cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Homo sapiens Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Hominidae
Homo
Homo sapiens

description: Homo sapiens [spec. nov.]
H. diurnus; varians cultura, loca.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 20, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quark contribution to the proton spin from 2+1+1-flavor lattice QCD
Creators: name: Lin, Huey-Wen
name: Gupta, Rajan
name: Yoon, Boram
name: Jang, Yong-Chull
name: Bhattacharya, Tanmoy
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the first chiral-continuum extrapolated up, down and strange quark spin contribution to the proton spin using lattice QCD. For the connected contributions, we use eleven ensembles of 2+1+1-flavor of Highly Improved Staggered Quarks (HISQ) generated by the MILC Collaboration. They cover four lattice spacings $a \approx \{0.15,0.12,0.09,0.06\}$ fm and three pion masses, $M_π\approx \{315,220,135\}$ MeV, of which two are at the physical pion mass. The disconnected strange calculations are done on seven of these ensembles, covering the four lattice spacings but only one with the physical pion mass. The disconnected light quark calculation was done on six ensembles at two values of $M_π\approx \{315,220\}$ MeV. High-statistics estimates on each ensemble for all three quantities allow us to quantify systematic uncertainties and perform a simultaneous chiral-continuum extrapolation in the lattice spacing and the light-quark mass. Our final results are $Δu \equiv \langle 1 \rangle_{Δu^+} = 0.777(25)(30)$, $Δd \equiv \langle 1 \rangle_{Δd^+} = -0.438(18)(30)$, and $Δs \equiv \langle 1 \rangle_{Δs^+} = -0.053(8)$, adding up to a total quark contribution to proton spin of $\sum_{q=u,d,s} (\frac{1}{2} Δq) = 0.143(31)(36)$. The second error is the systematic uncertainty associated with the chiral-continuum extrapolation. These results are obtained without model assumptions and are in good agreement with the recent COMPASS analysis $0.13 < \frac{1}{2} ΔΣ< 0.18$, and with the $Δq$ obtained from various global analyses of polarized beam or target data.
description: Published version. 8 pages 4 figures
title: ADCO, Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Cart. 184 (11 H 987), 105 folios, f. 0097
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0097, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0097, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
CCD PHOTOMETRY OF VARIABLE STARS IN THE GLOBULAR CLUSTER RU 106
Creators: name: Kaluzny, Janusz
name: Krzeminski, Wojciech
name: Mazur, Beata
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: BV photometry is presented for 12 RR Lyr variables discovered in the presumably young galactic globular cluster Ruprecht 106. All variables are type RRab, and their periods span a narrow range from 0.574 to 0.652 day. We report also on the discovery of 3 SX Phe variables among the cluster blue stragglers. A likely background RR Lyr variable and two foreground contact binaries were also found in the cluster field. The reddening of Ruprecht 106 is estimated at E(B-V)=0.20 based on the (B-V) colors exhibited by the cluster RR Lyr variables at minimum light. Analysis of the "period" versus "amplitude" and "period" versus "rise-time" diagrams suggests similar metallicities of Ruprecht 106 and M3. A peak (or bump) is present in the luminosity function of the red giant branch of Ruprecht 106. Its position relative to the horizontal branch is consistent with a cluster metallicity of [Fe/H]>= -1.6.
description: 25 pages, uuencoded compressed postscript file (including 13 figures)
Forces inside hadrons: pressure, surface tension, mechanical radius, and all that
Creators: name: Polyakov, Maxim V.
name: Schweitzer, Peter
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The physics related to the form factors of the energy momentum tensor spans a wide spectrum of problems, and includes gravitational physics, hard exclusive reactions, hadronic decays of heavy quarkonia, and the physics of exotic hadrons described as hadroquarkonia. It also provides access to the "last global unknown property:" the D-term. We review the physics associated with the form factors of the energy-momentum tensor and the D-term, their interpretations in terms of mechanical properties, their applications, and the current experimental status.
