cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Wide-range Prandtl/Schmidt number power spectrum of optical turbulence and its application to oceanic light propagation
Creators: name: Yao, Jin-Ren
name: Zhang, Hua-Jun
name: Wang, Ruo-Nan
name: Cai, Jian-Dong
name: Zhang, Yu
name: Korotkova, Olga
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Light influenced by the turbulent ocean can be fully characterized with the help of the power spectrum of the water's refractive index fluctuations, resulting from the combined effect of two scalars, temperature and salinity concentration advected by the velocity field. The Nikishovs' model [ Fluid Mech. Res. 27, 8298 (2000)] frequently used in the analysis of light evolution through the turbulent ocean channels is the linear combination of the temperature spectrum, the salinity spectrum and their co-spectrum, each being described by an approximate expression developed by Hill [ J. Fluid Mech. 88, 541562 (1978)] in the first of his four suggested models. The fourth of the Hill's models provides much more precise power spectrum than the first one expressed via a non-linear differential equation that does not have a closed-form solution. We develop an accurate analytic approximation to the fourth Hill's model valid for Prandtl/Schmidt numbers in the interval [3, 3000] and use it for the development of a more precise oceanic power spectrum. To illustrate the advantage of our model, we include numerical examples relating to the spherical wave scintillation index evolving in the underwater turbulent channels with different average temperatures, and, hence, different Prandtl numbers for temperature and different Schmidt numbers for salinity. Since our model is valid for a large range of Prandtl number (or/and Schmidt number), it can be readily adjusted to oceanic waters with seasonal or extreme average temperature and/or salinity or any other turbulent fluid with one or several advected quantities.
title: Contact: A Journal for Contemporary Music (1971-1988), No 4 (1972): Contact: A Journal for Contemporary Music
title: Contact: A Journal for Contemporary Music
titleType: AlternativeTitle
Creators: name: Contact: A Journal For Contemporary Music (1971-1988)
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: Editorial The Music of Peter Maxwell Davies, Part 1 Louis Armstrong’s Greatest Years, Part 2 A Broadening of the Smile Athens: The 4th Hellenic Week of Contemporary Music Record Reviews Review of 1971/11/18 and 1971/12/02 Concert at Town Hall, Birmingham. Humphrey Searle's 'Labyrinth' and Peter Dickinson's Organ Concerto played by the CBSO. Review of 1971/11/19 Concert at Barber Institute of Fine Arts (University of Birmingham) "Bell Piece '71" by Annea Lockwood and David Jones Review of 1972/01/04 Concert at Purcell Room, London. Concert of contemporary works by Mouth of Hermes. Review of 1972/01/17 Concert at The Roundhouse, London. BBC Symphony Orchestra, conducted by Pierre Boulez Review of 1972/01/20 Concert at BBC Pebble Mill Studio. BBC Invitation Concert. Review of 1972/01/29 Concert at Birmingham and Midland Institute. The Chasm: Judith Jones (soprano), Simon Desorgher (flute), Peter Lawson (piano) Review of 1972/02/06 Concert at Birmingham Arts Laboratory. A Day in the Life of the Arts Lab or A Performer's eye-view of a Cardew sound workshop. Review of 1972/02/12 Concert at Carr's Lane Church Centre. The New Music Chamber Orchestra conducted by Paul Venn
A nonunitary interpretation for a single vector leptoquark combined explanation to the $B$-decay anomalies
Creators: name: Hati, C.
name: Kriewald, J.
name: Orloff, J.
name: Teixeira, A. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In order to simultaneously account for both $R_{D^{(\ast)}}$ and $R_{K^{(\ast)}}$ anomalies in $B$-decays, we consider an extension of the Standard Model by a single vector leptoquark field, and study how one can achieve the required lepton flavour non-universality, starting from a priori universal gauge couplings. While the unitary quark-lepton mixing induced by $SU(2)_L$ breaking is insufficient, we find that effectively nonunitary mixings hold the key to simultaneously address the $R_{K^{(\ast)}}$ and $R_{D^{(\ast)}}$ anomalies. As an intermediate step towards various UV-complete models, we show that the mixings of charged leptons with additional vector-like heavy leptons successfully provide a nonunitary framework to explain $R_{K^{(\ast)}}$ and $R_{D^{(\ast)}}$. These realisations have a strong impact for electroweak precision observables and for flavour violating ones: isosinglet heavy lepton realisations are already excluded due to excessive contributions to lepton flavour violating $Z$-decays. Furthermore, in the near future, the expected progress in the sensitivity of charged lepton flavour violation experiments should allow to fully probe this class of vector leptoquark models.
description: 34 pages, 6 figures, v2 matches the published version (includes some new references and refinements in the analysis)
A new formation model for M32: A threshed early-type spiral?
