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
Radioctivity
The phenomena by which unstable nuclei spontaneously emit particles and/or radiations to attain stability
Law of Radioactive Decay
The rate of disintegration (dN/dt) at a given time is directly proportional to the number of atoms (i.e., nuclei) present at that time (Nₜ)
(dN/dt) ∝ Nₜ
(dN/dt) = -λNₜ [λ → decay/disintegration constant]
Nₜ = N₀e^(-λt)
Half-Life
Time taken to reduce the activity or concentration of a radioactive sample to half its initial value
t = 0.693/λ
Mean-Life
Time taken to reduce the activity or concentration of a radioactive sample to 1/e its initial value
𝜏 = λ⁻¹
- λ can be defined as the ti
Activity of a Sample
The rate of decay of radioactive nuclei in a sample
Aₜ = λNₜ = A₀e^(-λt) [A₀ = λN₀]
- Units:
(i) 1 Bq = 1 decay s⁻¹ [Bq → Baquerel]
(ii) 1 Cu = 3.7 x 10¹⁰ decay s⁻¹ [Cu → Curie]
Nuclear Force
Force between the nucleons which keep them together, overcoming even the electrostatic forces of repulsion between the protons
Properties of Nuclear Force
(i) Strongest known force
(ii) Short range
(iii) Charge independent
(iv) Shows saturation property
(v) Generally attractive, but can repulsive for very short distances
Conclusions from PE vs. Distance Graph for Two Nucleons
(i) Since PE values are in MeV order, nuclear force is very strong
(ii) Since PE approaches zero in a short fermi distance, nuclear force is short range
(iii) Nuclear force can be repulsive (for very short distances) or attractive
α - Decay
Process by which unstable nuclei emit α-particle in the process of attaining stability
Eg: ₉₂U²³⁸ ⟶ ₉₀Th²³⁴ + ₂He⁴ + Q
- The daughter element formed has A less by 4 and Z less by 2.
- Q value of α - decay is a characteristic of parent nucleus (same nuclei have same value of Q)
α - Particle
α = ₂He⁴ = He nucleus m = 4mₚ q = 2qₚ = 2(+e)