23
Atomic Structure Radioactivity History of discovery Becquerel Discovery of radioactivity Curie Extraction of radium and polonium Rutherford Study the nature of , and radiation Nature of radioactivity particle fast moving helium nuclei 5% of speed of light particle very fast moving electron up to 99% speed of light radiation high energy EM wave 100% speed of light Origin of radioactivity particle replusion among proton binding force between proton and neutron lowering of p:n ratio particle instablility of neutron when isolated increasing of p:n ration radiation Nature state of atoms after the big bang / nucelus formation re-orientation of the spinning proton Nuclear Reaction Natural decay Meaning of Half-life Constant Half-life First order reaction Independent of temp. Artificial transmutation Use of Radioactive isotope Leak Detection Geiger-Muller counter Bio-tracer I-131 (thyroid disease) P-32 (metabolism of plant) Radiotherapy I-131 (thyroid cancer) Co-60 / Cs-137 (tumor) Carbon-14 dating Nuclear power Nuclear bomb Mass of an atom Mass spectrometer Construction Vaporization chamber Ionization chamber Accelerating plates Deflecting magnetic field Detector Recorder Vacuum Pump Working principle - response to m/e ratio To determine the ionization energy of an atom Interpretation of mass spectrum Determination of isotopic mass Determination of atomic mass Determination of molecular mass Determination of molecular structure Relative isotopic mass The relative mass of a particular isotope in C-12 scale where C-12 isotope is defined to have exactly 12 units of mass. Relative atomic mass The weighted average of the relative isotopic masses for a particular element in C-12 scale according to their natural abundance Relative molecular mass The relative mass of a molecule where that the value is the same as the sum of relative atomic mass of all atoms present in the molecule. Development of atomic model Democritus Idea of atom introduced No experimental evidence Dalton Atom is the smallest unit of matter and is not breakable With experimental evidence from the study of gas Goldstein Invention of cathode ray tube Thomson Behaviour of cathode ray in magnetic and electric field Negatively charged fast moving particle Invention of the word "electron". Raisin pudding model of atom Atom is no longer unbreakable Rutherford Gold foil scattering experiment The idea of presence of tiny nucleus Chadwick Discovery of neutron Study of radioactivity The idea of nucleus is breakable 1. Atomic Structure.mmap - 2005/5/23 -

Mindmap of Alevel.physical Chemistry

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  • Atom

    ic Structure

    Radioactivity

    History of discovery

    BecquerelD

    iscovery of radioactivity

    Curie

    Extraction of radium and

    polonium

    Rutherford

    Study the nature of,

    andradiation

    Nature of radioactivity

    particlefast m

    oving helium nuclei

    5% of speed of light

    particlevery fast m

    oving electron

    up to 99% speed of light

    radiationhigh energy EM

    wave

    100% speed of light

    Origin of radioactivity

    particle

    replusion among proton

    binding force between proton

    and neutron

    lowering of p:n ratio

    particle

    instablility of neutron when

    isolated

    increasing of p:n ration

    radiation

    Nature state of atom

    s afterthe big bang / nucelusform

    ation

    re-orientation of the spinningproton

    Nuclear Reaction

    Natural decay

    Meaning of H

    alf-life

    Constant Half-life

    First order reaction

    Independent of temp.

    Artificial transmutation

    Use of Radioactive isotope

    Leak Detection

    Geiger-M

    uller counter

    Bio-tracerI-131 (thyroid disease)

    P-32 (metabolism

    of plant)

    RadiotherapyI-131 (thyroid cancer)

    Co-60 / Cs-137 (tumor)

    Carbon-14 dating

    Nuclear pow

    erN

    uclear bomb

    Mass of an atom

    Mass spectrom

    eter

    Construction

    Vaporization chamber

    Ionization chamber

    Accelerating plates

    Deflecting m

    agnetic field

    Detector

    Recorder

    Vacuum Pum

    p

    Working principle - response to

    m/e ratio

    To determine the ionization

    energy of an atom

    Interpretation of mass

    spectrum

    Determ

    ination of isotopic mass

    Determ

    ination of atomic m

    ass

    Determ

    ination of molecular m

    ass

    Determ

    ination of molecular structure

    Relative isotopic mass

    The relative mass of a particular isotope in C-12 scale w

    hereC-12 isotope is defined to have exactly 12 units of m

    ass.

    Relative atomic m

    ass

    The weighted average of the relative isotopic m

    asses for a particularelem

    ent in C-12 scale according to their natural abundance

    Relative molecular m

    ass

    The relative mass of a m

    olecule where that the value is the

    same as the sum

    of relative atomic m

    ass of all atoms present

    in the molecule.

    Developm

    ent of atomic

    model

    Dem

    ocritusIdea of atom

    introduced

    No experim

    ental evidence

    Dalton

    Atom is the sm

    allest unit ofm

    atter and is not breakable

    With experim

    ental evidencefrom

    the study of gas

    Goldstein

    Invention of cathode ray tube

    Thomson

    Behaviour of cathode ray inm

    agnetic and electric fieldN

    egatively charged

    fast moving particle

    Invention of the word "electron".

    Raisin pudding model of atom

    Atom is no longer unbreakable

    RutherfordG

    old foil scattering experiment

    The idea of presence of tiny nucleus

    Chadwick

    Discovery of neutron

    Study of radioactivityThe idea of nucleus is breakable

    1. Atom

    ic Structure.m

    map - 2005/5/23 -

  • Mole Concept

    How

    much

    is onem

    ole ?

    How

    many ?

    Definition

    Avogadro constant(Experim

    entalm

    easurement required)

    How

    heavy ?

    Molar

    mass

    Carbon-12 Scale

    How

    large ?

    Molar volum

    e

    Molar

    volume

    of a gas

    r.t.p.

    s.t.p.

    Avogadro's law

    Charges

    Relationship between

    Current I, Amount of charge

    Q and tim

    e t i.e Q=It

    Faraday'sLaw

    s ofelectrolysis

    1st Lawm

    Q

    2nd Lawm

    1/n

    Charges carried by1 m

    ole of electronFaraday constant

    1 F = 96500 C

    Behaviour of Ideal gas

    Boyle's Law P

    1/V

    Charles' Law V

    T

    Avogadro's Law V

    N

    Ideal gas Law/ EquationPV = nRT

    Determ

    ination of m

    olecular mass

    of a volatile liquid

    Principle

    Volatile liquid vaporizes easily by heating

    Assuming the vapor behaves ideally

    No interaction am

    ong particles

    Individual particle occupies no volume

    Molecular m

    ass is numerically the

    same as m

    olar mass

    Conditions a real gas behavesvirtually ideal

    High tem

    perature

    particles arem

    oving fastinteraction am

    ong particles is negligible

    Low pressure

    particles arefar apart

    space occupied by individual particle is negligible

    Setup of apparatus

    Measurem

    ent of PBarom

    eter in the laboratory

    Measurem

    ent of V

    Increase in volume of

    the gas syringePrecaution

    Take reading only when the

    reading is steady

    Some liquid m

    ay havenot vaporized

    The vapor may be still

    expanding

    Measurem

    ent of m

    Difference in m

    ass ofthe hypoderm

    ic syringebefore and afterinjection

    Precaution

    Hold the hypoderm

    icsyringe horizontal

    The liquid may leak out.

    Volatile liquid usuallyhas low

    surface tension.

    Hold the end of the

    syringe only

    Body warm

    th may heat up

    the liquid and expel it fromthe syringe

    Insert the needle fullyinto the gas syringe

    Inject the liquid into thedeeper part, usually hotter,of the gas syringe toensure better vaporization.

    Measurem

    ent of T

    Therm

    ometer

    (final reading)Precaution

    Take reading only when the

    reading is steadyThe system

    may have not

    reach thermo-equilibrium

    yet.

    Operation

    Allow the system

    to reach a thermo-equilibrium

    Take all initial readings

    Take final reading when all readings are steady

    Dalton's Law

    of partialpressure

    Total pressure of a gaseousm

    ixture is the same of the sum

    of the partial pressure of all ofthe com

    ponent present

    Definition of partial pressure - the pressure

    of a component in the gaseous m

    ixture ifthat com

    ponent occupies the same volum

    eby itself alone.

    mole fraction (percentage by num

    ber)

    2. Mole C

    oncept.mm

    ap - 21/5/2005 -

  • Chemical Equations

    and Stoichiom

    etry

    Formulae

    Formulae of

    Compounds

    Empirical form

    ulaSim

    plest whole num

    ber ratio

    Molecular form

    ulaActual no. of atom

    s

    Structural formula

    Connectivity of atoms

    Determ

    inationof Form

    ulae

    Empirical form

    ulaBy Com

    bustion Analysis

    From Com

    position by mass

    Molecular form

    ula

    From em

    pirical formula and

    m

    olecular mass

    Water of crystallization

    Chemical Equations

    Word Equation

    Chemical Equation

    Stoichiometry

    Stoichiometric coefficients

    Calculation based on equationsReacting m

    asses

    Volumes of gases

    Volum

    etricA

    nalysis

    Titration

    Standard solutionA solution w

    ith accurately known concentration

    Standardization

    Process of determination of concentration of a

    non-standard solution

    Primary standard

    A substance which can be used to prepare a

    standard solution directly

    criteria

    known com

    position

    stable composition

    readily soluble

    preferably with higher

    m

    olecular mass

    Equivalence point

    The point at which the 2 reagents just react w

    ith

    each other completely.

