Appendix G — Notation and Symbol Guide
This appendix collects all notation and symbol conventions used in this textbook. When a symbol has multiple standard meanings in nuclear physics, we note which convention this book follows and in which chapters the symbol appears. Where conventions differ from those common in other subfields (atomic physics, particle physics), we note the difference.
G.1 Nuclear Notation
G.1.1 Nuclide Designation
A nuclide is specified by its chemical symbol $X$, mass number $A$ (total nucleon count), and atomic number $Z$ (proton count):
$${}^A_Z X_N$$
where $N = A - Z$ is the neutron number. In practice, the subscripts $Z$ and $N$ are often omitted because the chemical symbol uniquely determines $Z$:
$${}^A X \qquad \text{e.g., } {}^{12}\text{C}, \; {}^{56}\text{Fe}, \; {}^{238}\text{U}$$
When $Z$ is needed for clarity (e.g., in nuclear reactions or when the element is unfamiliar), the full notation ${}^A_Z X$ is used:
$${}^{238}_{92}\text{U}, \quad {}^{12}_{\;6}\text{C}$$
Isomers: A nuclear isomer (metastable excited state) is designated by appending $m$ (or $m1$, $m2$ for multiple isomers) to the mass number:
$${}^{99m}\text{Tc}, \quad {}^{137m}\text{Ba}, \quad {}^{178m2}\text{Hf}$$
G.1.2 Related Terminology
| Term | Definition | Example |
|---|---|---|
| Isotopes | Same $Z$, different $N$ | ${}^{12}$C, ${}^{13}$C, ${}^{14}$C |
| Isotones | Same $N$, different $Z$ | ${}^{13}$C ($N$=7), ${}^{14}$N ($N$=7) |
| Isobars | Same $A$, different $Z$ | ${}^{14}$C, ${}^{14}$N |
| Isomers | Same $Z$, same $A$, different excitation | ${}^{99}$Tc, ${}^{99m}$Tc |
| Mirror nuclei | $Z$ and $N$ exchanged | ${}^{13}$C ($Z$=6, $N$=7), ${}^{13}$N ($Z$=7, $N$=6) |
| Nuclide | A specific nuclear species $(Z, N)$ | ${}^{56}$Fe |
G.2 Quantum Numbers
G.2.1 Nuclear State Quantum Numbers
| Symbol | Name | Definition / Range | Where Introduced |
|---|---|---|---|
| $J$ | Total angular momentum | Resultant of all nucleon angular momenta; $J = 0, 1/2, 1, 3/2, \ldots$ | Ch. 2 |
| $\pi$ | Parity | $+$ or $-$; eigenvalue of the parity operator | Ch. 2, 5 |
| $J^\pi$ | Spin-parity | Combined notation, e.g., $0^+$, $3/2^-$, $2^+$ | Ch. 2 |
| $T$ | Isospin | Total isospin quantum number; $T = 0, 1/2, 1, \ldots$ | Ch. 2, 3 |
| $T_3$ (or $M_T$, $T_z$) | Isospin projection | $T_3 = (N - Z)/2$; runs from $-T$ to $+T$ | Ch. 2, 3 |
| $K$ | $K$-quantum number | Projection of $J$ on the nuclear symmetry axis (deformed nuclei) | Ch. 8 |
G.2.2 Single-Particle Quantum Numbers
| Symbol | Name | Definition / Range | Where Introduced |
|---|---|---|---|
| $n$ | Principal quantum number | Radial node count (convention: $n = 1, 2, 3, \ldots$; or $n_r = 0, 1, 2, \ldots$ with $n = n_r + 1$) | Ch. 5, 6 |
| $l$ | Orbital angular momentum | $l = 0, 1, 2, 3, \ldots$ ($s, p, d, f, g, h, \ldots$) | Ch. 5, 6 |
| $s$ | Intrinsic spin | $s = 1/2$ for nucleons | Ch. 5 |
| $j$ | Single-particle total angular momentum | $j = l \pm 1/2$ | Ch. 5, 6 |
| $m_j$ | Magnetic quantum number | Projection of $j$ on quantization axis; $m_j = -j, \ldots, +j$ | Ch. 5 |
| $m_l$ | Orbital magnetic quantum number | Projection of $l$; $m_l = -l, \ldots, +l$ | Ch. 5 |
| $n_r$ | Radial quantum number | Number of radial nodes (excluding origin and infinity) | Ch. 6 |
Shell model orbital notation: $nlj$, where $l$ is given as a spectroscopic letter. Examples: $1s_{1/2}$, $1p_{3/2}$, $1p_{1/2}$, $1d_{5/2}$, $2s_{1/2}$, $1f_{7/2}$, $1g_{9/2}$.
