Single photon infrared emission spectroscopy:: A study of IR emission from UV laser excited PAHs between 3 and 15 μm

被引:65
作者
Cook, DJ [1 ]
Schlemmer, S [1 ]
Balucani, N [1 ]
Wagner, DR [1 ]
Harrison, JA [1 ]
Steiner, B [1 ]
Saykally, RJ [1 ]
机构
[1] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA
关键词
D O I
10.1021/jp9724434
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Single-photon infrared emission spectroscopy (SPIRES) has been used to measure emission spectra from polycyclic aromatic hydrocarbons (PAHs). A supersonic free-jet expansion has been used to provide emission spectra of rotationally cold and vibrationally excited naphthalene and benzene. Under these conditions, the observed width of the 3.3-mu m (C-H stretch) band resembles the bandwidths observed in experiments in which emission is observed from naphthalene with higher rotational energy. To obtain complete coverage of IR wavelengths relevant to the unidentified infrared bands (UIRs), UV laser-induced desorption was used to generate gas-phase highly excited PAHs. Lorentzian band shapes were convoluted with the monochromator-slit function in order to determine the widths of PAH emission bands under astrophysically relevant conditions. Bandwidths were also extracted from bands consisting of multiple normal modes blended together. These parameters are grouped according to the functional groups mostly involved in the vibration, and mean bandwidths are obtained. These bandwidths are larger than the widths of the corresponding UIR bands. However, when the comparison is limited to the largest PAHs studied, the bandwidths are slightly smaller than the corresponding UIR bands. These parameters can be used to model emission spectra from PAH cations and cations of larger PAHs, which are better candidate carriers of the UIRs.
引用
收藏
页码:1465 / 1481
页数:17
相关论文
共 65 条
  • [1] Allain T, 1996, ASTRON ASTROPHYS, V305, P616
  • [2] Allain T, 1996, ASTRON ASTROPHYS, V305, P602
  • [3] INTERSTELLAR POLYCYCLIC AROMATIC-HYDROCARBONS - THE INFRARED-EMISSION BANDS, THE EXCITATION EMISSION MECHANISM, AND THE ASTROPHYSICAL IMPLICATIONS
    ALLAMANDOLA, LJ
    TIELENS, AGGM
    BARKER, JR
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1989, 71 (04) : 733 - 775
  • [4] Allamandola LJ, 1995, ASTR SOC P, V73, P23
  • [5] POLYCYCLIC AROMATIC-HYDROCARBONS AND THE UNIDENTIFIED INFRARED-EMISSION BANDS - AUTO EXHAUST ALONG THE MILKY-WAY
    ALLAMANDOLA, LJ
    TIELENS, AGGM
    BARKER, JR
    [J]. ASTROPHYSICAL JOURNAL, 1985, 290 (01) : L25 - L28
  • [6] THE DISCOVERY OF A NEW INFRARED-EMISSION FEATURE AT 1905 WAVENUMBERS (5.25 MICRONS) IN THE SPECTRUM OF BD +30-DEGREES-3639 AND ITS RELATION TO THE POLYCYCLIC AROMATIC HYDROCARBON MODEL
    ALLAMANDOLA, LJ
    BREGMAN, JD
    SANDFORD, SA
    TIELENS, AGGM
    WITTEBORN, FC
    WOODEN, DH
    RANK, D
    [J]. ASTROPHYSICAL JOURNAL, 1989, 345 (01) : L59 - L62
  • [7] THE EBULLIOMETRIC METHOD OF VAPOR-PRESSURE MEASUREMENT - VAPOR-PRESSURES OF BENZENE, HEXAFLUOROBENZENE, AND NAPHTHALENE
    AMBROSE, D
    EWING, MB
    GHIASSEE, NB
    OCHOA, JCS
    [J]. JOURNAL OF CHEMICAL THERMODYNAMICS, 1990, 22 (06) : 589 - 605
  • [8] [Anonymous], 1984, OPTICAL RAD DETECTOR
  • [9] [Anonymous], 1996, IG PRO
  • [10] BARKER JR, 1987, ASTROPHYS J, V315, P661