cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Pelomys fallax
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys fallax

description: Pelomys fallax (Peters, 1852). Monatsb. Preuss. Akad. Wiss. Berlin, p. 275. TYPE LOCALITY: Mozambique, Caya Dist., Zambesi River and Boror, Licuare River. DISTRIBUTION: Kenya to Mozambique and Botswana; Angola. COMMENT: Includes luluae; subgenus Pelomys; see Misonne, 1974, Part 6:24. ISIS NUMBER: 5301410011051004001 as P. fallax. 5301410011051008001 as P. luluae.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Additional file 3 of The distribution of microbiomes and resistomes across farm environments in conventional and organic dairy herds in Pennsylvania
Creators: name: Pitta, Dipti W.
name: Nagaraju Indugu
name: Toth, John D.
name: Bender, Joseph S.
name: Baker, Linda D.
name: Hennessy, Meagan L.
name: Vecchiarelli, Bonnie
name: Aceto, Helen
name: Zhengxia Dou
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 3: Table S3. Results of PERMANOVA analysis for organic and conventional farms. R2 and P values given for farm type, sample type, and their interaction for microbiome and resistome.
Consequences of Weyl Consistency Conditions
Creators: name: Grinstein, Benjamin
name: Stergiou, Andreas
name: Stone, David
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The running of quantum field theories can be studied in detail with the use of a local renormalization group equation. The usual beta-function effects are easy to include, but by introducing spacetime-dependence of the various parameters of the theory one can efficiently incorporate renormalization effects of composite operators as well. An illustration of the power of these methods was presented by Osborn in the early 90s, who used consistency conditions following from the Abelian nature of the Weyl group to rederive Zamolodchikov's c-theorem in d=2 spacetime dimensions, and also to obtain a perturbative a-theorem in d=4. In this work we present an extension of Osborn's work to d=6 and to general even d. We compute the full set of Weyl consistency conditions, and we discover among them a candidate for an a-theorem in d=6, similar to the d=2,4 cases studied by Osborn. Additionally, we show that in any even spacetime dimension one finds a consistency condition that may serve as a generalization of the c-theorem, and that the associated candidate c-function involves the coefficient of the Euler term in the trace anomaly. Such a generalization hinges on proving the positivity of a certain "metric" in the space of couplings.
description: 19 pages, Mathematica file with consistency conditions included in submission. v2: Fixed typos
Pelomys harringtoni Thomas 1903
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys harringtoni

description: Pelomys harringtoni Thomas, 1903. Proc. Zool. Soc. Lond., 1902(2):313. TYPE LOCALITY: Ethiopia, Western Shoa, Kutai, Katchisa. DISTRIBUTION: Ethiopia. COMMENT: Subgenus Desmomys; see Misonne, 1974, Part 6:23. Reviewed by Dieterlen, 1974, Z. Saugetierk., 39:229-231. ISIS NUMBER: 5301410011051005001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
The Properties and Fate of the Galactic Center G2 Cloud
Creators: name: Shcherbakov, Roman V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The object G2 was recently discovered descending into the gravitational potential of the supermassive black hole (BH) Sgr A*. We test the photoionized cloud scenario, determine the cloud properties, and estimate the emission during the pericenter passage. The incident radiation is computed starting from the individual stars at the locations of G2. The radiative transfer calculations are conducted with CLOUDY code and $2011$ broadband and line luminosities are fitted. The spherically symmetric, tidally distorted, and magnetically arrested cloud shapes are tested with both the interstellar medium dust and $10$~nm graphite dust. The best-fitting magnetically arrested model has the initial density $n_{\rm init}=1.8\times10^5{\rm cm}^{-3}$, initial radius $R_{\rm init}=2.2\times10^{15}{\rm cm}=17 {\rm mas}$, mass $m_{\rm cloud}=4M_{\rm Earth}$, and dust relative abundance $A=0.072$. It provides a good fit to $2011$ data, is consistent with the luminosities in $2004$ and $2008$, and reaches an agreement with the observed size. We revise down the predicted radio and X-ray bow shock luminosities to be below the quiescent level of Sgr A*, which readily leads to non-detection in agreement to observations. The magnetic energy dissipation in the cloud at the pericenter coupled with more powerful irradiation may lead to an infrared source with an apparent magnitude $m_{L'}\approx13.0$. No shock into the cloud and no X-rays are expected from cloud squeezing by the ambient gas pressure. Larger than previously estimated cloud mass $m_{\rm cloud}=(4-20)M_{\rm Earth}$ may produce a higher accretion rate and a brighter state of Sgr A* as the debris descend onto the BH.
description: 12 pages, 5 figures, and 1 table, accepted to ApJ
THz radiation induced circular Hall effect in graphene
Creators: name: Candussio, S.
name: Bernreuter, S.
name: Rockinger, T.
name: Watanabe, K.
name: Taniguchi, T.
name: Eroms, Jonathan
name: Dmitriev, I. A.
name: Weiss, Dieter
name: Ganichev, Sergey
Publisher: name: Universität Regensburg
Year: 2022
Subjects: subject: 530 Physik

