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      1 

     AUSTRALIAN CHEMISTRY OLYMPIAD(AChO)

    2015PREPARATORY

    NOTES0. INTRODUCTION

    The AChO Summer School is a 2 week intensive program that aims to present new,

    interesting and challenging chemistry to students who have shown a talent in the subject.

    Each year, AChO students come from diverse backgrounds. In particular, the high school

    curricula vary from state to state. The aim of these preparatory notes is to provide you with

    some background information which will help you get into gear for the camp. It is important

    that you read these notes and are familiar with the material before arriving in January.

    We are also happy to provide guidance if you find any part of these notes unclear. Feel free tocontact us by email:

    •  Sam Alsop email: [email protected] 

    •  Audrey Lee email: [email protected]

    We hope you will spend some time going through these notes and we look forward to seeing

    you in the summer.

    The Australian Chemistry Olympiad Team

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    1. MATHEMATICS

    As with all branches of science, the accurate modelling of physical phenomena requires a

    mathematical toolkit to aid and concrete the description. You will find that these

    mathematical tools pop up frequently during the Summer School, particularly in the physical

    chemistry and analytical chemistry topics. For this reason, it is important to read the

    following section thoroughly and attempt the problems associated with each section. Along

    with what is covered here, it is also expected that students:

    •  are confident solving simple linear and quadratic equations and inequations

    •  are able to solve a system of simultaneous equations using elimination and

    substitution techniques

    •  are comfortable with tabulating, graphing and interpreting data (particularly during

    laboratory sessions)

    1.1 Significant Figures

    When you are doing any sort of scientific calculations you need to be aware of significant

    figures, decimal places, and how accurately you can report your results.

     Significant figures include every figure in the number except zeros that are used to place the

    decimal point

     Example. The following all have three significant figures

    a. 0.465

     b. 0.0465

    c. 15.0 (this zero is not placing the decimal point but makes the number more accuratethan 15 so is significant)

    When performing operations with numbers with different significant figures, one must be

    aware of the accuracy with which the answer can be reported. The following table is a

    summary of the rules to use:

    Operation Rule Example

    a + b = c

    a – b = c

    The answer should be given to the same

    number of decimal places as the original

    numbers (whichever of a or b has fewer)

    53.06 – 52.1 = 1.0

    c ba

    c ba

    =!

     The answer should be given to the same

    number of significant figures as the original

    numbers (whichever of a or b has fewer)

    43 ! 0.01 = 0.4

    log b a = c The answer should be given to the same

    number of decimal places as significant figures

    in the original number a.

    log10 11.2 = 1.049

    10a = c The answer should be given to the same

    number of significant figures as decimal places

    in the original number a.

    100.42

     = 2.6

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     Note that multiplication and division take priority over addition and subtraction so would be

    reported to the correct number of significant figures.

     Rounding  of a number should not occur until the final answer. When rounding the following

    rules apply for the first number excluded from the answer:

     Less than 5 (0-4): nothing will change

    Greater or equal to 5 (5-9): the last number that you have in your answer will be

    increased by one

     Example. Round the following to 2 significant figures:

    a. 34.5 = 35

     b. 0.09385 = 0.094

    c. 1.34 = 1.3

    Additional References:

    www.chem.tamu.edu/class/fyp/mathrev/mr-sigfg.html

    chemed.chem.purdue.edu/genchem/topicreview/bp/ch1/sigfigs.html

    Problem Set 1.1:

    1.1. Write the following to the correct number of significant figures or decimal places as

    required.

    a. 32.15-7.98

     b.

    c. (34.5+12.45)-1.00

    d.

    e. 10.0)11.932.12(   ÷+  

    1.2 Logarithms

    Logarithms are used to solve equations such as 10x = 100 by rearranging the equation to give

    log10 100 = x allowing for the solving of x. It is the inverse (reverse action) function of an

    exponential function (log10x is the inverse of 10x, log2x for 2

    x etc.). While it might seem

    redundant for simple propositions like the one above, once x starts to change from a whole

    integer it becomes much more important. For example, 10x = 567.

    There are two common forms of logarithms, or logs, used in chemistry. The first is log to the

     base 10 written as log10 or more simply as log. The other is the natural log, loge or more

    simply as ln, where the base e is approximately equal to 2.71828.

    For all purposes in chemistry the answer of a log can be produced using a calculator.

    However manipulating an equation may become important for simplifying problems. The

    following rules should be obeyed and apply to log and ln equally.

    04556.0253.0   !

    000.5)00.900.10(   ÷!

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    Logarithm Law

    Equation Rearranged equation(associated logarithm law) 

    Example Calculation (Solve for x) 

    10y = x log x = y Solve ex = 901

    x = ln 901 = 6.804

    log x = y 10y = x Solve log x = 1.69

    x = 101.69

     = 49

    log (a ! b) = y log (a) + log (b) = y

    (logarithm of a product of

    two elements is the sum of

    the logarithm of each

    element)

    Solve log (10 ! x) = 2

    log (10) + log (x) = 2

    1 + log (x) = 2

    log (x) = 1

    x = 10

    log (a ÷ b) = y log (a) – log (b) = y

    (logarithm of a quotient of

    two elements is the

    difference of the logarithm

    of each element)

    Solve log (x ÷42) = -0.26

    log (x) - log (42) = -0.26

    log(x) = -0.26 + log (42)

    x = 10-0.26 + log (42)

     

    x = 23

    log (ac) = y c ! log (a) = y

    (follows from the 3rd

     property)

    Solve ln (4x) = 19

    x ln (4) = 19

    x = 19 ÷ ln (4)

    x = 17.71

    logx x = y y = 1

    (logarithm of a number to

    the base of itself is 1)

    Solve ex = 901

    ln(ex) = ln (901)

    x ln(e) = ln (901)

    x = ln (901) = 6.804

    logx1 = y y = 0

    (the logarithm of 1 is 0 in

    any base y)

    Solve log (1 ÷ x ) = 2

    log (1) – log (x) =2

    log (x) = -2

    x = 10-2

     = 0.01

    log b (x) = loga (x) ÷ loga (b)

    (changing the base of a

    logarithm from a to b)

    Find log3 (7) in terms of logarithms to the

     base 10 only.

    log3 (7) = log10 (7) ÷ log10 (3)

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    Additional References:

    www.physics.uoguelph.ca/tutorials/LOG/

    www.chem.tamu.edu/class/fyp/mathrev/mr-log.html

    Problem Set 1.2.:

    1.2 Find y remembering to use the correct number of significant figures.

    a. log y = 0.20

     b. 10y = 14

    c. log y = -5.87

    d. log (12 ! 3.00) = y

    e. log (y ÷ 3.00) = 0.60

    f. log y-1

     = 5.60

    1.3 Calculus

    1.3.1 Functions, Operators and Functionals

    Functions are the working objects of basic calculus. A function of a variable, f, maps an input

     x (usually a real number) to another number f  ( x) as determined by the function. It defines a

    one-to-one relationship between one variable and another.

     Figure 1.3.1: the action of a function

    Many phenomena can be expressed as such relationships. Some examples include:

    a) the position of a car on a road could be expressed as a function of time, i.e. x(t )

     b) the population of whales in a given region of ocean might be expressible in terms

    of a function of the average krill population in that region, i.e. w pop(k  pop).

    We are most familiar with functions in their graphical form: the set of points ( x, f ( x)) on two

    axes. For instance, we have all probably seen graphs of y =  f( x) = x2 (a parabola) and

    y = f ( x) = sin( x) (the sine wave function).

    These functions are called analytic as the action of the function is expressible in some closed

    algebraic form. Note that there is no restriction that states functions have to be analytic - we

    could imagine a function which was still a one-to-one relationship but that we could not

    express with any algebra known to us (consider a random scatter of points). In fact, it is

    frequently the case that physical problems involving functions cannot be solved in any

    closed/analytic form. In this case a lot more work is required to describe the function. Luckily

    for us, most of the functions we'll deal with at the Summer School are smooth-looking

    (continuous) and analytic!

