Diffusion timescales for DBAZ white dwarfs with DBAZ atmosphere models as boundary condition (D. Koester 2020) ------------------------------------------------------------------- The atmosphere models, which provide the boundary conditions for the envelopes, use the latest code with a number of improvements (e.g. a more accurate treatment of molecule formation, more absorption processes), which are most important at the cool end of the sequence. The envelope code is a completely new development, described in more detail in Koester et al. (2020, A&A 635,103). The diffusion code has been completely rewritten. Major changes are the inclusion of nonideal effects in the diffusion equation after Beznogov & Yakovlev (2013, Phys. Rev. E, 111, 161101), new calculations for the collision integrals by Stanton & Murillo (2016, Phys.Rev. E, 93, 043203), and the Thomas-Fermi mean ionization model for the determination of average charges of all elements at higher densities. In the current version the average charges are calculated from the Saha equation (including nonideal effects) for log density < -3.0 and from the TF model for log densities >-2.0 g/cm3. In the intermediate region a smooth transition is provided. The DBAZ calculations use ML2/alpha=0.8 for the convection in atmosphere and envelope. The hydrogen abundance is [H/He] = -4.50 (log number abundances). The atmosphere models include the 15 most important elements (Z = 1,2,6,7,8,10,11,12,13,14,15,16,20,26,28) consistently with Bulk Earth composition relative to Ca, which is used as metallicity parameter. The envelope models include only H and He, since the trace elements have no influence on the structure. However, the sinking time scales are calculated for 30 elements at the border of the convection zone (optionally including 1 Hp overshoot). Structure of tables: OV0 = no overshoot, OV1 one Hp overshoot DBAZ_difftable825_OV1: log g = 8.25, 1 Hp overshoot first line: Teff, log g, overshoot second line: metallicity parameter [Ca/He] from -7 to -15 third line: fractional mass log q of the convection zone remaining lines: log taudiff for elements Z=3 to 30.