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Quantitative EEG during Early Recovery from Hypoxic-Ischemic Injury in Immature Piglets: Burst Occurrence and Duration

1999

This study examined the course of EEG recovery in an animal model of hypoxic-ischemic injury. The model used periods of hypoxia, room air and asphyxia to induce cardiac arrest. One-week-old piglets (n = 16) were exposed to a period of hypoxia, room air and complete asphyxia for 7 minutes. After cardiac arrest and resuscitation, two EEG features were evaluated as prognostic indicators of behavioral outcome as assessed by a neuroscore at 24 hours after insult. A prominent EEG feature was the number and duration of bursts evident during recovery. Episodes of bursting were detected through the thresholds on sustained periods of elevated power. After the animal was resuscitated, the EEG was moni…

AsphyxiaResuscitationmedicine.diagnostic_testSwinebusiness.industryElectroencephalographyElectroencephalographyHypoxia (medical)030227 psychiatryQuantitative eeg03 medical and health sciencesBursting0302 clinical medicineAnimal modelAnimals NewbornAnesthesiaHypoxia-Ischemia BrainRoom air distributionmedicineAnimalsNeurology (clinical)medicine.symptombusiness030217 neurology & neurosurgeryClinical Electroencephalography
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Reconstruction of inclined air showers detected with the Pierre Auger Observatory

2014

We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles greater than $60^\circ$ detected with the surface array of the Pierre Auger Observatory. The measured signals at the ground level are fitted to muon density distributions predicted with atmospheric cascade models to obtain the relative shower size as an overall normalization parameter. The method is evaluated using simulated showers to test its performance. The energy of the cosmic rays is calibrated using a sub-sample of events reconstructed with both the fluorescence and surface array techniques. The reconstruction method described here provides the basis of complementary analyses including an…

AstrofísicaAstronomyCiencias Físicas01 natural sciencesultra high energy cosmic rayHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]ENERGYHigh Energy Physics - Experiment (hep-ex)EXPERIMENTS[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]HIGHPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCascadeComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASNormalization (statistics)[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]COSMICAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesEnergy spectrum010306 general physicsULTRAZenithShower reconstructionPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Ultra-high energy cosmic raysRAYSComputational physicsAstronomíaInclined extensive air showersExperimental High Energy Physicscosmic ray experiments[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

2014

The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60° and different energies of the primary particle. From these distributions, we define Xμmax as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of Xμmax as a useful observable to infer the mass compositi…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyCiencias Físicasmuonshadronic interaction modelsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentAuger//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Air showersProduction depthSURFACE DETECTOR ARRAY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh-Energy Cosmic Rays[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Pierre Auger ObservatoryObservableInstrumentation and Detectors (physics.ins-det)COSMIC-RAYSlongitudinal developmentCore (optical fiber)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayNuclear physicscosmic rays[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesextensive air showers[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Física//purl.org/becyt/ford/1.3 [https]ASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaMODELExperimental High Energy PhysicsHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]muonic componentSYSTEM
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Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

2012

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargüe and averaged monthly models, the utility of the GDAS data is shown.

AstronomyAtmospheric modelAtmospheric monitoringAtmospheric sciencesCosmic Rays Shower01 natural scienceslaw.inventionData assimilationlawcosmic rays; extensive air showers; atmospheric monitoring; atmospheric modelsDEPENDENCEATMOSFERA (OBSERVAÇÃO)TEMPERATUREPhysics::Atmospheric and Oceanic PhysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]Cascada atmosférica extensaOPTICAL DEPTH[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryAtmospheric temperatureRadiación cósmicaAtmosphere of EarthComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRadiosondeFísica nuclearREFRACTIVE-INDEXAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]MeteorologyAtmospheric MonitoringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic Rays ShowersEXTENSIVE AIR-SHOWERSCosmic RayAtmósferaWeather stationAtmospheric models0103 physical sciencesExtensive air showers010306 general physicsCosmic raysDETECTORCiencias ExactasPierre Auger ObservatoryAtmospheric models010308 nuclear & particles physicsFísicaAstronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsEMISSION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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PBH assisted search for QCD axion dark matter

2022

The entropy production prior to BBN era is one of ways to prevent QCD axion with the decay constant $F_{a}\in[10^{12}{\rm GeV},10^{16}{\rm GeV}]$ from overclosing the universe when the misalignment angle is $\theta_{\rm i}=\mathcal{O}(1)$. As such, it is necessarily accompanied by an early matter-dominated era (EMD) provided the entropy production is achieved via the decay of a heavy particle. In this work, we consider the possibility of formation of primordial black holes during the EMD era with the assumption of the enhanced primordial scalar perturbation on small scales ($k>10^{4}{\rm Mpc}^{-1}$). In such a scenario, it is expected that PBHs with axion halo accretion develop to ultracomp…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)axionsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmustat aukotAstrophysics::Cosmology and Extragalactic Astrophysicshiukkasfysiikkakosmologianeutron starspimeä aineHigh Energy Physics - Phenomenology (hep-ph)neutronitähdetParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEdark matter experimentsHigh Energy Physics::Phenomenologyprimordial black holesAstronomy and Astrophysicshep-phHigh Energy Physics - Phenomenologyastro-ph.COkvanttiväridynamiikkaHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Electroweak baryogenesis from a dark sector