Creators: name: Bekki, Kenji
name: Couch, Warrick J.
name: Drinkwater, Michael
name: Gregg, Michael D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The origin of the closest compact elliptical galaxy (cE) M32 is a longstanding problem of galaxy formation in the Local Group. Our N-body/SPH simulations suggest a new scenario in which the strong tidal field of M31 can transform a spiral galaxy into a compact elliptical. As a low luminosity spiral galaxy plunges into the central region of M31, most of the outer stellar and gaseous components of its disk are dramatically stripped due to M31's tidal field The central bulge component, on the other hand, is just weakly influenced by the tidal field owing to its compact configuration, and retains its morphology. M31's strong tidal field also induces rapid gas transfer to the central region, triggers a nuclear starburst, and consequently forms the central high density and more metal-rich stellar populations with relatively young ages. Thus, in this scenario, M32 was previously the bulge of a spiral tidally interacting with M31 several Gyr ago. Furthermore, we suggest cEs like M32 are rare, the result of both the rather narrow parameter space for tidal interactions which morphologically transform spirals into cEs and the very short time scale ($
description: 12 pages 4 figures, 2001, accepted by ApJL
Microcryptus muelleri KISS 1929
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Microcryptus
Microcryptus muelleri

description: Microcryptus muelleri KISS 1929
 Microcryptus mülleri KISS 1929: 114 f. – Holotypus (!) von SAWONIEWICZ (1984: 326) revidiert. Kiss hat den Typus irrtümlich als beschrieben. Der Typenfundort Heltau liegt bei Sibiu in Rumänien.
 G ü l t i g e r N a m e Apaeleticus inimicus (GRAVENHORST 1820) (SAWONIEWICZ, l.c.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 780, DOI: 10.5281/zenodo.5429664
Additional file 1 of Recruitability and effect of PEEP in SARS-Cov-2-associated acute respiratory distress syndrome
Creators: name: Beloncle, François M.
name: Pavlovsky, Bertrand
name: Desprez, Christophe
name: Fage, Nicolas
name: Olivier, Pierre-Yves
name: Asfar, Pierre
name: Richard, Jean-Christophe
name: Mercat, Alain
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Hematology
subject: Virology

description: Additional file 1: Figure S1. A. Study protocol. Positive end-expiratory pressure level (PEEP) was set to 15 cmH2O. Arterial and central venous blood gases were collected after a 10 min period and respiratory mechanics was assessed. Respiratory rate (RR) was decreased to 10/min and PEEP was decreased to 5 cmH2O (see below, Additional file 1: Figure S1B). After a 10 min period with PEEP 5 cmH2O, arterial and central venous blood gases were collected and respiratory mechanics was assessed. A low flow insufflation (5L/min) from PEEP 5 cmH2O was performed after a prolonged expiration. A visual analysis of the pressure–time curve on the ventilator screen allowed to identify a potential airway closure (and to measure a potential airway opening pressure) (see a representative tracing below). B. Measurement of the recruited lung volume. After decreasing RR to 10/min, expired tidal volume displayed by the ventilator at PEEP 15 cmH2O was noted. PEEP was abruptly decreased to 5 cmH2O and expired volume displayed by the ventilator immediately after the maneuver was noted. Plateau pressure at PEEP 5 cmH2O was measured. Initial RR was then resumed. C. Representative tracing of a low flow insufflation allowing to identify a complete airway closure and to measure the airway occlusion pressure (AOP).
title: Contact: A Journal for Contemporary Music (1971-1988), No 5 (1972): Contact: A Journal for Contemporary Music
title: Contact: A Journal for Contemporary Music
titleType: AlternativeTitle
Creators: name: Contact: A Journal For Contemporary Music (1971-1988)
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: Editorial The Third Act of Schoenberg’s Moses und Aron Jani Cristou Solo Music for the Double Bass Music from Silesia Musical Smørrebrød Interview with Zigmund Long Review of 1972/08/13 Concert at Roundhouse, London. HPSCHD: John Cage. Review of 1972/08 International Carnival of Experimental Sound Review of 1972/08/29 Concert at Albert Hall, London. London Sinfonietta conducted by David Atherton. Review of 1972/10/13 Concert at Barber Institute, University of Birmingham. Jane Manning, soprano, Peter Lawson, piano. 'Yellow Music': Forty Years On
Additional file 2 of Recruitability and effect of PEEP in SARS-Cov-2-associated acute respiratory distress syndrome
Creators: name: Beloncle, François M.
name: Pavlovsky, Bertrand
name: Desprez, Christophe
name: Fage, Nicolas
name: Olivier, Pierre-Yves
name: Asfar, Pierre
name: Richard, Jean-Christophe
name: Mercat, Alain
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Hematology
subject: Virology

description: Additional file 2: Figure S2. Distribution of recruited lung volume (VREC) within 36 h after intubation in the highly recruitable and poorly recruitable patients groups. *, p < 0.01. Horizontal lines represent median and interquartile range values.
