase Flow in Porous Media
Creators: name: Fyhn, Hursanay
name: Sinha, Santanu
name: Hansen, Alex
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We consider immiscible and incompressible two-phase flow in porous media under steady-state conditions using a dynamic pore network model. We focus on the fluctuations in a Representative Elementary Area (REA), with the aim to demonstrate that the statistical distributions of the volumetric flow rate and the saturation within the REA become independent of the size of the entire model when the model is large enough. This independence is a necessary condition for developing a local statistical theory for the flow, which in turn opens for the possibility to formulate a description at scales large enough for the typical pore size to be negligible using differential equations.
Microtus kirgisorum
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus kirgisorum

description: Microtus kirgisorum (Ognev, 1950). [Mammals of USSR and Adjacent Countries], 7:219. TYPE LOCALITY: Kazakhstan, Tuyouk, Khirgiski Mtns. DISTRIBUTION: Recorded from S Kazakhstan, Kirghizia, Tadzhikistan, and SE Turkmenistan; may also occur in N Afghanistan. COMMENTS: Subgenus Microtus, arvalis species group sensu Zagorodnyuk (1990). Originally described as a subspecies of M. arvalis but later elevated to a separate species (Meier, 1983; Meier et al., 1981), as observed by Corbet (1984) and Pavlinov and Rossolimo (1987). Chromosomal data presented by Orlov et al. (1983) in context of phylogenetic study among members of the M. arvalis group.
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 523, DOI: 10.5281/zenodo.7353098
description: {"references": ["Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Corbet, G. B. 1984. The mammals of the Palearctic region: A taxonomic review. Supplement. British Museum (Natural History), London, 45 pp.", "Pavlinov, I. Ya., and O. L. Rossolimo. 1987. Sistematika mlekopitayushchikh SSSR [Systematics of the mammals of the USSR.]. Moscow University Press, Moscow, 282 pp. (in Russian)."]}
Enhancement of electron spin lifetime in GaAs crystals: the benefits of dichotomous noise
Creators: name: Spezia, Stefano
name: Adorno, Dominique Persano
name: Pizzolato, Nicola
name: Spagnolo, Bernardo
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The electron spin relaxation process in n-type GaAs crystals driven by a fluctuating electric field is investigated. Two different sources of fluctuations are considered: (i) a symmetric dichotomous noise and (ii) a Gaussian correlated noise. Monte Carlo numerical simulations show, in both cases, an enhancement of the spin relaxation time by increasing the amplitude of the external noise. Moreover, we find that the electron spin lifetime versus the noise correlation time: (i) increases up to a plateau in the case of dichotomous random fluctuations, and (ii) shows a nonmonotonic behaviour with a maximum in the case of bulks subjected to a Gaussian correlated noise.
description: 6 pages, 3 figures
Neutrino production from photo-hadronic interactions of the gamma flux from Active Galactic Nuclei with their gas content
Creators: name: Arteaga-Velazquez, J. C.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The diffuse neutrino flux from FRI and BL Lac type galaxies generated from interactions of their own gamma radiation with the gas and dust at the sources is reported. This neutrino-production channel has not been studied in detail up to now. The calculations are based on individual estimations of the neutrino flux in two nearby AGN's: Centaurus A and M87, assuming the validity of the AGN unification model. The predictions for Centaurus A and M87 involved the parameterization of the measured gamma-ray luminosities and the modeling of the material of the galaxies both based on observations performed by several detectors. No hadronic origin for the TeV photons is assumed. The results show that, although the corresponding neutrino flux ($E^{2} Φ_{ν+ \barν} < 10^{-13} s^{-1} sr^{-1} GeV cm^{-2}$) is not competitive at high-energies ($E_ν> 1 TeV$) with that from hadronic models, FRI and BL Lac galaxies with gamma emission should be already contributing to the diffuse flux of neutrinos in the universe.
description: 25 pages, 9 figures, published in Astroparticle Physics
Top-Down Racial Biases in Size Perception: A Registered Replication and Extension of Wilson et al. (2017)
Creators: name: Mayan Navon
name: Reggev, Niv
name: Moran, Tal
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Social and Behavioral Sciences

description: This is a pre-registration of Study 2 -- conceptual replication -- in a registered replication project of Wilson et al. (2017, JPSP).