    We can also have functions of more than one variable. For instance, the population of whales

    might depend on both the population of krill and the average temperature. So we write the

    function as w pop(k  pop, Tavg), in terms of variables k  pop and Tavg.

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    We have just defined a function as a relationship that maps one real number to another real

    number. There are other kinds of relationships, such as:

    •  An operator maps a function to another function - that is, if you take a function, and

    apply an operator, you'll get another function. Lots of operators have a special

    notation, a circumflex or 'hat' above them: Oˆ

    . Examples are the differential andindefinite integral operators, as explained in the following sections.

    •  A functional maps a function to real number - that is, if you take a function and

    apply a functional, you'll end up with a real number. The simplest example of a

    functional is a definite integral, as defined below.

    1.3.2 Differentiation 

     KEY IDEA:

     Differentiation is about finding the rate of change of one variable compared to another, or

    the rate of change of a (continuous) function f(x) with respect to the variable x.

     If we have a graph comparing two variables (e.g. y, x), where y = f(x), then differentiation is

    equivalent to finding the gradient of the curve.

    The gradient of a straight line function is given by “Rise over Run”. We can express the

    gradient as , where is the change in y and x !  the change in x between two

     points (see Fig 1). For a graph/function that is curved (for instance for the graph  2x  y   = ) the

    gradient is no longer constant, but is different at each point. We get closer to the true value of

    the gradient at a certain point by decreasing the size of x !  and  y !  (see Fig 2).

    Differentiation finds the true value of the gradient by allowing x !  and to approach (or

    get infinitely close to) zero.

     Notation:

    An infinitely small value of x !  is expressed as “dx”, and  y !  as “dy”

    The true value of the gradient for any function (at a given point) is given by:

    m =" y," x#0lim

     " y

    " x=

    dy

    dx 

    m =" y

    " x y !

     y !

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    In terms of the function defining the y variable, this equivalently becomes:

     x

     x f   x x f  

    dx

     xdf  

    dx

    dy

     x   !

    "!+==

    #!

    )()()(lim

    0

     

    This object, d f /d x, is referred to as the derivative (rate of change) of the function f  with respect to the variable x.

    Differentiation changes one function into another.

    As we said, the value of the gradient (the derivative) can vary from point to point (like in a

     parabolic function). For this reason, we expect the action of taking the derivative

    (differentiating ) of a function to return another function (an operator relationship). For

    instance, to find the derivative of the function2)(   x x f     = , we start with:

     x

     x x x

    dx

    df  

     x   !

    "!+=

    #!

    22

    0

    )(

    lim   (1)

    Expanding gives:

     x

     x x

     x

     x x x

     x

     x x x x x

    dx

    df  

     x

     x

     x

    2

    )2(

    )2(

    )(2

    lim

    lim

    lim

    0

    0

    222

    0

    =

    !+=

    !

    !!+=

    !

    "!+!+=

    #!

    #!

    #!

     

    where the last line follows from the fact that " x is approaching 0.

    Therefore  xdx

    df  2= , where f ( x) = x

    2.

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    Table of Derivatives 

    Luckily for us, it is unnecessary to apply the formal definition of differentiation every time

    we want to find a derivative. In fact, in practical use - no-one does. We use short-cuts. Below

    is a tabulated list of common derivatives and how to find them. It is very important to learn

    these. 

    ( )   0=C dx 

    d  

    Differentiating a constant gives zero

    (i.e. a horizontal line has zero

    gradient)

    ( )   a b ax dx 

    d =+  

    Differentiating a linear equation gives

    a constant (i.e. the gradient of a

    straight line is constant)

    ( )   1!=   nn nx x dx 

    d  

    Differentiating a polynomial lowers its

     power by 1, but multiplies the result

     by the original power (recall the

    derivative of2

    x  y   = )

    ( )   x x  e e dx 

    d =  

    Differentiating the exponential of

    Euler’s constant e (e = 2.71828…)

    gives itself

    ( )x 

    x dx 

    d    1ln   =  

    Differentiating the natural logarithm

    gives 1/x

    ( ) ( )   x x dx 

    d x x dx 

    d  sincos,cossin   !==   Differentiating sine gives cosine, anddifferentiating cosine gives thenegative of sine

    ( ) ( ) ( ))()()lg()(   x g dx

    d l  x f  

    dx

    d k  x xkf  

    dx

    d !+!=+  

    where k, l are constants.

    The linearity property:

    - the derivative of a scalar multiple of

    a function is just the scalar times the

    derivative of the function.

    - the derivative of the sum of two

    functions is the sum of the two

    derivatives

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    Product Rule (by illustration):

    Suppose that two functions x(t) and y(t) change

    with time t  in Fig 3, e.g. the side lengths of a

    rectangle.

     Note that

    )()()(   t  yt  xt  Area   = .

    Then the change in area:

     ydx xdy Aread    +=)(  

    dx dy !  is infinitely small compared with

    either of dy , dx and is thus negligible.

    Hence:

    dt 

    dx  y 

    dt 

    dy x 

    dt 

    Area d +=

    )( 

    In general:

    dx

    df   g 

    dx

    dg  f  

    dx

     fg d +=

    )( 

    where f  and g  are arbitrary functions. This result is called the product rule and allows one to

    calculate more complicated derivatives.

    Chain Rule:

    When there is a function within a function (e.g. when )ln(sin)(  x x z    =

    , which is equivalentto stating two functional relationships:  x x y   sin)(   =   and    y y z    ln)(   = ), then

    dx 

    dy 

    dy 

    dz 

    dx 

    dz !=  

    In the given example,x 

    x x 

    x  y dx 

    dy 

    dy 

    dz 

    dx 

    dz 

    tan

    1cos

    sin

    1cos

    1=!=!=!=  

    Problem Set 1.3.2: 

    1.3.1. Evaluatedx 

    dy , using the appropriate rules:

     Differential Rules

    a.  154  2

    !+!=   x x  y   

     b. x 

    e x x  y    5cosln   !+=  

     Product Rule

    c.  x x  y    ln=  

    d.  x x  y    cossin=  

    e. 41  22 +!=   x x  y   

    Chain Rule 

    f. ( )kx  y    sin=  

    g. 2

    sin   x  y  =  

    h. ( )33 1+=   x y  

    NB: k  is a constant.

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    1.3.3 Integration

     KEY IDEAS:

    1. Integration is the opposite operation of differentiation. It computes an antiderivative.

     It takes you from a rate of change function to an explicit relationship between the two

    quantities. This means if you have a rate of change of a quantity expressible in functional form f(x) and want to calculate a direct relationship between the quantity and the

    variable, you would integrate the rate of change f(x) with respect to x.  Since this action

    takes a function to a function, it is an operator . We call this taking an indefinite integral .

    For example, if you knew the rate of change of position with respect to time (the

    velocity), as v(t ) = d x(t )/dt , you would integrate the function v(t) to find the function x(t ).

    2. Integration can also find the area under the curve ( x, f(x)) between two points. If you

    take the indefinite integral function, F(x), found from Key Idea #1 and compute the

    difference in F(x) between two points you will obtain the area (bounded by the axis)

    under the original function f(x). Since this takes a function to a number (an area), it is a

     functional . We call this taking a definite integral. 

    How can both these ideas be true? It turns out they're equivalent. This is proved below for

    your reference. This is not essential knowledge, however, and may be skipped at your

    discretion.

    Proof:

    Suppose you are trying to estimate the area under a curve )(x f   y  =  by drawing rectangles

    under the curve and calculating its area (Fig 4). By decreasing the width (   x ! ) of the

    rectangles, you arrive at a better estimate (Fig 5). Obviously, the best  estimate is when x !  is

    infinitely small (i.e. x !  approaches zero).

