Chapter 2: Structure of Atom
2.1 Discovery of Subatomic Particles
Discovery of Electron — Cathode Ray Experiment (J.J. Thomson, 1897)
When a high voltage is applied across a cathode ray discharge tube at very low pressure (~0.001 mm Hg), a stream of particles moves from the cathode to the anode. These are called cathode rays.
Properties of Cathode Rays:
- Travel in straight lines
- Consist of negatively charged particles (electrons)
- Independent of the material of the cathode or gas in the tube
- Possess kinetic energy and can rotate a paddle wheel
Charge-to-mass ratio of electron (J.J. Thomson):
\[ \frac{e}{m_e} = 1.758820 \times 10^{11};\text{C/kg} \]
Charge of electron (R.A. Millikan — Oil Drop Experiment):
\[ e = 1.6022 \times 10^{-19};\text{C} \]
Mass of electron:
\[ m_e = 9.1094 \times 10^{-31};\text{kg} \]
Discovery of Proton — Anode Rays (Canal Rays)
When a perforated cathode is used in a discharge tube, a stream of positively charged particles moves towards the cathode. These are anode rays or canal rays.
Properties:
- The charge-to-mass ratio depends on the gas in the tube
- The lightest particles are obtained with hydrogen → protons
\[ m_p = 1.6726 \times 10^{-27};\text{kg}, \quad e_p = +1.6022 \times 10^{-19};\text{C} \]
Discovery of Neutron (James Chadwick, 1932)
Chadwick bombarded beryllium with α-particles and observed the emission of electrically neutral particles with a mass slightly greater than that of protons — neutrons.
\[ {}^{9}_{4}\text{Be} + {}^{4}_{2}\text{He} \rightarrow {}^{12}_{6}\text{C} + {}^{1}_{0}\text{n} \]
\[ m_n = 1.6750 \times 10^{-27};\text{kg} \]
| Particle | Symbol | Charge (C) | Mass (kg) | Mass (u) |
|---|---|---|---|---|
| Electron | \(e^-\) | \(-1.6022 \times 10^{-19}\) | \(9.109 \times 10^{-31}\) | 0.00055 |
| Proton | \(p^+\) | \(+1.6022 \times 10^{-19}\) | \(1.6726 \times 10^{-27}\) | 1.00727 |
| Neutron | \(n^0\) | 0 | \(1.6750 \times 10^{-27}\) | 1.00866 |
2.2 Atomic Number, Mass Number, Isotopes, and Isobars
Atomic number (Z) = Number of protons = Number of electrons (in a neutral atom)
Mass number (A) = Number of protons + Number of neutrons
\[ A = Z + \text{number of neutrons} \]
Notation: \( {}^{A}_{Z}\text{X} \), e.g., \( {}^{12}_{6}\text{C} \), \( {}^{23}_{11}\text{Na} \)
| Term | Definition | Example |
|---|---|---|
| Isotopes | Same Z, different A | \({}^{1}_{1}\text{H}\), \({}^{2}_{1}\text{H}\), \({}^{3}_{1}\text{H}\) |
| Isobars | Same A, different Z | \({}^{40}_{18}\text{Ar}\), \({}^{40}_{19}\text{K}\), \({}^{40}_{20}\text{Ca}\) |
| Isotones | Same number of neutrons | \({}^{14}_{6}\text{C}\), \({}^{15}_{7}\text{N}\) (both have 8 neutrons) |
2.3 Thomson’s Model of Atom (1904)
J.J. Thomson proposed the “plum pudding” model: the atom is a sphere of positive charge in which electrons are embedded, like plums in a pudding.
Limitation: Could not explain the results of Rutherford’s scattering experiment.
2.4 Rutherford’s Nuclear Model (1911)
The α-Particle Scattering Experiment
Rutherford bombarded a thin gold foil (0.0004 cm thick) with α-particles from a radioactive source.