Multiphoton coherent states for bilayer graphene
Creators: name: C., David J. Fernández
name: Martínez-Moreno, Dennis I.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The multiphoton coherent states, a generalization to coherent sates, are derived for electrons in bilayer graphene placed in a constant homogeneous magnetic field which is orthogonal to the bilayer surface. For that purpose a generalized annihilation operator is constructed in order to determine the multiphoton coherent states as eigenstates of such operator with complex eigenvalue. In addition, some physical quantities are calculated for these states, as the Heisenberg uncertainty relation, probability density and mean energy value. Finally, in order to study the dynamics of the system the time evolution is explored and the time-correlation function is computed.
Companilactobacillus allii Zheng & Wittouck & Salvetti & Franz & Harris & Mattarelli & O'Toole & Pot & Vandamme & Walter & Watanabe & Wuyts & Felis & Gänzle & Lebeer 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
Companilactobacillus
Companilactobacillus allii

description: DESCRIPTIONOF COMPANILACTOBACILLUS ALLII COMB. NOV.
Companilactobacillus allii (al’li.i. L. gen. n. allii of Egyptian onions (Allium proliferum), the source of fermented onions, pa-kimchi, from which the type strain was isolated).
Basonym: Lactobacillus allii Jung et al. 2017, 4939 VP
Growth is observed at 25 and 37 °C; hexoses and disaccharides but not pentoses are fermented [117]. The genome size is 2.51 Mbp. The mol% G+C content of DNA is 35.3.
Isolated from scallion kimchi.
Thetypestrainis WiKim39 T =KCTC 21077 T =JCM 31938 T.
Genome sequence accession numbers: CP019323 (chromosome) and CP019324 (plasmid).
16S RNA gene sequence accession number: NR_159082.
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 2803, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
THE PRACTICES AND CHALLENGES OF SCHOOL LEADERSHIP IN THE SECONDARY SCHOOLS OF BOLE SUBCITY
Creators: name: DEMELASH MISGANA
Publisher: name: Zenodo
Year: 2022

description: The purpose of the study was to assess the practices of school leadership and the challenges that school leaders face in performing their duties in Secondary Schools of Bole sub city. The study employed a descriptive survey design. Principals, vice principals and supervisors were selected using purposive sampling. Semi structured interview was also utilized to substantiate the data gained through the questionnaires. Both primary and secondary sources were used. The primary sources of this study were principals, vice principals, supervisors and teachers of the selected schools. On the other hand secondary sources were relevant documents of the schools in the study area. To gather the necessary data three types of data collection instruments namely questionnaire consisting of closed ended item, structured interview and document analysis were used descriptive approach such as percentage, frequency, mean, standard deviation and grand mean were utilized to analyze the data .The qualitative data obtained through interview was analyzed using themes. The results of the study revealed that all school principals have qualification in school leadership but some of school vice principals involved in leading the school without having prior qualification in school leadership and trainings. The study concluded that principals are less effective in their leadership due to problem of working with parents and community, work overload and lack of sharing the problems of school leadership by higher officials. Finally, the point of the recommended that qualified secondary school principals and vice principals be assigned it is on the basis of their experience and academic merits, providing in-service and pre-service training and build productive relationships with parents and the wider community.
