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Atoms And Nuclei JEE Main Physics: Authentic Shift PYQs (2021-2026) with 2.5-Min Shortcut Tricks & Trap Defense

Published: November 01, 2026 Author: NEET & JEE STUDY HUB
🎯 Curriculum & Exam Overview

This chapter explores the quantum nature of matter through Bohr’s atomic model and the binding energy characteristics of atomic nuclei. It carries high weightage because it bridges theoretical quantum concepts with practical energy calculations, appearing frequently in both MCQ and high-order thinking (HOTS) numerical sections.

🚀 NTA JEE Main 2027 Countdown January Session 1 Sprint

JEE Main 2027 Engineering Focus: High-Yield Problem Solving & Negative Marking Defense

  • Session 1 Registration Timeline: Registration for JEE Main 2027 Session 1 opens in November on jeemain.nta.nic.in. January exam performance sets your prime percentile baseline.
  • Negative Marking Safeguard (-1): Eliminate blind guesswork. Prioritize question selection, dimensional checks, and options elimination to maximize net marks.
  • Multi-Concept Problem Linkages: JEE questions integrate multiple domains (e.g. Calculus with Mechanics, or Thermodynamics with Equilibrium) into single composite problems.
  • Timed Shift PYQ Practice: Solve at least 15-20 recent shift questions (2021-2026) under a strict 2.5-minute timer per numerical/MCQ.
⚡ JEE Main Exam Blueprint & Problem-Solving Guidelines
📊 Expected Weightage
Expected 4 to 8 marks in CBSE board exam (typically 1-2 MCQs + 1 Short/Long Answer or Case Study).
✍️ Examiner & Scoring Insight
Examiners award partial step marks for formula definition, intermediate substitution, correct SI units, and neat labeled diagrams.

1. ⚡ High-Speed Formula Sheet & Concept Limits

1
Bohr’s Postulates: Electrons revolve in stationary orbits with quantized angular momentum L = nh/2Ï€.
2
Binding Energy per Nucleon: The average energy required to separate a nucleus into its constituent nucleons, determining nuclear stability.
3
Nuclear Force Properties: Short-range, strong, charge-independent forces that act between nucleons to overcome electrostatic repulsion.
⚡ High-Yield Formula & Reaction Sheet
  • 1/λ = R(1/n₁² - 1/n₂²): Rydberg formula where R is the Rydberg constant and λ is the emitted photon wavelength.
  • BE = [Zmₚ + (A-Z)mâ‚™ - M]c²: Binding energy formula where Z is proton count, A is mass number, and M is nuclear mass.
⚠️ Common Board Trap Alert
Students frequently confuse the sign of energy levels (negative sign denotes a bound state) and often forget to convert Atomic Mass Units (u) into MeV/c² when calculating binding energy, leading to massive magnitude errors.
📺 High-yield video lesson for this chapter will premiere on @qbnexa_official.
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3. ⚡ NTA JEE Shift Practice & Rank-Booster Problems

Question 1 • MCQ 🔥 MHT CET (2026)
4 Mark(s)
If 'E' and 'L' denote the magnitude of total energy and angular momentum of revolving electron in $n^{th}$ Bohr orbit then
(A) $E \propto L$
(B) $E \propto L^{-1}$
(C) $E \propto L^{-2}$
(D) $E \propto L^{2}$
🚀 View Fast Shortcut Solution & Trap Defense

Correct Answer: (c)

Explanation: For an electron in the $n^{\text{th}}$ Bohr orbit, the angular momentum is quantised as $ L = \frac{nh}{2\pi} $ So, $ L \propto n $ Now, the total energy of an electron in the $n^{\text{th}}$ Bohr orbit is $ E_n = -\frac{13.6}{n^2} \text{ eV} $ Since the question asks for the magnitude of total energy, $ E = |E_n| = \frac{13.6}{n^2} $ So, $ E \propto \frac{1}{n^2} $ But $L \propto n$, so $n \propto L$. Hence, $ E \propto \frac{1}{L^2} $ $ E \propto L^{-2} $ So the correct option is: $ \boxed{\text{Option C } \; E \propto L^{-2}} $

Question 2 • MCQ 🔥 AP EAPCET (2025)
4 Mark(s)
The ratio of the time periods of the revolution of the electrons in the second and third excited states of hydrogen atom is
(A) $9: 16$
(B) $27: 64$
(C) $4: 9$
(D) $8: 27$
🚀 View Fast Shortcut Solution & Trap Defense

Correct Answer: (b)

Explanation: $T \propto n^3$ $ \frac{T_2}{T_3}=\left(\frac{n_2}{n_3}\right)^3 $ For the second excited state, $n_2=3$ For the third excited state, $n_3=4$ $ \begin{array}{ll} \therefore & \frac{T_2}{T_3}=\left(\frac{3}{4}\right)^3=\frac{27}{64} \\ \Rightarrow & T_2: T_3=27: 64 \end{array} $

