cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Orbital Period of the Accreting Pulsar GX1+4
Creators: name: Pereira, Marildo G.
name: Braga, Joao
name: Jablonski, Francisco J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report strong evidence for a ~304-day periodicity in the spin history of the accretion-powered pulsar GX1+4 that is most probably associated with the orbital period of the system. We have used data from the Burst and Transient Source Experiment on the Compton Gamma Ray Observatory to show a clear periodic modulation of the pulsar frequency from 1991 to date, in excellent agreement with the ephemeris proposed by Cutler, Dennis & Dolan (1986). Our results indicate that the orbital period of GX1+4 is 303.8 +- 1.1 days, making it the widest known low-mass X-ray binary system by more than one order of magnitude and putting this long-standing question to rest. A likely scenario for this system is an elliptical orbit in which the neutron star decreases its spin-down rate (or even exhibits a momentary spin-up behavior) at periastron passages due to the higher torque exerted by the accretion disk onto the magnetosphere of the neutron star. These results are not inconsistent with both the X-ray pulsed flux light curve measured by BATSE during the same epoch and the X-ray flux history from the All-Sky Monitor (ASM) onboard the Rossi X-Ray Timing Explorer.
description: 14 pages, 2 PS figures, LaTeX file using aasms4.sty (not included), accepted for publication in Ap.J. Letters
Plagiolepis
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Plagiolepis

description: 1. Subgenus Plagiolepis Mayr.
Mayr., 1861, Europ. Formicid. p. 42. Emery, 1925, Gen. Insect., Formicinae, p. 19.
Mesonotum non saillant sur le profil, epinotum non releve, deprime ou peu convexe. Tout l'ancien continent. Ocelles absents. Type: Formica pygmeae Latreille, 1798.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 14
Strain-induced Defect Superstructure on the SrTiO3(110) Surface
Creators: name: Wang, Zhiming
name: Li, Fengmiao
name: Meng, Sheng
name: Zhang, Jiandi
name: Plummer, E. W.
name: Diebold, Ulrike
name: Guo, Jiandong
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report on a combined scanning tunneling microscopy and density functional theory calculation study of the SrTiO3(110)-(4 x 1) surface. It is found that antiphase domains are formed along the [1-10]-oriented stripes on the surface. The domain boundaries are decorated by defects pairs consisting of Ti2O3 vacancies and Sr adatoms, which relieve the residual stress. The formation energy of, and interactions between, vacancies result in a defect superstructure. It is suggested that the density and distributions of defects can be tuned by strain engineering, providing a fexible platform for the designed growth of complex oxide materials.
{$K^0$}-{$\overline{K}^0$} mixing and the CKM parameters $(ρ,η)$ from the Laplace sum rules
Creators: name: Narison, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Using the Laplace sum rule (LSR) approach, which is less affected by the contribution of the higher mass hadronic states than the Finite Energy Sum Rule (FESR), we test the reliability of the existing estimate of the $K^0$-$\overline {K}^0$ mixing parameter from the four-quark two-point correlator. We obtain, for the renormalization group invariant $B$-parameter $\Big[ f_K/(1.2f_π)\Big]^2 \hat {B}_K$, the upper bound: 0.83 and the $best$ estimate: $0.55 \pm 0.09$. Combining the previous estimate with the updated value of $f_B\sqrt{B_B}=(1.49\pm 0.14)f_π$ obtained from the same LSR method, one can deduce the $best$ fitted values $(ρ,η)\approx (0.41,0.09)$ of the CKM parameters.
description: 6 pages in latex file + 3 figure in ps files (sent by requests), CERN-TH.7441/94 (1994) (some missprints in the previous version may lead to some confusion)
Additional file 7 of Characterization of novel LncRNA P14AS as a protector of ANRIL through AUF1 binding in human cells
Creators: name: Ma, Wanru
name: Qiao, Juanli
name: Zhou, Jing
name: Gu, Liankun
name: Deng, Dajun
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 7 Table S2. Function annotations for P14AS-upregulated genes (n = 241) with fold change > 2 in HCT116 cells with the David 6.8: Functional Annotation Tools at the website http://david.ncifcrf.gov/tools.jsp [13]
Acantholepis (Lepisiota)
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Acantholepis
Plagiolepis
Plagiolepis rothneyi

description: 1. Subgenus Lepisiota, n. subg.
Plagiolepis (Anacantholepis) Santschi 1914 (partim),
Medd. Goeteborgs Mus. Zool., III, p. 36.
Ocelles bien developpes (1) et variabilite assez grande de la taille; ecaille mousse inerme. Epinotum faiblement anguleux. Especes d'Asie.