The generalized scaling relations for X-ray galaxy clusters: the most powerful mass proxy
Creators: name: Ettori, S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The application to observational data of the generalized scaling relations (gSR) presented in Ettori et al. (2012) is here discussed. We extend further the formalism of the gSR in the self-similar model for X-ray galaxy clusters, showing that for a generic relation M_tot ~ L^a M_g^b T^c, where L, M_g and T are the gas luminosity, mass and temperature, respectively, the values of the slopes lay in the plane 4*a+3*b+2*c=3. Using published dataset, we show that some projections of the gSR are the most efficient relations, holding among observed physical X-ray quantities, to recover the cluster mass. This conclusion is based on the evidence that they provide the lowest chi^2, the lowest total scatter and the lowest intrinsic scatter among the studied scaling laws on both galaxy group and cluster mass scales. By the application of the gSR, the intrinsic scatter is reduced in all the cases down to a relative error on M_tot below 16 per cent. The best-fit relations are: M_tot ~ M_g^a T^{1.5-1.5a}, with a~0.4, and M_tot ~ L^a T^{1.5-2a}, with a~0.15. As a by product of this study, we provide the estimates of the gravitating mass at Delta=500 for 120 objects (50 from the Mahdavi et al. 2013 sample, 16 from Maughan 2012; 31 from Pratt et al. 2009; 23 from Sun et al. 2009), 114 of which are unique entries. The typical relative error in the mass provided from the gSR only (i.e. not propagating any uncertainty associated with the observed quantities) ranges between 3-5 per cent on cluster scale and is about 10 per cent for galaxy groups. With respect to the hydrostatic values used to calibrate the gSR, the masses are recovered with deviations in the order of 10 per cent due to the different mix of relaxed/disturbed objects present in the considered samples. In the extreme case of a gSR calibrated with relaxed systems, the hydrostatic mass in disturbed objects is over-estimated by about 20 per cent.
description: 13 pages, 3 figures, 5 tables. MNRAS in press
Instability of spherically-symmetric black holes in Quadratic Gravity
Creators: name: Held, Aaron
name: Zhang, Jun
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate the linear stability of the two known branches of spherically-symmetric black holes in Quadratic Gravity. We extend previous work on the long-wavelength (Gregory-Laflamme) instability of the Schwarzschild branch to a corresponding long-wavelength instability in the non-Schwarzschild branch. In both cases, the instability sets in below a critical horizon radius at which the two black-hole branches intersect. This suggests that classical perturbations enforce a lower bound on the horizon radius of spherically-symmetric black holes in Quadratic Gravity.
description: 10 pages, 4 figures + appendix and references
Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
Creators: name: Pullen, Anthony R.
name: Breysse, Patrick C.
name: Oxholm, Trevor
name: Switzer, Eric R.
name: Anderson, Christopher J.
name: Barrentine, Emily
name: Bolatto, Alberto D.
name: Cataldo, Giuseppe
name: Essinger-Hileman, Thomas
name: Maniyar, Abhishek
name: Stevenson, Thomas
name: Somerville, Rachel S.
name: Volpert, Carrie
name: Wollack, Edward
name: Yang, Shengqi
name: Yung, L. Y. Aaron
name: Zhou, Zilu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a balloon-borne cryogenic telescope that will survey the spectrum of diffuse emission from both the Milky Way and the cosmic web to probe star formation, the interstellar medium, and galaxy evolution across cosmic time. EXCLAIM's primary extragalactic science survey maps 305 deg$^2$ along the celestial equator with an R=512 spectrometer over the frequency range ν=420-540 GHz, targeting emission of the [CII] line over redshifts 2.5
description: 19 pages, 14 figures, will submit to MNRAS
Microtus leucurus
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus leucurus

description: Microtus leucurus (Blyth, 1863). J. Asiat. Soc. Bengal, 32:89. TYPE LOCALITY: India, Ladakh, near Lake Chomoriri (= Tsomoriri). DISTRIBUTION: Chinese provinces of S Qinghai (Zheng and Wang, 1980) and Xizang (Feng et al., 1986) on the Tibetan Plateau, and high altitudes in the Himalayas west to Kashmir (see Niethammer, 1970). SYNONYMS: everesti, petulans, strauchi, waltoni, zadoensis. COMMENTS: Classified by Zagorodnyuk (1990) under the subgenus Phaiomys of the genus Neodon; others have recognized Phaiomys as a genus (Repenning et al., 1990). Whatever its ranking, leucurus may date from the early evolution of the genus, as suggested by its association with the late Pliocene Allophaiomys, a taxon regarded by most as ancestral to Microtus (see Martin, 1989b; Repenning et al., 1990). As classified in the genus Microtus, this species can still be called leucurus; the older leucurus Gerbe, 1852, is a synonym of nivalis, a species which has been reallocated from Microtus to Chionomys (see that account).
