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The RDM method problems in SDPA sparse format

This GitHub repository is a "modern" presentation of the original RDM library by Nakata, Maho [email protected] or [email protected] hosted at http://nakatamaho.riken.jp/rdmsdp/sdp_rdm.html.

The data directory contains only the eight largest problem Instances from the first table.

Introduction

The RDM method is promising method, using 2-RDM as a basic variable and minimize the total energy which is a linear to the Hamiltonian with respect to so called N-representability conditions. Since N-representability condition is known to be very hard to solve, we pose approximate N-representability conditions like P, Q, G, T1, T2, or T2'. The total energies by this method is comparable to CCSD(T), and these SDPs are really huge, and are challenge in both mathematical programming and chemistry.

Try them with your SDP solver! Format is the SDPA's sparse format. You can solve problems with your SDP solver, which are available as SDPA, SDPA-GMP, SeDuMi, CSDP, and SDTP3 etc.

Notes

All files are gzip'ed to reduce the size. For molecules' case you should add the core energy to the optimal to reproduce the results. The rank is the twice of number of molecular orbitals and define the size of the problems. If the rank (twice # of MO) becomes bigger, problem size becomes bigger. Not all the results of 1D hubbard model are uploaded, also I recalculated. For the Hubbard models, you may need multiple precision version of SDP solver, like SDPA-GMP, SDPA-QD, or SDPA-DD.

All data in one file

Citations (Citation count by the web of science)

  • Problems: Variational calculation of second-order reduced density matrices by strong N-representability conditions and an accurate semidefinite programming solver

    Maho Nakata, Bastiaan J. Braams, Katsuki Fujisawa, Mituhiro Fukuda, Jerome K. Percus, Makoto Yamashita, and Zhengji Zhao. Journal of chemical physics, 128, 16 164113 (2008) (5) DOI: 10.1063/1.2911696

  • Basics: Variational calculations of fermion second-order reduced density matrices by semidefinite programming algorithm.

    Maho Nakata, Hiroshi Nakatsuji, Masahiro Ehara, Mituhiro Fukuda, Kazuhide Nakata, and Katsuki Fujisawa. Journal of Chemical Physics, 114, 8282-8292 (2001) (96) DOI: 10.1063/1.1360199

SDP problem files in SDPA sparse format

Atoms and molecules

Randomly chosen from [1]. You should add the core energy to the optimal to reproduce the paper's results.