Type: Plagiolepis rothneyi, Forel 1984.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 15
Melting probe technology for subsurface exploration of extraterrestrial ice - Critical refreezing length and the role of gravity
Creators: name: Schüller, Kai
name: Kowalski, Julia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The 'Ocean Worlds' of our Solar System are covered with ice, hence the water is not directly accessible. Using melting probe technology is one of the promising technological approaches to reach those scientifically interesting water reservoirs. Melting probes basically consist of a heated melting head on top of an elongated body that contains the scientific payload. The traditional engineering approach to design such melting probes starts from a global energy balance around the melting head and quantifies the power necessary to sustain a specific melting velocity while preventing the probe from refreezing and stall in the channel. Though this approach is sufficient to design simple melting probes for terrestrial applications, it is too simplistic to study the probe's performance for environmental conditions found on some of the Ocean's Worlds, e.g. a lower value of the gravitational acceleration. This will be important, however, when designing exploration technologies for extraterrestrial purposes. We tackle the problem by explicitly modeling the physical processes in the thin melt film between the probe and the underlying ice. Our model allows to study melting regimes on bodies of different gravitational acceleration, and we explicitly compare melting regimes on Europa, Enceladus and Mars. In addition to that, our model allows to quantify the heat losses due to convective transport around the melting probe. We discuss to which extent these heat losses can be utilized to avoid the necessity of a side wall heating system to prevent stall, and introduce the notion of the 'Critical Refreezing Length'. Our results allow to draw important conclusions towards the design of melting probe technology for future missions to icy bodies in our Solar System.
Additional file 1: of A randomized, controlled study to investigate the efficacy and safety of a topical gentamicin-collagen sponge in combination with systemic antibiotic therapy in diabetic patients with a moderate or severe foot ulcer infection
Creators: name: Ilker Uรงkay
name: Kressmann, Benjamin
name: Malacarne, Sarah
name: Toumanova, Anna
name: Jaafar Jaafar
name: Lew, Daniel
name: Lipsky, Benjamin
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: DFUI WOUND SCORE-TARGET INFECTION ( ULCER WITH HIGHEST DFI WOUND (DOC 79 kb)
IMPORTANCE OF DEVELOPMENT OF PISTACHIO FARMING IN UZBEKISTAN
Creators: name: Hamzaev, Abdushukur
name: Inomova, Munira
Publisher: name: Zenodo
Year: 2024

description: It is no secret that water reserves are limited in the territory of our republic. The way to solve existing problems is to organize efficient use, develop methods of efficient use of existing water resources, selective cultivation of drought-resistant, low-water consumption and high-yield plant species is one of the problems in the field of forestry. In our opinion, one of the plant species that can meet the above requirements is the pistachio tree (Pistacia vera L.).
Constraints On The Delayed Transition to Detonation in Type Ia Supernovae
Creators: name: Lisewski, A. M.
name: Hillebrandt, W.
name: Woosley, S. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the possibility of a delayed detonation in a type Ia supernova under the assumption that the transition to detonation is triggered by turbulence only. Our discussion is based on the Zeldovich mechanism and suggests that typical turbulent velocities present during the explosion are not strong enough to allow this transition to occur. Although we are able to show that in carbon-rich matter (e.g., $X(^{12}$C$) = 0.75$) the possibility of a deflagration to detonation transition (DDT) is enhanced, even in this case the turbulent velocities needed are larger than the expected value of $u'(L) \approx 10^7 {cm s}^{-1}$ on a length-scale of $L \approx 10^6$ cm. Thus we conclude that a DDT may not be a common event during a thermonuclear explosion of a Chandrasekhar-mass white dwarf.
description: 18 pages, 5 figures, accepted for publication in the ApJ
How sharp is the chiral crossover phenomenon for realistic meson masses?