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 523, DOI: 10.5281/zenodo.7353098
description: {"references": ["Zheng Chang-lin and Wang Sung. 1980. [On the taxonomic status of Pitymys leucurus Blyth.] Acta Zootaxonomica Sinica, 5: 106 - 112 (in Chinese).", "Feng Zuo-jiang, Cai Gui-quan, and Zheng Chang-lin. 1986. [The mammals of Xizang. The comprehensive scientific expedition to the Qinghai-Xizang Plateau]. Science Press, Academia Sinica, Beijing, 423 pp. (in Chinese).", "Niethammer, J. 1970. Die Wuhlmause (Microtinae) Afghanistans. Bonner Zoologische Beitrage, 21: 1 - 24.", "Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Repenning, C. A., O. Fejfar, and W. - D. Heinrich. 1990. Arvicolid rodent biochronology of the Northern Hemisphere. Pp. 385 - 417, in International symposium evolution, phylogeny and biostratigraphy of arvicolids (Rodentia, Mammalia) (O. Fejfar and W. - D. Heinrich, eds.). Geological Survey, Prague, 448 pp.", "Martin, R. A. 1989 b. Arvicolid rodents of the early Pleistocene Java Local Fauna from north-central South Dakota. Journal of Vertebrate Paleontology, 9: 438 - 450."]}
Acceptability and efficacy of a single-session repetitive negative thinking intervention: a pilot study
Creators: name: Hughes, Christopher David
Publisher: name: No Publisher Supplied
Year: 2020

description: Repetitive Negative Thinking (RNT) is a cognitive process that is repetitive, passive/unproductive, difficult to control, and focused predominantly on negative content. RNT has been identified as a transdiagnostic risk factor associated with the development and/or maintenance of a wide variety of psychological disorders and problematic behaviors. While evidence-based treatments exist that address RNT in some way, they are limited in their ability to reach the wide range of individuals experiencing problems with RNT. The present study sought to develop a single-session mindfulness-based skills-training video aimed at reducing RNT and assess its acceptability and preliminary efficacy across multiple methods. Participants, adult community members screened for high trait RNT (n = 71), completed baseline questionnaires and scheduled an in-person lab visit. Participants were randomly assigned to either the active (skills-training) or the control (no skills training) condition. The intervention’s preliminary efficacy was then assessed by comparing the groups’ levels of RNT and Negative Affect (NA): following an RNT induction during the lab visit, over the course of a five-day Ecological Momentary Assessment (EMA) monitoring period, and self-reported at follow-up relative to baseline. The intervention’s acceptability was assessed based on participants expectations at the end of the lab visit, their momentary reports of skills use and perceived effectiveness, and their retrospective satisfaction and perceived utility of the intervention at follow-up.Overall, results were promising for the intervention. The active condition demonstrated statistically and clinically significant and reliable reductions in RNT and NA at follow-up compared to baseline. They also reported less RNT and NA and more frequent and successful skills use over the course of the EMA monitoring period. However, we were unable to assess the impact of the skills training immediately after training in the lab because the RNT induction failed to induce RNT or NA in either condition. Finally, active condition participants reported finding the intervention acceptable across all three assessment timepoints. These finding indicate that a single-session mindfulness-based skills-training intervention is acceptable and potentially efficacious in reducing RNT. Together with the intervention’s preliminary promise, its brevity, low cost, ability to be delivered online, and applicability to a wide range of populations, make this a promising intervention that warrants continued investigation, development, and refinement.
Characterization of the Young Open Cluster G144.9+0.4 in the Camelopardalis OB1 Association
Creators: name: Lin, Chien-Cheng
name: Chen, W. P.
name: Panwar, Neelam
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Our star-count analysis of the Two Micron All Sky Survey point sources resulted in an identification of the star cluster G144.9+0.4. The cluster was found, but not characterized, by Glushkova et al. We show that the cluster is physically associated with the Cam OB1 association at a distance of about 1 kpc and with an age of 1-2 Myr. Pre-main sequence stars are identified on the basis of photometric and proper motion data. A total of 91 additional OB star candidates was found in subgroups 1A and 1B, a significant increase from the currently known 43 OB stars. The OB members show an age spread that indicates a sustained star formation for at least the last 10-15 Myr. The young cluster G144.9+0.4 represents the latest episode of sequential star formation in this cloud complex.
