Search results for "ARTICLES"

showing 10 items of 9626 documents

Questions and controversies in the study of time-varying functional connectivity in resting fMRI.

2020

The brain is a complex, multiscale dynamical system composed of many interacting regions. Knowledge of the spatiotemporal organization of these interactions is critical for establishing a solid understanding of the brain’s functional architecture and the relationship between neural dynamics and cognition in health and disease. The possibility of studying these dynamics through careful analysis of neuroimaging data has catalyzed substantial interest in methods that estimate time-resolved fluctuations in functional connectivity (often referred to as “dynamic” or time-varying functional connectivity; TVFC). At the same time, debates have emerged regarding the application of TVFC analyses to re…

confound regression strategiesComputer scienceBrain networksRest1.1 Normal biological development and functioningdynamic connectivityReviewDynamical systemlcsh:RC321-57103 medical and health sciencesFunctional connectivity0302 clinical medicineArtificial IntelligenceUnderpinning researchBehavioral and Social Sciencestate fmricognitive controlmotion correctionReview Articleslcsh:Neurosciences. Biological psychiatry. Neuropsychiatry030304 developmental biologyindividual-differencesRest (physics)0303 health sciencesApplied MathematicsGeneral NeuroscienceResting fmriFunctional connectivitytest-retest reliabilityfMRINeurosciencesComputer Science ApplicationsMental HealthNeurologicalwhole-brainNeurosciencedefault mode030217 neurology & neurosurgeryBrain dynamics
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Sp1 transcription factor interaction with accumulated prelamin a impairs adipose lineage differentiation in human mesenchymal stem cells: essential r…

2012

Abstract Lamin A (LMNA)-linked lipodystrophies may be either genetic (associated with LMNA mutations) or acquired (associated with the use of human immunodeficiency virus protease inhibitors [PIs]), and in both cases they share clinical features such as anomalous distribution of body fat or generalized loss of adipose tissue, metabolic alterations, and early cardiovascular complications. Both LMNA-linked lipodystrophies are characterized by the accumulation of the lamin A precursor prelamin A. The pathological mechanism by which prelamin A accumulation induces the lipodystrophy associated phenotypes remains unclear. Since the affected tissues in these disorders are of mesenchymal origin, we…

congenital hereditary and neonatal diseases and abnormalitiesLipodystrophySp1 Transcription FactorCellular differentiationAdipose tissueBiologyLMNAHumansProtein PrecursorsTranscription factorOriginal Articles and ReviewsAdipogenesisintegumentary systemSecretory VesiclesMesenchymal stem cellnutritional and metabolic diseasesNuclear ProteinsCell DifferentiationMesenchymal Stem CellsCell BiologyGeneral MedicineLamin Type ALipid MetabolismCell biologyExtracellular MatrixBiochemistryAdipose TissueGene Expression RegulationAdipogenesisDifferentiationMutationMesenchymal stem cellsTranscription factorStem cellExperimental modelsLaminDevelopmental BiologyStem cells translational medicine
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Musculoskeletal ultrasound in hemophilia: Results and recommendations from a global survey and consensus meeting

2021

Abstract Introduction For persons with hemophilia, optimization of joint outcomes is an important unmet need. The aim of this initiative was to determine use of ultrasound in evaluating arthropathy in persons with hemophilia, and to move toward consensus among hemophilia care providers regarding the preferred ultrasound protocols for global adaptation. Methods A global survey of hemophilia treatment centers was conducted that focused on understanding how and why ultrasound was being used and endeavored to move toward consensus definitions of both point‐of‐care musculoskeletal ultrasound (POC‐MSKUS) and full diagnostic ultrasound, terminology to describe structures being assessed by ultrasou…

congenital hereditary and neonatal diseases and abnormalitiesmedicine.medical_specialtyDiagnostic ultrasoundMusculoskeletal ultrasoundUnmet needsTerminologysurveyshemic and lymphatic diseaseshemophiliaHealth careMedicineImage acquisitionMedical physicsDiseases of the blood and blood-forming organsClinical caremusculoskeletalbusiness.industryOriginal ArticlesHematologyultrasonographyconsensus hemophilia musculoskeletal surveys ultrasonographyconsensusOriginal ArticlePatient representativesRC633-647.5businessResearch and Practice in Thrombosis and Haemostasis
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Predator mimicry, not conspicuousness, explains the efficacy of butterfly eyespots

