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Nuclear
Composition
And Properties
Study composition of nucleus, proton, neutron, atomic number, mass number, isotopes, isobars, isotones, nuclear radius, nuclear density and nuclear force.
Understanding what the nucleus is made of — the foundation of nuclear physics.
What is the Nucleus?
The nucleus is the tiny, dense, positively charged core at the centre of an atom. It was discovered by Ernest Rutherford through his famous gold foil experiment (1911).
Key facts about the nucleus:
- The nucleus is composed of two types of particles: protons and neutrons.
- Protons carry a positive electric charge (+e).
- Neutrons are electrically neutral (charge = 0).
- Together, protons and neutrons are called nucleons.
- Nearly the entire mass of the atom is concentrated in the nucleus (>99.9%).
- The nucleus occupies an extremely small fraction of the total atomic volume (radius ≈ 10⁻¹⁵ m vs atomic radius ≈ 10⁻¹⁰ m).
- Electrons revolve around the nucleus in orbits (shells).
- The nucleus is held together by the very strong nuclear force, which overcomes the electrostatic repulsion between protons.
Fig 1.1 — Structure of a typical atom showing nucleus (protons + neutrons) and electrons revolving in shells.
- Atomic radius ≈ 10⁻¹⁰ m | Nuclear radius ≈ 10⁻¹⁵ m
- Nucleus is about 10⁵ times smaller than the atom.
- If the atom were enlarged to the size of a football stadium, the nucleus would be like a tiny pea at the centre.
The positively charged particle inside the nucleus — it defines the identity of an element.
Properties of the Proton
- The proton is a positively charged particle found inside the nucleus.
- It was discovered by Ernest Rutherford in 1919.
- The number of protons in a nucleus is called the atomic number (Z).
- Each element has a unique number of protons — changing the proton count changes the element.
- Protons contribute to both the mass and the charge of the nucleus.
- Protons experience electrostatic repulsion with each other, which is overcome by the nuclear force.
- Symbol: p or 11H (hydrogen nucleus)
The electrically neutral particle inside the nucleus — essential for nuclear stability.
Properties of the Neutron
- The neutron is an electrically neutral particle found inside the nucleus.
- It was discovered by James Chadwick in 1932.
- Neutrons contribute to the mass number (A) but not to the atomic number (Z).
- Neutrons help stabilise the nucleus by adding mass without increasing electrostatic repulsion.
- Free neutrons are unstable and undergo beta decay with a half-life of about 10 minutes.
- Inside a stable nucleus, neutrons remain stable.
- Symbol: n or 10n
mₙ − mₚ ≈ 2.3 × 10⁻³⁰ kg ≈ 1.29 MeV/c²
The two fundamental numbers that describe every nucleus.
Fig 4.1 — Standard nuclear notation showing mass number (A) and atomic number (Z).
Examples
| Nucleus | Symbol | Z (Protons) | A (Mass No.) | N = A−Z (Neutrons) | Nucleons |
|---|---|---|---|---|---|
| Carbon-12 | 126C | 6 | 12 | 12−6 = 6 | 12 |
| Oxygen-16 | 168O | 8 | 16 | 16−8 = 8 | 16 |
| Uranium-235 | 23592U | 92 | 235 | 235−92 = 143 | 235 |
Same element, different masses — isotopes share the same atomic number but differ in neutron count.
Definition
Isotopes are atoms of the same element that have the same atomic number (Z) but different mass numbers (A). They differ only in the number of neutrons in their nuclei.
Examples of Isotopes
| Nucleus | Name | Z | A | N = A−Z | Type |
|---|---|---|---|---|---|
| 11H | Protium | 1 | 1 | 0 | Isotopes of H |
| 21H | Deuterium | 1 | 2 | 1 | |
| 31H | Tritium | 1 | 3 | 2 | |
| 126C | Carbon-12 | 6 | 12 | 6 | Isotopes of C |
| 136C | Carbon-13 | 6 | 13 | 7 | |
| 146C | Carbon-14 | 6 | 14 | 8 | |
| 23592U | Uranium-235 | 92 | 235 | 143 | Isotopes of U |
| 23892U | Uranium-238 | 92 | 238 | 146 |
Same mass number, different elements — isobars are nuclei of different elements with equal A.
Definition
Isobars are atoms of different elements that have the same mass number (A) but different atomic numbers (Z).
Examples of Isobars
| Nucleus | Element | Z | A | N = A−Z | Note |
|---|---|---|---|---|---|
| 4018Ar | Argon | 18 | 40 | 22 | A = 40 (Isobars) |
| 4020Ca | Calcium | 20 | 40 | 20 | |
| 146C | Carbon | 6 | 14 | 8 | A = 14 (Isobars) |
| 147N | Nitrogen | 7 | 14 | 7 | |
| 31H | Tritium | 1 | 3 | 2 | A = 3 (Isobars) |
| 32He | Helium-3 | 2 | 3 | 1 |
Same neutron number, different elements — isotones share the same N = A − Z.
Definition
Isotones are nuclei that have the same number of neutrons (N) but different atomic numbers (Z) and different mass numbers (A). The condition is: N = A − Z = constant.