    End pointThe point w

    hen the end of titration is detected

    Acid-base

    titration

    Using indicator

    Choice of indicator

    strong acid vs strong base

    methyl orange or

    phenolphthalein

    strong acid vs weak base

    methyl orange

    weak acid vs strong base

    phenolphthalein

    Without indicator

    pH m

    eter (titration curve)

    thermom

    etric titration

    conductometric titration

    Redox titration

    Iodometric titration

    iodine / potassium iodide

    starch solution

    sodium thiosulphate

    Determ

    ination of concentration of

    chlorine bleach

    KMnO

    4 vs FeSO4

    KMnO

    4 vs H2C2O

    4.2H2O

    Constant heating is required

    Back titrationExam

    ple

    Determ

    ination of percentage by mass of calcium

    carbonate in chalk

    Analysis of aspirin

    Used if the reaction of direct titration is not instantaneous

    / if no suitable indicator for direct titration

    methods for titration of

    weak acid vs w

    eak alkali

    3. Chem

    ical Equations and S

    toichiometry.m

    map - 8/1/2005 -

  • The ElectronicStructure of A

    toms

    Different m

    odels ofatom

    Bohr's model

    Atomic Em

    ission spectrum of

    hydrogen

    Setup of the apparatus

    gas discharge tube

    slit

    prism or diffraction grating

    photographic film

    Characteristic of the hydrogenspectrum

    Num

    erous lines

    Different series

    Unevenly spaced lines in each

    series

    Convergence limits at the

    higher frequency end of eachseries

    Continuum

    Interpretation of the hydrogenspectrum

    Line spectrum

    Introduction of concept ofquantum

    Planck's equation

    Process of excitation andrelaxation

    ground state

    excited state

    Num

    erous lines

    Presence of numerous energy

    levels (shells)

    principalquantum

    number

    Multiple transitions take place at the sam

    e time

    Unevenly spaced lines

    Unevenly spaced energy levels

    Convergence limit

    and continuumIonization of atom

    Uniqueness of atom

    ic emission

    spectraAs a m

    ean of identification

    Flame test

    Atomic em

    ission spectroscopy

    Discovery of helium

    Identification of element at

    remote star

    Red shift

    Neon light w

    ith differentcolours

    Ionization energies

    Definition

    Successive ionization energiesEvidence of shell

    1st ionization energies acrossperiods

    Evidence of subshell

    Features of Bohr's model

    Electrons are orbiting around the nucleus in orbits with w

    ith different energy

    The allowed energy of the electron in an atom

    is quantumized

    Able to explain the emission spectrum

    of hydrogen spectrum but fail to explain the em

    ission spectrum of those

    multi-electron system

    .

    Wave-m

    echanical model /

    Orbital m

    odel

    Wave-particle duality of electron

    Heisenberg's uncertainty principle

    Quantum

    numbers

    By mathem

    atical modeling

    Principal (n)

    n = 1,2,3 ...

    principal energy

    size

    shell no.

    Subsidiary (l)

    l = 0,1,2...(n-1)

    shape of orbital / subshell

    energy in multi-electron

    system

    Magnetic (m

    )m

    = -l,...,0,...+l

    spatial orientation of orbital

    Spin (s)s = +

    or -

    spin of electron

    Pauli Exclusion principle

    Orbital / Electron cloud representation

    Radial probability distribution

    Nodal surface

    Nodal plane

    Background knowledge

    Electromagnetic Spectrum

    Continuous Spectrum

    Line Spectrum

    4. The Electronic S

    tructure of Atom

    s.mm

    ap - 19/1/2005 -

  • Electronicconfigurations andthe Periodic table

    Building up of electronicconfiguration on paper

    Aufbau PrincipleElectrons occupy the orbital w

    ith the lowest energy first

    Order of energy of different orbitals

    Pauli exclusion principle

    All electrons behave different in an atom i.e. no 2

    electrons in an atom have the sam

    e set of quantum no.

    Each orbital can accomm

    odate2 electrons w

    ith opposite spin

    Hund's Rule (Rule of M

    aximum

    Multiplicity)

    Electrons will occupy degenerate orbitals singly

    with parallel spin before pairing up occurs.

    Irregularity

    Energy of 4s orbital is only a littlebit low

    er than that of 3d orbital

    The difference gets even smaller w

    hen3d orbitals are being filled up

    3d electrons shield 4s electron from the nucleus

    and make 4s electrons m

    ore energetic

    Exception

    Chromium

    half-filled 3d and 4s orbital

    no electron pair-up in 3d and 4sless repulsion

    more evenly distributed electron cloud

    less repulsion

    Copperfull-filled 3d and half-filled 4s orbital

    more evenly distributed electron cloud

    less repulsion

    Representation ofelectronic configuration

    by notation

    by electron in boxes

    use of abbreviationN

    oble gas cores e.g. [He], [N

    e] etc.

    Completely filled quantum

    shell e.g. K, L, M

    Variation of Successiveionization energies

    Successive ionization energy is always

    much higher than its predecessor

    the p to e- ratio is increasing

    the repulsion/shielding among electron is getting less

    more difficult to rem

    ove electron from a positive particle

    Plot of Successive ionizationenergies of an atom

    In log scale

    the increases in successive ionization energies are toolarge to be represented by linear scale

    appear in tiersProof of the presence of shells

    Plot of successive ionizationenergies of different atom

    s

    shift upwards

    the p to e- ratio is increasing

    shift to the right

    the electronic configuration of an ion is the same as

    the electron configuration of the preceding atom

    Atom

    ic radius

    Covalent radius

    including metallic radius

    half of the distance between 2 chem

    icallybonded nuclei of the sam

    e element

    Depending

    on

    Attraction with the nucleus

    Nuclear charge

    Repulsionam

    ongelectrons

    Relative position of theouterm

    ost e- (Electronic configurationof the atom

    )

    Primary

    shielding effect

    repulsion with

    the inner e-

    usually stronger

    Secondary shielding effect

    repulsion with the

    e- in the same shell

    usually weaker

    General trend

    contract across a period

    the increase in nuclear charge outweighs the increase in

    secondary shielding effect.

    expand down a group

    the increase in primary shielding effect outw

    eighs theincrease in nuclear charge

    van der Waals' radius

    half of the distance between 2 nuclei of the sam

    e element w

    hichare not chem

    ically bonded together in a crystal lattice

    Periodic Tables-block, p-block, d-block and f-block elem

    ents

    Variation of FirstIonization energyacross the first 20elem

    ents

    Definition

    Energy required torem

    ove 1 mole of

    electrons from 1

    mole of gaseous

    atom

    Value reflects the netattraction betw

    een the outerm

    ost electronand the nucleus

    Gets m

    ore endothermic w

    henincrease in attraction w

    ith e-> increase in repulsion am

    ongelectrons, and vice versa

    Energy required to move the outerm

    ost electron to infinityand escape from

    the attraction of the nucleus

    Variation

    Depending

    on

    Effective nuclearcharge (nuclearcharge - shieldingeffect)experienced bythe outerm

    ost e-

    Attraction with the nucleus

    Nuclear charge

    Repulsionam

    ongelectrons

    Relativeposition of theouterm

    ost e- (Electronicconfiguration ofthe atom

    )

    Primary

    shielding effect

    repulsion with

    the inner e-

    usually stronger

    Secondary shielding effect

    repulsion with the

    e- in the same shell

    usually weaker

    Position of the outermost e- (Size of atom

    )

    General

    pattern

    Main trend

    Getting m

    ore endothermic

    across a period

    the increase in nuclear chargeoutw

    eighs the increase insecondary shielding effect

    Getting less endotherm

    ic down

    a group

    the increase in primary

    shielding effect outweighs the

    increase in nuclear charge

    Showing 2-3-3

    pattern acrossperiod 2 and 3

    Imply presence of subshell

    Imply pairing up of electrons in an orbital

    Unexpected drops

    at B and Al(or peaks at Be and M

    g)

    Electron goes into a more

    energetic p-subshell(or full filled s-subsell in Beand M

    g - more evenly

    distributed charges)

    Unexpected drops

    at O and S

    (or peaks at N and P)

    Electrons starts pairing up in Oand S - extra repulsion (or halffilled p-subshell in N

    and P - m

    ore evenly distributed charges)

    5. Electronic configurations and the P

    eriodic table.mm

    ap - 6/1/2005 -

  • Energetics SignificanceThe link betw

    een the microscopic interaction am

    ongparticles and m

    acroscopic observable change.

