Search results for "INOS"

showing 10 items of 2075 documents

Cytosolic Ca2+ and Phosphoinositide Hydrolysis Linked to Constitutively Active α1d-Adrenoceptors in Vascular Smooth Muscle

2003

In the present study, we analyzed changes in intracellular Ca2+ levels and inositol phosphate accumulation related to a population of alpha 1d-adrenoceptors in rat aorta resembling constitutively active receptors. Following intracellular Ca2+ store depletion by noradrenaline in Ca2+-free medium and removal of the agonist, restoration of extracellular Ca2+ induced four signals: a biphasic (transient and sustained) increase in [Ca2+]i, inositol phosphate accumulation, and a contractile response in the aorta. The transient increase in Ca2+, the inositol phosphate accumulation, and the contractile response were not observed in aortae incubated with prazosin or BMY 7378 [8-[2-[4-(2-methoxyphenyl…

Guanethidinemedicine.medical_specialtyVascular smooth muscleInositol PhosphatesPopulationchemistry.chemical_elementCalciumBiologyPhosphatidylinositolsMuscle Smooth VascularAdrenergic AgentsReceptors Adrenergic alpha-1Internal medicinemedicinePrazosinExtracellularAnimalsRats WistarInositol phosphateeducationAortaPharmacologyCalcium metabolismchemistry.chemical_classificationeducation.field_of_studyHydrolysisCalcium Channel BlockersRatsEndocrinologychemistryBiophysicsMolecular MedicineCalciumIntracellularSignal Transductionmedicine.drugJournal of Pharmacology and Experimental Therapeutics
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Supplementation with d-chiro-inositol in women

2023

The world of natural compounds has been investigated with the aim of discovering possible medical applications ever since the origin of medicine. Recently, the field of gynecology has developed a growing interest regarding inositols. Inositols are cyclic polyols with a key role in many metabolic pathways. Their stability throughout the evolution of life can mark these molecules as prebiotic, due to their biochemical importance. These molecules can be classified into nine stereoisomeric compounds; among them, myo-inositol (MI) is the most important and frequent form found in nature. Inositols were first discovered in 1850 by Johanes Joseph Scherer and extracted from muscle cells, the name of…

GynecologyWomen's healthD-chiro-inositolSettore MED/40 - Ginecologia E Ostetricia
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Effects of hormonal contraception on vaginal flora, can contraceptive use lead to vulvovaginal candidiasis (VVC) or bacterial vaginosis (BV)

2016

Gynecologymedicine.medical_specialtyObstetricsbusiness.industryVaginal floraObstetrics and Gynecologymedicine.diseaseContraceptive useReproductive MedicineVulvovaginal CandidiasisHormonal contraceptionmedicineBacterial vaginosisbusinessEuropean Journal of Obstetrics & Gynecology and Reproductive Biology
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Dacriocistitis por Candida Lusitaniae

2007

espanolCaso clinico: Se presenta el caso de una mujer de 60 anos con episodios recurrentes de dacriocistitis aguda derecha que no cedian con tratamiento medico ni tras una dacriocistorrinostomia con intubacion bicanalicular. Presento tambien una dacriocistitis izquierda que requirio una dacriocistorrinostomia. Se tomaron muestras intraoperatorias y en el cultivo aparecio Candida Lusitaniae como germen responsable. Tras tratamiento topico con Anfotericina B, asociado a dacriocistorrinostomia, la clinica desaparecio. Discusion: La dacriocistitis por Candida Lusitaniae es muy rara. Cabria preguntarse si Candida Lusitaniae es el germen primario o la dacriocistitis podria ser por sobreinfeccion …

Gynecologymedicine.medical_specialtybiologyMedical treatmentbusiness.industryCandida lusitaniaemedicine.medical_treatmentDacryocystorhinostomyRight lacrimal sacTopical treatmentdacriocistitis fúngicabiology.organism_classificationmedicine.diseaseDacryocystitisOphthalmologyAntibiotic therapymedicineCandida LusitaniaebusinessAnfotericina bdacriocistitis crónicaanfotericina Bdacriocistorrinostomía
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Flower ontogeny inCapparis spinosa(Capparaceae) with special emphasis on symmetry expression

2015

The flower ontogeny of Capparis spinosa L. was studied using scanning electron microscopy (SEM) in order to shed light on the early expression of symmetry in a representative member of Capparaceae. Sepals start decussately with the abaxial and adaxial sepals, followed by the lateral ones. Petal appearance proceeds uni-directionally from the abaxial to the adaxial side. Stamens develop centrifugally on an androecial ring. Five to seven carpel lobes arise on a gynoecial ring. Monosymmetry is established in early development by the uni-directional petal appearance and is further enhanced by the acquisition of an abaxial nectary appendage and differential development of perianth organs at anthe…

GynoeciumbiologyCapparis spinosaStamenCapparaceaePlant Sciencebiology.organism_classificationSepalfood.foodfoodAnthesisBotanyPetalPerianthEcology Evolution Behavior and SystematicsNordic Journal of Botany
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Search for high-mass resonances decaying to dimuons at CDF.

