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ITT Chng Ch 07 Electronic Structure of Atoms

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    Quantum Theory and theElectronic Structure of Atoms

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    Properties of Waves

    Wavelength() is the distance between identical points onsuccessive waves.

    Amplitudeis the vertical distance from the midline of a

    wave to the pea or trou!h.".#

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    Properties of Waves

    Frequency() is the number of waves that pass throu!h a

    particular point in # second ($% & # cycle's).

    The speed (u

    ) of the wave &

    ".#

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    awell (#*"+), proposed that visible li!ht consists of

    electroma!netic waves.

    Electromagnetic

    radiationis the emission

    and transmission of ener!y

    in the form of

    electroma!netic waves.

    Speed of li!ht (c) in vacuum & +.-- #-*m's

    Allelectroma!netic radiation

    = c".#

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    ".#

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    x= c

    = c/

    = +.-- #-*m's/.- #-/$%= 0.- #-+m

    1adio wave

    A photon has a fre2uency of .- #-/$%. 3onvert

    this fre2uency into wavelen!th (nm). 4oes this fre2uency

    fall in the visible re!ion5

    = 0.- #-#6nm

    ".#

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    ystery 7#, 89lac 9ody Problem:

    Solved by Planc in #;--

    Ener!y (li!ht) is emitted or

    absorbed in discrete units

    (2uantum).

    E & h

    Planc?s

    ".#

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    @i!ht has both

    #. wave nature

    6. particle nature

    h& BE C 9E

    ystery 76, 8Photoelectric Effect:

    Solved by Einstein in #;-0

    Photonis a 8particle: of li!ht

    BE & h= 9E

    h

    BE e=

    ".6

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    E & h

    E & .+ #-=+/(>?s) +.-- #- *(m's) ' -.#0/ #-=;(m)

    E & #.6; #- =#0>

    E & h c '

    ".6

    When copper is bombarded with hi!h=ener!y electrons,

    D rays are emitted. 3alculate the ener!y (in oules)

    associated with the photons if the wavelen!th of the D

    rays is -.#0/ nm.

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    ".+

    @ine Emission Spectrum of $ydro!en Atoms

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    ".+

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    #. e=can only have specific(2uanti%ed) ener!y

    values

    6. li!ht is emitted as e=

    moves from one ener!y

    level to a lower ener!y

    level

    Bohrs Model of

    the Atom (1913)

    En& =1$ ( )

    #

    n6

    n(principal 2uantum number) & #,6,+,F

    1$(1ydber! constant) & 6.#* #-=#*>

    ".+

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    E & h

    E & h

    ".+

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    Ephoton& E & Ef= Ei

    Ef& =1$ ( )#

    n6f

    Ei& =1$ ( )#

    n6i

    i f

    E & 1$( )#

    n6#

    n6

    nf & #

    ni & 6

    nf & #

    ni & +

    nf & 6

    ni & +

    ".+

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    Ephoton& 6.#* #-=#*

    > (#'60 = #';)Ephoton& E & =#.00 #-

    =#;>

    & .+ #-=+/(>?s) +.-- #-* (m's)'#.00 #-=#;>

    *- nm

    3alculate the wavelen!th (in nm) of a photon

    emitted by a hydro!en atom when its electron

    drops from the n& 0 state to the n& + state.

    Ephoton& h c '

    & h c ' Ephoton

    i f

    E & 1$( )#

    n6#

    n6Ephoton&

    ".+

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    4e 9ro!lie (#;6/) reasoned

    that e=is both particle and

    wave.

    Why is e=ener!y 2uanti%ed5

    "./

    u & velocity of e=

    m & mass of e=

    2r & n =h

    mu

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    = h'mu

    = .+ #-=+/' (6.0 #-=+ #0.)