     Note: if the curve is in below the horizontal axis, the “area” between the zero line and the

    curve is negative in value.

     Now, let us define )(x F  y  =  which we can use to find the area under the curve of )(x f   y   = .

    Here is how the function works (see Fig 6):

    An area bordered on the left by x = A, on the right by x = B, above by )(x f   y  = , and below

     by y = 0 is given by

     AREA = )()(   AF B F    !   (This is AREA (2) in Fig 6) 

     NB: If the curve )(x f   y  =  lies below y = 0 (i.e. is negative), then the value of this “area” is

    also negative

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    Using these rules, we can see that AREA (1) is expressed as

     AREA (1) = F(A) – F(0),

    and the sum of AREA (1) and AREA (2) is given by

     AREA (1) + AREA (2) = F(B) – F(0)

    Then the area bounded by the infinitely small rectangles we were exploring in Figure 4 and 5

    is given by:

    x x f  x F x x F AREA   !="!+=   )()()(  

    As x !  approaches zero, this becomes:

    dx x f  x F dx x F AREA   )()()(   =!+=  

     Note that )()(   x F dx x F    !+  is simply another way of writing change in y (or dy ) or 

    )(x dF  ! 

    Rearranging:

    )()()()(

    x f  dx 

    x dF 

    dx 

    x F dx x F ==

    !+

     

    Thus, the differential of our “area under the curve” function is the original function.

    Definite and Indefinite Integrals:

    An indefinite integral in the above example is simply   )(x F  y   = , a reverse of differentiation.

     F(x) is called the anti-derivative.

     Notation:

    A definite integral is an expression that finds the area bound by the curve, horizontal axis,and two horizontal axis values (the vertical lines x = a and x = b).

     Notation:  ! ="b

    a

    dx x f   A F  B F    )()()(  

     ! =   dx x f  x F    )()(

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     Note: In this way (expressed in Figure 5 above), the integral notation is actually a continuous

    sum! It sums the product f(x)dx (product of the graphical height of the function f(x) and the

    width of each rectangle) continuously between the bounds a and b. This can be expressed

    mathematically as:

    ! " =

    #$%=

    b

    an

    nnn

    b

    a

     x x f  dx x f     )(lim)(  

    (where xn is the midpoint of the one of the rectangles, n is the number of rectangles, and " xn is

    the width of the each rectangle (which decreases as the number of rectangles increases)).

     Example. To find the area under the curve2

    x  y   =  between 1=x   and 4=x  , we find the

    indefinite integral, which is C x dx x    += !   32

    3

    1 (see the table below), and then turn it into a

    definite integral by substituting the lower and upper bounds (i.e. the “A” and “B”):

    213

    63

    3

    1

    3

    4

    3)(

    334

    1

    34

    1

    2==!="

    #

    $%&

    '===  (  (    x dx x dx x f  AREA

    A

     

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    Table of Indefinite Integrals 

    Luckily, once again, we do not have to use the formal definition of integration to compute

    integrals - we have rules. These rules for computing anti-derivatives are summarised in the

    table below. You'll notice that they are simply the reverse of differentiating.

     Note that indefinite integrals always contain an integration constant, C. This is because

    differentiating a constant gives 0 (previous section), so we are free to choose an arbitrary

    constant in the reverse process. The constant is often determined after the integration by using

    a physical condition given to us (for instance, the value of the new function at a particular

    value of  x). This integration constant will always cancel out  in definite integrals.

    C dx = ! 0   Integrating anything gives an infinitenumber of similar functions, all varying by a constant number C.

    C axadx   += !   Integrating a constant gives a linear

    equation

    (a curve with a constant gradient is

    obviously any straight line with that

    gradient)

    C x dx nx   nn

    += !   "1

     OR From the derivative law!

    C e dx e 

      x x 

    += !    From the derivative law!

    C x dx x 

    += !    ln1

       !    dx x 

    1is sometimes written as  ! 

     x

    dx 

    C x dx C x dx    +=+!=  "  "    sincos;cossin   Simple reversals of the differentiationrules

    [ ]   C dx x g bdx x f  adx xbg  xaf     ++=+  !  !  !    )()()()(  Integrals, like derivatives, are linear. 

    Problem Set 1.3.3:

    1.4. Integrate

    a.  !    ++   dx x x    352

     

     b.  !    +   xdx x    sincos  

    c.  ! x 

    kdx  where k is a constant

    d.  !    nx 

    kdx  where k, n are constants and n > 1

    C n

    x dx x 

    n

    n+

    +

    =

    +

     ! 1

    1

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    1.3.4 Representation as Operators

    We've talked about the fact that both differentiating (finding the derivative) and integrating

    (finding the indefinite integral) are operations, so now it's time to make some important

    distinctions.

    •   If we write before a function, it means we take that function and return its

    derivative. 

    •  Similarly, if we write after  a function and place the integration (  !   ) sign in front of it, it means we take that function and return its integral.

    e.g.  x xdx

    d 2)(

      2=  ,  !    =

    22   x xdx  

    This idea of representing a differential operator as is not to be confused with the idea of

    the derivative itself,dx

    df   , which is a well-defined quantity (a ratio of two changes) and is no

    longer an operator. The derivative can be manipulated in a normal way, for instance if

    dxdf  

    dx

    df  

    =!

    =1 

    is implied.

    We can take the derivative of a function more than once. For example, the second derivative 

    of a function  f   is defined as2

    2

    )(dx

     f  d 

    dx

    df  

    dx

    d = . For examples, the second derivative of

     position with respect to time is acceleration in mechanics. Higher derivatives are defined

    similarly.

    Note:  at no point can you cancel the d letters. Remember that df   and dx   represent

    changes in a particular variable and can be manipulated in the normal algebraic way,

    and that the d  by itself is meaningful only as an operator. 

    1.3.5 Separable Differential Equations

    These calculus ideas actually underpin most of physics (and hence physical chemistry). The

    most common form in which one finds calculus is differential equations.  Differential

    equations involve relationships between derivatives and functions, and are often incredibly

    complicated to solve. They are often unsolvable in terms of analytic functions.

    The reason they are so common in physics is because physics describes dynamics, or rates of

    change (derivatives). The most obvious exam is Newton's law of motion, which translates

    into a simple differential equation.

    ma = F,

    where F is force, m is mass and a is acceleration

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    In differential equation language, this translates to:

    2

    2

    ( )( , )

    d x t m F x t  

    dt =  

    These differential equations also have more obvious chemical applications, particularly inthermodynamics and chemical kinetics.

    At Summer School, you will only have to solve a special class of differential equations called

    separable differential equations. This means that all variables of one type can be collected

    on one side of the equation by algebraic manipulation, and all variables of the other type can

     be collected on the other side. Since both sides (infinitesimal changes) are equal everywhere,

     both sides can be easily integrated (summed) to give the explicit relationship desired. This

    technique is demonstrated in the example below.

     Solve kA

    dt 

    dA=  (where k is a constant)

     Solution: 

    (1) We separate the two variables, A and t, to either side:

    dAA

    kdt   1=  

    (2) We integrate both sides:

     !  !    =   dA A

    kdt   1

     

    (3) The desired relationship is reached:

    t

    +=  where C is the constant of integration

    (4) The constant of integration is either left arbitrary, or determined by some given

    condition (e.g. the value of A when t  = 0)

    Problem Set 1.3.5:

    1.5.1. The concentration of a reagent A (denoted [A]) is found to decrease as a function of

    time t via the following relationship:kt 

    e AA  !

    = 0][][  (where k is a constant and

    0][A  is the initial concentration of reagent A). Show that the rate of change of [A]

    (i.e.dt 

    Ad    ][) is proportional to the concentration of [A].

    1.5.2. The rate of a reaction is found to vary according to the following relation:

    2][

    ][Ak 

    dt 

    Ad != . The initial concentration (i.e. t = 0) of the reagent is [A]0 

    a. By separating variables, prove that kt C A

    !=+

    !

