Comprehensive Study Notes on Radioactivity and Modern Physics

Structure of the Atom and Nucleus

  • Historical Discovery and Foundation:

    • The structure of the atom and nucleus was established towards the end of the nineteenth century following the discovery of electrons by Sir J.J. Thomson and alpha particle scattering experiments performed by Rutherford and others.

  • Atomic Constituents:

    • An atom consists of three primary subatomic particles: electrons, protons, and neutrons.

    • Protons and neutrons reside inside the centrally located nucleus.

    • Electrons revolve around the nucleus in specific paths called stationary orbits (or stationary shells).

    • Electrons moving in stationary orbits do not radiate energy. Every stationary shell corresponds to a definite electron energy level.

  • Electron Shell Configuration:

    • The total number of shells in an atom depends on its total electron count, with each shell having a strict capacity limit.

    • The maximum number of electrons a shell can accommodate is given by the formula 2n22n^2, where nn represents the shell number.

    • Shell designations, corresponding values of nn, and their maximum electron capacities are:

      • n=1n = 1: K shell, maximum 22 electrons

      • n=2n = 2: L shell, maximum 88 electrons

      • n=3n = 3: M shell, maximum 1818 electrons

      • n=4n = 4: N shell, maximum 3232 electrons

      • n=5n = 5: O shell, maximum 5050 electrons

      • n=6n = 6: P shell, maximum 7272 electrons

      • n=7n = 7: Q shell, maximum 9898 electrons

    • Electron energy increases progressively as the shell number nn increases.

  • Dimensions of Atom and Nucleus:

    • The overall size of an atom is determined by the radius of its outermost electron shell and is of the order of 10−10 m10^{-10}\,\text{m}.

    • The nucleus is positioned at the center of the atom with a size of the order of 10−15 m10^{-15}\,\text{m} to 10−14 m10^{-14}\,\text{m} (which is 10−510^{-5} to 10−410^{-4} times the overall size of the atom).

  • Properties of Subatomic Particles:

    • Electron:

      • Symbol: ee

      • Charge: −1.6×10−19 C-1.6 \times 10^{-19}\,\text{C} (or −e-e)

      • Mass: 9.1×10−31 kg9.1 \times 10^{-31}\,\text{kg}, which is approximately 11840\frac{1}{1840} times the mass of a proton.

    • Proton:

      • Symbol: pp

      • Charge: +1.6×10−19 C+1.6 \times 10^{-19}\,\text{C} (or +e+e)

      • Mass: 1.67×10−27 kg1.67 \times 10^{-27}\,\text{kg} (more precisely mp=1.6726×10−27 kgm_p = 1.6726 \times 10^{-27}\,\text{kg}).

    • Neutron:

      • Symbol: nn

      • Charge: Zero (electrically neutral particle)

      • Mass: 1.67×10−27 kg1.67 \times 10^{-27}\,\text{kg} (more precisely mn=1.6749×10−27 kgm_n = 1.6749 \times 10^{-27}\,\text{kg}).

  • Nucleons, Atomic Mass, and Charge:

    • Protons and neutrons, being the main constituent particles of the nucleus, are collectively termed nucleons.

    • Atomic Number (ZZ): The number of protons in the nucleus of an atom. In a neutral atom, it is equal to the number of orbital electrons. It determines the position of the element in the periodic table.

      • Atomic Number (Z)=number of protons in the nucleus\text{Atomic Number } (Z) = \text{number of protons in the nucleus}

    • Mass Number (AA): The total number of nucleons (protons plus neutrons) in the nucleus.

      • Mass Number (A)=number of protons+number of neutrons\text{Mass Number } (A) = \text{number of protons} + \text{number of neutrons}

    • Nuclear Charge and Mass:

      • The nucleus carries a total positive charge of +Ze+Ze.

      • The mass of the nucleus is approximately equal to the mass of a proton or neutron multiplied by mass number AA.

      • Because the mass of an electron is negligible relative to protons or neutrons, the total mass of an atom is considered identical to the mass of its nucleus.

  • Atomic Symbol Specification and Models:

    • An atom is specified symbolically as ZAX{}_Z^A \text{X}, where X\text{X} is the chemical symbol of the element.

    • For any specified nuclide ZAX{}_Z^A \text{X}:

      • Number of electrons=Z\text{Number of electrons} = Z

      • Number of protons=Z\text{Number of protons} = Z

      • Number of neutrons=A−Z\text{Number of neutrons} = A - Z

    • Specific Atomic Examples:

      • Hydrogen (11H{}_1^1 \text{H}): Lightest atom; A=1A = 1, Z=1Z = 1. Nucleus contains 11 proton and 00 neutrons; 11 electron revolves in the K shell.

      • Helium (24He{}_2^4 \text{He}): A=4A = 4, Z=2Z = 2. Nucleus contains 22 protons and 22 neutrons (A−Z=4−2=2A - Z = 4 - 2 = 2); 22 electrons revolve in the K shell.