БУХГАЛТЕРИЯДА РАҚАМЛАШТИРИШ: САМАРАДОРЛИКНИ ОШИРИШ ВА МОЛИЯВИЙ ҲИСОБОТЛАРДА ШАФФОФЛИКНИ ТАЪМИНЛАШ
Creators: name: Пулатова, Нозима
Publisher: name: Zenodo
Year: 2025

description: Мазкур мақолада бухгалтерияда рақамлаштириш жараёнларининг самарадорликка ва молиявий ҳисоботларда шаффофликка таъсири таҳлил қилинади. Бухгалтерияда рақамли технологиялардан фойдаланиш молиявий жараёнларни автоматлаштириш, хатоларни камайтириш, харажатларни қисқартириш ва фирибгарликнинг олдини олиш имконини беради. Шунингдек, мақолада рақамлаштиришнинг асосий афзалликлари, унга таъсир этувчи технологиялар, жорий этишдаги муаммолар ва уларни ҳал этиш йўллари муҳокама қилинади. Хусусан, булутли бухгалтерия, сунъий интеллект ва блокчейн технологияларининг бухгалтерия ҳисобида қўлланиши ва уларнинг аҳамияти ҳақида фикр юритилади. Муаллиф рақамлаштириш жараёнларини самарали жорий қилиш учун кадрлар тайёргарлиги, киберхавфсизлик чоралари ва автоматлаштирилган дастурий таъминот танлаш каби муҳим омилларга эътибор қаратиш лозимлигини таъкидлайди
title: Contact: A Journal for Contemporary Music (1971-1988), No 7 (1974): Contact: A Journal for Contemporary Music
title: Contact: A Journal for Contemporary Music
titleType: AlternativeTitle
Creators: name: Contact: A Journal For Contemporary Music (1971-1988)
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: Editorial Electronic Music Systems: Their History and Future Contemporary Japanese Music and Interview with Toru Takemitsu Experimental Music Catalogue: Eddie Prévost: Spirals and Richard Reason: Games for Musicians Experimental Music Catalogue: Keyboard Anthology Experimental Music Catalogue: Verbal Anthology Review of Pop Music and the Blues by Richard Middleton Review of Stockhausen, Life and Work by Karl H. Worner Review of 1974/05/06 Concert at The Round House, London. Concert of The Music of Toru Takemitsu Review of 1973/09 Music Nova in Glasgow Review of October 14th Concert at Young Vic, London. Bertram Turetzky, with Nancy Turetzky and Barry Guy.
title: Resilience of Coastal Freshwater Wetland Vegetation to Climate Change
Creators: name: Grieger, Rebekah
Publisher: name: Griffith University
Year: 2021
Subjects: subject: Coastal freshwater wetlands (CFWs)
subject: climate change
subject: southeast Queensland
subject: soil
subject: vegetation patterns
subject: hydrology and salinity
subject: species extirpation
subject: wetland

description: Coastal wetlands are globally important ecosystems, valued for their provision of habitat, storm mitigation, water quality improvement, and carbon sequestration. Coastal wetlands are also one of the ecosystems most likely to be impacted by projected changes in climate, particularly changes associated with sea level rise, altered rainfall patterns, and changes to storm patterns and severity. Coastal freshwater wetlands (CFWs) are amongst the most understudied group of coastal wetlands and are characterised by freshwater dominated hydrology but can also experience periods of salinity associated with their proximity to the coast (i.e. as the result of storm surge and spring high tides). CFWs commonly occur as the most landward of coastal wetlands and many adjoin urban development, exposing them to anthropogenic impacts (nutrient enrichment, clearing, hydrology alteration). This position in the coastal landscape makes CFWs highly susceptible to salinity stress, particularly climate change induced sea level rise. Research investigating CFWs, their ecology, and responses to climate change threats, is greatly lacking, particularly for areas outside the United States of America (USA). This thesis investigates the resilience of CFWs to climate change and aims to address significant knowledge gaps by investigating: 1) the current knowledge of CFW responses to projected climate change globally; 2) the structure and composition of CFW vegetation in southeast Queensland and exploring drivers of vegetation patterns; 3) the role of soil seed banks in vegetation resilience for CFWs in southeast Queensland through contributions to vegetation dynamics; and 4) the regenerative potential and responses of CFW vegetation communities to altered hydrology and salinity regimes simulating sea level rise. [...]
Direct Detection Anomalies in light of $Gaia$ Data
Creators: name: Buckley, Matthew R.
name: Mohlabeng, Gopolang
name: Murphy, Christopher W.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Measurements from the Gaia satellite have greatly increased our knowledge of the dark matter velocity distributions in the Solar neighborhood. There is evidence for multiple cold structures nearby, including a high-velocity stream counterrotating relative to the Sun. This stream could significantly alter the spectrum of recoil energies and increase the annual modulation of dark matter in direct detection experiments such as DAMA/Libra. We reanalyze the experimental limits from Xenon1T, CDMSlite, PICO-60 and COSINE-100, and compare them to the results of the DAMA/Libra experiment. While we find that this new component of the dark matter velocity distribution can greatly improve the fit to the DAMA/Libra data, both spin-independent and spin-dependent interpretations of the DAMA/Libra signal with elastic and inelastic scattering continue to be ruled out by the null results of other experiments, in particular Xenon1T.
description: 23 pages, 17 figures, updated references. Version published in PRD
Association Between Intravenous Fluid Bolus and Biomarker Trajectory During Prehospital Care
Creators: name: Brant, Emily B.
name: Kennedy, Jason
name: Martin-Gill, Christian
name: Jackson, Vanessa
name: Palmer, Octavia M. Peck
name: Callaway, Clifton W.
name: Kahn, Jeremy M.
name: Yealy, Donald M.
name: Angus, Derek C.
name: Seymour, Christopher W.
