Search results for "FOS"

showing 10 items of 15075 documents

Momentum distributions of cosmic relics: Improved analysis

2022

We solve coupled momentum-dependent Boltzmann equations for the phase space distribution of cosmic relic particles, without resorting to approximations of assuming kinetic equilibrium or neglecting backscattering or elastic interactions. Our method is amendable to precision numerical computations. To test it, we consider two benchmark models where the momentum dependence of dark matter distribution function is potentially important: a real singlet scalar extension near the Higgs resonance and a sterile neutrino dark matter model with a singlet scalar mediator. The singlet scalar example shows that the kinetic equilibrium may hold surprisingly well even near sharp resonances. However, the in…

pimeä aineHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Cosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::PhenomenologyneutriinotBaryogenesisFOS: Physical sciencesDark-matterkosmologia114 Physical sciencesAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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Self-interacting dark matter and cosmology of a light scalar mediator

2015

We consider a fermionic dark matter candidate interacting via a scalar mediator coupled with the Standard Model through a Higgs portal. We consider general setting including both scalar and pseudoscalar interactions between the scalar and fermion, and illustrate the relevant features for dark matter abundance, direct search limits and collider constraints. The case where dark matter has a self-interaction strength $\left\langle \sigma_V \right\rangle/m_\psi \sim 0.1-1 \,\mathrm{cm}^2/\mathrm{g}$ is strongly constrained, in particular by the Big Bang Nucleosynthesis. We show that these constraints can be alleviated by introducing a new light sterile neutrino $N$. The allowed region for the e…

pimeä aineHigh Energy Physics - PhenomenologyStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Cosmology and Nongalactic Astrophysics (astro-ph.CO)sterile neutrinosfermionsHigh Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics::Experimentscalar mediatorsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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La anamorfosis como acontecimiento visual

2015

A pesar de que el de anamorfosis es un concepto cuya definición parece clara, se observa vacilación e incluso contradicción a la hora de calificar como tal a diversos tipos de imágenes. Este trabajo busca establecer de la manera más precisa posible qué es y qué no es anamorfosis. Para ello revisa las notas o componentes esenciales que se hallan en las definiciones que se han hecho desde su aparición como neologismo en 1657. Profundiza en las fuentes de confusión que se derivan de ideas como "deformación", "transformación" y "engaño", para establecer las diferencias entre anamorfosis y otros tipos de imágenes con las que suele ser confundida, especialmente con el trampantojo, las correccione…

pinturaperspectivaUNESCO::HISTORIA::Historia por especialidades::Historia del arteanamorfosiscultura visualUNESCO::CIENCIAS DE LAS ARTES Y LAS LETRAS::Teoría análisis y crítica de las Bellas Artes::Pintura:CIENCIAS DE LAS ARTES Y LAS LETRAS::Teoría análisis y crítica de las Bellas Artes::Estética de las Bellas Artes [UNESCO]UNESCO::CIENCIAS DE LAS ARTES Y LAS LETRAS::Teoría análisis y crítica de las Bellas Artes::Estética de las Bellas Artes:HISTORIA::Historia por especialidades::Historia del arte [UNESCO]metaimagen:CIENCIAS DE LAS ARTES Y LAS LETRAS::Teoría análisis y crítica de las Bellas Artes::Pintura [UNESCO]
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A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251

2013

We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting microlensing observations towards the Galactic Bulge. Based on detailed modelling of the observed light curve, we find that the lens is composed of two masses with a mass ratio q=1.9 x 10^-3. Thanks to our detection of higher-order effects on the light curve due to the Earth's orbital motion and the finite size of source, we are able to measure the mass and distance to the lens unambiguously. We find that the lens is made up of a planet of mass 0.53 +- 0.21,M_Jup orbiting an M dwarf host star with a mass of 0.26 +- 0.…

