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7-1 Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability.

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Presentation on theme: "7-1 Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability."— Presentation transcript:

1 7-1 Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability of Fission Fission Product Distributions §Total Kinetic Energy Release §Fission Product Mass Distributions §Fission Product Charge Distributions Fission in Reactors §Delayed neutron Proton induced fission

2 7-2 Nuclear Fission Fission discovered by Otto Hahn and Fritz Strassman, Lisa Meitner in 1938 §Demonstrated neutron irradiation of uranium resulted in products like Ba and La àChemical separation of fission products For induced fission, odd N §Addition of neutron to form even N §Pairing energy In 1940 G. N. Flerov reported that 238 U undergoes fission spontaneously §half life of round 10 16 y §Several other spontaneous fission isotopes found àZ > 90 §Partial fission half lives from nanoseconds to 2E17 years

3 7-3 Fission Can occur when enough energy is supplied by the bombarding particle for the Coulomb barrier to be surmounted §Fast neutron §Proton Spontaneous fission occurs by tunneling through barrier §Similar to alpha decay Thermal neutron induced fission from pairing of unpaired neutron §Nuclides with odd number of neutrons fissioned by thermal neutrons with large cross sections §follow 1/v law at low energies, sharp resonances at high energies

4 7-4 Energetics Calculations Why does 235 U undergo neutron induced fission for thermal energies? §Where does energy come from? Generalized energy equation § A Z + n  A+1 Z + E For 235 U §E=(40.914+8.071)-42.441 §E=6.544 MeV For 238 U §E=(47.304+8.071)-50.569 §E=4.806 MeV For 233 U §E=(36.913+8.071)-38.141 §E=6.843 MeV Fission requires around 5-6 MeV

5 7-5 Fission Process Usually asymmetric mass split §M H /M L  1.4 for uranium and plutonium §due to shell effects, magic numbers àHeavy fragment peak near A=132, Z=50, N=82 §Symmetric fission is suppressed by at least two orders of magnitude relative to asymmetric fission Occurs in nuclear reactions §Competes with evaporation of nucleons in region of high atomic numbers As mass of the fissioning system increases §Location of heavy peak in the fission remains constant §position of the light peak increases Fission Process Nucleus absorbs energy §Excites and deforms §Configuration “transition state” or “saddle point” Nuclear Coulomb energy decreases during deformation §Nuclear surface energy increases Saddle point key condition §rate of change of the Coulomb energy is equal to the rate of change of the nuclear surface energy §Induces instability that drives break up of nucleus

6 7-6 Fission Process If the nucleus deforms beyond this point it is committed to fission §Neck between fragments disappears §Nucleus divides into two fragments at the “scission point.” àtwo highly charged, deformed fragments in contact Large Coulomb repulsion accelerates fragments to 90% final kinetic energy within 10 -20 s

7 7-7 Fission Products Fission yield curve varies with fissile isotope 2 peak areas for U and Pu thermal neutron induced fission Variation in light fragment peak Influence of neutron energy observed 235 U fission yield

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9 7-9 Fission Primary fission products always on neutron-excess side of  stability §high-Z elements that undergo fission have much larger neutron-proton ratios than the stable nuclides in fission product region §primary product decays by series of successive  - processes to its stable isobar Yields can be determined §Independent yield: specific for a nuclide §Cumulative yield: yield of an isobar àBeta decay to valley of stability §Data for independent and cumulative yields can be found or calculated For reactors §Emission of several neutrons per fission crucial for maintaining chain reaction §“Delayed neutron” emissions important in control of nuclear reactors Comparison of cumulative and independent yields for A=141

10 7-10 Fission products Particles form more spherical shapes §Converting potential energy to emission of “prompt” neutrons §Gamma emission after neutrons  Then  decay  Occasionally one of these  decays populates a high lying excited state of a daughter that is unstable with respect to neutron emission §“delayed” neutrons §0.75 % of total neutrons à 137-139 I and 87-90 Br as examples

11 7-11 Delayed Neutrons Fission fragments are neutron rich §More neutron rich, more energetic decay §In some cases available energy high enough for leaving the residual nucleus in such a highly excited state àAround 5 MeV àneutron emission occurs

12 7-12 Delayed Neutrons in Reactors Control of fission §0.1 msec for neutron from fission to react àNeed to have tight control à0.1 % increase per generation *1.001^100, 10 % increase in 10 msec Delayed neutrons useful in control §Longer than 0.1 msec §0.65 % of neutrons delayed from 235 U à0.26 % for 233 U and 0.21 % for 239 Pu Fission product poisons influence reactors § 135 Xe capture cross section 3E6 barns

