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  • 1
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 94 (1991), S. 818-819 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 672 (1992), S. 0 
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 105 (1996), S. 2298-2308 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: We report the 790 nm photofragmentation of mass-selected I−2⋅Arn clusters, n=1 to 27. We determine the I−+I caging efficiency as a function of the number of solvent Ar atoms and compare these results with I−2 in CO2 clusters. Caging is much less effective with Ar. In addition to "normal'' caged photoproducts (I−2⋅Arm, where m〈n), the evaporation process following photoexcitation produces "solvent-separated'' (I−...I)⋅Arm photofragments, where the I−2 bond has not reformed. These metastable species comprise ∼55% of the photofragment yield for precursor clusters for n≥14 and have lifetimes (approximately-greater-than)5 μs. This unusual photofragment exists either as a trapped excited electronic state or as a solvent-separated pair at an internuclear separation of ∼5.5 A(ring). The photofragmentation data also exhibit the existence of two distinct isomeric forms of the precursor I−2⋅Arn, for n≤14. These forms are evaporatively distinct in that one isomer displays highly nonstatistical fragmentation, probably arising from a cluster in which the I−2 resides on the surface, rather than in the interior. The photofragmentation distribution of the other form exhibits statistical behavior, consistent with the evaporation of an I−2 solvated inside the cluster. © 1996 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 106 (1997), S. 1402-1410 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: We report time-resolved photodissociation and geminate recombination dynamics of I2− in size-selected I2− Arn and I2−(CO2)n cluster ions by using ultrafast pump–probe techniques at 790 nm in conjunction with a tandem time-of-flight mass spectrometer. The absorption recovery, which reflects the time scale for photodissociation followed by recombination and vibrational relaxation of I2− inside the cluster, shows a strong dependence on the composition of the surrounding cluster solvent. The absorption recovery time for I2−(CO2)16 is ∼1 ps, whereas for I2−Ar20 it is ∼130 ps. This difference is discussed in terms of electrostatic and hard sphere interactions. We also observe the time dependence of the destruction of the Ar solvent cage for I2−Ar16. Finally, absorption recovery data for I2−(CO2)n cluster ions taken with 790 nm pump–probe wavelengths are compared with the greater energy release 720 nm data. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 78 (1995), S. 3792-3796 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We report on manipulation of nucleation by means of periodic modulation of the growth rate R, both during molecular beam epitaxial growth of Si on Si(111) and using a simulated bilayer structure. We have found that the bilayer-by-bilayer growth can be improved and that the surface roughness can be reduced by applying the R modulation synchronized with the deposition of a multiple of full bilayers. For nonsynchronized growth the phase of reflection high-energy electron diffraction (RHEED) intensity oscillations could be shifted relative to the bilayer deposition period and a beating phenomenon of the RHEED oscillations was observed, which can be attributed to the superimposed effects of the R modulation and the regular bilayer-by-bilayer growth. We have used the phenomenological correspondence between the surface step density and the RHEED oscillations as a basis to discuss the growth. By employing a kinetic solid-on-solid Monte Carlo model without vacancies and overhangs all significant experimental features could be simulated. © 1995 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)
    Review of Scientific Instruments 72 (2001), S. 4300-4301 
    ISSN: 1089-7623
    Source: AIP Digital Archive
    Topics: Physics , Electrical Engineering, Measurement and Control Technology
    Notes: Laser induced fluorescence spectroscopy has been applied for the first time on a stored fast molecular ion beam. The rotational temperature of the N2+ ion beam was studied as a function of storage time. For up to 1 s of storage time, a temperature of 1040 K can be used to describe the rotational energy distribution. © 2001 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)
    Journal of Applied Physics 82 (1997), S. 1507-1510 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The capability of diffraction intensity fluctuations to probe dynamic phenomena at equilibrium is studied. The summation of fluctuations over different domains that scatter incoherently, the role of statistically "white-noise" generated fluctuations and the time necessary to collect a sufficiently long signal are investigated. The factors that determine the number of incoherent regions, and maximize the relative fluctuation without reducing the count rate to such low values that impractically long acquisition times are needed are discussed. Monte Carlo simulations modeling thermally generated step fluctuations are used to illustrate the results. © 1997 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 65 (1994), S. 1409-1411 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: High quality, completely relaxed Ge films have been grown on Si(111) using Sb as surfactant at the initial stage of growth. After desorbing the surface Sb layer, cusplike reflection high-energy electron diffraction intensity oscillations indicated excellent Ge layer-by-layer epitaxy. High resolution x-ray diffraction analysis showed a very high crystalline quality and well resolved thickness fringes consistent with a flat relaxed Ge layer. Chemical preferential etching experiments revealed a defect density of down to ∼3×104 cm−2.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 83 (1985), S. 3034-3041 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: HCN has been observed to be a constituent of late type carbon-rich stellar atmospheres and has recently been suggested to be a very important opacity source in cooler carbon stars. The transitions giving rise to the combination vibration–rotation bands in the near infrared region may be expected to be the most important HCN transitions for the structure of the carbon-star atmospheres. In this paper CASSCF and CCI calculations of vibrational bands in the interval 3000–10 000 cm−1 are presented. Accounting for the HCN opacity extends the model atmosphere by a factor of 5, and lowers the gas pressure in the surface layers by one or two orders of magnitude. The structures, e.g., the gas pressures, in the upper layers of these models are uncertain by more than a factor of 3 as a result of the uncertainties in the potential surface of the molecule and in the method for handling the degeneracy for the vibrational bands. These uncertainties are, however, of minor importance in practical applications in present carbon-star work.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 85 (1986), S. 4208-4208 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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