Electronic excitation in transmission of relativistic H{sup {minus}} ions through thin foils
Conference
·
OSTI ID:658430
- Oak Ridge National Lab., TN (United States). Physics Div.
- Centre Interdisciplinaire de Recherche avec les Ions Lourds, Caen (France)
The authors describe a theoretical model to study the transmission of relativistic H{sup {minus}} ions through thin carbon foils. The approach is based on a Monte Carlo solution of the Langevin equation describing electronic excitations of the atoms during the transport through the foil. Calculations for the subshell populations of outgoing hydrogen atoms are found to be in good agreement with recent experimental data on an absolute scale and show that there exists a propensity for populating extreme Stark states.
- Research Organization:
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- Sponsoring Organization:
- USDOE Office of Energy Research, Washington, DC (United States)
- DOE Contract Number:
- AC05-96OR22464
- OSTI ID:
- 658430
- Report Number(s):
- ORNL/CP-98338; CONF-980564-; ON: DE98005661; BR: KC0301030; TRN: 98:011272
- Resource Relation:
- Conference: 4. international symposium on swift heavy ions in matter (SHIM 98), Berlin (Germany), 11-15 May 1998; Other Information: PBD: 7 May 1998
- Country of Publication:
- United States
- Language:
- English
Similar Records
Excited-state subshell population of hydrogen atoms after transmission of relativistic H{sup {minus}} ions through thin foils
Simulation of excited-state formation of hydrogen in transmission of relativistic H{sup {minus}} ions through thin foils
Monte Carlo simulation of transmission of relativistic H{sup {minus}} beams through thin carbon foils
Journal Article
·
Tue Sep 01 00:00:00 EDT 1998
· Physical Review A
·
OSTI ID:658430
+1 more
Simulation of excited-state formation of hydrogen in transmission of relativistic H{sup {minus}} ions through thin foils
Journal Article
·
Wed May 01 00:00:00 EDT 1996
· Physical Review A
·
OSTI ID:658430
Monte Carlo simulation of transmission of relativistic H{sup {minus}} beams through thin carbon foils
Conference
·
Sat Dec 31 00:00:00 EST 1994
·
OSTI ID:658430