description: 33pages, 10 figures, published in ApJ
Assessing lack of common support in causal inference using Bayesian nonparametrics: Implications for evaluating the effect of breastfeeding on children's cognitive outcomes
Creators: name: Hill, Jennifer
name: Su, Yu-Sung
Publisher: name: arXiv
Year: 2013
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: Causal inference in observational studies typically requires making comparisons between groups that are dissimilar. For instance, researchers investigating the role of a prolonged duration of breastfeeding on child outcomes may be forced to make comparisons between women with substantially different characteristics on average. In the extreme there may exist neighborhoods of the covariate space where there are not sufficient numbers of both groups of women (those who breastfed for prolonged periods and those who did not) to make inferences about those women. This is referred to as lack of common support. Problems can arise when we try to estimate causal effects for units that lack common support, thus we may want to avoid inference for such units. If ignorability is satisfied with respect to a set of potential confounders, then identifying whether, or for which units, the common support assumption holds is an empirical question. However, in the high-dimensional covariate space often required to satisfy ignorability such identification may not be trivial. Existing methods used to address this problem often require reliance on parametric assumptions and most, if not all, ignore the information embedded in the response variable. We distinguish between the concepts of "common support" and common causal support." We propose a new approach for identifying common causal support that addresses some of the shortcomings of existing methods. We motivate and illustrate the approach using data from the National Longitudinal Survey of Youth to estimate the effect of breastfeeding at least nine months on reading and math achievement scores at age five or six. We also evaluate the comparative performance of this method in hypothetical examples and simulations where the true treatment effect is known.
description: Published in at http://dx.doi.org/10.1214/13-AOAS630 the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Synthesis of cold and trappable fully stripped HCI's via antiproton-induced nuclear fragmentation in traps
Creators: name: Kornakov, G.
name: Cerchiari, G.
name: Zieliński, J.
name: Lappo, L.
name: Sadowski, G.
name: Doser, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The study of radioisotopes as well as of highly charged ions is a very active and dynamic field. In both cases, the most sensitive probes involve species trapped in Penning or Paul traps after a lengthy series of production and separation steps that limit the types and lifetimes of species that can be investigated. We propose a novel production scheme that forms fully (or almost fully) stripped radionuclei in form of highly charged ions (HCI's) directly in the trapping environment. The method extends the range of species, among them radioisotopes such as $^{21}$F, $^{100}$Sn or $^{229}$Th, that can be readily produced and investigated and is complementary to existing techniques.
description: 9 pages, 6 figures
Hierarchy of quasi-symmetries and degeneracies in chiral crystal materials CoSi
Creators: name: Hu, Lun-Hui
name: Guo, Chunyu
name: Sun, Yan
name: Felser, Claudia
name: Elcoro, Luis
name: Moll, Philip J. W.
name: Liu, Chao-Xing
name: Bernevig, B. Andrei
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In materials, certain approximated symmetry operations can exist in a lower-order approximation of the effective model but are good enough to influence the physical responses of the system, and these approximated symmetries were recently dubbed "quasi-symmetries" \cite{guo_arxiv_2021}. In this work, we reveal a hierarchy structure of the quasi-symmetries and the corresponding nodal structures that they enforce via two different approaches of the perturbation expansions for the effective model in the chiral crystal material CoSi. In the first approach, we treat the spin-independent linear momentum (k) term as the zero-order Hamiltonian. Its energy bands are four-fold degenerate due to an SU(2)$\times$SU(2) quasi-symmetry. We next consider both the k-independent spin-orbit coupling (SOC) and full quadratic-k terms as the perturbation terms and find that the first-order perturbation leads to a model described by a self-commuting "stabilizer code" Hamiltonian with a U(1) quasi-symmetry that can protect nodal planes. In the second approach, we treat the SOC-free linear-k term and k-independent SOC term as the zero-order. They exhibit an SU(2) quasi-symmetry, which can be reduced to U(1) quasi-symmetry by a choice of quadratic terms. Correspondingly, a two-fold degeneracy for all the bands due to the SU(2) quasi-symmetry is reduced to two-fold nodal planes that are protected by the U(1) quasi-symmetry. For both approaches, including higher-order perturbation will break the U(1) quasi-symmetry and induce a small gap $\sim$ 1 meV for the nodal planes. These quasi-symmetry protected near degeneracies play an essential role in understanding recent quantum oscillation experiments in CoSi.
