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The , , and band spectra of HCSi radical were investigated by means of near-infrared diode laser spectroscopy to determine precise molecular constants for the and states. The detailed analysis of the rotationally resolved band spectra, studied for the first time in the present investigation, leads to the precise determination of molecular constants for the state associated with the Renner-Teller interaction. We obtained −0.15126663(53) and 495.00698(30) cm−1 as the Renner-Teller parameter ε and the bending vibrational frequency ω2, respectively. Based on the molecular constants for the and states, the rotational levels of the state were analyzed to obtain molecular constants and information on upper state perturbations. Using the available spectroscopic data, valence force fields for both the and states were estimated to aid in understanding the vibrational energy levels of the HCSi radical.  相似文献   

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High precision rotational spectra of isotopic oxygen O2 (with or ) in its electronic ground state have been measured in selected frequency regions between 0.4 and 2.0 THz. The main isotopic species, , was also investigated in its first excited electronic state . The new data, analyzed together with previous measurements, yielded improved spectroscopic parameters.  相似文献   

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A. Chafiq 《Optics Communications》2009,282(13):2590-2594
Based on the irradiance moments definitions, the expression of factor of truncated zeroth-order Mathieu-Gauss beams (MGBs) is derived analytically. Furthermore, the propagation equation of kurtosis parameter of non-truncated MBGs passing through a paraxial ABCD optical system is established. Particularly, the dependence of factor and kurtosis parameter on the spatial profile of the beam are illustrated numerically and analyzed in details.  相似文献   

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Since the energy of a reactor neutrino is a few MeV, all , and oscillations are accessible by reactor neutrino experiments. KamLAND observed the oscillation and currently Double Chooz, RENO and Dayabay experiments are under construction aiming to detect oscillation. There are still good prospects for future reactor neutrino experiments after them. For example, there is room to further improve sin22θ13 accuracy at a baseline of ∼1.5 km, a very precise sin22θ12 measurement and the determination of mass hierarchy may be possible at a baseline ∼50 km, and if KamLAND is enlarged to the SuperKamiokande size, better measurement of and sin22θ12 will be anticipated. It is important to take into account such possibilities when planning future neutrino program after θ13 is measured by current experiments.  相似文献   

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