description: typos fixed, published version
A clinically relevant model and a potential treatment of perinatal hypoxic ischaemic encephalopathy in mice
Creators: name: Zheng, Xia
Publisher: name: Imperial College London
Year: 2016

description: Hypoxia ischaemia (HI) due to neonatal asphyxia is the most common cause of acute mortality and chronic neurological disability. Currently there is no effective means to repair the damaged brain. The aim of this study was to 1) establish a clinically relevant intrauterine model of perinatal hypoxic ischaemic encephalopathy (HIE) in mice, 2) determine whether lipopolysaccharide (LPS) induced maternal systemic inflammation worsened the outcome of neonates who had previously suffered HIE brain damage and 3) use the mouse HIE model to study whether a docosahexaenoic acid (DHA) enriched maternal diet has the potential to alleviate this harmful clinical condition. This is the first time that the intrauterine HI model has been established in mice. Pups exposed to 15 minutes of HI showed a higher mortality rate at 1 hour and those who survived displayed worse short term outcomes. However, the results were inconsistent with regards to the cellular changes observed such as inflammation and apoptosis, histological evidence and long-term neurocognitive outcomes. LPS-induced maternal systemic inflammation combined with HI showed no difference in survival rates compared to HI alone with a lower hypoxia-inducible factor 1-alpha and higher phospho-p38 and phospho-bad levels in the pup brains being observed. A maternal diet enriched with DHA did not result in a better outcome in the DHA + HI pups. The greater mortality rates in both Caesarean section (CS) and HI groups regardless of DHA in the diet indicated that other factors may influence neonatal death rates. Based on these data, this study concludes that the 15 minutes intrauterine HIE model cannot provide sustained damage observed in the mice brain and that the maternal LPS induced systemic inflammation did not show a clear better or worse outcome in the offspring. In addition, no clear neuroprotective effect was seen for the DHA enriched diet group.
Collisional baryonic dark matter halos
Creators: name: Walker, Mark A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: If dark halos are composed of dense gas clouds, as has recently been inferred, then collisions between clouds lead to galaxy evolution. Collisions introduce a core in an initially singular dark matter distribution, and can thus help to reconcile scale-free initial conditions -- such as are found in simulations -- with observed halos, which have cores. A pseudo-Tully-Fisher relation, between halo circular speed and visible mass (not luminosity), emerges naturally from the model: visible mass proportional to V^3.5. Published data conform astonishingly well to this theoretical prediction. For our sample of galaxies, the mass-velocity relationship has much less scatter than the Tully-Fisher relation, and holds as well for dwarf galaxies (where diffuse gas makes a sizeable contribution to the total visible mass) as it does for giants. It seems very likely that this visible-mass/velocity relationship is the underlying physical basis for the Tully-Fisher relation, and this discovery in turn suggests that the dark matter is both baryonic and collisional.
description: Revised version; 6 pages, 2 figures, to appear in MNRAS
The Association between diet and working hours with markers of cardiometabolic health in the British police force
Creators: name: Gibson, Rachel
Publisher: name: Imperial College London
Year: 2016

description: Long hours and shift work have been associated with cardiometabolic disease risk. Despite diet being an established modifiable risk factor, few studies have examined how dietary behaviours vary in relation to working hours. The aim of this thesis was to investigate the relationship between working hours and diet quality with markers of cardiometabolic health. Cross-sectional analyses were conducted using data from The Airwave Health Monitoring Study - a British police occupational cohort (n=5,849). Number of weekly working hours was determined from questionnaire data. The Dietary Approaches to Stop Hypertension score was calculated using 7-day diet data to measure diet quality. Markers of cardiometabolic health included: adiposity (body mass index, waist circumference and body fat), blood pressure, cholesterol, HbA1c and C-reactive protein. Sub-group analyses were conducted in participants with available shift work data (based on police radio records) (n=2,323). As part of this thesis a revised food diary and shift work questionnaire were developed and piloted for use in future studies. Male employees (n=3,332) working >49hrs per week (vs. 35-40hrs) were more likely to have a dietary pattern associated with elevated cardiometabolic risk. There was a positive dose-response relationship across working hours (!35-40, 41-48, 49-54, !55hrs per week) with markers of adiposity in male employees. Diet quality did not modify this association. Based on limited shift work data: night workers (vs. day) were found to consume a higher quantity of sugar-sweetened beverages. However shift work was not associated with increased cardiometabolic risk. This thesis suggests a sex specific positive association between weekly working hours and adiposity that is independent of established risk factors. Temporal eating pattern and previous shift work data collected using the revised food diary and shift questionnaire will be important to future studies exploring the relationship between diet, work hours and health.
The Microlensing and Halo Models of the Galaxy
Creators: name: Kan-ya, Yukitoshi
name: Nishi, Ryoichi
name: Nakamura, Takashi
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigated the dependence of the optical depth $τ$ of the microlensing events on model parameters of the Galactic halo. We only consider Galactic mass models in which the rotation curve inside the Sun is compatible with the observation and LMC is bound to the Galaxy. It is found that $τ$ varies up to a factor 2.5 from the standard spherical and flat rotation halo model. This implies that only the most centrally concentrated halo model can be consistent with the observation if the halo consists of only MACHOs. We also calculate the power $x$ of IMF of MACHO consistent with Tyson's CCD survey as well as Bahcall \etal's observation by {\em HST}. It is found that $x$ is greater than 5.
