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  • 1
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 78 (1995), S. 5109-5119 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Zinc selenide layers grown by molecular beam epitaxy (MBE) and doped with ZnO have been characterized using low temperature photoluminescence (PL) measurements as a function of excitation level, temperature, and laser energy (i.e., selectively excited donor-acceptor pair luminescence or SPL), as well as reflectance measurements. An O-related donor-to-acceptor (D0−A0) pair band is clearly observed in all of the ZnO-doped layers, whose position varies from 2.7196 to 2.7304 eV, depending on the excitation level. The same peak occurs in a number of undoped, As-doped, and Ga-doped MBE samples, showing that O can occur as a residual impurity. Temperature-dependent measurements reveal the existence of a corresponding conduction band-to-acceptor (e−A0) peak at 2.7372 eV (39.8 K), confirming the existence of the acceptor level. The binding energy of this acceptor is about 84±2 meV, which is 27 meV shallower than that of N. The SPL measurements reveal four excited states of the shallow acceptor level, separated from the 1s3/2 ground state by 48.2 (2p3/2), 57.1 (2s3/2), 64.3 (2p5/2:Γ7), and 67.7 meV (3p3/2:Γ8), respectively (all values ±1 meV). These energies fit well to conventional effective mass theory, which demonstrates that this O-related acceptor level is effective-mass-like. However, luminescence and secondary ion mass spectrometry show that the ZnO doping technique introduces shallow donor impurities into the material in addition to O acceptors, specifically high levels of chemical contaminants (mainly B and Ga) originating from the doping source. This effect may account for the lack of reproducibility in obtaining p-type conduction with ZnO doping, and suggests that more effective O incorporation methods should be devised. © 1995 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 59 (1986), S. 2833-2836 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Origin of a nonradiative center in AlGaAs grown by molecular-beam epitaxy was investigated by secondary ion mass spectroscopy and deep-level transient spectroscopy, from the change of photoluminescence intensity with anneal treatment, and from its comparison with GaAs. Aluminum-oxygen complex is a most probable defect which acts as a nonradiative center in AlGaAs, and the oxygen would evaporate as Al2O from the surface, which would be a reason why the photoluminescence intensity increases under higher substrate temperature and lower V/III flux ratio. The electron-trap level at 0.76 eV from the conduction band would be the recombination center, and the photoluminescence intensity is inversely proportional to the trap concentration.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 86 (1999), S. 5993-5999 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Extended x-ray absorption fine structure (EXAFS), Rutherford-backscattering ion channeling, and particle induced x-ray emission channeling (PIXE/C) measurements have been performed in order to investigate compensation centers in Cl doped ZnSeTe. The EXAFS results from Cl doped ZnSeTe suggest that almost all Cl atoms are incorporated into substitutional Se lattice sites, which seems to indicate that Cl atoms themselves are not responsible for the compensation centers. The PIXE/C angular profiles were measured across the 〈100〉, 〈110〉, and 〈111〉 axes for undoped ZnSeTe. Comparing the angular profiles for Zn Kα, Se Kα, and Te Lα x-ray yields, it was found that some portion of the Te atoms (∼1020 cm−3) are located at tetrahedral interstitial sites. From these results, the difficulty of realizing n-type ZnSeTe is considered to be due to the existence of the interstitial Te atoms which act as acceptors. © 1999 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 59 (1991), S. 1482-1484 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We studied vacancy type defects in Ga-doped ZnSe films grown by molecular beam epitaxy using an energy-variable monoenergetic positron beam. We found that the concentration of negative charged vacancies, such as Zn vacancies, increases as the Ga atom concentration increases. This result indicates that the doping by Ga atoms induces the formation of Zn vacancies in a ZnSe film. We believe that these defects will cause the saturation of active carriers in n-type ZnSe films.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 4 (1997), S. 3101-3112 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Interaction of charged particles with various types of one-dimensional pulses is investigated systematically. Gaussian pulses of arbitrary velocity and polarization, both electrostatic and electromagnetic, are considered. The pulses range from ordinary wave packets to impulses. Analytic expressions are obtained for velocities of charged particles interacting with those traveling pulses, and are compared with numerical counterparts. Dependence of the interaction on pulse size, initial particle velocity, and external magnetic field is investigated. For many nonrelativistic pulses traveling along an external magnetic field, the interaction can be divided into two types, i.e., transit-time acceleration and reflection in the wave frame. In the absence of the magnetic field, transit-time acceleration is significant only for impulses with sizes of less than one wavelength. On the other hand, with a magnetic field (transit-time) cyclotron acceleration becomes possible for pulses of sizes greater than one wavelength. With larger amplitudes the wave-frame reflection becomes increasingly important, typically occurring at the pulse head or tail. However, it tends to be suppressed by external magnetic fields. Compact expressions are obtained for final velocities of the particles for the two types of interaction. Both types of acceleration mechanism may be important in dissipating relatively large-amplitude waves. