Search results for "ground"

showing 10 items of 2432 documents

Dark Radiation and Inflationary Freedom after Planck 2015

2016

The simplest inflationary models predict a primordial power spectrum (PPS) of the curvature fluctuations that can be described by a power-law function that is nearly scale-invariant. It has been shown, however, that the low-multipole spectrum of the CMB anisotropies may hint the presence of some features in the shape of the scalar PPS, which could deviate from its canonical power-law form. We study the possible degeneracies of this non-standard PPS with the neutrino anisotropies, the neutrino masses, the effective number of relativistic species and a sterile neutrino or a thermal axion mass. The limits on these additional parameters are less constraining in a model with a non-standard PPS w…

PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsScalar (mathematics)Cosmic microwave backgroundSpectral densityFOS: Physical sciences01 natural sciencessymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark radiation0103 physical sciencessymbolsPlanckNeutrino010306 general physicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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New opportunities at the next-generation neutrino experiments I: BSM neutrino physics and dark matter

2020

Abstract The combination of the high intensity proton beam facilities and massive detectors for precision measurements of neutrino oscillation parameters including the charge-parity violating (CPV) phase will open the door to help make beyond the standard model (BSM) physics reachable even in low energy regimes in the accelerator-based experiments. Large-mass detectors with highly precise tracking and energy measurements, excellent timing resolution, and low energy thresholds will enable the searches for BSM phenomena from cosmogenic origin, as well. Therefore, it is also conceivable that BSM topics in the next-generation neutrino experiments could be the dominant physics topics in the fore…

PhysicsParticle physicsSterile neutrinoPhysics beyond the Standard ModelDark matterGeneral Physics and AstronomyScale (descriptive set theory)Tracking (particle physics)01 natural sciences0103 physical sciencesDeep Underground Neutrino ExperimentHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationReports on Progress in Physics
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Partition function based analysis of cosmic microwave background maps

1999

We present an alternative method to analyse cosmic microwave background (CMB) maps. We base our analysis on the study of the partition function. This function is used to examine the CMB maps, making use of the different information embedded at different scales and moments. Using the partition function in a likelihood analysis in two dimensions (Qrms-PS, n), we find the best-fitting model to the best data available at present (the COBE–DMR 4 years data set). By means of this analysis we find a maximum in the likelihood function for n=1.8-0.65+0.35 and Qrms-PS = 10-2.5+3μ K (95 per cent confidence level) in agreement with the results of other similar analyses [Smoot et al. (1 yr), Bennet et a…

PhysicsPartition function (quantum field theory)Cosmic microwave backgroundFísicaAstronomy and AstrophysicsMultifractal systemFunction (mathematics)Measure (mathematics)Cosmic microwave backgroundData setTheoretical physicsDistribution (mathematics)Methods: data analysisSpace and Planetary ScienceStatistical physicsdata analysis [Methods]Likelihood functionMonthly Notices of the Royal Astronomical Society
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Fractional Tajimi–Kanai model for simulating earthquake ground motion

2014

The ground acceleration is usually modeled as a filtered Gaussian process. The most common model is a Tajimi–Kanai (TK) filter that is a viscoelastic Kelvin–Voigt unit (a spring in parallel with a dashpot) carrying a mass excited by a white noise (acceleration at the bedrock). Based upon the observation that every real material exhibits a power law trend in the creep test, in this paper it is proposed the substitution of the purely viscous element in the Kelvin Voigt element with the so called springpot that is an element having an intermediate behavior between purely elastic (spring) and purely viscous (dashpot) behavior ruled by fractional operator. With this choice two main goals are rea…

PhysicsPeak ground accelerationGround motionBuilding and ConstructionWhite noiseMechanicsGeotechnical Engineering and Engineering GeologyFree fieldViscoelasticityDashpotsymbols.namesakeAccelerationGeophysicsSpring (device)Fractional viscoelasticitysymbolsTajimi–Kanai filterGaussian processCivil and Structural Engineering
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Photonic Nambu-Goldstone bosons

2017

We study numerically the spatial dynamics of light in periodic square lattices in the presence of a Kerr term, emphasizing the peculiarities stemming from the nonlinearity. We find that, under rather general circumstances, the phase pattern of the stable ground state depends on the character of the nonlinearity: the phase is spatially uniform if it is defocusing whereas in the focusing case, it presents a chess board pattern, with a difference of $\pi$ between neighboring sites. We show that the lowest lying perturbative excitations can be described as perturbations of the phase and that finite-sized structures can act as tunable metawaveguides for them. The tuning is made by varying the in…

