name: nuclear
description: > Expert nuclear physics assistant for physicists and students. Use this skill whenever the user needs: help with nuclear structure, radioactive decay, nuclear reactions, fusion and fission energy, or radiation detection. Includes both theoretical foundations and applications. trigger: Any nuclear physics question - from structure to reactions to medical and energy applications. license: MIT compatibility: opencode metadata: audience: physicists category: physics
Nuclear Physics — Structure, Decay, and Reactions
Covers: Nuclear Structure · Radioactive Decay · Nuclear Reactions · Fusion · Fission · Radiation Detection
Nuclear Structure
Nuclear Composition
Nucleus = protons + neutrons (nucleons):
- Atomic number Z: number of protons
- Neutron number N: number of neutrons
- Mass number A = Z + N
Isotopes: same Z, different N. Isotones: same N, different Z. Isobars: same A, different Z.
Nuclear Sizes
Charge radius:
R = r₀ A^{1/3}, r₀ ≈ 1.2 fm
Matter radius slightly larger: r₀ ≈ 1.4 fm.
Nuclear Density
Roughly constant inside nucleus:
ρ ≈ 0.16 nucleons/fm³
Uniform density → Fermi gas model.
Nuclear Spin
Total angular momentum I = combination of:
- Orbital angular momentum l of each nucleon
- Spin s of each nucleon (½)
Nuclear Moments
Magnetic dipole moment:
μ = g_I μ_N I
μ_N = eℏ/2m_p (nuclear magneton)
Electric quadrupole moment: Q measures deviation from spherical.
Nuclear Shell Model
Nucleons in shells (like electrons):
- Magic numbers: 2, 8, 20, 28, 50, 82, 126
- Extra stability at magic numbers
Spin-orbit interaction causes shell splitting.
Magic Numbers and Shell Closures
| Magic | Protons | Neutrons |
|---|---|---|
| 2 | He | n |
| 8 | O | O |
| 20 | Ca | Ca |
| 28 | Ni | Ni |
| 50 | Sn | Sn |
| 82 | Pb | Pb |
| 126 | - | - |
Collective Model
Deformed nuclei:
- Vibrational states
- Rotational bands
- Quadrupole moments
Liquid Drop Model
Semi-empirical mass formula:
B(A,Z) = a_V A - a_S A^{2/3} - a_C Z²/A^{1/3} - a_A (A-2Z)²/A + δ(A,Z)
| Term | Description | Typical Value |
|---|---|---|
| Volume | a_V A | 15.8 MeV |
| Surface | a_S A^{2/3} | 18.3 MeV |
| Coulomb | a_C Z²/A^{1/3} | 0.714 MeV |
| Asymmetry | a_A (A-2Z)²/A | 23.2 MeV |
| Pairing | δ | ±12 MeV |
Mass Excess and Binding Energy
Mass excess: ΔM = [M - A u] c² Binding energy: B = Z m_p + N m_n - M
Nuclear Forces
Short-range (~1 fm):
- Strong interaction
- Spin-dependent
- Charge independent
- Spin-orbit term
NN potential: Reid, Argonne, Nijmegen.
Deuteron Properties
- Bound state: B = 2.22 MeV
- Quadrupole moment
- Spin triplet (S=1)
Nucleon-Nucleon Scattering
Phase shift analysis:
- Singlet, triplet channels
- Partial wave expansion
Radioactive Decay
Decay Modes
| Mode | Description | Particles |
|---|---|---|
| α | He nucleus emitted | ⁴He |
| β⁻ | neutron → proton + e⁻ + ν̅_e | e⁻ |
| β⁺ | proton → neutron + e⁺ + ν_e | e⁺ |
| EC | e⁻ capture | ν_e |
| γ | Photon emission | γ |
| n | neutron emission | n |
| Fission | Split | Fragments |
Alpha Decay
Tunneling through Coulomb barrier:
T ∝ exp(-2G), G = (2m|Q|R/ℏ²)^{1/2}
Geiger-Nuttall law:
log T = aZ/√A + b
Beta Decay
Fermi's Golden Rule:
λ = (2π/ℏ) |M|² ρ(E)
Allowed transitions:
- Fermi: Δπ = no, ΔS = 0
- Gamow-Teller: Δπ = no, ΔS = 1
Forbidden transitions: ΔL > 0, suppressed.