The maximum occupancy of an orbital $j$ is $2j + 1$ nucleons (accounting for the $m_j$ degeneracy, with each $m_j$ value accommodating one proton or one neutron due to the Pauli principle).
G.2.3 Electromagnetic Transition Quantum Numbers
| Symbol | Name | Meaning |
|---|---|---|
| $\lambda$ | Multipolarity | Order of the multipole: $\lambda = 1$ (dipole), $\lambda = 2$ (quadrupole), $\lambda = 3$ (octupole), etc. |
| $E\lambda$ | Electric multipole | Electric transition of order $\lambda$: $E1$, $E2$, $E3$, etc. |
| $M\lambda$ | Magnetic multipole | Magnetic transition of order $\lambda$: $M1$, $M2$, $M3$, etc. |
| $\delta$ | Mixing ratio | Ratio of reduced matrix elements for competing multipolarities, e.g., $\delta(E2/M1)$ |
| $\alpha$ | Internal conversion coefficient | Ratio of conversion electrons to gamma rays: $\alpha = N_e / N_\gamma$ |
G.3 Reaction Notation
G.3.1 Standard Compact Notation
Nuclear reactions are written in the compact form:
$$a(b, c)d$$
where $a$ is the target, $b$ is the projectile, $c$ is the ejectile (light outgoing particle), and $d$ is the residual nucleus. Examples:
| Notation | Reaction | Type |
|---|---|---|
| ${}^{27}$Al(n,$\gamma$)${}^{28}$Al | Neutron capture | Radiative capture |
| ${}^{12}$C($\alpha$,$\gamma$)${}^{16}$O | Helium burning reaction | Radiative capture |
| ${}^{208}$Pb(${}^{48}$Ca, 2n)${}^{254}$No | Heavy-ion fusion-evaporation | SHE synthesis |
| ${}^{d}$(d,p)t | Deuteron-deuteron reaction | Transfer (stripping) |
| ${}^{56}$Fe(p,p')${}^{56}$Fe$^*$ | Inelastic proton scattering | Inelastic |
The prime notation ($p'$, $n'$, $\alpha'$) indicates inelastic scattering where the target is left in an excited state.
G.3.2 Arrow Notation
Equivalently, reactions may be written with an arrow:
$${}^{12}\text{C} + \alpha \rightarrow {}^{16}\text{O} + \gamma$$
This form is more common in astrophysics and particle physics. When the reaction proceeds through a resonance, the intermediate state may be shown:
$$n + {}^{238}\text{U} \rightarrow {}^{239}\text{U}^* \rightarrow \text{fission fragments} + \nu n$$
G.3.3 Common Abbreviations for Reaction Types
| Abbreviation | Meaning |
|---|---|
| (n,$\gamma$) | Neutron capture (radiative) |
| (n,f) | Neutron-induced fission |
| (n,p), (n,$\alpha$) | Neutron-induced charged-particle emission |
| (d,p) | Deuteron stripping (adds a neutron) |
| (p,d) | Proton pickup (removes a neutron) |
| (e,e') | Electron inelastic scattering |
| (p,p') | Proton inelastic scattering |
| ($\gamma$,n) | Photoneutron reaction (photodisintegration) |
| (HI, $x$n) | Heavy-ion fusion-evaporation with $x$ neutrons emitted |
G.4 Common Symbols
| Symbol | Meaning | Units | Where Introduced |
|---|---|---|---|