PhysicsPhase (waves)FOS: Physical sciencesContext (language use)Pattern Formation and Solitons (nlin.PS)Òptica01 natural sciencesNonlinear Sciences - Pattern Formation and SolitonsSymmetry (physics)Square (algebra)Partícules (Física nuclear)010309 opticsNonlinear systemQuantum Gases (cond-mat.quant-gas)Quantum mechanics0103 physical sciencesGoldstone boson010306 general physicsGround stateCondensed Matter - Quantum GasesBosonPhysics - OpticsOptics (physics.optics)
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Positron Production In Heavy-Ion Collisions

1985

Atomic systems with a nuclear charge Z much greater than 100 exhibit a number of unique features not otherwise found in nature. Two characteristic properties are illustrated in Figs. 1 and 2. In Fig. 1 we have plotted the binding energy of a K-shell electron around hypothetical nuclei up to Z ≈ 200. For Z > 150 the binding energy exceeds the rest energy m e c 2 of the electron; i.e., adding the electron to the nucleus actually diminishes the total mass of the system. At the critical charge Z c ≈ 170–175 the binding energy reaches twice the electron rest mass, the threshold for spontaneous creation of an electron-positron pair. As has been discussed extensively in the literature (Pieper and …

PhysicsPhase transitionBinding energyElectron rest massElectron shellCharge (physics)ElectronAtomic physicsGround stateEffective nuclear charge
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The Topological Phase Transitions Related to Fermion Condensate

2014

In this chapter, we consider so-called topological phase transitions, taking place in normal Fermi liquid. In other words, here we are dealing with different instabilities of normal Fermi liquids relative to several kinds of perturbations of initial quasiparticle spectrum \(\varepsilon (p)\) and occupation numbers \(n(p)\) associated with the emergence of a multi-connected Fermi surface. Depending on the parameters and analytical properties of the Landau interaction, such instabilities lead to several possible types of restructuring of initial Landau Fermi liquid ground state. This restructuring generates topologically distinct phases. One of them is the FC discussed above, another one belo…

PhysicsPhase transitionPhase (matter)QuasiparticleFermi surfaceFermionFermi liquid theoryGround stateTopologyFermi Gamma-ray Space Telescope
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Magnetic field and temperature dependent correlations in the singlet ground state system CsFeBr3

1992

Abstract In the singlet ground state system CsFeBr 3 the temperature and magnetic field dependence of the magnetic dispersion curves have been measured by inelastic neutron scattering. At a field of 4.1 T magnetic Bragg peaks appear at (⅓ ⅓ 1) and (⅔ ⅔ 1). The correlation lengths were derived from the experimental data by integrating the constant Q -scans over the energy transfer. The Q -dependence was fitted to Lorentzians and correlations lengths were extracted for different directions in the lattice. These correlation lengths decrease with increasing temperature and increase with increasing field. Above the phase transition the correlation lengths decrease again.

PhysicsPhase transitionSinglet ground stateCondensed matter physicsLattice (order)Energy transferCondensed Matter PhysicsInelastic neutron scatteringElectronic Optical and Magnetic MaterialsMagnetic fieldJournal of Magnetism and Magnetic Materials
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Photoluminescence at the ground-state level anticrossing of the nitrogen-vacancy center in diamond: A comprehensive study

2021

Physical review / B 103(3), 035307 (2021). doi:10.1103/PhysRevB.103.035307

PhysicsPhotoluminescenceSpinsBand gapCenter (category theory)Diamond02 engineering and technologyengineering.material021001 nanoscience & nanotechnologyCondensed Matter Physics53001 natural sciences3. Good health0103 physical sciencesengineeringddc:530Atomic physics010306 general physics0210 nano-technologyNitrogen-vacancy centerGround stateSpin (physics)Den kondenserade materiens fysik
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The evolution of the large-scale emission in Fanaroff-Riley type I jets

2011

Recent observations in X-rays and gamma-rays of nearby Fanaroff-Riley type I (FR I) radio galaxies have raised the question of the origin of the emission detected in the termination structures of their jets. The study of these structures can give information on the conditions for particle acceleration and radiation at the front shocks. In addition, an evolutionary scenario can help to disentangle the origin of the detected X-ray emission in young FR I sources, like some gigahertz peaked spectrum active galactic nuclei. This work focuses on the nature and detectability of the radiation seen from the termination regions of evolving FR I jets. We use the results of a relativistic, two-dimensio…

PhysicsPhotonActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundCosmic background radiationSynchrotron radiationAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveParticle accelerationSpace and Planetary ScienceMonthly Notices of the Royal Astronomical Society
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