    EnthalpyandInternalenergy

    Enthalpy changeD

    efinition : heat change of a system at constant pressure

    Internal energy change

    Definition : heat change of a system

    at constantvolum

    e

    Relationship between Enthalpy

    change and Internal energychange

    Enthalpy change = Internal energy change +W

    ork done on the atmosphere

    Exothermic and

    Endothermic process

    Exothermic

    process

    Heat flow

    s out of the system because of the

    increase in temperature of the system

    Potential energy among the particles is converted

    to heat energy when there is an overall

    strengthening of attractions among the particles.

    Bond formation > Bond breaking

    Endothermic

    process

    Heat flow

    s into the system as the tem

    peratureof the system

    decreases

    Heat energy is converted to potential energy

    when there is an overall w

    eakening of attractionsam

    ong the particles.

    Bond formation < Bond breaking

    Hess's Law

    The total enthalpy change of a chemical reaction is independent

    of the route by which the reaction takes place

    Another version of law of

    conservation of energy

    Energy cannot be created ordestroyed

    Energy cycle & energy level diagram

    Born-Haber cycle as energy cycle used

    to determine the heat of form

    ation

    Need of H

    ess's Law

    Some changes has no direct reaction at all

    The direct reaction may be too vigorous

    and too dangerous to be carried out

    The extent (% of conversion) ofreaction cannot be controlled.

    Formation of side products

    Calculation

    Prerequisite

    Balanced equation according to definitions

    Calculation involving heat capacity

    Calculation of mole

    Patience and careful manipulation

    Some com

    mon references in

    constructing energy cycles

    1. Constituent elements

    2. Combustion products

    3. Constituent atoms

    unit and sign of the answer

    + and - sign must be included

    Unit, usually in kJm

    ol-1 must

    be included

    Standard enthalpychanges

    Standard conditions298K

    1 atm

    Standard state

    pure, if it is a liquid or solid

    most stable form

    at 298K, 1 atm

    1M if it is an solution

    Need of standard state and

    condition

    Presence of allotrope andpolym

    orph

    Different form

    s of the same elem

    ent /com

    pound in the same physical state

    e.g. graphite and diamond,

    ozone and diatomic oxygen

    Enthalpy change as Heat flow

    (q) of a system at constant pressure returning

    the system to the original tem

    perature under a specific condition.

    Examples and definitions

    Heat of N

    eutralizationForm

    ation of 1 mole of w

    ater

    Neutralization of strong/w

    eak acid / alkali

    Heat of Solution

    A solution with specific concentration /

    an infinitely dilute solution is prepared.

    Heat of Form

    ation

    1 mole of com

    pound is formed from

    its constituentelem

    ents in their standard states

    Heat of Com

    bustion

    Complete com

    bustion of 1 mole of a specific

    substance in excess oxygen

    Heat of H

    ydration

    Formation of 1 m

    ole of hydrated crystalfrom

    anhydrous solid

    Experimental determ

    ination

    bomb calorim

    etry todeterm

    ine the internalenergy change

    Experimental setup

    conversion to enthalpy changeby calculation

    Philips Harris calorim

    eter todeterm

    ine heat of combustion

    Experimental setup

    simple calorim

    etry todeterm

    ine the enthaplychange

    Experimental setup

    Polystyrene cup + cover

    Insulating layer

    thermom

    eter

    stirrer

    Com

    mon

    assumptions

    Specific heat capacity ofsolution is the sam

    e as that ofw

    ater

    The rate of heat loss isuniform

    / No heat loss to the

    surrounding.

    The heat capacity of some

    components in the system

    canbe ignored.

    The specific heat capacities ofsom

    e components are only

    approximation.

    Heat evolved w

    ill be the same

    as heat flow in the original

    definition of enthalpy change

    6. Energetics.m

    map - 17/1/2005 -

  • Ionic Bonding

    Energeticsofform

    ation

    Born Haber Cycle

    Heat of form

    ationform

    ation of 1 mole of com

    pound

    Atomization energy of elem

    ent

    formation of 1 m

    ole of gaseousatom

    s

    always positive

    Ionization enthalpy of atom

    Removal of 1 m

    ole of electronsfrom

    1 mole of gaseous atom

    s/ ions

    always positive

    Electron Affinity of atom

    Addition of 1 mole of electrons

    to 1 mole of gaseous atom

    s /ions

    negative : attraction between the incom

    ingelectron and the nucleus > the repulsion betw

    eenthe incom

    ing electron and the existing electrons

    positive : attraction between the incom

    ingelectron and the nucleus < the repulsionbetw

    een the incoming electron and the existing

    electrons

    Lattice energy

    Formation of 1 m

    ole of ioniccom

    pound from its constituent

    gaseous ions

    always negative

    a measure of strength of ionic

    bond

    depending on charge densityof ions involved

    depending on the packingefficiency i.e. crystalarrangem

    ent

    Stoichiometry

    ofioniccom

    pounds

    Limitation of using stable

    electronic configuration toexplain

    Positive metal ion + free electron are actually m

    oreenergetic (less stable) than a gaseous m

    etal atom

    Indeed, the stability of an ionic compound is m

    ainlyarising from

    the formation of ionic bond am

    ongoppositely charged ions.

    Nature prefers the

    stoichiometry w

    iththe m

    ost exothermic

    heat of formation

    i.e. highest stability com

    paring with the

    constituent elements

    Construction of Born Harber cycle for

    the naturally occurring ioniccom

    pound e.g MgCl2

    Construction of BornH

    aber Cycle for thehypothetical ioniccom

    pounds e.g. M

    gCl and MgCl3

    Hypothetical lattice energy

    calculated from the ionic m

    odel

    Assum

    ptionsofionicm

    odel

    The latticearrangem

    ent of thehypothetical com

    poundis know

    n

    All ions are perfect spheres

    Cations and anions are just incontact w

    ith each other

    The bond is purely ionic

    The value of heat of formation is m

    ainly determined

    by the values of ionization energies and lattice energy

    Ioniccrystals

    Different

    arrangements

    of lattice points

    face centered cubic(f.c.c.) structure

    e.g. NaCl

    C.N. = 6 for both ions

    simple cubic structure

    e.g. CsClC.N

    . = 8 for both ions

    Actual arrangement is

    depending on

    Stoichiometry of the

    compound

    ionic radius ratio

    Some term

    s

    Coordination number (C.N

    .) -no. of nearest neighbour

    Determ

    ination of empirical

    formula

    Unit Cell

    Definition

    1. the smallest unit containing

    all the fundamentals of a crystal

    without repetition.

    2. the smallest unit of a crystal

    from w

    hich the original crystalstructure can be recreated byrepetition in 3-dim

    ensional space.

    Determ

    ination of no. ofdifferent ions in an unit cell

    Determ

    ination ofem

    pirical formula

    Lattice point

    The position of a formula unit

    of the compound considered.

    ionic radius

    Definition - D

    istance from the centre of an ion to

    the point of zero electron density between 2

    adjacent ions.

    determined by X-ray

    diffractionElectron density m

    ap

    Value

    depending on

    no. of atoms

    present

    polyatomic ion

    is bigger thansim

    ple ion

    p to e- ratio

    In general, negativeion is bigger thanpositive ion

    Size of isoelectronicion

    As the no. of electrons andelectronic configurations are thesam

    e, the size is only dependingon the num

    ber of protons present.

    Balance between

    non-directionalelectrostatic attractionand repulsion

    Attraction among oppositely

    charged ions

    Repulsion among sim

    ilarlycharged ions

    Potential well diagram

    7. Ionic bonding.mm

    ap - 19/1/2005 -

  • Covalent bonding

    Balance between

    electrostatic attractionand repulsion

    Attraction between nucleus,

    bonding electron and anothernucleus

    directional attraction

    Replusion among the electrons

    Replusion between the nuclei

    Potential well diagram

    Formation of

    covalent bond

    Overlapping of atom

    ic orbital

    Constructive interference ofatom

    ic orbitals

    Increase in electron densityalong the inter-nuclear axis

    Pairing up ofunpaired electrons(bonding electrons)

    Promotion of paired electrons

    to low lying energy orbital

    (e.g. 2p comparing w

    ith 2s, 3dcom

    paring with 3p) to yield

    more unpaired electrons for

    bond formation

    Formation of

    more bonds

    More overall

    exothermic change

    High overall stability

    Dative covalent bond

    a covalent bond in which the

    bonding electrons are suppliedby one atom

    only

    Overlapping of a lone pair w

    itha vacant orbital

    e.g. NH

    4+, H3O

    + NH

    3BF3, Al2Cl6

    Draw

    ing of Lewis

    structure

    Formal charge

    # of p - # of e- associated with

    an atom assum

    ing that bondinge- are equally shared

    Oxidation num

    ber

    # of p - # of e- associated with

    an atom assum

    ing that allbonding e- are belonging tothe m

    ore electronegative atom

    Cases obeying octet rule

    Period 2 elements never

    excess octet

    3s orbital has much higher

    energy than 2p orbital

    Energetically unfavorable

    Can be lessthan octet

    e.g. BF3

    an electron acceptor with a

    vacant p-orbital for dativebond form

    ation

    Cases not obeyingoctet rule

    Expansion of octet

    Availability of low lying energy

    orbital (e.g. 3d orbitalcom

    paring with 3p orbital)

    e.g. PCl5, SO42-

    Giant Covalent Structure

    Diam

    ond

    tetrahedrally arranged

    strong C-C single bond only

    high hardness, high melting point, electrical insulator, excellent heat conductor

    Graphite

    arrange in hexagonal layers

    strong C-C bond, bond order 1 1/3, within layer

    weak van der W

    aals force between layers

    low hardness, very high m

    elting point, conducting along the layer, slipperybetw

    een layers

    Quartz (SiO

    2)high hardness, high m

    elting point

    Shape of molecules and

    polyatomic ions

    Valence shell electron pairrepulsion theory

    Electron centres : lone pair,single bond, double bond,triple bond

    Electrons centres tend toseparate from

    each other asfar as possible to m

    inimize

    mutual repulsion

    Electrostatic repulsion is verysensitive to distance

    repulsion between lone

    pair-lone pair > lone pair-bondpair > bond pair-bond pair

    lone pair always occupies

    equatorial position in a fiveelectron centres system

    Description of shapes

    linear, angular (V-shaped or bent), trigonal planar, tetrahedral, trigonalpyram

    idal, trigonal bipyramidal, seesaw

    , T-shaped, octehedral, squareplanar

    In the describing of the shape of molecule, the presence of lone pair is

    not included.

