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Reincorporated velocity drag into energy and momentum equations, and added controls to toggle
Added a new test suite make_pre_ccsn_13BVN for testing velocity drag, for v_flag (#535)
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Co-authored-by: Rob Farmer <[email protected]>
Co-authored-by: EbF <[email protected]>
Co-authored-by: Evan Bauer <[email protected]>
Co-authored-by: Ebraheem Farag <[email protected]>
This test suite evolves a solar metalicity 12 |MSun| model from the pre-ms to helium depletion, strips the hydrogen envelope, and then evolves to core collapse.
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This test suite is made to be similar (almost identical) to the 13BVN model from MESA IV. (This is a sensitive test_suite)
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Physical checks
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===============
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Tests the functionality of velocity drag for v_flag for damping large surfaces velocities from He shell (N-alpha) flashes during advanced burning.
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Tests energy conservation for regions where v_drag is applied.
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Tests the use of OP_split_burn as split burn <4d9 leads to large temperature swings and single zone burning in the core, and split burn >4.5d9 needs smaller timesteps.
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This case illustrates strong coupling between burning and hydro: OP_split_burn lower and higher thresholds can only be exceeded with very tight timesteps.
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Inlists
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=======
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This test case has five parts.
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* Part 1 (``inlist_to_zams``) creates a 12 |Msun|, Z=2*10^-2 metallicity, pre-main sequence model and evolves it the zero age main sequence.
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* Part 2 (``inlist_before_remove``) takes the model to core helium depletion.
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* Part 3 (``inlist_remove``) removes the hydrogen envelope, leaving a stripped, evolved helium core.
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* Part 4 (``inlist_after_remove``) replaces the remaining hydrogen in the envelope with helium.
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* Part 5 (``inlist_to_pre_si_burn``) evolves the model until log_center_T = 9.45d0, just before Si-core burning.
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* Part 6 (``inlist_to_cc``) evolves the model until core collapse (300 km/s infall).
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