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Comprehensive vocabulary flashcards covering atomic masses, nuclear structure, mass defect, binding energy, nuclear forces, radioactive decay laws, alpha/beta/gamma decay, nuclear fission reactors, and stellar fusion.
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Atomic Mass Unit (u)
A standard unit of mass defined as 121th of the mass of an unbound carbon-12 (12C) atom, equivalent to 1.660539×10−27kg or 931.6MeV.
Isotopes
Atomic species of the same chemical element having identical atomic number (Z) and electronic structure, but differing mass numbers (A) and neutron numbers (N).
Neutron
A neutral subatomic nucleon discovered by James Chadwick in 1935 with a mass of mn=1.00866u=1.6749×10−27kg, which is stable within the nucleus but unstable as a free particle with a mean life of about 1000s.
Isobars
Nuclides of different chemical elements that share the same mass number (A) but have different atomic numbers (Z), such as 13H and 23He.
Isotones
Nuclides that have the same neutron number (N) but different atomic numbers (Z), such as 80198Hg and 79197Au.
Nuclear Radius
The radius of a nucleus with mass number A, governed by the relationship R=R0A1/3, where R0=1.2×10−15m.
Nuclear Density
The mass density of nuclear matter, which is independent of the mass number A and is approximately constant across all nuclei at 2.3×1017kgm−3.
Mass Defect (ΔM)
The difference between the total combined mass of the constituent protons and neutrons and the actual mass of the bound nucleus, given by ΔM=[Zmp+(A−Z)mn]−M.
Nuclear Binding Energy (Eb)
The total energy released when constituent nucleons assemble into a bound nucleus, or equivalently, the total energy required to completely separate a nucleus into its individual constituent nucleons.
Binding Energy per Nucleon (Ebn)
The ratio of the total nuclear binding energy Eb to the mass number A (Ebn=AEb), serving as a direct measure of nuclear stability.

Binding Energy per Nucleon Curve
A plot of Ebn versus mass number A, showing an approximately constant value of 8.5MeV for intermediate nuclei (30<A<170) with a maximum of about 8.75MeV for 56Fe, and declining values for both light (A<30) and heavy (A>170) nuclei.
Nuclear Force
A short-range, charge-independent attractive force acting equally between nucleons that is substantially stronger than the Coulomb force, falling rapidly to zero beyond a few femtometers and becoming repulsive at separations below approximately 0.8fm.
N/Z Ratio
The neutron-to-proton ratio required for nuclear stability (1≤ZN≤1.6), which increases beyond unity in heavier nuclei to counteract electrostatic proton repulsion through additional attractive nuclear forces.
Radioactivity
A nuclear phenomenon wherein an unstable parent nucleus spontaneously disintegrates by emitting ionizing radiation such as alpha particles, beta particles, or gamma rays.
Law of Radioactive Decay
The physical principle stating that the disintegration rate per unit time is proportional to the total number of undecayed radioactive nuclei present in a sample: dtdN=−λN, leading to N(t)=N0e−λt.

Radioactive Decay Curve
An exponential decay plot showing the progressive reduction of undecayed nuclei N over time according to N=N0e−λt, halving at each successive interval of half-life T1/2.
Decay Constant (λ)
The characteristic proportionality constant or disintegration constant of a radionuclide that represents the decay probability per unit time.
Activity (R)
The total disintegration rate of a radioactive sample, defined mathematically as R=−dtdN=λN=R0e−λt.
Becquerel (Bq)
The SI unit of radioactive activity, defined as exactly 1 disintegration or nuclear decay per second.
Curie (Ci)
A non-SI unit of radioactivity defined as 1Ci=3.7×1010decays per second=3.7×1010Bq.
Half-Life (T1/2)
The duration of time required for the quantity of undecayed radioactive nuclei in a sample to decrease to half of its initial value, given by T1/2=λln(2)=λ0.693.
Mean Life (τ)
The average lifetime of a radioactive nucleus before disintegrating, defined as τ=λ1 and related to half-life by T1/2=τln(2).
Alpha (α) Decay
A mode of radioactive disintegration wherein an unstable nucleus ZAX emits an alpha particle (24He), yielding a daughter nucleus Z−2A−4Y and positive disintegration energy Q.
Beta-Minus (β−) Decay
A radioactive process wherein a neutron converts into a proton inside the nucleus, emitting an electron (e−) and an antineutrino (νˉ): n→p+e−+νˉ.
Beta-Plus (β+) Decay
A radioactive process occurring inside the nucleus where a proton converts into a neutron, emitting a positron (e+) and a neutrino (ν): p→n+e++ν.

Gamma (γ) Decay of Cobalt-60 (60Co)
A two-step nuclear de-excitation following β− decay of 2760Co, where the excited 2860Ni daughter nucleus cascades down to its ground state by sequentially emitting two gamma photons of energies Eγ=1.17MeV and Eγ=1.33MeV.
K-Capture
A nuclear transformation in which a nucleus captures an inner atomic electron (from the K-shell), converting a proton into a neutron with the emission of a neutrino: ZAX+e−→Z−1AY+ν.
Nuclear Fission
A nuclear reaction wherein a heavy nucleus (such as 92235U) absorbs a neutron and splits into two intermediate-mass fragments, producing free neutrons and releasing approximately 200MeV of energy.
Moderator
A light-nuclei medium within a nuclear reactor core (such as light water, heavy water D2O, or graphite) used to slow fast fission neutrons down to thermal energies via elastic scattering.
Multiplication Factor (K)
The ratio of the number of fissions produced by a given generation of neutrons to the number of fissions produced in the preceding generation within a nuclear reactor.
Control Rods
Rods fabricated from neutron-absorbing materials such as cadmium that are inserted or withdrawn from the reactor core to adjust the multiplication factor K and control the fission rate.

Nuclear Reactor
A thermal device engineered to initiate and control a self-sustaining nuclear fission chain reaction, consisting of a fuel core, moderator, control rods, reflector, coolant, and steam generator.
Thermonuclear Fusion
A nuclear reaction in which two light nuclei combine to form a heavier nucleus at extremely high temperatures (around 109K), providing sufficient thermal kinetic energy to overcome electrostatic Coulomb repulsion.
Proton-Proton (p–p) Cycle
The multi-step thermonuclear fusion mechanism in the Sun's core where four hydrogen nuclei (11H) combine to form a helium-4 (24He) nucleus, releasing 26.7MeV of energy.