description: We report on the observation of the circular transversal terahertz photoconductivity in monolayer graphene supplied by a back gate. The photoconductivity response is caused by the free carrier absorption and reverses its sign upon switching the radiation helicity. The observed dc Hall effect manifests the time inversion symmetry breaking induced by circularly polarized terahertz radiation in the absence of a magnetic field. For low gate voltages, the photosignal is found to be proportional to the radiation intensity and can be ascribed to the alignment of electron momenta by the combined action of THz and static electric fields as well as by the dynamic heating and cooling of the electron gas. Strikingly, at high gate voltages, we observe that the linear-in-intensity Hall photoconductivity vanishes; the photoresponse at low intensities becomes superlinear and varies with the square of the radiation intensity. We attribute this behavior to the interplay of the second- and fourth-order effects in the radiation electric field which has not been addressed theoretically so far and requires additional studies.
A low-luminosity type-1 QSO sample: I. Overluminous host spheroidals or undermassive black holes?
Creators: name: Busch, Gerold
name: Zuther, Jens
name: Valencia-S., Mónica
name: Moser, Lydia
name: Fischer, Sebastian
name: Eckart, Andreas
name: Scharwächter, Julia
name: Gadotti, Dimitri A.
name: Wisotzki, Lutz
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Recognizing the properties of the host galaxies of quasi-stellar objects (QSOs) is essential to understand the suspected coevolution of central supermassive black holes (BHs) and their host galaxies. We selected a subsample of the Hamburg/ESO survey for bright UV-excess QSOs, containing only the 99 nearest QSOs with redshift z<=0.06, that are close enough to allow detailed structural analysis. From this "low-luminosity type-1 QSO sample", we observed 20 galaxies and performed aperture photometry and bulge-disk-bar-AGN-decomposition with BUDDA on near-infrared J, H, K band images. From the photometric decomposition of these 20 objects and visual inspection of images of another 26, we find that ~50% of the hosts are disk galaxies and most of them (86%) are barred. Stellar masses, calculated from parametric models based on inactive galaxy colors, range from 2x10^9 M_sun to 2x10^11 M_sun. Black hole masses measured from single epoch spectroscopy range from 1x10^6 M_sun to 5x10^8 M_sun. In comparison to higher luminosity QSO samples, LLQSOs tend to have lower stellar and BH masses. Also, in the effective radius vs. mean surface-brightness projection of the fundamental plane, they lie in the transition area between luminous QSOs and "normal" galaxies. This can be seen as further evidence that they can be pictured as a "bridge" between the local Seyfert population and luminous QSOs at higher redshift. Eleven low-luminosity QSOs for which we have reliable morphological decompositions and BH mass estimations lie below the published BH mass vs. bulge luminosity relations for inactive galaxies. This could be partially explained by bulges of active galaxies containing much younger stellar populations than bulges of inactive galaxies. Also, one could suspect that their BHs are undermassive. This might hint at the growth of the host spheroid to precede that of the BH.
description: 26 pages, 14 figures; accepted for publication in A&A
The Analysis of Factors Affecting Thai Flight Crews’ Safety Behaviors: Supervised Machine Learning Technique
Creators: name: Maneechaeye, Pattarachat
Publisher: name: figshare
Year: 2023
Subjects: Social psychology

