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Class 12 Physics • Comprehensive Chapter Notes
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Chapter 12: Atoms

Dear Class 12 Student! The journey into the heart of matter begins here. Atoms were once thought to be indivisible, solid spheres (Thomson's plum pudding model). But through the elegant scattering experiments of Rutherford and the profound quantum insights of Niels Bohr, we mapped the true structure of the nucleus and orbiting electrons. This chapter is a treasure trove for Boards (derivations & spectral series) and forms the mathematical backbone for JEE Modern Physics. Let's unlock the atom!

1. Alpha-Particle Scattering and Rutherford’s Nuclear Model

In 1911, H. Geiger and E. Marsden, under the direct supervision of Ernest Rutherford, performed the landmark Gold Foil Experiment. They aimed a highly energetic beam of alpha particles ($\text{He}^{2+}$ ions) at an incredibly thin gold foil (thickness $\approx 2.1 \times 10^{-7} \text{ m}$).

[AI Image Placeholder: Landscape (16:9) - Background: #FFFFFF]
AI Prompt: "Detailed schematic of Geiger-Marsden Scattering Experiment. A radioactive source (Bismuth-214) inside a thick lead block emits a beam of alpha particles. The beam passes through lead collimator bricks to become narrow, striking a very thin gold foil in the center. A rotatable circular Zinc Sulfide (ZnS) screen with a microscope surrounds the foil. Rays show most passing straight, some bending slightly, and one or two bouncing drastically backwards. Professional textbook style, white background."

Observations and Revolutionary Conclusions

They observed flashes of light on the Zinc Sulfide (ZnS) screen to track where the alpha particles went. The results shattered classical physics:

Distance of Closest Approach ($r_0$)

Imagine an alpha particle (charge $q_1 = +2e$, mass $m$) fired directly head-on at a gold nucleus (charge $q_2 = +Ze$). As it approaches, the massive electrostatic repulsion slows it down. At the "Distance of Closest Approach" ($r_0$), its velocity becomes zero. Here, its initial Kinetic Energy ($K$) is completely converted into Electrostatic Potential Energy ($U$).

Derivation Using the Law of Conservation of Energy:
Initial Kinetic Energy = Final Potential Energy
$$K = \frac{1}{4\pi\epsilon_0} \frac{q_1 q_2}{r_0}$$
$$K = \frac{1}{4\pi\epsilon_0} \frac{(2e)(Ze)}{r_0}$$
$$r_0 = \frac{1}{4\pi\epsilon_0} \frac{2Ze^2}{K}$$ Significance: This calculation proved that the radius of a nucleus is roughly $10^{-15} \text{ m}$ to $10^{-14} \text{ m}$, which is $10,000$ to $100,000$ times smaller than the radius of the whole atom ($10^{-10} \text{ m}$).
JEE Main Transition: Impact Parameter ($b$) Impact Parameter ($b$): It is defined as the perpendicular distance of the initial velocity vector of the alpha particle from the central axis of the nucleus.
The scattering angle ($\theta$) is deeply related to the impact parameter:
$$b = \frac{1}{4\pi\epsilon_0} \frac{Z e^2 \cot(\theta/2)}{K}$$
Conceptual deductions:
- If $b$ is large, $\cot(\theta/2)$ is large $\implies \theta$ is extremely small (particle grazes past with little deflection).
- If $b = 0$ (head-on collision), $\cot(\theta/2) = 0 \implies \theta = 180^\circ$ (particle rebounds perfectly).

Drawbacks of Rutherford's Model

While correct about the nucleus, Rutherford's model had two fatal flaws regarding electrons:

  1. Atom Instability: According to classical electromagnetic theory (Maxwell), any charged particle undergoing acceleration must continuously radiate electromagnetic energy. An electron orbiting a nucleus is constantly changing direction, hence it is constantly accelerating ($v^2/r$). It should radiate energy, spiral inward, and crash into the nucleus within $10^{-8}$ seconds. Matter shouldn't exist!
  2. Continuous Spectra: If an electron spirals inward, its orbital frequency changes continuously. It should emit a continuous rainbow spectrum of light. In reality, gases like Hydrogen emit highly specific, discrete line spectra.