13 7-13 Nuclear reactors Probable neutron energy from fission is 0.7 MeV §Fast reactors àHigh Z reflector §Thermal reactors need to slow neutrons àWater, D 2 O, graphite *Low Z and low cross section Power proportional to number of available neutrons §Should be kept constant under changing conditions àControl elements and burnable poisons §k=1 (multiplication factor) àRatio of fissions from one generation to the next *k>1 at startup

14 7-14 Fission Process and Damage Neutron spatial distribution is along the direction of motion of the fragments Energy release in fission is primarily in the form of the kinetic energies Energy is “mass-energy” released in fission due to the increased stability of the fission fragments Recoil length about 10 microns, diameter of 6 nm §About size of UO 2 crystal §95 % of energy into stopping power àRemainder into lattice defects *Radiation induced creep §High local temperature from fission à3300 K in 10 nm diameter

15 7-15 Energetics Any nucleus of A> 100 into two nuclei of approximately equal size is exoergic. §Why fission at A>230 Separation of a heavy nucleus into two positively charged fragments is hindered by Coulomb barrier §Treat fission as barrier penetration àBarrier height is difference between *Coulomb energy between the two fragments when they are just touching *the energy released in the fission process Near uranium both these quantities have values close to 200 MeV

16 7-16 Energetics 200 Hg give 165 MeV for Coulomb energy between the fragments and 139 MeV for energy release §Lower fission barriers for U when compared to Hg Barrier height increases more slowly with increasing nuclear size compared to fission decay energy Spontaneous fission is observed only among the very heaviest elements Half lives generally decrease rapidly with increasing Z

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18 7-18 Energetics Generalized Coulomb barrier equation §Compare with Q value for fission Determination of total kinetic energy §Equation deviates at heavy actinides (Md, Fm) Consider fission of 238 U §Assume symmetric § 238 U  119 Pd + 119 Pd + Q à Z=46, A=119 *V c =46 2 *1.440/(1.8(119 1/3 )2)=175 MeV *Q=47.3087-(2*-71.6203) = 190.54 MeV §asymmetric fission § 238 U  91 Br + 147 La + Q àZ=35, A=91 àZ=57, A=147 *V c =(35)(57)*1.44/(1.8*(91 1/3 +147 1/3 ))=164 MeV *Q=47.3087-(-61.5083+-66.8484) = 175.66 MeV Realistic case needs to consider shell effects

19 7-19 Fission Isomers Some isomeric states in heavy nuclei decay by spontaneous fission with very short half lives §Nano- to microseconds Fissioning isomers are states in these second potential wells §Also called shape isomers §Exists because nuclear shape different from that of the ground state, Around 30 fission isomers are known, from U to Bk Induced by neutrons, protons, deuterons, and  particles

20 7-20 Fission Isomers: Double-humped fission barrier At lower mass numbers, the second barrier is rate- determining, whereas at larger A, inner barrier is rate determining Symmetric shapes are the most stable at two potential minima and the first saddle, but some asymmetry lowers second saddle

21 7-21 Proton induced fission Energetics impact fragment distribution excitation energy of the fissioning system increases §Influence of ground state shell structure of fragments would decrease §Fission mass distributions shows increase in symmetric fission

22 7-22 Topic Review Mechanisms of fission §What is occurring in the nucleus during fission Understand the types of fission §Particle induced §Spontaneous Energetics of fission §Q value and coulomb barrier The Probability of Fission §Cumulative and specific yields Fission Product Distributions §Total Kinetic Energy Release §Fission Product Mass Distributions

23 7-23 Questions Compare energy values for the symmetric and asymmetric fission of 242 Am. What is the difference between prompt and delayed neutrons in fission. What is the difference between induced and spontaneous fission. What influences fission product distribution? Compare the Coulomb barrier and Q values for the fission of Pb, Th, Pu, and Cm. Describe what occurs in the nucleus during fission. Compare the energy from the addition of a neutron to 242 Am and 241 Am. Which isotope is likely to fission from an additional neutron.

24 7-24 Pop Quiz Provide calculations showing why 239 Pu can be fissioned by thermal neutron but not 240 Pu. Compare the Q value and Coulomb energy (V c ) from the fission of 239 Pu resulting in 138 Ba and 101 Sr. Is this energetically favored?

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