description: 17 pages (including 8 figures), uuencoded gz-compressed postscript
3D Finite Volume Simulation of Accretion Discs with Spiral Shocks
Creators: name: Makita, Makoto
name: Matsuda, Takuya
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We perform 2D and 3D numerical simulations of an accretion disc in a close binary system using the Simplified Flux vector Splitting (SFS) finite volume method. In our calculations, gas is assumed to be the ideal one, and we calculate the cases with gamma=1.01, 1.05, 1.1 and 1.2. The mass ratio of the mass losing star to the mass accreting star is unity. Our results show that spiral shocks are formed on the accretion disc in all cases. In 2D calculations we find that the smaller gamma is, the more tightly the spiral winds. We observe this trend in 3D calculations as well in somewhat weaker sense.
description: 2 pages, LaTeX with 2 ps figures using crckapb.sty. To appear in the Proceedings of Numerical Astrophysics 1998, Tokyo, Japan, 10-13 March, 1998, eds. S. M. Miyama, K. Tomisaka and T. Hanawa (Kluwer Academic Publishers)
Homo sapiens subsp. ferus Linnaeus, 1758, subspec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Hominidae
Homo
Homo sapiens
Homo sapiens subsp. ferus

description: Homo sapiens subsp. ferus [subspec. nov.]
tetrapus, mutus, hirsutus.
Juvenis Ursinus lithunus. 1661.
Juvenis Lupinus hessensis 1344.
Juvenis Ovinus hibernus Tulp. obs. IV. 9
Juvenis Hannoveranus.
Pueri 2 Pyrenaici. 1719.
Johannes Leodicensis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 20, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Dynamical critical scaling of long-range interacting quantum magnets
Creators: name: Defenu, Nicolo
name: Enss, Tilman
name: Kastner, Michael
name: Morigi, Giovanna
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Slow variations (quenches) of the magnetic field across the paramagnetic-ferromagnetic phase transition of spin systems produce heat. In systems with short-range interactions the heat exhibits universal power-law scaling as a function of the quench rate, known as Kibble-Zurek scaling. In this work we analyze slow quenches of the magnetic field in the Lipkin-Meshkov-Glick (LMG) model, which describes fully connected quantum spins. We analytically determine the quantum contribution to the residual heat as a function of the quench rate $δ$ by means of a Holstein-Primakoff expansion about the mean-field value. Unlike in the case of short-range interactions, scaling laws in the LMG model are only found for a ramp ending at the critical point. If instead the ramp is symmetric, as in the typical Kibble-Zurek scenario, after crossing the critical point the system tends to reabsorb the defects formed during the first part of the ramp: the number of excitations exhibits a crossover behavior as a function of $δ$ and tends to a constant in the thermodynamic limit. Previous, and seemingly contradictory, theoretical studies are identified as specific limits of this dynamics. Our results can be tested on several experimental platforms, including quantum gases and trapped ions.
description: 10 pages, 5 figures, new version improves figure 1 quality and expands the discussion of the results
Mammalian community responses to a gradient of land-use intensity on the island of Borneo
Creators: name: Wearn, Oliver
Publisher: name: Imperial College London
Year: 2015

description: Southeast Asian rainforests have, in recent decades, experienced the highest rates of deforestation and logging across the major tropical regions. This has left a vast estate of degraded forest in the region, which is under threat from further degradation and conversion to agriculture, principally for the expansion of oil palm (Elaeis guineensis) plantations. However, knowledge of the relative conservation value of different land-uses in the region is still limited, and a robust quantitative basis for resolving land-use tradeoffs, in particular between agricultural yield and biodiversity, is lacking. I aimed to assess terrestrial mammal species richness, abundance and β-diversity across a gradient of land-use intensity (old-growth forest, logged forest and oil palm) in Sabah, Malaysian Borneo. Overall mammal species richness was conserved even in the intensively-logged forests that I sampled, as were the majority of apparent old-growth specialists. Oil palm, on the other hand, harboured a highly depauperate mammal community. These broad patterns were echoed for overall mammal abundance, as well as in the potential ecosystem functions of mammals that I examined. However, I found evidence that the fundamental drivers of community assembly were altered across the land-use gradient and so, consequently, were patterns of β-diversity. Fine-grained β-diversity, in particular, was highest across the land-uses in logged forest, reflecting the increased environmental heterogeneity in this habitat. In addition, community composition and species abundance were not stable across land-uses. Omnivores and herbivores were more abundant in logged forest compared to old-growth forest, and only a limited number of carnivore species persisted in oil palm. Invasive species increased in abundance with land-use intensity. My findings underline the conservation importance of the large areas of degraded forest in Southeast Asia, and the extremely limited value offered by oil palm. If sustainability of the palm oil industry is to be achieved, new plantations should be diverted away from all remaining unfragmented forests, both old-growth and degraded forests alike.