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Background: Patients with acute illness who receive intravenous (IV) fluids prior to hospital arrival may have a lower in-hospital mortality. To better understand whether this is a direct treatment effect or epiphenomenon of downstream care, we tested the association between a prehospital fluid bolus and the change in inflammatory cytokines measured at prehospital and emergency department timepoints in a sample of non-trauma, non-cardiac arrest patients at risk for critical illness. Methods: In a prospective cohort study, we screened 4,013 non-trauma, non-cardiac arrest encounters transported by City of Pittsburgh Emergency Medical Services (EMS) to 2 hospitals from August 2013 to February 2014. In 345 patients, we measured prehospital biomarkers (IL-6, IL-10, and TNF) at 2 time points: the time of prehospital IV access placement by EMS and at ED arrival. We determined the relative change for marker X as: ([XED – XEMS]/XEMS). We determined the risk-adjusted association between prehospital IV fluid bolus and relative change for each marker using multivariable linear regression. Results: Among 345 patients, 88 (26%) received a prehospital IV fluid bolus and 257 (74%) did not. Compared to patients who did not receive prehospital fluids, median prehospital IL-6 was greater initially in subjects receiving a prehospital IV fluid bolus (22.3 [IQR 6.4–113] vs. 11.5 [IQR 5.5–47.6]). Prehospital IL-10 and TNF were similar in both groups (IL-10: 3.5 [IQR 2.2–25.6] vs. 3.0 [IQR 1.9–9.0]; TNF: 7.5 [IQR 6.4–10.4] vs. 6.9 [IQR 6.0–8.3]). After adjustment for demographics, illness severity, and prehospital transport time, we observed a relative decrease in IL-6 at hospital arrival in those receiving a prehospital fluid bolus (adjusted β = −10.0, 95% CI: −19.4, −0.6, p = 0.04), but we did not detect a significant change in IL-10 (p = 0.34) or TNF (p = 0.53). Conclusions: Among non-trauma, non-cardiac arrest patients at risk for critical illness, a prehospital IV fluid bolus was associated with a relative decrease in IL-6, but not IL-10 or TNF.
Band-selective clean- and dirty-limit superconductivity with nodeless gaps in the bilayer iron-based superconductor CsCa$_2$Fe$_4$As$_4$F$_2$
Creators: name: Xu, B.
name: Wang, Z. C.
name: Sheveleva, E.
name: Lyzwa, F.
name: Marsik, P.
name: Cao, G. H.
name: Bernhard, C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The optical properties of the new iron-based superconductor CsCa$_2$Fe$_4$As$_4$F$_2$ with $T_c \sim 29$~K have been determined. In the normal state a good description of the low-frequency response is obtained with a superposition of two Drude components of which one has a very low scattering rate (narrow Drude-peak) and the other a rather large one (broad Drude-peak). Well below $T_c \sim 29$~K, a pronounced gap feature is observed which involves a complete suppression of the optical conductivity below $\sim$ 110~cm$^{-1}$ and thus is characteristic of a nodeless superconducting state. The optical response of the broad Drude-component can be described with a dirty-limit Mattis-Bardeen-type response with a single isotropic gap of $2Δ\simeq 14$~meV. To the contrary, the response of the narrow Drude-component is in the ultra-clean-limit and its entire spectral weight is transferred to the zero-frequency $δ(ω)$ function that accounts for the loss-free response of the condensate. These observations provide clear evidence for a band-selective coexistence of clean- and dirty-limit superconductivity with nodeless gaps in CsCa$_2$Fe$_4$As$_4$F$_2$.
description: 5 pages, 4 figures
Fine-structure diagnostics of neutral carbon toward HE 0515-4414
Creators: name: Quast, Ralf
name: Baade, Robert
name: Reimers, Dieter
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: New high-resolution high signal-to-noise spectra of the $z=1.15$ damped Lyman $α$ (DLA) system toward the quasi-stellar object HE 0515-4414 reveal absorption lines of the multiplets 2 and 3 in \ion{C}{i}. The resonance lines are seen in two components with total column densities of $\log N=13.79\pm0.01$ and $\log N=13.36\pm0.01$, respectively. The comparision of theoretical calculations of the relative fine-structure population with the ratios of the observed column densities suggests that the \ion{C}{i} absorbing medium is either very dense or exposed to very intense UV radiation. The upper limit on the local UV energy density is 100 times the galactic UV energy density, while the upper limit on the \ion{H}{i} number density is 110 cm$^{-3}$. The excitation temperatures of the ground state fine-structure levels of $T=15.7$ and $T=11.1$ K, respectively, are consistent with the temperature-redshift relation predicted by the standard Friedmann cosmology. The cosmic microwave background radiation (CMBR) is only a minor source of the observed fine-structure excitation.
description: 5 pages, 5 figures, uses A&A macro package, gzipped tar archive, accepted by A&A
Chalicotherium Kaup 1833
Creators: name: Anquetin, Jérémy
name: Antoine, Pierre-Olivier
name: Tassy, Pascal
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Perissodactyla
Chalicotheriidae
Chalicotherium

description: CHALICOTHERIUM KAUP, 1833 A
 Macrotherium Pictet, 1844
 Diagnosis: Amoung Chalicotheriinae (height of the mandibular corpus increasing posteriorly; protoloph of P 3 and P 4 lost; protoloph not reaching the protocone on molars; upper molars subsquare), Chalicotherium is diagnosed by two unambiguous synapomorphies (see cladistic analysis): occipital condyles elongated vertically; postfossette more pinched on M 3 than on other molars.
 The cranial anatomy of Chalicotherium is far less derived than that of Anisodon and retains numerous plesiomorphic traits, such as: a rather long snout and skull; parallel (in ventral view) and straight (in lateral view) upper tooth rows; lack of a lacrimal tubercle; no groove between the ventral border of the zygomatic arch and M 3; postorbital process on the jugal absent; tent-shaped braincase (not swollen); ventrally orientated paroccipital process; upper part of the occiput projected posteriorly; retromolar space present on both the maxilla and mandible; tympanic bulla not extended anterior to the postglenoid process; angulus mandibulae straight (not expanded ventrally); metacone at least as lingual as the paracone on M 1 and M 2; external walls of the metacone and metastyle subperpendicular to the mesiodistal lengthening on M 3; strong ‘metastylid’ on lower molars.
