Search results for "Dwarf"

showing 10 items of 136 documents

Palaeogeographical evolution of the Egadi Islands (western Sicily, Italy). Implications for late Pleistocene and early Holocene sea crossings by huma…

2019

Abstract The continental shelf morphology offshore of western Sicily suggests that during the Last Glacial Maximum (LGM, 20 ka cal BP), two of the Egadi Islands, Favignana and Levanzo, were connected to Sicily by a wide emerged plain, while Marettimo was only separated from the other islands by a narrow channel. We studied the relative sea-level variation from the LGM until today, focussing on two important time slices: the Mesolithic (9.5–13 ka cal BP) and the Neolithic (6.5–7.5 ka cal BP). In this research, we discuss a sea-level rise model by means of geomorphological, archaeological and geophysical observations and new radiocarbon dating of marine and terrestrial fossil fauna. The resul…

Mediterranean climatePalaeoshorelineDwarf elephantsSettore GEO/02 - Geologia Stratigrafica E Sedimentologica010504 meteorology & atmospheric sciencesPleistoceneSettore GEO/03 - Geologia StrutturaleFaunaDwarf elephants; Egadi archipelago; Food remains; Mammals; Marine geological data; Mediterranean voyaging; Palaeogeographical reconstruction; Palaeoshorelines; Vertical tectonic movements010502 geochemistry & geophysics01 natural sciencesMammallaw.inventionPaleontologylawVertical tectonic movementMediterranean voyagingRadiocarbon datingPalaeoshorelinesMesolithicHolocene0105 earth and related environmental sciencesMammalsgeographygeography.geographical_feature_categoryContinental shelfLast Glacial MaximumFood remainDwarf elephantPalaeogeographical reconstructionGeneral Earth and Planetary SciencesFood remainsMarine geological dataEgadi archipelagoEarth and Planetary Sciences (all)Vertical tectonic movementsEarth-Science Reviews
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Morphological and genetic variation of Chamaerops humilis (Arecaceae) in relation to the altitude

2021

The Mediterranean dwarf palm (Chamaerops humilis L.) is native to Western and Central Mediterranean. Since classical times this species has been cultivated and several varieties have been described on material of unknown origins. In this study, plants grown from seeds collected in the wild from seven populations spread along the Mediterranean basin were cultivated under the same environmental conditions, investigated morphologically and genetically by screening the polymorphism of ten SSR loci. Two groups are clearly separated, the populations growing at low altitudes and those living above a thousand meters of altitude. Due to morphological, geographic and environmental isolation, here it …

Moroccodwarf fan palmlcsh:Biology (General)lcsh:CytologySettore AGR/07 - Genetica AgrariamorphologyEuropean fan palmfood and beverageslcsh:QH573-671lcsh:QH301-705.5SSR markerdiversity
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Systematic uncertainties from halo asphericity in dark matter searches

2015

Although commonly assumed to be spherical, dark matter halos are predicted to be non-spherical by N-body simulations and their asphericity has a potential impact on the systematic uncertainties in dark matter searches. The evaluation of these uncertainties is the main aim of this work, where we study the impact of aspherical dark matter density distributions in Milky-Way-like halos on direct and indirect searches. Using data from the large N-body cosmological simulation Bolshoi, we perform a statistical analysis and quantify the systematic uncertainties on the determination of local dark matter density and the so-called $J$ factors for dark matter annihilations and decays from the galactic …

N-body SimulationsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayDwarf galaxy problemDark matterScalar field dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMany-body problemHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesDark matter010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsPotential impactAnnihilation010308 nuclear & particles physicsHot dark matterGalactic CenterAstronomyAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestriaxial halosDark matter haloHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Cuspy halo problemHaloDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for dark matter from the Galactic halo with the IceCube neutrino telescope

2011

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004
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IceCube search for dark matter annihilation in nearby galaxies and galaxy clusters

2013

Physical review / D 88(12), 122001 (2013). doi:10.1103/PhysRevD.88.122001

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy merger53001 natural sciencesSIGNALSGalaxy group0103 physical sciencesPARTICLESHALOESddc:530Interacting galaxy010306 general physicsGalaxy clusterAstrophysics::Galaxy AstrophysicsDwarf galaxyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomyCONSTRAINTSGalaxyEVOLUTIONPhysics and AstronomyElliptical galaxyHigh Energy Physics::ExperimentDark galaxyAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Is it possible to explore Peccei-Quinn axions from frequency dependence radiation dimming?