2017

Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ lepto…

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)standard model of particle physicsPhysics beyond the Standard ModelSTANDARD MODELFOS: Physical sciences01 natural sciences7. Clean energy114 Physical sciencesdark matterHiggs sectorStandard Modelpimeä aineHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesSINGLET010306 general physicsParticle Physics - PhenomenologyPhysicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalliRADIATIVE NEUTRINO MASShep-phSphaleronBaryogenesisHigh Energy Physics - Phenomenologyastro-ph.COHiggs bosonPHASE-TRANSITIONHigh Energy Physics::ExperimentMATTERAstrophysics - Cosmology and Nongalactic Astrophysics
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Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E > 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
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Mixed-Phase Clouds: Progress and Challenges

2017

Mixed-phase clouds represent a three-phase colloidal system consisting of water vapor, ice particles, and coexisting supercooled liquid droplets. Mixed-phase clouds are ubiquitous in the troposphere, occurring at all latitudes from the polar regions to the tropics. Because of their widespread nature, mixed-phase processes play critical roles in the life cycle of clouds, precipitation formation, cloud electrification, and the radiative energy balance on both regional and global scales. Yet, in spite of many decades of observations and theoretical studies, our knowledge and understanding of mixed-phase cloud processes remains incomplete. Mixed-phase clouds are notoriously difficult to represe…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologybusiness.industryEarth scienceCloud physicsCloud computing010502 geochemistry & geophysicsOceanographyNumerical weather prediction01 natural sciencesTroposphere13. Climate actionInternational Satellite Cloud Climatology Projectddc:550Clouds; Aircraft observations; Lidars/Lidar observations; Microwave observations; Radars/Radar observations; Climate modelsEnvironmental scienceClimate modelPrecipitationbusinessWater vaporAstrophysics::Galaxy AstrophysicsPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciences
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Intercomparison and evaluation of global aerosol microphysical properties among AeroCom models of a range of complexity

2014

Many of the next generation of global climate models will include aerosol schemes which explicitly simulate the microphysical processes that determine the particle size distribution. These models enable aerosol optical properties and cloud condensation nuclei (CCN) concentrations to be determined by fundamental aerosol processes, which should lead to a more physically based simulation of aerosol direct and indirect radiative forcings. This study examines the global variation in particle size distribution simulated by 12 global aerosol microphysics models to quantify model diversity and to identify any common biases against observations. Evaluation against size distribution measurements from…

Atmospheric Science010504 meteorology & atmospheric sciencesParticle numbergeneral-circulation modelmixing state010501 environmental sciencesEnvironmentclimate modelblack carbonAtmospheric sciences01 natural sciencesTropospherelcsh:ChemistryZeppelinobservatorietUrban Developmentddc:550Cloud condensation nucleiBuilt Environmentnumber size distributionsPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesMicrophysicsparticle formationEarth / EnvironmentalCloud physicsatmospheric aerosolCAS - Climate Air and SustainabilityRadiative forcinglcsh:QC1-999Aerosolcloud condensation nucleimarine boundary-layerlcsh:QD1-99913. Climate actionClimatologyEnvironmental scienceClimate modelELSS - Earth Life and Social Sciencesoff-line modellcsh:Physics
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Aviation Contrail Cirrus and Radiative Forcing Over Europe During 6 Months of COVID‐19

2021

Abstract The COVID‐19 pandemic led to a 72% reduction of air traffic over Europe in March–August 2020 compared to 2019. Modeled contrail cover declined similarly, and computed mean instantaneous radiative contrail forcing dropped regionally by up to 0.7 W m−2. Here, model predictions of cirrus optical thickness and the top‐of‐atmosphere outgoing longwave and reflected shortwave irradiances are tested by comparison to Meteosat‐SEVIRI‐derived data. The agreement between observations and modeled data is slightly better when modeled contrail cirrus contributions are included. The spatial distributions and diurnal cycles of the differences in these data between 2019 and 2020 are partially caused…

Atmospheric Science010504 meteorology & atmospheric sciencesPollution: Urban Regional and GlobalcirrusForcing (mathematics)Atmospheric Composition and Structure010502 geochemistry & geophysicsAtmospheric sciencesBiogeosciences01 natural sciencesOceanography: Biological and ChemicalCloud/Radiation InteractionRadiative transferWolkenphysikInstitut für Physik der AtmosphäreMarine PollutioncontrailOceanography: GeneralGeophysicsPollution: Urban and RegionalAtmospheric ProcessesCirrusClouds and AerosolssatelliteMegacities and Urban Environmentcontrail aircraft climate observation model traffic Meteosat CoCiPRadiation: Transmission and ScatteringAtmospherePaleoceanographyEvolution of the EarthCOVID‐19Research LetterGlobal ChangeBiosphere/Atmosphere InteractionsUrban Systems0105 earth and related environmental sciencesEvolution of the AtmosphereAerosolsradiative forcingVerkehrsmeteorologieAtmosphereLongwaveAtmosphärische SpurenstoffeRadiative forcingAerosols and ParticlesNumerical weather predictionTectonophysicsaviationGeneral Earth and Planetary SciencesEnvironmental scienceShortwaveNatural HazardsGeophysical Research Letters
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