Observations:
- Most α-particles passed through undeflected → atom is mostly empty space
- A small fraction was deflected by small angles → positive charge is concentrated
- Very few (~1 in 20,000) bounced back → the positive charge occupies a very small volume (nucleus)
Rutherford’s Conclusions:
- The atom has a tiny, dense, positively charged centre called the nucleus (radius ~ \(10^{-15}\) m)
- Nearly all mass is concentrated in the nucleus
- Electrons revolve around the nucleus in circular orbits
- The atom is mostly empty space (radius ~ \(10^{-10}\) m)
Limitations:
- Could not explain the stability of atoms (accelerating charged particles should radiate energy and spiral into the nucleus)
- Could not explain line spectra of atoms
2.5 Bohr’s Model of the Hydrogen Atom (1913)
Niels Bohr proposed a model for hydrogen-like atoms based on quantum ideas:
Postulates
-
Electrons revolve in fixed circular orbits (called stationary states or shells) without radiating energy.
-
Quantized angular momentum: The angular momentum of an electron in a stationary state is an integral multiple of \(\frac{h}{2\pi}\):
\[ m_e v r = n \frac{h}{2\pi}, \quad n = 1, 2, 3, \ldots \]
- Energy transitions: When an electron jumps from a higher orbit (\(n_2\)) to a lower orbit (\(n_1\)), energy is emitted as a photon:
\[ \Delta E = E_{n_2} - E_{n_1} = h\nu \]
Key Results for Hydrogen-like Species
Radius of \(n\)-th orbit:
\[ r_n = \frac{n^2 a_0}{Z} \]
where \( a_0 = 52.9;\text{pm} \) (Bohr radius), \(Z\) = atomic number.
Energy of \(n\)-th orbit:
\[ E_n = -\frac{13.6,Z^2}{n^2};\text{eV} = -\frac{2.18 \times 10^{-18},Z^2}{n^2};\text{J} \]
Velocity of electron:
\[ v_n = \frac{2.18 \times 10^6 , Z}{n};\text{m/s} \]
Hydrogen Spectrum
When excited hydrogen atoms return to lower energy levels, they emit photons of specific wavelengths, producing line spectra.
\[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \]
where \( R_H = 1.097 \times 10^7;\text{m}^{-1} \) (Rydberg constant)
| Series | \(n_1\) | \(n_2\) | Region |
|---|---|---|---|
| Lyman | 1 | 2, 3, 4, … | Ultraviolet |
| Balmer | 2 | 3, 4, 5, … | Visible |
| Paschen | 3 | 4, 5, 6, … | Infrared |
| Brackett | 4 | 5, 6, 7, … | Infrared |
| Pfund | 5 | 6, 7, 8, … | Far infrared |
Limitations of Bohr’s Model:
- Works only for hydrogen-like (one-electron) species
- Could not explain the fine structure of spectral lines
- Could not explain the Zeeman effect or Stark effect
- Does not account for electron-electron repulsion in multi-electron atoms
2.6 Dual Nature of Matter and Radiation
Wave-Particle Duality
Light exhibits both wave and particle nature:
- Wave nature: Diffraction, interference
- Particle nature: Photoelectric effect, black-body radiation
Planck’s quantum theory:
\[ E = h\nu = \frac{hc}{\lambda} \]
where \( h = 6.626 \times 10^{-34};\text{J·s} \) (Planck’s constant)
Photoelectric effect (Einstein):
\[ h\nu = h\nu_0 + \frac{1}{2}m_e v^2 \]
where \( \nu_0 \) = threshold frequency
de Broglie Relation
Louis de Broglie (1924) proposed that matter also has a dual nature:
\[ \lambda = \frac{h}{mv} = \frac{h}{p} \]
where \( \lambda \) = wavelength, \( m \) = mass, \( v \) = velocity, \( p \) = momentum.
Note: The wave nature is significant only for microscopic particles (electrons, protons) and negligible for macroscopic objects.
2.7 Heisenberg’s Uncertainty Principle
\[ \Delta x \cdot \Delta p \geq \frac{h}{4\pi} \]
or equivalently:
\[ \Delta x \cdot m\Delta v \geq \frac{h}{4\pi} \]
It is impossible to simultaneously determine the exact position and exact momentum of an electron. This principle makes the concept of fixed orbits (Bohr model) meaningless.
