Nuclear Shell model. C. Prediction of spins and Parities: GROUND RULES 1. Even-Even Nuclei. I π = 0 +

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Noreen Copeland
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1 Nuclear Shell model C. Prediction of spins and Parities: GOUND ULES 1. Even-Even Nuclei I π = 0 + ULE: ll nucleon orbitals are filled pairwise, i.e., ν,l, j, m j state followed by ν, l, j, m j state NO EXCEPTIONS 2. Odd- Nuclei INDEPENDENT PTICLE SSUMPTION Nucleons fill orbitals pairwise up to last odd nucleon. ULE: Last odd nucleon determines quantum properties of entire nucleus esult: a. 1 X core is e-e; 0+ b. Last particle Iπ given by HO model with strong spin-orbit coupling; c. Total Nucleus I = (core) + (last nucleon) = 0 + j = j π = π (core) π (last nucleon) = + ± = ±

3 NOTE: On figure of energy levels with spin-orbit coupling, parity alternates from shell to shell (ν ν + 1) Filling levels: same as doing electron configurations in Bohr atom 3. Odd-Odd Nuclei Must couple last odd proton to last odd neutron. I = j n + j p NOT COVEED: difficult angular momentum (vector additions). 4. Examples: a. { 12 C, 24 O, 184 Pb, } ll Iπ = 0+ b. 119 In = 118 Cd + p th proton in level is: 1 g 9/2 ; j = 9/2 ; g state: π = + Get from figure of energy levels with spin-orbit coupling = 4 Predict Iπ = 9/2 + This is observed.

4 47 46 c. : Ca Ca + n 20 : 20 Get from figure of energy levels with spin-orbit coupling th neutron is 1 f 7/2 j = 7/2, l = 3, π = Predict: Iπ = 7/2 5. Bottom Line: Same counting game as in atoms (1s 2 2s 2 2p 6 3s 2...) Works near closed shells ; deviations away from them.

5 D. Excited States 1. Particles and elative Energies Given by level scheme: e.g. 15 8O 7 Ground state (7) (6) (2) 1p 1/2 1p 3/2 1s 1/2

6 15 8O 7 Excited state 2s 1/2 1d 3/2 E 3 1/2+ E 2 3/2+ single particle state 1d 5/2 E 1 5/2+ (7) (6) (2) 1p 1/2 1p 3/2 1s 1/2 2. otational and Vibrational States also exist Due to collective motion of nucleus, superimposed on single-particle state.

7 E. The Shell Model and the eal World 1. Closed Shells Correct 2. Spins, Parities and Magnetic Moments described systematically a. e-e: lways right b. o-: usually correct for spherical nuclei (near closed shells). Less accurate in between c. o-o: difficult horseshoes 3. Low-lying energy levels also correct near closed shells. VIII. Unified Model Combines LD and Shell models; allows for deformed shapes changes order of levels between shells, but not magic numbers. V ( r) ax by cz = V

8 Nuclear Potentials and adioactive Decay I. Nuclear Stability and Basic Decay Modes. Schematic epresentation: Synthesis Equilibration Decay X+Y + Energy τ s Z Z * τ ~ s Composite nucleus (ctivated Complex)

9 B. Stable Nuclei 1. N/Z composition: Does not change with time peak of <BE> curve Kinetic vs. Thermodynamic stability; detection limit y 2. Total: 266 t least one stable nucleus for all Z=1 83 EXCEPT 43 Tc and 61 Pm C. adioactive Nuclei 1. Definition: nucleus that SPONTNEOUSLY alters its neutron/proton composition or energy state FIST-ODE TE POCESS DIOCTIVE DECY IS IDENTICL WITH N ELEMENTY UNIMOLECUL DISSOCITION IN CHEMISTY. ( B + C) Contrast with: nuclear reactions n/p changes induced by collisions, 2 nd order NUCLE ECTIONS HVE THE SME FOM S N ELEMENTY BIMOLECUL CHEMICL ECTION ( + B C + D)

10 2. Half-life: t 1/2 Definition: The length of time required for one-half the nuclei in a sample to disintegrate (decay): N( t) λ = = N 0 e t 1/ 2 λt 3. Primary Decay Modes 4 a. lpha Decay: He emission 2 b. Beta Decay: neutron proton conversion β specifies nuclear origin e specifies atomic origin c. Gamma Decay: γ, photon emission γ = nuclear origin ; x-ray, uv, visible, ir = atomic/molecular origin d. Exotic decay modes: fission, protons, neutrons, 14 C, etc.

