Search results for "Gamma"

showing 10 items of 3093 documents

Semi-automatic Brain Lesion Segmentation in Gamma Knife Treatments Using an Unsupervised Fuzzy C-Means Clustering Technique

2016

MR Imaging is being increasingly used in radiation treatment planning as well as for staging and assessing tumor response. Leksell Gamma Knife (R) is a device for stereotactic neuro-radiosurgery to deal with inaccessible or insufficiently treated lesions with traditional surgery or radiotherapy. The target to be treated with radiation beams is currently contoured through slice-by-slice manual segmentation on MR images. This procedure is time consuming and operator-dependent. Segmentation result repeatability may be ensured only by using automatic/semi-automatic methods with the clinicians supporting the planning phase. In this paper a semi-automatic segmentation method, based on an unsuperv…

Computer scienceGamma knifeBrain lesions Gamma knife treatments MR imaging Semi-automatic segmentation Unsupervised FCM clusteringFuzzy logicBrain lesions; Gamma knife treatments; MR imaging; Semi-automatic segmentation; Unsupervised FCM clustering030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineComputer visionSegmentationRadiation treatment planningCluster analysisSettore ING-INF/05 - Sistemi Di Elaborazione Delle InformazioniSemi-automatic segmentationBrain lesionsbusiness.industryMr imagingUnsupervised FCM clusteringBrain lesionGamma knife treatmentBrain lesionsSemi automaticArtificial intelligencebusinessGamma knife treatments030217 neurology & neurosurgeryMR imaging
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Error mitigation using RaptorQ codes in an experimental indoor free space optical link under the influence of turbulence

2015

In free space optical (FSO) communications, several factors can strongly affect the link quality. Among them, one of the most important impairments that can degrade the FSO link quality and its reliability even under the clear sky conditions consists of optical turbulence. In this work, the authors investigate the generation of both weak and moderate turbulence regimes in an indoor environment to assess the FSO link quality. In particular, they show that, due to the presence of the turbulence, the link experiences both erasure errors and packet losses during transmission, and also compare the experimental statistical distribution of samples with the predicted Gamma Gamma model. Furthermore,…

Computer scienceOptical linkReliability (computer networking)Optical linksTelecommunication network reliabilityRytov variance valueSettore ING-INF/01 - ElettronicaTelecomunicacióRaptorQ codesRedundancy (information theory)Indoor free space optical linkFSO communicationsStatisticsTEORIA DE LA SEÑAL Y COMUNICACIONESRedundancy (engineering)Gamma Gamma modelrateless codeElectrical and Electronic Engineeringpacket error rate (PER)Error-free transmissionNetwork packetbusiness.industrySettore ING-INF/03 - TelecomunicazioniSettore ING-INF/02 - Campi ElettromagneticiÒpticaComputer Science ApplicationsTransmission (telecommunications)Bit error rateErasureProbability distributionFree Space Optical (FSO) communicationTelecommunicationsbusinessOptical turbulenceFSO link reliabilityindoor linkError mitigation
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"Table 2" of "Measurement of the shape of the boson transverse momentum distribution in p anti-p ---> Z / gamma* ---> e+ e- + X events produced…

2008

Correlation matrix for all rapidity Z bosons for the 12 bins used for PT < 30.

Condensed Matter::Quantum GasesInclusiveZ ProductionElectron productionPBAR P --> E+ E- XCORRHigh Energy Physics::PhenomenologyPBAR P --> GAMMA* XAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics::Data Analysis; Statistics and ProbabilityPBAR P --> Z0 X
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Hartree-Fock-Bogoliubov theory of polarized Fermi systems

2008

Condensed Fermi systems with an odd number of particles can be described by means of polarizing external fields having a time-odd character. We illustrate how this works for Fermi gases and atomic nuclei treated by density functional theory or Hartree-Fock-Bogoliubov (HFB) theory. We discuss the method based on introducing two chemical potentials for different superfluid components, whereby one may change the particle-number parity of the underlying quasiparticle vacuum. Formally, this method is a variant of non-collective cranking, and the procedure is equivalent to the so-called blocking. We present and exemplify relations between the two-chemical-potential method and the cranking approxi…