    Strength of Covalentbond

    In the range of 150-1000 kJmol-1

    Bond Dissociation Energy

    D(X-Y)

    Energy required to break a particular bond

    (Average) Bondenthalpy/energy E(X-Y)

    The average energy required to break a type of bond

    Estimation using enthalpy change of atom

    ization

    Using bond energy to estim

    ate the enthalpy change of a reaction

    Factors affecting bondstrength

    Bond orderno. of bonding electrons / 2

    Bond length

    The longer the bond length, the weaker w

    ill be thebond(Prim

    ary) shielding effect affects the nuclearattraction experienced by the bonding electrons

    Atomic size

    (covalent radius)

    Estimation of bond length

    Breakup of additivity ofcovalent radius

    Polarity of bond

    Resonance

    bond polarity

    covalent bond with certain ionic character is found to be

    stronger than purely covalent or purely ionic bond

    repulsion among the lone pairs

    on adjacent atoms

    e.g. weak F-F, O

    -O and N

    -Nbond

    8. Covalent bonding.m

    map - 2005/5/21 -

  • Intermediate Type ofBonding

    Starting frompure ionic bond

    Assum

    ptionsof sim

    pleionicm

    odel

    The lattice arrangement of the com

    pound is known, if it is hypothetical

    All ions are perfect spheres

    Cations and anions are just in contact with each other

    and clearly separated from each other

    The bond is purely ionic. i.e. no sharing of electron or incomplete transfer of electron

    For all real ionic com

    pounds

    The lattice energycalculated based onthe ionic m

    odel isnever the sam

    e asthe experim

    entalvalue

    A more agreed value im

    pliesa situation sim

    ilar to theassum

    ptions of ionic model -

    pure ionic bonde.g. N

    aCl (almost purely ionic)

    A very differentvalue im

    plies failureof the ionic m

    odel -w

    ith strongcovalent character

    The ions are notperfectlyspherical

    Mutual repulsion

    of electron cloudin an ionic lattice

    Polarization ofanion

    Ions may not

    clearly separatedfrom

    each other

    Certain covalentcharacter

    Polarization ofanion

    Anion is always

    polarized bythe cation

    Polarization - distortion of electron cloudof anion under the influence of cation

    e.g. AgCl, AgBr, AgI, ZnS

    Polarizabilityof an anion

    ease of distortion ofelectron cloud

    inversely proportionalto the nuclearattraction on theelectron cloud

    p to e- ratio

    electronicconfiguration

    primary

    shieldingeffect

    secondaryshieldingeffect

    Polarizing power of a cation

    directly proportional to thecharge density of a cation

    Electronegativity

    Tendency of an atom to

    attract the bonding electron ina stable m

    olecule

    Increase across a period andup a group

    Not applicable to noble gases

    Depending on the effective

    nuclear charge experienced bythe bonding electron

    nuclear charge

    shielding effect

    Pauling's scale

    ionization energy

    reflects the attraction on theouterm

    ost electron in an atom

    electron affinity

    reflects the attraction on theincom

    ing electron to be addedto an atom

    Fluorine has the highest assigned value : 4.0

    The percentage of ionic character of a covalent bond is depending onthe difference in electronegativity of the 2 elem

    ents bonded together

    Starting frompure covalentbond

    Pure covalent bond

    The bonding electronsare shared equally

    The bond isnon-polar

    e.g. Cl2

    Polarcovalentbond

    The bonding electronsare not shared equally

    atoms have different

    electronegativitye.g. H

    Cl

    (Permanent)

    Dipole

    mom

    ent

    Definition - product of quantity of charge (q)

    and distance of charge separation (d)

    The dipole mom

    ent along a bond is pointing fromthe less electronegativity atom

    to the more

    electronegativity atom

    Lone pair

    Contribute a dipole mom

    entpointing aw

    ay from the atom

    Polarityof am

    olecule

    Depending on the vector

    sum of all dipole

    mom

    entsG

    eometry of the m

    olecule

    magnitude of individual

    dipole mom

    ent

    Non-polar

    molecule

    A molecule w

    ith non-polarbond only

    A molecule w

    ith all dipolem

    oments canceling out each

    other

    Do not /

    weakly

    attracted byan electricfield

    Non-polar m

    oleculesare also attracted byan electric field as aw

    eak temporary dipole

    mom

    ent will be

    induced onto them by

    the electric field

    Polar molecule (D

    ipole)

    A molecule w

    ith non-zeronet dipole m

    oment

    May not be able to tell the

    actual direction of the netdipole m

    oment

    Attracted by an electric field

    9. Intermeidate type of bonding.m

    map - 26/1/2005 -

  • Metallic bonding

    Nature of m

    etallic bond

    Sea of electrons model

    lattice of positive ions

    imm

    ersed in a sea ofdelocalized electrons

    Electrostatic attraction among positive

    ions and sea of delocalized electronsN

    on-directional in nature

    metallic radius = covalent radius

    uniqueproperties ofm

    etal

    high conductivity

    agitation of delocalizedelectrons

    high ductility andm

    alleability

    delocalized electrons capable to reform the

    metallic bond even if the positive ions are shifted

    metallic luster

    delocalized electrons getexcited and give out luster

    Strength of metallic

    bond

    In the range of 100-500 kJmol-1

    Attraction on the delocalizedelectrons

    Charge density of the positiveion e.g. N

    a+ > K+ > Rb+

    Availability of delocalizedelectron

    no. of valence electrons e.g.Al > M

    g > Na

    high charge density of the positive ion limited the

    availability of the valence electrons e.g. Hg

    Big difference between m

    .p.and b.p.

    In molten state, m

    ost metallic

    bond are not broken

    Metallic crystal (G

    iantm

    etallic structure)

    close-packed structure (74%)

    hexagonal close packing(h.c.p.)

    C.N. = 12

    abab... pattern

    (face centred) cubic closepacking (f.c.c. or c.c.p.)

    C.N. = 12

    abcabc... pattern

    tetrahedral holes andoctahedral holes

    open-structure (68%)body centered cubic (b.c.c.)

    C.N. = 8

    Determ

    ination of no. of atoms

    in an unit cell10. M

    etallic bonding.mm

    ap - 22/2/2005 -

  • Intermolecular

    Forces

    Type of dipole (polarm

    olecule)

    permanent dipole

    permanent separation of centre of positive charge and centre of negative charge

    possessed by all polar molecules (dipoles)

    instantaneous/temporary

    dipole

    the fluctuation of electron cloud createsan instantaneous dipole

    possessed by all kinds of molecules including polar m

    olecules

    induced dipoleinduced by a perm

    anent dipole

    induced by instantaneous dipole

    van der Waals forces

    EvidenceReal gas equation

    Real gas doesnot obey idealgas lawperfectly

    assumption of

    ideal gas law

    individual particle occupies novolum

    e

    no interaction (attraction andrepulsion) am

    ong particles

    van der Waals' constants

    a - attraction among particles

    b - volume of individual particle

    Condensation of solid and liquid at low tem

    p.

    Origin

    dipole-dipole interaction

    also called permanent

    dipole-permanent dipole

    interaction

    attractions among opposite

    ends of permanent dipole

    dipole-induced dipoleinteraction

    also called permanent dipole

    induced dipole interaction

    a permanent dipole induce a

    temporary dipole onto another

    polar/non-polar molecule

    the opposite ends attractedeach other

    instantaneous dipole-induceddipole interaction

    other names

    dispersion force

    London force

    temporary dipole-tem

    porarydipole interaction

    induced dipole-induced dipoleinteraction

    an instantaneous dipole inducea tem

    porary dipole on anotherm

    olecule

    the opposite end of differenttem

    porary dipoles attract eachother

    Strength (1/10 ofcovalent bond)5-50 kJm

    ol-1

    Polarm

    olecules

    with dipole-dipole

    interaction, dipole-induceddipole interaction andinstantaneousdipole-induced dipoleinteraction

    stronger overallstrength form

    olecules with

    comparable size

    higher b.p. and m.p.

