Nuclear Physics: Nuclei, Radioactivity, and Nuclear Energy

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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.

Last updated 3:52 PM on 10/10/26
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34 Terms

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Atomic Mass Unit (u\text{u})

A standard unit of mass defined as 112th\frac{1}{12}\text{th} of the mass of an unbound carbon-12 (12C^{12}\text{C}) atom, equivalent to 1.660539×10−27 kg1.660539 \times 10^{-27}\,\text{kg} or 931.6 MeV931.6\,\text{MeV}.

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Isotopes

Atomic species of the same chemical element having identical atomic number (ZZ) and electronic structure, but differing mass numbers (AA) and neutron numbers (NN).

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Neutron

A neutral subatomic nucleon discovered by James Chadwick in 1935 with a mass of mn=1.00866 u=1.6749×10−27 kgm_n = 1.00866\,\text{u} = 1.6749 \times 10^{-27}\,\text{kg}, which is stable within the nucleus but unstable as a free particle with a mean life of about 1000 s1000\,\text{s}.

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Isobars

Nuclides of different chemical elements that share the same mass number (AA) but have different atomic numbers (ZZ), such as 13H^3_1\text{H} and 23He^3_2\text{He}.

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Isotones

Nuclides that have the same neutron number (NN) but different atomic numbers (ZZ), such as 80198Hg^{198}_{80}\text{Hg} and 79197Au^{197}_{79}\text{Au}.

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Nuclear Radius

The radius of a nucleus with mass number AA, governed by the relationship R=R0A1/3R = R_0 A^{1/3}, where R0=1.2×10−15 mR_0 = 1.2 \times 10^{-15}\,\text{m}.

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Nuclear Density

The mass density of nuclear matter, which is independent of the mass number AA and is approximately constant across all nuclei at 2.3×1017 kg m−32.3 \times 10^{17}\,\text{kg\,m}^{-3}.

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Mass Defect (ΔM\Delta M)

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\Delta M = [Z m_p + (A - Z) m_n] - M.

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Nuclear Binding Energy (EbE_b)

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.

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Binding Energy per Nucleon (EbnE_{bn})

The ratio of the total nuclear binding energy EbE_b to the mass number AA (Ebn=EbAE_{bn} = \frac{E_b}{A}), serving as a direct measure of nuclear stability.

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<p>Binding Energy per Nucleon Curve</p>

Binding Energy per Nucleon Curve

A plot of EbnE_{bn} versus mass number AA, showing an approximately constant value of 8.5 MeV8.5\,\text{MeV} for intermediate nuclei (30<A<17030 < A < 170) with a maximum of about 8.75 MeV8.75\,\text{MeV} for 56Fe^{56}\text{Fe}, and declining values for both light (A<30A < 30) and heavy (A>170A > 170) nuclei.

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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 0.8 fm0.8\,\text{fm}.

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N/ZN/Z Ratio

The neutron-to-proton ratio required for nuclear stability (1≤NZ≤1.61 \le \frac{N}{Z} \le 1.6), which increases beyond unity in heavier nuclei to counteract electrostatic proton repulsion through additional attractive nuclear forces.

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Radioactivity

A nuclear phenomenon wherein an unstable parent nucleus spontaneously disintegrates by emitting ionizing radiation such as alpha particles, beta particles, or gamma rays.

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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: dNdt=−λN\frac{dN}{dt} = -\lambda N, leading to N(t)=N0e−λtN(t) = N_0 e^{-\lambda t}.

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<p>Radioactive Decay Curve</p>

Radioactive Decay Curve

An exponential decay plot showing the progressive reduction of undecayed nuclei NN over time according to N=N0e−λtN = N_0 e^{-\lambda t}, halving at each successive interval of half-life T1/2T_{1/2}.

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Decay Constant (λ\lambda)

The characteristic proportionality constant or disintegration constant of a radionuclide that represents the decay probability per unit time.

