0000000000979965

AUTHOR

Pinamonti M.

showing 2 related works from this author

Search for Magnetic Monopoles and Stable High-Electric-Charge Objects in 13 Tev Proton-Proton Collisions with the ATLAS Detector

2020

We thank CERN for the very successful operation of the LHC, aswell as the support staff fromour institutionswithout whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; FWF, BMWFW, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, FAPESP, Brazil; NSERC, CFI, NRC, Canada; CERN; CONICYT, Chile; CAS, NSFC, MOST, China; COLCIENCIAS, Colombia; VSC CR, MSMT CR, MPO CR, Czech Republic; DNSRC, DNRF, Denmark; IN2P3-CNRS, CEA-DRF/IRFU, France; SRNSFG, Georgia; MPG, HGF, BMBF, Germany; GSRT, Greece; RGC, Hong Kong SAR, Hong Kong China; Benoziyo Center, ISF, Israel; INFN, Italy; JSPS, MEXT, Japan; JINR; CNRST, Morocco; NWO, Nether…

electric [charge]Drell-Yan process:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Magnetic monopolesProton13000 GeV-cmsPhysics::Instrumentation and Detectorselectromagnetic [calorimeter]magnetic [charge]General Physics and Astronomy7. Clean energy01 natural scienceschannel cross section: upper limitHigh Energy Physics - Experimentmagnetic monopole: massSubatomär fysikparticle: stabilityHigh Energy Physics - Experiment (hep-ex)magnetic monopole: pair productionSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]tracking detectorstability [particle]0 [spin]1/2 [spin]Particle productionHadron collidersPhysicsRange (particle radiation)Large Hadron Colliderupper limit [channel cross section]DetectorSettore FIS/01 - Fisica Sperimentalemass [magnetic monopole]ATLAS3. Good health:Nuclear and elementary particle physics: 431 [VDP]CERN LHC Collhigh [ionization]ATLAS Detectorslower limit [mass]atlas; lhc; higgs;colliding beams [p p]pair production [magnetic monopole]Particle Physics - ExperimentsignatureDirect Productionp p: scatteringHigh-Ionizationdirect production [magnetic monopole]530 PhysicsCiências Naturais::Ciências Físicasmass: lower limit:Ciências Físicas [Ciências Naturais]Magnetic monopolespin: 0FOS: Physical sciencesLHC ATLAS High Energy Physicsddc:500.2Electromagnetic CalorimeterElectric chargeComputer Science::Digital LibrariesChargeNuclear physicsionization: high0103 physical sciencesTransition Radiation Trackersddc:530High Energy Physicsspin: 1/2010306 general physicsCiencias ExactasATLAS Collaborationcharge: magneticmagnetic monopolesS028CScience & Technologyhep-excharge: electricFísicaCharge (physics)triggerPair productioncalorimeter: electromagneticProton Proton CollisionsExperimental High Energy PhysicsMagnetic ChargesElementary Particles and FieldsHigh Energy Physics::Experimenttransition radiationHadron-hadron collisionsp p: colliding beamsmagnetic monopole: direct productionexperimental resultsPhysical Review Letters
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Abundance signature of M dwarf stars

2020

Most of our current knowledge on planet formation is still based on the analysis of main-sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M-dwarf planet hosts are still missing. We aim to test whether the correlations between the metallicity, individual chemical abundances, and mass of the star and the presence of different type of planets found for FGK stars still holds for the less massive M dwarf stars. Methods to determine in a consistent way stellar abundances of M dwarfs from high-resolution optical spectra are still missing. The present work is a first attempt to fill this gap. We analyse in a coherent and homogeneous way a large sample of M dwarf…

Astrophysics and AstronomyRadial velocityPhysicsExoplanetsChemical abundancesexoplanet astronomyAstrophysics::Cosmology and Extragalactic AstrophysicsLate type starsstellar astronomyInterdisciplinary Astronomyobservational astronomyM starsMetallicityAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesLate-type starsAstrophysics::Galaxy AstrophysicsSpectroscopy
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