Creators: name: Meyer-Ortmanns, Hildegard
name: Schaefer, Bernd-Jochen
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The mass dependence of the chiral phase transition is studied in the linear $SU(3)\times SU(3)$ sigma-model to leading order in a $1/N_f$-expansion, $N_f$ denoting the number of flavours. For realistic meson masses we find a smooth crossover between $T\sim181.5$ to 192.6~[MeV]. The crossover looks more rapid in the light quark condensate than in thermodynamic quantities like the energy and entropy densities. The change in the light quark condensate in this temperature interval is $\sim$~50\% of the zero-temperature condensate value, while the entropy density increases by ($5.5\pm0.8)\cdot10^{-3}$~[GeV$^3$]. Since the numerical error is particularly large in this region, we cannot rule out a finite latent heat smaller than 0.2~[GeV/fm$^3$]. The chiral transition is washed out for an average pseudoscalar meson octet mass of 203~[MeV]. This gives an upper bound on the first-order transition region in the meson mass parameter space. The corresponding ratio of critical to realistic light current quark masses $m^{crit}_{u,d}/m_{u,d}$ is estimated as $0.26\pm0.08$. This result is by an order of magnitude larger than the corresponding mean-field value. Therefore the
description: LaTeX, HD--TVP--94--16, Please contact authors via email for figures
Effective electronic-only Kohn-Sham equations for the muonic molecules
Creators: name: Rayka, Milad
name: Goli, Mohammad
name: Shahbazian, Shant
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Other Condensed Matter (cond-mat.other)
subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A set of effective electronic-only Kohn-Sham (EKS) equations are derived for the muonic molecules (containing a positively charged muon), which are completely equivalent to the coupled electronic-muonic Kohn-Sham equations derived previously within the framework of the Nuclear-Electronic Orbital density functional theory (NEO-DFT). The EKS equations contain effective non-coulombic external potentials depending on parameters describing muon vibration, which are optimized during the solution of the EKS equations making muon KS orbital reproducible. It is demonstrated that the EKS equations are derivable from a certain class of effective electronic Hamiltonians through applying the usual Hohenberg-Kohn theorems revealing a duality between the NEO-DFT and the effective electronic-only DFT methodologies. The EKS equations are computationally applied to a small set of muoniated organic radicals and it is demonstrated that a mean effective potential maybe derived for this class of muonic species while an electronic basis set is also designed for the muon. These computational ingredients are then applied to muoniated ferrocenyl radicals, which had been previously detected experimentally through adding muonium atom to ferrocene. In line with previous computational studies, from the six possible species the staggered conformer, where the muon is attached to the exo position of the cyclopentadienyl ring, is deduced to be the most stable ferrocenyl radical.
Kinetic Mixing, Proton Decay and Gravitational Waves in SO(10)
Creators: name: Maji, Rinku
name: Shafi, Qaisar
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present an $SO(10)$ model in which a dimension five operator induces kinetic mixing at the GUT scale between the abelian subgroups $U(1)_{B-L}$ and $U(1)_R$. We discuss in this framework gauge coupling unification and proton decay, as well as the appearance of superheavy quasistable strings with $Gμ\sim 10^{-8} - 10^{-5}$, where $μ$ denotes the dimensionless string tension parameter. We use Bayesian analysis to show that for $Gμ$ values $\sim 4 \times 10^{-7} - 10^{-5}$, the gravitational wave spectrum emitted from the quasistable strings is in good agreement with the recent pulsar timing array data. Corresponding to $G μ$ values $\sim 10^{-8} - 2 \times 10^{-7}$, proton decay is expected to occur at a rate accessible in the Hyper-Kamiokande experiment. Finally, we present the gravitational wave spectrum emitted by effectively stable strings with $Gμ\approx 10^{-8}$ that have experienced a certain amount of inflation. This can be tested with future detectors in the $μ$Hz frequency range.
description: 20 pages, 5 captioned figures, published in JHEP
Additional file 9: of Efficacy of extracorporeal shock wave therapy for knee tendinopathies and other soft tissue disorders: a meta-analysis of randomized controlled trials
Creators: name: Chun-De Liao
name: Xie, Guo-Min
name: Jau-Yih Tsauo
name: Hung-Chou Chen
name: Tsan-Hon Liou
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Computational Biology

description: Figure S7. Data and forest plot of clinical efficacy of extracorporeal shock wave therapy for performance-based functional outcomes over the overall follow-up duration. (PDF 60 kb)
Additional file 7 of Cotton roots are the major source of gossypol biosynthesis and accumulation
Creators: name: Zhao, Tianlun
name: Xie, Qianwen
name: Li, Cong
name: Li, Cheng
name: Mei, Lei
name: Yu, John
name: Chen, Jinhong
name: Zhu, Shuijin
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Molecular Biology
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Plant Biology

description: Additional file 7: Table S4. All primers used in this study.
Tuning Spin Dynamics and Localization Near the Metal-Insulator Transition in Fe/GaAs heterostructures
Creators: name: Ou, Yu-Sheng
name: Harmon, N. J.
name: Odenthal, Patrick
name: Kawakami, R. K.
name: Flatté, M. E.
name: Johnston-Halperin, E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present a simultaneous investigation of coherent spin dynamics in both localized and itinerant carriers in Fe/GaAs heterostructures using ultrafast and spin-resolved pump-probe spectroscopy. We find that for excitation densities that push the transient Fermi energy of photocarriers above the mobility edge there exist two distinct precession frequencies in the ob-served spin dynamics, allowing us to simultaneously monitor both localized and itinerant states. For low magnetic fields (below 3 T) the beat frequency between these two excitations evolves linearly, indicating that the nuclear polarization is saturated almost immediately and that the hyperfine coupling to these two states is comparable, despite the 100x enhancement in nuclear polarization provided by the presence of the Fe layer. At higher magnetic fields (above 3 T) the Zeeman energy drives reentrant localization of the photocarriers. Subtracting the constant hyperfine contribution from both sets of data allows us to extract the Lande g-factor for each state and estimate their energy relative to the bottom of the conduction band, yielding -2.16 meV and 17 meV for localized and itinerant states, respectively. This work advances our fundamental understanding of spin-spin interactions between electron and nuclear spin species, as well as between localized and itinerant electronics states, and therefore has implications for future work in both spintronics and quantum information/computation.