    ][

     b. At t = 3 sec, prove using a definite integral that k AA

    3][

    1

    ][

    1

    03

    =!

     

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    1.4 Complex Numbers

    If you were asked to solve the equation !! ! !!, what would your response be? If your

    answer is anything along the lines of “you can’t take the square root of a negative number”,

    then boy, is this the section for you! Read on, brave Summer Scholar, to discover the world of

    complex numbers.

    1.4.1 The ! in the sky

    I’m going to go out on a limb here, and define a number called !, which stands for imaginary.

    This number is defined by this simple equation:

    !   !   !! 

    ! itself is called the imaginary unit.

    “You can’t do that!” I hear you say.

    Why not? Just as all numbers are inventions, so too is this new one. As long as it fits neatly

    into our current system of numbers, why can’t we use it alongside what we already know? In

    fact, let’s see what happens when we apply some simple maths and see where that leads us:

    !!!   !!

    !

    !  !! 

    !!! !!!

    !! !!!! ! !! 

    !!! !

    !!!

    !! !!!!! ! ! 

    That’s pretty cool, so if we try multiplying ! by itself lots of times, we always end up going in

    a circle of !!!!!!!!!!   !!! 

    !! !   !!!! !   !!   !! ! !! 

    And now, we can take square roots of any number!

    Problem Set 1.4.1:

    Evaluate the following:

    a)  !! 

     b)  !!!" 

    c)  !!"" 

    d)  !!" 

    e)  !!" 

    f)  !   !!"" 

    Solve the following equations:

    g)  !!!

    !!" 

    h)  !! ! !!" 

    i)  !! ! !! ! !" ! ! 

    1.4.2 Things are going to get more complex

    So, things are about to get more complex. How so? Think a moment about the numbers you

    use every day. In mathematical jargon, these are called real numbers.

    What happens if we put both real numbers and imaginary numbers together?

    ! ! !   ! ! 

    We can’t actually combine the two into one single number – they are fundamentally different

    types of things. The best we can do is write it out just like we have above, with a realcomponent, and an imaginary component. This sum we’ve just created still represents one

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    c)  !! !!   !   ! ! !!  

    d)  !! ! !   !   !! ! !  

    e)  !! !!   !   ! ! !  

    f)  !   !! !!!!!   ! ! !!! 

    g)  !!! !! ! !! ! !! 

    h)  !!

      !   !   !!

    !   !  i)  Challenge – What is !! 

    Hint – Write !   ! ! ! !" and solve !! ! !. Remember that ! and ! are real.

    1.4.2 Egad! !’s gone crazy!

    So, for Summer School, there’s just one more important piece of info you need to know about

    complex numbers. And it’s something called Euler’s Formula.

    Perhaps you’ve come across this wacky but devastatingly beautiful equation:

    !

    !"

    ! !!

    Five of the key numbers of mathematics united in one equation. It brings a tear to your eye,

    doesn’t it? This can easily be shown using Euler’s Formula, which states:

    !!"! !"# ! ! ! !"# ! 

    We must briefly touch on radians in order to use this formula.

    What are radians you ask? So everybody’s been familiar with dividing circles into 360° since

     primary school. A radian is simply dividing the circle into !! radians. Simple! As an

    example, have a look at the following table:

    Degrees Radians0 0

    30 !   ! 

    60 !   ! 

    90 !   ! 

    180 ! 

    360 !! 

    Degrees are probably the standard units for angles that you've come across so far. However, it

    turns out that mathematically, there are very deep and fundamental reasons why radians are

    used, as annoying as they may seem right now! So we'll be using radians when we apply

    Euler's formula.

    For example, let’s prove our favourite equation by substituting !   ! ! into Euler’s Formula.

    !!"! !"# ! ! ! !"# ! !! !"#  !"#$ ! ! !"# !"#$! 

    ! !! ! !!! !  !! 

    Problem Set 1.4.3:

    Find exact expressions for the following:

    a)  !!!" 

     b)  !!"   ! 

    c)  !!!"   ! 

    d)  !!"#!"   ! 

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    2. ORGANIC NOMENCLATURE 

    The rules for naming organic compounds are set by an international body called the

    International Union for Pure and Applied Chemistry (or IUPAC for short). The basics of

    naming and drawing organic molecules will be covered here, to be expanded upon oversummer.

    2.1 Basics:

    There are three ways of writing formulae of organic compounds:

    Structural Formulae:  show all atoms, including hydrogen atoms which becomes difficult

    when molecules become more complex

     Example: 2-chloropropane

    C C C

    ClH

    H

    H

    H H

    H

    H

     

    Condensed Structural Formulae:  we just write out how many hydrogen atoms are present

    without drawing those carbon to hydrogen bonds

     Example: 2-chloropropane

    CH3

    CH

    CH3

    Cl

     

    Skeletal Formulae  – there is a carbon at every vertex and the appropriate number of

    hydrogen atoms is assumed to be bonded to each carbon atom. Hydrogen atoms are drawn

    when bonded to non-carbon atoms.

     Example: 2-chloropropane

    Cl

     

     Example: diethylamine

    NH 

    Any organic molecule contains three main components:

    •  the carbon backbone

    •  the principal functional group, which influences the properties of the compound, is

    referred to in the suffix of the name

    •  substituents, which are secondary functional groups are named as prefixes 

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    2.2 The carbon backbone:

    The name of the backbone arises from how many carbon atoms are in the longest chain within

    the molecule. For an example it is best to look at the alkanes, which are the simplest organic

    compounds, containing only carbon and hydrogen with only single bonds between them. The

     prefix (in bold) is used throughout molecule naming to describe a chain length with that manycarbon atoms in it.

    CH4  methane 1 carbon

    C2H6 ethane 2 carbons

    C3H8  propane 3 carbons

    C4H10  butane 4 carbons

    C5H12  pentane 5 carbons

    C6H14  hexane 6 carbons

    C7H16  heptane 7 carbons

    C8H18  octane 8 carbons

    We can then add any of a number of substituents to the chain and as you can see, when a

     basic carbon chain is added the same prefix appears:

    -CH3  methyl- -F fluoro-

    -CH3CH2  ethyl- -Cl chloro-

    -CH3CH2CH2   propyl- -Br  bromo-

    isopropyl- -I iodo-

    -CH2CH2CH2CH3  butyl- -NO2 nitro-

    tert -butyl- -NH2  amino-

    -OCH3  methoxy- -OCH2CH3 ethoxy-

    At this point, there are a number of rules to introduce:

    1.  When there is more than one type of substituent, order prefixes in alphabetical

    order.

     Example: bromochloromethane not chlorobromomethane.

    H

    CH Cl

    Br   

    CH3 

    -CH CH3

    -C-CH3

    CH3 

    CH3

    C

    H

    HH

    H

    H3C  CH3

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    2.  When there is more than one of a substituent type, use prefixes di-, tri-, tetra- etc. to

    signify the number. These prefixes do not contribute to the alphabetical order.

     Example: dibromochloromethane not chlorodibromomethane

    H

    CBr Cl

    Br   

    3.  To define where a substituent is attached, assign numbers to the carbon chain. Start

    numbering from the end that will result in the lowest number for the substituent at

    the first point of difference.

     Example:  1-chloropropane not 3-chloropropane

    Cl 

    4.  Put a dash between all numbers and letters, a comma between numbers, and leave no

    spaces between letters.

     Example:  1,3-dichloropropane

    ClCl 

    5.  Make sure that the backbone is the longest chain.

    Examples of other Carbon Backbones:

    Cycloalkanes:  Are alkanes which have joined into a ring. These are named in exactly the

    same way as alkanes, with a cyclo- prefix.