Problems (dat-s, gzip'ed) result (gzip'ed) rank core energy comment
C.3P.DZ.pqg.dat-s.gz C.3P.DZ.pqg.result.gz 20 0.0 PQG
C.3P.DZ.pqgt1.dat-s.gz C.3P.DZ.pqgt1.result.gz 20 0.0 PQGT1
C.3P.DZ.pqgt1t2.dat-s.gz C.3P.DZ.pqgt1t2.result.gz 20 0.0 PQGT1T2
C.3P.DZ.pqgt1t2p.dat-s.gz C.3P.DZ.pqgt1t2p.result.gz 20 0.0 PQGT1T2'
Ne.1S.DZ.pqg.dat-s.gz Ne.1S.DZ.pqg.result.gz 20 0.0 PQG
Ne.1S.DZ.pqgt1.dat-s.gz Ne.1S.DZ.pqgt1.result.gz 20 0.0 PQGT1
Ne.1S.DZ.pqgt1t2.dat-s.gz Ne.1S.DZ.pqgt1t2.result.gz 20 0.0 PQGT1T2
Ne.1S.DZ.pqgt1t2p.dat-s.gz Ne.1S.DZ.pqgt1t2p.result.gz 20 0.0 PQGT1T2'
O2+.2Pig.STO6G.pqg.dat-s.gz O2+.2Pig.STO6G.pqg.result.gz 20 3.033620918667e+01 PQG
O2+.2Pig.STO6G.pqgt1.dat-s.gz O2+.2Pig.STO6G.pqgt1.result.gz 20 3.033620918667e+01 PQGT1
O2+.2Pig.STO6G.pqgt1t2.dat-s.gz O2+.2Pig.STO6G.pqgt1t2.result.gz 20 3.033620918667e+01 PQGT1T2
O2+.2Pig.STO6G.pqgt1t2p.dat-s.gz O2+.2Pig.STO6G.pqgt1t2p.result.gz 20 3.033620918667e+01 PQGT1T2'
NH.1Delta.DZ.pqg.dat-s.gz NH.1Delta.DZ.pqg.result.gz 24 3.582091425394e+00 PQG
NH.1Delta.DZ.pqgt1.dat-s.gz NH.1Delta.DZ.pqgt1.result.gz 24 3.582091425394e+00 PQGT1
NH.1Delta.DZ.pqgt1t2.dat-s.gz NH.1Delta.DZ.pqgt1t2.result.gz 24 3.582091425394e+00 PQGT1T2
NH.1Delta.DZ.pqgt1t2p.dat-s.gz NH.1Delta.DZ.pqgt1t2p.result.gz 24 3.582091425394e+00 PQGT1T2'
CH.2Pir.DZ.pqg.dat-s.gz CH.2Pir.DZ.pqg.result.gz 24 2.835131256362e+00 PQG
CH.2Pir.DZ.pqgt1.dat-s.gz CH.2Pir.DZ.pqgt1.result.gz 24 2.835131256362e+00 PQGT1
CH.2Pir.DZ.pqgt1t2.dat-s.gz CH.2Pir.DZ.pqgt1t2.result.gz 24 2.835131256362e+00 PQGT1T2
CH.2Pir.DZ.pqgt1t2p.dat-s.gz CH.2Pir.DZ.pqgt1t2p.result.gz 24 2.835131256362e+00 PQGT1T2'
HF.1Sigma+.DZ.pqg.dat-s.gz HF.1Sigma+.DZ.pqg.result.gz 24 5.194757507570e+00 PQG
HF.1Sigma+.DZ.pqgt1.dat-s.gz HF.1Sigma+.DZ.pqgt1.result.gz 24 5.194757507570e+00 PQGT1
HF.1Sigma+.DZ.pqgt1t2.dat-s.gz HF.1Sigma+.DZ.pqgt1t2.result.gz 24 5.194757507570e+00 PQGT1T2
HF.1Sigma+.DZ.pqgt1t2p.dat-s.gz HF.1Sigma+.DZ.pqgt1t2p.result.gz 24 5.194757507570e+00 PQGT1T2'
F-.1S.DZ+d.pqg.dat-s.gz F-.1S.DZ+d.pqg.result.gz 26 0.0 PQG
F-.1S.DZ+d.pqgt1.dat-s.gz F-.1S.DZ+d.pqgt1.result.gz 26 0.0 PQGT1
F-.1S.DZ+d.pqgt1t2.dat-s.gz F-.1S.DZ+d.pqgt1t2.result.gz 26 0.0 PQGT1T2
F-.1S.DZ+d.pqgt1t2p.dat-s.gz F-.1S.DZ+d.pqgt1t2p.result.gz 26 0.0 PQGT1T2'
H2O.1A1.DZ.pqg.dat-s.gz H2O.1A1.DZ.pqg.result.gz 28 9.188690490978e+00 PQG
H2O.1A1.DZ.pqgt1.dat-s.gz H2O.1A1.DZ.pqgt1.result.gz 28 9.188690490978e+00 PQGT1
H2O.1A1.DZ.pqgt1t2.dat-s.gz H2O.1A1.DZ.pqgt1t2.result.gz 28 9.188690490978e+00 PQGT1T2
H2O.1A1.DZ.pqgt1t2p.dat-s.gz H2O.1A1.DZ.pqgt1t2p.result.gz 28 9.188690490978e+00 PQGT1T2'

1D Hubbard model with high correlation limits

From [1]. Note not all results have been uploaded, and may not all problems are solved in the referenced paper. You may need multiple precision version of SDP solver like SDPA-GMP, SDPA-QD, or SDPA-DD.