description: There are few studies that focus on flight crew safety behaviors by using data science methodology. Therefore, this study aims to analyze factors, indicators and find components affecting Thai flight crews’ safety behaviors. This study also provides quantitative analysis by using data mining technique with supervised machine learning regression. According to an analysis of previous studies, there were 4 factors including safety climate, safety knowledge, safety motivation and safety compliance. First 3 factors would be analyzed as predictors and the last factor will be analyzed as label. Then, multiple regression model was developed by trainset. The result showed that all 3 predictors affected label significantly and the model prediction performance was moderate. Future studies should focus on longitudinal studies or comparative studies between civilian and government flight crew safety behaviors.
Constraining turbulence and conduction in the hot ICM through density perturbations
Creators: name: Gaspari, M.
name: Churazov, E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Using 3D high-resolution hydrodynamic simulations, tracking both electrons and ions, we study the effects of turbulence and conduction in the hot intracluster medium. We show how the power spectrum of the gas density perturbations can accurately constrain both processes. The characteristic amplitude of density perturbations is linearly related to the strength of turbulence, i.e. the 3D Mach number, as A(k)_max = 0.25 M. The slope of A(k) in turn reflects the level of conduction. In a non-conductive medium, subsonic stirring motions advect density with a similar nearly Kolmogorov cascade. Increasing conduction (via magnetic suppression f = 0.001-1) progressively steepens the spectrum towards the Burgers-like regime. The turbulent Prandtl number defines the dynamic similarity of the flow; at scales where Pt < 100, the spectrum develops a significant decay. The transition is gentle for highly suppressed conduction, f < 0.001, while sharp in the opposite regime. For strong conductivity (f > 0.1), Pt ~ 100 occurs on spatial scales larger than the injection scale. The velocity spectrum is instead not much affected by conduction. The f > 0.1 regime affects the appearance of X-ray images, in which Kelvin-Helmholtz and Rayleigh-Taylor rolls and filaments are washed out. In a stratified system, weak/strong turbulence induces higher isobaric/adiabatic fluctuations, while conduction forces both modes towards the intermediate isothermal regime. We provide a general analytic fit which is applied to new deep Chandra observations of Coma. The observed spectrum is best consistent with strongly suppressed effective isotropic conduction, f = 0.001, and mild subsonic turbulence, M = 0.45 (with injection at ~250 kpc). The low conductivity corroborates the survival of sharp features in the ICM (cold fronts, filaments, bubbles), and indicates that cooling flows may not be balanced by conduction.
description: Accepted by A&A - added several insights and comments; 17 pages, 11 figures
Superspace formulation and correlation functions of 3d superconformal field theories
Creators: name: Nizami, Amin A.
name: Sharma, Tarun
name: Umesh, V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study $3d$ SCFTs in the superspace formalism and discuss superfields and on-shell higher spin current multiplets in free $3d$ SCFTs with $\mathcal{N}= 1,2,3,4$ and $6$ superconformal symmetry. For $\mathcal{N}=1$ 3d SCFTs we determine the superconformal invariants in superspace needed for constructing 3-point functions of higher spin operators, find the non-linear relations between the invariants and consequently write down all the independent invariant structures, both parity even and odd, for various 3-point functions of higher spin operators.
description: typos corrected, references added. Accepted for publication in JHEP
INSEGURANÇA ALIMENTAR E NUTRICIONAL ENTRE ADULTOS COM DOENÇA FALCIFORME: UM PROTOCOLO DE REVISÃO DE ESCOPO
Creators: name: De Brito Sottero, Silvana Castro
name: Zannety Conceição Silva Do Nascimento Souza
name: Brito, Luana Santana
name: De Lima Borges, Carine
name: Pricila Oliveira De Araújo
name: Vale, Paulo Roberto Lima Falcão Do
name: Evanilda De Souza Santana Carvalho
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: Social and Behavioral Sciences
subject: human right to adequate food
subject: review scoping
subject: sickle cell
subject: sickle cell anemia
subject: nutrition
subject: insecurity food
subject: adults