     Example: 1-chloro-1-methylcyclohexane

    Cl

     

    Alkenes:  Contain one or more double bonds. Similar rules to those applied to alkanes apply

    here also. But you must number only the first carbon that has the double bond, and replace the

    -ane of the alkane with -ene.

     Example: 1-butene or but-1-ene

     Example: 1,3-butadiene or buta-1,3-diene

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    The double bond takes priority over halo substituents so number from the end that will give

    the lowest number to the alkene.

     Example: 4-chloro-1-butene or 4-chlorobut-1-ene

    Cl 

    Alkynes:  Contain one or more triple bonds, and have the suffix -yne. The same rules as

    alkenes apply, but if both are present then the alkene has higher priority than the alkyne.

     Example: but-1-en-3-yne, not but-3-en-1-yne. 

    2.3 Functional groups:

    Alcohols contain the –OH group. Remember because the hydrogen is bonded to the oxygen it

    is still drawn. If the alcohol is the principal functional group, the compound is named with an

    -ol suffix, and numbering begins at the end which will give the lowest number for the carbon

    attached to the –OH.

     Example: 1-propanol or propan-1-ol

    OH 

     Example: 3-chloro-1-propanol or 3-chloropropan-1-ol

    Cl OH 

    If there is another group of higher priority, –OH is named as a substituent, with the prefix

    hydroxy- and is numbered accordingly. We will see the order of priority later.

    Carbonyl compounds  contain the R1

    O

    R2  group. Varying either R 1  or R 2  will then

    change the type of carbonyl group. There are a number of different types of carbonyl

    compounds:

    Aldehyde - when one R group is a –H and the other is a carbon atom bonded to anything else.

    These are named with the suffix -al. An aldehyde will only be present at the end of a chain as

    it cannot extend in both directions due to the requirement of the hydrogen.

     Example: butanal

    O

     

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    Ketone - when both R groups are a carbon atom bonded to anything else. These are named

    with a suffix -one. Remember that because the C=O is in the middle of the chain, its position

    will need to be shown by numbering.

     Example

    O

     

    2-butanone or butan-2-one

    Carboxylic acid: when one R group is an –OH and the other is a carbon atom bonded to

    anything else. These are named with the suffix -oic acid. Again this must be at the end of a

    chain.

     Example

    O

    OH 

     butanoic acid

    We now come to priorities of functional groups. If a molecule is composed of more than

    one functional group, the group of highest priority determines the root of the name (suffix)

    and must be included in the longest chain. Any other functional groups are treated as

    substituents and are described with the prefix.

       i  n  c  r  e  a  s   i  n  g

      p  r   i  o  r   i   t  y

     

    functional group suffix prefix

    carboxylic acid -oic acid

    aldehyde -al oxo-

    ketone -one oxo-

    alcohol -ol hydroxy-

    alkene -ene -en-

    alkyne -yne -yn-

    alkane -ane -an-

     Example: 2-hydroxypropanoic acid 

    OOH

    OH 

     Example: 2-oxopropanoic acid 

    OO

    OH 

     Example: but-3-enal 

    O

     

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    2.4 Aromatic compounds:

    We now move to an entirely different area of organic chemistry, that of benzene.

    Benzene consists of alternating double and single bonds, and can be represented as a

    resonance of the above two forms. For simplicity, it is also represented by

    A number of compounds of benzene have special names, listed here in order of

    decreasing priority (as you read from left to right).

    OOH

     

    OH

     

    NH2

     

    OCH3

     

    CH3

     

     benzoic acid phenol aniline anisole toluene

    If there are more than two groups attached, we need to define the positions:

    Ortho, meta and para can be abbreviated to o, m and p.

     Examples:

    Cl

    Cl 

    OH

    Br   

    meta-dichlorobenzene  p-bromophenol

    orthoortho

    meta meta

    ara

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    If there are more than 2 substituents, then we use numbering.

     Example:

    OH

    Cl

    Cl

     

    3,4-dichlorophenol

    If benzene is a substituent, it is known as the phenyl group, and can be abbreviated to –Ph in

    formulae.

     Example:

    OH

    O

      or Ph   OH

    O

     

    3-phenylbutanoic acid

    Additional References:

    Brown and Poon, Introduction to Organic Chemistry, 3rd Ed, Wiley International

    2005, Sections 3.1-3.6, 9.4, 13.3, 14.3 and pg 101-102.

    Silberberg, Chemistry The Molecular Nature of Matter and Change, Sections 15.2:“The Structures and Classes of Hydrocarbons”, 15.4: “ Properties and Reactivities of

    Common Functional Groups”

    Problem Set 2:

    2.1 Name the following compounds

    a.

     b.

    c.

    d.

    e.

    O

     

    f.

    OOH

     

    g. 

    O

     

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    h.

    Cl

    Cl

      i.

    NH2

    OH

     

     j.   OH

    OO

     

    2.2. A compound has been named 3-chloro-2-ethyl-5-methyl-heptane. What should it

    actually be called?

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    3. TRANSITION METAL CHEMISTRY

    3.1 Introduction:

    At Summer School, we will be talking about coordination compounds, also known as metal

    complexes, which are known for all metals, but we will mostly be looking at the transition

    metals. The molecules and ions which coordinate to the metal centre are called ligands. In

    general, we can think of a coordinate bond formed between the metal and a ligand, in which

    the ligand donates a pair of electrons to the metal centre. This bonding can quite drastically

    change the reactivity of the metal and ligand.

    For example, hexacyanidoferrate(III) (also called ferricyanide) comprises of six cyanide

    ligands and an iron(III) centre. Usually the cyanide ion is very toxic, however

    hexacyanidoferrate(III) has a very low toxicity, due to the strong iron-carbon bonds.

    Another point to note is that hexacyanidoferrate(III) is an anion, so there is a positive counter

    ion. The counter ion, frequently sodium or potassium for hexacyanidoferrate(III), is not

    covalently bound to the metal or ligands and does not drastically change the reactivity.

    One thing you may not have seen before is the wedged bonds. These are used to show that a bond is not in the plane of the page. The solid wedged bonds come out of the page and the

    dashed bonds go into the page. Here is another diagram of the hexacyanidoferrate(III) ion to

    compare with the structure before.

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    3.2 How to draw a metal complex:

    Metal complexes can have from one to twelve atoms attached to the metal centre so it is

    important to be able to clearly show the geometry around the metal centre. The number ofatoms attached to the metal is called the coordination number, often abbreviated to CN.

    Coordination numbers of 4 and 6 are the most common and there are multiple different

    geometries around the metal centre that can be observed for the same coordination number.

    CN = 6

    Complexes with coordination numbers of six are usually octahedral, which puts the metal

    centre at the centre of an octahedral formed by the atoms attached to it. The

    hexacyanidoferrate(III) above is an example of an octahedral complex. This is the most

    common way to draw octahedral complexes, however sometimes we draw them as shown

     below.

    CN = 4

    Complexes with a coordination number of four can be either square planar or tetrahedral and

    we will discuss why at Summer School. For the purpose of getting you to practice drawing

    them, you will be told if a complex is square planar or tetrahedral for the exercises.

    Tetrahedral Square Planar (either is acceptable)

    3.3 Naming:

    There are a number of rules for naming coordination compounds.

    1. The cation is names before the anion, as you've seen for naming simple ionic

    compounds.

    2. The ligands are named (in alphabetical order) before the metal.

    3. If the ligand is anionic, replace the final -e with an -o.

    4. If the ligand is neutral, use the full name. Do not abbreviate the name.

    5. For multiples of the same ligand, use the prefixes below

    Fe

    NC

    NC CN

    CN

    CN

    CN

    3-

    Br

    Ni

    Br Br

    Br

    2-

    Pt NH3

    NH3

    H3N

    NH3

    2+

    Pt

    H3N

    H3N NH3

    NH3

    2+

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    If the ligand doesn't contain one of the

    following prefixes e.g. chlorido

    If the ligand does contain one of the following prefixes

    e.g. 1,2-ethanediamine

    2 di Bis

    3 tri Tris

    4 tetra tetrakis

    5 penta pentakis

    6 hexa hexakis

    6. If the complex is anionic, add -ate onto the end of the name of the metal. If it ends in -ium

    or -um, replace it with -ate. Some metals also go back to their Latin roots.