YOSH OILALARGA  IJTIMOIY-PSIXOLOGIK VA  PEDAGOGIK YORDAM KO'RSATISH ASOSLARI
Creators: name: JDPU Baratov Nasriddin Karshibayevich o'qituvchi
Publisher: name: Zenodo
Year: 2024

description: Yoshlarni oilaviy hayotga tayyorlash bugungi kunning muhim vazifalaridan biridir. Shu asosda ushbu maqolada yosh oilalarga ijtimoiy-psixologik va pedagogik yordam ko’rsatish to’g’risida fikr yuritilgan
Additional file 3: of Progression-specific genes identified in microdissected formalin-fixed and paraffin-embedded tissue containing matched ductal carcinoma in situ and invasive ductal breast cancers
Creators: name: Schultz, Silke
name: Bartsch, Harald
name: Sotlar, Karl
name: Petat-Dutter, Karina
name: Bonin, Michael
name: Kahlert, Steffen
name: Harbeck, Nadia
name: Vogel, Ulrich
name: Seeger, Harald
name: Fehm, Tanja
name: Neubauer, Hans
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Plant Biology
subject: 60506 Virology

description: Validation 5 FFPE samples analogue to FF samples, Description: A) Analogue samples FFPE-Cryo: The selected progression-associated genes are significantly differential expressed between DCIS and IBC of the same tumour (P
Unsupervised Learning for Fast Probabilistic Diffeomorphic Registration
Creators: name: Dalca, Adrian V.
name: Balakrishnan, Guha
name: Guttag, John
name: Sabuncu, Mert R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: Traditional deformable registration techniques achieve impressive results and offer a rigorous theoretical treatment, but are computationally intensive since they solve an optimization problem for each image pair. Recently, learning-based methods have facilitated fast registration by learning spatial deformation functions. However, these approaches use restricted deformation models, require supervised labels, or do not guarantee a diffeomorphic (topology-preserving) registration. Furthermore, learning-based registration tools have not been derived from a probabilistic framework that can offer uncertainty estimates. In this paper, we present a probabilistic generative model and derive an unsupervised learning-based inference algorithm that makes use of recent developments in convolutional neural networks (CNNs). We demonstrate our method on a 3D brain registration task, and provide an empirical analysis of the algorithm. Our approach results in state of the art accuracy and very fast runtimes, while providing diffeomorphic guarantees and uncertainty estimates. Our implementation is available online at http://voxelmorph.csail.mit.edu .
description: MICCAI 2018 (Oral Presentation). Proceedings: LNCS 11070, pp 729-738
The nature of the optical---radio correlations for powerful radio galaxies
Creators: name: Tadhunter, C. N.
name: Morganti, R.
name: Robinson, A.
name: Dickson, R.
name: Villar-Martin, M.
name: Fosbury, R. A. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nature of the optical--radio correlations for powerful radio galaxies is investigated using spectroscopic observations of a complete sample of southern 2Jy radio sources. In line with previous work, we find that significant correlations exist between the luminosities of the [OIII]5007, [OII]3727 and Hbeta emission lines and the radio luminosity. However, our observations are not easily reconciled with the idea that these correlations are caused by the increase in the power of the photoionizing quasar as the jet power increases, with average ISM properties not changing appreciably with redshift or radio power: not only do we find that the scatter in the L_[OIII] vs. L_radio correlation is significantly larger than in L_[OII]} vs. L_radio and L_Hbeta vs. L_radio correlations, but the ionization state deduced from the emission lines does not increase with radio power as predicted by the simple, constant ISM, photionization model. We conclude that: (a) there exists a considerable range in the quasar ionizing luminosity at a given redshift; and (b) that the mean density of the emission line clouds is larger in the high redshift/high power radio sources. The latter density enhancement may either be a consequence of the increased importance of jet-cloud interactions or, alternatively, due to a higher pressure in the confining hot ISM, in the high redshift objects. Deep spectra show that many of the sources in our sample are broad line radio galaxies (BLRG). The fact that the BLRG are observed out the redshift limit of the survey, overlapping in redshift with the quasars, argues against the idea that BLRG are simply the low radio power counterparts of high power, high redshift quasars.
description: 37 pages, LateX, including 11 figures and 3 tables. To appear in MNRAS
Maxwell's Theory of Solid Angle and the Construction of Knotted Fields
Creators: name: Binysh, Jack
name: Alexander, Gareth P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We provide a systematic description of the solid angle function as a means of constructing a knotted field for any curve or link in $\mathbb{R}^3$. This is a purely geometric construction in which all of the properties of the entire knotted field derive from the geometry of the curve, and from projective and spherical geometry. We emphasise a fundamental homotopy formula as unifying different formulae for computing the solid angle. The solid angle induces a natural framing of the curve, which we show is related to its writhe and use to characterise the local structure in a neighborhood of the knot. Finally, we discuss computational implementation of the formulae derived, with C code provided, and give illustrations for how the solid angle may be used to give explicit constructions of knotted scroll waves in excitable media and knotted director fields around disclination lines in nematic liquid crystals.