    Non-polar

    molecules

    with instantaneous

    dipole-induced dipoleinteraction only

    weaker overall strength

    for molecules w

    ithcom

    parable sizelow

    er b.p. and m.p.

    depending on thepolarizability ofthe m

    olecule

    increases with increasing

    molecular size / surface area

    e.g butane vs 2-methylpropane

    branched isomer

    of hydrocarbonhas low

    er boilingpoint

    polarizability of constituent atoms

    e.g. telfon/poly(tetrafluoroethene)

    van der Waals' radius

    half of the internuclear distance between 2 atom

    sof the sam

    e element w

    hich are not chemically

    bonded together in a crystal lattice

    Molecular crystal

    iodine

    face-centred cubic structure(f.c.c)

    dry ice

    face-centred cubic structure(f.c.c)

    Hydrogen bond

    An exceptionally strong directional dipole-dipole interaction

    Attraction between a

    naked proton and a lonepair

    hydrogen atom bonded onto a very

    electronegative atom / entity

    H on F, O

    and N

    including H on CH

    Cl3lone pair on a very electronegative atomlone pair on F, O

    and N only

    Strength (1/10 of covalent bond)5-50 kJm

    ol-1

    overall strength depends on

    difference in electronegatvitiy

    average no. of hydrogen bondper m

    olecule

    2 per H2O

    molecule, 1 per H

    F,N

    H3, M

    eOH

    molecule

    hydrogen bonded molecules also

    possesses van der Waals' forces

    Hydrogen bonded m

    olecule has higher boiling point thatordinary polar m

    olecule with com

    parable size.

    e.g. HF, H

    2O, N

    H3, M

    eOH

    comparing w

    ith otherm

    olecules with com

    parable size

    Estimation of strength of hydrogen bond

    Experimental

    H-bond form

    ationM

    ixing trichoromethane and ethyl ethanoate

    H-bond breaking

    Mixing ethanol and hexane

    Period 2 hydrides comparing w

    ith hydrides of period 3 to 5

    intermolecular and

    intramolecular hydrogen

    bond

    intermolecular

    formed betw

    een molecules

    (usually) gives higher b.p.

    (usually) gives higher solubilityin w

    ater

    formation of new

    intermolecular forces >

    breaking of old intermolecular

    forcesa substance w

    ould be soluble

    ability to form hydrogen bond w

    ith water

    overall polarity of the molecule

    (actually more im

    portant thanability to form

    H-bond)

    e.g. trans-butenedioic acid

    e.g. alcohols

    intramolecular

    formed w

    ithin a molecule

    prevents the formation of interm

    olecular hydrogen bond(usually) gives a low

    er b.p.

    Examples

    dimerization of carboxylic

    acids in vapour state /non-aqueous solvent

    forming bond is better than

    not forming bond

    forming strong bond is better

    than forming w

    eak bond

    unique properties of water

    highest density at 4 C

    Low density of ice

    water expands upon freezing

    open structure of icediam

    ond like structure

    six mem

    bered rings of O linked

    by O-H

    O linkage

    Variation of density with

    temperature (K.E.)

    from below

    0 C to 0 C

    thermal expansion of solid

    structuredensity drops

    at 0 Cm

    elting of ice

    rapid collapsing of open structuredensity increases sharply

    from 0 C to 4 C

    continuous collapsingof open structure

    density increases continuously

    still possesses certain hexagonal network

    from 4 C to 100 C

    thermal expansion of liquid w

    aterdensity drops

    formation of secondary

    structure in protein and DN

    A

    Proteinsingle helical structure

    hydrogen bond between N

    -H and C=O

    group among different am

    idegroups along the polypeptide chain

    DN

    Adouble helical structure

    hydrogen bond between

    heterocyclic bases on 2separate strands

    cytosine - guanine pair3 H

    -bonds

    thymine - adenine pair

    2 H-bonds

    11. Intermolecular Forces.m

    map - 2005/5/23 -

  • Structure andproperties of

    materials M

    olecular structure

    Simple m

    olecular

    e.g. H2O

    , NO

    2, S8, P4

    under 100 atoms

    fat and oil - marginal cases, w

    ith just over 100 atoms

    weaker interm

    olecular forces

    usually gases, liquids or low m

    elting solids

    soft and weak

    solubility depending on the polarity of the solute and solventIn general, like dissolves like

    Macrom

    olecular

    e.g. starch, protein, plastic

    over thousands of atoms

    stronger intermolecular forces

    usually solid

    non-conductingno delocalized electrons

    Giant structure

    Giant covalent structure

    e.g. diamond, quartz, graphite

    strong covalent bond

    hard

    high density

    high melting point

    insoluble in any solventinterm

    olecular forces never stronger than covalent bond

    usually non-conductor ofelectricity

    bonding electrons in most covalent bonds are not delocalized

    usually poor conductor of heat

    Exception - diamond is an

    excellent conductor of heatthe rigid structure transm

    its thevibration of the C atom

    s efficiently

    Speical case : Graphite

    brittlew

    eak van der Waals' forces betw

    een layers

    slipperyflat hexagonal layers

    weak van der W

    aals' forces between layers

    conductingpresence of delocalized electrons along the hexagonal layers

    high melting, even higher than diam

    ondstrong C-C bond, bond order 1 1/3

    lower density than diam

    ondlarge space betw

    een layersw

    eak van der Waals' forces

    between layers

    Giant ionic structure

    strong ionic bond

    high m.p. and b.p.

    hard

    high density

    brittleslight dislocation brings ions of sim

    ilar charge togetherrepulsion cleaves the crystal

    presence of ionsthe ions are not free to m

    ove in solid stateonly conducts in m

    olten or aqueous state

    If soluble, only soluble in aqueous solventdipole - ion interaction

    increase in disorderness

    Giant m

    etallic structure

    sometim

    e, strong metallic bond

    high m.p. and b.p.

    hard

    high density

    Presence of sea of delocalized electronsm

    alleable and ductile

    high conductivity of heat and electricity

    Soluble in mercury

    12. Structures and properties of m

    aterials.mm

    ap - 2005/6/5 -

  • Rate of Chemical

    Reactions Definition of Rate

    Change in quantity per unit time

    Quantity is usually expressed in m

    oldm-3

    Other possible units : m

    ol, g For gases : Pa, m

    mH

    g, atm,

    cm3, dm

    3

    Time is usually expressed in s

    Unit of rate of reaction

    Depending on the units of quantity and tim

    e

    Usually expressed in m

    oldm-3s-1

    Different rate

    Average Rate

    Instantaneous rate

    Initial Rate(Instantaneous rate at t = 0)

    Differential form

    of rate equation / law

    Measuring of

    Reaction Rate

    Constant time approach

    (fix the time interval

    and determine the

    amount present)

    By titrationQ

    uenching of reaction before titration is done

    by sudden cooling

    by dilution with a large am

    ount of water

    by removing the catalyst

    by removing one of the reactant

    By measuring a physical quantity related to the

    amount of a chem

    ical

    Measuring of volum

    e of gas

    Measuring of colour intensity

    Transmittance and Absorbance

    Need of a calibration curve

    Measuring of m

    ass of thereaction m

    ixture

    Constant amount approach

    (fix the amount to be

    reacted and determine

    the time required to

    complete the reaction)

    Disproportionation of

    Na2S2O

    3 in acidic medium

    constant amount of S ppt.

    produced to mask the cross

    Methanal Clock

    experiment

    constant amount of m

    ethanal reacted / HSO

    3- consumed

    phenolphthaleinindicator

    Iodine Clockexperim

    entI- vs H

    2O2

    constant amount of I2 produced / S2O

    32- consumed

    starch indicator

    Reactionbetw

    een Br- andBrO

    3- in acidicm

    edium

    constant amount of Br2 produced / phenol consum

    ed

    methyl red

    indicator

    Factors affectingReaction Rates

    Concentration of reactants

    Pressure

    Temperature

    Surface Area

    Catalyst

    Light

    v

    13. Rate of C

    hemical R

    eactions.mm

    ap - 2005/6/5 -

  • Rate Equations andOrder of Reactions

    Rate Equation / Law

    Differential form

    Ordinal form

    Order of reactionOrder with respect to individual reactant

    Overall order of the reaction

    Rate constant k

    Unit of rate constant is depending on the overall order ofthe reaction

    A value depending on temperature only

    Different order withrespect to a reactant

    Zeroth order

    the rate is independent of theconcentration of the reactant

    Usually occurring in catalyzed reactionwhere the availability of the catalystsurface is the limiting factor of the rate

    First order

    the rate is directly proportional to theconcentration of the reactant

    Second order

    the rate is directly proportional to thesquare of the concentration of thereactant

    Integratedform

    Zeroth order reaction

    half life

    First orderreaction

    half lifecarbon-14dating

    The concentration of C-14 inatmosphere is assumed to beconstant

    The percentage of C-14 in a livingorganism is assumed to be constant.

    By comparing the percentage/betaemission of C-14 in an archaeologicalsample and the percentage/beta emissionof C-14 in a new sample, the age of thearchaeological sample can be estimated.

