Solute vs Solvent: solute is dissolved; solvent is dissolving medium; water is universal solvent.
Gaseous, liquid, and solid solutions exist (e.g., air, salt water, alloys).
2.4.1 Aqueous Solutions
Water dissolves many substances; stable mixture; common in labs.
2.4.2 Saturated Solution
Contains maximum solute at given temperature; dynamic equilibrium with undissolved solute.
2.4.3 Unsaturated Solution
Can dissolve more solute at current temperature.
2.4.5 Supersaturated Solution
Contains more solute than a saturated solution at a given temperature; unstable; crystallization occurs on seeding.
2.4.6 Concentrated and Dilute Solutions
Dilute: small amount of solute; Concentrated: large amount of solute.
2.4.7 Solubility
Maximum solute that dissolves in a solvent at a specific temperature; affected by solvent, temperature, and pressure.
2.4.8 Effect of Temperature on Solubility
Some solutes increase solubility with temperature (e.g.,
ext{KCl}, ext{NH}4 ext{Cl}); others decrease (e.g., ext{Ca(OH)}2).
2.5 Colloids & Suspensions
Colloid: heterogeneous mixture with particle sizes 1–1000 nm; particles undissolved but distributed; do not settle; Tyndall effect demonstrates light scattering.
Examples: starch, albumin, milk, ink, toothpaste.
Suspension: heterogeneous mixture with particles >1000 nm; particles settle; e.g., chalk in water, milk of magnesia, paints.
KEY POINTS
Matter has defined macroscopic properties and categorization (solids, liquids, gases, plasmas).
Distinguish pure substances vs mixtures; colloids vs suspensions; solute/solvent distinctions.
Solubility and solution types depend on temperature and solvent.
Unit 3: Atomic Structure
SLOs
Explain the atom as a central nucleus of neutrons and protons surrounded by electrons in shells.
Understand energy levels (shells) and larger shells imply higher energy/distance from nucleus.
Electrons are quantum particles with probabilistic paths; exact paths cannot be mapped (uncertainty principle).
Nucleus composed of protons and neutrons bound by strong nuclear force.
Atomic model as an aid to understanding structure, not a literal physical replica.
Relative charge/masses of subatomic particles: electron, proton, neutron.
3.1 Atomic Models
Dalton’s atomic theory (1803): elements are composed of atoms; atoms of the same element identical; chemical reactions involve combining/arranging atoms; atoms not created/destroyed.
Defects of Rutherford model: classical physics predicts radiating energy causes collapse of orbit; continuous spectrum issues.
Bohr model (1913): electrons orbit nucleus in fixed energy levels; energy depends on distance from nucleus; angular momentum quantized: L = rac{nh}{2 } (n is the principal quantum number); absorption/emission occur when electrons jump between levels; energy difference riangle E = E2 - E1.
Quantum Mechanical Model: electrons described by orbitals; probabilistic regions where electrons may be found; Heisenberg Uncertainty Principle: cannot simultaneously know exact position and trajectory.
de Broglie: electrons have wave-particle duality; experimental confirmation by Davisson and Germer (1927).
Atomic Model concept: models help interpret observations; nucleus contains protons and neutrons; electrons occupy surrounding shells; mass concentrated in nucleus; nucleus held together by strong nuclear force.
3.2 Subatomic Particles
Protons: +1 charge; ~1 amu; located in nucleus.
Neutrons: 0 charge; ~1 amu; located in nucleus.
Electrons: −1 charge; ~1/1836 amu; orbit nucleus.
Relative masses: protons and neutrons ~1 amu; electrons negligible mass.
Electric field effects on charged particles: in a uniform field, protons bend toward negative plate, electrons toward positive plate; neutrons pass straight through.
3.3 Proton Number (Atomic Number) and Isotopes
Atomic number Z: number of protons; unique to element; determines identity and periodic table position.
Isotopes: atoms with same Z but different mass numbers A (= Z + N); neutrons vary; chemical properties largely unchanged; isotopes used in dating and imaging.
Nucleon number (mass number) A: total protons + neutrons; neutrons = A − Z.
Radioactivity: some isotopes unstable; radioactive decay changes either neutrons or protons; examples: Carbon-14 → Nitrogen-14; Uranium-238 → decays to Lead-206.
3.4 Relative Atomic Mass and Atomic Mass Unit
Standard: Carbon-12 (C-12) defined as exactly 12 amu; one amu = 1/12 of C-12 mass.
Relative atomic mass (Ar) of an element is the weighted average of isotopic masses considering their natural abundances:
ext{Ar} = rac{\sumi ( ext{abundance}i \,\times\, ext{mass}_i)}{100}.
Example: Hydrogen isotopes have abundances and masses leading to Ar(H) ≈ 1.008 amu.
3.5 Isotopes
Hydrogen isotopes: protium ({}^1H), deuterium ({}^2H or D), tritium ({}^3H or T).