description: 18 pages, 3 figures
Longitudinal Transitions Of Baryon Resonances in Constituent Quark Model
Creators: name: Li, Zhenping
name: Dong, Yubing
name: Ma, Weihsing
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A longitudinal transition operator that satisfies the gauge invariance requirement is introduced in constituent quark model. The corresponding longitudinal transitions between the nucleon and baryon resonances are calculated. We show that the study of the longitudinal coupling plays an important role in understanding the structure of baryons.
description: 13 pages with 5 figures in ps. file can be obtained from author
Quantum-Chromodynamic Potential Model for Light-Heavy Quarkonia and the Heavy Quark Effective Theory
Creators: name: Gupta, Suraj N.
name: Johnson, James M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We have investigated the spectra of light-heavy quarkonia with the use of a quantum-chromodynamic potential model which is similar to that used earlier for the heavy quarkonia. An essential feature of our treatment is the inclusion of the one-loop radiative corrections to the quark-antiquark potential, which contribute significantly to the spin-splittings among the quarkonium energy levels. Unlike $c\bar{c}$ and $b\bar{b}$, the potential for a light-heavy system has a complicated dependence on the light and heavy quark masses $m$ and $M$, and it contains a spin-orbit mixing term. We have obtained excellent results for the observed energy levels of $D^0$, $D_s$, $B^0$, and $B_s$, and we are able to provide predicted results for many unobserved energy levels. Our potential parameters for different quarkonia satisfy the constraints of quantum chromodynamics. We have also used our investigation to test the accuracy of the heavy quark effective theory. We find that the heavy quark expansion yields generally good results for the $B^0$ and $B_s$ energy levels provided that $M^{-1}$ and $M^{-1}\ln M$ corrections are taken into account in the quark-antiquark interactions. It does not, however, provide equally good results for the energy levels of $D^0$ and $D_s$, which indicates that the effective theory can be applied more accurately to the $b$ quark than the $c$ quark.
description: 17 pages of LaTeX. To appear in Physical Review D. Complete PostScript file is available via WWW at http://gluon.physics.wayne.edu/wsuhep/jim/heavy.ps
The Radio Afterglow From GRB 980519: A Test of the Jet and Circumstellar Models
Creators: name: Frail, D. A.
name: Kulkarni, S. R.
name: Sari, R.
name: Taylor, G. B.
name: Shepherd, D. S.
name: Bloom, J. S.
name: Young, C. H.
name: Nicastro, L.
name: Masetti, N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present multi-frequency radio observations from the afterglow of GRB 980519 beginning 7.2 hours after the gamma-ray burst and ending 63 days later. The fast decline in the optical and X-ray light curves for this burst has been interpreted either as afterglow emission originating from a collimated outflow -- a jet -- or the result of a blast wave propagating into a medium whose density is shaped by the wind of an evolved massive star. These two models predict divergent behavior for the radio afterglow, and therefore, radio observations are capable, in principle, of discriminating between the two. We show that a wind model describes the subsequent evolution of the radio afterglow rather well. However, we see strong modulation of the light curve, which we interpret as diffractive scintillation. These variations prevent us from decisively rejecting the jet model.
description: ApJ, submitted
Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?
Creators: name: Bisht, Mukesh Singh
name: Banerjee, Projjwal
name: Nath, Biman B.
name: Shchekinov, Yuri
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The recent detection of large column density absorption lines from highly ionized gas in a few directions through the circumgalactic medium (CGM) of the Milky Way (MW) has been puzzling. The inferred temperature from these absorption lines far exceeds the virial temperature of the MW, and the column densities are also too large to be easily explained. In this paper, we propose a novel idea to explain these observations and claim that they may not have originated from the CGM, but from a totally different type of source, namely, stellar ejecta from supernovae (SNe) above the Galactic disk that happen to lie in the line of sight to the background quasars. About $\sim 20\%$ of massive OB stars (progenitors of core-collapse supernovae) are known to be runaway stars that have high ejection velocities near the Galactic plane and can end up exploding as SNe above the Galactic disk. We show that the associated reverse shock in the supernova remnant in the early non-radiative phase can heat the ejecta to temperatures of $\gtrsim 10^7\,{\rm K}$ and can naturally explain the observed high column density of ions in the observed `super-virial' phase along with $α$-enriched super-solar abundance that is typical of core-collapse supernovae. However, SNe from runaway stars has a covering fraction of $\lesssim 0.7 \%$ and thus can only explain the observations along limited sightlines.