 Type species: Chalicotherium goldfussi Kaup, 1833a.
 Included species: Chalicotherium brevirostris.
description: Published as part of Anquetin, Jérémy, Antoine, Pierre-Olivier & Tassy, Pascal, 2007, Middle Miocene Chalicotheriinae (Mammalia, Perissodactyla) from France, with a discussion on chalicotheriine phylogeny, pp. 577-608 in Zoological Journal of the Linnean Society 151 (3) on page 587, DOI: 10.1111/j.1096-3642.2007.00327.x, http://zenodo.org/record/5428275
MOESM1 of T2STIR preparation for single-shot cardiovascular magnetic resonance myocardial edema imaging
Creators: name: Zhu, Yanjie
name: Yang, Dan
name: Zou, Lixian
name: Chen, Yucheng
name: Liu, Xin
name: Chung, Yiu-Cho
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 1. 1. The formulas for Signal difference, SNR, CNR and contrast ratio. 2. The extent of edema identified using different methods. 3. The effect of arrhythmia on T2 maps.
On the self-consistency of evolutionary synthesis models
Creators: name: Cervino, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Evolutionary synthesis models have been used to study the physical properties of unresolved populations in a wide range of scenarios. Unfortunately, their self-consistency are difficult to test and there are some theoretical open questions without an answer: (1) The change of the homology relations assumed in the computation of isochrones due to the effect of stellar winds (or rotation) and the discontinuities in the stellar evolution are not considered. (2) There is no a consensus about how the isochrones must be integrated. (3) The discreteness of the stellar populations (that produce an intrinsic statistical dispersion) usually are not taken into account, and model results are interpreted in a deterministic way instead a statistical one... The objective of this contribution is to present some inconsistencies in the computation and some cautions in the application of the results of such codes.
description: 4 pages, to appear in "The Evolution of Galaxies III. From Simple Approaches to Self-consistent Models" G.Hensler et al. (eds.)
Basic Approach to the Problem of Cosmological Constant and Dark Energy
Creators: name: Carmeli, Moshe
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Most of the calculations done to obtain the value of the cosmological constant use methods of quantum gravity, a theory that has not been established as yet, and a variety of results are usually obtained. The numerical value of the cosmological constant is then supposed to be inserted in the Einstein field equations, hence the evolution of the Universe will depend on the calculated value. Here we present a fundamental approach to the problem. The theory presented here uses a Riemannian four-dimensional presentation of gravitation in which the coordinates are those of Hubble, i.e. distances and velocity rather than space and time. We solve these field equations and show that there are three possibilities for the Universe to expand but only the accelerating Universe is possible. From there we calculate the cosmological constant and find that its value is given by 1.934x10^(-35)s^-2. This value is in excellent agreement with the measurements obtained by the High-Z Supernova Team and the Supernova Cosmology Project. Finally it is shown that the three-dimensional space of the Universe is Euclidean, as the Boomerang experiment shows.
description: 19 pages LaTeX, 6 figures in gzipped "eps" files, paper presented at COSMO-01, to be published in the Proceedings
Copelatus caelatipennis subsp. princeps Young 1963
Creators: name: Megna, Yoandri S.
name: Epler, John H.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dytiscidae
Copelatus
Copelatus caelatipennis
Copelatus caelatipennis princeps young, 1963

description: Copelatus caelatipennis princeps Young, 1963
(Fig. 26)
 Copelatus caelatipennis: SCHAEFFER (1908: 17), LENG & MUTCHLER (1918: 87), BLATCHLEY (1919: 313), YOUNG (1954: 107, 1953b: 5).
 Copelatus caelatipennis princeps Young, 1963: 59.
 Copelatus caelatipennis princeps: SPANGLER (1981: 153), EPLER (1996: 3.33, 2010: 5.45), LARSON et al. (2000: 48), NILSSON (2001: 59), PECK (2005: 44).
 Type locality. USA, Florida, Dade Co., Miami River.
 Material examined. CUBA: ISLA DE LA JUVENTUD: Punta del Este, 22.v.2006, Y.S. Megna leg., 7 exs.; Cerro Caudal, 22.v.2006, Y. S. Megna leg., 9 exs. GUANTÁNAMO: Cabacú, 16.ii.2010, R. Correa leg., 7 exs., 21.ii.2010, R. Correa leg., 3 exs.; Jobo Dulce, 11.ii.2010, R. Correa leg., 3 exs., 18.ii.2010, R. Correa leg., 12 exs., 20.ii.2010, R. Correa leg., 12 exs.; La Alegría, 10.ii.2010, R. Correa leg., 5 exs., 13.ii.2010, R. Correa leg., 9 exs., 15.ii.2010, R. Correa leg., 1 ex., 19.ii.2010, R. Correa leg., 12 exs.; El Yunque, 29.i.2010, R. Correa leg., 1 ex.
 Diagnosis. Corresponding to C. caelatipennis angustatus in all diagnostic characters mentioned under that subspecies, but may be separated from it by the short, uniformly distributed strioles on the pronotal disc in both sexes. In addition, females of C. c. princeps often bear short strioles also on the basal third of the elytra.
