Search results for "Absorption"

showing 10 items of 2701 documents

A Novel Method Of Measuring Light Absorption On A Self-Assembled Single Quantum Dot

2005

Abstract. We present a novel method by wich excitonic interband optical transitions within single InAs self-assembled quantum dots can be directly observed in a transmission experiment. Due to the extremely high resolution of the tecnique, individual peaks associated to single exciton absorption resonances in single quantum dots can be spectrally resolved. Using this technique we investigate the oscillator strength, homogeneous linewidth and fine structure splitting in a collection of such individual resonances.

Physicsbusiness.industryOscillator strengthExcitonCondensed Matter::Mesoscopic Systems and Quantum Hall EffectMolecular physicsSelf assembledLaser linewidthHomogeneousQuantum dotOptoelectronicsFine structureAbsorption (electromagnetic radiation)business
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The role of nonlinear optical absorption in narrowband difference-frequency terahertz-wave generation

2010

We present a general analysis of the influence of nonlinear optical absorption on terahertz generation via optical difference frequency generation, when reaching for the quantum conversion efficiency limit. By casting the equations governing the process in a suitably normalized form, including either two-photon- or three-photon-absorption terms, we have been able to plot universal charts for phase matched optical-to-terahertz conversion for different values of the nonlinear absorption coefficients. We apply our analysis to some experiments reported to date, in order to understand to what extent multiphoton absorption could have played a role and also to predict the maximum achievable conver…

Physicsbusiness.industryTerahertz radiationEnergy conversion efficiencyFOS: Physical sciencesPhysics::OpticsNonlinear opticsStatistical and Nonlinear PhysicsTwo-photon absorptionAtomic and Molecular Physics and OpticsPhoton countingOptical rectificationOpticsNarrowbandOptical frequency conversion Optical materials Optical parametric amplifiers Optical phase matching Optical propagation in nonlinear media Optical pulse generation Optical waveguides Frequency conversion Semiconductor materials Semiconductor waveguidesbusinessAbsorption (electromagnetic radiation)Optics (physics.optics)Physics - OpticsJournal of the Optical Society of America B
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Unusual optical properties of the dense nonequilibrium plasmas

2005

A concise overview of new optical properties of dense nonequilibrium plasma formed on the solid state target boundary is given. In this chapter, we describe phenomena such as the third harmonic generation in the skin layer, collisionless electron heating in the high frequency skin-effect regime, absorption, and reflection and transmission of radiation by a plasma with anisotropic electron distribution.

Physicsbusiness.industryWaves in plasmasPlasmaElectronSlot-waveguideOpticsPhysics::Plasma PhysicsPhysics::Space PhysicsReflection (physics)High harmonic generationAtomic physicsAbsorption (electromagnetic radiation)businessAnisotropyInternational Quantum Electronics Conference, 2005.
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The role of synchrotron self-absorption in the late radio emission of SN1993J

2001

The standard model for radio supernovae considers that the observed synchrotron radio emission arises from the high-energy shell that results from the strong interaction between the expanding supernova ejecta and the circumstellar medium. This emission is considered to be only partially absorbed by ionized thermal electrons in the circumstellar wind of the progenitor star. Based on a study of the radio light curves of the type II supernova SN1993J, we present evidence of synchrotron self-absorption. Our modeling of the radio light curves requires a large initial magnetic field, of about 30 Gauss, and the existence of an (initially) highly-relativistic population of electrons. We also show t…

Physicseducation.field_of_studyAstrophysics::High Energy Astrophysical PhenomenaPopulationAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsElectronAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsType II supernovaLight curveAstrophysicsSynchrotronlaw.inventionSupernovaSpace and Planetary SciencelawIonizationAstrophysics::Solar and Stellar AstrophysicsAbsorption (electromagnetic radiation)educationAstrophysics::Galaxy Astrophysics
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Nonlinear effects in optical pumping of a cold and slow atomic beam

2015

By photoionizing hyperfine (HF) levels of the Cs state $6{\phantom{\rule{0.16em}{0ex}}}^{2}{P}_{3/2}$ in a slow and cold atom beam, we find how their population depends on the excitation laser power. The long time (around $180\phantom{\rule{4pt}{0ex}}\ensuremath{\mu}\mathrm{s})$ spent by the slow atoms inside the resonant laser beam is large enough to enable exploration of a unique atom-light interaction regime heavily affected by time-dependent optical pumping. We demonstrate that, under such conditions, the onset of nonlinear effects in the population dynamics and optical pumping occurs at excitation laser intensities much smaller than the conventional respective saturation values. The ev…

Physicseducation.field_of_studyPopulation02 engineering and technologysaturation spectroscopy; mutilevel atoms; cesium; laser; absorption: photoionization; intesity; systems; state; trap021001 nanoscience & nanotechnologyLaser01 natural sciencesAtomic and Molecular Physics and OpticsNumerical integrationlaw.inventionOptical pumpinglawUltracold atom0103 physical sciencesPhysics::Atomic PhysicsLaser power scalingAtomic physics010306 general physics0210 nano-technologyeducationHyperfine structureExcitationPhysical Review A
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Chandra Observation of the Persistent Emission from the Dipping Source XB 1916-053