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 3 (1996), S. 2559-2563 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A new mechanism for Langmuir wave localization is investigated. Typical computer simulation of weak electron beam–plasma instabilities proceeds as follows: As Langmuir waves grow out of the noise, they react back on the beam particles by trapping. The subsequent phase shift puts the electrons out of phase with the waves. Then the instability is locally quenched, resulting in strong wave modulation, even before saturation of the instabilities. The typical size of wave packets is given by 2πvp/ω¯t, where vp and ω¯t denote the phase speed of the dominant wave and the average bounce frequency, respectively. The time scale for this process is considerably shorter than that of parametric instabilities. © 1996 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 2 (1995), S. 649-653 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Parametric instabilities of Langmuir waves in strong magnetic fields such that Ωe(approximately-greater-than)ωe were investigated, where Ωe(ωe) denotes the electron cyclotron (plasma) frequency. It has been well established that as a plasma is more strongly magnetized, the parametric instabilities of Langmuir waves become more field aligned and thus one dimensional. Here, it is demonstrated that this trend continues only up to Ωe/ωe=1, and that above this value, most Langmuir waves decay to relatively short wavelength oblique-Langmuir and ion waves that are damped rapidly. These new parametric instabilities have growth rates greater than those of the conventional modulational and decay instabilities. Consequently, the scenario of strong Langmuir turbulence in which Langmuir solitons play a major role may not apply to the strong magnetic-field regime. In the weak Langmuir turbulence regime these decay instabilities make the turbulence more isotropic. Therefore, it is concluded that there occurs a type of phase transition in magnetized Langmuir turbulence at Ωe/ωe∼1. © 1995 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 31 (1988), S. 1505-1514 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Stochastic interactions of charged particles with electrostatic waves propagating at arbitrary angles to an external magnetic field are studied based on a relativistic canonical Hamiltonian formalism. The present theory, however, is valid also for electromagnetic waves after a slight modification. The stochasticity threshold is derived utilizing Chirikov's criterion. It is found that relativistic effects are important for electrons interacting with relatively high phase velocity waves even at nonrelativistic initial energies. In particular, the relativistic generalization of a previous theory [Phys. Rev. Lett. 34, 1613 (1975); Phys. Fluids 21, 2230 (1978)] moves the degeneracy of primary resonances in nearly perpendicular directions to the angles where the parallel phase speed approximately equals the speed of light. It was also demonstrated for the first time that initially low energy electrons can gain relativistic energies (γ(very-much-greater-than)1) by means of the stochastic interaction with an electrostatic wave, where γ is the relativistic factor. Moreover, properties of second-order islands that form within primary islands have been studied. Finally, the nature of the stochastic particle energization by electrostatic waves is compared with that by electromagnetic waves, and the results are applied to the problem of electron acceleration during ionospheric modification experiments.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 31 (1988), S. 2185-2189 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A series of computer simulations is reported showing the generation of electromagnetic radiation by strong Langmuir turbulence. The simulations were carried out with a fully electromagnetic 2 1/2 -dimensional fluid code. The radiation process takes place in two stages that reflect the evolution of the electrostatic turbulence. During the first stage while the electrostatic turbulence is evolving from an initial linear wave packet into a planar soliton, the radiation is primarily at ωe. During the second stage when transverse instabilities lead to the collapse and dissipation of the solitons, 2ωe and ωe radiation are comparable, and 3ωe is also present. The radiation power at ω=2ωe is in good agreement with theoretical predictions for electromagnetic emissions by collapsing solitons.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 2 (1990), S. 606-628 
    ISSN: 1089-7666
    Source: AIP Digital Archive
    Topics: Physics
    Notes: A general theory for the acceleration of a charged particle by a coherent wave of arbitrary polarization, propagation angle, and phase velocity in the presence of a uniform and strong magnetic field is presented. It is shown that the Hamiltonian surfaces are topologically open for waves with parallel phase velocity, ω/k(parallel), equal to or larger than the speed of light. The trapping width is found to be a strong function of the index of refraction (N), and for N=1 the trapping width increases as a function of the harmonic number. Particular emphasis is put on waves with N(parallel) ≡ck(parallel)/ ω=1, and it is demonstrated that the physics of such waves is the relativistic counterpart of the nonrelativistic particle acceleration by a perpendicularly propagating wave. It is found that even at small wave amplitudes particles can be accelerated coherently to very large energies (relativistic factor γ〉8) in the presence of such waves. The autoresonance acceleration mechanism [Sov. Phys. JETP 16, 629 (1963); Phys. Rev. A 135, 381 (1964)] is shown to be a special case of particle acceleration by waves with N(parallel) =1. A detailed analysis of the dispersion properties of these waves in a cold plasma is given. Finally, a novel mechanism for coherently accelerating particles to unlimited energies is presented. This new mechanism requires waves with N(parallel) (approximately-less-than)1 and wave amplitudes large enough so that the zeroth-order particle motion is the trapping due to the wave ("weak'' magnetic field limit) rather than the Larmor gyration which was the case for the autoresonance mechanism. This new mechanism is somewhat similar to the surfatron mechanism [Phys. Rev. Lett. 51, 392 (1983)] but can operate even if the wave amplitude is smaller than the magnetic field as a result of the oblique propagation angle of the wave.
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