Search results for "SPECTRA"

showing 10 items of 3542 documents

Hyperfine structure in the rotational spectra of trans-formic acid: Lamb-dip measurements and quantum-chemical calculations

2010

Context. Formic acid, HCOOH, is the simplest organic acid and the first that has been identified in the interstellar medium. Its astrophysical relevance has motivated this spectroscopic study. Aims. The aim of this investigation is to provide very accurate rest frequencies for the trans isomer of HCOOH as well as to improve the spectroscopic and hyperfine parameters available in the literature for this molecule. Methods. The Lamb-dip technique has been exploited in order to record the rotational spectrum of trans-HCOOH at sub-Doppler resolution in the millimeter- and submillimeter-wave frequency ranges and, when possible, to resolve the hyperfine structure due to the hydrogen nuclei. THz me…

PhysicsFormic acidTerahertz radiationRotational transitionAstronomy and AstrophysicsContext (language use)Spectral lineInterstellar mediumchemistry.chemical_compoundchemistrySpace and Planetary ScienceMoleculePhysics::Atomic PhysicsAtomic physicsHyperfine structureAstronomy and Astrophysics
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AC-Stark shift and photoionization of Rydberg atoms in an optical dipole trap

2010

We have measured the AC-Stark shift of the $14D_{5/2}$ Rydberg state of rubidium 87 in an optical dipole trap formed by a focussed CO$_2$-laser. We find good quantitative agreement with the model of a free electron experiencing a ponderomotive potential in the light field. In order to reproduce the observed spectra we take into account the broadening of the Rydberg state due to photoionization. The extracted cross-section is compatible with previous measurements on neighboring Rydberg states.

PhysicsFree electron modelAtomic Physics (physics.atom-ph)General Physics and AstronomyFOS: Physical sciencesPhotoionizationSpectral linePhysics - Atomic Physicssymbols.namesakeDipoleStark effectRydberg atomsymbolsRydberg formulaPhysics::Atomic PhysicsRydberg stateAtomic physics
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Monte Carlo analysis of electronic noise in semiconductors under sub‐terahertz cyclostationary mixed fields

2006

This paper reports the results of Monte Carlo simulations of electronic noise in a GaAs bulk driven by two mixed high-frequency large-amplitude periodic electric fields. Under these conditions, the system response shows some peculiarities in the noise performance, such as a resonant-like enhancement of the spectra near the two frequencies of the applied fields. The relations among the frequency response and the velocity fluctuations as a function of intensities and frequencies of the sub-terahertz mixed excitation fields have been investigated. (© 2006 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

PhysicsFrequency responseCondensed matter physicsTerahertz radiationCyclostationary processElectric fieldMonte Carlo methodCondensed Matter PhysicsNoise (electronics)ExcitationSpectral linephysica status solidi c
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Wave-mixing effects on electronic noise in semiconductors

2006

The results of a Monte Carlo analysis of hot-electron intrinsic noise in a n-type GaAs bulk driven by two mixed large-amplitude alternating electric fields having frequency in the subterahertz range are presented. The noise properties are investigated by studying the velocity autocorrelation function and the noise spectrum. We explored the relations among the frequency response and the velocity fluctuations as a function of the frequencies and intensities of the mixed fields. When the semiconductor is driven by two mixed ciclostationary electric fields, a resonant-like enhancement of the spectra near the two frequencies of the applied fields is found.

PhysicsFrequency responseCondensed matter physicsbusiness.industryMonte Carlo methodAutocorrelationNoise (electronics)Atomic and Molecular Physics and OpticsSpectral lineElectronic Optical and Magnetic MaterialsSemiconductorModeling and SimulationElectric fieldRange (statistics)Electrical and Electronic Engineeringbusiness
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The Fučík spectrum for nonlocal BVP with Sturm–Liouville boundary condition

2014

Boundary value problem of the form x''=-μx++λx-, αx(0)+(1-α)x'(0)=0, ∫01 x(s)ds=0 is considered, where μ,λ∈ R and α∈ [0,1]. The explicit formulas for the spectrum of this problem are given and the spectra for some α values are constructed. Special attention is paid to the spectrum behavior at the points close to the coordinate origin.