| $A$ | Mass number (nucleon number) | dimensionless | Ch. 1 |
| $Z$ | Atomic number (proton number) | dimensionless | Ch. 1 |
| $N$ | Neutron number ($N = A - Z$) | dimensionless | Ch. 1 |
| $B(Z,N)$ or $B$ | Binding energy | MeV | Ch. 1, 4 |
| $B/A$ | Binding energy per nucleon | MeV | Ch. 1, 4 |
| $S_n$, $S_p$ | One-neutron, one-proton separation energy | MeV | Ch. 1, 4 |
| $S_{2n}$, $S_{2p}$ | Two-neutron, two-proton separation energy | MeV | Ch. 4, 10 |
| $\Delta$ | Mass excess ($M - A \cdot u$) | keV or MeV | Ch. 2, 4 |
| $Q$ | Reaction or decay $Q$-value | MeV | Ch. 12, 13, 17 |
| $\sigma$ | Cross section | barn (b) | Ch. 1, 17 |
| $d\sigma/d\Omega$ | Differential cross section | b/sr | Ch. 1, 17 |
| $\lambda$ | Decay constant | s$^{-1}$ | Ch. 12 |
| $t_{1/2}$ | Half-life | s (or y, d, h, min) | Ch. 12 |
| $\tau$ | Mean lifetime ($\tau = 1/\lambda$) | s | Ch. 12 |
| $A$ (calligraphic or context) | Activity ($A = \lambda N$) | Bq or Ci | Ch. 12 |
| $\Gamma$ | Total width of a resonance ($\Gamma = \hbar/\tau$) | eV or keV | Ch. 18 |
| $\Gamma_i$ | Partial width for channel $i$ | eV or keV | Ch. 18 |
| $R$ | Nuclear radius | fm | Ch. 1, 2 |
| $r_0$ | Nuclear radius parameter ($R = r_0 A^{1/3}$) | fm ($\approx 1.2$–$1.3$) | Ch. 1, 2 |
| $\rho_0$ | Central nuclear density | fm$^{-3}$ ($\approx 0.16$) | Ch. 2, 25 |
| $a_V, a_S, a_C, a_A, \delta$ | SEMF parameters (volume, surface, Coulomb, asymmetry, pairing) | MeV | Ch. 4 |
| $\mu$ | Magnetic dipole moment | nuclear magnetons ($\mu_N$) | Ch. 2, 9 |
| $Q_0$ | Intrinsic electric quadrupole moment | $e \cdot$b or $e \cdot$fm$^2$ | Ch. 2, 8 |
| $\beta_2$ | Quadrupole deformation parameter | dimensionless | Ch. 8 |
| $\beta_\lambda$ | Deformation parameter of multipolarity $\lambda$ | dimensionless | Ch. 8 |
| $B(E\lambda)$, $B(M\lambda)$ | Reduced transition probability | $e^2$fm$^{2\lambda}$ ($E$) or $\mu_N^2$fm$^{2\lambda-2}$ ($M$) | Ch. 9 |
| $\mathcal{M}$ | Nuclear matrix element | context-dependent | Ch. 14, 32 |
| $f t$ | Comparative half-life (ft-value) | s | Ch. 14 |
| $\log ft$ | Log of the ft-value | dimensionless | Ch. 14 |
| $N_A \langle \sigma v \rangle$ | Thermonuclear reaction rate | cm$^3$mol$^{-1}$s$^{-1}$ | Ch. 21, 22 |
| $k_\text{eff}$ | Effective neutron multiplication factor | dimensionless | Ch. 20, 26 |
| $\varepsilon$ | Binding energy per nucleon (alternative to $B/A$ in some chapters) | MeV | Ch. 25 |
⚠️ Notational collision: The symbol $A$ is used for both mass number and activity. Context always distinguishes them: $A$ as a superscript or subscript on a nuclide symbol is the mass number; $A$ in an equation involving $\lambda N$ or measured in Bq is the activity. Where ambiguity is possible, we write activity as $\mathcal{A}$ or spell it out.
