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A highly optimized code for calculating atomic data at neutron star magnetic field strengths using a doubly self-consistent Hartree–Fock–Roothaan method

✍ Scribed by Schimeczek, C.; Engel, D.; Wunner, G.


Book ID
122148733
Publisher
Elsevier Science
Year
2014
Tongue
English
Weight
313 KB
Volume
185
Category
Article
ISSN
0010-4655

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