2. Bohr Model of the Hydrogen Atom

In 1913, Niels Bohr boldly mixed classical mechanics with Max Planck's new quantum theory to save the atom. He proposed three revolutionary postulates.

Bohr's Three Postulates (Must-Know)
  1. Stationary Orbits: An electron in an atom can revolve in certain specific, stable circular orbits without radiating any electromagnetic energy. These are called "Stationary States".
  2. Quantization of Angular Momentum: Out of infinite possible orbits, the electron can only exist in those specific orbits where its orbital angular momentum ($L$) is an exact integral multiple of $\frac{h}{2\pi}$.
    $$L = mvr = \frac{nh}{2\pi}$$ (where $n = 1, 2, 3 \dots$ is the Principal Quantum Number).
  3. Energy Transitions: Energy is absorbed or emitted only when an electron makes a sudden quantum "jump" from one stationary orbit to another. If it jumps from a higher energy state ($E_i$) to a lower state ($E_f$), a single photon is emitted:
    $$h\nu = E_i - E_f$$

A. Derivation of Radius of $n^{th}$ Orbit ($r_n$)

For an electron (mass $m$, charge $e$, velocity $v$) orbiting a nucleus of charge $+Ze$, the required centripetal force is provided exactly by the electrostatic force of attraction:

$$F_c = F_e$$

$$\frac{mv^2}{r} = \frac{1}{4\pi\epsilon_0} \frac{(Ze)(e)}{r^2}$$

$$mv^2 = \frac{Ze^2}{4\pi\epsilon_0 r} \quad \text{--- (Equation 1)}$$

From Bohr's Second Postulate, we extract velocity $v$:
$mvr = \frac{nh}{2\pi} \implies v = \frac{nh}{2\pi mr}$.

Substitute this $v$ into Equation 1:
$$m \left( \frac{nh}{2\pi mr} \right)^2 = \frac{Ze^2}{4\pi\epsilon_0 r}$$
$$\frac{m n^2 h^2}{4\pi^2 m^2 r^2} = \frac{Ze^2}{4\pi\epsilon_0 r}$$
Solving for $r$, we get the radius of the $n^{th}$ orbit:

Radius Formula $$r_n = \frac{n^2 h^2 \epsilon_0}{\pi m Z e^2}$$
Notice that all terms except $n$ and $Z$ are constants. Therefore:
$$r_n \propto \frac{n^2}{Z}$$
For the innermost orbit of Hydrogen ($n=1, Z=1$), substituting the constant values gives the Bohr Radius ($a_0$):
$a_0 = 0.529 \times 10^{-10} \text{ m} = 0.529 \text{ Å}$.

B. Derivation of Velocity of Electron ($v_n$)

Substitute the derived value of $r_n$ back into the angular momentum equation ($v = \frac{nh}{2\pi mr}$):

$$v_n = \frac{nh}{2\pi m \left( \frac{n^2 h^2 \epsilon_0}{\pi m Z e^2} \right)}$$

Velocity Formula $$v_n = \frac{Z e^2}{2 h \epsilon_0 n}$$
$$v_n \propto \frac{Z}{n}$$
For Hydrogen ground state ($n=1, Z=1$), $v_1 \approx 2.18 \times 10^6 \text{ m/s}$. Interestingly, this is roughly $\frac{c}{137}$ (where $c$ is the speed of light).
JEE Main Foundation: Orbit Mechanics 1. Frequency of Revolution ($f$): The number of times the electron goes around the nucleus per second.
$f = \frac{v}{2\pi r}$. Since $v \propto Z/n$ and $r \propto n^2/Z$, we get: $f \propto \frac{Z^2}{n^3}$.

2. Equivalent Orbit Current ($I$): A moving electron constitutes a tiny circular current loop.
$I = \frac{Charge}{Time} = e \times f$. Therefore, $I \propto \frac{Z^2}{n^3}$.

