Search results for " format"

showing 10 items of 2156 documents

Study of J/$\psi$ production in p-U, O-U and S-U interactions at 200 GeV per nucleon

1991

Abstract In a search for quark-gluon plasma formation, the production of J/ψ and muon pairs in the mass continuum region is studied in oxygen-uranium and sulphur-uranium interactions. The yield of J/ψ relative to the continuum is measured to be a decreasing function of the neutral transverse energy produced in the collision, i.e. of the energy density. A comparison is made with proton-uranium reactions.

PhysicsNuclear and High Energy PhysicsParticle physicsMuonPlasma formation010308 nuclear & particles physicsContinuum (design consultancy)7. Clean energy01 natural sciencesNuclear physicsYield (chemistry)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesEnergy densityProduction (computer science)Nuclear Experiment010306 general physicsNucleon
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Fitting Simpson's neutrino into the standard model

1985

Abstract I show how to accomodate the 17 keV state recently reported by Simpson as one of the neutrinos of the standard model. Experimental constraints can only be satisfied if the μ and τ neutrino combine to a very good approximation to form a Dirac neutrino of 17 keV leaving a light ν e . Neutrino oscillations will provide the most stringent test of the model. The cosmological bounds are also satisfied in a natural way in models with Goldstone bosons. Explicit examples are given in the framework of majoron-type models. Constraints on the lepton symmetry breaking scale which follow from astrophysics, cosmology and laboratory experiments are discussed.

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsDirac (video compression format)Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaStandard ModelGoldstone bosonMeasurements of neutrino speedHigh Energy Physics::ExperimentSymmetry breakingNeutrinoNeutrino oscillationParticle Physics - PhenomenologyLepton
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Neutrinos as the messengers of CPT violation

2001

CPT violation has the potential to explain all three existing neutrino anomalies without enlarging the neutrino sector. CPT violation in the Dirac mass terms of the three neutrino flavors preserves Lorentz invariance, but generates independent masses for neutrinos and antineutrinos. This specific signature is strongly motivated by braneworld scenarios with extra dimensions, where neutrinos are the natural messengers for Standard Model physics of CPT violation in the bulk. A simple model of maximal CPT violation is sufficient to explain the exisiting neutrino data quite neatly, while making dramatic predictions for the upcoming KamLAND and MiniBooNE experiments. Furthermore we obtain a promi…

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsDirac (video compression format)High Energy Physics::PhenomenologyFísicaFOS: Physical sciencesLorentz covarianceStandard ModelMiniBooNEBaryogenesisHigh Energy Physics - PhenomenologyExtra dimensionsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNeutrino
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Flavour-symmetric type-II Dirac neutrino seesaw mechanism

2018

We propose a Standard Model extension with underlying A4 flavour symmetry where small Dirac neutrino masses arise from a Type-II seesaw mechanism. The model predicts the "golden" flavour-dependent bottom-tau mass relation, requires an inverted neutrino mass ordering and non-maximal atmospheric mixing angle. Using the latest neutrino oscillation global fit we derive restrictions on the oscillation parameters, such as a correlation between Dirac CP phase and the lightest neutrino mass.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsOscillationDirac (video compression format)High Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesSymmetry (physics)lcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Standard-Model Extension0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationlcsh:PhysicsPhysics Letters B
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Model-independent fit to Planck and BICEP2 data

2014

Inflation is the leading theory to describe elegantly the initial conditions that led to structure formation in our universe. In this paper, we present a novel phenomenological fit to the Planck, WMAP polarisation (WP) and the BICEP2 datasets using an alternative parameterisation. Instead of starting from inflationary potentials and computing the inflationary observables, we use a phenomenological parameterisation due to Mukhanov, describing inflation by an effective equation-of-state, in terms of the number of e-folds and two phenomenological parameters $\alpha$ and $\beta$. Within such a parametrisation, which captures the different inflationary models in a model-independent way, the valu…

PhysicsNuclear and High Energy PhysicsSpectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)Structure formationFOS: Physical sciencesSigmaFísicaObservableAstrophysics::Cosmology and Extragalactic AstrophysicsParameter spaceCMB cold spotsymbols.namesakeTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonsymbolsAstronomiaPlanckAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmic Microwave Background anisotropies from second order gravitational perturbations

1997

This paper presents a complete analysis of the effects of second order gravitational perturbations on Cosmic Microwave Background anisotropies, taking explicitly into account scalar, vector and tensor modes. We also consider the second order perturbations of the metric itself obtaining them, for a universe dominated by a collision-less fluid, in the Poisson gauge, by transforming the known results in the synchronous gauge. We discuss the resulting second order anisotropies in the Poisson gauge, and analyse the possible relevance of the different terms. We expect that, in the simplest scenarios for structure formation, the main effect comes from the gravitational lensing by scalar perturbati…