Condensed Matter::Quantum GasesPhysicsNuclear TheoryCondensed Matter - SuperconductivityNuclear TheoryHartree–Fock methodFOS: Physical sciencesAtomic and Molecular Physics and OpticsSuperconductivity (cond-mat.supr-con)Nuclear Theory (nucl-th)SuperfluidityQuantum mechanicsQuantum electrodynamicsAtomic nucleusQuasiparticleParity (mathematics)Nuclear theoryFermi Gamma-ray Space TelescopePhysical Review A
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Ultracold atomic Bose and Fermi spinor gases in optical lattices

2006

We investigate magnetic properties of Mott-insulating phases of ultracold Bose and Fermi spinor gases in optical lattices. We consider in particular the F=2 Bose gas, and the F=3/2 and F=5/2 Fermi gases. We derive effective spin Hamiltonians for one and two atoms per site and discuss the possibilities of manipulating the magnetic properties of the system using optical Feshbach resonances. We discuss low temperature quantum phases of a 87Rb gas in the F=2 hyperfine state, as well as possible realizations of high spin Fermi gases with either 6Li or 132Cs atoms in the F=3/2 state, and with 173Yb atoms in the F=5/2 state.

Condensed Matter::Quantum GasesPhysicseinstein condensationSpinorBose gasCondensed matter physicsFOS: Physical sciencesGeneral Physics and Astronomyresonant lightQuantum phasesState (functional analysis)quantum phasesCondensed Matter - Other Condensed Matterground-statesone bosonssystemsddc:530Condensed Matter::Strongly Correlated ElectronsantiferromagnetsDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHyperfine structureOther Condensed Matter (cond-mat.other)Spin-½Fermi Gamma-ray Space TelescopeNew Journal of Physics
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Flat Bands and Salient Experimental Features Supporting the Fermion Condensation Theory of Strongly Correlated Fermi

2020

The physics of strongly correlated Fermi systems, being the mainstream topic for more than half a century, still remains elusive. Recent advancements in experimental techniques permit to collect important data, which, in turn, allow us to make the conclusive statements about the underlying physics of strongly correlated Fermi systems. Such systems are close to a special quantum critical point represented by topological fermion-condensation quantum phase transition which separates normal Fermi liquid and that with a fermion condensate, forming flat bands. Our review paper considers recent exciting experimental observations of universal scattering rate related to linear temperature dependence…

Condensed Matter::Quantum GasesQuantum phase transitionSuperconductivityPhysicsNuclear and High Energy PhysicsCondensed matter physics010308 nuclear & particles physicsFermion01 natural sciencesAtomic and Molecular Physics and OpticsElectrical resistivity and conductivityQuantum critical pointScattering rate0103 physical sciencesFermi liquid theory010306 general physicsFermi Gamma-ray Space TelescopePhysics of Atomic Nuclei
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Nrg1 haploinsufficiency alters inhibitory cortical circuits

2021

Neuregulin 1 (NRG1) and its receptor ERBB4 are schizophrenia (SZ) risk genes that control the development of both excitatory and inhibitory cortical circuits. Most studies focused on the characterization ErbB4 deficient mice. However, ErbB4 deletion concurrently perturbs the signaling of Nrg1 and Neuregulin 3 (Nrg3), another ligand expressed in the cortex. In addition, NRG1 polymorphisms linked to SZ locate mainly in non-coding regions and they may partially reduce Nrg1 expression. Here, to study the relevance of Nrg1 partial loss-of-function in cortical circuits we characterized a recently developed haploinsufficient mouse model of Nrg1 (Nrg1tm1Lex). These mice display SZ-like behavioral d…