2011

Abstract We explore how the Peccei–Quinn (PQ) axion parameter space can be constrained by the frequency-dependence dimming of radiation from astrophysical objects. To do so we perform accurate calculations of photon–axion conversion in the presence of a variable magnetic field. We propose several tests where the PQ axion parameter space can be explored with current and future astronomical surveys: the observed spectra of isolated neutron stars, occultations of background objects by white dwarfs and neutron stars, the light-curves of eclipsing binaries containing a white dwarf. We find that the lack of dimming of the light-curve of a detached eclipsing white dwarf binary recently observed, l…

Nuclear and High Energy PhysicsBinary numberAstrophysicsParameter spaceAstronomical survey01 natural sciencesSpectral linePartícules (Física nuclear)Planet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAxionParticles (Nuclear physics)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomyWhite dwarfEstels nansCromodinàmica quànticaNeutron starDwarf starsAstrophysics::Earth and Planetary AstrophysicsQuantum chromodynamics
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A systematic study of hidden sector dark matter: application to the gamma-ray and antiproton excesses

2020

In hidden sector models, dark matter does not directly couple to the particle content of the Standard Model, strongly suppressing rates at direct detection experiments, while still allowing for large signals from annihilation. In this paper, we conduct an extensive study of hidden sector dark matter, covering a wide range of dark matter spins, mediator spins, interaction diagrams, and annihilation final states, in each case determining whether the annihilations are s-wave (thus enabling efficient annihilation in the universe today). We then go on to consider a variety of portal interactions that allow the hidden sector annihilation products to decay into the Standard Model. We broadly class…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsCosmology of Theories beyond the SMGalaxyUniverseDwarf spheroidal galaxyHidden sectorHigh Energy Physics - PhenomenologyAntiprotonBeyond Standard Modellcsh:QC770-798Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Theoretical profiles of the Mg + resonance lines perturbed by collisions with He

2016

International audience; The effects of collision broadening by He are central to understanding the opacity of cool stellar atmospheres. Aims. DZ white dwarfs show metal lines which are, in many cases, believed to come from some rocky material, a remnant of a former exoplanetary system. The analysis of the Mg + resonance lines is a valuable method to determine the chemical abundances in these systems. Methods. Unified profiles of the strongest of the UV lines of Mg + have been calculated in the semi-classical approach using very recent ab initio potential energies. Results. We present the first theoretical line profile calculations of the resonance lines of Mg + that have been perturbed by h…

Opacity[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ab initiochemistry.chemical_elementAstrophysics01 natural sciencesResonance (particle physics)Metal0103 physical sciencesstars: atmospheresAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsHeliumAstrophysics::Galaxy AstrophysicsLine (formation)white dwarfsPhysicsStellar atmosphereWhite dwarfAstronomy and Astrophysicsline: profileschemistry13. Climate actionSpace and Planetary Sciencevisual_artvisual_art.visual_art_mediumAstrophysics::Earth and Planetary AstrophysicsAtomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A syntaxonomical survey of the Sicilian dwarf shrub vegetation belonging to the class Rumici-Astragaletea siculi

2005

Basing on literature data and unpublished relevés from Sicily, a survey of the syntaxa belonging to the class Rumici-Astragaletea siculi Pignatti & Nimis 1980 em. Mucina 1997 (= Cerastio-Carlinetea nebrodensis Brullo 1984) is presented. The class groups orophilous plant communities dominated by dwarf- shrubs, often with a pulvinate and thorny growth form. The class is represented in Sicily by two orders: Rumici-Astragaletalia siculi Pignatti & Nimis 1980, including the sole alliance Rumici-Astragalion siculi Poli 1965, restricted to Mount Aetna, and Erysimo-Jurinetalia bocconei Brullo 1984, including two alliances: the acidophilous Armerion nebrodensis Brullo 1984 and the basiphilous Cerast…

PHYTOSOCIOLOGYRUMICI-ASTRAGALETEA SICULIlcsh:BotanyOROPHILOUS VEGETATION DWARF SHRUBMountain vegetation dwarf-shrubs Phytosociology syntaxonomy SicilySettore BIO/03 - Botanica Ambientale E ApplicataSICILYlcsh:QK1-989
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Osteodysplastic primordial dwarfism (ODPD): notes on brain imaging

1998

Pathologymedicine.medical_specialtyNeuroimagingmedicineOsteodysplastic primordial dwarfismBiologyGenetics (clinical)American Journal of Medical Genetics
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