    The rate of decay is independent oftemperature as it doesn't involve collisionamong particles

    Second order reaction

    half life

    Determination ofrate equation / law

    Initial Rate method From the initial rate with different initial concentrations

    By plottinggraph

    If there is more than one reactant involved, keep the concentrations of all reactantsother than the one being studied virtually constant by keeping them in large excess

    By trial anderror

    By plottingconcentration againsttime Straight inclined line

    zeroth order

    By plotting rate againstconcentration

    Horizontal line zeroth order

    Straight inclined line first order

    parabola second order

    By plotting rate against [A] or [A]2 etc to see which will givea straight inclined line passing through the origin

    By plotting [A] or ln[A] or 1/[A] against time

    Plotting log (rate) against log(concentration)

    The slope will be the order of reaction withrespect to the reactant

    14. Rate Equations and Order of Reactions.mmap - 2005/1/31 -

  • The Effect ofTem

    perature Changeand Catalyst onReaction Rate

    Simple Collision

    Theory (EffectiveCollision)

    (A)Arrhenius Constant

    (Z) CollisionFrequency

    Vary only a little when the tem

    perature change

    (P) Orientation / geom

    etrical/ probability factor

    Depending on the

    nature of the reaction

    Energy larger thanactivation energy

    Arrhenius Equation

    Activation Energy

    An energy barrier the reactants need to overcome for the reaction to proceed.

    Determ

    ination ofactivation energy

    By varying the temperature and m

    easuring the rate of a reactionA plot of ln k versus 1/TA plot of ln rate versus 1/T ifinitial rate m

    ethod is usedA plot of ln 1/t versus 1/T if constantam

    ount approach is adopted

    Repeat a reaction at two

    different temperature

    In the reaction k can bereplaced by rate if initial ratem

    ethod is usedk can be replaced by 1/t if constantam

    ount approach is adopted

    Energy profile

    transition state (oractivated com

    plex)

    e.g. a pentavalent transitionstate

    can never be isolated

    Single stage reaction

    Multi-stage Reaction

    Reaction intermediate

    e.g. carbocation

    can be isolated at low tem

    perature

    rate-determining step

    (r.d.s.)The step w

    ith the highest activation energyThe step w

    ith the lowest rate

    Other exam

    ples

    Haber process

    Fe(s)

    Contact processPt(s) or V2O

    5(s)hydrogenation of oilN

    i(s), Pt(s) or Pd(s)

    Gasification of naphtha in product of tow

    n gasN

    i(s) and NiO

    Catalytic ConverterRh(s) and Pt(s)

    Enzymes

    zymase in the ferm

    entation by yeast

    Catalysis

    Effect of catalyst

    Providing analternative pathw

    ayw

    ith a differentactivation energy,usually low

    er.

    positive catalyste.g iron in H

    arber processBy breaking up a single step into a m

    ulti-stepsreaction w

    ith lower activation energy

    negative catalyste.g. H

    + in decomposition of H

    2O2

    homogeneous

    catalysis

    The catalyst has the same phase as the reactants and product

    e.g.acid-catalysedesterification

    heterogeneouscatalysis

    The catalyst has a different phase as the reactants and product

    e.g. Catalyticdecom

    positionof hydrogenperoxide bym

    aganese(IV)oxide

    chemsorption / adsorption on the surface of the catalysis

    Maxw

    ell-Boltzmann

    distribution ofm

    olecular speeds

    The distribution istem

    peraturedependent

    The total area under the curve is independent of temperature.

    i.e. the total no. of particles present

    15. The Effect of Tem

    perature Change and C

    atalyst on Reaction R

    ate.mm

    ap - 21/5/2005 -

  • Dynam

    ic Equilibrium

    Equilibrium

    A state where no m

    acroscopic

    change is observed.

    All chemical equilibria are

    dynam

    ic in nature. i.e.

    forward rate = backw

    ard rateExam

    ples

    Thermal dissociation of

    calcium

    carbonate

    Esterification

    Action of acid and alkali on

    bromine w

    ater

    Action of acid and alkaline on

    potassium dichrom

    ate

    Action of acid and alkali on

    bismuth chloride

    The amounts of reactant and

    product are usually not equal

    in an equilibrium

    .

    Equilibrium

    position

    Definition : a set of reactant and product concentration

    Reaction Quotient (Q

    )

    Using of equilibrium

    constant and reaction quotient

    to predict the direction to which the equilibrium

    position w

    ill be shifted.

    Q = K : the system

    is at equilibrium

    Q > K : the equilibrium

    position will be shifted to the left

    Q < K : the equilibrium

    position will be shifted to the right

    Le Chatelier's principle

    The principle states that when a system

    in equilibrium is

    subjected to a change, the system

    will response in a w

    ay so that

    the effect of the change imposed w

    ill be minim

    ized.

    Effect of change in concentration

    Effect of change

    in pressure

    by decreasing/increasing the volume

    by adding one of the product/reactant

    by adding an inert gas

    this has no effect on

    the equilibrium

    position

    Effect of change in

    tem

    perature

    Use of change in

    distribution of m

    olecular

    speed to explain the

    effect of change in

    temperature on the

    equilibrium

    position.

    The rate of a reaction

    with a higher

    activation energy is

    more sensitive to the

    change in

    tem

    perature

    Effect of catalyst

    Catalyst has no effect on the equilibrium position.

    It only shortens the tim

    e required for a system to

    reach a state of equilibrium

    .

    Catalyst does not change the relative stability of

    the products comparing w

    ith the reactants

    Equilibrium

    Law

    At equilibrium and only at equilibrium

    ,

    the order of reaction with respect to a

    species w

    ill be the same as the

    stochiom

    etric coefficient of the species

    Equilibrium

    constants

    Examples

    Generic equilibrium

    constant, Kincluding all species

    Equilibrium constant in term

    s

    of concentration, Kc

    Equilibrium constant in term

    s

    of partial pressure, Kp

    Unit of equilibrium

    constant

    Determ

    ination of Equilibrium

    constant

    The equilibrium concentrations of all species are determ

    ined by the

    initial concentrations of them and the equilibrium

    concentration of

    any one of them.

    Esterification

    Assuming that the rate of reaction is extrem

    ely slow

    and quenching is not required before any titration is

    done.

    Formation of

    [Fe(NCS)]2+(aq)

    complex

    Construction of a

    calibration curve

    using colorimeter

    Preparation of solutions with

    know

    n [Fe(NCS)]2+(aq)

    concentration using excess

    Fe3+(aq) or N

    CS-(aq)

    Determ

    ination of the equilibrium concentration of

    [Fe(N

    CS)]2+(aq) using colorimeter and the calibration

    curve prepared

    Reaction between

    Fe2+(aq) and Ag+(aq)

    Assuming that the rate of reaction is extrem

    ely

    slow and quenching is not required before any

    titration is done

    The titration is self-indicating if standard

    KCNS(aq) is used in the determ

    ination of the

    concentration of Ag+(aq). The solution will turn

    red at the end point w

    ith the formation of

    blood red [Fe(N

    CS)]2+(aq) complex.

    Significance of equilibrium

    constant

    The value shows the relative am

    ounts of products and reactants when

    the system

    is at equilibrium i.e. extent of reaction at equilibrium

    .

    The value is depending on the

    relative stability of the

    products comparing w

    ith the

    reactants

    The value is temperature

    dependent.

    Excluding those species having no

    effect on the equilibrium position e.g.

    solvent(species in large excess),

    insoluble solid/liquid

    16. Dynam

    ic Equilibrium

    .mm

    ap - 6/4/2005 -

  • Acid Base

    Equilibrium

    I : Basic Concepts

    Different

    definitions

    Arrhenius definition

    acid : substance that produces

    H+ in w

    ater

    base : substance that produces

    OH

    - ions in water

    Bronsted Lowry

    definition

    acid : proton donor

    base : proton acceptor

    Lewis defintion

    acid : electron acceptor

    base : electron donor

    An Arrhenius acid (base) must be a Bronsted Low

    ry acid (base) and a

    Bronsted Lowry acid m

    ust be a Lewis acid (base) but not vice versa.

    Auto-ionization

    (dissociation) of w

    ater

    Water is a very poor conductor as it alw

    ays possesses very small

    am

    ount of H3O

    +(aq) and OH

    -(aq) ions i.e. 1 pair of ions for every 556

    million w

    ater molecules

    A neutral solution

    has a pH

    7

    only at 25C.

    pH scale

    Originated from

    French "pouvoir hydrogene" (power of hydrogen).

    Every unit increase / decrease in pH scale m

    eans a ten-fold decrease / increase

    in the concentration of hydroxonium (H

    3O+) ion

    Measurem

    ent of pH

    using pH paper / universal indicator

    Using pH

    meter

    Need of calibration using a

    buffer solution before use

    Acidity and

    Basicity

    constants

    A more negative pKa (pKb) value m

    eans a larger Ka (Kb)

    value, thus a stronger acid (base).