      • Sodium (1123Na{}_{11}^{23} \text{Na}): A=23A = 23, Z=11Z = 11. Nucleus contains 1111 protons and 1212 neutrons (23−11=1223 - 11 = 12); 1111 electrons distributed as 22 in K shell, 88 in L shell, and 11 in M shell.

      • Strontium Observation: A single atom of Strontium trapped in an electric field has been photographed. Its nucleus contains 3838 protons, and its atomic diameter measures a few millionths of a millimeter.

Chemical versus Nuclear Changes

  • Fundamental Mechanisms:

    • Chemical Change: Occurs at low energy and involves changes only in the number or configuration of orbital electrons.

    • Nuclear Change: Occurs at high energy and involves changes in the number of nucleons inside the atomic nucleus.

  • Energy Requirements:

    • A chemical change requires low energy, on the order of a few eV\text{eV}.

    • A nuclear change requires significantly higher energy, on the order of a few MeV\text{MeV}.

    • The energy required for a nuclear change is approximately 10610^6 times higher than that required for a chemical change.

  • Conservation Laws in Nuclear Reactions:

    • Both Atomic Number (ZZ) and Mass Number (AA) are strictly conserved during nuclear reactions.

    • ∑Zreactants=∑Zproducts\sum Z_{\text{reactants}} = \sum Z_{\text{products}}

    • ∑Areactants=∑Aproducts\sum A_{\text{reactants}} = \sum A_{\text{products}}

Classification of Nuclides

  • Isotopes:

    • Definition: Atoms of the same element having the same atomic number ZZ but different mass numbers AA.

    • Properties: Isotopes occupy the exact same position in the periodic table. They possess the same number of protons (ZZ) and orbital electrons (ZZ), giving them identical chemical properties, but contain different numbers of neutrons (A−ZA - Z).

    • Abundance: Different isotopes of an element occur in varying proportions in nature. Usually, one isotope has a dominant relative abundance, and the element is commonly specified by the mass number of that most abundant isotope.

    • Examples of Isotopes:

      • Hydrogen: Protium (11H{}_1^1 \text{H}, ordinary hydrogen; 11 proton, 00 neutrons), Deuterium (12H{}_1^2 \text{H} or H\text{H}, heavy hydrogen; 11 proton, 11 neutron), and Tritium (13H{}_1^3 \text{H}; 11 proton, 22 neutrons). Each has 11 orbital electron.

      • Carbon: 612C{}_6^{12} \text{C}, 613C{}_6^{13} \text{C}, and 614C{}_6^{14} \text{C}. Each contains 66 protons and 66 electrons. 612C{}_6^{12} \text{C} (most abundant) has 66 neutrons, 613C{}_6^{13} \text{C} has 77 neutrons, and 614C{}_6^{14} \text{C} has 88 neutrons.

      • Chlorine: 1735Cl{}_{17}^{35} \text{Cl} and 1737Cl{}_{17}^{37} \text{Cl}, existing in nature in a relative abundance ratio of 3:13 : 1. Each has 1717 protons and 1717 electrons; 1735Cl{}_{17}^{35} \text{Cl} contains 1818 neutrons, while 1737Cl{}_{17}^{37} \text{Cl} contains 2020 neutrons.

    • Types of Isotopes:

      • Stable Isotopes: Possess a neutron count nearly equal to their proton count (N≈ZN \approx Z).

      • Unstable or Radioactive Isotopes (Radioisotopes): Possess a neutron count significantly greater than their proton count (N≫ZN \gg Z), driving them to undergo spontaneous radioactive decay. Used extensively in medical and industrial applications.

      • Examples of Radioisotopes: 92235U{}_{92}^{235} \text{U} (9292 protons, 143143 neutrons) and 92238U{}_{92}^{238} \text{U} (9292 protons, 146146 neutrons); 614C{}_6^{14} \text{C} is also a radioisotope.

    • Note: Tin (Sn\text{Sn}) possesses the largest number of isotopes (1010 isotopes).

  • Isobars:

    • Definition: Atoms of different elements having the same mass number AA but different atomic numbers ZZ.

    • Properties: Isobars contain the same total number of nucleons (AA), but different numbers of protons (ZZ), neutrons (A−ZA - Z), and orbital electrons (ZZ). Consequently, they exhibit different chemical properties.

    • Examples of Isobars:

      • 1123Na{}_{11}^{23} \text{Na} (1111 protons, 1212 neutrons, 1111 electrons) and 1223Mg{}_{12}^{23} \text{Mg} (1212 protons, 1111 neutrons, 1212 electrons). Total nucleons = 2323 each.

      • 614C{}_6^{14} \text{C} (66 protons, 88 neutrons, 66 electrons) and 714N{}_7^{14} \text{N} (77 protons, 77 neutrons, 77 electrons). Total nucleons = 1414 each.

