Nuclei Flashcards
Isotope
Same atomic no. (Z), but different mass no. (A)
Eg: ₁H¹ (protium), ₁H² (deuterium), and ₁H³ (tritium) are isotopes of hydrogen
Isobar
Same mass no. (A), but different atomic no. (Z)
Eg: ₆C¹⁴, ₇N¹⁴
Isotone
Same number of neutrons
Eg: ₁H³, ₂He⁴ (Nₙ=2)
Isomer
Same atomic no. and mass no., but different energy levels
Eg: z*Xᴬ, zXᴬ
Average Atomic Mass
Aₐᵥ = m₁x₁% + m₂x₂% + m₃x₃% + …
Radius of Nuclei
R = Rₒ∛A, Rₒ = 1.2 x 10⁻¹⁵
Density of Nucleus
Is constant, regardless the mass no.
ρ = 2.12 x 10¹⁷ kg m⁻³
Mass Defect
The difference between the sum of masses of protons and neutrons, and the actual mass of the nucleus
Δm = Zmₚ + (A-Z)mₙ - Mⁿᵘᶜˡᵉᵘˢ
Mass-Energy Conservation in Nuclear Reactions
A + B ⟶ C + D + Q [Q→Energy released]
Δm = (Mᴀ+Mʙ) - (Mᴄ+Mᴅ)
Q = Δmc² J [Δm in kg]
= 931.5Δm MeV [Δm in amu]
Atomic Mass Unit
1 amu = 1 u = 1/12 (m ₆C¹²) ≈ (1.67 x 10⁻²⁷) kg
E ₁ₐₘᵤ = 931.5 MeV
Binding Energy
Energy lost during formation of a nucleus
OR
Energy supplied to separate nucleons of a nucleus to infinite distances apart
Eʙ = Δmc² J [Δm in kg]
= 931.5Δm MeV [Δm in amu]
- It is the reason for mass defect.
Binding Energy per Nucleus
Eʙɴ = Eʙ/A
Eʙɴ ∝ Stability of nucleus
Light and Heavy Nuclei
Light Nuclei → A < 30
Heavy Nuclei → A > 170
- Both heavy and light nuclei have low Eʙɴ value, i.e.,
they are unstable
Middle-Mass Nuclei
30 > A > 170
- Highly stable nuclei
Most Stable Nuclei
Fe⁵⁶, Eʙɴ = 8.75 MeV