Examples of Isotones
| Nucleus | A | Z | N = A − Z | Conclusion |
|---|---|---|---|---|
| 146C | 14 | 6 | 14 − 6 = 8 | Isotones (N=8) |
| 157N | 15 | 7 | 15 − 7 = 8 | |
| 3014Si | 30 | 14 | 30 − 14 = 16 | Isotones (N=16) |
| 3115P | 31 | 15 | 31 − 15 = 16 | |
| 3919K | 39 | 19 | 39 − 19 = 20 | Isotones (N=20) |
| 4020Ca | 40 | 20 | 40 − 20 = 20 | |
| 136C | 13 | 6 | 13 − 6 = 7 | Isotones (N=7) |
| 147N | 14 | 7 | 14 − 7 = 7 |
How big is the nucleus? The empirical formula relates nuclear radius to mass number.
Empirical Formula for Nuclear Radius
Experiments show that the nuclear radius depends on mass number A as:
Key Implications
- R ∝ A^(1/3) → nuclear radius is proportional to the cube root of mass number.
- Larger nuclei (higher A) have larger radius, but the growth is slow (cube root).
- Volume V = (4/3)πR³ = (4/3)πR₀³ A → V ∝ A (volume is directly proportional to A).
- R vs A^(1/3) graph is a straight line through origin with slope R₀.
Solved Numericals — Nuclear Radius
▶ View Solution
Given: A = 27, R₀ = 1.2 × 10⁻¹⁵ m
Formula: R = R₀ A^(1/3)
R = 3.6 × 10⁻¹⁵ m = 3.6 fm
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Given: A = 125, R₀ = 1.2 × 10⁻¹⁵ m
R = 6.0 fm
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Formula: R₁/R₂ = (A₁/A₂)^(1/3)
The nucleus with A=64 has twice the radius of the nucleus with A=8.
Ratio of Volumes: V₁/V₂ = (R₁/R₂)³ = (1/2)³ = 1/8 → V₂ = 8 V₁
One of the most remarkable results in nuclear physics — nuclear density is the same for ALL nuclei.
Derivation of Nuclear Density
Let mₙ = mass of a nucleon (approximately same for proton and neutron)
Step 1: Mass of nucleus
Step 2: Volume of nucleus
Step 3: Nuclear density
If a teaspoon of nuclear matter were brought to Earth, it would weigh about one billion tonnes.
NEET/JEE style shortcuts and solved problems using R = R₀A^(1/3).
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R_Cu : R_Al = 4 : 3
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V(Te) : V(Al) = 125 : 27
Note: Volume ∝ A (direct proportion), not A^(1/3)!
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Nuclear radius ≈ 1/28000 of atomic radius
The strongest fundamental force — holds the nucleus together against electrostatic repulsion.
What is Nuclear Force?
The nuclear force (also called the strong nuclear force) is the fundamental force that binds protons and neutrons together inside the nucleus. It acts between all nucleons (proton–proton, neutron–neutron, and proton–neutron pairs).
- It is an extremely strong attractive force at internucleon distances of about 1–2 fm.
- It has a very short range — effective only up to about 1–2 femtometres (fm). Beyond ~3 fm it becomes negligible.
- At very small separations (< 0.5 fm), it becomes strongly repulsive — this prevents the nucleus from collapsing.
- It is charge-independent — the nuclear force between p–p, n–n, and p–n pairs is approximately the same.
- It has saturation property — a nucleon interacts only with its nearest neighbours, not with all nucleons.
- It is spin-dependent and non-central in nature (unlike gravity or electromagnetic force).
Fig 11.1 — Nuclear force (F) vs internucleon distance (r): strongly repulsive at very small r, attractive near 1 fm, negligible beyond 3 fm.
Eight key properties every physics student must know.
1. Strongest Force
Nuclear force is the strongest of all fundamental forces at short ranges. It is about 100 times stronger than the electromagnetic force and 10³⁸ times stronger than gravity at nuclear distances.
2. Short Range Force
It acts only within a very small range of about 1–2 fm. Beyond 3 fm it becomes effectively zero. This is why it does not affect electrons in their orbits.
3. Attractive at Normal Separation
At typical nucleon separations (~1 fm), the nuclear force is strongly attractive, holding the nucleus together against electrostatic repulsion between protons.
4. Repulsive at Very Small Separation
At distances less than about 0.5 fm, the nuclear force becomes strongly repulsive. This prevents the nucleus from collapsing under the attractive force.
5. Charge Independent
The nuclear force between p–p, n–n, and p–n pairs is approximately the same. It does not depend on the electric charge of the nucleons.
6. Saturation Property
Each nucleon interacts with only a limited number of nearest neighbours, not with all nucleons. This is why binding energy per nucleon remains roughly constant for medium and heavy nuclei.
7. Non-Central Nature
The nuclear force is not purely central. It depends on the orientation of nucleon spins relative to the line joining them, unlike gravitational or Coulomb forces.
8. Responsible for Stability
Nuclear force is responsible for the stability of the nucleus. Without it, the nucleus would fly apart due to electrostatic repulsion between protons.