Problems (dat-s, gzip'ed) result (gzip'ed) rank U/t comment
hubbard_X4N4p.1000.0.pqg.dat-s.gz hubbard_X4N4p.1000.0.pqg.result.gz 8 1000.0 PQG
hubbard_X4N4p.1000.0.pqgt1.dat-s.gz hubbard_X4N4p.1000.0.pqgt1.result.gz 8 1000.0 PQGT1
hubbard_X4N4p.1000.0.pqgt1t2.dat-s.gz hubbard_X4N4p.1000.0.pqgt1t2.result.gz 8 1000.0 PQGT1T2
hubbard_X4N4p.1000.0.pqgt1t2p.dat-s.gz hubbard_X4N4p.1000.0.pqgt1t2p.result.gz 8 1000.0 PQGT1T2'
hubbard_X4N4p.10000.0.pqg.dat-s.gz hubbard_X4N4p.10000.0.pqg.result.gz 8 10000.0 PQG
hubbard_X4N4p.10000.0.pqgt1.dat-s.gz hubbard_X4N4p.10000.0.pqgt1.result.gz 8 10000.0 PQGT1
hubbard_X4N4p.10000.0.pqgt1t2.dat-s.gz hubbard_X4N4p.10000.0.pqgt1t2.result.gz 8 10000.0 PQGT1T2
hubbard_X4N4p.10000.0.pqgt1t2p.dat-s.gz hubbard_X4N4p.10000.0.pqgt1t2p.result.gz 8 10000.0 PQGT1T2'
hubbard_X4N4p.100000.0.pqg.dat-s.gz hubbard_X4N4p.100000.0.pqg.result.gz 8 100000.0 PQG
hubbard_X4N4p.100000.0.pqgt1.dat-s.gz hubbard_X4N4p.100000.0.pqgt1.result.gz 8 100000.0 PQGT1
hubbard_X4N4p.100000.0.pqgt1t2.dat-s.gz hubbard_X4N4p.100000.0.pqgt1t2.result.gz 8 100000.0 PQGT1T2
hubbard_X4N4p.100000.0.pqgt1t2p.dat-s.gz hubbard_X4N4p.100000.0.pqgt1t2p.result.gz 8 100000.0 PQGT1T2'
hubbard_X6N6p.1000.0.pqg.dat-s.gz hubbard_X6N6p.1000.0.pqg.result.gz 12 1000.0 PQG
hubbard_X6N6p.1000.0.pqgt1.dat-s.gz hubbard_X6N6p.1000.0.pqgt1.result.gz 12 1000.0 PQGT1
hubbard_X6N6p.1000.0.pqgt1t2.dat-s.gz hubbard_X6N6p.1000.0.pqgt1t2.result.gz 12 1000.0 PQGT1T2
hubbard_X6N6p.1000.0.pqgt1t2p.dat-s.gz hubbard_X6N6p.1000.0.pqgt1t2p.result.gz 12 1000.0 PQGT1T2'
hubbard_X6N6p.10000.0.pqg.dat-s.gz hubbard_X6N6p.10000.0.pqg.result.gz 12 10000.0 PQG
hubbard_X6N6p.10000.0.pqgt1.dat-s.gz hubbard_X6N6p.10000.0.pqgt1.result.gz 12 10000.0 PQGT1
hubbard_X6N6p.10000.0.pqgt1t2.dat-s.gz hubbard_X6N6p.10000.0.pqgt1t2.result.gz 12 10000.0 PQGT1T2
hubbard_X6N6p.10000.0.pqgt1t2p.dat-s.gz hubbard_X6N6p.10000.0.pqgt1t2p.result.gz 12 10000.0 PQGT1T2'
hubbard_X6N6p.100000.0.pqg.dat-s.gz hubbard_X6N6p.100000.0.pqg.result.gz 12 100000.0 PQG
hubbard_X6N6p.100000.0.pqgt1.dat-s.gz hubbard_X6N6p.100000.0.pqgt1.result.gz 12 100000.0 PQGT1
hubbard_X6N6p.100000.0.pqgt1t2.dat-s.gz hubbard_X6N6p.100000.0.pqgt1t2.result.gz 12 100000.0 PQGT1T2
hubbard_X6N6p.100000.0.pqgt1t2p.dat-s.gz hubbard_X6N6p.100000.0.pqgt1t2p.result.gz 12 100000.0 PQGT1T2'
hubbard_X8N8p.1000.0.pqg.dat-s.gz hubbard_X8N8p.1000.0.pqg.result.gz 16 1000.0 PQG
hubbard_X8N8p.1000.0.pqgt1.dat-s.gz hubbard_X8N8p.1000.0.pqgt1.result.gz 16 1000.0 PQGT1
hubbard_X8N8p.1000.0.pqgt1t2.dat-s.gz hubbard_X8N8p.1000.0.pqgt1t2.result.gz 16 1000.0 PQGT1T2
hubbard_X8N8p.1000.0.pqgt1t2p.dat-s.gz hubbard_X8N8p.1000.0.pqgt1t2p.result.gz 16 1000.0 PQGT1T2'
hubbard_X8N8p.10000.0.pqg.dat-s.gz hubbard_X8N8p.10000.0.pqg.result.gz 16 10000.0 PQG
hubbard_X8N8p.10000.0.pqgt1.dat-s.gz hubbard_X8N8p.10000.0.pqgt1.result.gz 16 10000.0 PQGT1
hubbard_X8N8p.10000.0.pqgt1t2.dat-s.gz hubbard_X8N8p.10000.0.pqgt1t2.result.gz 16 10000.0 PQGT1T2
hubbard_X8N8p.10000.0.pqgt1t2p.dat-s.gz hubbard_X8N8p.10000.0.pqgt1t2p.result.gz 16 10000.0 PQGT1T2'
hubbard_X8N8p.100000.0.pqg.dat-s.gz hubbard_X8N8p.100000.0.pqg.result.gz 16 100000.0 PQG
hubbard_X8N8p.100000.0.pqgt1.dat-s.gz hubbard_X8N8p.100000.0.pqgt1.result.gz 16 100000.0 PQGT1
hubbard_X8N8p.100000.0.pqgt1t2.dat-s.gz hubbard_X8N8p.100000.0.pqgt1t2.result.gz 16 100000.0 PQGT1T2
hubbard_X8N8p.100000.0.pqgt1t2p.dat-s.gz hubbard_X8N8p.100000.0.pqgt1t2p.result.gz 16 100000.0 PQGT1T2'