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Activity (RR)

The total disintegration rate of a radioactive sample, defined mathematically as R=−dNdt=λN=R0e−λtR = -\frac{dN}{dt} = \lambda N = R_0 e^{-\lambda t}.

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Becquerel (Bq\text{Bq})

The SI unit of radioactive activity, defined as exactly 11 disintegration or nuclear decay per second.

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Curie (Ci\text{Ci})

A non-SI unit of radioactivity defined as 1 Ci=3.7×1010 decays per second=3.7×1010 Bq1\,\text{Ci} = 3.7 \times 10^{10}\,\text{decays per second} = 3.7 \times 10^{10}\,\text{Bq}.

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Half-Life (T1/2T_{1/2})

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=ln⁡(2)λ=0.693λT_{1/2} = \frac{\ln(2)}{\lambda} = \frac{0.693}{\lambda}.

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Mean Life (τ\tau)

The average lifetime of a radioactive nucleus before disintegrating, defined as τ=1λ\tau = \frac{1}{\lambda} and related to half-life by T1/2=τln⁡(2)T_{1/2} = \tau \ln(2).

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Alpha (α\alpha) Decay

A mode of radioactive disintegration wherein an unstable nucleus ZAX^A_Z\text{X} emits an alpha particle (24He^4_2\text{He}), yielding a daughter nucleus Z−2A−4Y^{A-4}_{Z-2}\text{Y} and positive disintegration energy QQ.

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Beta-Minus (β−\beta^-) Decay

A radioactive process wherein a neutron converts into a proton inside the nucleus, emitting an electron (e−e^-) and an antineutrino (νˉ\bar{\nu}): n→p+e−+νˉn \rightarrow p + e^- + \bar{\nu}.

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Beta-Plus (β+\beta^+) Decay

A radioactive process occurring inside the nucleus where a proton converts into a neutron, emitting a positron (e+e^+) and a neutrino (ν\nu): p→n+e++νp \rightarrow n + e^+ + \nu.

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<p>Gamma ($$\gamma$$) Decay of Cobalt-60 ($$^{60}\text{Co}$$)</p>

Gamma (γ\gamma) Decay of Cobalt-60 (60Co^{60}\text{Co})

A two-step nuclear de-excitation following β−\beta^- decay of 2760Co^{60}_{27}\text{Co}, where the excited 2860Ni^{60}_{28}\text{Ni} daughter nucleus cascades down to its ground state by sequentially emitting two gamma photons of energies Eγ=1.17 MeVE_\gamma = 1.17\,\text{MeV} and Eγ=1.33 MeVE_\gamma = 1.33\,\text{MeV}.

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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^A_Z\text{X} + e^- \rightarrow ^A_{Z-1}\text{Y} + \nu.

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Nuclear Fission

A nuclear reaction wherein a heavy nucleus (such as 92235U^{235}_{92}\text{U}) absorbs a neutron and splits into two intermediate-mass fragments, producing free neutrons and releasing approximately 200 MeV200\,\text{MeV} of energy.

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Moderator

A light-nuclei medium within a nuclear reactor core (such as light water, heavy water D2O\text{D}_2\text{O}, or graphite) used to slow fast fission neutrons down to thermal energies via elastic scattering.

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Multiplication Factor (KK)

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.

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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 KK and control the fission rate.

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<p>Nuclear Reactor</p>

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.

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Thermonuclear Fusion

A nuclear reaction in which two light nuclei combine to form a heavier nucleus at extremely high temperatures (around 109 K10^9\,\text{K}), providing sufficient thermal kinetic energy to overcome electrostatic Coulomb repulsion.

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Proton-Proton (p–pp\text{--}p) Cycle

The multi-step thermonuclear fusion mechanism in the Sun's core where four hydrogen nuclei (11H^1_1\text{H}) combine to form a helium-4 (24He^4_2\text{He}) nucleus, releasing 26.7 MeV26.7\,\text{MeV} of energy.