Comparison: Nuclear Force vs Electrostatic Force vs Gravitational Force
| Property | Nuclear Force | Electrostatic Force | Gravitational Force |
|---|---|---|---|
| Range | Short (~2 fm) | Long range (∞) | Long range (∞) |
| Strength | Strongest (1) | ~1/100 of nuclear | Weakest (~10⁻³⁸) |
| Nature | Attractive + Repulsive | Attractive + Repulsive | Always Attractive |
| Charge dependence | Charge-independent | Depends on charge | Independent of charge |
| Acts between | Nucleons only | Charged particles | All massive bodies |
| Carrier particle | Pions (π mesons) | Photons (γ) | Gravitons (theoretical) |
| Saturation | Yes | No | No |
| Non-central? | Yes | No (central) | No (central) |
These five graphs appear directly in CBSE, NEET and JEE exams — study each carefully.
Straight line through origin. Slope = R₀ = 1.2 fm
Straight line through origin. V = (4/3)πR₀³ × A
Constant horizontal line — nuclear density is independent of A.
Nuclear potential energy vs distance — potential well at r₀ ≈ 1 fm.
Each problem includes: Question | Given | Formula | Solution | Final Answer | Exam Tip
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Formula: N = A − Z
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Exam-wise PYQs with complete solutions. Select your exam board below.
📚 CBSE Board Questions
▶ Solution
Mass number (A): The total number of nucleons (protons + neutrons) in a nucleus. A = Z + N.
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Examples: 1H (N=0), 2H (N=1), 3H (N=2) — all have Z=1.
12C (N=6), 14C (N=8) — both have Z=6.
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Example: 4018Ar and 4020Ca — both have A=40, but Z=18 and Z=20 respectively.
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Mass M ≈ Amₙ; Volume V = (4/3)πR³ = (4/3)πR₀³A
ρ = M/V = Amₙ/[(4/3)πR₀³A] = 3mₙ/(4πR₀³)
Since A cancels, ρ is independent of mass number A.
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2. Nature: Nuclear force can be repulsive at very small separations; gravity is always attractive.
3. Strength: Nuclear force is far stronger at nuclear distances; gravity is the weakest force.
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(ii) Nuclear density is independent of A, so ρ₁ = ρ₂ (ratio = 1:1)
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Isotones: Same N, different Z and A. Example: 14C (N=8) and 15N (N=8).
▶ Solution
R(Cu) = 1.2 × (64)^(1/3) = 1.2 × 4 = 4.8 fm
R(Al)/R(Cu) = 3.6/4.8 = 3/4. So R(Cu) is 4/3 times R(Al).
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For Z=11, A=23: N = 23 − 11 = 12 neutrons (this is Sodium-23)
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• For r < r₀ (≈0.8 fm): PE is positive and increases steeply → repulsive region
• At r = r₀ (≈0.8 fm): PE = 0 (equilibrium, force changes sign)
• For r slightly > r₀: PE becomes negative (minimum around 1 fm) → maximum attractive force
• For r > 3 fm: PE → 0 (force negligible)
The minimum of PE corresponds to the equilibrium separation of nucleons.
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∴ R₁ : R₂ = 1 : 2
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2. Nuclear force is charge-independent; electrostatic force depends on charges of particles.
3. Nuclear force is stronger at nuclear distances; electrostatic can be repulsive or attractive.
▶ Solution
For 14C: N = 14−6 = 8
Isotones: 157N (N=8) and 168O (N=8)
▶ Solution
R = R₀ × (8)^(1/3) = R₀ × 2
Given R = 1.2 × 2^(1/3)? Wait — for A=8: R = 1.2 × ∛8 = 1.2 × 2 = 2.4 fm.
So R₀ = R / A^(1/3) = 2.4 / 2 = 1.2 fm ✓
🏥 NEET Questions (40)
(a) 3.6 fm (b) 6.0 fm (c) 7.2 fm (d) 8.4 fm
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Answer: (c) 7.2 fm
(a) More for heavier nuclei (b) Less for heavier nuclei (c) Same for all nuclei (d) Zero for very light nuclei
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Answer: (c) Same for all nuclei
(a) 32S and 40Ar (b) 14C and 14N (c) 14N and 15O (d) 12C and 14C
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(b) ¹⁴C: N=8; ¹⁴N: N=7 → Isobars, not isotones
(c) ¹⁴N: N=7; ¹⁵O: N=7 → Same N=7 → Isotones ✓
(d) ¹²C: N=6; ¹⁴C: N=8 → Isotopes, not isotones
Answer: (c)
(a) 3:5 (b) 5:3 (c) 9:25 (d) 27:125
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Answer: (a) 3:5
(a) Obeys inverse square law (b) Is charge dependent (c) Is short range (d) Is always repulsive
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Answer: (c)
(a) 92 (b) 146 (c) 238 (d) 330
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Answer: (b) 146
(a) 1:2 (b) 2:1 (c) 1:8 (d) 1:4
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Answer: (a) 1:2
(a) 1H, 2H (b) 14C, 14N (c) 12C, 13C (d) 3H, 3He
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(d) ³H (Z=1, A=3) and ³He (Z=2, A=3): same A, different Z → Also isobars
Both b and d are isobars, but (d) is more commonly given as the standard answer.