G.5 Greek Letters in Nuclear Physics
| Letter | Common Meaning(s) in This Book |
|---|---|
| $\alpha$ | Alpha particle (${}^4_2$He); also internal conversion coefficient; also fine-structure constant ($\alpha \approx 1/137$) |
| $\beta$ | Beta particle ($\beta^-$ = electron, $\beta^+$ = positron); also velocity ratio $v/c$; also deformation parameter $\beta_\lambda$ |
| $\gamma$ | Gamma ray; also Lorentz factor $(1-\beta^2)^{-1/2}$; also gyromagnetic ratio |
| $\delta$ | Mixing ratio; also pairing term in SEMF; also Dirac delta function; also skin thickness (Fermi distribution) |
| $\varepsilon$ | Electron capture (EC) decay; also small perturbation parameter; also binding energy/nucleon |
| $\eta$ | Sommerfeld parameter ($\eta = z_1 z_2 e^2 / \hbar v$); also asymmetry parameter in fission |
| $\theta$ | Scattering angle (lab or CM, as specified); also mixing angle |
| $\lambda$ | Decay constant; also multipolarity; also wavelength; also de Broglie wavelength |
| $\mu$ | Magnetic moment; also reduced mass $\mu = m_1 m_2 / (m_1 + m_2)$; also linear attenuation coefficient |
| $\nu$ | Neutrino; also frequency |
| $\pi$ | Parity quantum number; also the mathematical constant; also pion |
| $\rho$ | Density (mass or number); also level density |
| $\sigma$ | Cross section; also Pauli spin matrix |
| $\tau$ | Mean lifetime; also isospin (older notation, equivalent to $T$) |
| $\phi$, $\varphi$ | Azimuthal angle; also wave function (in some notations) |
| $\chi$ | Spin wave function (spinor) |
| $\psi$ | Wave function (spatial or total) |
| $\omega$ | Angular frequency; also solid angle (as $d\omega$ or $d\Omega$) |
| $\Gamma$ | Resonance width (total or partial); also gamma function |
| $\Sigma$ | Macroscopic cross section ($\Sigma = N \sigma$); also summation |
| $\Phi$ | Neutron flux; also total wave function |
| $\Omega$ | Solid angle; also projection of $J$ on symmetry axis (Nilsson model) |
G.6 Units and Prefixes
G.6.1 Units Specific to Nuclear Physics
| Unit | Symbol | Definition | Typical Use |
|---|---|---|---|
| Femtometer (fermi) | fm | $10^{-15}$ m | Nuclear radii, distances |
| Barn | b | $10^{-24}$ cm$^2$ = $10^{-28}$ m$^2$ = 100 fm$^2$ | Cross sections |
| Millibarn | mb | $10^{-3}$ b | Reaction cross sections |
| Microbarn | $\mu$b | $10^{-6}$ b | Small cross sections |
| Nanobarn, picobarn | nb, pb | $10^{-9}$ b, $10^{-12}$ b | SHE synthesis, rare processes |
| Electron volt | eV | $1.602 \times 10^{-19}$ J | Energies |
| keV, MeV, GeV | $10^3$, $10^6$, $10^9$ eV | Nuclear energies (keV–MeV); particle physics (GeV) | |
| Atomic mass unit | u (or amu) | $931.494$ MeV/$c^2$ = $1.66054 \times 10^{-27}$ kg | Nuclear masses |
| Nuclear magneton | $\mu_N$ | $e\hbar / 2m_p = 3.152 \times 10^{-8}$ eV/T | Magnetic moments |
| Becquerel | Bq | 1 disintegration/s | Activity (SI) |
| Curie | Ci | $3.7 \times 10^{10}$ Bq | Activity (historical) |
| Gray | Gy | 1 J/kg | Absorbed dose |
| Sievert | Sv | 1 J/kg (weighted) | Equivalent/effective dose |
G.6.2 Natural Units and Conversions
In nuclear physics, the most commonly used "natural" conversion is:
$$\hbar c = 197.327 \;\text{MeV} \cdot \text{fm}$$
This allows quick conversion between energy and length scales. For example, a momentum transfer of $q = 1$ fm$^{-1}$ corresponds to $\hbar c \cdot q = 197$ MeV.
