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--- data:models0 [2022/03/08 11:44] – jcsuarez
+++ data:models0 [2022/12/22 14:33] (current) – external edit 127.0.0.1
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+======= Models (exercise #0) ========
+The table below organises the data used in each exercise. Data consists in packages compresses with .tar.gz or zip, which can be downloaded by clicking on the provided links.
+===== Data ======
+^Package ^Date ^Author ^Description   ^Format ^Download |
+^wp121130_ex0-smodels|21/01/2019 | A. Serenelli | stellar interior models| gong, amdl | ([[https://drive.google.com/file/d/1wt9k343_fRFg29rr5EGGQ8ieAzxbIpdt/view?usp=sharing| ex0-smodels.tar.gz]]) |
+^wp121130_ex0-omodels|21/01/2019 | ALL | oscillations|  - |([[https://drive.google.com/file/d/1J_y6wFwFVbOtDKN33g49Us-BNCEV5yEd/view?usp=sharing | ex0-frequencies.tar.gz]]) |
+===== Global properties ======
+^Model ^Mass ^[Fe/H] ^alpha  ^ovsh  ^Nshell ^Phase ^Notes|
+|0-001 |1.04     | +0.05 | 1.6   | 0.00  |3000    | MS  | Representative of 16Cyg ~7Gyr (Travis et al. 2015)|
+|0-002 |1.04     | +0.05 | 1.6   | 0.00  |4000    | SG  | -|
+|0-003 |1.50     | +0.00 | 1.6   | 0.00  |3000    | MS  | Small convective core (around 8% of the stellar mass)|
+|0-004 |1.50     | +0.00 | 1.6   | 0.00  |4000    | TAMS| -|
+|0-005 |1.50     | +0.00 | 1.6   | 0.00  |4000    | SG  | -|
+===== Physics ======
+^Code | Garstec (A- Wess rev., 2015)|||||
+^Convection| MLT, alpha = 1.801|||||
+^Overshoot | diffusion equation with exponential decay (Herwig type), including geometric limit applied to small convective cores (H_p towards the center makes overshoot regions too large). Proportion factor f = 0.02 (equivalent to  0.2 - 0.25 Hp in tradicional formulation) |||||
+^Extra mixing | Under the convective envelope (Vandenberg et al. 2012) as a function of its mass. Free parameters calibration forced to reproduce the solar Li and chemical abundances observed in globular clusters (e.g. Korn et al. en NGC 6397).|||||
+^gradT | Temperature gradient in overshoot regions is radiative.|||||
+^Wind | 1e-13 Msun / yr to avoid depletion of He and metals (included in extra missing calibration) |||||
+^Atmosphere | Eddington T-tau |||||
+^Nuclear rates | Adelberger et al. 2011, which includes de "low" value of LUNA's N14+p |||||
+^Screening | Weak (Salpeter)/intermediate (Graboske et al. 1973, subgiants) |||||
+^EOS |FreeEOS de Irwin |||||
+^Opacities | OPAL + Ferguson 2005 for low temperatures |||||
+^mDiffusion | For all chemical elements |||||
+^rLevitation | No |||||
+^Relevant constants||||||
+^G | 6.67232e-8 (c.g.s.) |||||