description: 14 pages, accepted for publication in the Astrophysical Journal (ApJ)
Black hole mergers in the universe
Creators: name: Zwart, Simon Portegies
name: McMillan, Stephen
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Mergers of black-hole binaries are expected to release large amounts of energy in the form of gravitational radiation. However, binary evolution models predict merger rates too low to be of observational interest. In this paper we explore the possibility that black holes become members of close binaries via dynamical interactions with other stars in dense stellar systems. In star clusters, black holes become the most massive objects within a few tens of millions of years; dynamical relaxation then causes them to sink to the cluster core, where they form binaries. These black-hole binaries become more tightly bound by superelastic encounters with other cluster members, and are ultimately ejected from the cluster. The majority of escaping black-hole binaries have orbital periods short enough and eccentricities high enough that the emission of gravitational radiation causes them to coalesce within a few billion years. We predict a black-hole merger rate of about $1.6 \times 10^{-7}$ per year per cubic megaparsec, implying gravity wave detection rates substantially greater than the corresponding rates from neutron star mergers. For the first generation Laser Interferometer Gravitational-Wave Observatory (LIGO-I), we expect about one detection during the first two years of operation. For its successor LIGO-II, the rate rises to roughly one detection per day. The uncertainties in these numbers are large. Event rates may drop by about an order of magnitude if the most massive clusters eject their black hole binaries early in their evolution.
description: 12 pages, ApJL in press
Small-X Quarks at HERA Predict the Ultra High Energy Neutrino-Nucleon Cross Section
Creators: name: Frichter, George M.
name: McKay, Douglas W.
name: Ralston, John P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: New structure function data at small Bjorken $x$ from HERA are used along with next-to-leading order QCD evolution to predict a cross section for charged-current interactions of ultrahigh energy neutrinos with nucleons. This new result is over twice the size of previous estimates and has important implications for cosmic ray experiments now underway as well as for KM3 arrays (cubic kilometer-scale neutrino telescopes) now in the planning stages.
description: KITCS94-9-1, 9 pages (REVTeX) plus 3 postscript figures all uuencoded
title: ADCO, Cinquième cartulaire de Saint-Étienne de Dijon (1664), Cart. 28 (G 132), 258 folios, f. 00127
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00127, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00127, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 8: of Efficacy of extracorporeal shock wave therapy for knee tendinopathies and other soft tissue disorders: a meta-analysis of randomized controlled trials
Creators: name: Chun-De Liao
name: Xie, Guo-Min
name: Jau-Yih Tsauo
name: Hung-Chou Chen
name: Tsan-Hon Liou
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Figure S6. Data and forest plot of clinical efficacy of extracorporeal shock wave therapy for patient-reported functional outcomes at each follow-up time point. (PDF 93 kb)
Statistical properties of SGR 1900+14 bursts
Creators: name: Gogus, Ersin
name: Woods, Peter M.
name: Kouveliotou, Chryssa
name: van Paradijs, Jan
name: Briggs, Michael S.
name: Duncan, Robert C.
name: Thompson, Christopher
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the statistics of soft gamma repeater (SGR) bursts, using a data base of 187 events detected with BATSE and 837 events detected with RXTE PCA, all from SGR 1900+14 during its 1998-1999 active phase. We find that the fluence or energy distribution of bursts is consistent with a power law of index 1.66, over 4 orders of magnitude. This scale-free distribution resembles the Gutenberg-Richter Law for earthquakes, and gives evidence for self-organized criticality in SGRs. The distribution of time intervals between successive bursts from SGR 1900+14 is consistent with a log-normal distribution. There is no correlation between burst intensity and the waiting times till the next burst, but there is some evidence for a correlation between burst intensity and the time elapsed since the previous burst. We also find a correlation between the duration and the energy of the bursts, but with significant scatter. In all these statistical properties, SGR bursts resemble earthquakes and solar flares more closely than they resemble any known accretion-powered or nuclear-powered phenomena. Thus our analysis lends support to the hypothesis that the energy source for SGR bursts is internal to the neutron star, and plausibly magnetic.
description: 11 pages, 4 figures, accepted for publication in ApJL
Solution to the Perturbative Infrared Catastrophe of Hot Gauge Theories
Creators: name: Braaten, Eric
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The free energy of a nonabelian gauge theory at high temperature $T$ can be calculated to order $g^5$ using resummed perturbation theory, but the method breaks down at order $g^6$. A new method is developed for calculating the free energy to arbitrarily high accuracy in the high temperature limit. It involves the construction of a sequence of two effective field theories by first integrating out the momentum scale $T$ and then integrating out the momentum scale $g T$. The free energy decomposes into the sum of three terms, corresponding to the momentum scales $T$, $gT$, and $g^2T$. The first term can be calculated as a perturbation series in $g^2(T)$, where $g(T)$ is the running coupling constant. The second term in the free energy can be calculated as a perturbation series in $g(T)$, beginning at order $g^3$. The third term can also be expressed as a series in $g(T)$ beginning at order $g^6$, with coefficients that can be calculated using lattice simulations of 3-dimensional QCD. Leading logarithms of $T/(gT)$ and of $gT/(g^2T)$ can be summed up using renormalization group equations.