 Ecology. According to YOUNG (1963), C. caelatipennis princeps usually occurs only in clear, unpolluted water in the USA. In Cuba, the species was collected in temporary lentic environments with turbid water and muddy bottom, from lowlands up to 50 m a.s.l.
 Distribution. In the USA known from New Jersey and Illinois to Florida and Texas (LARSON et al. 2000). In Cuba, Copelatus caelatipennis princeps is recorded from both western (Isla de la Juventud) and eastern parts of the country (Guantánamo province) (Fig. 26). This is the first record of this subspecies from the West Indies.
description: Published as part of Megna, Yoandri S. & Epler, John H., 2012, A review of Copelatus from Cuba, with the description of two new species (Coleoptera: Dytiscidae: Copelatinae), pp. 383-410 in Acta Entomologica Musei Nationalis Pragae 52 (2) on pages 390-391, DOI: 10.5281/zenodo.5331014
Thermal transport in long-range interacting Fermi-Pasta-Ulam chains
Creators: name: Wang, Jianjin
name: Dmitriev, Sergey V.
name: Xiong, Daxing
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Studies of thermal transport in long-range (LR)interacting systems are currently particularly challenging. The main difficulties lie in the choice of boundary conditions and the definition of heat current when driving systems in an out-of-equilibrium state by the usual thermal reservoirs. Here, by employing a reverse type of thermal baths that can overcome such difficulties, we reveal the intrinsic features of thermal transport underlying a LR interacting Fermi-Pasta-Ulam chain. We find that under an appropriate range value of LR exponent $σ=2$, while a \emph{nonballistic} power-law length ($L$) divergence of thermal conductivity $κ$, i.e., $κ\sim L^α$ still persists, its scaling exponent $α\simeq 0.7$ can be much larger than the usual predictions in short-range interacting systems. The underlying mechanism is related to the system's new heat diffusion process, weaker nonintegrability and peculiar dynamics of traveling discrete breathers. Our results shed light on searching for low-dimensional materials supporting higher thermal conductivity by involving appropriate LR interactions.
description: 7 pages, 7 figures. The manuscript has been published in Phys. Rev. Research and now has been updated to the published version
Critical metrics for the determinant of the Laplacian in odd dimensions
Creators: name: Okikiolu, K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: Let M be a closed compact n-dimensional manifold with n odd. We calculate the first and second variations of the zeta-regularized determinants det^\primeΛand det L as the metric on M varies, where Δdenotes the Laplacian on functions and L denotes the conformal Laplacian. We see that the behavior of these functionals denotes the conformal Laplacian. We see that the behavior of these functionals depends on the dimension. Indeed, every critical metric for (-1)^{(n-1)/2}det^\primeΛor (-1)^{(n-1}/2}| det L| has finite index. Consequently there are no local maxima if n=4m+1 and no local minima if n=4m+3. We show that the standard 3-sphere is a local maximum for det^\primeΛwhile the standard (4m-3)-sphere with m=1,2,...,4, is a saddle point. By contrast, for all odd n, the standard n-sphere is a local extremal for det L. An important tool in our work is the canonical trace on odd class operators in odd dimensions. This trace is related to the determinant by the formula det Q = TR log Q, and we prove some basic results on how to calculate the trace.
description: 61 pages, published version
Energy dependence study of directed flow in Au+Au collisions using an improved coalescence in AMPT model
Creators: name: Nayak, Kishora
name: Shi, Shusu
name: Xu, Nu
name: Lin, Zi-Wei
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The rapidity-odd component of directed flow ($v_{1}$) of identified hardons ($π^{\pm}$, $K^{\pm}$, $K^{0}_{S}$, $p$, $\bar{p}$, $ϕ$, $Ξ$, $\barΞ$, $Λ$, $\barΛ$) and partons ($u$, $\bar{u}$, $d$, $\bar{d}$, $s$, $\bar{s}$) in Au+Au collisions at various beam energies ($\sqrt{s_{\rm NN}}$ = 7.7, 11.5, 14.5, 19.6, 27, 39, 54.4, 62.4, 200 GeV) using a multi-phase transport model is analyzed. A data driven approach (inspired from the experimental analysis) is performed here to distinguish the transported and produced quarks which are found to have different directed flow values at various collision beam energies. The coalescence sum rule (Number of Constituent Quark scaling) violation is observed at lower energies where hadronic matters dominate. The strange quark ($s$) and $ϕ$ meson slope (d$v_{1}$/d$y$) show a double sign change around 14.5 GeV, unlike other partons and hadrons. It suggests that strange quark is more sensitive to the softening of Equation of State (EoS).
description: 9 pages, 8 figures, submitted to Phys. Rev. C
title: Contemporary and Historical Influences on the Taxonomy and Distributions of Cherax Species in South Eastern Quensland, Australia
Creators: name: Bentley, Andrew I
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Freshwater crayfish
subject: Decapod crustaceans
subject: Genus Cherax
subject: Australian Cherax, South-East Queensland

description: Freshwater crayfish are a highly diverse group of decapod crustaceans that are distributed across all but the Indian and Antarctic continents. Their broad distribution suggests a strong ability to disperse and adapt to a wide range of habitats and environmental niches. In particular, freshwater crayfish have been discovered in caves, burrows, streams, lakes and sometimes even terrestrial habitats. This dispersed distribution across a range of habitats is particularly evident for the genus Cherax, with at least 47 species identified from throughout Australia. With some species highly diverse and others widely distributed, it is unclear what effect geographic, behavioural and ecological isolation has had on the current biogeographic structure of Australian Cherax. By investigating variation across a nested series of scales, the primary aim of this study was to distinguish the historical and contemporary drivers that may have caused and maintained the high level of biodiversity observed in Australian and more specifically South-East Queensland (SEQ) Cherax.