    • Mirror Isobars: Isobars in which the numeric values of protons and neutrons are mutually interchanged, such as 1123Na{}_{11}^{23} \text{Na} (1111 p, 1212 n) and 1223Mg{}_{12}^{23} \text{Mg} (1212 p, 1111 n).

  • Isotones:

    • Definition: Atoms having different numbers of protons (ZZ) and different mass numbers (AA), but the exact same number of neutrons (A−ZA - Z).

    • Properties: They belong to different elements and have different numbers of electrons.

    • Examples of Isotones:

      • 1123Na{}_{11}^{23} \text{Na} (1111 protons) and 1224Mg{}_{12}^{24} \text{Mg} (1212 protons): Each contains exactly 1212 neutrons (23−11=1223 - 11 = 12 and 24−12=1224 - 12 = 12).

      • 1939K{}_{19}^{39} \text{K} (1919 protons) and 2040Ca{}_{20}^{40} \text{Ca} (2020 protons): Each contains exactly 2020 neutrons (39−19=2039 - 19 = 20 and 40−20=2040 - 20 = 20).

  • Summary Comparison of Nuclide Classifications:

    • Isotope: Atomic Number ZZ is Same; Mass Number AA is Different; Neutron Count A−ZA - Z is Different.

    • Isobar: Atomic Number ZZ is Different; Mass Number AA is Same; Neutron Count A−ZA - Z is Different.

    • Isotone: Atomic Number ZZ is Different; Mass Number AA is Different; Neutron Count A−ZA - Z is Same.

Fundamentals of Radioactivity

  • Discovery and History:

    • Discovered by Henry Becquerel in 1896.

    • Becquerel wrapped a uranium salt in black paper and placed it on a photographic plate inside a dark room. Upon later inspection, the photographic plate was found to be exposed.

    • Subsequent tests with other uranium salts yielded identical results, confirming that uranium and its salts spontaneously emit invisible radiations capable of penetrating paper, glass, or wood. These emissions were initially termed Becquerel rays.

  • Definitions:

    • Radioactive Substances: Substances that disintegrate or decay by the spontaneous emission of radiation. Examples include uranium, radium, polonium, thorium, and actinium.

    • Natural Radioactivity: Isotopes of nearly all elements with atomic numbers higher than 8282 (elements positioned after lead in the periodic table) are naturally radioactive because their nuclei contain a massive excess of neutrons over protons.

  • Radioactivity as a Nuclear Phenomenon:

    • Radioactivity is purely a nuclear process; it is the spontaneous emission of α\alpha, β\beta, or γ\gamma radiations from atomic nuclei during their disintegration.

    • Proof of Nuclear Origin: No external physical change (such as variations in pressure or temperature) or chemical change (such as extreme heating, freezing, application of strong electric/magnetic fields, chemical reagents, or oxidation) alters either the nature of the radiation emitted or the rate of decay. Because orbital electrons are easily perturbed by such treatments without altering radiation properties, radioactivity cannot be attributed to orbital electrons.

  • Random Nature of Decay:

    • In any radioactive sample containing a large number of atoms, it is impossible to predict precisely when or which individual nucleus will decay at any given moment.

    • Radioactive decay is fundamentally a random phenomenon governed by no deterministic law predicting individual nuclear disintegrations.

Radiation Analysis and Properties

  • Rutherford's Magnetic Field Experiment (1903):

    • Rutherford analyzed emissions from a radioactive sample placed inside a lead box by subjecting them to a magnetic field oriented perpendicular to their path (directed perpendicularly into the plane of the paper).

    • The emissions separated into three distinct components:

      • Alpha (α\alpha) particles: Deflected to the left (determined by Fleming's left-hand rule), indicating positive electric charge.

      • Beta (β\beta) particles: Deflected to the right, indicating negative electric charge. Beta particles exhibit significantly greater trajectory curvature/deflection than alpha particles.

      • Gamma (γ\gamma) radiations: Deflected zero degrees, passing straight through. This confirms they are uncharged neutral electromagnetic waves similar to light.

  • Electric Field Deflection Experiment:

    • When radioactive emissions pass through an electric field perpendicular to their direction of flight:

      • Alpha (α\alpha) particles: Curve toward the negative plate, confirming positive charge.

      • Beta (β\beta) particles: Curve toward the positive plate, confirming negative charge. Beta particles undergo greater deflection than alpha particles.

      • Gamma (γ\gamma) radiations: Pass completely undeviated, confirming neutrality.

  • Properties of Alpha (α\alpha) Particles:

    • An alpha particle consists of 22 protons and 22 neutrons bound together.

    • It is identical to a doubly ionised helium atom (He2+\text{He}^{2+}), which is a helium nucleus that has lost both of its orbital electrons.

    • Represented symbolically as 24He{}_2^4 \text{He} or He2+\text{He}^{2+}.