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:

$${}^{99m}\text{Tc}, \quad {}^{137m}\text{Ba}, \quad {}^{178m2}\text{Hf}$$

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:

  1. 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.

  2. Mass excess: $\Delta = M - A \cdot u$ in keV, using atomic masses (including electron masses and binding energies). This is the AME convention.

  3. $Q$-value: $Q = \sum M_i(\text{initial}) - \sum M_f(\text{final})$, so that $Q > 0$ indicates an exothermic reaction.

  4. 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.

  5. Reduced matrix elements: We use the Bohr-Mottelson convention: $$\langle J_f M_f | \hat{T}^{(\lambda)}_\mu | J_i M_i \rangle = (-1)^{J_f - M_f} \begin{pmatrix} J_f & \lambda & J_i \\ -M_f & \mu & M_i \end{pmatrix} \langle J_f \| \hat{T}^{(\lambda)} \| J_i \rangle$$

  6. Spherical harmonics: We follow the Condon-Shortley phase convention with the factor $(-1)^m$ included in $Y_l^m$.