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Transition probabilities for the hydrogen atom in intense magnetic fields using the adiabatic approximation: Comparison with variational results

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/158312· OSTI ID:6635655
Using accurate numerical wave functions within the adiabatic approximation, we calculate transition rates for the hydrogen atom in strong magnetic fields (of order 10/sup 10/--10/sup 12/ gauss, which are assumed for neutron stars), and compare with variational results of Wadehra. An error inherent in his work is pointed out. It is found that using numerical wave functions within the adiabatic approximation leads to values for the transition rates which are larger than the ones of the variational calculation by about 15%.
Research Organization:
Institut fuer Theoretische Physik, Universitaet Erlangen-Nuernberg, West Germany
OSTI ID:
6635655
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 242:3; ISSN ASJOA
Country of Publication:
United States
Language:
English