2.8 Quantum Mechanical Model of the Atom
Schrödinger Wave Equation
\[ \hat{H}\psi = E\psi \]
The full time-independent equation:
\[ \frac{\partial^2 \psi}{\partial x^2} + \frac{\partial^2 \psi}{\partial y^2} + \frac{\partial^2 \psi}{\partial z^2} + \frac{8\pi^2 m}{h^2}(E - V)\psi = 0 \]
- \(\psi\) = wave function
- \(|\psi|^2\) = probability density of finding the electron
- \(E\) = total energy
- \(V\) = potential energy
Quantum Numbers
Each electron in an atom is described by a set of four quantum numbers:
| Quantum Number | Symbol | Values | Describes |
|---|---|---|---|
| Principal | \(n\) | 1, 2, 3, … | Shell (energy level), size of orbital |
| Azimuthal | \(l\) | 0 to \(n-1\) | Subshell (shape of orbital) |
| Magnetic | \(m_l\) | \(-l\) to \(+l\) | Orientation of orbital in space |
| Spin | \(m_s\) | \(+\frac{1}{2}\) or \(-\frac{1}{2}\) | Spin of electron |
Subshell notation:
| \(l\) | 0 | 1 | 2 | 3 |
|---|---|---|---|---|
| Subshell | s | p | d | f |
| No. of orbitals | 1 | 3 | 5 | 7 |
| Max. electrons | 2 | 6 | 10 | 14 |
2.9 Shapes of Orbitals
s Orbitals (\(l = 0\)) — Spherical
- Spherically symmetric
- Node at nucleus for \(n \geq 2\) (radial node)
- Number of radial nodes = \(n - l - 1\)
p Orbitals (\(l = 1\)) — Dumbbell shaped
- Each p orbital has two lobes with a nodal plane at the nucleus
- Three p orbitals are oriented along x, y, and z axes (mutually perpendicular)
d Orbitals (\(l = 2\)) — Cloverleaf shapes
There are five d orbitals: \(d_{xy}\), \(d_{yz}\), \(d_{xz}\), \(d_{x^2-y^2}\), \(d_{z^2}\).
- \(d_{xy}\), \(d_{yz}\), \(d_{xz}\): four lobes between the axes
- \(d_{x^2-y^2}\): four lobes along x and y axes
- \(d_{z^2}\): two lobes along z-axis with a doughnut-shaped ring in the xy plane
2.10 Rules for Filling Electrons in Orbitals
1. Aufbau Principle
Electrons fill orbitals in order of increasing energy (\(n + l\) rule). If \(n + l\) values are equal, the orbital with the lower \(n\) fills first.
Energy order:
\[ 1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p < 5s < 4d < 5p < 6s < 4f \ldots \]
2. Pauli’s Exclusion Principle
No two electrons in an atom can have the same set of four quantum numbers. Consequently, each orbital can hold a maximum of 2 electrons with opposite spins.
3. Hund’s Rule of Maximum Multiplicity
Electrons are distributed among orbitals of a subshell in such a way as to give the maximum number of unpaired electrons with parallel spins. Pairing occurs only after all degenerate orbitals are singly occupied.
2.11 Electronic Configuration of Atoms
The electronic configuration is written as: \(nl^x\), where \(n\) = principal quantum number, \(l\) = subshell, \(x\) = number of electrons.
| Element | Z | Electronic Configuration |
|---|---|---|
| H | 1 | \(1s^1\) |
| He | 2 | \(1s^2\) |
| Li | 3 | \([He],2s^1\) |
| C | 6 | \([He],2s^2,2p^2\) |
| N | 7 | \([He],2s^2,2p^3\) |
| O | 8 | \([He],2s^2,2p^4\) |
| Ne | 10 | \([He],2s^2,2p^6\) |
| Na | 11 | \([Ne],3s^1\) |
| Ar | 18 | \([Ne],3s^2,3p^6\) |
| K | 19 | \([Ar],4s^1\) |
| Ca | 20 | \([Ar],4s^2\) |
| Fe | 26 | \([Ar],3d^6,4s^2\) |
| Cu | 29 | \([Ar],3d^{10},4s^1\) ★ |
| Cr | 24 | \([Ar],3d^5,4s^1\) ★ |
| Zn | 30 | \([Ar],3d^{10},4s^2\) |
★ Anomalous configurations: Cr and Cu achieve extra stability from half-filled (\(d^5\)) and completely filled (\(d^{10}\)) d-subshells respectively.
Stability of Half-filled and Completely Filled Subshells
Two factors contribute:
- Symmetrical distribution of electrons → lower energy
- Exchange energy — electrons with parallel spins in degenerate orbitals can exchange positions, releasing energy. More exchanges → greater stability.