3. Magnetic Moment ($M$): The orbiting electron acts as a tiny magnet. $M = I \times A = (ef)(\pi r^2)$.
Solving this yields $M = \frac{n e h}{4\pi m}$. Thus, $M \propto n$.

3. Energy Levels in Hydrogen Atom

To understand energy transitions, we must find the total energy of the electron in the $n^{th}$ orbit.

The Magic Energy Relation By comparing the expressions for $K$, $U$, and $E$, we establish a vital shortcut relationship used heavily in numerical problems: $$E = -K = \frac{U}{2}$$ Example: If Total Energy $E = -3.4 \text{ eV}$, then Kinetic Energy $K = +3.4 \text{ eV}$ and Potential Energy $U = -6.8 \text{ eV}$.

Now, substituting the radius formula $r_n$ into the Total Energy expression gives us the exact energy for any orbit:

$$E_n = - \frac{m Z^2 e^4}{8 \epsilon_0^2 h^2 n^2}$$

Substituting all the massive constants ($m, e, \epsilon_0, h$) yields the energy in Joules, which we convert to Electron-volts (eV):

Final Energy Level Formula $$E_n = -13.6 \frac{Z^2}{n^2} \text{ eV}$$ The negative sign signifies that the electron is strongly bound to the nucleus. Energy must be supplied from the outside to free the electron.
[AI Image Placeholder: Landscape (16:9) - Background: #FFFFFF]
AI Prompt: "Energy Level Diagram for Hydrogen Atom (Z=1). Draw thick horizontal lines acting like steps. Bottom step is Ground State (n=1) labeled E1 = -13.6 eV. A large gap exists before the next step n=2 (First Excited State) labeled E2 = -3.4 eV. Smaller gap to n=3 labeled E3 = -1.51 eV. Even smaller gap to n=4 labeled E4 = -0.85 eV. The steps bunch up tightly until the top line labeled n=infinity (E=0 eV). Draw vertical downward arrows showing transitions: Lyman series (dropping to n=1), Balmer (dropping to n=2), Paschen (dropping to n=3). Clean educational vector graphic, white background."

Energy Definitions

4. The Line Spectra of Hydrogen Atom

When an excited electron (at orbit $n_2$) spontaneously falls to a lower, more stable orbit ($n_1$), it must shed the excess energy as an electromagnetic photon. The energy of this photon is $\Delta E = E_{n2} - E_{n1}$.

Using the energy formula, $\Delta E = 13.6 Z^2 \left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right) \text{ eV}$.

Converting this to wavelength using $E = \frac{hc}{\lambda}$ yields the empirical Rydberg Formula:

Rydberg Formula $$\frac{1}{\lambda} = R Z^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$$ Where $\frac{1}{\lambda}$ is the wave number ($\bar{\nu}$), and $R$ is the Rydberg Constant.
$R = \frac{me^4}{8\epsilon_0^2 h^3 c} \approx 1.097 \times 10^7 \text{ m}^{-1}$.

Spectral Series of Hydrogen (High Board Priority)

Depending on which lower orbit ($n_1$) the electron ultimately crashes into, the emitted photons fall into distinct named series:

Series Name Final Orbit ($n_1$) Initial Orbit ($n_2$) Electromagnetic Region
Lyman Series $n_1 = 1$ $n_2 = 2, 3, 4, 5 \dots$ Ultraviolet (UV)
Balmer Series $n_1 = 2$ $n_2 = 3, 4, 5, 6 \dots$ Visible Light
Paschen Series $n_1 = 3$ $n_2 = 4, 5, 6, 7 \dots$ Near Infrared (IR)
Brackett Series $n_1 = 4$ $n_2 = 5, 6, 7, 8 \dots$ Mid Infrared (IR)
Pfund Series $n_1 = 5$ $n_2 = 6, 7, 8, 9 \dots$ Far Infrared (IR)
JEE Main Transition: Min & Max Wavelengths Every spectral series has boundaries. For any given series (fixed $n_1$):
1. Longest Wavelength ($\lambda_{max}$) / Minimum Energy:
Occurs for the shortest possible jump. Set $n_2 = n_1 + 1$ (the immediate next orbit).
Example: Balmer $\lambda_{max}$ is for $n=3 \rightarrow n=2$ (called the $H_\alpha$ line).