    Metal Anionic Name Metal Anionic Name

     Nickel Nickelate Palladium Palladate

    Copper Cuprate Iron Ferrate

    Lead Plumbate Gold Aurate

    Silver Argentate Tin Stannate

    Mercury Mercurate Manganese Manganate

    7. Write the oxidation number of the metal in Roman numerals after the metal. For example,

    Fe(III).

    For formulas, there are similar rules.

    1. Cation before anion, as for ionic compounds.2. The formula of the complex is in square brackets.

    3. Inside the square brackets, the metal centre is first.

    4. Ligands are written with the atom attached to the metal first or abbreviated and

    ordered alphabetically. If there are multiples of the one ligand, follow with a

    subscript. If the ligand comprises of multiple atoms, surround it with round

     brackets.

     Examples:

    tris(1,2-ethanediamine)cobalt(III) nitrate potassium tetrachloridocuprate(II)

    [Co(en)3](NO3)3 K 2[CuCl4]

    Co

    NH2

    H2N NH2

    NH2

    H2N

    H2N

    NO3

    -

    NO3-

    NO3-

    3+

    K+

    K+

    Cl

    Cu

    ClCl

    Cl

    2-

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    3.4 Common ligands:

    There are a number of common ligands, which we will repeatedly see during Summer School.

    The most important of these, namely water, ammonia, carbon monoxide and nitrogen

    monoxide, are the exceptions to the rule for the names of neutral ligands are unchanged. The

    differences are highlighted in the table below.

    There are also ligands that can attach to the metal centre at two or more atoms, like

    1,2-ethanediamine as before, through its two nitrogen atoms. These are called polydentate

    ligands. Ligands which can only bind through one atom are called monodentate. Ligands with

    two binding atoms are called bidentate; three tridentate, and so on. These can be contrasted

    with ligands like the nitrite ion (NO2 – ) and the thiocyanate ion (SCN

     – ), which have a lone pair

    on more than one atom in the ion, so they can bind through either, but not both atoms. These

    are called ambidentate ligands.

    Molecule or ion Ligand name ( - if neutral) Formula (abbreviation) Donor atoms

    ammonia ammine NH3  N

    water aqua H2O O

    carbon monoxide carbonyl CO C

    nitrogen monoxide nitrosyl NO N

    acetonitrile - NCCH3  N

     bromide bromido Br -  Br

    carbonate carbonato CO32-

      O or 2 O (can be

    monodentate or

     bidentate)

    chloride chlorido Cl-  Cl

    cyanide cyanido CN-  C

    iodide iodido I-  I

    nitrite nitrito NO2-  N or O

    nitride nitrido N3-

      N (triply bonded to

    the metal)

    oxide oxido O2-

      O (doubly bonded

    to the metal)

    thiocyanate thiocyanato SCN-  S or N

     pyridine -

    C5H5 N (py)

     N

    1,2-ethanediamine

    (ethylenediamine)

    - H2 NCH2CH2 NH2 (en) 2 N

    oxalate (ethanedioate) oxalato 

    C2O4- (ox) 2 O

    2,2'-bipyridine - 2 N

    N

    N   N

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    C10H8 N2 (bipy)

    triphenylphosphine -

    P(C6H5)3, PPh3

    P

    glycinate glycinato H2 NCH2COO- (gly) 1 N and 1 O

    ethylenediaminetetracetate

    (EDTA)

    ethylenediaminetetracetato

    C10H16 N2O8 (EDTA)

    2 N and 4 O

    Problem Set 3:

     Note that some of these complexes have isomers, but we will discuss isomerism in detail at

    Summer School.

    1. Name and write the formula for each of the following complexes.

    a) b)

    2. Draw and write the formula for each of the following complexes.

    a) diaquabis(2,2'-bipyridine)iron(II) chloride b) diamminedichloridoplatinum(II) – square planar

    3. Draw and name each of the following complexes.

    a) [RhCl(PPh3)3] – square planar

     b) [Zn(gly)2] – tetrahedral

    P

    O-

    N

    -

    O

    O

    N-O

    O O-

    O

    O

    Cr

    H3N

    H3N Cl

    Cl

    OH2

    NH3

    +

    NO3-

    Mn

    O

    O OH2

    OH

    CO

    OHO

    ONa+

    Na+

    2-

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    4. THEROETICAL CHEMISTRY / ELECTRONIC

    STRUCTURE

    In principle, all the chemical properties of matter can be derived from physical laws of

    motion. For example, the simplest chemical system – a hydrogen atom – consists of a positively charged nucleus accompanied by a negatively charged electron. The two particles

    experience an attractive force and from this, the motion of the electron can be calculated.

    From this, chemically important properties like the radius of a hydrogen atom, the ionization

    energy and even the colour can be calculated.

    As part of Summer School we will attempt to approach chemistry from this bottom-up

    approach by considering what occurs at the microscopic level (electronic structure) but also

    the physics behind chemical transformations. Both of these concepts originally had their roots

    in simple classical physics.

    4.1 Basic Mechanics

    At Summer School, we will begin by considering the classical (pre-20th  century) laws of

     physics, particularly classical mechanics and classical wave theory. You should be familiar

    with some of the very basic concepts before you arrive. This section will contain no examples

    - it just aims to familiarise you with some of the vocabulary we will be using. Most of this is

    covered in a standard year 11/12 physics course.

    Particles

    In classical mechanics, the state of a particle is described by quantities such as position (x),

    velocity (v, directional speed, measured in ms-1), acceleration  (a, measured in m s-2)momentum ( p, measured in kg m s

    -1), energy ( E, measured in J) (kinetic ( K ) and potential 

    (V )), forces acting on ( F , in N), mass (m, in kg), etc. The important terms are defined in the

    table at the end of the section. In mechanics calculations, SI units should be used at all times.

    Velocity and momentum describe the direction and magnitude of motion, while energy is a

    number which describes the ability of a particle to push against forces (do 'work').

    In classical mechanics, objects stay in constant motion (with a constant velocity and

    momentum) unless they are acted upon by a force. Forces acting on a particle change the

    momentum of a particle, and hence change its motion:

     F dt dp =  

    Common forces include gravity, and electric forces.

    •  Electrostatic: !   !!

    !!!!

    !!!!

    !!

     

    •  Gravitational: !   ! !!!!!

    !!

     

    where r  is the distance between the objects, qi  is the charge of particle i and mi  is the mass of

     particle i.

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    In particular, classical motion obeys Newton's Law:

    ma F   = ,

    Computation of the motion of a complicated system can be difficult, so often we can use the

    more general conservation laws  to aid us in our calculations:

    •  Conservation of energy ( E ): total energy in an isolated physical system is constant

    over time. 

    •  Conservation of momentum ( p): in a closed system of objects, with no external

    forces, momentum is constant over time. 

    Waves

    A wave is a form of energy which is spread out and transmitted through space - a disturbance

    or oscillation which propagates through time. There are many different kinds of waves that

    we are familiar with:

    - Mechanical waves involve deformation or vibration of substances (water waves, sound

    waves, etc.)

    - Electromagnetic waves (light, X-rays, radio waves, etc.) are the oscillation of electric and

    magnetic fields which can carry energy through a vacuum.

    Waves are characterised by a frequency ( f , number of cycles per unit time), a wavelength (!  ,

    the length from crest to crest), an amplitude ( A, the height of the oscillations) and a speed (v =

     f ! ) which relate directly to their properties. Waves are subject to many special phenomena,

    including diffraction, reflection, refraction and interference, all of which will be discussed at

    the Summer School.

