Experimental transition probabilities and J-file sum rule test for the transition array 3p-3d in neutral neon

被引:7
作者
Baclawski, A. [1 ]
机构
[1] Opole Univ, Inst Phys, PL-45052 Opole, Poland
关键词
D O I
10.1088/0953-4075/41/22/225701
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Seventy four intensities of neutral neon lines (Ne I), belonging to transitions 3p-3d, 3p'-3d, 3p-3d', and 3p'-3d' (all in short denoted as 3p-3d), have been measured. The neon plasma produced in a wall-stabilized arc has been applied as the excitation source for neon atoms. From measured Ne I line intensities the respective relative transition probabilities (A(ki)) have been determined. The absolute scale for the Aki data has been established by normalizing them to the radiative lifetime value for the level 2s(2)2p(5) (P-2(1/2)degrees) 3d(2)[3/2](2)degrees. The obtained transition probabilities have been compared with theoretical data and with results of previous experiments. The transition probabilities have been then converted to line strengths data and used for testing the J-file sum rule for the transition array 3p-3d. Some discrepancies between the measured data set and the results predicted by the J-file sum rule have been found.
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页数:12
相关论文
共 26 条
[1]   ANALYSES OF LIGHT-ION SPECTRA IN STELLAR ATMOSPHERES .5. NEON I IN B STARS [J].
AUER, LH ;
MIHALAS, D .
ASTROPHYSICAL JOURNAL, 1973, 184 (01) :151-166
[2]   TRANSITION PROBABILITIES FOR PROMINENT RED LINES OF NE-I [J].
BRIDGES, JM ;
WIESE, WL .
PHYSICAL REVIEW A, 1970, 2 (02) :285-&
[3]   Neon abundances in B stars of the Orion association: Solving the solar model problem? [J].
Cunha, Katia ;
Hubeny, Ivan ;
Lanz, Thierry .
ASTROPHYSICAL JOURNAL, 2006, 647 (02) :L143-L146
[4]  
CZERNICHOWSKI A, 1977, J PHYS-PARIS, V38, P1065, DOI 10.1051/jphys:019770038090106500
[5]  
del Val JA, 2000, ASTRON ASTROPHYS, V357, P1137
[6]   VALIDITY CONDITIONS FOR LOCAL THERMODYNAMIC EQUILIBRIUM [J].
DRAWIN, HW .
ZEITSCHRIFT FUR PHYSIK, 1969, 228 (02) :99-+
[7]   Neon abundances in normal late-B and mercury-manganese stars [J].
Dworetsky, MM ;
Budaj, J .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2000, 318 (04) :1264-1272
[8]   Breit-Pauli energy levels, lifetimes, and transition probabilities for the beryllium-like to neon-like sequences [J].
Fischer, CF ;
Tachiev, G .
ATOMIC DATA AND NUCLEAR DATA TABLES, 2004, 87 (01) :1-184
[9]   2-PHOTON LASER EXCITATION OF 2P5(2P1/2) 3D LEVELS OF NEON [J].
GARCIA, G ;
ORTIZ, M ;
BLANCO, F ;
SANCHEZ, JA ;
CAMPOS, J .
CANADIAN JOURNAL OF PHYSICS, 1989, 67 (10) :977-979
[10]   ENERGIES, OSCILLATOR-STRENGTHS, AND LIFETIMES FOR NEON-LIKE IONS UP TO KR-XXVII [J].
HIBBERT, A ;
LEDOURNEUF, M ;
MOHAN, M .
ATOMIC DATA AND NUCLEAR DATA TABLES, 1993, 53 (01) :23-112