TY - JOUR
T1 - Spectral intensities in trivalent lanthanide systems. Applications to the Cs2NaDyCl6 and Cs2NaHoCl6 crystals
AU - Acevedo, Roberto
AU - Soto-Bubert, Andrés
AU - Bosch, Paul
AU - Strek, Wieslaw
N1 - Funding Information:
RA and ASB would like to express gratitude towards the financial support received from the Universidad de Chile, Universidad Diego Portales and Conicyt. The research project # 10.03.25.008 from the Vicerrectoria Académica-UDP is gratefully acknowledged. Finally but not at last, the Organizing Committee of the 6th International Conference on f-Elements. ICFÉ6 is truthfully acknowledged for the kindness and hospitality towards each and all participants, 4–9, September, 2006, Wroclaw, Poland.
PY - 2008/8/11
Y1 - 2008/8/11
N2 - The main goal of this research work is to rationalize the rich vibronic structure of lanthanide type crystals, such as Cs2NaDyCl6 and Cs2NaHoCl6, in the space group F m 3 m (Oh5). These systems are known to be highly relativistic and as a consequence, major corrections to previous model calculations should be taken into account so as to explain from a semi-quantitative viewpoint, the observed spectral intensities. We have decided to tackle this study taking special care, of both the physics and the chemistry involved with special emphasis on the theoretical model to be employed as well as, in the strategy to be followed to rationalize the available experimental data. This paper aims to advance our understanding of the intensity mechanisms, associated with observed radiative transitions, say for complex highly relativistic systems, in the solid state physics. The spectral intensities associated with superpositions (juxtapositions) of peaks and/or bands in the absortion and emission spectra are considered in detail and a preliminary working methodology is put forward with reference to the Cs2NaDyCl6 and Cs2NaHoCl6 crystals.
AB - The main goal of this research work is to rationalize the rich vibronic structure of lanthanide type crystals, such as Cs2NaDyCl6 and Cs2NaHoCl6, in the space group F m 3 m (Oh5). These systems are known to be highly relativistic and as a consequence, major corrections to previous model calculations should be taken into account so as to explain from a semi-quantitative viewpoint, the observed spectral intensities. We have decided to tackle this study taking special care, of both the physics and the chemistry involved with special emphasis on the theoretical model to be employed as well as, in the strategy to be followed to rationalize the available experimental data. This paper aims to advance our understanding of the intensity mechanisms, associated with observed radiative transitions, say for complex highly relativistic systems, in the solid state physics. The spectral intensities associated with superpositions (juxtapositions) of peaks and/or bands in the absortion and emission spectra are considered in detail and a preliminary working methodology is put forward with reference to the Cs2NaDyCl6 and Cs2NaHoCl6 crystals.
KW - CsNaDyCl and CsNaHoCl systems
KW - Spectral intensities
UR - http://www.scopus.com/inward/record.url?scp=44649199223&partnerID=8YFLogxK
U2 - 10.1016/j.jallcom.2008.01.129
DO - 10.1016/j.jallcom.2008.01.129
M3 - Article
AN - SCOPUS:44649199223
SN - 0925-8388
VL - 461
SP - 53
EP - 57
JO - Journal of Alloys and Compounds
JF - Journal of Alloys and Compounds
IS - 1-2
ER -