Question 3 • MCQ 🔥 AP EAPCET (2024)
4 Mark(s)
The speed of the electron in a hydrogen atom in the $n=3$ level is (Planck's constant $=6.6 \times 10^{-34} \mathrm{Js}$ )
(A) $62 \times 10^5 \mathrm{~ms}^{-1}$
(B) $3.7 \times 10^5 \mathrm{~ms}^{-1}$
(C) $7.3 \times 10^5 \mathrm{~ms}^{-1}$
(D) $1.6 \times 10^5 \mathrm{~ms}^{-1}$
🚀 View Fast Shortcut Solution & Trap Defense

Correct Answer: (c)

Explanation: To calculate the speed of the electron in a hydrogen atom when it is in the $ n=3 $ energy level, we use the formula: $ v_n = \frac{e^2}{2 \varepsilon_0 h n} $ where: $ e = 1.6 \times 10^{-19} \mathrm{C} $ is the charge of the electron, $ \varepsilon_0 = 8.85 \times 10^{-12} \mathrm{F/m} $ is the permittivity of free space, $ h = 6.64 \times 10^{-34} \mathrm{Js} $ is Planck's constant, and $ n = 3 $ is the principal quantum number for the energy level. Substituting these values into the formula, we calculate: $ v_3 = \frac{(1.6 \times 10^{-19})^2}{2 \times 8.85 \times 10^{-12} \times 6.64 \times 10^{-34} \times 3} $ Simplifying this, we find: $ v_3 \approx 0.0073 \times 10^8 \mathrm{~m/s} $ Thus, the speed of the electron in the $ n=3 $ level is: $ v_3 = 7.3 \times 10^5 \mathrm{~m/s} $

Question 4 • MCQ 🔥 MHT CET (2020)
4 Mark(s)
The ratio of energies of photons produced due to transition of electron of hydrogen atom from its (i) second to first energy level and (ii) highest energy level to second level is respectively
(A) $2.5: 1$
(B) $3: 1$
(C) $2: 1$
(D) $4: 1$
🚀 View Fast Shortcut Solution & Trap Defense

Correct Answer: (b)

Explanation: The energy of photons is given by $E=R h c\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right)$ where, $R$ is Rydberg constant, $h$ is Planck's constant and $c$ is the speed of light. (i) Energy of photon produced from second to first energy level, $\begin{aligned} & E_1=R h c\left(\frac{1}{1^2}-\frac{1}{2^2}\right) \\ & E_1=\frac{3}{4} R h c \end{aligned}$ (ii) Energy of photon produced from highest energy level (i.e., $\infty$) to second level, $\begin{aligned} & E_2=R h c\left(\frac{1}{2^2}-\frac{1}{\infty}\right)=\frac{1}{4} R h c \\ \therefore \quad & \frac{E_1}{E_2}=\frac{\frac{3}{4} R h c}{\frac{1}{4} R h c}=\frac{3}{1} \text { or } 3: 1 \end{aligned}$

Question 5 • MCQ 🔥 JEE Main (2007)
4 Mark(s)
In gamma ray emission from a nucleus
(A) only the proton number changes
(B) both the neutron number and the proton number change
(C) there is no change in the proton number and the neutron number
(D) only the neutron number changes
🚀 View Fast Shortcut Solution & Trap Defense

Correct Answer: (c)

Explanation: There is no change in the proton number and the neutron number as the $\gamma$ -emission takes place as a result of excitation or de-excitation of nuclei. $\gamma$ -rays have no charge or mass.

4. ❓ Frequently Asked Questions (Exam Strategy)

❓ How many questions appear from Atoms And Nuclei JEE Main Physics: Authentic Shift PYQs (2021-2026) with 2.5-Min Shortcut Tricks & Trap Defense in JEE Main Session 1?
Typically 1 to 2 questions (4 to 8 marks) appear from Atoms And Nuclei JEE Main Physics: Authentic Shift PYQs (2021-2026) with 2.5-Min Shortcut Tricks & Trap Defense, frequently featuring combined multi-topic concepts.
❓ What is the best approach to avoid negative marks in Atoms And Nuclei JEE Main Physics: Authentic Shift PYQs (2021-2026) with 2.5-Min Shortcut Tricks & Trap Defense?
Master standard shortcut formulas, verify boundary states (e.g. t=0, infinity), and skip uncertain numerical value questions.
❓ Why are nuclear forces considered charge-independent?
Experimental evidence shows that nuclear forces between proton-proton, neutron-neutron, and proton-neutron pairs are approximately equal. This indicates the force depends solely on the distance between nucleons, not their charge.
❓ What happens to the total energy of an electron when it jumps to a higher orbit?
The electron absorbs a photon and its total energy increases by the energy difference between the two orbits. However, its kinetic energy decreases while its potential energy becomes less negative.
❓ Does the mass of a nucleus equal the sum of the masses of its individual nucleons?
No, the actual mass of the nucleus is always less than the sum of the individual masses of protons and neutrons. This 'mass defect' is converted into binding energy as per Einstein’s mass-energy equivalence principle.
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