output
19952025
most citedRecent developments in the PySCF program package

1.2k citations

42 papers

physics.chem-ph2025★ 8 cited

MC-PDFT Nuclear Gradients and L-PDFT Energies with Meta and Hybrid Meta On-Top Functionals for Ground- and Excited-State Geometry Optimization and Vertical Excitation Energies

Matthew R. Hennefarth, Younghwan Kim, Bhavnesh Jangid +4

Multiconfiguration pair-density functional theory (MC-PDFT) is a post-MCSCF multireference electronic-structure method that explicitly models strong electron correlation, and linea…

physics.chem-ph2020★ 69 cited

The Variational Localized Active Space Self-Consistent Field Method

Matthew R. Hermes, Laura Gagliardi

Fragmentation methods applied to multireference wave functions constitute a road towards the application of highly accurate ab initio wave function calculations to large molecules…

physics.chem-ph2020★ 53 cited

Multi-State Pair-Density Functional Theory

Jie J. Bao, Chen Zhou, Zoltan Varga +3

Multiconfiguration pair-density functional theory (MC-PFDT) has previously been applied successfully to carry out ground-state and excited-state calculations. However, because it i…

physics.chem-ph2020★ 1.2k cited

Recent developments in the PySCF program package

Qiming Sun, Xing Zhang, Samragni Banerjee +46

PYSCF is a Python-based general-purpose electronic structure platform that both supports first-principles simulations of molecules and solids, as well as accelerates the developmen…

physics.comp-ph2018★ 6 cited

WENO-Wombat: Scalable Fifth-Order Constrained-Transport Magnetohydrodynamics for Astrophysical Applications

J. M. F. Donnert, H. Jang, P. Mendygral +3

Due to increase in computing power, high-order Eulerian schemes will likely become instrumental for the simulations of turbulence and magnetic field amplification in astrophysical…

astro-ph.GA2018★ 10 cited

A 1D fluid model of the Centaurus A jet

Sarka Wykes, Bradford T. Snios, Paul E. J. Nulsen +11

We implement a steady, one-dimensional flow model for the X-ray jet of Centaurus A in which entrainment of stellar mass loss is the primary cause of dissipation. Using over 260 ks…