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### Connections to Littlewood’s Conjecture  We show the energy radiated in the convective region to be proportional  to the mass in the radiative layer between the stellar surface and the  upper boundary of the convective zone, as shown in the following table and in Figure \ref{fig:fig1}:  |**Phase** | **Time** | **M\(_ 1\)** | **M\(_ 2\)** | **\(\Delta M\)** | **P** | **\(v_{\rm rot,1}\)** | **\(v_{\rm rot,2}\)** |   |:------------------|:----------|-------------|-------------|----------------|-------|---------------------|---------------------|  |1 ZAMS | 0 | 16 | 15 | – | 5.0 | 230 | 230 |   |2 Case B | 9.89 | 15.92 | 14.94 | 0.14 | 5.1 | 96 | 85 |   |3 ECCB | 11.30 | 3.71 | 20.86 | 6.44 | 42.7 | 40 | 767 |   |4 ECHB | 18.10 | – | 16.76 | – | – | – | 202 |   |5 ICB | 18.56 | – | 12.85 | – | – | – | 191 |   |6 ECCB | 18.56 | – | 12.83 | – | – | – | 258 |