description: Scoping Review to investigative the causes and manifestations of food and nutrition insecurity in adults with sickle cell disease. Method: scoping review of the developed following the recommendations proposed by the JBI manual. The search sources will be: SCIELO, LILACS (BVS), MEDLINE via PubMed, COCHRANE LIBRARY (Wiley), CINAHL (Ebsco), SCOPUS (Elsevier), Web of Science Core Collection (Clarivate Analytics), EMBASE (Elsevier), theses and dissertations will be analyzed in the databases of Google Scholar and Periodical Portal of the Coordination for the Improvement of Higher Education Personnel (CAPES, DART-E theses Europe; OATD - Open Access Theses and Dissertations, Canadian Theses and Dissertations Portal, Database of African Theses and Dissertations and Research (DATAD-R). Publications will be selected by two independent reviewers and disagreements will be analyzed by a third reviewer. For analysis of references (remove duplications, organization, inclusion and exclusion according to the adopted inclusion criteria) we will use EndNote Web 20 (Clarivate Analytics, PA, USA) and Rayyan Data will be extracted with the help of an instrument developed by the reviewers and the results will be presented through charts, flowcharts and narrative synthesis. This review will follow the recommendations proposed by the JBI methodology for the same and will use the Preferred Reporting Items for Scope Reviews (PRISMA-ScR) extension as a reporting guideline. A preliminary review was carried out in March 2023 using the terms Medical Subject Headings (MeSH): “nutrition” and “sickle cell disease” in the databases of PUBMED and CINAHL and PROSPERO, Pubmed and OSF for knowledge of the subject and identification of studies of scoping review with the same phenomenon, but no protocol with the present theme was found
Tractable Simulation of Error Correction with Honest Approximations to Realistic Fault Models
Creators: name: Puzzuoli, Daniel
name: Granade, Christopher
name: Haas, Holger
name: Criger, Ben
name: Magesan, Easwar
name: Cory, D. G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In previous work, we proposed a method for leveraging efficient classical simulation algorithms to aid in the analysis of large-scale fault tolerant circuits implemented on hypothetical quantum information processors. Here, we extend those results by numerically studying the efficacy of this proposal as a tool for understanding the performance of an error-correction gadget implemented with fault models derived from physical simulations. Our approach is to approximate the arbitrary error maps that arise from realistic physical models with errors that are amenable to a particular classical simulation algorithm in an "honest" way; that is, such that we do not underestimate the faults introduced by our physical models. In all cases, our approximations provide an "honest representation" of the performance of the circuit composed of the original errors. This numerical evidence supports the use of our method as a way to understand the feasibility of an implementation of quantum information processing given a characterization of the underlying physical processes in experimentally accessible examples.
description: 34 pages, 9 tables, 4 figures
The energy spectrum of gravitational waves in a loop quantum cosmological model
Creators: name: Morais, Joao
name: Bouhmadi-Lopez, Mariam
name: Henriques, Alfredo B.
Publisher: name: arXiv
Year: 2013
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We explore the consequences of loop quantum cosmology (inverse-volume corrections) in the spectrum of the gravitational waves using the method of the Bogoliubov coefficients. These corrections are taken into account at the background level of the theory as well as at the first order in the perturbations theory framework. We show that these corrections lead to an intense graviton production during the loop super-inflationary phase prior to the standard slow-roll era, which leave their imprints through new features on the energy spectrum of the gravitational waves as would be measured today, including a new maximum on the low frequency end of the spectrum.
description: 8 pages, 4 figures. RevTex4-1 Expanded version. Version accepted in PRD
Pelomys hopkinsi Hayman 1955
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys hopkinsi

description: Pelomys hopkinsi Hayman, 1955. Rev. Zool. Bot. Afr., 52:323. TYPE LOCALITY: Uganda, Rwamachuchu. DISTRIBUTION: Rwanda; Uganda. COMMENT: Subgenus Komemys; see Misonne, 1974, Part 6:23. ISIS NUMBER: 5301410011051006001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Constraint driven condensation in large fluctuations of linear statistics
Creators: name: Szavits-Nossan, Juraj
name: Evans, Martin R.
name: Majumdar, Satya N.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Condensation is the phenomenon whereby one of a sum of random variables contributes a finite fraction to the sum. It is manifested as an aggregation phenomenon in diverse physical systems such as coalescence in granular media, jamming in traffic and gelation in networks. We show here that the same condensation scenario, which normally happens only if the underlying probability distribution has tails heavier than exponential, can occur for light-tailed distributions in the presence of additional constraints. We demonstrate this phenomenon on the sample variance, whose probability distribution conditioned on the particular value of the sample mean undergoes a phase transition. The transition is manifested by a change in behavior of the large deviation rate function.
description: 5 pages, 3 figures
Pelomys isseli
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys isseli

description: Pelomys isseli (De Beaux, 1924). Ann. Mus. Civ. Stor. Nat. Genova, 51:207. TYPE LOCALITY: Uganda, Lake Victoria, Kome Isl. DISTRIBUTION: Lake Victoria islands of Kome, Bugala, and Bunyama (Uganda). COMMENT: Subgenus Komemys; see Misonne, 1974, Part 6:23. ISIS NUMBER: 5301410011051007001 as P. isselli (sic).
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Crystallization mechanism in melts of short n-alkane chains
Creators: name: Anwar, Muhammad
name: Turci, Francesco
name: Schilling, Tanja
Publisher: name: arXiv
Year: 2013
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We study crystallization in a model system for eicosane (C20) by means of molecular dynamics simulation and we identify the microscopic mechanisms of homogeneous crystal nucleation and growth. For the nucleation process, we observe that chains first align and then straighten. Then the local density increases and finally the monomer units become ordered positionally. The subsequent crystal growth process is characterized by a sliding-in motion of the chains. Chains preferably attach to the crystalline cluster with one end and then move along the stems of already crystallized chains towards their final position. This process is cooperative, i.e. neighboring chains tend to get attached in clusters rather than independently
title: Развивающая игрушка при работе с детьми с ограниченными возможностями здоровья
Creators: name: ELS IPR BOOKS
Publisher: name: Ай Пи Ар Медиа
Year: 2022