11 4. adioactivity in Nature (t 1/ y) a. U Th Decay series U ( y) 92 6β U ( y) 4β Th 90 ( y) 4β 206 Pb 82 (24.1%) = 4n Pb (22.1%) = 4n Pb 82 (52.3%) = 4n where n is an integer Np (2 106 y) Bi (100%) = 4n EXTINCT: 4β TOTL: 45 NUCLEI (t 1/2 of all daughters < t 1/2 of parents)

13 b. Lighter adionuclides in Nature (1) Survivors of Nucleosynthesis ; esp. 40 K, 87 b, 147 Sm TOTL = 15 (2) Cosmic-ay-Induced ctivity 3 H(12y), 14 C(5280y), 7 Be(52d), 10 Be(~10 6 y), c. Natural radioactivities carry history of solar system and its evolution

14 5. Synthetic Nuclei (t 1/ y) Isotopes of all elements: Z = 0 to 117 ( and more?) 6. Grand Total: 3500 nuclei and still counting Factors that Govern Decay ate 1. Energetics large Q rapid decay (short half-life) B + C + Q 2. Quantum Structure Spin and Parity: Changes in Iπ between parent and daughter slow down decay rate e.g. 3 s 1/2 2 d 5/2 1 p 3/2 Iπ = 1/2+ 5/2+ 3/2- π even even odd

15 II. lpha Decay. Mechanism: Z 4 He Z-2 X Y + Q He 2+ Y 2 tomic Ionization State lpha ecoil B. Energetics 1. Spectra: Discrete energies 2. Q = Δ(X) - Δ(Y) - Δ() 3. Energy systematics ange of values: Q ~ MeV measured Th Example 228 Th 224 a + 4 He + Q 90 2 Q = ( 228 Th) ( 224 a) () = = MeV Measure: E = MeV WHY?

16 5. Disposition of Q (1) Kinetic energy of + recoil : E + E (2) Internal excitation energy ( heat) of recoil nucleus, E* ( has no stable excited states) Case I: Q Kinetic Energy Only X Y X, Y all in lowest (ground) energy state i.e., E* = 0 (T = 0) Energy Conservation: Q = E + E (E = 1/2 Mv 2 ) Linear Momentum Conservation p + p = 0 p = 2ME

17 esult of energy and linear momentum conservation E E = = M M M + M M + M Q Q + + Q Q True for all 2-body breakup processes SPECT MUST BE DISCETE, since, Q, M are all constants Tag for nucleus ID b. Case II: Decay to Excited States X Y* E* Eγ i.e., system then undergoes γ-decay Kinetic energy of alpha particle : E a Kinetic energy of recoil nucleus: E Energy Conservation: Q = E + E + E* = E + E + E γ Q γ E γ since M γ = 0

18 Momentum Conservation 0 = p + p + p γ p γ 0 since ; neglect 0 = p + p esult of energy and linear momentum conservation for this case: ) ( ) ( γ γ E Q E Q M M M E + + = ) ( ) ( γ γ E Q E Q M M M E + + = NOTE: TOTL ENEGY MUST BE THE SME, EGDLESS OF PTHWY Q E 1 E 2 E γ

20 C. lpha Decay Probability 1. Energetics: Q positive for all >140 nuclei 2. ange of Measured Half-Lives (~10 44 ) y > t 1/2 > s 3. Why? a. Proton & Neutron Emission: Q p, Q n are negative near valley of beta stability (peak of peninsula); Thermodynamically forbidden b. Other Nuclei ; e.g. 12 C, 16 O Q( 12 C), Q( 16 O) positive ; therefore possible Probability is low (i.e., t 1/2 ) is long) -- P( 14 C)/P ~ P Th 14 C+ 218 Po FCTS (Exotic decay mode) 11.7 MeV particles from 212m Po are the highest energy alphas from a radioactive source 2.0 MeV alphas from Sm are the among lowest energy alphas from a radioactive source Most alpha particles from radioactive sources fall in the range of 4-8 MeV. ssociated with this narrow range in energy is the enormous range in half-life noted above. WHY?

Composite Nucleus (Activated Complex)

Composite Nucleus (Activated Complex) Lecture 10: Nuclear Potentials and Radioactive Decay I. Nuclear Stability and Basic Decay Modes A. Schematic Representation: Synthesis Equilibration Decay X + Y + Energy A Z * Z ( 10 20 s) ( ~ 10 16 10