description: 20 pages, 9 figures
Spiral Structure in IP Peg: Confronting Theory and Observations
Creators: name: Matsuda, Takuya
name: Makita, Makoto
name: Yukawa, Hiroshi
name: Boffin, Henri M. J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first convincing piece of evidence of spiral structure in the accretion disc in IP Pegasi was found by Steeghs et al. (1997). We performed two kinds of 2D hydrodynamic simulations, a SFS finite volume scheme and a SPH scheme, with a mass ratio of 0.5. Both results agreed well with each other. We constructed Doppler maps and line flux-binary phase relations based on density distributions, the results agreeing well with those obtained by observation.
description: 4 pages, LaTeX with 2 ps figures using crckapb.sty. To appear in the Proceedings of Numerical Astrophysics 1998, Tokyo, Japan, 10-13 March, 1998, eds. S. M. Miyama, K. Tomisaka and T. Hanawa (Kluwer Academic Publishers)
Magnetic field dependence of the electron spin revival amplitude in periodically pulsed quantum dots
Creators: name: Kleinjohann, Iris
name: Evers, Eiko
name: Schering, Philipp
name: Greilich, Alex
name: Uhrig, Götz S.
name: Bayer, Manfred
name: Anders, Frithjof B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Periodic laser pulsing of singly charged semiconductor quantum dots in an external magnetic field leads to a synchronization of the spin dynamics with the optical excitation. The pumped electron spins partially rephase prior to each laser pulse, causing a revival of electron spin polarization with its maximum at the incidence time of a laser pulse. The amplitude of this revival is amplified by the frequency focusing of the surrounding nuclear spins. Two complementary theoretical approaches for simulating up to 20 million laser pulses are developed and employed that are able to bridge between 11 orders of magnitude in time: a fully quantum mechanical description limited to small nuclear bath sizes and a technique based on the classical equations of motion applicable for a large number of nuclear spins. We present experimental data of the nonmonotonic revival amplitude as function of the magnetic field applied perpendicular to the optical axis. The dependence of the revival amplitude on the external field with a profound minimum at $4\;$T is reproduced by both of our theoretical approaches and is ascribed to the nuclear Zeeman effect. Since the nuclear Larmor precession determines the electronic resonance condition, it also defines the number of electron spin revolutions between pump pulses, the orientation of the electron spin at the incidence time of a pump pulse, and the resulting revival amplitude. The magnetic field of $4\;$T, for example, corresponds to half a revolution of nuclear spins between two laser pulses.
description: 21 pages, 16 figures
Supplementary document for Flame temperature and emissivity distribution measurement of solid ropellant based on clustering analysis of multispectral images - 7204733.pdf
Creators: name: Ni, Hu
name: Qiang, Kejie
name: Wang, Wensong
name: Yang, Bin
name: Tao, Jinxin
name: Yang, Yang
name: Shi, Zhiquan
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Optimal band range and thermocouple verification
Full phase diagram of active Brownian disks: from melting to motility-induced phase separation
Creators: name: Digregorio, Pasquale
name: Levis, Demian
name: Suma, Antonio
name: Cugliandolo, Leticia F.
name: Gonnella, Giuseppe
name: Pagonabarraga, Ignacio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We establish the complete phase diagram of self-propelled hard disks in two spatial dimensions from the analysis of the equation of state and the statistics of local order parameters. The equilibrium melting scenario is maintained at small activities, with coexistence between active liquid and hexatic order, followed by a proper hexatic phase and a further transition to an active solid. As activity increases, the emergence of hexatic and solid order is shifted towards higher densities. Above a critical activity and for a certain range of packing fractions, the system undergoes MIPS and demixes into low and high density phases; the latter can be either disordered (liquid) or ordered (hexatic or solid) depending on activity.
Computational models of belief propagation
Creators: name: Ng, Khin Hua
Publisher: name: Imperial College London
Year: 2015

description: In this thesis we aim to gain better understanding on the working of the belief propagation algorithm designed for graphical models in other computational frameworks like the neural systems, as well as the error associated with loopy belief propagation in Bayesian networks. In the first part, we examine a few recent neural computational models of belief propagation and highlight the significance of these models that demonstrate the viability of performing belief propagation using neural computations by transforming it into a dynamical system. We also propose the idea of implementing the belief propagation in computational models like the Hopfield network through free energy minimisation. It is widely known that exact inference in loopy graphs is computationally difficult and thus there has been a lot of effort spent in the area of developing practical approximate inference algorithms. Loopy belief propagation is a widely used approximate inference algorithm for graphical models. In the second part of this thesis, we analyse the loopy error and propose two exact inference algorithms using belief propagation with loop correction for Bayesian networks with generic loops. We also propose a new approximate inference method called the 2-Pass loopy belief propagation and demonstrate empirically its potential for use as a fast approximate inference algorithm with comparable accuracy to standard loopy belief propagation. We also discuss issues related to its application as an approximate inference method.
