Search results for "Universe"

showing 10 items of 2171 documents

New Ordovician mitrates (Echinodermata, Stylophora) from the Ancenis Basin (South Armorican Domain, France): Palaeogeographic and palaeoenvironmental…

2006

8 pages; International audience; Fossil echinoderms are extremely rare in Ordovician deposits of the South Armorican Domain (SAD), a structurally complex area stacked to the Medio-North Armorican Domain during the Hercynian orogeny. Two new occurrences of mitrate stylophorans are documented in the eastern part of the SAD (Ancenis Basin). The youngest known specimen of Lagynocystis pyramidalis is described from the Schistes du Fresne Formation (Late Ordovician). Mitrocystites mitra is reported from the Pierre Meliere Formation (Middle Ordovician), and for the first time, outside of Bohemia. The presence of these two cool-adapted taxa (both abundant in the Prague Basin) in the Ancenis Basin d…

PaleontologybiologyOrdovicianStylophora[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/PaleontologyStructural basinbiology.organism_classificationGeologyDomain (software engineering)[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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First record of early Aptian Oceanic Anoxic Event 1a from the Paris Basin (France) - Climate signals on a terrigenous shelf

2021

Abstract In 2013, Andra (French National Radioactive Waste Management Agency) drilled boreholes to the south-east of the Paris Basin, to characterise Aptian and Albian clayey formations, including the ‘Argiles a Plicatules’ Formation dated as early Aptian. One of these boreholes intersected this formation with an excellent recovery allowing detailed biostratigraphy (ammonites), sedimentology, clay mineralogy, isotope geochemistry (δ13Corg) and Rock-Eval analyses to be performed. The base of the formation corresponds to transgressive dark-grey silty clays with iron oolites and plant debris indicating a coastal environment evolving up-section to upper offshore environments. Higher in the succ…

Palynology010506 paleontologyAptianTerrigenous sedimentGeochemistryPaleontology[SDU.STU]Sciences of the Universe [physics]/Earth Sciences15. Life on landBiostratigraphyengineering.material010502 geochemistry & geophysics01 natural sciencesCretaceous13. Climate actionIsotope geochemistryIlliteengineering14. Life underwaterSedimentologyGeologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences
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Les faunes d'ammonites du Pliensbachien inférieur des séries dauphinoises de la Durance (Jurassique inférieur, barrage de Serre-Ponçon, Hautes-Alpes,…

2008

21 pages; Les faunes d'ammonites du Lias et particulièrement celles du Pliensbachien inférieur ont joué un rôle important pour la compréhension du cadre stratigraphique des séries dauphinoises des chaînes subalpines méridionales (dôme de Remollon). Ces faunes n'ont pourtant jamais fait l'objet d'études paléontologiques et elles sont décrites et illustrées pour la première fois dans le présent travail. Elles comportent une vingtaine d'espèces qui attestent de l'ensemble du Pliensbachien inférieur. Elles sont peu diversifiées et présentent un cachet euroboréal affirmé et sont surtout constituées de taxons en général abondants et largement répandus dans le Nord-Ouest de l'Europe. Malgré une po…

Paléobiodiversité010506 paleontologyPliensbachien inférieurAlpes externesPaleontology010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesBiostratigraphieSpace and Planetary ScienceAmmonites[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/Paleontology0105 earth and related environmental sciencesPaléobiogéographie[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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Les ammonites du Pliensbachien et du Toarcien basal dans la carrière de la Roche Blain (Fresnay-le-Puceux, Calvados, Basse-Normandie, France). Taxono…

2008

65 pages; International audience; Résumé Ce travail étudie les riches faunes d'ammonites du Pliensbachien et de la base du Toarcien dans la localité très fossilifère de la carrière de la Roche Blain (Calvados). Une cinquantaine d'espèces pliensbachiennes, récoltées dans une douzaine de niveaux distincts sont toutes décrites et illustrées. Leur préservation est parfois remarquable. Des structures fragiles comme les péristomes ou les mégastries sont assez souvent préservées. A l'exception de deux spécimens d'affinités téthysiennes (Arieticeras cf. amalthei (Oppel, 1853) et Dactylioceras (Eodactylites) sp.), les ammonites récoltées à la Roche Blain se rattachent toutes, sans ambiguïté, aux fau…

PaléobiodiversitéPaléobiodiversité.Systématique[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/StratigraphyPliensbachien[SDV.BID.SPT]Life Sciences [q-bio]/Biodiversity/Systematics Phylogenetics and taxonomyNormandieBiostratigraphieAmmonites[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy[SDV.BID.SPT] Life Sciences [q-bio]/Biodiversity/Systematics Phylogenetics and taxonomy[SDU.STU.ST] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/PaleontologyToarcien basalBassin anglo-parisien[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/Paleontology[ SDV.BID.SPT ] Life Sciences [q-bio]/Biodiversity/Systematics Phylogenetics and taxonomy[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/PaleontologyPaléobiogéographie
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Hettangian ammonites from the old iron mine of Beauregard (Thoste, Côte-d’Or, France).