PhysicsFucík spectrumApplied MathematicsSturm–Liouville boundary conditionMathematical analysisSpectrum (functional analysis)lcsh:QA299.6-433Sturm–Liouville theorylcsh:AnalysisSpectral lineboundary value problemBoundary value problemAnalysisintegral conditionNonlinear Analysis: Modelling and Control
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Tilted precession bands in Nd135

2021

Two new excited bands built on the πh11/2 configuration have been identified in Nd135 in addition to the known πh11/2 band. The energy spectra of the excited bands and the available electromagnetic transition probabilities are in good agreement with theoretical results obtained using quasiparticle-plus-triaxial-rotor model calculations. The properties of the bands identify them as tilted precession bands instead of wobbling bands. Our results give a new insight into the interpretation of the low-lying bands in odd-A mass nuclei, and can stimulate future studies to address the nuclear triaxiality.

PhysicsFuture studies010308 nuclear & particles physicsExcited state0103 physical sciencesNuclear structurePrecessionAtomic physics010306 general physics01 natural sciencesSpectral linePhysical Review C
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Line Identification of Atomic and Ionic Spectra of Holmium in the Near-UV. Part I. Spectrum of Ho i

2017

The Fourier Transform spectra of a Holmium hollow cathode discharge lamp have been investigated in the UV spectral range from 25,000 up to 31,530 cm−1 (317 to 400 nm). Two Ho spectra have been measured with neon and argon as buffer gases. Based on the intensity ratios from these two spectra, a distinction was made between atomic and ionic lines (ionic lines are discussed in an accompanying paper). Using the known Ho i energy levels, 71 lines could be classified as transitions of atomic Ho, 34 of which have not been published previously. Another 32 lines, which could not be classified, are listed in the literature and assigned as atomic Ho. An additional 370 spectral lines have been assigned…

PhysicsGas-discharge lampArgon010504 meteorology & atmospheric scienceschemistry.chemical_elementIonic bondingAstronomy and Astrophysics01 natural sciencesCathodeSpectral linelaw.invention010309 opticsNeonchemistrySpace and Planetary Sciencelaw0103 physical sciencesAtomic physicsHolmium0105 earth and related environmental sciencesLine (formation)The Astrophysical Journal Supplement Series
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Delayed-Neutron Spectra Following Decay ofAs85andSb135

1974

PhysicsGeneral Physics and AstronomyAtomic physicsDelayed neutronSpectral linePhysical Review Letters
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The T[sub z] = −1→ T[sub z] =0 beta decays and comparison with Charge Exchange reactions

2011

Gamow‐Teller (GT) transitions can be studied in both β decay and charge exchange (CE) reactions. If isospin is a good quantum number, then the Tz = −1→0 and Tz = +1→0 GT mirror transitions, are identical. Therefore, a comparison of the results from studies of β decay and CE should shed light on this assumption. Accordingly we have studied the β decay of the Tz = −1 fp‐shell nuclei, 54Ni, 50Fe, 46Cr, and 42Ti, produced in fragmentation and we have compared our results with the spectra from (3He, t) measurements on the mirror Tz = +1 target nuclei studied in high resolution at RCNP, Osaka. The β decay experiments were performed as part of the STOPPED beam RISING campaign at GSI.

PhysicsGood quantum numberNuclear physicsDecay schemeFragmentation (mass spectrometry)Helium-3IsospinAtomic physicsBeta decaySpectral lineParticle detectorAIP Conference Proceedings
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OCTOCAM: A fast multichannel imager and spectrograph for the 10.4m GTC

2010

OCTOCAM is a multi-channel imager and spectrograph that has been proposed for the 10.4m GTC telescope. It will use dichroics to split the incoming light to produce simultaneous observations in 8 different bands, ranging from the ultraviolet to the near-infrared. The imaging mode will have a field of view of 2' x 2' in u, g, r, i, z, J, H and Ks bands, whereas the long-slit spectroscopic mode will cover the complete range from 4,000 to 23,000 {\AA} with a resolution of 700 - 1,700 (depending on the arm and slit width). An additional mode, using an image slicer, will deliver a spectral resolution of over 3,000. As a further feature, it will use state of the art detectors to reach high readout…

PhysicsGran Telescopio Canariasbusiness.industryResolution (electron density)Near-infrared spectroscopyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesField of viewlaw.inventionTelescopeOpticslawObservatorySpectral resolutionbusinessAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Spectrograph
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