Additional file 15: of Integrated genomic analyses in PDX model reveal a cyclin-dependent kinase inhibitor Palbociclib as a novel candidate drug for nasopharyngeal carcinoma
Creators: name: Cheng-Lung Hsu
name: Kar-Wai Lui
name: Lang-Ming Chi
name: Yung-Chia Kuo
name: Yin-Kai Chao
name: Yeh, Chun-Nan
name: Lee, Li-Yu
name: Yenlin Huang
name: Tung-Liang Lin
name: Mei-Yuan Huang
name: Lai, Yi-Ru
name: Yeh, Yuan-Ming
name: Hsien-Chi Fan
name: Lin, An-Chi
name: Yen-Jung Lu
name: Chia-Hsun Hsieh
name: Chang, Kai-Ping
name: Ngan-Ming Tsang
name: Hung-Ming Wang
name: Chang, Alex
name: Yu-Sun Chang
name: Hsin-Pai Li
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
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: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S7. Immnunohistochemical (IHC) staining of cyclin D1 in 139 NPC tissues from year 2002 to 2016. (PDF 415 kb)
Homo sapiens subsp. americanus Linnaeus, 1758, subspec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Hominidae
Homo
Homo sapiens
Homo sapiens subsp. americanus

description: Homo sapiens subsp. americanus [subspec. nov.]
rufus, cholericus, rectus.
Pilis nigris, rectis, crassis; Naribus patulis; Facie ephelitica, Mento subimberbi.
Pertinax, hilaris, liber.
Pingit se lineis daedaleis rubris.
Regitur Consvetudine.
(*) Nosse Se Ipsum gradus est primus sapientiae, dictumque Solonis, quondam scriptum, litteris aureis supra Dianae Templum. Mus. ADOLPH. FRID. Praefat.
Physiologice: Te contextum Nervis, intertextum Fibris, Machina tenella, sed adolescente in perfectissimam, faeultatibus instructam fere omnibus pluribusque, quam reliqua cuncta. Nudum in nuda humo, natali die, abjecit natura ad vagitus statim & ploratum, manibus pedibusque devinciendum Animal caeteris imperaturum; cui scire nihil sine doctrina: non fari, non ingredi, non vesci, non aliud natura sponte. Plin. Vides itaque qualem vitam nobis rerum natura promisit, quae primum nascentium omen fletum esse voluit. Seneca.
Diaetetice: Te sanitate & tranquillitate, si noveris, felicem: Moderatis conservandum, Nimiis destruendum, Variatis afficiendum, Insvetis frangendum, Consvetis indurandum; polyphagum Culina instructissima, per errores gratissima, igne vinoque horrenda. Parvo fames constat, magno fastidium. Seneca.
Pathologice: Te tumidam usque dum crepueris bullam, piloque pendulam in puncto fugientis temporis. Nihil enim homine imbecillius terra alit. Homer. Nulli vita fragilior; nulli tot Morbi, tot Curae, tot Pericula. Breve universum utique aevi tempus: Pars aequa morti similis exigitur; nec reputantur Infantiae anni, qui sensu carent; nec Senectae in poenam vivaces: hebescunt Sensus, torpent Membra, praemoriuntur Visus, Auditus, Incessus, Dentes, Ciborum instrumenta. Plin. Sic magna pars mortis jam praeteriit, quidquid aetatis retro est Mors tenet. Totum denique hunc, quem vides populum, quousque cogitas esse; cito natura revocavit & condet; Mors omnes aeque vocat; iratis Diis propitiisque moriendum. Senec. II: 59.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 20, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 5 of Eimeria falciformis secretes extracellular vesicles to modulate proinflammatory response during interaction with mouse intestinal epithelial cells
Creators: name: Olajide, Joshua Seun
name: Xiong, Ling
name: Yang, Shunli
name: Qu, Zigang
name: Xu, Xiao
name: Yang, Bin
name: Wang, Jing
name: Liu, Baohong
name: Ma, Xueting
name: Cai, Jianping
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 5: Electrophoretic gel, bioinformatic result, and result from non-treated control.