Answer: (b) and (d) are both correct; typically (d) ³H and ³He
(a) Gravitational force (b) Electrostatic force (c) Nuclear force (d) Magnetic force
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(a) 26 (b) 34 (c) 60 (d) 86
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Answer: (b) 34
(a) Isobars (b) Isotones (c) Isotopes (d) None
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Answer: (c) Isotopes
(a) 1.0 fm (b) 1.2 fm (c) 1.4 fm (d) 1.6 fm
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Answer: (b) 1.2 fm
(a) Isotopes (b) Isobars (c) Isotones (d) Isomers
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(a) 10³ kg/m³ (b) 10¹⁰ kg/m³ (c) 10¹⁷ kg/m³ (d) 10²⁴ kg/m³
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(a) Greater (b) Smaller (c) Equal (d) Zero
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Answer: (c) Equal
(a) 9.1 × 10⁻³¹ kg (b) 1.67 × 10⁻²⁷ kg (c) 1.67 × 10⁻³¹ kg (d) 9.1 × 10⁻²⁷ kg
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(a) 3:5 (b) 5:3 (c) 9:25 (d) 1:1
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Answer: (a) 3:5
(a) 14N (b) 14C (c) 12C (d) 12B
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Answer: (b) 14C
(a) 10⁻¹⁰ m (b) 10⁻¹⁵ m (c) 10⁻² m (d) 10⁻⁷ m
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(a) Same A, different Z (b) Same Z, different A (c) Same N, different Z (d) Same A and Z
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(a) 27:64 (b) 3:4 (c) 9:16 (d) 64:27
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Answer: (a) 27:64
(a) Attractive (b) Repulsive (c) Zero (d) Infinite
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(a) 3:5 (b) 5:3 (c) 25:9 (d) 9:25
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Answer: (b) 5:3
(a) +e (b) −e (c) 0 (d) +2e
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(a) 1.67 × 10⁻²⁷ kg (b) 9.1 × 10⁻³¹ kg (c) 1.67 × 10⁻³¹ kg (d) 3.34 × 10⁻²⁷ kg
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(a) 10² (b) 10²⁰ (c) 10³⁸ (d) 10⁵⁰
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(a) 26 (b) 30 (c) 56 (d) 82
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Answer: (b) 30
(a) Same mass number (b) Same atomic number (c) Same neutron number (d) Same nucleon number
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(a) Inverse square law (b) Acts between neutral particles (c) Can be attractive (d) Long range
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Answer: (b) Acts between neutral particles
(a) −1.6×10⁻¹⁹ C (b) +1.6×10⁻¹⁹ C (c) 0 (d) +3.2×10⁻¹⁹ C
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(a) Nuclear force saturates at some max value (b) Each nucleon interacts only with nearest neighbours (c) Force decreases with time (d) Force is attractive only
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Answer: (a)
(a) F/2 (b) F (c) 2F (d) 0
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Answer: (b) F
(a) Radius of hydrogen nucleus (b) A fundamental constant ≈ 1.2 fm (c) 1 fm (d) Bohr radius
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Answer: (b)
(a) Farad-metre (b) Femtometre (10⁻¹⁵ m) (c) Force-momentum (d) 10⁻¹² m
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(a) 6p, 12n (b) 6p, 6n (c) 12p, 6n (d) 12p, 12n
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Answer: (b) 6p, 6n
(a) 1H (b) 4He (c) 56Fe (d) All are equal
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Answer: (d) All are equal
(a) Isotopes (b) Isobars (c) Isotones (d) Mirror nuclei
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Answer: (b) Isobars
(a) Attractive (b) Zero (c) Repulsive (d) Infinite
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(a) 2 (b) 2^(1/3) (c) 4 (d) 8
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Answer: (b) 2^(1/3) ≈ 1.26 times
⚙️ JEE Main Questions (40)
(a) 27:64 (b) 64:27 (c) 1:1 (d) 3:4
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Answer: (c) 1:1
(a) 7 (b) 36 (c) 65 (d) 58
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Answer: (c) 65 — this is Copper-65 (65Cu)
(a) 2:1 (b) 8:1 (c) 4:1 (d) 1:8
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Answer: (b) 8:1
(a) 79 (b) 118 (c) 197 (d) 276
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Answer: (c) 197
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All three are isotones (N = 8 each)
(a) Linear (b) Yukawa type (exponential decay) (c) Inverse fourth power (d) Constant
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Answer: (b) Yukawa type — exponentially decaying
(a) 15.6 (b) 125/8 (c) 5/2 (d) (5/2)³
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Answer: (b) 125/8 ≈ 15.625
(a) 11 (b) 12 (c) 23 (d) 34
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Answer: (b) 12
(a) A^(2/3) (b) A (c) A^(1/3) (d) A²
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Answer: (a) A^(2/3)
(a) It is short range (b) It obeys inverse square law (c) It is charge independent (d) It is the strongest force at 1 fm
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Answer: (b) — This is the incorrect statement about nuclear force
(a) 1.2 fm (b) 2.4 fm (c) 0.6 fm (d) 3.6 fm
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Answer: (a) 1.2 fm
(a) 26 (b) 30 (c) 56 (d) 0
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Answer: (d) 0
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R₀ ≈ 1.2 fm
(a) Short range (b) Charge independent (c) Repulsive at very short distances (d) Long range
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A_P = A_Q (they are isobars)
(a) 1000 times more (b) Same (c) 10 times more (d) 100 times more
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(a) Z = mass no., A = atomic no. (b) A = mass no., Z = atomic no. (c) A = neutron no., Z = proton no. (d) A = nucleon no., Z = electron no.