    Successive

    ionization of polyprotic

    (polybasic) acid

    Ka1 is always m

    uch

    larger than Ka2

    HA- is relatively m

    ore stable

    when com

    paring with H

    2A than

    A2- when com

    paring with H

    A-

    A2- has a much higher charge

    density than H

    A- and has a very

    high potential energy i.e. more

    unstable

    It is more difficult to rem

    ove a

    positive proton from negative

    H

    A-(aq) than from electrically

    neutral H

    2A(aq)

    Beside the small value of Ka2, the second step of the

    ionization is also suppressed by the presence of H

    3O+ from

    the first step of dissociation w

    hich will tend to shift the

    equilibrium

    position of the second step to the left. This is

    known as com

    mon ion effect (of H

    3O+ in this case).

    Eventually, the am

    ount of H3O

    + from the second step of

    ionization w

    ill be very minim

    al.

    Determ

    ination of acidity constant Ka by half-way neutralization

    The value of Ka is only depending on temperature but the % of dissociation of a

    w

    eak acid is depending on concentration as well.

    Introduction of the concept of

    conjugate acid-base pair

    17. Acid B

    ase Equilibrium

    I.mm

    ap - 6/4/2005 -

  • Acid-base

    Equilibrium II :

    Buffers andIndicators Buffer solution

    Definition : A solution that resists change in pH

    when

    a small am

    ount of acid or base is added to it.

    Composition : A m

    ixture of weak acid and w

    eak basei.e. usually a w

    eak acid (base) and its salt i.e. theconjugate base (acid).

    In the calculation of the pH of a buffer solution, it is

    assumed that the inter-conversion betw

    een the acid(base) and its salt upon m

    ixing is negligible.

    The buffering capacity of a buffer solution is dependingon the concentrations of the acid/base and its salt.

    Acid-base

    indicators

    Acid-base indicator is usually a weak acid (base) w

    hichcolour is different from

    its conjugate base (acid).

    Hum

    an eyes are only capable to detect a colour changew

    hen the concentration of one coloured substance is more

    than 10 times of another coloured substance.

    Double

    indicatortitration

    Add phenolphthalein to the mixture, then

    do the first part of the titration (V1).Thereafter, add m

    ethyl orange and do thesecond part of the titration (V2).

    Examples

    A mixture of N

    a2CO3 (V1+V2)

    and NaH

    CO3 (V2)

    A mixture of N

    aOH

    (V1) andN

    a2CO3 (V1+V2)

    A mixture of N

    aOH

    (V1)and N

    aHCO

    3 (V2)

    Choosing ofindicator andpH

    titrationCurves

    strong acid vsstrong alkali

    phenolphthaleinor m

    ethyl orange

    strong acid vsw

    eak alkalim

    ethyl orange

    weak acid vs

    strong alkaliphenolphthalein

    weak acid vs

    weak alkali

    no suitableindicator

    18. Acid-base E

    quilibrium II.m

    map - 21/5/2005 -

  • Redox Reactions

    Definition

    of redoxreaction

    Oxidation

    Addition of oxygen atom

    Removal of hydrogen atom

    Losing of electron

    Increase in oxidation no.

    Reduction

    Removal of oxygen atom

    Addition of hydrogen atom

    Gaining of electron

    Decrease in oxidation no.

    Disproportionation

    reaction

    A redox reaction inw

    hich an element

    undergoesoxidation andreduction at thesam

    e time.

    Oxidation

    no.

    no. of proton - no. of electron associatedw

    ith an atom assum

    ing that all bondingelectrons are belonging to the m

    oreelectronegative atom

    Rules ofassigningoxidationnum

    ber

    the sum of the oxidation no. of

    all atoms in a species equals

    the overall charge carried bythe species.

    BalancingRedoxEquations

    By Combining

    two half

    equations

    Oxidation

    halfequation

    Remem

    ber thecom

    mon strong

    reducing agents

    reducing agent isthe reagent w

    hichis oxidized in aredox reaction

    Reductionhalfequation

    Remem

    ber thecom

    mon strong

    oxidizing agents

    oxidizing agent isthe reagentw

    hich is reducedin a redoxreaction

    By change inoxidation no.

    The change in oxidation no. per atom is the sam

    eas the no. of electron being lost or gained by thatparticular atom

    Figure out the no. of atom that w

    ill be oxidized andthe no. of atom

    that will be reduced by using the

    change in O.N

    .

    Add H2O

    to either side of the equation to get thenum

    ber of O atom

    balanced if necessary.

    Add H+ to either side of the equation to get the

    number of H

    atom balanced if necessary.

    Check the presence of H+ or O

    H- on the both sides

    to ensure it agrees with the acidity/alkalinity of

    the medium

    used.

    Check them

    edium of

    reaction

    For reactions in acidic medium

    , there shouldbe no O

    H- ion on the both sides of the

    equation

    For reactions in alkaline medium

    , thereshould be no H

    + ion on both sides of theequation

    19. Redox R

    eactions.mm

    ap - 2005/5/23 -

  • Electrochemical Cells

    Electrode potential(of a half-cell)

    Definition : The difference betw

    een the charge on an electrode and thecharge in the solution in w

    hich the electrode is imm

    ersed in.

    Practically, it is not possible to determine the absolute potential of a half cell. Therefore, for the

    sake of comparison, the electrode potential of standard hydrogen electrode is defined as 0 V.

    The value is depending on the activity of the electrons in the electrode

    This value is also related to the nature, including concentration, of theelectrolyte in w

    hich the electrode is imm

    ersed in.

    By definition, the electrodepotential of an unknow

    n half-cellis the e.m

    .f. of anelectrochem

    ical cell measured at

    standard condition where a

    standard hydrogen electrode(SH

    E) is used as the left-handelectrode and the unknow

    nelectrode is used as theright-hand electrode.

    By definition, overall e.m.f of a cell = E(right) - E(left).

    When hydrogen electrode is used as the left-hand electrode,

    E(right, the unknown electrode) = overall e.m

    .f. of the cell

    The sign of the electrode potential of the unknown half cell

    is the same as the polarity of the right hand electrode

    (unknown half cell) in the cell diagram

    .

    Half

    cell

    Involvingm

    etal

    The metal concerned w

    ill be usedas the electrode im

    mersed in a

    solution containing the salt of them

    etal. e.g. Cu(s) | CuSO

    4(aq)

    In some cases, the solution w

    ill be saturatedw

    ith the salt and with som

    e insoluble saltpresent. e.g. Ag(s)|AgCl(s)|Cl-(aq)

    Not involving

    metal

    An inert electrode, e.g. Pt, is imm

    ersedin a m

    ixture of the reduced and oxidizedform

    s of the reagent concerned. e.g. Fe3+(aq) /Fe2+(aq) , I2(aq)/I-(aq)

    e.g. Pt(s) | Fe2+(aq) , Fe3+(aq)

    e.g. C(graphite) | 2I-(aq) , I2(aq)

    Standard hydrogen electrodePlatinized = covered w

    ith platinum black

    = covered with platinum

    powder

    Pt(s) | H2(g) | 2H

    +(aq)

    Electrochemical cells

    The electrodes of the two half cells are connected

    together by an external wire.

    The electrolytes of the two

    half cell are connectedtogether by using a salt bridge.

    Only KN

    O3 and N

    H4Cl are used in the salt

    bridge since the migration speed of the

    cation and anion are similar and the voltage

    reading will not be affected.

    The salt bridge is used to provide cations andanions to balance the negative and positivecharge cum

    ulated in the two half cells during

    the discharge of the cell.

    In some electrochem

    ical cell,a porous partition is used toseparate the tw

    o electrolytesinstead of using a salt bridge.

    The use of porous partition will create a

    junction potential across the partition andthe voltage m

    easured will be different from

    the case if a salt bridge is used.

    Measurem

    ent of e.m.f of an

    electrochemical cells.

    To measure the e.m

    .f. of a cell, the currentflow

    ing through the external circuit should bekept as m

    inimal as possible.

    Use a voltm

    eter with high im

    pedance

    Use a potentiom

    eter

    IUPA

    C Celldiagram

    A set of symbols are used to represent the set up of an electrochem

    ical cell.

    Symbols

    used

    Depending on the em

    phasis and interpretation of the actual setup, it may be

    possible to construct more than one IU

    PAC cell diagram for a given chem

    ical cell.

    For a given half-cell, no matter it is being used as a left-hand or right-hand electrode, the reduced form

    should be placed on the leftif the reduced form

    and oxidized form are in the sam

    e phase. e.g. Pt(s) | Fe2+(aq) , Fe3+(aq) and Fe2+(aq) , Fe3+(aq) | Pt(s)

    Some

    examples

    Primary cell

    e.g. Zinc-carbon cell

    Secondary cell(rechargeablecell)

    e.g. Lead acid accumulator

    Fuel celle.g. H

    ydrogen-oxygen fuel cell

    Electrochemical Series

    (ECS)

    Electrochemical series is constructed by arranging the standard electrode

    potentials measured in an ascending order. i.e. the m

    ost negative value first.

    By convention, the reduction half equations are tabulatedin the ECS. Therefore, standard electrode potential is alsoknow

    n as standard reduction potential.