Carbon isotopes: {}^{12}C, {}^{13}C, {}^{14}C with natural abundances leading to Ar(C) ≈ 12.00026 amu.
Isotopes share chemical properties but differ in physical properties due to mass differences.
Relative atomic mass Ar uses C-12 as standard; mass unit is amu.
Cations form by losing electrons; anions by gaining electrons; ion formation depends on valence electrons.
Electronic configuration determines block (s/p/d/f) and group/period placement in the periodic table.
Unit 4: Periodic Table and Periodicity of Properties
SLOs
Define periodic table as arrangement by periods and groups in increasing atomic number.
Identify group/period/block from electronic configuration (subshells indicate blocks).
Relate group number to ion charge formed by elements in that group.
Explain similarities/differences of elements in same group/period; trends in atomic radius, electron affinity, electronegativity, ionization energy, metallic character, density.
Positioning unknown elements using electronic configuration; predicting properties (melting point, density, reactivity) from group/period.
Noble gases electronic configuration; comparison of metals vs non-metals in physical properties (thermal/electrical conductivity, malleability, hardness).
4.4.2 Reactivity
Reactivity trends: increases down a group; left-to-right across a period the reactivity shifts depending on left-side metals vs right-side nonmetals.
KEY POINTS
Periodic law: element properties repeat periodically with increasing atomic number.
Block designation (s/p/d/f) correlates with valence electron configuration and group/period placement.
Ion formation follows predictable patterns based on valence electrons.
Physical properties show general trends (atomic size, ionization energy, electronegativity, etc.) with notable exceptions.
Unit 5: Chemical Bonding
SLOs
Explain noble gas electronic configuration, octet/duplet rules to predict main-group chemistry.
Compare formation of cations and anions.
Explain electropositive/electronegative nature of metals/non-metals.
Define ionic, covalent, coordinate covalent and metallic bonds.
Differentiate between ionic and covalent compounds.
Explain structure/property relationships in bonding; conduction mechanisms; solubility/ionization in water; graphite vs diamond vs metals.
5.1 Noble-Gas Configurations and Octet/duplet Rules
Noble gas core provides stable electron configuration; octet rule: main-group elements tend to attain eight electrons in their valence shell via bonding.
Duplet rule for hydrogen, helium, lithium (2 electrons in the valence shell).
Examples: Na (loses 1 electron to achieve Ne-like configuration); Cl (gains 1 electron to complete octet).
5.2 Electropositive vs Electronegative Elements
Metals: electropositive; lose electrons to form cations; low ionization energy and low electronegativity.
Non-metals: electronegative; gain electrons to form anions; high electron affinity.
5.3 Types of Bonds
Ionic bonds: electrostatic attraction between oppositely charged ions (formed by transfer of electrons).
Covalent bonds: sharing of electron pairs between atoms.
5.3.2 Covalent Bonds: single, double, and triple bonds; Lewis structures and dot-cross representations; examples H2, O2, CO2, H2O, CH4, NH3, etc.
5.3.3 Bond Polarity: Non-polar covalent bonds (equal sharing; identical atoms or shared electronegativity) vs Polar covalent bonds (unequal sharing; electronegativity difference).
5.3.4 Coordinate Covalent Bonds: shared electron pair originates from one atom; common in complex ions (e.g., NH4+, H3O+); examples: NH3-BF3 adducts, hydronium (H3O+).
5.4 Intermolecular Forces
Dipole-dipole interactions: occur between polar molecules; light scattering (Tyndall effect) distinguishes colloids from true solutions.
Hydrogen bonding: strong dipole-dipole interaction involving H bonded to N, O, or F with lone pairs on nearby electronegative atoms; important in water, proteins, DNA, and glues.
5.5 Nature of Bonding, Structure and Properties
Factors affecting properties: type of particles (ions, atoms, molecules), strength of bonds, and structural arrangement (giant vs discrete molecules).
Conduction in ionic compounds: solid-state ions are immobile; molten or dissolved ions conduct electricity.
Covalent compounds: generally poor conductors; high-melting points when giant covalent networks (e.g., SiO2, diamond); low melting points for simple covalent molecules due to weak intermolecular forces.
5.5.1 Graphite
Graphite: carbon layer structure; each C forms 3 covalent bonds in layers; weak van der Waals between layers; good lubricative properties; conducts electricity.
5.5.2 Diamond
Diamond: tetrahedral network of carbon; each C bonded to four C; very hard; high melting point; poor electrical conductivity.
5.5.3 Contrasting Ionic and Covalent Compounds
Ionic compounds: high melting/boiling points; conduct electricity when molten or dissolved; brittle.
Covalent compounds: variable melting/boiling points; poor conductors; can be polar or non-polar; many have low melting points.
5.6 Metallic Bonds
In metals, valence electrons are delocalized as an electron sea; cations form a lattice held by electrostatic attraction to the electron cloud.
Results: malleability, ductility, high electrical and thermal conductivity, high melting points, metallic luster.