Calculation Logs

= Calculation Log =

NOTE: Figures and data are basically stored in Dropbox.

PPN
- 10/9-10/2019: Calculated overproduction factor (abundance ratio to the case with the Kappeler 1994 rate) as per request of Greg and Grisha. 5 solar mass with solar system metallicity (asplund). Trajectory.inpu was obtained from star.log. See 191010. The results do not agree much with Heshani's NEWTON calculations. But I checked trajectories, etc, carefully, so my calculations should be ok.

- 10/12: Since I found the calculations above are not right (used Z=0.01 Asplund 2005 abundance), I recalculated with Z=0.02 abundance files (GN93). The results still don't match with Heshani's calculations, but they changed quite a bit from Z=0.01 ones.

- 10/13: Run XRB examples.Learned many heavy p-rich nuclei are actually produced by successive (p,g) on stable heavy nuclei (not simply started from light stable nuclei).

MPPNP
- 10/10-14/2019 (GCA): Calculated 5M Z=0.02 from the Canfar hdf5 data. 22Ne(a,n/g) rates are (probably) set to Kappeler1994??. Because PPN results didn't agree with Talwar or Heshani either, so I just hoped MPPNP might improve the disagreement.

- 10/17/2019 - (WENDI) : Calculated 5M Z=0.02 from the Canfar hdf5 data. 22Ne(a,n/g) rates are set to Longland2012.

- 10/17/2019 - (GCA) : Calculated 5M Z=0.02 from the Canfar hdf5 data. 22Ne(a,n/g) rates are set to Talwar2016.

MESA
- 6/23/2019: Calculated neutron abundance in 25 solar mass stars. See 190623

- 10/9/: Calculated 5 solar mass AGB (based on 7M_prems_to_AGB). Checked HR diagram and T-rho curves, etc. Confirmed the T-rho trajectory agrees very well with Canfar data's trajectory.

- 10/11: Calculated nova and 25M_pre_ms_to_core_collapse from test_suite on WENDI (just for curiosity). Nova trajectory seems very different from XRB trajectory on PPN examples. Also, 25M trajectory is not similar to 25M_ccsn on PPN examples (but this is probably PPN shows C or He burning's trajectory).

- 10/12: Calculated C13_pocket and He_core_flash from test_suite on WENDI (for curiosity).