Nuclear and Particle - University of Edinburghdwatts1/np3_07_l7.pdf · Nuclear and Particle Physics...
Transcript of Nuclear and Particle - University of Edinburghdwatts1/np3_07_l7.pdf · Nuclear and Particle Physics...
Nuclear and ParticlePhysics
3rd Year Junior HonoursCourse
Monday January 30th
Dr Daniel Watts
Lecture 7
Main points of lecture 6
3/13/2
AZaAaAa)Z,A(B
2
Csv −−= + δ (A,Z)A
)Z2A(a2
a−−
Liquid Drop model – nucleus viewed as being similar to a droplet of incompressible fluid
Volumeterm Asymmetry
termSurface
term
Coulombterm
Pairingterm
Parameters are extracted from fits to experimental data
Model gives good description of changes in binding energy per nucleon, and therefore M(A,Z), for all nuclei. Allows predictions of minimum stable isobars, energy released infission/fusion …etc
Notes Notes
Experimental evidence of shell effects in atomic physics
Atomic radii
Ionization energies
Ato
mic
rad
ius
(nm
)
Z
Separation energies Isotopic abundances
Neutron capture cross section
Nucleon number
Experimental evidence of shell effects in the nucleus
Notes Notes
Experimental evidence of shell effects in the nucleus
Stable Isotopes/ Isotones
Energy of 1st excited state of even-even nuclei
ASSUMPTIONS: ordered structure within nucleusnucleons move independently in potential wellallowed energy states determined by V(r)
SHELL MODEL
ANALOGY: atomic electron configuration⇒ high stability at closed-shell structures
(e.g. noble gases)⇒ chemical properties determined by
valence electrons
use V(r) in Schrödinger eqn. ⇒ predict quantised energy levels
IDEA: fill in states according to n and l quantum numberstry to reproduce nuclear MAGIC NUMBERS
Z, N = 2, 8, 20, 28, 50, 82, (126)
Question: How can you get independent nucleon motion in a densely packed nucleus? How do nucleons travel far enough between collisions to have definite spatial orbits?
Explanation: For nucleons to collide they must be quantum states available for scattered nucleon(s) to go into – many collisions are blocked in the nucleus as the possible states which the scattered nucleons could enter are already filled (Pauli blocking). Therefore nucleons generally orbit the nucleus as though they were transparent to each other!
Notes Notes
infinite square well potential
harmonic oscillator potential
Only smallest magic numbers are reproduced – even with a realisticpotential which reflects the measured charge distribution
Exclusion principle(applies independently to neutron and protons)
⇓
occupancy of each level: 2(2l +1)
ms
ml
What form for the potential?
PUZZLING PROBLEM
Short range of the nuclear force → expect potential to be similar shape to the proton (charge) distribution
NB. Proton distribution ~ same size as matter (protanand neutron) distribution e.g. 208Pb: 82 prot 126 neut. ∴ neutrons more densely packed!
(Mayer, 1949)
multiplicity
occupation of state = 2j+1
Shell model +
spin-orbit interaction L·S
Energy splitting ∆E ~ L·S
ENERGY of nucleon DECREASES when L // S
J = L + S has MAXIMUM possible value when L // Shigher J ⇒ lower energy
Use: n, l, j and mj as good quantum numbers
Exclusion principle ⇒ 2j + 1 possible values of mj
NOTE: labelling the state with j includes the effect of spin
closed shellsindicated by
“magic numbers”of nucleons
quantum energy states of potential well
+ angular momentum effects
spin-orbit splitting
Notes
1. Spin-orbit interaction much stronger in nuclei than in atoms
2. Its sign is opposite to the atomic case
3. Nuclear spin-orbit interaction is NOT of MAGNETIC origin,
but rather a PROPERTY of NUCLEAR FORCE
4. Atoms have either LS or JJ coupling
Nuclei almost all have JJ coupling as spin-orbit interaction
is much stronger in nuclei than in atoms
Differences between atomic and nuclear shell models
n = radial behaviour of wave functionradial node quantum number
l = angular behaviour of wave functionorbital quantum number
(see for example Eisberg & Resnick, p.536-541)
N.B. n is NOT the same as in atomic physics ( nprinc = nrad + l )!⇓
there are no restrictions on the value of l for any given n !