2006

We present the results of a 50 ks long Chandra observation of the dipping source XB 1916-053. During the observation two X-ray bursts occurred and the dips were not present at each orbital period. From the zero-order image we estimate the precise X-ray coordinates of the source with a 90% uncertainty of 0.6''. In this work we focus on the spectral study of discrete absorption features, during the persistent emission, using the High Energy Transmission Grating Spectrometer on board the Chandra satellite. We detect, for the first time in the 1st-order spectra of XB 1916-053, absorption lines associated to Ne X, Mg XII, Si XIV, and S XVI, and confirm the presence of the Fe XXV and Fe XXVI abso…

Physicsline : formationAbsorption spectroscopySpectrometerAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsOrbital periodstars : neutronSpectral linestars : individual (XB 1916-053)Neutron starline : identificationSpace and Planetary Scienceformation; line : identification; stars : individual (XB 1916-053); stars : neutron; X-rays : binaries; X-rays : general [line]Absorption (electromagnetic radiation)X-rays : binarieDiffraction gratingLine (formation)X-rays : general
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A Complex Environment around Circinus X-1

2007

We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X-1 during the phase passage 0.223-0.261. We focus on the study of detected emission and absorption features using the HETGS. A comparative analysis of X-ray spectra, selected at different flux levels of the source, allows us to distinguish between a very hard state, at a low count rate, and a brighter, softer, highly absorbed spectrum during episodes of flaring activity. The spectrum of the hard state clearly shows emission lines of highly ionized elements, while, during the flaring state, the spectrum also shows strong resonant absorption lines. The most intense and interesting feature in this …

Physicsline : formationAccretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaX-ray binaryAstronomy and AstrophysicsAstrophysicsSpectral lineline : identificationAbsorption edgeSpace and Planetary ScienceIonizationCircinusEmission spectrumstars : individual (Circinus X-1)formation; line : identification; stars : individual (Circinus X-1); X-rays : binaries; X-rays : general [line]Atomic physicsAbsorption (electromagnetic radiation)X-rays : binarieX-rays : general
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Chandra observation of the Big Dipper X 1624–490

2006

We present the results of a 73 ks long Chandra observation of the dipping source X 1624-490. During the observation a complex dip lasting 4 hours is observed. We analyse the persistent emission detecting, for the first time in the 1st-order spectra of X 1624-490, an absorption line associated to \ion{Ca}{xx}. We confirm the presence of the \ion{Fe}{xxv} K$_\alpha$ and \ion{Fe}{xxvi} K$_\alpha$ absorption lines with a larger accuracy with respect to a previous XMM observation. Assuming that the line widths are due to a bulk motion or a turbulence associated to the coronal activity, we estimate that the lines have been produced in a photoionized absorber between the coronal radius and the out…

Physicsstars : individual : X 1624-490Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysicsaccretion accretion diskstars : neutronBulk motionSpectral lineIonAccretion discSpace and Planetary ScienceX-rays : starX-rays : binarieindividual : X 1624-490; stars : neutron; X-rays : stars; X-rays : binaries; X-rays : general [accretion accretion disks; stars]X-rays : generalLine (formation)Astronomy & Astrophysics
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Theoretical study of the discrete and continuum spectrum of BeH

2008

The transition intensities supplied in this Letter are directly connected with a description of the discrete and continuum spectrum of BeH. An attempt to meet our goal requires the calculation of the absorption oscillator strengths of several transitions to Rydberg states of BeH, together with differential oscillator strengths which give rise to different dipole-allowed photoionization channels from the molecular ground state. The calculations have been performed with the molecular-adapted quantum defect orbital (MQDO) approach. Predictions of new spectroscopic data on BeH at energies where high Rydberg transitions can take place, including the continuum region of the spectrum have been mad…

Physicssymbols.namesakeQuantum defectSpectrum (functional analysis)Continuum (design consultancy)Rydberg formulasymbolsGeneral Physics and AstronomyPhotoionizationPhysical and Theoretical ChemistryAtomic physicsGround stateAbsorption (electromagnetic radiation)Chemical Physics Letters
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Total absorption studies of high priority decays for reactor applications: 86Br and 91Rb

2017

Preliminary results from beta decay studies of nuclei that are important for reactor applications are presented. The beta decays have been studied using the total absorption technique (TAS) and the pure beams provided by the JYFLTRAP system at the IGISOL facility of the University of Jyväskylä. peerReviewed

Physicsta114010308 nuclear & particles physicsPhysicsQC1-99901 natural sciencesBeta decayNuclear physicsnuclear massesBeta (plasma physics)0103 physical sciencesstructuredecay data measurementsAtomic physics010306 general physicsAbsorption (electromagnetic radiation)Nuclear ExperimentEPJ Web of Conferences
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