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2022
DOI: 10.1021/acs.jpca.2c05952
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Toward Large-Scale Restricted Active Space Calculations Inspired by the Schmidt Decomposition

Abstract: We present an alternative, memory-efficient, Schmidt decomposition-based description of the inherently bipartite restricted active space (RAS) scheme, which can be implemented effortlessly within the density matrix renormalization group (DMRG) method via the dynamically extended active space procedure. Benchmark calculations are compared against state-of-the-art results of C2 and Cr2, which are notorious for their multireference character. Our results for ground and excited states together with spectroscopic c… Show more

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Cited by 6 publications
(9 citation statements)
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“…Next, using the predicted full-CI energy, E RAS-X = −2086.891, we show in Figure 7c that the linear scaling on double logarithmic axes for different values is recovered, as expected. Comparing our result to multireference configuration interaction (MRCI), coupled cluster singles, doubles, and perturbative triples (CCSD(T)), coupled cluster singles, doubles and triples (CCSDT), and coupled cluster singles, doubles, triples and quadruples (CCSDTQ) 27 (E = −2086.7401, −2086.8785, −2086.8675, −2086.8689, respectively), we conclude that our data point E 0 (17, 2) = −2086.8769 is already below the CCSDTQ by 8 × 10 −3 . The extrapolated energy is E RAS-X = 2086.891 (p RAS-X = 1.88) using all 14 data points in the figure.…”
Section: Results For Large Basis Sets and The Stability Of The Dmrg-r...mentioning
confidence: 88%
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“…Next, using the predicted full-CI energy, E RAS-X = −2086.891, we show in Figure 7c that the linear scaling on double logarithmic axes for different values is recovered, as expected. Comparing our result to multireference configuration interaction (MRCI), coupled cluster singles, doubles, and perturbative triples (CCSD(T)), coupled cluster singles, doubles and triples (CCSDT), and coupled cluster singles, doubles, triples and quadruples (CCSDTQ) 27 (E = −2086.7401, −2086.8785, −2086.8675, −2086.8689, respectively), we conclude that our data point E 0 (17, 2) = −2086.8769 is already below the CCSDTQ by 8 × 10 −3 . The extrapolated energy is E RAS-X = 2086.891 (p RAS-X = 1.88) using all 14 data points in the figure.…”
Section: Results For Large Basis Sets and The Stability Of The Dmrg-r...mentioning
confidence: 88%
“…We remark here that the -dependence hinges on a good choice of the CAS space and on the chosen basis. 27,62 Since the orbitals lying close to the Fermi surface possess the largest one-orbital entropies, 25 a selection based on orbital entropy together with keeping the almost fully occupied orbitals in the CAS space is an efficient protocol. 25,46,63 Let us also note that a very accurate extrapolation procedure requires to perform CAS and DMRG-RAS calculations for various χ values for each in order to perform an extrapolation to the DMRG truncation-free limit, i.e, to obtain = E ( lim E ( )…”
Section: Numerical Resultsmentioning
confidence: 99%
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