description: 4+41 pages, welcomes are welcome
Low-energy nuclear physics and global neutron star properties
Creators: name: Carlson, Brett V.
name: Dutra, Mariana
name: Lourenço, Odilon
name: Margueron, Jérôme
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We address the question of the role of low-energy nuclear physics data in constraining neutron star global properties, e.g., masses, radii, angular momentum, and tidal deformability, in the absence of a phase transition in dense matter. To do so, we assess the capacity of 415 relativistic mean field and non-relativistic Skyrme-type interactions to reproduce the ground state binding energies, the charge radii and the giant monopole resonances of a set of spherical nuclei. The interactions are classified according to their ability to describe these characteristics and we show that a tight correlation between the symmetry energy and its slope is obtained providing $N=Z$ and $N\ne Z$ nuclei are described with the same accuracy (mainly driven by the charge radius data). By additionally imposing the constraints from isobaric analog states and neutron skin radius in $^{208}$Pb, we obtain the following estimates: $E_{sym,2}=31.8\pm 0.7$ MeV and $L_{sym,2}=58.1\pm 9.0$ MeV. We then analyze predictions of neutron star properties and we find that the 1.4$M_\odot$ neutron star (NS) radius lies between 12 and 14 km for the "better" nuclear interactions. We show that i) the better reproduction of low-energy nuclear physics data by the nuclear models only weakly impacts the global properties of canonical mass neutron stars and ii) the experimental constraint on the symmetry energy is the most effective one for reducing the uncertainties in NS matter. However, since the density region where constraints are required are well above densities in finite nuclei, the largest uncertainty originates from the density dependence of the EDF, which remains largely unknown.
description: 26 pages, 20 figures
Transitional $γ$ strength in Cd isotopes
Creators: name: Larsen, A. C.
name: Ruud, I. E.
name: Bürger, A.
name: Goriely, S.
name: Guttormsen, M.
name: Görgen, A.
name: Hagen, T. W.
name: Harissopulos, S.
name: Nyhus, H. T.
name: Renstrøm, T.
name: Schiller, A.
name: Siem, S.
name: Tveten, G. M.
name: Voinov, A. V.
name: Wiedeking, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The level densities and $γ$-ray strength functions of $^{105,106,111,112}$Cd have been extracted from particle-$γ$ coincidence data using the Oslo method. The level densities are in very good agreement with known levels at low excitation energy. The $γ$-ray strength functions display no strong enhancement for low $γ$ energies. However, more low-energy strength is apparent for $^{105,106}$Cd than for $^{111,112}$Cd. For $γ$ energies above $\approx$ 4 MeV, there is evidence for some extra strength, similar to what has been previously observed for the Sn isotopes. The origin of this extra strength is unclear; it might be due to $E1$ and $M1$ transitions originating from neutron skin oscillations or the spin-flip resonance, respectively.
description: 10 pages, 11 figures
Implicit Full Waveform Inversion with Deep Neural Representation
Creators: name: Sun, Jian
name: Innanen, Kristopher
Publisher: name: arXiv
Year: 2022
Subjects: subject: Geophysics (physics.geo-ph)
subject: Machine Learning (cs.LG)
subject: Signal Processing (eess.SP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Full waveform inversion (FWI) commonly stands for the state-of-the-art approach for imaging subsurface structures and physical parameters, however, its implementation usually faces great challenges, such as building a good initial model to escape from local minima, and evaluating the uncertainty of inversion results. In this paper, we propose the implicit full waveform inversion (IFWI) algorithm using continuously and implicitly defined deep neural representations. Compared to FWI, which is sensitive to the initial model, IFWI benefits from the increased degrees of freedom with deep learning optimization, thus allowing to start from a random initialization, which greatly reduces the risk of non-uniqueness and being trapped in local minima. Both theoretical and experimental analyses indicates that, given a random initial model, IFWI is able to converge to the global minimum and produce a high-resolution image of subsurface with fine structures. In addition, uncertainty analysis of IFWI can be easily performed by approximating Bayesian inference with various deep learning approaches, which is analyzed in this paper by adding dropout neurons. Furthermore, IFWI has a certain degree of robustness and strong generalization ability that are exemplified in the experiments of various 2D geological models. With proper setup, IFWI can also be well suited for multi-scale joint geophysical inversion.