2015

Large conspicuous eyespots on butterfly wings have been shown to deter predators. This has been traditionally explained by mimicry of vertebrate eyes, but recently the classic eye-mimicry hypothesis has been challenged. It is proposed that the conspicuousness of the eyespot, not mimicry, is what causes aversion due to sensory biases, neophobia or sensory overloads. We conducted an experiment to directly test whether the eye-mimicry or the conspicuousness hypothesis better explain eyespot efficacy. We used great tits ( Parus major ) as model predator, and tested their reaction towards animated images on a computer display. Birds were tested against images of butterflies without eyespots, wi…

conspicuousness hypothesispredator mimicryBiologyEyeGeneral Biochemistry Genetics and Molecular BiologyPredationbutterfly eyespotsSongbirdsmedicineAnimalsWings AnimalResearch ArticlesBiological MimicryGeneral Environmental ScienceParusCommunicationGeneral Immunology and MicrobiologyPigmentationbusiness.industryBiological MimicryNeophobiaAnimal colorationGeneral Medicinebiology.organism_classificationmedicine.diseasegreat titsEvolutionary biologyButterflyVisual PerceptionMimicryta1181EyespotGeneral Agricultural and Biological SciencesbusinessButterfliesProceedings of the Royal Society B: Biological Sciences
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Functionalization of nanoparticles in specific targeting and mechanism release

2017

The development of various nanotechnologies have provided a new field of research, which allows the manipulation of molecular components of matter and covers a vast array of nanodevices. The “smart” multifunctional nanostructures should work as customizable, targeted drug-delivery vehicles capable of carrying large doses of therapeutic agents into malignant cells. Some nanomedical approaches are based on the use of functionalized nanoparticles (NPs), not only to reduce toxicity and side effects of drugs but, also in potential the biological barriers crossing on, such as: the blood–brain barrier, different cellular compartments, including the nucleus. Currently, many materials are used for n…

controlled-releaseMaterials sciencefood.ingredienttechnology industry and agricultureNanoparticleNanotechnology02 engineering and technologyEPR effect010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesControlled releaseGelatin0104 chemical sciencesfoodDrug deliverySelf-healing hydrogelstargeted-nanoparticlesSurface modificationfunctionalizationChemical bindingNanocarriers0210 nano-technologyDrug-delivery system
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The effective cross section for double parton scattering within a holographic AdS/QCD approach

2017

A first attempt to apply the AdS/QCD framework for a bottom-up approach to the evaluation of the effective cross section for double parton scattering in proton-proton collisions is presented. The main goal is the analytic evaluation of the dependence of the effective cross section on the longitudinal momenta of the involved partons, obtained within the holographic Soft-Wall model. If measured in high-energy processes at hadron colliders, this momentum dependence could open a new window on 2-parton correlations in a proton.

correlation: two-particleNuclear and High Energy PhysicsParticle physicsp p: scatteringNuclear TheoryProton[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryHadronFOS: Physical sciencesParton01 natural sciences[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]quantum chromodynamics: holographyNuclear Theory (nucl-th)Nuclear physicsMomentumCross section (physics)12.38.AwHigh Energy Physics - Phenomenology (hep-ph)parton: multiple scattering0103 physical sciencesparton: correlation010306 general physicsNuclear Experimentparton: interaction[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Quantum chromodynamicsPhysicsAdS/CFT correspondence010308 nuclear & particles physicsScattering[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics::Phenomenology12.39.Kilcsh:QC1-999High Energy Physics - PhenomenologyAdS/CFT correspondence[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]14.20.DhPhysics::Accelerator Physics[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentlcsh:Physics
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Search for Cosmic Neutrino Point Sources with Four Year Data of the ANTARES Telescope