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(a) 3:2 (b) 2:3 (c) 3:∛2 (d) ∛(27/8)
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Answer: (a) 3:2
(a) 12C and 13N (b) 14N and 15P (c) 12C and 14C (d) 14N and 14C
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(b) ¹⁴N: N=7; ¹⁵P: N=15−15=0 → No
Answer: (a) ¹²C and ¹³N are isotones (both N=6)
(a) Very large negative (b) Very large positive (c) Zero (d) Moderately positive
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Answer: (b) Very large positive
(a) 0 (b) 1 (c) 2 (d) 3
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Answer: (b) 1
(a) R ∝ A (b) R ∝ A² (c) R ∝ A^(1/3) (d) R ∝ A^(1/2)
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(a) Photons (b) Gluons (c) Pions (π mesons) (d) W bosons
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Answer: (c) Pions (π mesons)
(a) Proton (b) Neutron (c) Electron (d) All nucleons
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Answer: (c) Electron
(a) 1.66 × 10⁻²⁴ kg (b) 1.66 × 10⁻²⁷ kg (c) 1.66 × 10⁻³¹ kg (d) 1.66 × 10⁻¹⁹ kg
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Q: same A=14, different Z → Isobars
R: ¹⁴N has N=7; ¹⁵O has N=15−8=7 → Isotones
P=Isotopes, Q=Isobars, R=Isotones
(a) ρ = 4πR₀³/(3mₙ) (b) ρ = 3mₙ/(4πR₀³) (c) ρ = mₙR₀³ (d) ρ = A/(R₀³)
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A = 64 (e.g., Copper-64 or Zinc-64)
(a) Total number of nucleons (b) Number of protons only (c) Mass number (d) Nuclear density
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Answer: (b) Number of protons only (and consequently neutrons)
(a) Greater than 3 fm (b) About 1 fm (c) Less than about 0.5–0.8 fm (d) Zero
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Q31: R ∝ ? → A^(1/3) | Q32: V ∝ ? → A | Q33: ρ ∝ ? → A⁰ (constant) | Q34: Surface area ∝ ? → A^(2/3) | Q35: Nuclear force range → ~1–2 fm | Q36: Nuclear force type at r=0.5 fm → Repulsive | Q37: Carrier of nuclear force → Pion | Q38: Charge of proton → +1.6×10⁻¹⁹ C | Q39: Charge of neutron → 0 | Q40: mₙ vs mₚ → mₙ slightly > mₚ
▶ Summary Answers
🔬 JEE Advanced Questions (20)
▶ Solution
∴ ρ₁/ρ₂ = 1
ρ₁ : ρ₂ = 1 : 1
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ρ = Amₙ/[(4/3)πR₀³A] = 3mₙ/(4πR₀³)
ρ = 3mₙ/(4πR₀³) ≈ 2.3 × 10¹⁷ kg/m³
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F → 0 exponentially as r → ∞ (force vanishes beyond ~3 fm)
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Same N=16, different Z and A → Isotones
Isotones, both with N=16
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n = 1/3
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Z = 27 (Cobalt), N = 54, A = 81 → ⁸¹Co
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Experimentally, n-p nuclear force is very slightly stronger due to additional exchange forces
F(n-p) ≥ F(n-n) ≈ F(p-p) — approximately equal (charge independent)
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Z = 9 → Fluorine (F); N = 13; A = 22
²²9F — Fluorine-22
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No nuclear force between electron and proton.
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Identical chemical properties (same Z, same electron configuration)
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ρ₂ = ρ (same density)
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Notation: ²⁰⁸82Pb
82 and 126 are nuclear magic numbers (shell model) — extra stability
²⁰⁸82Pb (Doubly Magic Nucleus)
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V₁/V₂ = A₁/A₂ = k³
R₁/R₂ = k; V₁/V₂ = k³
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Nuclear force saturates because of its short range (~1–2 fm); gravity is long range and never saturates.
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Yes, mirror nuclei are isobars (same A, different Z).
Q16: Z=?, Q17: N=?, Q18: R=? (R₀=1.2fm), Q19: density=?, Q20: Is density same as ¹H?
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Z=92, N=146, R≈7.4 fm, ρ≈2.3×10¹⁷ kg/m³, same as ¹H
🌍 IB Physics Questions (15)
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Isotope: Nuclei of the same element (same Z) with different mass numbers (different A/N).
Nuclide: A nucleus characterised by a specific Z and A (e.g., ¹²C is a specific nuclide).
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2. Charge independent (same between p-p, n-n, p-n).
3. Attractive at ~1 fm but repulsive at <0.5 fm.
4. Saturation property — acts only between nearest neighbours.
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ρ = M/V = Amₙ/[(4/3)πR₀³A] = 3mₙ/(4πR₀³) — A cancels → constant ✓
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R(Po) = 2 × 3.6 = 7.2 fm
▶ Solution
Example: ⁴⁰Ar (Z=18) and ⁴⁰Ca (Z=20)
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• r < 0.5 fm: Large positive (repulsive)
• r ≈ 0.8 fm: Force = 0 (equilibrium)
• r ≈ 1–2 fm: Maximum attractive (negative)
• r > 3 fm: Force → 0
See Fig 11.1 in Section 11 for the SVG graph.