Cortical neuronsReceptor ErbB-4Neuregulin-1Gene ExpressionneuronsNeurosciences. Biological psychiatry. NeuropsychiatryHaploinsufficiencyBiologyInhibitory postsynaptic potentialHippocampusMagnetic&nbspMiceInterneuronsNeuregulin 3mental disordersMagnetic resonance spectroscopyAnimalsRNA MessengerneurotransmissionNeuregulin 1GABAergic Neuronsgamma-Aminobutyric AcidInhibitory&nbspCerebral CortexNrg1resonance spectroscopyNeural InhibitionMagnetic Resonance ImagingCortex (botany)Inhibitory neurotransmissionParvalbuminsNeurologyInhibitory Postsynaptic PotentialsCalbindin 2Vesicular Glutamate Transport Protein 1biology.proteinExcitatory postsynaptic potentialSchizophreniaCalretininHaploinsufficiencyCortical&nbspNeuroscienceParvalbuminRC321-571Neurobiology of Disease
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THE MISSING LINK: MERGING NEUTRON STARS NATURALLY PRODUCE JET-LIKE STRUCTURES AND CAN POWER SHORT GAMMA-RAY BURSTS

2011

Short Gamma-Ray Bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their "central-engine" remains unknown. Considering a binary of magnetized neutron stars and solving Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~ 10^{12} G to produce an ordered poloidal field of ~ 10^{15} G along the bl…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesmagnetohydrodynamics binary neutron stars gravitational waves010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsTorusGalaxyMagnetic fieldBlack holeNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstAstrophysics - Cosmology and Nongalactic AstrophysicsThe Astrophysical Journal
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Characteristics of the diffuse astrophysical electron and Tau neutrino flux with six years of IceCube high energy cascade data

2020

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010-2015. Assuming standard oscillations, the astrophysical neutrinos in this dedicated cascade sample are dominated (∼90%) by electron and tau flavors. The flux, observed in the sensitive energy range from 16 TeV to 2.6 PeV, is consistent with a single power-law model as expected from Fermi-type acceleration of high energy particles at astrophysical sources. We find the flux spectral index to be γ=2.53±0.07 and a flux normalization for each neutrino flavor of φastro=1.66-0.27+0.25 at E0=100 TeV, in agreement with IceCube's complementary muon neutrino results and wit…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyElectronpower spectrumflux [electron]energy [particle]01 natural sciencesIceCubeNuclear physics5/3Tau neutrinomuon0103 physical scienceslow [energy]Muon neutrinoddc:530010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyflavor [neutrino]RAYSflux [neutrino]accelerationshowersoscillationPhysics and Astronomy13. Climate actionEnergy cascadePhysique des particules élémentairesastro-ph.COhigh [energy]cascade [energy]High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Shining primordial black holes

2021

We study the well-motivated mixed dark matter (DM) scenario composed of a dominant thermal WIMP, highlighting the case of $SU(2)_L$ triplet fermion "winos", with a small fraction of primordial black holes (PBHs). After the wino kinetic decoupling, the DM particles are captured by PBHs leading to the presence of PBHs with dark minihalos in the Milky Way today. The strongest constraints for the wino DM come from the production of narrow line gamma rays from wino annihilation in the Galactic Center. We analyse in detail the viability of the mixed wino DM scenario, and determine the constraints on the fraction of DM in PBHs assuming a cored halo profile in the Milky Way. We show that already wi…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayAstrophysics::High Energy Astrophysical PhenomenaastrofysiikkaDARK-MATTER ANNIHILATIONFOS: Physical sciencesmustat aukotPrimordial black holeAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicskosmologia7. Clean energy01 natural sciences114 Physical sciencesGeneral Relativity and Quantum Cosmologypimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsGalactic CenterGAMMA-RAYSCONSTRAINTSFermionHigh Energy Physics - PhenomenologyMixed dark matterMILKYHaloAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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