Tchaplyguine M, Kivimäki A, Peredkov S, Sorensen S L, Ohrwall G, Schulz J, Lundwall M, Rander T, Lindblad A, Rosso A, Svensson S, Mårtensson N, Björneholm O
MAX-lab, Lund University, P.O. Box 118, SE-221 00 Lund, Sweden.
J Chem Phys. 2007 Sep 28;127(12):124314. doi: 10.1063/1.2770460.
We present Auger spectroscopy studies of large krypton clusters excited by soft x-ray photons with energies on and just above the 3d(52) ionization threshold. The deexcitation spectra contain new features as compared to the spectra measured both below and far above threshold. Possible origins of these extra features, which stay at constant kinetic energies, are discussed: (1) normal Auger process with a postcollision interaction induced energy shift, (2) recapture of photoelectrons into high Rydberg orbitals after Auger decay, and (3) excitation into the conduction band (or "internal" ionization) followed by Auger decay. The first two schemes are ruled out, hence internal ionization remains the most probable explanation.
我们展示了对由能量处于并略高于3d(52)电离阈值的软X射线光子激发的大氪团簇的俄歇光谱研究。与在阈值以下和远高于阈值处测量的光谱相比,去激发光谱包含新的特征。讨论了这些保持恒定动能的额外特征的可能起源:(1) 具有碰撞后相互作用引起的能量位移的正常俄歇过程,(2) 俄歇衰变后光电子重新俘获到高里德堡轨道,以及(3) 激发到导带(或“内部”电离)随后进行俄歇衰变。前两种方案被排除,因此内部电离仍然是最有可能的解释。