2. Shortest Wavelength ($\lambda_{min}$) / Series Limit / Maximum Energy:
Occurs for the largest possible jump. Set $n_2 = \infty$.
Here, the formula vastly simplifies: $\frac{1}{\lambda_{min}} = \frac{R Z^2}{n_1^2} \implies \mathbf{\lambda_{min} = \frac{n_1^2}{R Z^2}}$.

5. De Broglie’s Explanation of Bohr’s Second Postulate

Bohr's quantization of angular momentum ($mvr = nh/2\pi$) worked perfectly, but it was essentially a lucky guess—he had no theoretical proof for why it had to be $h/2\pi$. Ten years later, Louis de Broglie provided the brilliant missing link using matter waves.

Concept: De Broglie argued that a revolving electron acts as a wave. For an orbit to be stable (stationary state), the electron wave must not destructively interfere with itself as it goes around. It must form a perfect Standing (Stationary) Wave.

Condition: A standing wave can only form in a circular orbit if the total circumference is an exact integral multiple of the electron's wavelength.

$$2\pi r = n\lambda$$ (where $n = 1, 2, 3 \dots$)

Derivation According to the De Broglie hypothesis, the wavelength of the electron is:
$$\lambda = \frac{h}{p} = \frac{h}{mv}$$
Substitute this $\lambda$ into the standing wave condition:
$$2\pi r = n \left( \frac{h}{mv} \right)$$
Rearranging the terms brings the momentum terms together:
$$mvr = \frac{nh}{2\pi}$$
Significance: This is exactly Bohr's second postulate! De Broglie proved that orbit quantization is a direct, unavoidable consequence of the wave nature of the electron.

6. Limitations of the Bohr Model

While historically monumental, the Bohr model is an incomplete semiclassical model. It eventually gave way to the full Quantum Mechanical Model (Schrödinger). Its flaws are:

Practice Problem 1 Question: The ground state energy of hydrogen atom is $-13.6 \text{ eV}$. What are the kinetic and potential energies of the electron in this state?
Solution:
1. We use the fundamental energy relations: $E = -K = \frac{U}{2}$.
2. Given Total Energy, $E = -13.6 \text{ eV}$.
3. Kinetic Energy $K = -E = -(-13.6 \text{ eV}) = \mathbf{+13.6 \text{ eV}}$.
4. Potential Energy $U = 2E = 2 \times (-13.6 \text{ eV}) = \mathbf{-27.2 \text{ eV}}$.
Practice Problem 2 Question: Calculate the ratio of the wavelengths of the first spectral line of the Lyman series to the first spectral line of the Balmer series in a Hydrogen atom.
Solution:
We use the Rydberg Formula: $\frac{1}{\lambda} = R \left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right)$ (since $Z=1$ for H).

Step 1: First line of Lyman series
Transition is from $n_2 = 2$ to $n_1 = 1$.
$\frac{1}{\lambda_L} = R \left(\frac{1}{1^2} - \frac{1}{2^2}\right) = R \left(1 - \frac{1}{4}\right) = \frac{3R}{4} \implies \lambda_L = \frac{4}{3R}$.

Step 2: First line of Balmer series
Transition is from $n_2 = 3$ to $n_1 = 2$.
$\frac{1}{\lambda_B} = R \left(\frac{1}{2^2} - \frac{1}{3^2}\right) = R \left(\frac{1}{4} - \frac{1}{9}\right) = R \left(\frac{9-4}{36}\right) = \frac{5R}{36} \implies \lambda_B = \frac{36}{5R}$.

Step 3: Calculate Ratio
Ratio = $\frac{\lambda_L}{\lambda_B} = \frac{4/3R}{36/5R} = \frac{4}{3} \times \frac{5}{36} = \frac{20}{108} = \mathbf{\frac{5}{27}}$.