Nuclei Flashcards

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1
Q

Isotope

A

Same atomic no. (Z), but different mass no. (A)

Eg: ₁H¹ (protium), ₁H² (deuterium), and ₁H³ (tritium) are isotopes of hydrogen

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2
Q

Isobar

A

Same mass no. (A), but different atomic no. (Z)

Eg: ₆C¹⁴, ₇N¹⁴

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3
Q

Isotone

A

Same number of neutrons

Eg: ₁H³, ₂He⁴ (Nₙ=2)

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4
Q

Isomer

A

Same atomic no. and mass no., but different energy levels

Eg: z*Xᴬ, zXᴬ

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5
Q

Average Atomic Mass

A

Aₐᵥ = m₁x₁% + m₂x₂% + m₃x₃% + …

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6
Q

Radius of Nuclei

A

R = Rₒ∛A, Rₒ = 1.2 x 10⁻¹⁵

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7
Q

Density of Nucleus

A

Is constant, regardless the mass no.

ρ = 2.12 x 10¹⁷ kg m⁻³

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8
Q

Mass Defect

A

The difference between the sum of masses of protons and neutrons, and the actual mass of the nucleus
Δm = Zmₚ + (A-Z)mₙ - Mⁿᵘᶜˡᵉᵘˢ

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9
Q

Mass-Energy Conservation in Nuclear Reactions

A

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]

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10
Q

Atomic Mass Unit

A

1 amu = 1 u = 1/12 (m ₆C¹²) ≈ (1.67 x 10⁻²⁷) kg

E ₁ₐₘᵤ = 931.5 MeV

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11
Q

Binding Energy

A

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.
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12
Q

Binding Energy per Nucleus

A

Eʙɴ = Eʙ/A

Eʙɴ ∝ Stability of nucleus

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13
Q

Light and Heavy Nuclei

A

Light Nuclei → A < 30
Heavy Nuclei → A > 170
- Both heavy and light nuclei have low Eʙɴ value, i.e.,
they are unstable

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14
Q

Middle-Mass Nuclei

A

30 > A > 170

- Highly stable nuclei

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15
Q

Most Stable Nuclei

A

Fe⁵⁶, Eʙɴ = 8.75 MeV

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16
Q

Radioctivity

A

The phenomena by which unstable nuclei spontaneously emit particles and/or radiations to attain stability

17
Q

Law of Radioactive Decay

A

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)

18
Q

Half-Life

A

Time taken to reduce the activity or concentration of a radioactive sample to half its initial value
t = 0.693/λ

19
Q

Mean-Life

A

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
20
Q

Activity of a Sample

A

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]
21
Q

Nuclear Force

A

Force between the nucleons which keep them together, overcoming even the electrostatic forces of repulsion between the protons

22
Q

Properties of Nuclear Force

A

(i) Strongest known force
(ii) Short range
(iii) Charge independent
(iv) Shows saturation property
(v) Generally attractive, but can repulsive for very short distances

23
Q

Conclusions from PE vs. Distance Graph for Two Nucleons

A

(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

24
Q

α - Decay

A

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)
25
Q

α - Particle

A
α = ₂He⁴ = He nucleus
m = 4mₚ
q = 2qₚ = 2(+e)