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TODO.md

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This file contains known bugs and a list of features and additions that may make the program better and/or more usable.

Additions are encouraged, you can either contact the author or implement the change and send a pull request via github

Known Bugs

  • The 2012 and 2016 nubase files added isospin, but in a way that can overlap with the spin parity values and the error on half-life. Two examples are:
007 0048   7Bei    26750       30     10980      30     RQ                     3/2-    T=3/2 03               p ?;3He ?;A ?
007 0050   7B      27677       25                            570     ys 140    (3/2-)        03 11Ch32t  1967 p=100
008 0020   8He     31609.68     0.09                         119.1   ms 1.2    0+            05          1965 B-=100;B-n=16 1;B-t=0.9 1
008 0030   8Li     20945.80     0.05                         839.40  ms 0.36   2+            05 10Fl01t  1935 B-=100;B-A=100
008 0038   8Lii    31768        5     10822       5     RQ                     0+      T=2   05
008 0040   8Be      4941.67     0.04                          81.9   as 3.7    0+            05          1932 A=100
008 0048W  8Bei    21568        3     16626       3                            2+  frg T=1      04Ti06e  2004 A~100

and

011 0050   11B      8667.9      0.4                          stbl              3/2-          12          1920 IS=80.1 7
011 0058   11Bxi   21228        9     12560       9     RQ              T=3/2  1/2+,(3/2+)   12          1963
011 0060   11C     10650.3      0.9                           20.364  m 0.014  3/2-          12          1934 B+=100
011 0068   11Cxi   22810       40     12160      40     RQ                     1/2+    T=3/2 12 71Wa21d  1971 p=?

There are isospin values for 195/5511 in 2012 and 205/5625 in 2016. Currently I'm inclined to simply remove them from the line rather than extract all of the necessary situations in order to correctly parse.

Things that need to be looked at (Not quite bugs)

  • The population of the member Nuclide::jpi needs to be looked at in relation to isotopes that have many different values/possibilities

Possible improvements/alterations (in no particular order)

  • Use useful exit values if we quit out before completion, e.g. 10=no mass table 11=bad input file, etc...