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Copy file name to clipboardExpand all lines: online-docs/pages/whats-new.rst
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Following is a brief list of important updates to the COMPAS code. A complete record of changes can be found in the file ``changelog.h``.
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**03.20.03 June 18, 2025**
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* Resolved an issue that appeared in 03.10.02 with some TPAGB stars in the ECSN range (but not satisfying ECSN conditions) exploding as core-collapse supernovae
Copy file name to clipboardExpand all lines: src/changelog.h
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// - Update white dwarf mass-radius relation (WhiteDwarfs::CalculateRadiusOnPhase_Static)
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// - Moved white dwarf related constants to constants.h (resolves issue #1351)
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// - Set merger on unstable RLOF from WD
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// 03.20.02 IM - May 30, 2026 - Defect repair, enhancement:
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// 03.20.02 IM - May 30, 2025 - Defect repair, enhancement:
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// - Included unit conversion in WhiteDwarfs::CalculateEtaPTY()
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// - All critical mass ratios now return the HURLEY_HJELLMING_WEBBINK_QCRIT_WD for white dwarfs and 0 for other remnant donors (only stable mass transfer) as fix for issue #1385
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// 03.20.03 IM - June 18, 2026 - Defect repair, enhancement:
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// 03.20.03 IM - June 18, 2025 - Defect repair, enhancement:
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// - TPAGB stars should no longer experience supernovae if SN conditions are not satisfied, rather than defaulting to CCSN (corrects the partial fix in 03.10.02)
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// - Added new parameter (threshold mass, generally expected to be MCH or MECS) to CalculateCoreMassAtSupernova_Static()
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// - Removed McSN from GBParams, instead computed on the fly when needed
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