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Meeting ID: 658 8106 3662
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Sushanta:
- Native source size distribution is similar in scaling to EPOS (increasing size with mT) but the size is much bigger
- After modelling the mT scaling looks good, baring the last bin which seems a little too high
- First look at Deuterons with Gaussian wave function: ~2x higher than data (~4x higher than EPOS)
- Will look through code with Maxi to find possible bugs
- Next step: add Hulthen (and eventually Argonne)
Maxi:
- still working on Argonne wave function fit
- Wigner function finally calculated
- Next step: calculate probability and add into coalescence afterburner
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