CBSE Class 12 Physics Chapter 24: Nuclei NCERT Solutions

NCERT Solutions PDF Class 12 PDF

This resource provides detailed NCERT Solutions for Class 12 Physics, Chapter 24, focusing on Nuclei. It covers essential concepts such as the calculation of isotopic abundances based on average atomic mass and the determination of neutron separation energies. The solutions break down complex problems into manageable steps, explaining the underlying principles and formulas. Students will find clear explanations for calculating the relative abundances of magnesium isotopes using their masses and the given average atomic mass. Additionally, the chapter delves into calculating the energy required to remove a neutron from a nucleus, a concept crucial for understanding nuclear stability. These solutions are designed to aid students in grasping these nuclear physics concepts thoroughly and preparing effectively for their board examinations.

Quick info

BoardCBSE
ClassClass 12
SubjectPhysics
Session2026
LanguageEnglish
TypeNCERT Solutions
ChapterChapter 24

Chapter summary

This chapter's NCERT Solutions for Class 12 Physics focus on nuclear properties. It includes exercises on calculating the natural abundances of isotopes given their masses and the average atomic mass, as demonstrated with magnesium isotopes. It also covers the concept of neutron separation energy, providing a method to calculate it using nuclear masses and the conversion factor from atomic mass units to MeV. The solutions offer step-by-step guidance for these calculations, reinforcing understanding of nuclear composition and energy.

Learning outcomes

  • Understand the concept of isotopes and their natural abundance.
  • Calculate the abundances of isotopes using average atomic mass and individual isotope masses.
  • Define and calculate neutron separation energy for a nucleus.
  • Apply mass-defect calculations to determine nuclear binding energies.
  • Relate mass differences to energy released or absorbed in nuclear reactions.

Topics covered

Paper topics

  • Isotopes
  • Average Atomic Mass
  • Natural Abundance
  • Nuclear Masses
  • Neutron Separation Energy
  • Mass Defect
  • Binding Energy
  • Nuclear Reactions

Important topics

  • Calculation of isotopic abundances
  • Concept and calculation of neutron separation energy
  • Relationship between mass and energy in nuclear processes

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Questions and Solutions

Question 13.23

In a periodic table, the average atomic mass of magnesium is given as 24.312 u. The average value is based on their relative natural abundance on Earth. The three isotopes and their masses are $^{24}_{12}$Mg (23.98504 u), $^{25}_{12}$Mg (24.98584 u), and $^{26}_{12}$Mg (25.98259 u). The natural abundance of $^{24}_{12}$Mg is 78.99% by mass. Calculate the abundances of the other two isotopes.
Solution:

We are given the average atomic mass of magnesium and the masses and abundance of its isotopes. We need to find the abundances of the other two isotopes.

Given:

  • Average atomic mass, $m = 24.312$ u
  • Mass of $^{24}_{12}$Mg isotope, $m_1 = 23.98504$ u
  • Mass of $^{25}_{12}$Mg isotope, $m_2 = 24.98584$ u
  • Mass of $^{26}_{12}$Mg isotope, $m_3 = 25.98259$ u
  • Abundance of $^{24}_{12}$Mg, $\eta_1 = 78.99\%$

Let the abundance of $^{25}_{12}$Mg be $x\%$. Then, the abundance of $^{26}_{12}$Mg will be $(100 - 78.99 - x)\% = (21.01 - x)\%$.

The formula for the average atomic mass ($m$) based on the masses ($m_i$) and abundances ($\eta_i$) of isotopes is:

m = \frac{m_1 \eta_1 + m_2 \eta_2 + m_3 \eta_3}{100}

Substituting the given values:

24.312 = \frac{(23.98504 \times 78.99) + (24.98584 \times x) + (25.98259 \times (21.01 - x))}{100}

Multiply both sides by 100:

2431.2 = (23.98504 \times 78.99) + (24.98584 \times x) + (25.98259 \times 21.01) - (25.98259 \times x)

Calculate the products:

2431.2 = 1894.5783096 + 24.98584x + 545.8942159 - 25.98259x

Combine the constant terms and the terms with $x$:

2431.2 = (1894.5783096 + 545.8942159) + (24.98584 - 25.98259)x

2431.2 = 2440.4725255 - 0.99675x

Rearrange the equation to solve for $x$:

0.99675x = 2440.4725255 - 2431.2

0.99675x = 9.2725255

x = \frac{9.2725255}{0.99675} \approx 9.300\%

So, the abundance of $^{25}_{12}$Mg is approximately $9.30\%$.