Neglect of Parity
Weak interaction violates parity:
- Only left-handed neutrinos
- Maximum parity violation
Electron Capture
p + e⁻ → n + ν_e:
- Competes with β⁺
- Q must be > 0.511 MeV
Gamma Decay
Electromagnetic transitions:
- E1: Δπ = yes, ΔL = 1
- E2: Δπ = no, ΔL = 2
- M1: Δπ = no, ΔL = 0,1
Weisskopf estimates for transition rates.
Internal Conversion
Energy → e⁻ instead of γ:
- Competes with γ
- Higher for low-energy transitions
Decay Chains
Long chains of decays:
- ²³⁸U → ... → ²⁰⁶Pb
- ²³⁵U → ... → ²⁰⁷Pb
- ²³²Th → ... → ²⁰⁸Pb
- ⁴⁰K → ⁴⁰Ar, ⁴⁰Ca
Decay Constants
Activity:
A = λN = A₀ e^{-λt}
Half-life: t_{1/2} = ln 2 / λ
Mean lifetime: τ = 1/λ
Branching Ratios
Multiple decay modes possible:
- Branching ratio = fraction in each mode
- Sum = 100%
Secular Equilibrium
For daughter with shorter half-life: N_2(t) = λ_1 N_1 / (λ_2 - λ_1) (e^{-λ_1 t} - e^{-λ_2 t})
Transient Equilibrium
When parent half-life comparable.
Nuclear Reactions
Q-Value
Energy released:
Q = (m_initial - m_final) c²
Positive: exothermic Negative: endothermic
Threshold Energy
For endothermic reactions:
E_th = -Q (m_final/m_projectile)
For charged particles, must overcome Coulomb barrier.
Reaction Types
| Type | Example |
|---|---|
| Elastic | a + A → a + A |
| Inelastic | a + A → a* + A |
| Capture | a + A → B + γ |
| Transfer | a + A → b + B |
| Spallation | p + A → many |
| Fusion | light → heavier |
| Fission | heavy → lighter |
Cross Section
σ = (rate)/(flux × target nuclei)
Units: barns (10⁻²⁴ cm²)
Compound Nucleus
High-energy intermediate:
- Equilibrium reached
- Statistical decay
Direct Reactions
Peripheral collisions:
- Stripping, pickup
- Few nucleons transferred
Optical Model
Complex potential:
U(r) = V(r) + iW(r)
Describes elastic scattering.
Compound Elastic
Through compound nucleus, interferes with direct.
Resonance Scattering
Breit-Wigner formula:
σ(E) = σ₀ (E_R/E) [(E_R/2)² + Γ²/4] / [(E-E_R)² + Γ²/4]
Fusion Reactions
D + T → α + n (14.1 MeV) D + D → T + p (4.0 MeV) D + D → ³He + n (3.3 MeV) p + ¹¹B → 3α (8.7 MeV)
Fission
Nuclei split:
- Heavy (A > 230) typically
- Energy ~200 MeV
Neutrons released → chain reaction.
Fission Products
Most at probable A ~ 95 and 140. Neutron-rich → β decay chains.
Fission Barriers
Double-humped for deformed:
- Outer barrier
- Inner barrier
- Isomeric states
Nuclear Models
Shell Model
Independent particles in potential:
- Harmonic oscillator
- Woods-Saxon potential
- Spin-orbit term
Configuration Mixing
Mix of Slater determinants. Shell model wavefunctions.
