scholarly journals Richardson–Gaudin mean-field for strong correlation in quantum chemistry

2020 ◽  
Vol 153 (10) ◽  
pp. 104110 ◽  
Author(s):  
Paul A. Johnson ◽  
Charles-Émile Fecteau ◽  
Frédéric Berthiaume ◽  
Samuel Cloutier ◽  
Laurie Carrier ◽  
...  
1988 ◽  
Vol 57 (2) ◽  
pp. 401-404 ◽  
Author(s):  
Yoshikazu Suzumura ◽  
Yasumasa Hasegawa ◽  
Hidetoshi Fukuyama

Author(s):  
Kenneth G. Dyall ◽  
Knut Faegri

It is well known from nonrelativistic quantum chemistry that mean-field methods, such as the Hartree–Fock (HF) model, provide mainly qualitative insights into the electronic structure and bonding of molecules. To obtain reliable results of “chemical accuracy” usually requires models that go beyond the mean field and account for electron correlation. There is no reason to expect that the mean-field approach should perform significantly better in this respect for the relativistic case, and so we are led to develop schemes for introducing correlation into our models for relativistic quantum chemistry. There is no fundamental change in the concept of correlation between relativistic and nonrelativistic quantum chemistry: in both cases, correlation describes the difference between a mean-field description, which forms the reference state for the correlation method, and the exact description. We can also define dynamical and nondynamical correlation in both cases. There is in fact no formal difference between a nonrelativistic spin–orbital-based formalism and a relativistic spinor-based formalism. Thus we should be able to transfer most of the schemes for post-Hartree–Fock calculations to a relativistic post-Dirac–Hartree–Fock model. Several such schemes have been implemented and applied in a range of calculations. The main technical differences to consider are those arising from having to deal with integrals that are complex, and the need to replace algorithms that exploit the nonrelativistic spin symmetry by schemes that use time-reversal and double-group symmetry. In addition to these technical differences, however, there are differences of content between relativistic and nonrelativistic methods. The division between dynamical and nondynamical correlation is complicated by the presence of the spin–orbit interaction, which creates near-degeneracies that are not present in the nonrelativistic theory. The existence of the negative-energy states of relativistic theory raise the question of whether they should be included in the correlation treatment. The first two sections of this chapter are devoted to a discussion of these issues. The main challenges in the rest of this chapter are to handle the presence of complex integrals and to exploit time-reversal symmetry.


2018 ◽  
Vol 149 (8) ◽  
pp. 081101 ◽  
Author(s):  
Jacqueline A. R. Shea ◽  
Eric Neuscamman

2011 ◽  
Vol 106 (9) ◽  
Author(s):  
Nan Lin ◽  
C. A. Marianetti ◽  
Andrew J. Millis ◽  
David R. Reichman

2016 ◽  
Vol 22 (1) ◽  
pp. 28
Author(s):  
Sri Yudawati Cahyarini ◽  
B. Suwargadi

Coral ?18O from Maudulung-Indonesia was analyzed using Finnigan MAT 251. Using statistical analysis from KNMI database is obtained that the seasonal mean field correlation between coral ? 18OSOI shows strong correlation during October. Field correlation of precipitation-coral ? 18O shows opposite pattern between eastern Pacific and western Pacific during strong El Nino event. Keywords: coral ?18O, field correlation, El Niño, Maudulung Sumba. Kandungan ?18O dalam koral dari wilayah Maudulung, Sumba, dianalisis dengan menggunakan Finnigan MAT 251. Korelasi spasial antara ?18O dengan SOI dalam skala musiman tinggi selama bulan Oktober. Korelasi spasial ini dilakukan dengan menggunakan fasilitas analisa statistik dalam database KNMI. Korelasi spasial antara presipitasi- coral ?18O menunjukkan pola-pola yang berlawanan antara wilayah timur dan barat Pasifi selama El Niño. Kata kunci: Koral ?18O, korelasi spasial, El Niño, Maudulung Sumba.


1988 ◽  
Vol 02 (10) ◽  
pp. 1205-1209 ◽  
Author(s):  
R.B. TAO ◽  
X. HU ◽  
M. SUZUKI

Baskaran’s mean field approximation of the Hubbard Hamiltonian with strong correlation and half-filling is discussed. Our calculations show that his decoupling of the Hamiltonian is not permissible in the half-filling case and that it destroys the equivalence of the Hubbard model to the Heisenberg magnetic system and violates some spin-spin relations.


2009 ◽  
Author(s):  
Christian Ochsenfeld ◽  
George Maroulis ◽  
Theodore E. Simos

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