Optical excitation function of H(1s-2p) produced by electron impact from threshold to 1.8 keV

被引:18
作者
James, GK
Slevin, JA
Shemansky, DE
McConkey, JW
Bray, I
Dziczek, D
Kanik, I
Ajello, JM
机构
[1] ST PATRICKS COLL, DEPT EXPT PHYS, MAYNOOTH, KILDARE, IRELAND
[2] UNIV SO CALIF, DEPT AEROSP ENGN, LOS ANGELES, CA 90089 USA
[3] UNIV WINDSOR, DEPT PHYS, WINDSOR, ON N9B 3P4, CANADA
[4] FLINDERS UNIV S AUSTRALIA, ELECT STRUCT MAT CTR, ADELAIDE, SA 5001, AUSTRALIA
[5] NICHOLAS COPERNICUS UNIV, INST PHYS, PL-87100 TORUN, POLAND
关键词
D O I
10.1103/PhysRevA.55.1069
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The optical excitation function of prompt Lyman-alpha radiation, produced by electron impact on atomic hydrogen, has been measured over the extended energy range from threshold to 1.8 keV. Measurements were obtained in a crossed-beams experiment using both magnetically confined and electrostatically focused electrons in collision with atomic hydrogen produced by an intense discharge source. A vacuum-ultraviolet monochromator system was used to measure the emitted Lyman-alpha radiation. The absolute H(1s-2p) electron impact excitation cross section was obtained from the experimental optical excitation function by normalizing to the accepted optical oscillator strength, with corrections for polarization and cascade. Our data are significantly different from the earlier experimental results of R. L. Long et at, J. Res. Natl. Bur. Stand. Sect. A 72A, 521 (1968) and J. F. Williams, J. Phys. B 9, 1519 (1976); 14, 1197 (1981), which are limited to energies' below 200 eV. Statistical and known systematic uncertainties in our data range from +/-4% near threshold to +/-2% at 1.8 keV. Multistate coupling affecting the shape of the excitation function up to 1 keV impact energy is apparent in both the present experimental data and present theoretical results obtained with convergent close-coupling (CCC) theory. This shape function effect leads to an uncertainty in absolute cross sections at the 10% level in the analysis of the experimental data. The derived optimized absolute cross sections are within 7% of the CCC calculations over the 14 eV-1.8 keV range. The present CCC calculations converge on the Bethe-Fano profile for H(1s-2p) excitation at high energy. For this reason agreement with the CCC values to within 3% is achieved in a nonoptimal normalization of the experimental data to the Bethe-Fano profile. The fundamental H(1s-2p) electron impact cross section is thereby determined to an unprecedented accuracy over the 14 eV - 1.8 keV energy range.
引用
收藏
页码:1069 / 1087
页数:19
相关论文
共 51 条
[31]   THE POLARIZATION OF ATOMIC LINE RADIATION EXCITED BY ELECTRON IMPACT [J].
PERCIVAL, IC ;
SEATON, MJ .
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1958, 251 (990) :113-138
[32]   THE LIFETIME OF THE 22S1/2 STATE OF HYDROGEN IN AN IONIZED ATMOSPHERE [J].
PURCELL, EM .
ASTROPHYSICAL JOURNAL, 1952, 116 (03) :457-462
[33]   BACKWARD PEAK IN THE ELECTRON SPECTRUM FROM COLLISIONS OF 70-KEV PROTONS WITH A TARGET FROM A HYDROGEN-ATOM SOURCE [J].
RUDD, ME ;
GEALY, MW ;
KERBY, GW ;
HSU, YY .
PHYSICAL REVIEW LETTERS, 1992, 68 (10) :1504-1506
[34]  
SCHARTNER KH, COMMUNICATION
[35]   ELECTRON-SCATTERING BY ATOMIC-HYDROGEN AT INTERMEDIATE ENERGIES .1. INTEGRATED ELASTIC, 1S-2S AND 1S-2P CROSS-SECTIONS [J].
SCOTT, MP ;
SCHOLZ, TT ;
WALTERS, HRJ ;
BURKE, PG .
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1989, 22 (19) :3055-3077
[36]   VACUUM ULTRAVIOLET STUDIES OF ELECTRON-IMPACT OF HELIUM - EXCITATION OF HE N 1PO RYDBERG SERIES AND IONIZATION-EXCITATION OF HE+ NL RYDBERG SERIES [J].
SHEMANSKY, DE ;
AJELLO, JM ;
HALL, DT ;
FRANKLIN, B .
ASTROPHYSICAL JOURNAL, 1985, 296 (02) :774-783
[37]   ELECTRON-IMPACT EXCITATION OF H-2 - RYDBERG BAND SYSTEMS AND THE BENCHMARK DISSOCIATIVE CROSS-SECTION FOR H-LYMAN-ALPHA [J].
SHEMANSKY, DE ;
AJELLO, JM ;
HALL, DT .
ASTROPHYSICAL JOURNAL, 1985, 296 (02) :765-773
[38]   THE VOYAGER-1 EUV SPECTRUM OF THE IO PLASMA TORUS [J].
SHEMANSKY, DE ;
SMITH, GR .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1981, 86 (NA11) :9179-9192
[39]  
SHEMANSKY DE, IN PRESS ASTROPHYS J
[40]   RADIO-FREQUENCY ATOMIC-HYDROGEN BEAM SOURCE [J].
SLEVIN, J ;
STIRLING, W .
REVIEW OF SCIENTIFIC INSTRUMENTS, 1981, 52 (11) :1780-1782