    Particle

    Mechanics

    Forces cause

    changes in

    momentum, and

    hence determine

    the motion ofobjects.

    Potential Energy 

    is associated with

    the location of a

     particle (its

    interaction withforces).

    Kinetic Energy 

    is associated

    with the motion

    of a particle. 

    Momentum 

    measures how

    much an object

    is moving

    (taking intoaccount mass).

    dx

    dV t  x F    !=),(   )( xV   

    2

    2

    1mv K    =   mv p   =  

    Properties

    of waves

    The speed of a wave, v,

    is related to frequency

    and wavelength.

    Frequency counts the number

    of oscillations of a wave per

    unit time.

    Wavelength is

    the spatial

    distance covered

     by a wave in

    one oscillation.

    v =f !    f   !  

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    4.2 Electronic Structure

    It is only since 1911 that chemists have known that atoms consist of electrons orbiting a tiny,

     positively charged nucleus. The orbits of the electron are similar to planetary orbits, and can

     be labeled by their average distance, angle of inclination etc. However, the laws of quantum

    mechanics imply that only a handful of the infinite possible orbits are allowed. We call thesequantised orbits “orbitals” and label them with each of the following:

    •  Shell Number: 

    which can be any of 1,2,3,4 … in order of increasing distance from the nucleus.

    •  Subshell Label: 

    which can be s, p, d, f, g, h … The nth shell has n subshells, e.g. the second shell has

    two subshells: 2s and 2p.

    •  Direction Indicator: 

    The “s” subshell has no particular direction and contains only one orbital, whereas the

    “p” subshell contains three orbitals (px, py, pz). The “d” subshell contains fiveorbitals; the “f” subshell contains seven and so on.

    •  Each orbital can hold two electrons, so long as they have opposite spin to each

    other. However, it is slightly more energetically advantageous to have electrons

    unpaired rather than paired.

    Electrons fill the orbitals so as to minimise total energy: the electrons fill the lowest shells

    first. We call this configuration the ground state.

    The main contribution to the energy is the distance from the nucleus, so the shells are filled in

    the order 1 < 2 < 3 < 4.

     Next, the subshells are filled in the order: s < p < d < f, but there is a catch. The 4s subshell is

    actually lower in energy than the 3d subshell! Likewise, the 5s subshell gets filled before the

    4d, and the 5p and 6s subshells both get filled before the 4f.

    s p d

    5

    ! ! ! " "

    4

    !   d xy  d xz  d  yz  d z2  d x2-y2 

    ! ! !  3d

    3

    !   p x    p  y    p z 

    s    ! ! !

     

    !

     

    !

     

    h

     

    l

    Subshel l

     

    Here is a helpful mnemonic for

    remembering the order in which the

    orbitals are filled. Write out all the

    orbitals as shown, then read them

    diagonally starting from the top right

    and going to the bottom left.

    1s 1s

    2s 2p 2s 2p3s 3p3d 3s 3p3d

    4s 4p4d4f 4s 4p4d4f

    5s 5p5d5f 5s 5p5d5f

    6s 6p6d 6s 6p6d

    7s 7p 7s 7p

     

    The order of filling orbitals is 1s, 2s,

    2p, 3s, 3p, 4s and so on…

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     Example The electron configuration of Nickel is 1s22s

    22p

    63s

    23p

    64s

    23d

    (as shown in the diagram above).

    Problem Set 4:

    3.1. Write the ground state electron configuration fora.  Fe

     b.  F –  

    c.  Hg.

    3.2. Which neutral elements would have the following ground state electron

    configurations

    a.  1s22s22p4 

     b.  1s22s

    22p

    63s

    23p

    64s

    23d

    c.  1s22s

    22p

    63s

    23p

    64s

    23d

    104p

    3.3. Can you work out a formula (in terms of n) for the number of orbitals in the nth shell?

    What about the maximum number of electrons allowed in the nth

     shell?

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    5. STOICHIOMETRY AND LABORATORY

    CALCULATONS

    At this stage, it is expected you would have a clear understanding of basic stoichiometryincluding use of the formulae:

    (g/mol)MassMolar

    (g)MassMoles =  

    (L)Volume(mol/L)ionConcentratMoles   !=  

    Students are also required to perform calculations with correct use of significant figures. (see

    Section 1.1)

    A recommended revision text is:

    Silberberg , Chemistry The Molecular Nature of Matter and Change, Chapter 3:

    “Stoichiometry” & Chapter 4: “The Major Classes of Chemical Reactions”.

    5.1 Empirical Formula

    The empirical formula is given as the simplest whole number ratio of elements in a

    compound.

     Examples:

    Consider acetic acid: CH3COOH. Its empirical formula is C1H2O1 or CH2O.

    The empirical formula of Methane CH4 is the same as its molecular formula.

    Many ionic compounds can only be expressed in terms of its empirical formula, such as table

    salt NaCl.

    Determining Empirical Formula:

    The composition of a compound of interest may be expressed in mass or as a percentage

    mass. As we are only interested in the ratio of elements, both can be treated the same:

     Example: Determine the empirical formula of Vitamin C, which has the following

    composition: 40.91% Carbon, 4.59% Hydrogen and 54.50% Oxygen.  

    Step 1. Determine the number of moles per element:

    Assume that 100g of the sample is present when percentages are given.

    Divide the mass of each element by its molar mass to determine the mole ratio:

    C:40.91 g

    12.01 g mol –1

    =3.406 mol  H:4.59 g

    1.008 g mol –1=4.55 mol  

    O:54.50 g

    16.00 g mol –1=3.406 mol  

    Our current preliminary formula is C3.406H4.59O3.406. 

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    Step 2. Convert to integer ratio:

    Divide each by the smallest number of moles present for an element, or by the smallest

    subscript. Here, both C and O are present in the least amount.

    C: 1=406.3

    406.3  H: 34.1=

    406.3

    55.4  O: 1=

    406.3

    406.3 

    Often integer ratios appear at this step. If this is not the case, we multiply to obtain whole

    numbers: here, we multiply by 3:

    C: 1!3= 3   H: 1.34!3= 4.01!   4   O: 1!3= 3  

    Thus, the empirical formula of Vitamin C is C3H4O3.

    Problem Set 5.1:

    4.1.1. Determine the empirical formula of an oxide of nitrogen containing 30.45% N and

    69.55% O by mass.

    4.1.2. A sample contains 0.80 g C; 0.134 g H; 1.066 g O. Suggest a molecular formula if

    its molecular weight is 180.16 g mol –1

     

    4.1.3. A 1.30 g sample of a unknown hydrocarbon undergoes complete combustion (in

    oxygen) to produce 4.40 g of CO2 and 2.70 g of H2O. Suggest a molecular formula

    if its molecular weight is 30.0 g mol –1

    .

    5.2 Laboratory Calculations

    The aim of this section is to illustrate the expected layout when writing laboratory

    calculations.

    Standard Titrations:

     In the standard titration , the concentration of a solution is determined by reaction with a set

    volume of a solution with known concentration.

     Example: The concentration of an unknown sodium hydroxide was determined by titration

    with 20.00 mL of approximately 0.2 mol L –1

     hydrochloric acid which was standardised with

    sodium carbonate.

    a. The standard was made by dissolving 5.617 g in 500.0 mL. Determine its molarity.

    Moles (Na2CO3) = Mass/ Molar Mass

    n(Na2CO3) = 5.617 g / 105.99 g mol –1

     

    n(Na2CO3) = 0.05300…mol (Don’t Round Off) 

    Concentration (Na2CO3) = n (Na2CO3)/ Volume

    [Na2CO3] = 0.05300 mol /0.500 L ( [ ] indicates concentration) 

    [Na2CO3] = 0.1060 mol L –1

      (Four sig. figs) 

     b. Titration of 20.00 mL of Na2CO3 with HCl gave an average titre of 19.71 mL.

    Determine the concentration of the acid.

