Sigma Percentile
JEE Advanced 2025
LEVELJEE Main

Animated Solution for Physics - Atoms and Nuclei: List-I shows various functional dependencies of energy () on the atomic number (). Energies associated with certain phenomena are given in List-II. Choose the option that describes the correct match between the entries in List-I to those in List-II.

List-I

(P)
(Q)
(R)
(S)
is practically independent of

List-II

(1)
energy of characteristic x-rays
(2)
electrostatic part of the nuclear binding energy for stable nuclei with mass numbers in the range 30 to 170
(3)
energy of continuous x-rays
(4)
average nuclear binding energy per nucleon for stable nuclei with mass number in the range 30 to 170
(5)
energy of radiation due to electronic transitions from hydrogen-like atoms

Select Matching Pairs:

PMatches
QMatches
RMatches
SMatches

Visualized Solution

Dependencies

  • Match the energy dependencies with physical phenomena.

  • For H-like atoms, the energy in the -th orbit is given by:
  • eV
  • Thus, the energy of radiation is proportional to .

  • According to Moseley's Law for characteristic X-rays:
  • For -series, , so .
  • Since , we get .

  • Inside a nucleus, the electrostatic repulsion acts between proton pairs.
  • The number of pairs among protons is .
  • Therefore, the electrostatic binding energy is proportional to .

  • The average nuclear binding energy per nucleon () is roughly constant.
  • For stable nuclei with , to MeV.
  • Thus, it is practically independent of .

Final Match

  • Combining all the derived relations:

The Sigma Insight: Bohr's Atomic Model and Energy Levels

Solution Diagram
Imagine you are a detective in the quantum realm. You are handed four mysterious energy dependencies and asked to match them with their physical origins. This is not just a matching exercise; it is a tour through the greatest hits of modern physics! Let's break them down one by one.

Unlocking the First Clue

Bohr's Model
Our first clue is the dependency . Where have we seen this before?
Recall Bohr's model for hydrogen-like atoms. The energy of an electron in the -th orbit is given by the famous equation:
When an electron jumps between energy levels, the energy of the emitted radiation is simply the difference between these levels. Because both levels scale with , the emitted radiation energy also scales with .
Thus, this dependency perfectly describes the energy of radiation due to electronic transitions from hydrogen-like atoms.

The Second Clue

Moseley's Law
Next, we encounter . This specific term is a massive hint.
It points directly to the shielding effect in multi-electron atoms. When we study characteristic X-rays, we rely on Moseley's Law, which states:
For -series X-rays, an electron drops into the innermost shell. The remaining electron in that shell shields the nucleus, making the effective nuclear charge approximately . This means the screening constant .
Since the energy of a photon is $E = h u$, squaring Moseley's equation reveals that the energy of characteristic X-rays is proportional to .

The Third Clue

Inside the Nucleus
Our third dependency is . This looks like a combinatorics problem, and that is exactly what it is!
Inside a nucleus, there are positively charged protons. Every single proton repels every other proton via the Coulomb force.
To find the total electrostatic repulsion, we must count the number of interacting proton pairs. The number of ways to choose 2 protons from a total of is given by:
Therefore, the electrostatic part of the nuclear binding energy scales directly with .

The Final Clue

The Plateau of Stability
Finally, we have an energy that is practically independent of .
Think about the curve of binding energy per nucleon () plotted against the mass number . For very light and very heavy nuclei, this value changes significantly.
However, for stable nuclei with mass numbers in the range of 30 to 170, the curve flattens out into a plateau. In this region, the strong nuclear force saturates, and the average nuclear binding energy per nucleon remains roughly constant at about to MeV.
It does not depend strongly on or , perfectly matching our final clue.

Bringing It All Together

We have successfully decoded all the clues.
The dependency belongs to hydrogen-like atoms. The dependency is the signature of characteristic X-rays. The term arises from proton pair repulsion in the nucleus. And the constant energy represents the stable plateau of binding energy per nucleon.
Final Answer: The correct matching is , , , and .

Similar Questions

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List-I

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(Q)
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(R)
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(B)
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* Multiple Correct Options
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(B)
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(C)
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(D)
Relative change in the angular momenta of two consecutive orbitals varies as
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(A)
(B)
(C)
(D)
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(B)
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(C)
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Highly excited states for hydrogen-like atoms (also called Rydberg states) with nuclear charge Ze are defined by their principle quantum number n, where n>>1. Which of the following statement(s) is (are) true?

* Multiple Correct Options
(A)
Relative change in the radii of two consecutive orbitals does not depend on Z
(B)
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(C)
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(D)
Relative change in the angular momenta of two consecutive orbitals varies as