description: В издание включены учебно-методические материалы к дисциплине «Развивающая игрушка при работе с детьми с ограниченными возможностями здоровья», представлены результаты проектной и учебно-методической деятельности студенческого объединения АГГПУ им. В.М. Шукшина «Мастерская развивающей игрушки». Приводится описание проектов участников и победителей конкурсов муниципального, регионального и федерального уровней; представлен каталог самодельных развивающих игрушек. Подготовлено в соответствии с Федеральным государственным образовательным стандартом высшего образования. Предназначено для студентов, обучающихся по направлениям подготовки 44.03.05 «Педагогическое образование», 44.03.02 «Психолого-педагогическое образование», 37.03.01 «Психология», 39.03.02 «Социальная работа», изучающих дисциплину «Развивающая игрушка при работе с детьми с ограниченными возможностями здоровья». Также издание рекомендуется родителям, в том числе имеющим детей с ограниченными возможностями здоровья.
On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
Creators: name: Ishikawa, Takashi
name: Totani, Tomonori
name: Nishimichi, Takahiro
name: Takahashi, Ryuichi
name: Yoshida, Naoki
name: Tonegawa, Motonari
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Redshift space distortion (RSD) observed in galaxy redshift surveys is a powerful tool to test gravity theories on cosmological scales, but the systematic uncertainties must carefully be examined for future surveys with large statistics. Here we employ various analytic models of RSD and estimate the systematic errors on measurements of the structure growth-rate parameter, $fσ_8$, induced by non-linear effects and the halo bias with respect to the dark matter distribution, by using halo catalogues from 40 realisations of $3.4 \times 10^8$ comoving $h^{-3}$Mpc$^3$ cosmological N-body simulations. We consider hypothetical redshift surveys at redshifts z=0.5, 1.35 and 2, and different minimum halo mass thresholds in the range of $5.0 \times 10^{11}$ -- $2.0 \times 10^{13} h^{-1} M_\odot$. We find that the systematic error of $fσ_8$ is greatly reduced to ~5 per cent level, when a recently proposed analytical formula of RSD that takes into account the higher-order coupling between the density and velocity fields is adopted, with a scale-dependent parametric bias model. Dependence of the systematic error on the halo mass, the redshift, and the maximum wavenumber used in the analysis is discussed. We also find that the Wilson-Hilferty transformation is useful to improve the accuracy of likelihood analysis when only a small number of modes are available in power spectrum measurements.
description: 10 pages, 8 figures, 1 table, accepted for publication in MNRAS
Pelomys minor Cabrera and Ruxton 1926
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys minor

description: Pelomys minor Cabrera and Ruxton, 1926. Ann. Mag. Nat. Hist., ser. 9, 17:601. TYPE LOCALITY: Zaire, Luluabourg. DISTRIBUTION: N.E. Angola; N.W. Zambia; S. Zaire. COMMENT: Subgenus Pelomys; see Misonne, 1974, Part 6:23. ISIS NUMBER: 5301410011051009001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Spectrum and entanglement of phonons in quantum fluids of light
Creators: name: Busch, Xavier
name: Carusotto, Iacopo
name: Parentani, Renaud
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the quantum state of phonons propagating on top of a fluid of light coherently generated in a planar microcavity device by a quasi-resonant incident laser beam. In the steady-state under a monochromatic pump, because of the finite radiative lifetime of photons, a sizable incoherent population of low frequency phonons is predicted to appear. Their mean occupation number differs from a Planck distribution and is independent on the photon lifetime. When the photon fluid is subjected to a sudden change of its parameters, additional phonon pairs are created in the fluid with remarkable two-mode squeezing and entanglement properties. Schemes to assess non-separability of the phonon state from measurements of the correlation functions of the emitted light are discussed.
description: 16 pages, 9 figures. Version 2 contains an added description of experimental setup, as in journal version
Herbrand-Confluence
Creators: name: Hetzl, Stefan
name: Straßburger, Lutz
Publisher: name: arXiv
Year: 2013
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences

