Search results for "SPECTRA"

showing 10 items of 3542 documents

Long lifetime of the E1u in-plane infrared-active modes of h -BN

2020

We present an infrared reflectivity study of the ${E}_{1u}$ in-plane phonons of hexagonal BN as a function of temperature in the 40--680 K range. The infrared reflectance spectra of high-quality lamellar single crystals are accurately fitted using Lowndes' factorized form of the dielectric response, where the longitudinal-optic (LO) frequency is an independent adjustable parameter. From this analysis we obtain reliable values for the phonon damping of the IR-active ${E}_{1u}$ phonons which couple to light and give rise to the phonon-polariton excitations in this hyperbolic material. Anharmonic coupling potentials are estimated from the temperature dependence of the damping parameters. The $…

PhysicsCondensed matter physicsScatteringPhononInfraredAnharmonicityInfrared spectroscopy02 engineering and technology021001 nanoscience & nanotechnologyCoupling (probability)01 natural sciencesSpectral line0103 physical sciencesLamellar structure010306 general physics0210 nano-technologyPhysical Review B
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Strong reduction of the Korringa relaxation in the spin-density wave regime ofEuFe2As2observed by electron spin resonance

2010

Electron spin resonance measurements in ${\text{EuFe}}_{2}{\text{As}}_{2}$ single crystals revealed an absorption spectrum of a single resonance with Dysonian line shape. Above the spin-density wave (SDW) transition at ${T}_{\text{SDW}}=190\text{ }\text{K}$ the spectra are isotropic and the Eu spins relax via the conduction electrons resulting in a Korringa-type increase in the linewidth. Below ${T}_{\text{SDW}}$, a distinct anisotropy develops and the relaxation behavior of the Eu spins changes drastically into one with characteristic properties of a magnetic insulating system, where dipolar and crystal-field interactions dominate. This indicates a spatial confinement of the conduction ele…

PhysicsCondensed matter physicsSpinsRelaxation (NMR)ResonanceElectronCondensed Matter PhysicsSpectral lineElectronic Optical and Magnetic Materialslaw.inventionDipolelawCondensed Matter::SuperconductivitySpin density waveCondensed Matter::Strongly Correlated ElectronsElectron paramagnetic resonancePhysical Review B
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The influence of disorder on the exciton spectra in two-dimensional structures

2019

We study the role of disorder in the exciton spectra in two-dimensional (2D) semiconductors. These can be heterostructures, thin films and multilayers (so-called van der Waals structures) of organometallic perovskites, transition metal dichalcogenides and other semiconductors for optoelectronic applications. We model the disorder by introduction of a fractional Laplacian (with Le´vy index m, defining the degree of disorder) to the Scro¨dinger equation with 2D Coulomb potential. Combining analytical and numerical methods, we observe that the exciton exists only for m 4 1, while the point m = 1 (strongest disorder) corresponds to the exciton collapse. We show also that in the fractional (diso…

PhysicsCondensed matter physicsSpintronicsbusiness.industryExcitonGeneral Physics and AstronomyHeterojunction02 engineering and technologyCondensed Matter::Mesoscopic Systems and Quantum Hall Effect010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesSpectral line0104 chemical sciencesCondensed Matter::Materials Sciencesymbols.namesakeSemiconductorPrincipal quantum numbersymbolsElectric potentialPhysical and Theoretical Chemistryvan der Waals force0210 nano-technologybusinessPhysical Chemistry Chemical Physics
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External Noise Effects in Doped Semiconductors Operating Under sub-THz Signals

2012

We study the noise-induced effects on the electron transport dynamics in low-doped n-type GaAs samples by using a Monte Carlo approach. The system is driven by an external periodic electric field in the presence of a random telegraph noise source. The modifications caused by the addition of external fluctuations are investigated by studying the spectral density of the electron velocity fluctuations for different values of the noise parameters. The findings indicate that the diffusion noise in low-doped semiconductors can be reduced by the addition of a fluctuating component to the driving electric field, but the effect critically depends on the features of the external noise source.

PhysicsCondensed matter physicsbusiness.industryMonte Carlo methodQuantum noiseShot noiseSpectral densityStatistical and Nonlinear PhysicsNoise (electronics)Semiconductortransport propertiesElectric fieldfluctuations and noise processeDiffusion (business)businessMonte Carlo simulationMathematical PhysicsReports on Mathematical Physics
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The atmospheric structure and fundamental parameters of Red Supergiants

2013

We present studies of the atmospheric structure and fundamental properties of the red supergiants (RSGs) VY CMa, AH Sco, UY Sct, and KW Sgr based on near-infrared K -band interferometry obtained with the VLTI/AMBER instrument with a spectral resolution of 1500. In our visibility data, we observe the presence of molecular layers of water and CO in extended atmospheres. For a uniform disk modeling, we observe size increases in the water band centered at 1.9 μ m and in the CO band at 2.3–2.5 μ m, with respect to the near-continuum bandpass (2.20–2.25 μ m). With our spectral resolution, we obtain diameters in the near-continuum, that are free from contamination by molecular layers. Using PHOENI…