Weighted F-free Edge Editing
Creators: name: Spinner, Jonas
Publisher: name: Karlsruher Institut für Technologie (KIT)
Year: 2019

description: Ein F-freier Graph besitzt keinen induzierten Teilgraphen aus einer Menge von verbotenen Teilgraphen F. Man kann Kanten in einem Graphen editieren (einfügen oder entfernen) um einen Graphen zu erreichen, der F-frei ist. Das Ziel von F-free Edge Editing ist es, eine minimale Menge an Editierungsoperation zu finden, die zu einem F-freien Graphen führen. Wir betrachten eine Generalisierung, Weighted F-free Edge Editing, die beliebige Kosten für die Editierungsoperationen erlaubt. In dieser Arbeit fokussieren wir uns auf einen parametrisierten Suchbaumalgorithmus (FPT) mit den Editierungskosten als Parameter. Wir adaptieren bereits existierende Beschleunigungstechniken für das ungewichteten Editieren für den gewichteten Fall. Unter anderem betrachten wir Algorithmen zum Berechnen von unteren Schranken und Strategien für die Auswahl von Teilgraphen zum Verzweigen. Außerdem diskutieren wir das Problem, die optimalen Editierungskosten für den Suchbaumalgorithmus zu finden und präsentieren dafür zwei neue Suchstrategien. Zusätzlich behandeln wir einen Algorithmus basierend auf ganzahliger linearer Optimierung (ILP) und Methoden, die die Anzahl der generierten Bedingungen beschränken. Des Weiteren evaluieren wir die FPT und ILP Algorithmen und ihre Beschleunigungstechniken auf Protein-Protein Interaktionsgraphen für F = {C4, P4}. Wir stellen fest, dass der FPT Algorithmus am meisten von dem Greedy-Algorithmus für untere Schranken und der Auswahlstrategie “most adjacent” profitiert. Letztere präferiert Teilgraphen, die zu vielen anderen verbotenen Teilgraphen adjazent sind. Auch fanden wir heraus, dass der Algorithmus für die untere Schranken, der auf lokaler Suche basiert, im gewichteten Fall größere Probleme mit lokalen Maxima hat. Weiterhin bemerken wir, dass das Beschränken der Anzahl der generierten Bedingungen den ILP Algorithmus signifikant schneller werden lässt. Schlussendlich haben wir beide Lösungsalgorithmen verglichen und kamen zum Schluss, dass der ILP Algorithmus konsistent besser ist als der FPT Algorithmus.
Can the fluctuations of the quantum vacuum solve the cosmological constant problem?
Creators: name: Cree, Samuel S.
name: Davis, Tamara M.
name: Ralph, Timothy C.
name: Wang, Qingdi
name: Zhu, Zhen
name: Unruh, William G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The cosmological constant problem arises because the magnitude of vacuum energy density predicted by quantum mechanics is about 120 orders of magnitude larger than the value implied by cosmological observations of accelerating cosmic expansion. Recently, some of the current authors proposed that the stochastic nature of the quantum vacuum can resolve this tension [Q, Wang, Z. Zhu, and W. G. Unruh, Phys. Rev. D 95, 103504, 2017]. By treating the fluctuations in the vacuum seriously and allowing fluctuations up to some high-energy cutoff at which Quantum Field Theory is believed to break down, a parametric resonance effect arises that leads to a slow expansion and acceleration. In this work, we thoroughly examine the implications of this proposal by investigating the resulting dynamics. First, we improve upon numerical calculations in the original work and show that convergence issues had overshadowed some important effects. Correct calculations reverse some of the conclusions in [Q. Wang, Z. Zhu, and W. G. Unruh, Phys. Rev. D 95, 103504, 2017], however the premise that parametric resonance can explain a very slowly accelerating expansion appears to remain sound. After improving the resolution and efficiency of the numerical tests, we explore a wider range of cutoff energies, and examine the effects of multiple particle fields. We introduce a simple model using the Mathieu equation (a prototypical example of parametric resonance), and find that it closely matches numerical results in regimes where its assumptions are valid. Using this model, we extrapolate to find that in a universe with 28 bosonic fields and a high-energy cutoff 40 times higher than the Planck energy, the acceleration would be comparable to what is observed.
description: 19 pages, 12 figures
Measuring Ω_0 from the Entropy Evolution of Clusters
Creators: name: Kay, Scott T.