description: 11 pages LaTeX, NUHEP-TH-94-24
Bio-inspired circular soft actuators for simulating defecation process of human rectum
Creators: name: Mao, Zebing
name: Suzuki, Sota
name: Wiranata, Ardi
name: Zheng, Yanqiu
name: Miyagawa, Shoko
Publisher: name: arXiv
Year: 2024
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Soft robots have found extensive applications in the medical field, particularly in rehabilitation exercises, assisted grasping, and artificial organs. Despite significant advancements in simulating various components of the digestive system, the rectum has been largely neglected due to societal stigma. This study seeks to address this gap by developing soft circular muscle actuators (CMAs) and rectum models to replicate the defecation process. Using soft materials, both the rectum and the actuators were fabricated to enable seamless integration and attachment. We designed, fabricated, and tested three types of CMAs and compared them to the simulated results. A pneumatic system was employed to control the actuators, and simulated stool was synthesized using sodium alginate and calcium chloride. Experimental results indicated that the third type of actuator exhibited superior performance in terms of area contraction and pressure generation. The successful simulation of the defecation process highlights the potential of these soft actuators in biomedical applications, providing a foundation for further research and development in the field of soft robotics.
Using Naive Bayes Algorithm to Students' bachelor Academic Performances Analysis
Creators: name: Razaque, Fahad
name: Soomro, Nareena
name: Shaikh, Shoaib Ahmed
name: Soomro, Safeeullah
name: Samo, Javed Ahmed
name: Kumar, Natesh
name: Dharejo, Huma
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Academic Data Mining was one of emerging field which comprise procedure of examined students details by different elements such as earlier semester marks, attendance, assignment, discussion, lab work were of used to improved bachelor academic performance of students, and overcome difficulties of low ranks of bachelor students. It was extracted useful knowledge from bachelor academic students data collected from department of Computing. Subsequently preprocessing data, which was applied data mining techniques to discover classification and clustering. In this study, classification method was described which was based on naive byes algorithm and used for Academic data mining. It was supportive to students along with to lecturers for evaluation of academic performance. It was cautionary method for students to progress their performance of study.
description: 2017
D4.1 - Analisi dettagliata dei requisiti dei casi d'uso
Creators: name: Adamo, Alessio
name: Arriva, Simona
name: Barbera, Roberto
name: Basile, Antonino
name: Cascio, Donato
name: Catania, Valentina
name: Dal Col, Alessandro
name: Di Gregorio, Giuseppe
name: Fazio, Salvatore
name: Ferri, Raffaele
name: Gallo, Giuseppe
name: Gambino, Orazio
name: Gelardi, Donatella
name: Grasso, Federica
name: Gulisano, Walter
name: Lo Presti, Domenico
name: Panerai, Simonetta
name: Pappalardo, Marco
name: Puzzo, Daniela
name: Lombardo, Marco
name: Patti, Michele
name: Pirrone, Roberto
name: Rundo, Francesco
name: Scardina, Alessandro
name: Tegolo, Domenico
name: Tropea, Maria Rosaria
Publisher: name: INFN Open Access Repository
Year: 2021
Subjects: 3DLab-Sicilia
Deliverable
D4.1

description: Scopo del presente documento è quello di fornire una descrizione dettagliata degli “use case” già identificati in fase di preparazione della proposta progettuale, inclusiva di un’analisi dei loro requisiti in termini di infrastruttura necessaria per la loro implementazione. A questo proposito, con riferimento a Technopedia2 e alla tassonomia introdotta da IEEE Computer Society, è stata elaborata una tassonomia di tutti i possibili requisiti dei casi d’uso del progetto già identificati.
 Lo schema del documento è il seguente. La Sezione 2 introduce la metodologia e l’analisi dei requisiti dei casi d’uso. I lemmi della tassonomia sono riportati nella in quella Sezione e sono poi riassunti per completezza nell’Appendice 1, nella quale ad ogni lemma è associato un codice numerico che è quello poi usato come riferimento nelle Sezioni successive del presente documento. La Sezione 3 presenta il modello di definizione dei casi d’uso in termini dei loro Scenari implementativi che sono poi dettagliati nelle Appendici 2-8. Le Sezioni che vanno dalla 4 alla 10 descrivono infine i 7 “use case” che sono stati già identificati. Per ciascuno di essi, l’informazione fornita è declinata sui seguenti aspetti: introduzione e stato dell’arte; descrizione; rilevanza; requisiti in termini di infrastruttura; prodotti attesi; indicatori di prestazione chiave e analisi dei rischi, che sono trattati in altrettante sotto-sezioni.