description: We consider cut-elimination in the sequent calculus for classical first-order logic. It is well known that this system, in its most general form, is neither confluent nor strongly normalizing. In this work we take a coarser (and mathematically more realistic) look at cut-free proofs. We analyze which witnesses they choose for which quantifiers, or in other words: we only consider the Herbrand-disjunction of a cut-free proof. Our main theorem is a confluence result for a natural class of proofs: all (possibly infinitely many) normal forms of the non-erasing reduction lead to the same Herbrand-disjunction.
description: 25 pages, final version, accepted for publication at LMCS, special issue for CSL 2012
The Bimodal Absorption System Imaging Campaign (BASIC). I. A Dual Population of Low-metallicity Absorbers at z < 1
Creators: name: Berg, Michelle A.
name: Lehner, Nicolas
name: Howk, J. Christopher
name: O’Meara, John M.
name: Schaye, Joop
name: Straka, Lorrie A.
name: Cooksey, Kathy L.
name: Tripp, Todd M.
name: Prochaska, J. Xavier
name: Oppenheimer, Benjamin D.
name: Johnson, Sean D.
name: Muzahid, Sowgat
name: Bordoloi, Rongmon
name: Werk, Jessica K.
name: Fox, Andrew J.
name: Katz, Neal
name: Wendt, Martin
name: Peeples, Molly S.
name: Ribaudo, Joseph
name: Tumlinson, Jason
Publisher: name: London : Institute of Physics Publ.
Year: 2023
Subjects: subject: star-forming galaxies
subject: Lyman-limit systems
subject: muse gas-flow
subject: characterizing circumgalatic gas
subject: Hubble-space-telelescope
subject: 520

description: The bimodal absorption system imaging campaign (BASIC) aims to characterize the galaxy environments of a sample of 36 H i-selected partial Lyman limit systems (pLLSs) and Lyman limit systems (LLSs) in 23 QSO fields at z ≲ 1. These pLLSs/LLSs provide a unique sample of absorbers with unbiased and well-constrained metallicities, allowing us to explore the origins of metal-rich and low-metallicity circumgalactic medium (CGM) at z < 1. Here we present Keck/KCWI and Very Large Telescope/MUSE observations of 11 of these QSO fields (19 pLLSs) that we combine with Hubble Space Telescope/Advanced Camera for Surveys imaging to identify and characterize the absorber-associated galaxies at 0.16 ≲ z ≲ 0.84. We find 23 unique absorber-associated galaxies, with an average of one associated galaxy per absorber. For seven absorbers, all with <10% solar metallicities, we find no associated galaxies with log M ⋆ ≳ 9.0 within ρ/R vir and ∣Δv∣/v esc ≤ 1.5 with respect to the absorber. We do not find any strong correlations between the metallicities or H i column densities of the gas and most of the galaxy properties, except for the stellar mass of the galaxies: the low-metallicity ([X/H] ≤ −1.4) systems have a probability of 0.39 − 0.15 + 0.16 for having a host galaxy with log M ⋆ ≥ 9.0 within ρ/R vir ≤ 1.5, while the higher metallicity absorbers have a probability of 0.78 − 0.13 + 0.10 . This implies metal-enriched pLLSs/LLSs at z < 1 are typically associated with the CGM of galaxies with log M ⋆ > 9.0 , whereas low-metallicity pLLSs/LLSs are found in more diverse locations, with one population arising in the CGM of galaxies and another more broadly distributed in overdense regions of the universe. Using absorbers not associated with galaxies, we estimate the unweighted geometric mean metallicity of the intergalactic medium to be [X/H] ≲ −2.1 at z < 1, which is lower than previously estimated.
Vevacious: A Tool For Finding The Global Minima Of One-Loop Effective Potentials With Many Scalars
Creators: name: Camargo-Molina, J. E.
name: O'Leary, B.
name: Porod, W.
name: Staub, F.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Several extensions of the Standard Model of particle physics contain additional scalars implying a more complex scalar potential compared to that of the Standard Model. In general these potentials allow for charge and/or color breaking minima besides the desired one with correctly broken SU(2)_L times U(1)_Y . Even if one assumes that a metastable local minimum is realized, one has to ensure that its lifetime exceeds that of our universe. We introduce a new program called Vevacious which takes a generic expression for a one-loop effective potential energy function and finds all the tree-level extrema, which are then used as the starting points for gradient-based minimization of the one-loop effective potential. The tunneling time from a given input vacuum to the deepest minimum, if different from the input vacuum, can be calculated. The parameter points are given as files in the SLHA format (though is not restricted to supersymmetric models), and new model files can be easily generated automatically by the Mathematica package SARAH. This code uses HOM4PS2 to find all the minima of the tree-level potential, PyMinuit to follow gradients to the minima of the one-loop potential, and CosmoTransitions to calculate tunneling times.
description: 44 pages, 1 figure, manual for publicly available software, v2 corresponds to version accepted for publication in EPJC [clearer explanation of scale dependence and region of validity, explicit mention that SLHA files should have blocks matching those expected by model files, updated references]
Pelomys rex
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Pelomys
Pelomys rex

