Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
recent_changes [2024/01/28 19:33] – [New features of MOLPRO2024.1] werner | recent_changes [2024/02/08 13:18] (current) – 2.x.x becomes 2.3.0 doll | ||
---|---|---|---|
Line 7: | Line 7: | ||
===== New features of MOLPRO2024.1 ===== | ===== New features of MOLPRO2024.1 ===== | ||
- | Various bug fixes | + | Various bug fixes and improvements of existing methods. |
- | ==== iMolpro | + | ==== iMolpro |
- | A new graphical user interface called '' | + | A new graphical user interface called '' |
- | ==== D4 dispersion correction | + | ==== D4 dispersion correction |
- | Unfortunately | + | Unfortunately |
- | ==== DFT funktional | + | |
+ | |||
+ | ==== DFT functional | ||
Many alias names for functionals computed with libxc have been added. These are compatible with those used in the D4 program. | Many alias names for functionals computed with libxc have been added. These are compatible with those used in the D4 program. | ||
+ | ==== Density-based basis set correction ==== | ||
+ | |||
+ | This program has been very much speeded up, with and without density fitting. Various functionals can now be used in it. | ||
+ | |||
+ | |||
+ | ==== Internally Contracted Multireference Coupled-Cluster Theory ==== | ||
+ | |||
+ | A CAS(2,2) version of icMRCCSD is now available, as published in [[https:// | ||
+ | ==== PNO-LMP2-F12 / PNO-LCCSD(T)-F12 ==== | ||
+ | |||
+ | New variables EMP2F12_PNO and EMP2F12_OSV are set for MP2-F12 energies computed with PNO or PAO/OSV projector, respectively. This happens in calculations with option projector=PAO or projector=MIXED. | ||
+ | |||
+ | ==== Nuclear-electronic orbital (NEO) methods ==== | ||
+ | |||
+ | A new automated procedure for the optimisation of quantum nuclei positions has been introduced (adaptive-NEO). The latter works by updating the nuclei position (meaning the nuclear basis centers, together with the respective electronic basis functions) to the nuclear orbital centroids during the SCF cycles. See [[nuclear-electronic_orbital_method# | ||
+ | |||
+ | ==== Basis set short names ==== | ||
+ | |||
+ | The short names [awc]vnz-dk (n=d,t,q,5) now refer to the [aug]-cc-p[wC]V(n+d)Z-DK sets for second-row elements Al-Cl. To avoid using the +d sets (not recommended!) use the full basis set name. | ||
+ | ===== GUI gmolpro 2.3.0 ===== | ||
+ | Version 2.3.0 is bundled with Molpro 2024.1 . | ||
+ | |||
+ | There is now a switch " | ||
+ | in the builder and viewer window to deal with those Mac's which have retina screens. | ||
+ | It switches from a normal display (retina factor 1) | ||
+ | to a display with doubled number of pixels in both directions (retina factor 2). | ||
+ | When this factor is changed, then it gets auto-saved in a configuration file $HOME/ | ||
+ | If necessary, this configuration file can be edited and retina factors different from 1 or 2 may be used. | ||
+ | LIBGL_ALWAYS_SOFTWARE is set to be true. This avoids a crash on some Linux distributions, | ||
+ | in the Mesa library. | ||
- | |||
===== New features of MOLPRO2023.1 ===== | ===== New features of MOLPRO2023.1 ===== |