One of the most practical nuclear reactions results from the compound nucleus that results from A>230 nuclei ab

1. Total ,4n Cross Section ,3n ,2n ,n Alpha particle energy One of the most practical nuclear reactions results from the compound nucleus that results from A>230 nuclei absorbing neutrons. Often split into two medium mass nuclear fragments plus additional neutrons. NUCLEAR FISSION

2. 1930 Bothe & Becker Studying -rays bombarding beryllium produced a very penetrating non-ionizing form of radiation -rays? Irène and Frédéric Joliot-Curie knocked protons free from paraffin targets the proton energy range revealed the uncharged radiation from Be to carry 5.3 MeV 1932 James Chadwick in discussions with Rutherford became convinced could not be s Assuming Compton Scattering to be the mechanism, E>52 MeV!

3. ionization (cloud) chamber Neutron chamber Replacing the paraffin with other light substances, even beryllium, the protons were still produced. Nature, February 27, 1932

4. Chadwick developed the theory explaining the phenomena as due to a 5.3 MeV neutral particle with mass identical to the proton undergoing head-on collisions with nucleons in the target. 1935 Nobel Prize in Physics 9Behas a loosely bound neutron (1.7 MeVbinding energy) above a closed shell: 5-6 MeV  from some other decay Q=5.7 MeV Neutrons produced by many nuclear reactions (but can’t be steered, focused or accelerated!)

5. Natural sources of neutrons Mixtures of 226Ra ( source) and 9Be ~constant rate if neutron production also strong  source so often replaced by210Po, 230Pu or 241Am Spontaneous fission, e.g. 252Cf (½ = 2.65 yr) only 3% of its decays are through fission 97%-decays Yield is still 2.31012 neutrons/gramsec !

6. A possible (and observed) spontaneous fission reaction 8.5 MeV/A 7.5 MeV/A Gains ~1 MeVper nucleon! 2119 MeV = 238 MeV released by splitting 238U 119Pd

7. Atomic (chemical) processes ~few eV Fission involves108as much energy as chemicalreactions! Yet ½ = 1016 yr is a rare decay: not as probable as the much more common -decay ½ = 4.5109 yr why?

8. From the curve of binding energy per nucleon the most stable form of nuclear matter is as medium mass nuclei.

9. Consider: The Q value (energy release) of this process is The mass differences cancel since the total number of constituents remains unchanged. For simplicity, if we assume the protons and neutrons divide in the same ratio as the total nucleons:

10. The difference in binding energy comes from the surface and coulomb terms so the energy released can then be expressed in terms of the surface energy Es and the coulombenergy Ec of the original nucleus (A,Z). maximumQis found by settingdQ/dy1 = 0 Note: maximum occurs wheny1 = y2 = 1/2.

11. Fission into two equal nuclei (symmetric fission) produces the largest energy output or Q value The process is exothermic (Q > 0) if Ec/Es > 0.7. in terms of the fission parameter, x >0.35 Suggesting all nuclei with (Z2/A) > 18 (ie heavier than 90Zr) should spontaneously release energy by undergoing symmetric fission. However

12. Half-life of spontaneous fission as a function of x where and R.Vandenbosch and J.R.Huizenga. Nuclear Fusion, Academic Press, New York, 1973.

13. There is a competition between the nuclear force binding the nucleus together and the coulomb repulsion trying to tear it apart

14. Induced fission as nuclear reaction suggests the absorption of the neutron (and its energy) may induce such distortions/vibrations in the nucleus.

16. The surface if any arbitrary figure can be expanded as If lm time-independent:permanent deformation of the nucleus If lm time-dependent:an oscillation of the nucleus

17. The Spherical Harmonics Yℓ,m(,) ℓ = 3 ℓ = 0 ℓ = 1 ℓ = 2

18. ℓ = 0 Nuclear Charge Density  z ℓ = 1

19. Lowest order to be considered: quadrupole deformation ℓ = 2 For which we write the nuclear radius The l=2, m=0 mode:

20. Z 

21. Nuclei do show spectra for such vibrational modes Example of a vibrational spectrum (levels denoted by the number of phonons, N) O.Nathan and S.G.Nilsson, Alpha- Beta- and Gamma-Ray Spectroscopy, Vol.1, (K. Siegbahn, ed.) North Holland, Amsterdam, 1965.