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    2H+

    (aq) + CO32-

    (aq) ! CO2 (g) +H2O(l) (Write a balanced equation)

    n(Na2CO3) = 0.1060 mol L –1

     " 0.02000 L

    = 0.002120 mol L –1

     

    n(HCl) = 2 x n(Na2CO3)

    = 0.004240 mol

    [HCl] = 0.004240 mol / 0.01971 L= 0.2151 mol L –1

      (Again, 4 sig figs) 

    c. Below are burette readings in the titration with sodium hydroxide. Determine the

    volumes of the NaOH titres and calculate its concentration.

    V(NaOH)

    (mL)

    Titre 1 Titre 2 Titre 3 Titre 4

    Initial Volume 0.34 0.23 0.45 0.34

    Final Volume 27.69 27.57 27.59 27.70

    Titre 27.35  27.34  27.14  27.36  

    Average 27.35 mL 

    (27.14mL titre is an outlier and not included in the results)

    HCl  + NaOH  ! H2O + NaCl 

    n(HCl) = 0.02000 L " 0.2151 mol L –1

     

    = 0.004302 mol

    n(HCl) = n(NaOH)

    [NaOH] = 0.004302 mol / 0.02735 L

    = 0.1573 mol L –1

     

    Back Titration:

    Sometimes a direct titration is not possible. In a Back Titration  the sample is reacted with an

    excess amount of reagent with volume and concentration known. The unreacted reagent is

    then titrated with a known solution, allowing for compositional analysis of the initial sample.

     Note that the limiting reagent runs out before the excess reagent does: i.e. The maximum

    number of moles of product is equivalent to the number of moles of limiting reagent.

     Exampl e: The calcium carbonate content in rock was analysed by treating the sample with

    15.00 mL of 0.912 mol L –1

     hydrochloric acid. The sample was back-titrated with

    17.77 mL of 0.130 mol L –1

      NaOH. Determine the mass of calcium carbonate in the

    sample.

    Total Amount of HCl

    Excess HCl reacted with NaOH

    Amount of HCl used by

    CaCO3 

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    HCl XS + NaOH! H2O + NaCl (Equation for back titration) 

    n(NaOH) = 0.130 mol L –1

     " 0.01777 L

    = 0.00231 mol

    n(HCl XS) = 0.00231 mol

    n(HCl total) = 0.9120 mol L

     –1

     "

     0.01500 L= 0.01368 mol

    n(HCl used) = n(HCl total) – n(HCl XS)

    = 0.01368 mol – 0.00231 mol

    = 0.0114 mol

    2HCl + CaCO3 ! CO2 + H2O + CaCl2  (Equation for HCl reaction with rock) 

    n(CaCO3) = # n(HCl)

    = 0.00569 mol

    m(CaCO3) = 0.00569 mol x 100.07 g mol –1

     

    = 0.569 g

    Yield:

    The theoretical yield  is the expected mass of a product in a reaction assuming 100%

    conversion has occurred .

     Example: a. Determine the theoretical yield of ethyl acetate in the following reaction, given

    the following data

    OHHO

    O

    +

    O

    O

    + H2O

     

    Ethanol Acetic Acid Ethyl AcetateVolume Used

    (mL)

    5 5

    Density (g mL –1

    ) 0.789 1.044 0.897

    Molecular

    Weight (g mol –1

    )

    46.07 60.05 88.105

    Mass(ethanol) = Density x Volume

    = 5 mL " 0.789 g mL –1

     

    = 3.95 g

    n (ethanol) = 3.945 / 46.07

    = 0.0856 mol

    Mass (acetic acid) = 5 mL x 1.044 g mL –1

     

    = 5.22 g

    n (acetic acid) = 5.22 g / 60.05 g mol –1

     

    = 0.0869 mol

    Ethanol is the limiting reagent and acetic acid is in excess.

    Theoretical Yield = Masscalc (ethyl acetate) (Masscalc is the theoretical mass) 

    = 0.0856 mol " 88.105 g mol –1

     

    = 7.54 g

    a.  Determine the percentage yield if 5 mL of ethyl acetate was obtained.

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      42 

     b.  Using a direct integral instead:  !  !    "=3

    0

    ][

    ][

    2

    3

    0

    ][][

    1dt k Ad 

    A

    A

    A

     becomes:

    )03(][

    1

    ][

    1

    03

    !!=

    !

    !

    !

    k AA

    which gives the answer.

    1.4.1

    a. -1

     b. 1

    c. ! 

    d. !! 

    e. !!   ! 

    f. !!"! 

    g. !!! 

    h. !!!   !" 

    i. !!

    !

    !  !"

    !

    1.4.2

    a. !" ! !! 

     b. !! ! !! 

    c. !!! ! 

    d. !! ! !! 

    e. !!" ! !! 

    f. !! ! !!   ! 

    g.!

    !!

    !

    !! 

    h. !  !

    !!

    !

    !! 

    i. !!!

    !

    !! 

    1.4.3

    a. !! 

     b. ! 

    c.!

    !!

    !

    !! 

    d. !!

    !!

      !

    !! 

    Section 2: Organic Nomenclature

    2.1 . The compounds are:

    a. 2-methylpentane

     b. 2-methylpent-1-ene or 2-methyl-1-pentene

    c. 1,4-dimethylcyclohexane

    d. 3-methylheptane

    e. hexan-3-one or 3-hexanone

    f. 4-hydroxypentan-2-one or 4-hydroxy-2-pentanone

    g. hex-1-en-3-one

    h. o-dichlorobenzene or 1,2-dichlorobenzene

    i. o-aminophenol or 2-aminophenol

     j. 3-oxobutanoic acid

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    2.2. 3,6-dimethyl-4-chlorooctane

    Section 3: Transition Metal Chemistry

    1. a) triammineaquadichloridochromium(III) nitrate, [CrCl2(NH3)3(OH2)]NO3 

     b) sodium aquacarbonyldihydroxidooxalatomanaganate, Na2[Mn(CO)(OH)2(OH2)(ox)]

    2. a) [Fe(bipy)2(OH2)2]Cl2  b) [PtCl2(NH3)2]

    3. a) chlorotris(triphenylphosphine)rhodium(I) b) bis(glycinato)zinc(II)

    Section 4: Electronic Configuration

    4.1 The electron configurations are

    a.  Fe 1s22s

    22p

    63s

    23p

    64s

    23d

     b.  F-  1s

    22s

    22p

    6  (note the extra electron)

    c.  Hg 1s22s

    22p

    63s

    23p

    64s

    23d

    104p

    65s

    24d

    105p

    66s

    24f 

    145d

    10 

    (or [Xe] 4f 14

    5d10

    6s2)

    4.2 The elements are (a, Oxygen) (b, Vanadium) (c, Gallium)

    4.3 The number of orbitals in the nth shell is the sum of the first n odd numbers, 1 + 3 + 5

    + … + (2n – 1) = n2. The maximum number of electrons is therefore 2 n2.

    Section 5: Stoichiometry and Laboratory Calculations

    5.1.1. NO2 

    5.1.2. C6H12O6 

    5.1.3. C2H6

    5.2.1. 0.609M

    5.2.2. 0.618g

    5.2.3. 40.4%

    Fe

    N

    NN

    OH2

    N

    OH2

    2+

    Cl-

    Cl-

    Pt

    Cl

    Cl NH3

    NH3

    Rh PPh3

    PPh3

    Cl

    PPh3

    NH

    Zn

    O

    O

    NH

    O

    O

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    7. ACKOWLEDGEMENTS

    These notes were written based on the previous notes compiled by Elizabeth New and

    Anthony Phillips. The material in these notes has been collated by Alex Wong, Tristan

    Reekie, Dustin Stuart, Anne Trinh, Shannon He, Nicholas Malouf, Trent Wallis and SamSalman. A special thanks is extended to William Jackson for his careful editing.