Now, calculate the abundance of $^{26}_{12}$Mg:

\eta_3 = (21.01 - x)\% = (21.01 - 9.30)\% = 11.71\%

Answer: The abundance of $^{25}_{12}$Mg is approximately 9.30%, and the abundance of $^{26}_{12}$Mg is approximately 11.71%.

Question 13.24

The neutron separation energy is defined as the energy required to remove a neutron from the nucleus. Obtain the neutron separation energies of the nuclei $^{41}_{20}$Ca and $^{27}_{13}$Al from the following data:

$m(^{40}_{20}\text{Ca}) = 39.962591$ u

$m(^{41}_{20}\text{Ca}) = 40.962278$ u

$m(^{26}_{13}\text{Al}) = 25.986895$ u

$m(^{27}_{13}\text{Al}) = 26.981541$ u

Also given: mass of neutron $m_n = 1.008665$ u.

Solution:

The neutron separation energy is the energy required to remove a neutron from a nucleus. This energy is equivalent to the mass defect of the process, converted into energy. The conversion factor is $1$ u $= 931.5$ MeV.

For $^{41}_{20}$Ca:

The process of removing a neutron from $^{41}_{20}$Ca can be represented as:

^{41}_{20}\text{Ca} \longrightarrow ^{40}_{20}\text{Ca} + ^{1}_{0}\text{n}

The masses involved are:

  • Mass of $^{41}_{20}$Ca nucleus, $m(^{41}_{20}\text{Ca}) = 40.962278$ u
  • Mass of $^{40}_{20}$Ca nucleus, $m(^{40}_{20}\text{Ca}) = 39.962591$ u
  • Mass of neutron, $m_n = 1.008665$ u

The mass defect ($\Delta m$) for this reaction is the difference between the mass of the reactants and the mass of the products:

\Delta m = m(^{41}_{20}\text{Ca}) - [m(^{40}_{20}\text{Ca}) + m_n]

\Delta m = 40.962278 \text{ u} - (39.962591 \text{ u} + 1.008665 \text{ u})

\Delta m = 40.962278 \text{ u} - 40.971256 \text{ u}

\Delta m = -0.008978 \text{ u}

The neutron separation energy ($S_n$) is the energy equivalent of this mass defect. Note that the calculation above represents the mass of the initial nucleus minus the mass of the final nucleus and neutron. The energy required to *separate* the neutron is the positive value of this difference if the initial nucleus is heavier, or the energy released if the final products are lighter. In this context, we calculate the energy required to break the nucleus apart.

The energy required to remove the neutron is:

S_n = [m(^{40}_{20}\text{Ca}) + m_n - m(^{41}_{20}\text{Ca})] \times 931.5 \text{ MeV/u}

S_n = [39.962591 \text{ u} + 1.008665 \text{ u} - 40.962278 \text{ u}] \times 931.5 \text{ MeV/u}

S_n = [40.971256 \text{ u} - 40.962278 \text{ u}] \times 931.5 \text{ MeV/u}

S_n = 0.008978 \text{ u} \times 931.5 \text{ MeV/u}

S_n \approx 8.363007 \text{ MeV}

For $^{27}_{13}$Al:

The process of removing a neutron from $^{27}_{13}$Al can be represented as:

^{27}_{13}\text{Al} \longrightarrow ^{26}_{13}\text{Al} + ^{1}_{0}\text{n}

The masses involved are:

  • Mass of $^{27}_{13}$Al nucleus, $m(^{27}_{13}\text{Al}) = 26.981541$ u
  • Mass of $^{26}_{13}$Al nucleus, $m(^{26}_{13}\text{Al}) = 25.986895$ u
  • Mass of neutron, $m_n = 1.008665$ u

The mass defect ($\Delta m$) for this reaction is:

\Delta m = m(^{27}_{13}\text{Al}) - [m(^{26}_{13}\text{Al}) + m_n]

\Delta m = 26.981541 \text{ u} - (25.986895 \text{ u} + 1.008665 \text{ u})

\Delta m = 26.981541 \text{ u} - 26.995560 \text{ u}

\Delta m = -0.014019 \text{ u}

The neutron separation energy ($S_n$) is the energy equivalent of the positive mass difference:

S_n = [m(^{26}_{13}\text{Al}) + m_n - m(^{27}_{13}\text{Al})] \times 931.5 \text{ MeV/u}

S_n = [25.986895 \text{ u} + 1.008665 \text{ u} - 26.981541 \text{ u}] \times 931.5 \text{ MeV/u}

S_n = [26.995560 \text{ u} - 26.981541 \text{ u}] \times 931.5 \text{ MeV/u}

S_n = 0.014019 \text{ u} \times 931.5 \text{ MeV/u}

S_n \approx 13.059 \text{ MeV}

Answer: The neutron separation energy for $^{41}_{20}$Ca is approximately 8.363007 MeV, and for $^{27}_{13}$Al, it is approximately 13.059 MeV.

Common mistakes

  • Errors in algebraic manipulation when solving for unknown abundances.
  • Incorrectly applying the formula for average atomic mass.
  • Using the wrong mass values (e.g., atomic mass instead of nuclear mass) in calculations.
  • Forgetting to convert mass defect to energy using the correct conversion factor (1 u = 931.5 MeV).

Revision tips

  • Review the formula for calculating average atomic mass and practice applying it with different isotope data.
  • Understand the definition of neutron separation energy and how it relates to the masses of the parent and daughter nuclei.
  • Practice converting mass differences (mass defect) into energy using the MeV conversion factor.
  • Ensure all calculations are performed accurately, paying close attention to decimal places and units.

Practice MCQs

Q1. What is the primary factor determining the average atomic mass of an element listed in the periodic table?

Q2. If the natural abundance of $^{24}$Mg is 78.99%, and its mass is 23.98504 u, what does this percentage represent?

Q3. Neutron separation energy is the energy required to:

Q4. The neutron separation energy can be calculated from the mass difference between:

Q5. If $m(^{A}_{Z}X)$ is the mass of a nucleus and $m(^{A-1}_{Z}X)$ is the mass of the daughter nucleus after a neutron is removed, and $m_n$ is the mass of a neutron, the neutron separation energy is approximately:

Frequently asked questions

What is the average atomic mass of magnesium?

The average atomic mass of magnesium is given as 24.312 u. This value is a weighted average based on the relative natural abundances of its isotopes.

How are the abundances of magnesium isotopes calculated?

The abundances are calculated using the formula for average atomic mass, where the average mass is equated to the sum of (isotope mass × abundance) for all isotopes. Given the abundance of one isotope, the abundances of the others can be solved algebraically.

What is neutron separation energy?

Neutron separation energy is defined as the minimum energy required to remove a single neutron from the nucleus of an atom.

How is neutron separation energy determined from nuclear masses?

It is determined by calculating the mass difference between the original nucleus and the resulting nucleus after a neutron is removed, plus the mass of the free neutron. This mass difference (mass defect) is then converted into energy using the conversion factor 1 u = 931.5 MeV.

Which isotopes of magnesium are discussed in this problem?

The isotopes of magnesium discussed are $^{24}_{12}$Mg, $^{25}_{12}$Mg, and $^{26}_{12}$Mg, with their respective masses provided.

What is the significance of the mass defect in calculating separation energy?

The mass defect represents the mass that is converted into energy (or vice versa) during a nuclear process. For neutron separation, the mass defect directly corresponds to the energy required to break the nuclear bond holding that neutron.

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