2009

We present a search for high-mass neutral resonances using dimuon data corresponding to an integrated luminosity of 2.3 fb(-1) collected in pp collisions at s=1.96 TeV by the CDF II detector at the Fermilab Tevatron. No significant excess above the standard model expectation is observed in the dimuon invariant-mass spectrum. We set 95% confidence level upper limits on sigma BR(pp -> X ->mu mu), where X is a boson with spin-0, 1, or 2. Using these cross section limits, we determine lower mass limits on sneutrinos in R-parity-violating supersymmetric models, Z(') bosons, and Kaluza-Klein gravitons in the Randall-Sundrum model.

HIGH MASS RESONANCEParticle physicsFermilab TevatronTevatronGeneral Physics and AstronomyFOS: Physical sciencesddc:500.2114 Physical sciencesResonance7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsHigh Energy Physics - Experiment (hep-ex)Integrated luminosities0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsBosonsBosonPhysicsMuonMass spectrometryhep-ex010308 nuclear & particles physicsPhysicsInvariant-mass spectrum13.85.Rm 13.85.Qk 12.60.Cn 14.70.Pw 04.50.-hHigh Energy Physics::PhenomenologyConfidence levelsGravitonSupersymmetryUpper limitsSupersymmetric modelsCross sectionsRandall–Sundrum modelThe standard modelsMass spectrumCDFHigh Energy Physics::ExperimentPhysical review letters
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Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

2019

High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient so…

HIGH-ENERGY NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaPopulationGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energy0103 physical sciencesMuon neutrinoddc:530education010303 astronomy & astrophysicsPhysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyMuon010308 nuclear & particles physicsSupernovaNeutron starPhysics and Astronomy13. Climate actionPhysique des particules élémentairesHigh Energy Physics::ExperimentNeutrinoGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube

2015

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere dataset consisting primarily of nu_e and nu_tau charged current and neutral current (cascade) neutrino interactions. In the analysis presented here, a data sample of approximately 35,000 muon neutrinos from the Northern sky was extracted from data taken during 659.5 days of livetime recorded between May 2010 and May 2012. While this sample is composed primarily of neutrinos produced by cosmic ray interactions in the Earth's atmosphere, the highest energy events are inconsistent with a hypothesis of …

HIGH-ENERGY NEUTRINOSFLUXESATMOSPHERIC MUONAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesIceCube Neutrino ObservatoryRATIO0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsSolar neutrino problemPhysics and AstronomyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena
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Tau neutrinos in the next decade: from GeV to EeV

2022

Tau neutrinos are the least studied particle in the standard model. This whitepaper discusses the current and expected upcoming status of tau neutrino physics with attention to the broad experimental and theoretical landscape spanning long-baseline, beam-dump, collider, and astrophysical experiments. This whitepaper was prepared as a part of the NuTau2021 Workshop.

HIGH-ENERGY NEUTRINOSMAGNETIC-MOMENTAstrophysics and AstronomyNuclear and High Energy PhysicsRADIO PULSESPhysics::Instrumentation and Detectorstau neutrinosFOS: Physical sciencesCHERENKOV LIGHT YIELDGeV530High Energy Physics - Experimenttau neutrino theorySubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)neutrino experimentsSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Particle Physics - PhenomenologyAIR-SHOWERSLEPTON FLAVORastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)hep-exPhysicshep-phtau neutrinos; neutrino experiments; tau neutrino theorylandscapeCOSMIC-RAYSHigh Energy Physics - PhenomenologyQUANTUM-GRAVITYCHARGED-PARTICLES[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]beam dumpPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentLORENTZ VIOLATION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Experiment
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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1~TeV and 1~PeV in 641 days of data taken from 2010--2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far bel…

HIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsParticle physicsAMANDAMesonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESFOS: Physical sciencesCosmic rayAstrophysicsFLUX PREDICTIONS01 natural sciencesIceCube Neutrino ObservatoryIceCubeObservatorySEARCH0103 physical sciencesddc:530Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPERFORMANCEBLAZARSPROMPT LEPTONSGAMMA-RAYPhysics and AstronomyHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsPhysical Review D
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