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    Atoms & Nuclei: Comprehensive NEET Physics Formulae

    1. Atoms

    1.1 Rutherford's Nuclear Model

    • Formula for Electrostatic Force:
      F=4πϵ0​1​⋅r2Ze2​
      • Explanation: The force of attraction between the nucleus (charge Ze) and the electron (charge e) is inversely proportional to the square of the distance r between them.
      • Conditions: Assumes point charges and Coulombic interactions.
    • Kinetic Energy of an Electron in Orbit:
      K=21​mv2=8πϵ0​rZe2​
      • Explanation: The kinetic energy is derived from the centripetal force needed to keep the electron in its orbit.
    • Potential Energy of Electron-Nucleus System:
      U=−4πϵ0​rZe2​
      • Explanation: The potential energy is negative, indicating that work is required to separate the electron from the nucleus.
    • Total Energy of an Electron:
      E=K+U=−8πϵ0​rZe2​
      • Explanation: The total energy is the sum of kinetic and potential energy, and it is negative, indicating a bound system.

    Common Mistake: Students often confuse the signs of potential energy and total energy. Remember that potential energy is negative, and total energy is less than zero in a bound system.

    1.2 Bohr’s Model of Hydrogen Atom

    • Quantization of Angular Momentum:
      L=n2πh​
      • Explanation: Angular momentum is quantized and is an integer multiple of 2πh​.
    • Radius of nth Orbit:
      rn​=πme2n2h2ϵ0​​
      • Explanation: The radius increases with the square of the principal quantum number n.
    • Energy of Electron in nth Orbit:
      En​=−n213.6eV​
      • Explanation: Energy levels are quantized and inversely proportional to the square of n.
    • Frequency of Emitted Photon:
      ν=hEi​−Ef​​
      • Explanation: The frequency of the photon emitted during a transition between orbits is related to the energy difference.

    NEET Tip: When calculating energy levels, always ensure that n is correctly identified, as mistakes here can lead to incorrect energy values.


    2. Nuclei

    2.1 Mass-Energy Equivalence

    • Einstein's Mass-Energy Relation:
      E=mc2
      • Explanation: Energy and mass are interchangeable, with c representing the speed of light in vacuum.

    Common Mistake: Confusing the energy units—always ensure that mass is in kilograms and energy in joules for consistent results.

    2.2 Nuclear Binding Energy

    • Binding Energy per Nucleon:
      BE/A=AΔmc2​
      • Explanation: Binding energy per nucleon indicates the stability of a nucleus.
    • Binding Energy:
      BE=Δmc2
      • Explanation: The energy required to disassemble a nucleus into its constituent protons and neutrons.

    NEET Problem-Solving Strategy: Always calculate the mass defect before applying the mass-energy equivalence formula. Incorrect mass defect calculations will lead to wrong binding energy results.

    2.3 Radioactive Decay

    • Decay Law:
      N(t)=N0​e−λt
      • Explanation: The number of undecayed nuclei decreases exponentially over time.
    • Half-Life:
      T1/2​=λln(2)​
      • Explanation: The time required for half the nuclei in a sample to decay.
    • Activity (Rate of Decay):
      A=λN
      • Explanation: The activity of a radioactive substance is proportional to the number of undecayed nuclei.

    Did You Know?: The concept of half-life is crucial in radiocarbon dating, which is used to determine the age of archaeological finds.


    Quick Recap

    • Electrostatic Force: F=4πϵ0​1​⋅r2Ze2​
    • Energy of nth Orbit: En​=−n213.6eV​
    • Mass-Energy Equivalence: E=mc2
    • Radioactive Decay: N(t)=N0​e−λt

    Practice Questions

    1. Calculate the radius of the second orbit in a hydrogen atom using Bohr's model.
    2. Determine the binding energy per nucleon for a nucleus with mass defect Δm=0.03u.
    3. Given a half-life of 10 years, how much of a 100g sample remains after 30 years?

    Solutions:

    1. Using the formula rn​=πme2n2h