General-order open-shell coupled-cluster method with partial-spin adaptation II: further formulations, simplifications, implementations, and numerical results
Cong Wang

TL;DR
This paper extends the general-order open-shell coupled-cluster method with partial-spin adaptation by introducing new formulations, simplifications, and implementation details, along with numerical results demonstrating its effectiveness.
Contribution
It provides further formulations, simplifications, and implementation strategies for the partial-spin adapted coupled-cluster method, along with numerical validation.
Findings
Enhanced formulations and simplifications for the PSA-CC method
Implementation strategies including hash-table canonicalizations
Numerical results demonstrating method performance
Abstract
This is a continuation of the previous work (arXiv:2403.10128). Additional aspects such as linear combinations of projections and hash-table canonicalizations are described. Implementations of the general-order partial-spin adaptation (PSA) coupled-cluster (CC) method are outlined. Numerical results are reported.
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Taxonomy
TopicsSolar and Space Plasma Dynamics