    The species on the left of thetable are oxidizing agents.

    The species on the right of thetable are reducing agents.

    Those oxidizing agents at the bottom of the list are strong oxidizing agents

    while those reducing agents at the top of the list are strong reducing agents.

    Concentration andtem

    peraturedependence ofelectrode potential

    The values list in an ECS are all measured at standard conditions

    and all species involved are in their standard states.

    Dependence on concentration

    An increase in concentration of an oxidzing agent will shift the

    equilibrium position to the right and m

    ake the value more positive.

    An increase in concentration of a reducing agent will shift the

    equilibrium position to the left and m

    ake the value more negative.

    The value is only depending onconcentration (including partial pressure incase of gas) and tem

    perature, the size ofthe electrode has no effect on the value.

    Nernst Equation

    (Not required in H

    KAL syllabus)Q

    : reaction quotient

    Use of

    electrochemical

    series

    Compare the strengths of oxidizing agents (or reducing agents)

    To predict the energeticfeasibility of a redoxreaction

    A redox reaction with a

    positive overall e.m.f.

    will be energetically

    feasible.

    The feasibility of a reaction is also depending on thekinetic stability (activation energy) of the system

    which is

    not related to the overall e.m.f. determ

    ined.

    e.g. disproportionation of Cu+(aq) in water

    To predict the overall e.m.f.

    of an electrochemical cell

    To ensure the overall e.m.f. of the cell be positive,

    E(cell) = E(cathode) - E(anode) = E(m

    ore positive) - E(less positive)

    20. Electrochem

    ical Cells.m

    map - 9/5/2005 -

  • Phase Equilibrium I :One-component system

    PhaseDefinition : region with identical properties.Phase is not the same as physical state. Usually, there are only 3 physical states i.e. solid, liquid and gas. e.g. Diamond and graphite are both in solidstate but they are two different phases of carbon.

    PVT surface

    Consider an ideal gas obeying ideal gas law PV=nRT, for a given amount of gas, P is a function of V and T. i.e. P(V,T).

    By plotting a graph usingP as the z-axis, V as thex-axis and T as they-axis, a PVT surface ofan ideal gas can beconstructed. PVT surface of of a

    real substance e.g. water

    As it isdifficultto study a3-dimensionalsurface,theprojectionsalong thevolumeaxis andthetemperatureaxis areusuallystudiedseparately.

    The projection alongthe temperature axis(Isotherms)

    Ideal gas

    The isotherms of an ideal gasshows that no matter how lowthe temperature is, the idealgas is still a gas and the volumeis always inversely proportionalto pressure.

    Real substance e.g. water Real gas doesn't obey Boyle's law at low temperature.

    Real gas starts condensing at a temp. lower than the critical temp. of the substance.

    Theprojectionalong thevolume axis(isochors)

    Ideal gasThe isochors of an ideal gas shows that no matter how low the temperature, the ideal gas is still a gas and has zero volume at 0 K.

    Real substance e.g. water

    The diagram is known as phase diagram.critical temp : above this temperature, gas cannot be compressed into liquid without cooling.AB : sublimation curve - conditions that solid and vapour can coexist at equilibrium.BC : vaporization / boiling curve - conditions that water and vapour can coexist at equilibrium.BD : fusion / melting curve - conditions that solid and liquid can coexist at equilibrium.B : triple point - the conditions that solid, liquid and vapor can coexist at equilibrium.BE : supercooling curve - the condition that a liquid exists at a temp. lower than its meltingpoint and the liquid is at a metastable state. This is because freezing also requires activationenergy. If a liquid is cooled very calmly, the liquid may become supercooled withoutsolidification.

    Real gas condenses at low temperature and becomes liquid and solid.

    Specialfeatures ofthe phasediagram ofwater

    The fusion curve of water has a negative slope. This implies that themelting point of water decreases with increasing pressure. When a greatpressure is applied to ice, the open structure of ice will collapse and theice will be turned to water.According to the Le Chatelier's principle, when a pressure is applied to an equilibriumsystem, the system will react in a way to minimize the effect of the change imposed. Forice, it will turn to water which has a smaller volume to lower the increase in pressure.

    Specialfeatures ofthe phasediagram ofcarbondioxide

    Like most substances, the fusion curve of carbon dioxide has a positiveslope. This implies that the melting point of carbon dioxide increaseswith increasing pressure.The triple point pressure is higher than atmospheric pressure. This implies that dry ice willsublime directly to gaseous carbon dioxide without going through the liquid state.

    Specialfeatures ofthe phasediagram ofcarbon

    It is possible to convert graphite to diamond by applying pressure tographite. However, the rate of conversion is very slow as this involvesrearrangement of atoms in solid state.If graphite is heated to molten state and allowed to crystallize under high pressure,artificial diamond can be made. Moreover, the crystallization is very fast comparing withthe natural process of formation of diamond, the diamond crystal obtained will be smalland may not be suitable for making jewelry.

    Isotherms

    Isochors

    Isotherms

    Phase diagram ofwater

    21.Phase Equilibrium I . One-component system.mmap - 2005/5/9 -

  • Phase Equilibrium II :

    Two-Com

    ponent System

    Difference betw

    een1-com

    ponent and2-com

    ponent systems

    In a 1-component system

    , the properties of a substance is a function of P and T. This requires a 3-dimensional space to represent.

    In a 2-component system

    , theproperties of a substance w

    illbe depending on P, T and X(m

    ole fraction) which w

    illneed a 4-dim

    ensional space torepresent.

    Instead of studying the problem in a 4-dim

    ensional space, the study will be lim

    ited to the case in which a liquid and its

    saturated vapour coexist in equilibrium.

    For a 1-component system

    , the (saturated) vapour pressure(P) of a substance is a constant at a given tem

    perature.

    For a 2-component system

    , the (saturated) vapourpressure at a given tem

    perature will be a function of X

    (mole fraction) of the com

    ponent present.

    Raoult's Law

    The boiling point of an ideal solution varies linearly with the com

    position approximately.

    Deviation from

    Raoult's Law(non-ideal solutions)

    Positivedeviation

    Azeotropic mixture (or constant boiling m

    ixture) - A mixture w

    ith a constant composition

    when it is being boiled continuously.

    i.e. the composition of the liquid m

    ixture = the composition of the vapour

    The components cannot be

    separated by fractionaldistillation com

    pletely.

    Extreme positive

    deviation(2 im

    miscible liquids)

    The 2 components vaporize independently and give a total

    vapour pressure higher than that of either component.

    Negative

    deviation

    Extreme negative

    deviation(a solution ofinvolatile solute)

    The lowering of vapour pressure w

    ill cause depression in melting point and elevation of boiling point of the solvent.

    22. Phase E

    quilibrium II . Tw

    o-Com

    ponent System

    .mm

    ap - 19/5/2005 -

  • Phase Equilibrium III :

    Three-Component

    Systems

    Partition of a solutebetw

    een 2 phases

    Solvent Extraction(betw

    een 2 imm

    isciblesolvents)

    Partition of a solute between 2 im

    miscible solvents

    At equilibrium, the rates of diffusion of the solute betw

    een two

    imm

    iscible solvents in opposite directions are the same.

    Partition Law - At a

    given temp. and at a

    state of equilibrium,

    the ratio ofconcentrations of asolute in tw

    oim

    miscible solvents is

    constant.

    As the unit of concentrationw

    ill be canceled out in thecalculation, the unit can beexpressed in any unit andpartition coefficient w

    ill haveno unit eventually.

    Most com

    mon organic solvent are lighter than w

    ater except chloroform(CH

    Cl3), tetrachloromethane(CCl4) and

    1,1,1-trichloroethane

    If the density of the solvents are not known, w

    hen we say solute A

    is partitioned between solvent B and C, it usually m

    eans

    The law is only application to the case if

    the solute has the same m

    olecularstructure in the tw

    o solvents.

    e.g. The partition law is not applicable to the case w

    here ethanoicacid is partitioned betw

    een hexane and water as ethanoic acid exists

    as dimm

    er in hexane (non-polar solvent) and as monom

    er in water

    (polar solvent)

    It would be m

    ore effective to carry out a solvent extraction in successive extractions, a small portion at a tim

    e, for a given amount of solvent.

    Paper Chromatography

    (between a stationery phase

    and a mobile phase)

    Partition of a solution between a

    stationery phase and a mobile phase

    Stationery phasee.g. the m

    icroscopic water film

    on the surface of the chromatography paper

    e.g. silica gel on an aluminium

    foil

    Mobile phase

    e.g. different kind of solvent or mixture of solvents

    At a given temperature, w

    ith agiven chrom

    atography paperand a given solvent, the solutebeing analyzed ischaracterized by its Rf value

    Analysis of amino acids - A m

    ixture of colourless amino acids can be separated by paper

    chromatography. The positions of am

    ino acids spot in the chromatograph can be detected by spraying

    with ninhydrin (a developer), w

    hich reacts with am

    ino acids to yield highly coloured products (usuallypurple in colour).

    23. Phase E

    quilibrium III . Three-C

    omponent S

    ystems.m

    map - 2005/5/23 -