2012

The ammonite fauna of the old iron mine of Beauregard is reviewed. Only nine specimens from this locality are presently known. They are housed in the collections of the “Musée de Semur-en-Auxois”, of the “Muséum national d’Histoire naturelle” (Paris) and of the “Ecole Nationale Supérieuredes Mines” (Claude Bernard University, Lyon 1). The age, or possibly the ages, of these ammonites remain to precise in a coarsely defined time-span including the upper part of the early Hettangian and the middle Hettangian (pro parte?). These fossils, usually finely preserved, were collected during the nineteenth century thanks to intensive mining in the Thoste-Beauregard area. They are illustrated uniforml…

PaléobiodiversitéStratigraphyEarly JurassicPalaeoecologyPaléoécologieJurassique inférieurTaxonomieStratigraphieCollections paléontologiquesPalaeobiogeographyPalaeobiodiversityAmmonitesPsiloceratidae[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/PaleontologyPalaeontological collectionsTaxonomyPaléobiogéographie
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L'Exposition Universelle de Paris 1931

2009

ParisUniverselleExpositionSettore ICAR/18 - Storia Dell'Architettura
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The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

2010

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

Particle physicsAMANDA[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAMANDA; Atmospheric neutrinos; Cherenkov radiation; Neural net; Unfoldingneural netFOS: Physical sciencesAetiology screening and detection [ONCOL 5]01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsunfoldingPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov radiationHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSolar neutrino problematmospheric neutrinosCosmic neutrino backgroundNeutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Precision calculations of dark matter relic abundance

2019

The dark matter annihilation channels sometimes involve sharp resonances. In such cases the usual momentum averaged approximations for computing the DM abundance may not be accurate. We develop an easily accessible momentum dependent framework for computing the DM abundance accurately and efficiently near such features. We apply the method to the case of a singlet scalar dark matter $s$ interacting with SM through higgs portal $\lambda_{\rm hs}s^2 h^2$ and compare the results with different momentum averaged methods. The accuracy of the latter depend strongly on the strength of the elastic interactions and corrections are large if WIMP has negligible interactions beyond the main annihilatio…

Particle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Dark matterFOS: Physical sciencesKinetic energykosmologia01 natural sciencesStandard ModelMomentumpimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesphysics of the early universeCOSMIC ABUNDANCES010306 general physicsParticle Physics - PhenomenologyPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsdark matter experimentsAstronomy and Astrophysicshep-ph115 Astronomy Space scienceHigh Energy Physics - PhenomenologyHiggs bosonastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Do we have any hope of detecting scattering between dark energy and baryons through cosmology?

2020

We consider the possibility that dark energy and baryons might scatter off each other. The type of interaction we consider leads to a pure momentum exchange, and does not affect the background evolution of the expansion history. We parametrize this interaction in an effective way at the level of Boltzmann equations. We compute the effect of dark energy-baryon scattering on cosmological observables, focusing on the Cosmic Microwave Background (CMB) temperature anisotropy power spectrum and the matter power spectrum. Surprisingly, we find that even huge dark energy-baryon cross-sections $\sigma_{xb} \sim {\cal O}({\rm b})$, which are generically excluded by non-cosmological probes such as col…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)cosmic background radiationAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologycosmic background radiation cosmological parameters cosmology observations dark energy large-scale structure of UniverseHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencescosmological parametersdark energy010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Matter power spectrumSpectral densityAstronomy and AstrophysicsCosmic varianceHigh Energy Physics - Phenomenologyobservations13. Climate actionSpace and Planetary ScienceDark energylarge-scale structure of UniversecosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Toward (finally!) ruling out Z and Higgs mediated dark matter models

2016

In recent years, direct detection, indirect detection, and collider experiments have placed increasingly stringent constraints on particle dark matter, exploring much of the parameter space associated with the WIMP paradigm. In this paper, we focus on the subset of WIMP models in which the dark matter annihilates in the early universe through couplings to either the Standard Model $Z$ or the Standard Model Higgs boson. Considering fermionic, scalar, and vector dark matter candidates within a model-independent context, we find that the overwhelming majority of these dark matter candidates are already ruled out by existing experiments. In the case of $Z$ mediated dark matter, the only scenari…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectDark matterScalar (mathematics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsUniversePseudoscalarHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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