▶ Solution
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This enormous difference shows that ordinary matter is mostly empty space — nuclei occupy only a tiny fraction of atomic volume.
▶ Solution
Different: A=1,2,3 and N=0,1,2 respectively — different neutron numbers and mass numbers
▶ Solution
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Symbol: ⁴⁰₂₀Ca
▶ Solution
A ∝ V → A₁/A₂ = 1/27
Volume ratio = 1:27; Mass number ratio = 1:27
🇬🇧 IGCSE Questions (15)
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(b) Mass number A = 17 + 18 = 35 → This is ³⁵Cl (Chlorine-35)
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Difference: Different number of neutrons (6 vs 8), different mass numbers (12 vs 14).
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(b) Neutron: 0 (neutral)
(c) Electron: −e = −1.6 × 10⁻¹⁹ C
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Atomic number (Z): Number of protons in a nucleus (defines the element).
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Different: A (235 vs 238), N (143 vs 146), mass, radioactive properties.
▶ Solution
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📗 ICSE Questions (15)
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Isotopes of Uranium: ²³⁵U (Z=92, N=143) and ²³⁸U (Z=92, N=146)
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2. Mass: neutron is slightly heavier (mₙ = 1.675×10⁻²⁷ kg, mₚ = 1.673×10⁻²⁷ kg).
3. Proton determines atomic number Z; neutron determines extra mass (N).
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³He, ⁴He → both have Z=2 → Isotopes of helium
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Atomic mass = actual mass of atom in u (slightly different from A due to binding energy — mass defect).
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2. Found in the nucleus alongside protons.
3. Mass ≈ 1.675 × 10⁻²⁷ kg (slightly heavier than proton).
4. Free neutron is unstable (half-life ≈ 10 min), but stable inside nucleus.
▶ Solution
🎓 A-Level Questions (15)
▶ Solution
= 5.01×10⁻²⁷ / (4π×1.728×10⁻⁴⁵)
= 5.01×10⁻²⁷ / (2.17×10⁻⁴⁴)
= 2.31×10¹⁷ kg m⁻³ ✓
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2. Nuclear force can be repulsive (at <0.5 fm); gravity is always attractive.
3. Nuclear force is much stronger at nuclear distances (10³⁸ times).
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∴ V = constant × A → V ∝ A ✓
▶ Solution
A = 216
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(b) ²³Na: N=12; ²⁴Mg: N=12 → Isotones
(c) Same Z=8, different A → Isotopes
▶ Solution
▶ Solution
Passage-based questions as per CBSE/NEET pattern — each case has a passage with 4 questions and detailed solutions.
Case Study 1: Nuclear Notation and Composition
Read the passage carefully and answer the questions that follow.
(a) 79 (b) 118 (c) 197 (d) 276
▶ Solution
Answer: (b) 118
(a) 29 (b) 36 (c) 65 (d) 7
▶ Solution
Answer: (c) 65
(a) 1.6×10⁻¹⁹ C (b) 8×1.6×10⁻¹⁹ C (c) 16×1.6×10⁻¹⁹ C (d) 0
▶ Solution
Answer: (b)
(a) Neutron (b) Electron (c) Proton (d) Nucleon
▶ Solution
Answer: (c) Proton
Case Study 2: Isotopes and Their Applications
(a) Mass number (b) Neutron number (c) Atomic number (d) All of the above
▶ Solution
Answer: (c) Atomic number
(a) 6 (b) 8 (c) 14 (d) 20
▶ Solution
Answer: (b) 8
(a) Same A (b) Same Z (c) Same N (d) Same density
▶ Solution
Answer: (b) Same Z
(a) They have different Z (b) They have different N and A (c) Different chemical properties (d) Same electron config
▶ Solution
Answer: (b)
Case Study 3: Isobars and Isotones
(a) ¹²C and ¹³C (b) ¹⁴C and ¹⁴N (c) ¹⁴N and ¹⁵O (d) ³H and ⁴He
▶ Solution
Answer: (b)
▶ Solution
Both have A=40, different Z → Isobars ✓ (they are NOT isotones since N differs)
Verified: isobars with A=40
▶ Solution
N = 7 for both
(a) Isotopes (b) Isobars (c) Isotones (d) None
▶ Solution
Answer: (c) Isotones
Case Study 4: Nuclear Radius and Volume
(a) 2.4 fm (b) 3.6 fm (c) 4.8 fm (d) 7.2 fm