planets and satellites: detection010504 meteorology & atmospheric sciencesSatellitesbulge [Galaxy]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsDiscoveryGravitational microlensing01 natural sciencesGalaxy: bulgeEinstein radiusLensgravitational lensing: weakSettore FIS/05 - Astronomia e AstrofisicaPlanetSnow0103 physical sciencesgravitational lensing; weak; planets and satellites; detection; planetary systems; Galaxy; bulgegravitational lensing: weak; planets and satellites: detection; planetary systems; Galaxy: bulgeBinaryQB Astronomy010303 astronomy & astrophysicsplanetary systemsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesQBPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Giant planetSystemsSearchAstronomy and AstrophysicsRadiusFrequencyPlanetary systemMass ratioMassLight curveStarsAlgorithmdetection [Planets and satellites]Planetary systemsSpace and Planetary ScienceDwarfAstrophysics::Earth and Planetary Astrophysicsweak [Gravitational lensing]Astrophysics - Earth and Planetary AstrophysicsAstronomy and Astrophysics
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Kohn-Sham Decomposition in Real-Time Time-Dependent Density-Functional Theory An Efficient Tool for Analyzing Plasmonic Excitations

2017

The real-time-propagation formulation of time-dependent density-functional theory (RT-TDDFT) is an efficient method for modeling the optical response of molecules and nanoparticles. Compared to the widely adopted linear-response TDDFT approaches based on, e.g., the Casida equations, RT-TDDFT appears, however, lacking efficient analysis methods. This applies in particular to a decomposition of the response in the basis of the underlying single-electron states. In this work, we overcome this limitation by developing an analysis method for obtaining the Kohn-Sham electron-hole decomposition in RT-TDDFT. We demonstrate the equivalence between the developed method and the Casida approach by a be…

plasmonic excitationsTheoretical computer scienceKohn-Sham decompositionComputer scienceta221Kohn–Sham equationsFOS: Physical sciencesPhysics::Optics02 engineering and technology01 natural sciencesPhysics - Chemical Physics0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Decomposition (computer science)Physics::Atomic and Molecular ClustersStatistical physicsPhysical and Theoretical ChemistryPhysics::Chemical Physics010306 general physicsta116PlasmonEigenvalues and eigenvectorsChemical Physics (physics.chem-ph)Condensed Matter - Materials ScienceCondensed Matter - Mesoscale and Nanoscale Physicsta114tiheysfunktionaaliteoriaMaterials Science (cond-mat.mtrl-sci)Time-dependent density functional theory16. Peace & justice021001 nanoscience & nanotechnologyComputer Science ApplicationsplasmonitBenzene derivativesnanohiukkaset0210 nano-technologyJOURNAL OF CHEMICAL THEORY AND COMPUTATION
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High-resolution laser spectroscopy of long-lived plutonium isotopes

2017

Long-lived isotopes of plutonium were studied using two complementary techniques, high-resolution resonance ionisation spectroscopy (HR-RIS) and collinear laser spectroscopy (CLS). Isotope shifts have been measured on the $5f^67s^2\ ^7F_0 \rightarrow 5f^56d^27s\ (J=1)$ and $5f^67s^2\ ^7F_1 \rightarrow 5f^67s7p\ (J=2)$ atomic transitions using the HR-RIS method and the hyperfine factors have been extracted for the odd mass nuclei $^{239,241}$Pu. Collinear laser spectroscopy was performed on the $5f^67s\ ^8F_{1/2} \rightarrow J=1/2\; (27523.61\text{cm}^{-1})$ ionic transition with the hyperfine $A$ factors measured for $^{239}$Pu. Changes in mean-squared charge radii have been extracted and s…

plutoniumAtomic Physics (physics.atom-ph)collinear laser spectroscopyFOS: Physical sciencesHigh resolutionPlutonium isotopes01 natural sciencesPhysics - Atomic PhysicsCLs upper limits0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsSpectroscopyHyperfine structureNuclear ExperimentisotopesPhysicsisotoopitta114010308 nuclear & particles physics/dk/atira/pure/subjectarea/asjc/3100/3107Charge (physics)Atomic and Molecular Physics and Opticshigh-resolution resonance ionization spectroscopyResonance ionizationAtomic physics
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Orbital angular momentum parton distributions in quark models