PhysicsNuclear and High Energy PhysicsStructure formationGeneral relativitymedia_common.quotation_subjectCosmic microwave backgroundScalar (mathematics)Astrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsUniverseTheoretical physicsGravitational lensClassical mechanicsTensormedia_common
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Zeptosecond contact times for element Z=120 synthesis

2020

The synthesis of new superheavy elements beyond oganesson (Z=118) requires fusion reactions with projectile nuclei with proton numbers larger than that of $^{48}$Ca (Z=20), which has been successfully employed for the synthesis of elements with Z=112-118. In such reactions, fusion is drastically hindered by fast non-equilibrated dynamical processes. Attempts to produce nuclei with Z=120 using the $^{64}$Ni+$^{238}$U, $^{58}$Fe+$^{244}$Pu, $^{54}$Cr+$^{248}$Cm, and $^{50}$Ti+$^{249}$Cf reactions have been made, which all result in larger Coulomb forces than for $^{48}$Ca-induced reactions, but no discovery has been confirmed to date. In this work, mass and angle distributions of fission frag…

PhysicsNuclear and High Energy PhysicsWork (thermodynamics)FusionSuperheavy-element formationProton010308 nuclear & particles physicsFissionProjectile01 natural scienceslcsh:QC1-9993. Good healthYield (chemistry)Quasifission0103 physical sciencesCoulombNuclear fusionddc:530Atomic physics010306 general physicsZ=120lcsh:PhysicsPhysics Letters
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Majorons: a simultaneous solution to the large and small scale dark matter problems

1984

Abstract It is shown that the existence of majorons, which enable a heavy neutrino, 500 eV ≲ mνH ≲ 25 keV to decay into a light neutrino mνL ≲ 8 eV and a majoron, with lifetime 104 yr ≲ τνH ≲ 108 yr can solve both the large and small scale dark matter problems. For a primordial “Zeldovich” spectrum of fluctuations the limits are m v H ≲ 550 eV and τ v H > 107 to 108 yr (the ranges mνH ≲ eV and τνH ≳ 108 yr are allowed by the model but galaxy formation becomes problematic). The large scale dark matter problem is how to achieve the critical density as implied by inflation, the small scale problems deal with the halos of galaxies and galaxy formation and perturbation growth. The heavy neutrino…

PhysicsNuclear and High Energy Physicsmedia_common.quotation_subjectDark matterFísicaDecoupling (cosmology)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologyGalaxyUniverseGalaxy formation and evolutionNeutrinoParticle Physics - Phenomenologymedia_commonMajoron
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On the correlation between phase-locking modes and Vibrational Resonance in a neuronal model

2018

International audience; We numerically and experimentally investigate the underlying mechanism leading to multiple resonances in the FitzHugh-Nagumo model driven by a bichromatic excitation. Using a FitzHugh-Nagumo circuit, we first analyze the number of spikes triggered by the system in response to a single sinusoidal wave forcing. We build an encoding diagram where different phase-locking modes are identified according to the amplitude and frequency of the sinusoidal excitation. Next, we consider the bichromatic driving which consists in a low frequency sinusoidal wave perturbed by an additive high frequency signal. Beside the classical Vibrational Resonance phenomenon, we show in real ex…

PhysicsNumerical AnalysisQuantitative Biology::Neurons and CognitionApplied MathematicsPerturbation (astronomy)phase locking modesLow frequencyneural networks01 natural sciences010305 fluids & plasmasComputational physicsCorrelationNonlinear systemnonlinear dynamicsSine waveAmplitude[NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]Control theoryModeling and Simulation0103 physical sciencesVibrational resonance[ NLIN.NLIN-PS ] Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]010306 general physicsvibrational resonanceExcitation
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Quantum Solitons on Quantum Chaos: Coherent Structures, Anyons, and Statistical Mechanics

1991

This paper is concerned with the exact evaluation of functional integrals for the partition function Z (free energy F = -β -1 ln Z, β -1 = temperature) for integrable models like the quantum and classical sine-Gordon (s-G) models in 1+1 dimensions.1–12 These models have wide applications in physics and are generic (and important) in that sense. The classical s-G model in 1+1 dimensions $${\phi _{xx}} - {\phi _{tt}} = {m^2}\sin \phi$$ (1) (m > 0 is a “mass”) has soliton (kink, anti-kink and breather) solutions. In Refs 1–12 we have reported a general theory of ‘soliton statistical mechanics’ (soliton SM) in which the particle description can be seen in terms of ‘solitons’ and ‘phonons’. The …

PhysicsOpen quantum systemQuantization (physics)Quantum mechanicsQuantum dynamicsQuantum simulatorSupersymmetric quantum mechanicsQuantum statistical mechanicsQuantum dissipationNonlinear Sciences::Pattern Formation and SolitonsQuantum chaos
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