Supernova Remnants in the Fossil Starburst in M82
Creators: name: de Grijs, Richard
name: O'Connell, Robert W.
name: Becker, George D.
name: Chevalier, Roger A.
name: Gallagher, John S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of ten compact H-alpha-bright sources in the post-starburst region northeast of the center of M82, ``M82 B.'' These objects have H alpha luminosities and sizes consistent with Type II supernova remnants (SNRs). They fall on the same H alpha surface brightness-diameter (Sigma-D) relation defined by SNRs in other nearby star-forming galaxies, with the M82 candidates lying preferentially at the small diameter end. These are the first candidates for optically-visible SNRs in M82 outside the heavily obscured central starburst within ~250 pc from the galactic center. If these sources are SNRs, they set an upper limit to the end of the starburst in region ``B2,'' about 500 pc from the galaxy's core, of ~50 Myr. Region ``B1,'' about 1000 pc from the core, lacks good SNR candidates and is evidently somewhat older. This suggests star formation in the galaxy has propagated inward toward the present-day intense starburst core.
description: Re-submitted to AJ, referee's comments taken into account, 15 pages LaTeX preprint style, 4 postscript figures; full-resolution figures available from http://www.astro.virginia.edu/~rd7a/snrs/ Changes: minor textual changes and orientation/axes of Fig. 2
Energy Relaxation of N$_2$O in Gaseous, Supercritical and Liquid Xenon and SF$_6$
Creators: name: Töpfer, Kai
name: Erramilli, Shyamsunder
name: Ziegler, Lawrence D.
name: Meuwly, Markus
Publisher: name: arXiv
Year: 2024
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Rotational and vibrational energy relaxation (RER and VER) of N$_2$O embedded in xenon and SF$_6$ environments ranging from the gas phase to the liquid, including the supercritical regime, is studied at a molecular level. Calibrated intermolecular interactions from high-level electronic structure calculations, validated against experiments for the pure solvents were used to carry out classical molecular dynamics simulations corresponding to experimental state points for near-critical isotherms. Computed RER rates in low-density solvent of $k_{\rm rot}^{\rm Xe} = (3.67\pm0.25)\cdot10^{10}$ s$^{-1}$M$^{-1}$ and $k_{\rm rot}^{\rm SF_6} = (1.25\pm0.12)\cdot10^{11}$ s$^{-1}$M$^{-1}$ compare well with rates determined by analysis of 2-dimensional infrared experiments. Simulations find that an isolated binary collision (IBC) description is successful up to solvent concentrations of $\sim 4$ M. For higher densities, including the supercritical regime, the simulations do not correctly describe RER, probably due to neglect of solvent-solute coupling in the analysis of the rotational motion. For VER, the near-quantitative agreement between simulations and pump-probe experiments captures the solvent density-dependent trends.
Broadband terahertz generation via the interface inverse Rashba-Edelstein effect
Creators: name: Zhou, C.
name: Liu, Y. P.
name: Wang, Z.
name: Ma, S. J.
name: Jia, M. W.
name: Wu, R. Q.
name: Zhou, L.
name: Zhang, W.
name: Liu, M. K.
name: Wu, Y. Z.
name: Qi, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Novel mechanisms for electromagnetic wave emission in the terahertz (THz) frequency regime emerging at the nanometer scale have recently attracted intense attention for the purpose of searching next-generation broadband THz emitters. Here, we report a new mechanism for broadband THz emission, utilizing the interface inverse Rashba-Edelstein effect. By engineering the symmetry of the Ag/Bi Rashba interface, we demonstrate a controllable THz radiation (~0.1-5 THz) waveform emitted from metallic Fe/Ag/Bi heterostructures following photo-excitation. We further reveal that this type of THz radiation can be selectively superimposed on the emission discovered recently due to the inverse Spin Hall effect, yielding a unique film thickness dependent emission pattern. Our results thus offer new opportunities for versatile broadband THz radiation using the interface quantum effects.
A Scheme for radiative CP violation
Creators: name: Chang, Darwin
name: Keung, W. -Y.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a simple model in which CP symmetry is spontaneously broken only after the radiative corrections are taken into account. The model includes two Higgs-boson doublets and two right-handed singlet neutrinos which induce the necessary non-hermitian interaction. To evade the Georgi-Pais theorem, some fine-tuning of coupling constants is necessary. However, we show that such fine-tuning is natural in the technical sense as it is protected by symmetry. Some phenomenological consequences are also discussed.
description: 10 pages, ANL-HEP-PR-94-65
Additional file 7: of Efficacy of extracorporeal shock wave therapy for knee tendinopathies and other soft tissue disorders: a meta-analysis of randomized controlled trials
Creators: name: Chun-De Liao
name: Xie, Guo-Min
name: Jau-Yih Tsauo
name: Hung-Chou Chen
name: Tsan-Hon Liou
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S5. Data and forest plot of clinical efficacy of extracorporeal shock wave therapy for patient-reported functional outcomes over the overall follow-up duration. (PDF 701 kb)
Effective Field Theory of the Linear $O(N)$ Sigma Model
Creators: name: Nyffeler, A.
