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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 C. Schimeczek; D. Engel; G. Wunner


Book ID
113554394
Publisher
Elsevier Science
Year
2012
Tongue
English
Weight
260 KB
Volume
183
Category
Article
ISSN
0010-4655

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