Practice Questions
Multiple Choice Questions (MCQs)
1. The number of angular nodes for a 4d orbital is:
(a) 1
(b) 2
(c) 3
(d) 4
2. Which of the following sets of quantum numbers is NOT possible?
(a) \(n = 2,\ l = 1,\ m_l = 0,\ m_s = +\frac{1}{2}\)
(b) \(n = 3,\ l = 2,\ m_l = -2,\ m_s = -\frac{1}{2}\)
(c) \(n = 2,\ l = 2,\ m_l = 0,\ m_s = +\frac{1}{2}\)
(d) \(n = 4,\ l = 0,\ m_l = 0,\ m_s = -\frac{1}{2}\)
3. If uncertainty in position of an electron is zero, the uncertainty in its momentum would be:
(a) zero
(b) \(\geq \frac{h}{4\pi}\)
(c) \(\lt \frac{h}{4\pi}\)
(d) infinite
4. The wavelength of a ball of mass 100 g moving with a velocity of 100 m/s is (\(h = 6.6 \times 10^{-34}\) J·s):
(a) \(6.6 \times 10^{-35}\) m
(b) \(6.6 \times 10^{-34}\) m
(c) \(6.6 \times 10^{-33}\) m
(d) \(6.6 \times 10^{-32}\) m
5. The electronic configuration of Cu (Z = 29) is:
(a) \([Ar],3d^9,4s^2\)
(b) \([Ar],3d^{10},4s^1\)
(c) \([Ar],3d^{10},4s^2\)
(d) \([Ar],3d^8,4s^2,4p^1\)
Short Answer Questions (2–3 Marks)
6. Calculate the wavelength of an electron moving with a velocity of \(2.05 \times 10^7\) m/s.
7. Write the electronic configuration of Fe²⁺ and Fe³⁺ ions. Which one is more stable and why?
8. What is the maximum number of electrons that can have the quantum numbers \(n = 3\), \(l = 2\)?
9. State Heisenberg’s uncertainty principle. Why is it significant for microscopic particles but not for macroscopic objects?
10. Write the four quantum numbers for the last electron of sodium (Z = 11).
Long Answer Questions (5 Marks)
11. (a) Explain the Bohr model of hydrogen atom. Derive the expression for the radius and energy of the \(n\)-th orbit.
(b) Calculate the wavelength of the first line in the Balmer series of hydrogen spectrum.
12. (a) Draw the shapes of the five d orbitals. How do \(d_{z^2}\) and \(d_{x^2-y^2}\) differ from the other three d orbitals?
(b) Explain why Cr has the electronic configuration \([Ar],3d^5,4s^1\) and not \([Ar],3d^4,4s^2\).
13. (a) State and explain the photoelectric effect. How did it provide evidence for the particle nature of light?
(b) A photon of wavelength 4 × 10⁻⁷ m strikes a metal surface, the work function of the metal being 2.13 eV. Calculate the kinetic energy and velocity of the emitted photoelectron.
Assertion-Reason Questions
14. Assertion (A): The energy of 2s orbital is less than that of 2p orbital in multi-electron atoms.
Reason (R): 2s electrons have greater penetration power than 2p electrons.
15. Assertion (A): The total number of nodes for 3p orbital is 2.
Reason (R): Total nodes = \(n - 1\), angular nodes = \(l\), radial nodes = \(n - l - 1\).
Answer Key
| Q | Answer |
|---|---|
| 1 | (b) — Angular nodes = \(l\) = 2 |
| 2 | (c) — For \(n=2\), max \(l = 1\), so \(l=2\) is not possible |
| 3 | (d) — If \(\Delta x = 0\), then \(\Delta p \to \infty\) by uncertainty principle |
| 4 | (a) — \(\lambda = h/mv = 6.6 \times 10^{-34}/(0.1 \times 100) = 6.6 \times 10^{-35}\) m |
| 5 | (b) — \([Ar],3d^{10},4s^1\) due to stability of completely filled d subshell |
| 14 | (a) — Both A and R true; R is the correct explanation of A |
| 15 | (a) — Both A and R true; R is the correct explanation (total = 3-1 = 2; angular = 1; radial = 1) |