Association Between Intravenous Fluid Bolus and Biomarker Trajectory During Prehospital Care
Creators: name: Brant, Emily B.
name: Kennedy, Jason
name: Martin-Gill, Christian
name: Jackson, Vanessa
name: Palmer, Octavia M. Peck
name: Callaway, Clifton W.
name: Kahn, Jeremy M.
name: Yealy, Donald M.
name: Angus, Derek C.
name: Seymour, Christopher W.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Background: Patients with acute illness who receive intravenous (IV) fluids prior to hospital arrival may have a lower in-hospital mortality. To better understand whether this is a direct treatment effect or epiphenomenon of downstream care, we tested the association between a prehospital fluid bolus and the change in inflammatory cytokines measured at prehospital and emergency department timepoints in a sample of non-trauma, non-cardiac arrest patients at risk for critical illness. Methods: In a prospective cohort study, we screened 4,013 non-trauma, non-cardiac arrest encounters transported by City of Pittsburgh Emergency Medical Services (EMS) to 2 hospitals from August 2013 to February 2014. In 345 patients, we measured prehospital biomarkers (IL-6, IL-10, and TNF) at 2 time points: the time of prehospital IV access placement by EMS and at ED arrival. We determined the relative change for marker X as: ([XED – XEMS]/XEMS). We determined the risk-adjusted association between prehospital IV fluid bolus and relative change for each marker using multivariable linear regression. Results: Among 345 patients, 88 (26%) received a prehospital IV fluid bolus and 257 (74%) did not. Compared to patients who did not receive prehospital fluids, median prehospital IL-6 was greater initially in subjects receiving a prehospital IV fluid bolus (22.3 [IQR 6.4–113] vs. 11.5 [IQR 5.5–47.6]). Prehospital IL-10 and TNF were similar in both groups (IL-10: 3.5 [IQR 2.2–25.6] vs. 3.0 [IQR 1.9–9.0]; TNF: 7.5 [IQR 6.4–10.4] vs. 6.9 [IQR 6.0–8.3]). After adjustment for demographics, illness severity, and prehospital transport time, we observed a relative decrease in IL-6 at hospital arrival in those receiving a prehospital fluid bolus (adjusted β = −10.0, 95% CI: −19.4, −0.6, p = 0.04), but we did not detect a significant change in IL-10 (p = 0.34) or TNF (p = 0.53). Conclusions: Among non-trauma, non-cardiac arrest patients at risk for critical illness, a prehospital IV fluid bolus was associated with a relative decrease in IL-6, but not IL-10 or TNF.
Potential formation sites of super star clusters in ultra-luminous infrared galaxies
Creators: name: Bekki, Kenji
name: Couch, Warrick J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent observational results on high spatial resolution images of ultra-luminous infrared galaxies (ULIGs) have revealed very luminous, young, compact, and heavily obscured super star clusters in their central regions, suggested to be formed by gas-rich major mergers. By using stellar and gaseous numerical simulations of galaxy mergers, we firstly demonstrate that the central regions of ULIGs are the most promising formation sites of super star clusters owing to the rather high gaseous pressure of the interstellar medium. Based on simple analytical arguments, we secondly discuss the possibility that super star clusters in an ULIG can be efficiently transferred into the nuclear region owing to dynamical friction and consequently merge with one another to form a single compact stellar nucleus with a seed massive black hole. We thus suggest that multiple merging between super star clusters formed by nuclear starbursts in the central regions of ULIGs can result in the formation of massive black holes.
description: 12 pages 4 figures, 2001, accepted by ApJL
A Global Jet/Circulation Model for Young Stars
Creators: name: Lery, T.
name: Henriksen, R. N.
name: Fiege, J. D.
name: Ray, T. P.
name: Frank, A.
name: Bacciotti, F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Powerful, highly collimated jets, surrounded by bipolar molecular outflows, are commonly observed near Young Stellar Objects (YSOs). In the usual theoretical picture of star formation, a jet is ejected from a magnetized accretion disk, with a molecular outflow being driven either by the jet or by a wider wind coming from the disk. Here, we propose an alternative global model for the flows surrounding YSOs. In addition to a central accretion-ejection engine driving the jet, the molecular outflow is powered by the infalling matter and follows a circulation pattern around the central object without necessarily being entrained by a jet. It is shown that the model produces a heated pressure-driven outflow with magneto-centrifugal acceleration and collimation. We report solutions for the three different parts of this self-similar model, i.e. the jet, the infalling envelope and the circulating matter that eventually forms the molecular outflow. This new picture of the accretion/outflow phase provides a possible explanation for several observed properties of YSO outflows. The most relevant ones are the presence of high mass molecular outflows around massive protostars, and a realistic fraction (typically 0.1) of the accretion flow that goes into the jet.