2012

In this paper, a time-integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an E ¿2 n; spectrum, these flux limits are at 1-10 ¿10¿8 GeV cm¿2 s¿1 for declinations ranging from ¿90° to 40°. Limits for specific models of RX J1713.7¿3946 and Vela X, which include information on the source morphology and spectrum, are also given.

cosmic neutrinosUNIVERSEFluxVela01 natural scienceslaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawSIGNALSABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]MAXIMUM-LIKELIHOOD010303 astronomy & astrophysicsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer database[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ASTRONOMYneutrinosastroparticle physicsFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaREMNANT RX J1713.7-3946Particle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescope[SDU.STU]Sciences of the Universe [physics]/Earth SciencesFOS: Physical sciencesddc:500.2Telescopeneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesPoint (geometry)ALGORITHMNeutrinosDETECTORCosmic raysUNDERWATER CHERENKOV NEUTRINO TELESCOPES010308 nuclear & particles physicsAstronomy and AstrophysicsHIGH-ENERGY PHOTONSSpace and Planetary ScienceFISICA APLICADAAstroparticle physics
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A strong electroweak phase transition from the inflaton field

2016

We study a singlet scalar extension of the Standard Model. The singlet scalar is coupled non-minimally to gravity and assumed to drive inflation, and also couple sufficiently strongly with the SM Higgs field in order to provide for a strong first order electroweak phase transition. Requiring the model to describe inflation successfully, be compatible with the LHC data, and yield a strong first order electroweak phase transition, we identify the regions of the parameter space where the model is viable. We also include a singlet fermion with scalar coupling to the singlet scalar to probe the sensitivity of the constraints on additional degrees of freedom and their couplings in the singlet sec…

cosmological inflationParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelScalar (mathematics)Degrees of freedom (physics and chemistry)FOS: Physical sciences01 natural sciences7. Clean energyStandard ModelGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsInflatonextensions of the Standard ModelHiggs fieldHigh Energy Physics - Phenomenologyelectroweak phase transitionAstrophysics - Cosmology and Nongalactic Astrophysics
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Status of Advanced Virgo

2017

The LIGO and the Virgo collaborations have recently announced the first detections of Gravitational Waves. Due to their weak amplitude, Gravitational Waves are expected to produce a very small effect on free-falling masses, which undergo a displacement of the order of 10-18 m for a Km-scale mutual distance. This discovery showed that interferometric detectors are suitable to reveal such a feeble effect, and therefore represent a new tool for astronomy, astrophysics and cosmology in the understanding of the Universe. To better reconstruct the position of the Gravitational Wave source and increase the signal-to-noise ratio of the events by means of multiple coincidence, a network of detectors…

cosmological modeldetector: performanceVirgo LIGO gravitational waveAstronomyinterferometerQC1-999detector: networkgravitational radiation: direct detection01 natural sciencesCoincidenceCosmologyPhysics and Astronomy (all)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGO010306 general physicsSettore FIS/01Physics010308 nuclear & particles physicsGravitational wavePhysicsDetectorgravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygravitational radiation detectorLIGOdetector: sensitivityInterferometryVIRGOAmplitudePhysics and Astronomygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

2019

Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing str…

cosmological neutrinosAstronomyFluxAstrophysics01 natural sciences7. Clean energycosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic rayssurface [detector]Ultra-high-energy cosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)cosmological neutrinoSettore FIS/01 - Fisica SperimentaleDETETORESneutrino: UHEUHE [neutrino]Augerobservatorytrajectoryneutrino: flavorProduction (computer science)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencescosmic ray experimentCosmic rayultra high energy cosmic raysneutrino: productionneutrino astronomyproduction [neutrino]TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530model [neutrino]High Energy Physicscosmic radiation: UHEZenithAstrophysiqueneutrino: modelPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsdetector: surfaceHigh Energy Physics::Phenomenologyflavor [neutrino]Astronomy and AstrophysicsAstronomiefluxExperimental High Energy PhysicsatmosphereHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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