▶ Solution
Answer: (c) 4.8 fm
(a) A^(1/3) (b) A (c) A² (d) A^(2/3)
▶ Solution
Answer: (b) A
(a) 3:5 (b) 5:3 (c) 125:27 (d) 27:125
▶ Solution
Answer: (c) 125:27
(a) 2× (b) 4× (c) 8× (d) 16×
▶ Solution
Answer: (c) 8 times
Case Study 5: Nuclear Density
(a) Mass ∝ A² and Volume ∝ A² (b) Mass ∝ A and Volume ∝ A (c) Density doesn't depend on matter (d) Nuclear force is constant
▶ Solution
Answer: (b)
(a) 10⁷ times (b) 10¹⁰ times (c) 10¹⁴ times (d) 10²⁰ times
▶ Solution
Answer: (c) ≈10¹⁴ times
(a) ρ = 4πR₀³/3mₙ (b) ρ = Amₙ/(4πR₀³) (c) ρ = 3mₙ/(4πR₀³) (d) ρ = A/(R₀³)
▶ Solution
(a) ρ_X > ρ_Y (b) ρ_X < ρ_Y (c) ρ_X = ρ_Y (d) Cannot determine
▶ Solution
Answer: (c) ρ_X = ρ_Y
Case Study 6: Nuclear Force — Nature and Properties
(a) 2–3 fm (b) About 1 fm (c) Less than ~0.8 fm (d) Greater than 3 fm
▶ Solution
(a) Force doesn't depend on charge (b) Nuclear force is the same between any two nucleons (c) Force acts on neutral particles only (d) Charge is not important in nucleus
▶ Solution
(a) 0.5 fm (b) 1 fm (c) 2 fm (d) ~3 fm
▶ Solution
(a) Very large force (b) Force proportional to 1/r² (c) Force → 0 exponentially (d) Constant force
▶ Solution
Answer: (c)
Case Study 7: Identifying Nuclear Relationships
(a) A, B, C (b) A, D, E (c) A, B, D (d) B, C, D
▶ Solution
Answer: (a) A, B, C
(a) F and G (¹⁴C and ¹⁴N) (b) C and D (³H and ³He) (c) Both (a) and (b) (d) None
▶ Solution
Answer: (c) Both
▶ Solution
F(¹⁴C), H(¹⁵N), I(¹⁶O) are isotones with N=8
¹⁴C, ¹⁵N, ¹⁶O are isotones (N=8)
▶ Solution
Answer: (a) Isotopes of Helium
Case Study 8: Nuclear Force vs Electrostatic Force in the Nucleus
(a) 1:100 (b) 100:1 (c) 1:1 (d) 10⁶:1
▶ Solution
(a) More neutrons weaken nuclear force (b) Increasing Coulomb repulsion eventually overcomes nuclear binding (c) Nuclear force decreases with A (d) Electrons enter the nucleus
▶ Solution
(a) Yes (b) No (c) Only at 1 fm (d) Only in excited states
▶ Solution
Answer: (b) No
(a) Coulomb repulsion from protons (b) Only nuclear attractive force (c) Nuclear force from other nucleons (d) No force at all
▶ Solution
Answer: (c)
Case Study 9: Size Comparison — Nucleus vs Atom
(a) 10² (b) 10⁵ (c) 10¹⁰ (d) 10¹⁵
▶ Solution
Answer: (b) 10⁵
(a) The nucleus (b) Protons (c) Empty space (electrons) (d) Neutrons
▶ Solution
Answer: (c) Empty space
▶ Solution
≈ 2.75 fm
(a) (R_nucleus/R_atom)³ = (10⁻⁵)³ = 10⁻¹⁵ (b) 10⁻¹⁰ (c) 10⁻⁵ (d) 50%
▶ Solution
Answer: (a) ~10⁻¹⁵ — nucleus occupies about 10⁻¹⁵ of atomic volume
Case Study 10: Mirror Nuclei and Special Nuclei
(a) Z (b) N (c) A (mass number) (d) Chemical properties
▶ Solution
Answer: (c) Same A (mass number)
(a) Its high mass (b) Both Z and N are magic numbers (c) Its high density (d) Many isotopes
▶ Solution
(a) ¹⁵N (Z=7, N=8) (b) ¹⁶O (Z=8, N=8) (c) ¹⁴N (d) ¹⁶F
▶ Solution
Answer: (a) ¹⁵N
(a) Highly radioactive (b) Unusually unstable (c) Exceptionally stable (d) Has no neutrons
▶ Solution
One-page revision sheet — formulas, concepts, mistakes, and exam tips for NEET/JEE/CBSE.
📐 20 Important Formulas and Facts
1. Nuclear Notation
AZX — A = mass no., Z = atomic no., X = symbol
2. Neutron Number
N = A − Z
3. Nuclear Radius
R = R₀ A^(1/3), R₀ = 1.2 fm
4. Nuclear Volume
V = (4/3)πR₀³ A → V ∝ A
5. Nuclear Density
ρ = 3mₙ/(4πR₀³) ≈ 2.3 × 10¹⁷ kg/m³
6. Radius Ratio
R₁/R₂ = (A₁/A₂)^(1/3)
7. Volume Ratio
V₁/V₂ = A₁/A₂
8. Surface Area Ratio
S₁/S₂ = (A₁/A₂)^(2/3)
9. Proton Charge
q_p = +1.6 × 10⁻¹⁹ C = +e
10. Proton Mass
mₚ = 1.6726 × 10⁻²⁷ kg ≈ 938.3 MeV/c²
11. Neutron Charge
q_n = 0 (neutral)
12. Neutron Mass
mₙ = 1.6749 × 10⁻²⁷ kg ≈ 939.6 MeV/c²
13. 1 fm
1 fm = 1 femtometre = 10⁻¹⁵ m
14. Isotopes
Same Z, different A/N
15. Isobars
Same A, different Z/N
16. Isotones
Same N, different Z/A
17. Nuclear Force Range
~1–2 fm (effective), ~3 fm (cutoff)
18. Find A from R
A = (R/R₀)³
19. Atomic Mass Unit
1 u = 1.66 × 10⁻²⁷ kg = 931.5 MeV/c²
20. Nuclear Charge
Q_nucleus = Ze
💡 20 Key Conceptual Points
1.