description: Pelomys rex (Thomas, 1906). Ann. Mag. Nat. Hist., ser. 7, 18:304. TYPE LOCALITY: Ethiopia, Kaffa, Charada Forest, 6000 ft. (1829 m). DISTRIBUTION: Known only from the type locality. COMMENT: Position is very doubtful; only known from skin of type; see Dieterlen, 1974, Z. Saugetierk., 39:229-231. ISIS NUMBER: 5301410011051010001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 540, DOI: 10.5281/zenodo.7353037
Additional file 2 of Accelerated fetal growth in early pregnancy and risk of preterm birth: a prospective cohort study
Creators: name: Elenis, Evangelia
name: Anna-Karin Wikström
name: Simic, Marija
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 2: Supplementary Table. Growth in early pregnancy and multivariable risk of overall preterm birth and its subcategories (very preterm, moderate preterm, spontaneous preterm and medically induced preterm birth).
Scale-dependent CMB asymmetry from primordial configuration
Creators: name: Kohri, Kazunori
name: Lin, Chia-Min
name: Matsuda, Tomohiro
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We demonstrate that a topological defect can explain the hemispherical power asymmetry of the CMB. The first point is that a defect configuration, which already exists prior to inflation, can source asymmetry of the CMB. The second point is that modulation mechanisms, such as the curvaton and other modulation mechanisms, can explain scale-dependence of the asymmetry. Using a simple analysis of the $δN$ formalism, we show models in which scale-dependent hemispherical power asymmetry is explained by primordial configuration of a defect.
description: 14 pages, 3 figures, accepted for publication in JCAP
Phloeomys Waterhouse 1839
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Phloeomys

description: Phloeomys Waterhouse, 1839. Proc. Zool. Soc. Lond., 1839:107. REVIEWED BY: B. R. Stein (BRS). ISIS NUMBER: 5301410011052000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 541, DOI: 10.5281/zenodo.7353037
Geometric structure of percolation clusters
Creators: name: Xu, Xiao
name: Wang, Junfeng
name: Zhou, Zongzheng
name: Garoni, Timothy M.
name: Deng, Youjin
Publisher: name: arXiv
Year: 2013
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We investigate the geometric properties of percolation clusters, by studying square-lattice bond percolation on the torus. We show that the density of bridges and nonbridges both tend to 1/4 for large system sizes. Using Monte Carlo simulations, we study the probability that a given edge is not a bridge but has both its loop arcs in the same loop, and find that it is governed by the two-arm exponent. We then classify bridges into two types: branches and junctions. A bridge is a {\em branch} iff at least one of the two clusters produced by its deletion is a tree. Starting from a percolation configuration and deleting the branches results in a {\em leaf-free} configuration, while deleting all bridges produces a bridge-free configuration. Although branches account for $\approx 43%$ of all occupied bonds, we find that the fractal dimensions of the cluster size and hull length of leaf-free configurations are consistent with those for standard percolation configurations. By contrast, we find that the fractal dimensions of the cluster size and hull length of bridge-free configurations are respectively given by the backbone and external perimeter dimensions. We estimate the backbone fractal dimension to be $1.643\,36(10)$.
description: 8 pages, 7 figures
Phloeomys cumingi
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Phloeomys
Phloeomys cumingi

description: Phloeomys cumingi (Waterhouse, 1839). Proc. Zool. Soc. Lond., 1839:108. TYPE LOCALITY: Philippines, Luzon. DISTRIBUTION: Luzon (Philippines). COMMENT: May include pallidus; see Musser and Gordon, 1981, J. Mammal., 62:523. Includes elegans; see Ellerman, 1941, The Families and Genera of Living Rodents, vol. 2, p. 293. ISIS NUMBER: 5301410011052001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 541, DOI: 10.5281/zenodo.7353037
description: {"references": ["Musser, G. G., and L. K. Gordon. 1981. A new species of Crateromys (Muridae) from the Philippines. Journal of Mammalogy, 62: 513 - 525.", "Ellerman, J. R. 1941. The families and genera of living rodents. Vol. II. Family Muridae. British Museum (Natural History), London, 690 pp."]}
Additional file 1 of Quantitative structure-activity relationship, molecular docking, drug-likeness, and pharmacokinetic studies of some non-small cell lung cancer therapeutic agents
Creators: name: Ibrahim, Muhammad Tukur
name: Adamu Uzairu
name: Sani Uba
name: Shallangwa, Gideon Adamu
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Supplementary Table 1. The Ligand-Receptor, Binding affinity, Hydrogen bond, Bond distance, and other interaction for the remaining compounds. Supplementary Table 2. Drug-likeness properties for the compounds under investigation. Supplementary Table 3. ADME properties for the compounds under investigation.
Asymptotically Exact Scenario of Strong-Disorder Criticality in One-Dimensional Superfluids
Creators: name: Pollet, Lode
name: Prokof'ev, Nikolay V.
name: Svistunov, Boris V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We present a controlled rare-weak-link theory of the superfluid-to-Bose/Mott glass transition in one-dimensional disordered systems. The transition has Kosterlitz-Thouless critical properties but may occur at an arbitrary large value of the Luttinger parameter $K$. In contrast to the scenario by Altman {\it et al.} [Phys. Rev. B {\bf 81}, 174528 (2010)], the hydrodynamic description is valid under the correlation radius and defines criticality via the renormalization of microscopically weak links, along the lines of Kane and Fisher [Phys. Rev. Lett. {\bf 68}, 1220 (1992)]. The hallmark of the theory is the relation $K^{(c)}=1/ζ$ between the critical value of the Luttinger parameter at macroscopic scales and the microscopic (irrenormalizable) exponent $ζ$ describing the scaling $\propto 1/N^{1-ζ}$ for the strength of the weakest link among the $N/L \gg 1$ disorder realizations in a system of fixed mesoscopic size $L$.
description: 6 pages, 2 figures
Phloeomys pallidus Nehring 1890
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Phloeomys
Phloeomys pallidus