Microtus limnophilus Buchner 1889
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Microtus
Microtus limnophilus

description: Microtus limnophilus Büchner, 1889. Wiss. Res. Przewalski Cent.-Asien. Reis. Zool., I:(Saugeth.), p. 110. TYPE LOCALITY: China, Qinghai. DISTRIBUTION: From Qinghai Prov. to W Mongolia. COMMENTS: Subgenus Pallasiinus, oeconomus species group sensu Zagorodnyuk (1990). Formerly included in M. oeconomus but separated as a species parapatric with M. oeconomus in W Mongolia (Malygin et al., 1990, and references therein).
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 523, DOI: 10.5281/zenodo.7353098
description: {"references": ["Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Malygin, V. M., V. N. Orlov, and V. N. Yatsenko. 1990. O vidovoi samostoyatel' nosti priozernoi polevki Microtus limnophilus, ee rodstvennykh svyazyakh s polevkoi-ekonomkoi M. oeconomus i rasprostranenii etikh vidov v Mongolii [Species independence of Microtus limnophilus, its relations with M. oeconomus and distribution of these species in Mongolia]. Zoologicheskii Zhurnal, 69 (4): 115 - 127 (in Russian)."]}
Study of the properties of Cosmic rays and solar X-Ray Flares by balloon borne experiments
Creators: name: Chakrabarti, S K
name: Bhowmick, D
name: Chakraborty, S
name: Palit, S
name: Mondal, S K
name: Bhattacharya, A
name: Midya, S
name: Chakrabarti, S
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Indian Centre for Space Physics is engaged in pioneering balloon borne experiments with typical payloads less than ~ 3.5kg. Low cost rubber balloons are used to fly them to a height of about 40km. In a double balloon system, the booster balloon lifts the orbiter balloon to its cruising altitude where data is taken for a longer period of time. In this Paper, we present our first scientific report on the variation of Cosmic Rays and muons with altitude and detection of several solar flares in X-rays between 20keV and 100keV. We found the altitude of the Pfotzer maximum at Tropic of Cancer for cosmic rays and muons and catch several solar flares in hard X-rays. We find that the hard X-ray (> 40keV) sky becomes very transparent above Pfotzer maximum. We find the flare spectrum to have a power-law distribution. From these studies, we infer that valuable scientific research could be carried out in near space using low cost balloon borne experiments. Published in Online version of Indian Journal of Physics.
description: 19 pages, 13 Figures and 1 Table
Large-rapidity ridge correlations from Color Glass Condensate
Creators: name: Zhang, Donghai
name: Zhao, Yeyin
name: Xu, Mingmei
name: Wu, Yuanfang
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Within the Color Glass Condensate (CGC) effective field theory, considering the violation of boost invariance of the rapidity distribution, we correct the normalization scheme of the longitudinal rapidity ridge correlations. After this correction, the large-rapidity ridge correlation rebounds after bottoming, consistent with the observed data from the CMS detector. It is also found that the correlation rebound appears around the sum of the saturation momentum of the projectile and target, and moves to larger rapidities at higher collision energies. These features directly result from the saturation and the quantum evolution of gluons within the framework of the CGC.