22. We can approximate any small elongation from a spherical shape by semi-major axis semi-minor axis The semi-empirical mass formula From which:

23. With the surface energy (strong nuclear binding force) proportional to area Coulomb force deforming nucleus surface tension holding spherical shape which we can write in the form where Notice > 0 (so the Coulomb force wins out) for: Same fission parameter introduced when estimating available Q in symmetric fission

24. comes from considering small perturbations from a sphere. As long as these disturbances are slight, the Separation, r, of distinct fragments linearly follows  r for small r V(r) At zero separation the potential just equals the release energy Q For Z2/A<49,  is negative. separation r

25. While for large r, after the fragments have been scissioned  r r r for small r V(r) for large r separation r

26. For such quadrupole distortions the figure shows the energy of deformation (as a factor of the original sphere’s surface energy Es) plotted against  for different values of the fission parameter x. When x > 1 (Z2/A>49) the nuclei are completely unstable to such distortions.

27. Z2/A=36 such unstable states decay in characteristic nuclear times ~10-22sec Z2/A=49 Tunneling does allow spontaneous fission, but it must compete with other decay mechanisms (-decay) The potential energy V(r) = constant-B as a function of the separation, r, between fragments.

29. No stable states with Z2/A>49! Tunneling probability drops as Z2/A drops (half-life increases).

30. At smaller values of x, fission by barrier penetration can occur, However recall that the transmission factor (e.g., for -decay) is where m while for  particles (m~4u) this gave reasonable, observable probabilities for tunneling/decay for the masses of the nuclear fragments we’re talking about,  can become huge and X negligible.

31. Neutron absorption by heavy nuclei can create a compound nucleus in an excited state above the activation energy barrier. As we have seen, compound nuclei have many final states into which they can decay: . . . in general: where Z1+Z2=92, A1+A2+=236 PROMPT NEUTRONS Experimentally find the averageA1/A2peaks at3/2

32. Thermal neutrons E< 1 eV Slow neutrons E ~ 1 keV Fast neutrons E ~ 100 keV – 10 MeV Typical of decay Products & nuclear reactions The incident neutron itself need not be of high energy. “Thermal neutrons” (slowed by interactions with any material they pass through) have been demonstrated to be particularly effective. Cross section incident particle velocity, v This merely reflects the general ~1/v behavior we have noted for all cross sections!

33. At such low excitation there may be barely enough available energy to drive the two fragments of the nucleus apart. Division can only proceed if as much binding energy as possible is transformed into the kinetic energy separating them out. (so MOST of the available Q goes into the kinetic energy of the fragments!) Thus the individual nucleons settle into the lowest possible energy configurations involving the most tightly bound final states.

34. There is a strong tendency to produce a heavy fragment of A ~ 140 (with double magic numbers N = 82 and Z = 50).

35. Recall A possible (and observed) spontaneous fission reaction 8.5 MeV/A 7.5 MeV/A Gains ~1 MeVper nucleon! 2119 MeV = 238 MeV released by splitting 238U 119Pd

36. 238 MeV represented an estimate of the maximum available energy for symmetric fission. For the observed distribution of final states the typical average is ~200 MeVper fission. This 200 MeV is distributed approximately as:

37. 235U

38. Recall Isobars off the valley of stability (dark squares on preceding slide) b-decay to a more stable state.

39. Recall a and b decays can leave a daughter in an excited nuclear state 1/2- 2- b- b- 187W 198Au 0.68610 1.088 MeV 0.61890 b- b- 0.20625 0.412 MeV 0.13425 5/2+ 0+ 187Re 198Hg

40. With the fission fragments radioactive, a decay sequence to stable nuclei must follow

41. With the fission fragments radioactive, a decay sequence to stable nuclei must follow 25 sec b,g 18 min b,g 4 hr b,g 33 d b,g 0.03% 65 sec b,g 13 d b,g 40 h b,g 6 sec b,g 7 min b,g 10 hr b,g 106 yr b,g 1.40% 5 sec b,g 3 hr b,g 4 h b,g sometimes or

42. For 235U fission, average number of prompt neutrons ~ 2.5 with a small number of additional delayedneutrons.

43. with every neutron freed comes the possibility of additional fission events This avalanche is the chain reaction.

44. 235U will fission (n,f) at all energies of the absorbed neutron. It is a FISSILE material. However such a reaction cannot occur in natural uranium (0.7% 235U, 99.3% 238U)

45. Total (t) and fission (f) cross sections of 235U. 1 b = 10-24 cm2

47. Notice: 238U has a threshold for fission (n,f) at a neutron energy of 1MeV. The difference between these two isotopes of uranium is explained by the presence of the pairing term in the semi-empirical mass formula. for Z even, N even for Z odd, N odd for A odd Like nucleons couple pairwise into especially stable configurations.

48. Note the strong resonant capture of neutrons (n, ) in the energy range 10-100 eV (particularly for 238U where the cross-section reaches high values)

49. The fission neutron energy spectrum peaks at around1 MeV

50. At 1 MeV the inelastic cross-section (n,n') in 238U exceeds the fission cross-section. This effectively prevents fission from occurring in 238U.