name: Bower, Richard G.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, we have extended the entropy-driven model of cluster evolution developed by Bower (1997) in order to be able to predict the evolution of galaxy clusters for a range of cosmological scenarios. We have applied this model to recent measurements of the evolution of the L_x-T normalisation and X-ray luminosity function in order to place constraints on cosmological parameters. We find that these measurements alone do not select a particular cosmological frame-work. An additional constraint is required on the effective slope of the power spectrum to break the degeneracy that exists between this and the background cosmology. We have therefore included a theoretical calculation of the Ω_0 dependence on the power spectrum, based on the cold dark matter paradigm, which infers Ω_0<0.55 (0.1
description: 14 pages including 5 figures; accepted for publication in MNRAS
Analysis of morphological and blood flow characteristics of the human thoracic aorta
Creators: name: Fatona, Oluwatoyin Fadeke
Publisher: name: Imperial College London
Year: 2016

description: The human aorta is often affected by many cardiovascular diseases, including atherosclerosis, aneurysm and dissection. There is considerable evidence suggesting that these diseases are associated with the morphology and haemodynamic functions of the aorta, but not all these parameters can be measured directly in vivo. In particular, the helical flow characteristics and haemodynamic wall parameters can only be evaluated from quantitative information on a flow field resolved both in space and time. This study provides a comprehensive analysis of geometric and haemodynamic characteristics of the human aorta through subject-specific simulations of blood flow based on medical images. Computational fluid dynamics (CFD) models of the thoracic aorta were developed based on in vivo anatomical and flow data acquired using magnetic resonance imaging (MRI). In order to capture potential transitional and turbulent flow in the aorta, the correlation based shear stress transporttransitional (SST-Trans) turbulence model was employed. Detailed flow analyses were performed on multiple cases of normal thoracic aortas with a tricuspid aortic valve (TAV) and abnormal aorta with a bicuspid aortic valve (BAV). Results obtained from this study gave quantitative insights into the flow distributions and wall shear stress (WSS) patterns in normal and abnormal aortas. Morphological features and flow patterns of the TAV and BAV aortas were compared. In addition to standard flow parameters, specific indices were evaluated to allow for direct comparisons between the two groups; these included flow reversal ratio (FRR), helicity flow index (HFI) and shear range index (SRI). The results showed that all examined aortas tapered from the proximal ascending segment to the distal descending segment, with the BAV aorta showing a more distinct tapering. Although flow patterns were qualitatively similar in the TAV and BAV aortas, there were substantial quantitative variations. Highly disturbed flow was observed in all examined aortas during part of the cycle, mostly in the systolic deceleration phase. Predicted WSS was higher in the TAV aorta than in the BAV aorta, with the highest WSS occurring in regions around the major arch branches. Comparisons between the predicted and measured velocities showed a good agreement, demonstrating that MR image-based CFD modelling methodology can be used to obtain reliable haemodynamic parameters that are important in clinical assessment and management of aortic diseases.
Chirality Josephson current due to a novel quantum anomaly in inversion-asymmetric Weyl semimetals
Creators: name: Zhang, Song-Bo
name: Erdmenger, Johanna
name: Trauzettel, Björn
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study Josephson junctions based on inversion-asymmetric but time-reversal symmetric Weyl semimetals under the influence of Zeeman fields. We find that, due to distinct spin textures, the Weyl nodes of opposite chirality respond differently to an external magnetic field. Remarkably, a Zeeman field perpendicular to the junction direction results in a phase shift of opposite sign in the current-phase relations of opposite chirality. This leads to a finite chirality Josephson current (CJC) even in the absence of a phase difference across the junction. This feature could allow for applications in chiralitytronics. In the long junction and zero temperature limit, the CJC embodies a novel quantum anomaly of Goldstone bosons at $π$ phase difference which is associated with a $\mathbb{Z}_2$ symmetry at low energies. It can be detected experimentally via an anomalous Fraunhofer pattern.
description: 15 pages, 8 figures
Spectral Indices in Cooling Flow Galaxies: Evidence for Star Formation
Creators: name: Cardiel, N.
name: Gorgas, J.
name: Aragon-Salamanca, A.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Through the study of two absorption spectral features in the optical range (Mg2 and the 4000 A break), we find evidence for star formation in the inner regions of cooling-flow galaxies. The application of simple stellar population models reveals that the measured indices are explained if a relatively small fraction of the total mass flow (5-17%) is forming new stars with a normal IMF. However, we argue that this is only a lower limit, and conclude that a large fraction of the gas accreted inside the galaxy could be forming stars. In addition, the analysis of line-strength gradients in the inner galaxy regions reveals that, in the mean, they are lower than those of normal ellipticals, and exhibit a hint of correlation with the mass accretion rate. Simultaneously, the spectral indices in the outer regions of some galaxies, with and without cooling flow, attain extremely low values, suggesting that they could be hosting star formation with an origin not related to the cooling flows.
description: PostScript file (compressed and encoded) containing 21 pages
Supplementary document for High quality factor, monodisperse micron-sized random lasers based on porous PLGA spheres - 7141917.pdf
Creators: name: Pham, Nhat
name: Nguyen, Quan
name: Van Nguyen, Toan
name: Nguyen, Tien-Anh
name: Ta, Duong
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Supplemental document 1. Illustration of the fabrication process of dye-doped PLGA spheres using a microfluidic system and optical images of dye-doped PLGA microspheres
MOESM5 of Genetic repertoires of anaerobic microbiomes driving generation of biogas
Creators: name: Grohmann, Anja
name: Yevhen Vainshtein
name: Euchner, Ellen
name: Grumaz, Christian
name: Bryniok, Dieter
name: Rabus, Ralf
name: Sohn, Kai
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Computational Biology

description: Additional file 5. Heatmap of top 500 differentially expressed transcripts.