A Systematic Search for Trojan Planets in the Kepler data
Creators: name: Janson, Markus
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Trojans are circumstellar bodies that reside in characteristic 1:1 orbital resonances with planets. While all the trojans in our Solar System are small (< ~100 km), stable planet-size trojans may exist in extrasolar planetary systems, and the Kepler telescope constitutes a formidable tool to search for them. Here we report on a systematic search for extrasolar trojan companions to 2244 known Kepler Objects of Interest (KOIs), with epicyclic orbital characteristics similar to those of the Jovian trojan families. No convincing trojan candidates are found, despite a typical sensitivity down to Earth-size objects. This fact can however not be used to stringently exclude the existence of trojans in this size range, since stable trojans need not necessarily share the same orbital plane as the planet, and thus may not transit. Following this reasoning, we note that if Earth-sized trojans exist at all, they are almost certainly both present and in principle detectable in the full set of Kepler data, although a very substantial computational effort would be required to detect them. On the same token, we also note that some of the existing KOIs could in principle be trojans themselves, with a primary planet orbiting outside of the transiting plane. A few examples are given for which this is a readily testable scenario.
description: 15 pages, 8 figures, accepted for publication in ApJ
Can the Production Cross-Section Uncertainties Explain the Cosmic Fluorine Anomaly?
Creators: name: Zhao, Meng-Jie
name: Bi, Xiao-Jun
name: Fang, Kun
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: The stable secondary-to-primary flux ratios of cosmic rays (CRs), represented by the boron-to-carbon ratio (B/C), are the main probes of the Galactic CR propagation. However, the fluorine-to-silicon ratio (F/Si) predicted by the CR diffusion coefficient inferred from B/C is significantly higher than the latest measurement of AMS-02. This anomaly is commonly attributed to the uncertainties of the F production cross sections. In this work, we give a careful test to this interpretation. We consider four different cross-section parametric models. Each model is constrained by the latest cross-section data. We perform combined fits to the B/C, F/Si, and cross-section data with the same propagation framework. Two of the cross-section models have good overall goodness of fit with $χ^2/n_{d.o.f.}\sim1$. However, the goodness of fit of the cross-section part is poor with $χ^2_{\rm{cs}}/n_{\rm{cs}}\gtrsim2$ for these models. The best-fitted F production cross sections are systematically larger than the measurements, while the fitted cross sections for B production are systematically lower than the measurements. This indicates that the F anomaly can hardly be interpreted by neither the random errors of the cross-section measurements nor the differences between the existing cross-section models. We then propose that the spatially dependent diffusion model could help to explain B/C and F/Si consistently. In this model, the average diffusion coefficient of the Ne-Si group is expected to be larger than that of the C-O group.
description: 13 pages, 7 figures
Feasibility Study of Real-Time Planning for Stereotactic Radiosurgery
Creators: name: Zhang, Qinghui
name: Song, Yulin
name: Chan, Maria
name: Burman, Chandra
name: Yamada, Yoshiya
Publisher: name: arXiv
Year: 2013
Subjects: subject: Medical Physics (physics.med-ph)
subject: FOS: Physical sciences

description: Purpose: 3D rotational setup errors in radiotherapy are often ignored by most clinics due to inability to correct or simulate them accurately and efficiently. There are two types of rotation-related problems in a clinical setting. One is to assess the affected dose distribution in real-time if correction is not applied and the other one is to correct the rotational setup errors prior to the initiation of the treatment. Here, we present our analytical solutions to both problems.
description: 10 figures, 34 pages
Companilactobacillus baiquanensis BAIQUANENSIS 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
Companilactobacillus
Companilactobacillus baiquanensis

description: DESCRIPTIONOF COMPANILACTOBACILLUS BAIQUANENSIS COMB. NOV.
Companilactobacillus baiquanensis (bai.quan.eńsis. N.L. masc. adj. baiquanensis, pertaining to Baiquan, a county in the Heilongjiang province of China).
Basonym: Lactobacillusbaiquanensis Weiand Gu 2019, 3192 VP
The type strain grows at 15 and 37 but not at 45 °C; DL-lactic acid isproduced from ribose, hexoses andmaltose [118]. The genome size is 2.24 Mbp; the mol% G+C content is 34.4.
Isolatedfromfermented Chinesecabbage.
Thetypestrainis 184–8 T =LMG 31050 T =NCIMB 15152 T =CCM 8895 T =KCTC 21131 T.
Genome sequence accession number: RHOQ00000000.
16S RNA gene sequence accession number: MK110828.
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 2803, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536