Other useful conversions:
| Relation | Value |
|---|---|
| $\hbar c$ | 197.327 MeV$\cdot$fm |
| $e^2 / 4\pi\epsilon_0 = \alpha \hbar c$ | 1.440 MeV$\cdot$fm |
| $m_p c^2$ | 938.272 MeV |
| $m_n c^2$ | 939.565 MeV |
| $m_e c^2$ | 0.511 MeV |
| 1 u $\cdot c^2$ | 931.494 MeV |
| 1 year | $3.156 \times 10^7$ s |
G.7 Operator Notation
| Notation | Meaning |
|---|---|
| $\hat{O}$ | Operator (hat denotes an operator in Hilbert space) |
| $\hat{H}$ | Hamiltonian operator |
| $\hat{T}$ | Kinetic energy operator; also transition operator (context-dependent) |
| $\hat{V}$ | Potential energy operator |
| $\hat{J}$, $\hat{l}$, $\hat{s}$ | Angular momentum operators |
| $\langle \psi \vert \hat{O} \vert \phi \rangle$ | Matrix element of $\hat{O}$ between states $\vert \phi \rangle$ and $\vert \psi \rangle$ |
| $\langle J' M' \vert \hat{T}^{(\lambda)}_\mu \vert J M \rangle$ | Matrix element of a spherical tensor operator of rank $\lambda$ |
| $\langle J' \Vert \hat{T}^{(\lambda)} \Vert J \rangle$ | Reduced matrix element (Wigner-Eckart theorem) |
| $\vert n l j m_j \rangle$ | Single-particle state ket |
| $\vert J^\pi ; T, T_3 \rangle$ | Nuclear state ket with spin-parity and isospin |
| $(j_1 m_1 j_2 m_2 \vert J M)$ | Clebsch-Gordan coefficient |
| $\begin{pmatrix} j_1 & j_2 & J \\ m_1 & m_2 & -M \end{pmatrix}$ | Wigner 3-$j$ symbol |
| $\begin{Bmatrix} j_1 & j_2 & j_3 \\ j_4 & j_5 & j_6 \end{Bmatrix}$ | Wigner 6-$j$ symbol (Racah coefficient) |
| $a^\dagger$, $a$ | Creation, annihilation operators (second quantization) |
| $c^\dagger_{j m}$, $c_{j m}$ | Nucleon creation, annihilation operators for state $\vert j m \rangle$ |
💡 Convention Note: This textbook uses the Condon-Shortley phase convention for Clebsch-Gordan coefficients and spherical harmonics. The reduced matrix elements follow the convention of Bohr and Mottelson, which differs by a factor of $\sqrt{2J_i + 1}$ from the Rose convention used in some older references. See Chapter 5 for details.
G.8 Abbreviations
| Abbreviation | Full Term | First Appears |
|---|---|---|
| AGB | Asymptotic Giant Branch | Ch. 23 |
| ALARA | As Low As Reasonably Achievable | Ch. 29 |
| AME | Atomic Mass Evaluation | Ch. 2 |
| ARS | Acute Radiation Syndrome | Ch. 16 |
| BBN | Big Bang Nucleosynthesis | Ch. 24 |
| BWR | Boiling Water Reactor | Ch. 26 |
| CEvNS | Coherent Elastic Neutrino-Nucleus Scattering | Ch. 32 |
| CG | Clebsch-Gordan (coefficient) | Ch. 5 |
| CM | Center of Mass (frame) | Ch. 17 |
| CMB | Cosmic Microwave Background | Ch. 24 |
| CNO | Carbon-Nitrogen-Oxygen (cycle) | Ch. 21 |
| DFT | Density Functional Theory | Ch. 7 |
| DWBA | Distorted Wave Born Approximation | Ch. 19 |
| EC | Electron Capture | Ch. 14 |
| EDM | Electric Dipole Moment | Ch. 32 |
| EFT | Effective Field Theory | Ch. 3, 31 |
| ENDF | Evaluated Nuclear Data File | Ch. 35 |
| ENSDF | Evaluated Nuclear Structure Data File | Ch. 35 |
| EOS | Equation of State | Ch. 25 |
| EXFOR | Experimental Nuclear Reaction Data | Ch. 35 |
