In the experimental determination of the outputs of reactions $(\gamma, \gamma')$ in the small interval of 5-9 MeV with a step up to 0.5 MeV there are points of deviation of the energy dependence of absolute outputs from a monotonically increasing curve [1]. This effect allows you to determine the values of individual or group of activation levels, through which the isomers of the nucleus are populated. In paper [1], the energy dependences of the outputs for reactions $(\gamma, \gamma')^m$ on the 77Se, 79Br, 89Y, 103Rh and 111Cd nuclei were analyzed for the presence of fractures.
Also, the dependences of the absolute output from energies [2-4] for the reactions $(\gamma, \gamma')^m$ on heavy nuclei 137Ba, 179Hf, 197Au and 199Hg are analyzed. The number of detected activation levels in each of these $(\gamma, \gamma')^m$- reactions ranges from one to three values.
The probabilities for $\gamma$- transitions can be approximately calculated from the formulas [5]:
$$W(EJ) \approx \frac{1}{\lambda} \left(\frac{R}{\lambda}\right)^{2J}; \qquad W(MJ) \approx \frac{1}{\lambda} \left(\frac{R}{\lambda}\right)^{2J+2};\tag{1}$$where $\lambda = \hbar c/E_{\gamma}$ - the wavelength for the emitted or absorbed $\gamma$- quanta's; J - multipolarity; EJ and MJ - the electric and magnetic $\gamma$- radiations with parity $P=(-1)^J$ and $P=(-1)^{J+1}$ accordingly; R - the radius of the emitted core. For the selenium nucleus, the transitions from metastable levels to the isomeric level 77mSe are shown in Table 1, where the ratio of the $\gamma$ transitions is indicated
$$\alpha = \frac{W(EJ)}{W(MJ)}.\tag{2}$$| λ, m | Eγ, keV | J | W(EJ), m-1 | W(MJ), m-1 | α |
|---|---|---|---|---|---|
| 1.48E-11 | 13.38 | 8 | 1.02E-44 | 1.44E-51 | 7.12E+06 |
| 2.25E-12 | 87.86 | 6 | 2.19E-20 | 1.33E-25 | 1.65E+05 |
| 1.42E-12 | 139.22 | 6 | 8.70E-18 | 1.32E-22 | 6.58E+04 |
| 7.12E-13 | 277.53 | 6 | 6.83E-14 | 4.12E-18 | 1.66E+04 |
| 3.81E-13 | 518.18 | 6 | 2.29E-10 | 4.82E-14 | 4.75E+03 |
| 2.98E-13 | 662.51 | 6 | 5.58E-09 | 1.92E-12 | 2.91E+03 |
Similar calculations of the probability ratio of electromagnetic $\gamma$- transitions can be made for nuclides 89mY, 103mRh, 179mHf and others.