PhysicsConvectionHertzsprung–Russell diagramGeneral EngineeringAstronomy and AstrophysicsAstrophysicsSpectral lineAtmosphereInterferometryStarssymbols.namesakeSpace and Planetary SciencesymbolsRed supergiantSpectral resolutionEAS Publications Series
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The X-ray Integral Field Unit (X-IFU) for Athena

2014

Athena is designed to implement the Hot and Energetic Universe science theme selected by the European Space Agency for the second large mission of its Cosmic Vision program. The Athena science payload consists of a large aperture high angular resolution X-ray optics (2 m2 at 1 keV) and twelve meters away, two interchangeable focal plane instruments: the X-ray Integral Field Unit (X-IFU) and the Wide Field Imager. The X-IFU is a cryogenic X-ray spectrometer, based on a large array of Transition Edge Sensors (TES), oering 2.5 eV spectral resolution, with approximately 5" pixels, over a field of view of 5' in diameter. In this paper, we present the X-IFU detector and readout electronics princi…

PhysicsCosmic VisionEquipment and servicesSpectrometerSpectral resolutionSpectrometersX-ray opticsbusiness.industrySensorsVisionDetectorAstrophysics::Instrumentation and Methods for AstrophysicsField of viewOpticsCardinal pointParticlesSettore FIS/05 - Astronomia E AstrofisicaX-raysImaging systemsAngular resolutionSpectral resolutionElectronicsbusinessImage resolution
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Running of featureful primordial power spectra

2017

Current measurements of the temperature and polarization anisotropy power spectra of the Cosmic Microwave Background (CMB) seem to indicate that the naive expectation for the slow-roll hierarchy within the most simple inflationary paradigm may not be respected in nature. We show that a primordial power spectra with localized features could in principle give rise to the observed slow-roll anarchy when fitted to a featureless power spectrum. Future CMB missions have the key to disentangle among the two possible paradigms and firmly establish the slow-roll mechanism as the responsible one for the inflationary period in the early universe. From a model comparison perspective, and assuming that …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundSpectral densityFOS: Physical sciencesCosmological modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPolarization (waves)01 natural sciencesSpectral linesymbols.namesake0103 physical sciencessymbolsStatistical analysisPlanck010306 general physicsAnisotropyAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Whispers from the dark side: Confronting light new physics with NANOGrav data

2021

The NANOGrav collaboration has recently observed first evidence of a gravitational wave background (GWB) in pulsar timing data. Here we explore the possibility that this GWB is due to new physics, and show that the signal can be well fit also with peaked spectra like the ones expected from phase transitions (PTs) or from the dynamics of axion like particles (ALPs) in the early universe. We find that a good fit to the data is obtained for a very strong PT at temperatures around 1 MeV to 10 MeV. For the ALP explanation the best fit is obtained for a decay constant of $F \approx 5\times 10^{17}$ GeV and an axion mass of $2\times 10^{-13}$ eV. We also illustrate the ability of PTAs to constrain…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysicsQC1-999Physics beyond the Standard Modelmedia_common.quotation_subjectGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsParameter space01 natural sciencesSpectral lineUniverseGravitational wave backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Pulsar0103 physical sciencesExponential decay010306 general physicsAxionAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_common
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Exponents of non-linear clustering in scale-free one-dimensional cosmological simulations

2012

One dimensional versions of cosmological N-body simulations have been shown to share many qualitative behaviours of the three dimensional problem. They can resolve a large range of time and length scales, and admit exact numerical integration. We use such models to study how non-linear clustering depends on initial conditions and cosmology. More specifically, we consider a family of models which, like the 3D EdS model, lead for power-law initial conditions to self-similar clustering characterized in the strongly non-linear regime by power-law behaviour of the two point correlation function. We study how the corresponding exponent \gamma depends on the initial conditions, characterized by th…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSpectral densityAstronomy and AstrophysicsCosmologyNumerical integrationMetric expansion of spaceUniversality (dynamical systems)Nonlinear systemTheoretical physicsSpace and Planetary ScienceExponentStatistical physicsCluster analysisAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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On the viability of a certain vector-tensor theory of gravitation

2010

A certain vector-tensor theory is revisited. Our attention is focused on cosmology. Against previous suggestions based on preliminary studies, it is shown that, if the energy density of the vector field is large enough to play the role of the dark energy and its fluctuations are negligible, the theory is not simultaneously compatible with current observations on: supernovae, the cosmic microwave background (CMB) anisotropy, and the power spectrum of the energy density fluctuations. However, for small enough energy densities of the vector field, the theory becomes compatible with all the above observations and, moreover, it leads to an interesting evolution of the so-called vector cosmologic…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityCosmic microwave backgroundFOS: Physical sciencesSpectral densityAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyGravitationTheoretical physicsSpace and Planetary ScienceDark energyVector fieldAnisotropyAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics and Space Science
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