Cluster Model
Preformed clusters:
- α-clustering in ⁸Be, ¹²C
- α + ¹²C in ¹⁶O
Mean Field
Hartree-Fock approach:
- Self-consistent potential
- Single-particle states
RPA (Random Phase Approximation)
Excited states:
- Correlated particle-hole
- Collective modes
Interacting Boson Model
IBM:
- s and d bosons
- SU(3), O(6) limits
Ab Initio Methods
Start from NN interaction:
- No-core shell model
- Green's function Monte Carlo
- Coupled cluster
Density Functional Theory
EDF approaches:
- Skyrme, Gogny forces
- Global fits to data
Radiation Detection
Detector Types
| Detector | Type | Application |
|---|---|---|
| Scintillator | Organic/inorganic | γ, β, α |
| Gas proportional | Gas amplification | α, β |
| Semiconductor | e-hole pairs | γ, charged |
| Cerenkov | Light from μ > c/n | μ, neutrinos |
| Calorimeter | Absorber + sensor | Energy measurement |
Energy Resolution
σ/E ∝ 1/√E
Better with semiconductor.
Pulse Height
Proportional to energy deposited. Calibration needed.
Photomultiplier Tubes
Light → photoelectron → cascade. Gain ~10⁶-10⁸.
Spectroscopy
- HPGe: high resolution
- NaI(Tl): high efficiency
- Si(Li): X-rays
Particle Identification
| Method | Measures |
|---|---|
| dE/dx | Energy loss |
| Time of flight | Velocity |
| Cerenkov | Velocity |
| TRD | Transition radiation |
| Muon chambers | Penetration |
Neutron Detection
Via reactions:
- ³He(n,p)³H
- B(n,α)
- Fission
Background
Cosmic rays:
- Muons, neutrons
- Shielding needed
Internal contamination:
- Natural radionuclides
- Cosmogenic activation
Dead Time
Paralyzable vs. non-paralyzable. Correct for high rates.
Coincidence Detection
Reduce background:
- Time coincidence
- Compton suppression
Pulse Shape Discrimination
Separate particles:
- n/γ in liquid scint
- α/β in some scintillators
Applications
Nuclear Energy
- Fission reactors
- Fusion (future)
- Radioisotope generators
Medical
- Radiotherapy (γ, e⁻)
- Imaging (PET, SPECT)
- Radioisotope production
Dating
- ¹⁴C dating (t₁/2 = 5730 y)
- K-Ar (t₁/2 = 1.25 Gy)
- U-Pb
Tracers
- Metabolic studies
- Industrial tracers
- Environmental
Astrophysics
- Nucleosynthesis (r, s, p processes)
- Solar neutrinos
- Cosmic rays
Materials
- Ion implantation
- Neutron activation analysis
- Radiation damage studies
Security
- Portal monitors
- SNM detection
- Arms control verification
Reactor Physics
Neutron Economy
- Production: fission
- Loss: absorption + leakage
- Breeding possible with fast reactors
Criticality
k_eff = 1:
- Prompt critical: exponential growth
- Delayed neutrons needed for control
Moderation
Slow neutrons:
- Hydrogen, deuterium
- Graphite
- Slowing down power
Cross Sections
- Capture: σ_γ
- Fission: σ_f
- Scattering: σ_s
Resonances important.
Reactor Types
| Type | Moderator | Fuel |
|---|---|---|
| PWR | H₂O | UO₂ (enriched) |
| BWR | H₂O | UO₂ |
| CANDU | D₂O | UO₂ (natural) |
| graphite | C | U (natural) |
| Fast | none | Pu, MOX |
Fuel Cycle
- Mining, enrichment
- Burnup in reactor
- Spent fuel
- Reprocessing
- Waste disposal
Criticality Safety
- Keep systems subcritical
- Double contingency
- Geometry control
Common Errors to Avoid
- Confusing mass number with atomic mass
- Using wrong units (keV vs MeV)
- Forgetting binding energy in Q-value
- Confusing decay constant with half-life
- Misapplying decay chain equations
- Confusing cross section with probability
- Forgetting Coulomb barrier in fusion
- Using classical instead of quantum tunneling
- Confusing neutrons and protons in strong force
- Ignoring parity violation in weak decays
Key References
- Introductory Nuclear Physics by Krane — Standard text
- Nuclear Physics by Wong — Theory
- Nuclear Physics: Principles and Applications — Modern
- Radiation Detection and Measurement — Knoll — Detection