description: accepted for publication in Astronomy and Astrophysics
NFDI4Objects TWG - Community-Standards for modelling fuzziness & wobbliness in research data using Semantic Web technologies and formalisms (FuzzyWobblySW)
Creators: name: Thiery, Florian
name: Tolle, Karsten
Publisher: name: Squirrel Papers, via Zenodo
Year: 2025

description: Bei der Erforschung von Objekten spielen sowohl exakte als auch interpretierende Aussagen eine zentrale Rolle. Letztere können durch “hidden assumptions” der Autor*innen, unvollständige Objekterhaltung oder ungenaue technische Konzepte stark beeinflusst werden. Die einheitliche Modellierung der damit verbundenen “fuzziness and wobbliness” (z. B. uncertainty, vagueness, accuracy and precision) in Forschungsdaten ist eine Herausforderung, da in den Forschungsdomänen unterschiedliche Ansätze entwickelt oder implementiert werden. Wichtig dabei ist zuerst die Definition von “fuzziness and wobbliness” (Whitepaper #1). Ziel der TWG ist es, bestehende graphbasierte (RDF-)Modellierungsansätze (Whitepaper #2), Software und Skripte (Whitepaper #3) für “fuzziness and wobbliness” in Forschungsdaten zu sammeln, zu bewerten und zu erweitern. Auf diese Weise sollen gemeinsame Schnittstellen identifiziert werden, die den Übergang von einem domainspezischen/forschungsdisziplinspezifischen Modellierungsansatz zu einem anderen ermöglichen. Neben der Sammlung mathematischer, informationstechnischer und anderer relevanter Implikationen bestehender Modellierungsansätze wird diese TWG prototypische Modellierungsansätze in Use Cases implementieren, um Wissenschaftler*innen und Studierenden die Möglichkeit zu geben, die Vor- und Nachteile nachprüfbar zu bewerten.
Plectocryptus muelleri KISS 1929
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Plectocryptus
Plectocryptus muelleri

description: Plectocryptus muelleri KISS 1929
 Plectocryptus mülleri KISS 1929: 112 f. – Holotypus () von SAWONIEWICZ (1984: 326) revidiert. Der Typenfundort Hermannstadt heisst jetzt Sibiu in Rumänien.
 G ü l t i g e r N a m e Crypteffigies lanius (GRAVENHORST 1829) (SAWONIEWICZ, l.c.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 781, DOI: 10.5281/zenodo.5429664
Additional file 1 of Comparative analyses of the Hymenoscyphus fraxineus and Hymenoscyphus albidus genomes reveals potentially adaptive differences in secondary metabolite and transposable element repertoires
Creators: name: Elfstrand, Malin
name: Chen, Jun
name: Cleary, Michelle
name: Halecker, Sandra
name: Ihrmark, Katarina
name: Karlsson, Magnus
name: Davydenko, Kateryna
name: Stenlid, Jan
name: Stadler, Marc
name: Durling, Mikael Brandström
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1:
Search for light pseudoscalar boson pairs produced from decays of the 125 GeV Higgs boson in final states with two muons and two nearby tracks in pp collisions at $\sqrt{s} =$ 13 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A search is presented for pairs of light pseudoscalar bosons, in the mass range from 4 to 15 GeV, produced from decays of the 125 GeV Higgs boson. The decay modes considered are final states that arise when one of the pseudoscalars decays to a pair of tau leptons, and the other one either into a pair of tau leptons or muons. The search is based on proton-proton collisions collected by the CMS experiment in 2016 at a center-of-mass energy of 13 TeV that correspond to an integrated luminosity of 35.9 fb${-1}$. The 2$μ$2$τ$ and 4$τ$ channels are used in combination to constrain the product of the Higgs boson production cross section and the branching fraction into 4$τ$ final state, $σ\mathcal{B}$, exploiting the linear dependence of the fermionic coupling strength of pseudoscalar bosons on the fermion mass. No significant excess is observed beyond the expectation from the standard model. The observed and expected upper limits at 95% confidence level on $σ\mathcal{B}$, relative to the standard model Higgs boson production cross section, are set respectively between 0.022 and 0.23 and between 0.027 and 0.19 in the mass range probed by the analysis.
description: Replaced with the published version. Added the journal reference and the DOI. All the figures and tables can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/HIG-18-006 (CMS Public Pages)
Bars and Dark Matter Halo Cores
Creators: name: Sellwood, J. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Self-consistent bars that form in galaxies embedded within cuspy halos are unable to flatten the cusp. Short bars form in models with quasi-flat rotation curves. They lose angular momentum to the halo through dynamical friction, but the continuous concentration of mass within the disk as the bar grows actually compresses the halo further, overwhelming any density reduction due to the modest angular momentum transfer to the halo. Thus the Weinberg-Katz proposed solution to the non-existence of the predicted cuspy halos from CDM simulations would seem to be unworkable. I also find that the concerns over the performance of N-body codes raised by these authors do not apply to the methods used here.
description: Latex 11 pages (uses emulateapj.sty), 8 figures, revised version to appear ApJ, very minor changes
Proscus ruber KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Proscus
Proscus ruber

description: Proscus ruber KISS 1924
 Proscus ruber KISS 1924: 51 – Holotypus () von DILLER (1983: 57) revidiert. Der Typenfundort Ferenczfalva heisst jetzt Valiug in Rumänien.
 G ü l t i g e r N a m e Homotherus locutor (THUNBERG 1824) (ROMAN 1939: 105).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 781, DOI: 10.5281/zenodo.5429664