Dear VASP community,
I've done a set of GW calculations on a 2D material using VASP 5.4.4 with HSE as the starting point. For the smallest system, INCAR includes the following keys:
NBANDS = 1120
NELM = 1
ALGO = GW0
NOMEGA = 100
LASPH = .TRUE.
LSPECTRAL = .TRUE.
LWANNIER90 = True
With a 6x6x1 KPOINTS and POTCAR includes PAW_PBE *_sv_GW
I could safely accomplish this calculation and the following GW band plots using wannier and solving BSE. For a postprocessing analysis, I am interested in extracting the static, macroscopic screened Coulomb interaction, W(r, ω→0), or at least W(G=G′=0, ω=0). My attempts to read WFULL0001.tmp using Python and Fortran fail due to either memory or I/O errors.
Since I already have WAVEDER, WAVECAR.chi, CHGCAR and WAVECAR file from this GW+LOPTICS run, my question is:
What is the recommended workflow in VASP 5.4.4 to obtain macroscopic W(ω=0) safely for large systems?
Is there a way to extract only W(G=G′=0, ω=0) without reading the entire WFULL files?
Are there existing post-processing tools or scripts compatible with VASP 5.4.4 for this purpose?
Any guidance, example scripts, post-processing tools, or pointers compatible with VASP 5.4.4 would be highly appreciated.
Thank you very much for your help.
Best regards,
Masoud

