History Graph
History Graph
Commit | Author | Details | Committed | |||
---|---|---|---|---|---|---|
1c0fbaf83a18 | revaz | GEAR: PyGear : we add the possibility in star_mass_from_age to correctely treat… | Jan 12 2017 | |||
b9a4fa236396 | revaz | PyChem : add the possibility to change the lifetime of stars. We now need… | Jan 12 2017 | |||
0a708f540a6f | revaz | GEAR: in chimie.c, if Cp->SNIa_Mpl < Cp->ms[Cp->n-1] or Cp->SNIa_Mpu < Cp->ms… | Dec 22 2016 | |||
4b9bf9049125 | revaz | GEAR: in kickback, remove the term corresponding to the PMGRID. In think this… | Dec 9 2016 | |||
d4467dbb7568 | revaz | FOF: now the star formation proceeds only if the group is under-virialized. in… | Nov 7 2016 | |||
c296c69f2272 | revaz | correct EgySpec in chimie_apply_thermal_feedback() | May 30 2016 | |||
37098855f4a8 | revaz | GEAR: chimie, a tiny bug corrected | Aug 21 2015 | |||
06341a4bd7bb | revaz | GEAR: add a new flag : CHIMIE_TIMEBET. It allows to performe the chemistry… | Aug 20 2015 | |||
dfd738c8ff58 | revaz | GEAR: some tiny corrections... | Jun 30 2015 | |||
c5b2bb3552ca | revaz | GEAR : CHIMIE_STATS, add the header for the SNs files | Feb 5 2015 | |||
46a53b3050c1 | revaz | GEAR: add a new flag CHIMIE_STATS, that allow to create txt files used to trace… | Feb 5 2015 | |||
4e325d0d8c28 | revaz | GEAR: CHIMIE_EJECTA_RADIUS == 2 , bug in the paralleisme is not corrected | Jan 8 2015 | |||
3eeb8b3a0607 | revaz | GEAR: CHIMIE_EJECTA_RADIUS == 2 works now. The ejecta radius is computed using… | Jan 6 2015 | |||
02d2bbfe24a3 | revaz | GEAR: add a new flag : CHIMIE_EJECTA_RADIUS that allows to fix the radius of… | Jan 6 2015 | |||
3b3281ba44bb | revaz | GEAR : CHIMIE : a new flag DCHIMIE_ELTS_WEIGHTING is added, which allows to… | Dec 29 2014 | |||
a136c2e88a2a | revaz | GEAR : CHIMIE_ONE_SN_ONLY : now, we must set the mass of the exploding SNIa. +… | Dec 29 2014 | |||
524ed04f6325 | revaz | PyChem : change return Py_BuildValue("O",myarray); to return PyArray_Return… | Nov 17 2014 | |||
292142f49670 | revaz | GEAR: correct a bug where for small stellar mass particles, the mass could go… | Sep 8 2014 | |||
1b7d64db28d6 | revaz | GEAR: add a new flag CHIMIE_AGB that allow to enable AGB (DYIN) stars in chimie. | Jun 26 2014 | |||
e9f8ecbdbffc | revaz | GEAR: FOF,FOF_SFR We discretize again fully the NSNIa value. Instead, NSNIa is… | May 21 2014 | |||
d924ce258f46 | revaz | GEAR: FOF,FOF_SFR for a portion of imf, the number of SN is the floor of the… | May 17 2014 | |||
2db018baf590 | revaz | aesthetic : add some spaces in chimie.c | May 16 2014 | |||
253dcbe7be08 | revaz | GEAR: FOF, FOF_SFR add Cp->MassMinForEjecta to stop the loop over discrete… | May 16 2014 | |||
d524ad073023 | revaz | GEAR : FOF, FOF_SFR take correctly the normalisation factor k, for each stellar… | May 15 2014 | |||
4d85d68c752e | revaz | GEAR : FOF, FOF_SFR correct the way a particle find its next mass… | May 15 2014 | |||
e9f208c9e84e | revaz | GEAR : FOF, FOF_SFR - the chemistry should now be done properly if the imf… | May 15 2014 | |||
2015550f99af | revaz | GEAR : add new conversion factor Code Mass Unit -> Solar Mass FOF_SFR : SNII… | May 2 2014 | |||
01edfb196b3c | revaz | GEAR : some cleaning in chimie.c | Apr 17 2014 | |||
894e1b811266 | revaz | GEAR : fof : add the new routine fof_star_formation_and_IMF_sampling and many… | Apr 17 2014 | |||
a4b2662bcf36 | revaz | GEAR: now works with the Optimal IMF Sampling implementation | Apr 4 2014 | |||
d54a87228d1e | revaz | GEAR, PyChem : add a new flag CHIMIE_OPTIMAL_SAMPLING This flag allows to use… | Apr 3 2014 | |||
fa2874de676c | revaz | in chimie.c, tiny correction conserning CHIMIE_ONE_SN_ONLY | Nov 19 2013 | |||
fc91e6acefa6 | revaz | add METAL_DIFFUSION, following the work of Alexis Arnaudon Simple tests have… | Nov 19 2013 | |||
f7405a23b244 | revaz | GEAR : The new flag CHIMIE_SMOOTH_METALS is introduced. The variable .Metals… | Jul 9 2013 | |||
f7e36798d4e7 | revaz | PyChem : we changed the chemistry table format to hdf5. AGB are included as… | Jul 9 2013 | |||
759ab396c8f5 | revaz | Add the possibility to use Wiersma type cooling/heating tables (COOLING_WIERSMA) | May 13 2013 | |||
1c6d5517bffc | revaz | A lot of changes: | May 10 2013 | |||
d561c359730c | revaz | add the starformation receipe 3 (following Hopkins 2013) | Mar 22 2013 | |||
89de58c240c5 | revaz | Two small modification in chimie.c and cooling.c | Jan 17 2013 | |||
68acf5d1271a | revaz | We have now fixed the problem of energy related to the use of the new flags… | Nov 30 2012 | |||
13557606a6f2 | revaz | only some printf removed. | Nov 9 2012 | |||
b3a44a0e17d6 | revaz | Improved conservation of energy in case of feedback. | Nov 6 2012 | |||
004c5dbbd4ad | revaz | We add the new flag SYNCHRONIZE_NGB_TIMESTEP that allows ngb particles to… | Oct 19 2012 | |||
f46b592fd8ff | revaz | DYIN stars are now correctely take into account in chimie.c | Jul 26 2012 | |||
73ca2cd44116 | revaz | The code can now start if we give stellar particles. | Jul 20 2012 | |||
49082be97808 | revaz | move all files into the new src directory | Mar 28 2012 |
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