name: Schenk, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The low energy structure of a theory containing light and heavy particle species which are separated by a mass gap can adequately be described by an effective theory which contains only the light particles. In this work we present a thorough analysis of the effective field theory of the linear $O(N)$ sigma model in the spontaneously broken phase. In particular, we present a detailed discussion of two techniques, a short-distance expansion and a method based on loop-integrals, which can be used to explicitly evaluate the functional relationships between the low energy constants of the effective theory and the parameters of the underlying theory. We furthermore provide a detailed analysis of the matching relation between the linear sigma model and its effective theory, in order to clarify some discrepancies which can be found in the literature.
description: 42 pages, LaTeX, BUTP-94/12, HUTP-94/A012, to appear in Ann. Phys
The space density of spiral galaxies as function of their scale size, surface brightness and luminosity
Creators: name: de Jong, Roelof S.
name: Lacey, Cedric
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The local space density of galaxies as a function of their basic structural parameters -luminosity, surface brightness and scale size- is still poorly known. Our poor knowledge is the result of strong selection biases against low surface brightness and small scale size galaxies in any optically selected sample. We derive bivariate space density distributions by correcting a sample of ~1000 local Sb-Sdm spiral galaxies for its selection effects. We present a parameterization of these bivariate distributions, based on a Schechter type luminosity function and a log-normal scale size distribution at a given luminosity. We next calculate the bivariate distributions as function of redshift using the Hubble Deep Field, and conclude that at higher redshift there is a decrease in space density of luminous, large scale size galaxies, but the density of smaller galaxies stays nearly the same.
description: 8 pages, 2 figures. To appear in the conference proceedings of "Toward a New Millennium in Galaxy Morphology" edited by D.L. Block, I. Puerari, A. Stockton and D. Ferreira (Kluwer, Dordrecht)
Studying $\varepsilon '/\varepsilon$ in the Chiral Quark Model: $γ_5$-Scheme Independence and NLO Hadronic Matrix Elements
Creators: name: Bertolini, S.
name: Eeg, J. O.
name: Fabbrichesi, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the $CP$-violating, $|ΔS| =1$ parameter $\varepsilon '/\varepsilon$ by computing the hadronic matrix elements in the chiral quark model. We estimate the coefficients of the next-to-leading order terms in the chiral expansion that correspond to the operators $Q_6$ and $Q_{11}$. We consider the impact of these corrections on the value of $\varepsilon '/\varepsilon$. We also investigate the possibility that the chiral quark model might drastically reduce the dimensional regularization $γ_5$-scheme dependence of current evaluations of $\varepsilon '/\varepsilon$.
description: 38 pages, LATEX, including 4 eps figures
ENG "UYQUCHI" VA DOIMIY DIEATADA YURADIGAN XALTALI AYIQCHA
Creators: name: Abdullayeva, Kamola
Publisher: name: Zenodo
Year: 2025

description: Avstraliyaning sharqiy va janubiy hududlarida tarqalgan endemik turlardan biri bo`lmish koala o`zining yoqimtoy ko`rinishi va bir tutam sochlari bilan ko`pchilikni o`ziga jalb qiladi. Kolaning faqatgina shu hududlarga yashashiga asosiy sabab esa uning asosiy oziqasi bo`lmish evkalipt daraxtining o`sishi uchun shu hududlardagina namlikning yetarli ekanligi hisoblanadi. Koala so‘zi aborigen tilidan olingan bo‘lib, "suv ichmaydigan" degan ma’noni anglatadi, chunki mahalliy aholining fikricha, bu hayvonlar umuman suv ichmaydi. XVIII asrlarda Yevropaga kelgan ilk ko`chmanchi odamlar bu hayvonni yumaloq tana shakliga ega ekanligini ko`rib uni koala ayiqchasi deb nomlashgan. Shuningdek, urg`ochi koalalarning qornida bolasini olib yurishi uchun maxsus xaltachasi ham mavjudligi, ushbu hayvinlarning ayiqlarga aloqasi yo`qligini ko`rsatadi. Hozirda koalalar koala oilasining yagona turi hisoblanadi.
Supplementary document for Exciton reservoir-induced destabilization and reformation of polariton condensate - 7441702.pdf
Creators: name: Park, Min
name: Koniakhin, Sergei
name: choi, Soohong
name: Choi, Daegwang
name: Park, Suk In
name: Park, S.Y.
name: Song, Jin Dong
name: Cho, Yong-Hoon
name: Choi, Hyungsoon
Publisher: name: Optica Publishing Group
Year: 2025
Subjects: Uncategorized

description: Descriptions of the figures related to the sample characteristics, the power-dependent S-curve, under-threshold experimental data, and time resolution.