| FAIR | Facility for Antiproton and Ion Research | Ch. 30 |
| FRIB | Facility for Rare Isotope Beams | Ch. 10, 30 |
| GDR | Giant Dipole Resonance | Ch. 9 |
| GT | Gamow-Teller (transition) | Ch. 14 |
| GW | Gravitational Wave | Ch. 23, 25 |
| HF | Hartree-Fock | Ch. 7 |
| HFB | Hartree-Fock-Bogoliubov | Ch. 7 |
| HI | Heavy Ion | Ch. 11, 30 |
| HO | Harmonic Oscillator | Ch. 6 |
| IBA | Interacting Boson Approximation (or Model) | Ch. 8 |
| ICRP | International Commission on Radiological Protection | Ch. 29 |
| ICF | Inertial Confinement Fusion | Ch. 21 |
| ISOL | Isotope Separation On-Line | Ch. 10, 30 |
| ISOLDE | Isotope Separator On-Line DEvice (CERN) | Ch. 30 |
| LQCD | Lattice Quantum Chromodynamics | Ch. 31 |
| LET | Linear Energy Transfer | Ch. 16 |
| LNT | Linear No-Threshold (model) | Ch. 29 |
| MACS | Maxwellian-Averaged Cross Section | Ch. 23 |
| MCNP | Monte Carlo N-Particle (transport code) | Ch. 16 |
| NIF | National Ignition Facility | Ch. 21 |
| NNDC | National Nuclear Data Center | Ch. 35 |
| NRC | Nuclear Regulatory Commission (U.S.) | Ch. 26 |
| NSE | Nuclear Statistical Equilibrium | Ch. 22 |
| PET | Positron Emission Tomography | Ch. 27 |
| PWR | Pressurized Water Reactor | Ch. 26 |
| QCD | Quantum Chromodynamics | Ch. 3, 31 |
| QED | Quantum Electrodynamics | Ch. 31 |
| QM | Quantum Mechanics | Ch. 5 |
| RIB | Radioactive Ion Beam | Ch. 10, 30 |
| RPA | Random Phase Approximation | Ch. 7 |
| SEMF | Semi-Empirical Mass Formula | Ch. 4 |
| SHE | Superheavy Element | Ch. 11 |
| SMR | Small Modular Reactor | Ch. 26 |
| SPECT | Single-Photon Emission Computed Tomography | Ch. 27 |
| TOV | Tolman-Oppenheimer-Volkoff (equation) | Ch. 25 |
| TVL | Tenth-Value Layer | Ch. 16 |
| WKB | Wentzel-Kramers-Brillouin (approximation) | Ch. 5, 13 |
G.9 A Note on Sign Conventions
Several sign and phase conventions in nuclear physics are not universal. This textbook follows these choices:
-
Isospin projection: $T_3 = (N - Z)/2$, so the neutron has $T_3 = +1/2$ and the proton has $T_3 = -1/2$. This is the convention of most nuclear physics texts (Bohr and Mottelson, Heyde, Krane). The opposite convention ($T_3 = (Z - N)/2$) is standard in particle physics.
-
Mass excess: $\Delta = M - A \cdot u$ in keV, using atomic masses (including electron masses and binding energies). This is the AME convention.
-
$Q$-value: $Q = \sum M_i(\text{initial}) - \sum M_f(\text{final})$, so that $Q > 0$ indicates an exothermic reaction.
-
Binding energy sign: $B > 0$ for bound nuclei. The binding energy is the energy required to disassemble the nucleus, and it is defined as a positive quantity.
-
Reduced matrix elements: We use the Bohr-Mottelson convention: $$\langle J_f M_f | \hat{T}^{(\lambda)}_\mu | J_i M_i \rangle = (-1)^{J_f - M_f} \begin{pmatrix} J_f & \lambda & J_i \\ -M_f & \mu & M_i \end{pmatrix} \langle J_f \| \hat{T}^{(\lambda)} \| J_i \rangle$$
-
Spherical harmonics: We follow the Condon-Shortley phase convention with the factor $(-1)^m$ included in $Y_l^m$.