| 31. | These baryons in principle have lots of decay modes available, and the ones that are observed experimentally aren't necessarily the most common.
|
| 32. | The primary decay mode before the most abundant isotope, 102 Ru, is electron capture and the primary mode after is beta emission.
|
| 33. | The primary decay mode before the most abundant stable isotope, 166 Er, is electron capture, and the primary mode after is beta decay.
|
| 34. | The primary decay mode before the most abundant stable isotope, 174 Yb is electron capture, and the primary mode after is beta emission.
|
| 35. | The primary decay mode before the most abundant stable isotope, 106 Pd, is electron capture and the primary mode after is beta decay.
|
| 36. | The primary decay mode before the most abundant stable isotope, 107 Ag, is electron capture and the primary mode after is beta decay.
|
| 37. | The primary decay mode before the most abundant stable isotope, 169 Tm, is electron capture, and the primary mode after is beta emission.
|
| 38. | The primary decay mode before the most abundant stable isotope, 48 Ti, is electron capture and the primary mode after is beta emission.
|
| 39. | The primary decay mode before the most abundant stable isotope, 153 Eu, is electron capture, and the primary mode after is beta decay.
|
| 40. | The primary decay mode before the most abundant stable isotope, 55 Mn, is electron capture and the primary mode after is beta decay.
|