Nucleus has protons + neutrons. Electrons are outside.
2.
Proton defines the element (Z = element identity).
3.
Neutron adds mass without charge — helps nuclear stability.
4.
Nuclear density is the SAME for all nuclei — remarkable fact!
5.
Nuclear radius ∝ A^(1/3) but nuclear volume ∝ A (directly).
6.
Isotopes have same chemical properties (same Z = same electrons).
7.
Nuclear force is the strongest force at nuclear distances.
8.
Nuclear force is SHORT range (~1–2 fm).
9.
Nuclear force is CHARGE INDEPENDENT (F_pp ≈ F_nn ≈ F_pn).
10.
Nuclear force is repulsive at r < 0.8 fm — prevents nuclear collapse.
11.
Nuclear force has SATURATION — nucleon interacts with nearest neighbours only.
12.
Electrons are NOT present in the nucleus.
13.
Nuclear radius (10⁻¹⁵ m) vs atomic radius (10⁻¹⁰ m) — ratio 1:10⁵.
14.
Nuclear density ≈ 2.3×10¹⁷ kg/m³ ≈ 10¹⁴ × water density.
15.
Carrier particle of nuclear force = Pion (Yukawa, 1935).
16.
Free neutron is unstable (t₁/₂ ≈ 10 min); in nucleus it is stable.
17.
ρ = constant because V ∝ A and M ∝ A → A cancels in ρ = M/V.
18.
Hydrogen has 3 isotopes: Protium, Deuterium, Tritium.
19.
Magic numbers: 2, 8, 20, 28, 50, 82, 126 — extra nuclear stability.
20.
Nuclear force is NON-CENTRAL — depends on spin orientation.
⚠️ 20 Common Mistakes to Avoid
❌ Mistake 1
Confusing A (mass number) with atomic mass. A = whole number; atomic mass includes binding energy correction.
❌ Mistake 2
Thinking Z = number of neutrons. Z = protons. N = neutrons = A−Z.
❌ Mistake 3
Confusing isotopes (same Z) with isobars (same A) with isotones (same N).
❌ Mistake 4
Writing N = Z − A instead of N = A − Z. Always A minus Z.
❌ Mistake 5
Thinking nuclear density increases with A. It is CONSTANT for all nuclei!
❌ Mistake 6
Confusing R ∝ A^(1/3) with V ∝ A. Radius is cube root; volume is linear in A.
❌ Mistake 7
Thinking nuclear force follows inverse square law. It does NOT — it's Yukawa type.
❌ Mistake 8
Thinking electrons are in the nucleus. They are NOT — they orbit outside.
❌ Mistake 9
Thinking nuclear force is always attractive. It is REPULSIVE at r < 0.8 fm.
❌ Mistake 10
Forgetting to write R₀ = 1.2 fm (not 1.0 fm or 1.5 fm).
❌ Mistake 11
Thinking nuclear force between p-p is stronger than n-n. They are equal (charge independent).
❌ Mistake 12
Confusing mass number A with molar mass (in grams). They are numerically similar but different concepts.
❌ Mistake 13
Thinking isotones have same A. They have same N (not A). ¹⁴C and ¹⁵N are isotones (N=8).
❌ Mistake 14
Volume ratio ≠ radius ratio. V₁/V₂ = A₁/A₂ (not (A₁/A₂)^(1/3)).
❌ Mistake 15
Thinking nuclear force acts on electrons. It doesn't — only between nucleons.
❌ Mistake 16
Using ρ = mₙ/(R₀³) instead of ρ = 3mₙ/(4πR₀³). Include the 4π/3 factor!
❌ Mistake 17
Confusing ¹H (protium) with deuterium (²H). They are different isotopes.
❌ Mistake 18
Writing nuclear notation as AZX (reversed). Correct: AZX.
❌ Mistake 19
Thinking nuclear density is very low (like gas). It is the HIGHEST density in nature — 10¹⁷ kg/m³.
❌ Mistake 20
Forgetting to cube the ratio when finding mass number from radius ratio: A₁/A₂ = (R₁/R₂)³.
🎯 NEET/JEE Exam Tips
- Memorise cube roots: ∛8=2, ∛27=3, ∛64=4, ∛125=5, ∛216=6, ∛1000=10
- Nuclear density ≈ 2.3 × 10¹⁷ kg/m³ — memorise this number
- R₀ = 1.2 fm — memorise this constant
- Iso memory trick: isoTOPES → same TOP(proton/Z) | isoBARS → same BAR(A) | isoTONES → same toNES(N)
- When A doubles: R increases by 2^(1/3) ≈ 1.26; V doubles
- If radius ratio is given, cube it to get mass number ratio
- Nuclear density ALWAYS constant — use this to quickly eliminate wrong options
- Nuclear force: short range, charge-independent, repulsive at very small r
- Surface area ∝ A^(2/3) — this appears in JEE Advanced
- Mirror nuclei are always ISOBARS (same A, Z and N swapped)
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