Nuclear Physics L1: Nucleus Structure & Mass Defect | IIT/NEET Prep

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Nuclear Basics
Nucleons
Key Terminology
Isotope Types
Nuclear Size
Nuclear Density
Mass Energy
Mass Defect
Defect Formula

Nuclear Basics

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Playing Section
  • 1

    Defines the nucleus as the atom's core, holding most of its mass.

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    Introduces the study topics: structure, properties, fission, and fusion.

Basic atomic structure, including the properties of protons, neutrons, and electrons, as well as Rutherford's alpha-scattering experiment.
Einstein's mass-energy equivalence principle (E=mc²) and how mass can be converted into energy.
Familiarity with atomic-scale units of measurement, specifically the atomic mass unit (amu or u) and energy units like electron-volts (eV and MeV).
Coulomb's Law of electrostatic forces to understand the repulsive forces acting between protons within a tight space.
Nuclear Binding Energy and the Binding Energy per Nucleon curve, which determines nuclear stability and why certain elements undergo fission or fusion.
The nature and characteristics of the Strong Nuclear Force that holds nucleons together despite electrostatic repulsion.
Radioactivity and radioactive decay laws, including alpha, beta, and gamma decay processes, half-life, and mean life.
Nuclear Fission and Fusion reactions, including calculation of the Q-value (energy released) in nuclear reactions.
529 views0likes46:03@DIGITALPHYSICSACADEMY-kb5onOriginal Release: 2026-01-07

Mass defect is the difference between the sum of the masses of individual nucleons (protons and neutrons) and the actual mass of the nucleus, occurring because when nucleons combine to form a nucleus, some mass is converted to binding energy according to Einstein's mass-energy equivalence (E=mc²), which holds the nucleus together.