description: Phloeomys pallidus Nehring, 1890. Sitzb. Ges. Naturf. Fr. Berlin, p. 106. TYPE LOCALITY: Philippines, Luzon. DISTRIBUTION: Luzon (Philippines). ISIS NUMBER: 5301410011052002001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 5), pp. 504-560 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 541, DOI: 10.5281/zenodo.7353037
Additional file 1 of The novel E-subgroup pentatricopeptide repeat protein DEK55 is responsible for RNA editing at multiple sites and for the splicing of nad1 and nad4 in maize
Creators: name: Ren, Ru Chang
name: Yan, Xu Wei
name: Zhao, Ya Jie
name: Wei, Yi Ming
name: Xiaoduo Lu
name: Zang, Jie
name: Wu, Jia Wen
name: Zheng, Guang Ming
name: Ding, Xin Hua
name: Zhang, Xian Sheng
name: Zhao, Xiang Yu
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Fig. S1. Amino acid alignment of maize DEK55 with homologous PPR proteins of other plant species. Fig. S2. Original gel images corresponding to Fig. 5a. Fig. S3. Original gel images corresponding Fig. 5c-d. Fig. S4. Original gel images corresponding to Fig. 6a-b. Fig. S5. Original gel images corresponding to Fig. 7b. Table S1. Genetic analysis of the mutant kernels in the segregating ear. Table S2. Primers used in this study.
The Matryoshka Run: Eulerian Refinement Strategy to Study Statistics of Turbulence in Virialized Cosmic Structures
Creators: name: Miniati, Francesco
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the statistical properties of turbulence driven by structure formation in a massive merging galaxy cluster at z=0. The development of turbulence is ensured as the largest eddy turnover time is much shorter than the Hubble time independent of mass and redshift. We achieve a large dynamic range of spatial scales through a novel Eulerian refinement strategy where the cluster volume is refined with progressively finer uniform nested grids during gravitational collapse. This provides an unprecedented resolution of 7.3 h^{-1} kpc across the virial volume. The probability density functions of various velocity derived quantities exhibit the features characteristic of fully developed compressible turbulence observed in dedicated periodic-box simulations. Shocks generate only 60% of the total vorticity within \rvir/3 region and 40% beyond that. We compute second and third order, longitudinal and transverse, structure functions for both solenoidal and compressional components, in the cluster core, virial region and beyond. The structure functions exhibit a well defined inertial range. The injection scale is comparable to the virial radius but increases towards the outskirts. Within \rvir/3, the spectral slope of the solenoidal component is close to Kolmogorov's, but for the compressional component is substantially steeper and close to Burgers'; the flow is mostly solenoidal and statistically rigorously consistent with fully developed, homogeneous and isotropic turbulence. Small scale anisotropy appears due to numerical artifact. Towards the virial region, the flow becomes compressional, the structure functions flatter and modest genuine anisotropy appear. In comparison, mesh adaptivity based on Lagrangian refinement and the same finest resolution, leads to lack of turbulent power on small scale and excess thereof on large scales, and unreliable density weighted structure functions.
description: 20 pages, 17 figures, accepted to ApJ. 5 new pages and 6 new figures. Expanded discussion on vorticity generation, which is found to be only partially generated by shocks. Direct comparison with Lagrangian AMR and new section on numerical convergence of the results. Full resolution images (recommended) available at http://www.exp-astro.phys.ethz.ch/miniati/turbulence.pdf