1999

At the low energy, {\sl hadronic}, scale we calculate Orbital Angular Momentum (OAM) twist-two parton distributions for the relativistic MIT bag model and for non-relativistic quark models. We reach the scale of the data by leading order evolution in perturbative QCD. We confirm that the contribution of quarks and gluons OAM to the nucleon spin grows with $Q^2$, and it can be relevant at the experimental scale, even if it is negligible at the hadronic scale, irrespective of the model used. The sign and shape of the quark OAM distribution at high $Q^2$ may depend strongly on the relative size of the OAM and spin distributions at the hadronic scale. Sizeable quark OAM distributions at the had…

polarized DIS; Generalized parton distributions; evolution equationsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)evolution equationsHigh Energy Physics::PhenomenologyNuclear TheoryPhysics::OpticsFOS: Physical sciencesHigh Energy Physics::ExperimentNuclear ExperimentGeneralized parton distributionspolarized DIS
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The Hamburg/ESO R-process Enhanced Star survey (HERES)

2004

We report on a dedicated effort to identify and study metal-poor stars strongly enhanced in r-process elements ([r/Fe] > 1 dex; hereafter r-II stars), the Hamburg/ESO R-process Enhanced Star survey (HERES). Moderate-resolution (~2A) follow-up spectroscopy has been obtained for metal-poor giant candidates selected from the Hamburg/ESO objective-prism survey (HES) as well as the HK survey to identify sharp-lined stars with [Fe/H] < -2.5dex. For several hundred confirmed metal-poor giants brighter than B~16.5mag (most of them from the HES), ``snapshot'' spectra (R~20,000; S/N~30 per pixel) are being obtained with VLT/UVES, with the main aim of finding the 2-3% r-II stars expected to be a…

population II [stars]PhysicsAstrophysics (astro-ph)FOS: Physical sciencesabundances [Galaxy]Astronomy and AstrophysicsAstrophysicsStar (graph theory)AstrophysicsSpectral lineabundances [stars]Neutron captureStarssurveysSpace and Planetary SciencePhenomenological modelhalo [Galaxy]Astronomy Astrophysics and Cosmologyr-processSpectroscopyRadioactive decayAstronomy & Astrophysics
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Effects of pyrolysis temperature on the hydrologically relevant porosity of willow biochar

2018

Biochar pore space consists of porosity of multiple length scales. In direct water holding applications like water storage for plant water uptake, the main interest is in micrometre-range porosity since these pores are able to store water that is easily available for plants. Gas adsorption measurements which are commonly used to characterize the physical pore structure of biochars are not able to quantify this pore-size range. While pyrogenetic porosity (i.e. pores formed during pyrolysis process) tends to increase with elevated process temperature, it is uncertain whether this change affects the pore space capable to store plant available water. In this study, we characterized biochar poro…

porosityMaterials scienceFOS: Physical sciencesApplied Physics (physics.app-ph)010501 environmental sciencesRaw materialkuivatislaus01 natural sciencesAnalytical ChemistryhuokoisuusAdsorptionimage analysisBiocharmedicinebiocharta216CharcoalPorosityta2180105 earth and related environmental sciencesCondensed Matter - Materials Sciencex-ray tomographybiohiilita114Materials Science (cond-mat.mtrl-sci)Physics - Applied Physics04 agricultural and veterinary sciencesAtmospheric temperature rangeslow pyrolysisWater retentionFuel TechnologykuvantaminenChemical engineeringvisual_artkuva-analyysi040103 agronomy & agriculturevisual_art.visual_art_medium0401 agriculture forestry and fisheriesmedicine.symptomPyrolysis
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El acoso escolar y su relación con las características físicas y el posicionamiento social observado a través de la teoría de grafos: un análisis exp…

2020

ente trabajo de investigación realiza un análisis exploratorio acerca del acoso escolar y el ciberacoso y su relación con el posicionamiento social y las características físicas, dentro del ámbito territorial de la comunidad valenciana. La investigación se centra en averiguar los niveles de acoso existentes actualmente en los cursos de 1º y 2º de secundaria en institutos públicos, observar las relaciones sociales de cada una de las clases analizadas y averiguar la inferencia existente entre los datos de autopercepción del acoso, el posicionamiento social, y las características físicas, a través del prisma de la teoría de grafos. Dicha teoría permite modelar un problema o una situación a tra…

posicionamiento socialcaracterísticas físicas:PEDAGOGÍA [UNESCO]acoso escolarUNESCO::PEDAGOGÍAteoria de grafos
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