    = #." #-=+6m & #." #-=6+nm

    What is the de 9ro!lie wavelen!th (in nm)

    associated with a 6.0 ! Pin!=Pon! ball

    travelin! at #0. m's5

    m in !h in >?s u in (m's)

    "./

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    Chemistry in Action: Laser The !lendid Li"ht

    @aser li!ht is (#) intense, (6) monoener!etic, and (+) coherent

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    Chemistry in Action: #lectron Microsco!y

    TM ima"e of iron atoms

    on co!!er s$rface

    e& -.--/ nm

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    Schrodin!er Wave E2uation

    Gn #;6 Schrodin!er wrote an e2uation that

    described both the particle and wave nature of the e=

    Wave function () describes

    #. ener!y of e=with a !iven

    6. probability of findin! e=in a volume of space

    Schrodin!er

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    Schrodin!er Wave E2uation

    = fn(n, l, ml, ms)

    principal 2uantum number n

    n& #, 6, +, /, F.

    n n&6 n&+

    ".

    distance of e=from the nucleus

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    Where ;-H of the

    e=

    density is foundfor the #s orbital

    ".

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    & fn(n, l, ml, ms)

    an!ular momentum 2uantum number l

    for a !iven value of n, l& -, #, 6, +, F n=#

    n & #, l = 0

    n & 6, l& - or#

    n & +, l& -, #, or6

    Shape of the 8volume: of space that the e=occupies

    l& - s orbital

    l& # p orbital

    l& 6 d orbital

    l& + f orbital

    Schrodin!er Wave E2uation

    ".

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    l& - (s orbitals)

    l& # (p orbitals)

    ".

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    l& 6 (d orbitals)

    ".

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    & fn(n, l, ml, ms)

    ma!netic 2uantum number ml

    for a !iven value of lml& =l, F., -, F. Cl

    orientation of the orbital in space

    if l& # (p orbital), ml& =#, -, or#

    if l& 6 (d orbital), ml& =6, =#, -, #, or6

    Schrodin!er Wave E2uation

    ".

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    ml& =# ml& - ml& #

    ml& =6 ml& =# ml& - ml& # ml& 6".

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    & fn(n, l, ml, ms)

    spin 2uantum number ms

    ms& CI or=I

    Schrodin!er Wave E2uation

    ms& =Ims& CI

    ".

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    Eistence (and ener!y) of electron in atom is described

    by its uniquewave function .

    Pauli exclusion principle= no two electrons in an atom

    can have the same four 2uantum numbers.

    Schrodin!er Wave E2uation

    & fn(n, l, ml, ms)

    Each seat is uni2uely identified (E, 1#6, S*)

    Each seat can hold only one individual at a

    time

    ".

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    ".

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    Schrodin!er Wave E2uation

    & fn(n, l, ml, ms)

    Shell J electrons with the same value of n

    Subshell J electrons with the same values of nandl

    Krbital J electrons with the same values of n, l, andml

    $ow many electrons can an orbital hold5

    Gf n, l, and mlare fied, then ms& I or = I

    & (n, l, ml, I) or & (n, l, ml, =I)

    An orbital can hold 6 electrons ".

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    $ow many 6p orbitals are there in an atom5

    6p

    n&6

    l& #

    Gf l& #, then ml& =#, -, or C#

    + orbitals

    $ow many electrons can be placed in the +d

    subshell5

    +d

    n&+

    l& 6

    Gf l& 6, then ml& =6, =#, -, C#, or C6

    0 orbitals which can hold a total of #- e=

    ".

    Ener!y of orbitals in a single electron atom

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    Ener!y of orbitals in a singleelectron atom

    Ener!y only depends on principal 2uantum number n

    En& =1$ ( )#

    n6

    n

    n&6

    n&+

    "."

    Ener!y of orbitals in a multi electron atom

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    Ener!y of orbitals in a multi=electron atom

    Ener!y depends on nand l

    n l& -

    n&6 l& -n&6 l& #

    n&+ l& -n&+ l& #

    n&+ l& 6

    "."

    8Lill up: electrons in lowest ener!y orbitals (Aufbau principle)

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    Lill up electrons in lowest ener!y orbitals (Aufbau principle)

    $ # electron

    $ #s#

    $e 6 electrons

    $e #s6

    @i + electrons

    @i #s66s#

    9e / electrons

    9e #s66s6

    9 0 electrons

    9 #s66s66p#

    3 electrons

    5 5

    ".;

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    3 electrons

    The most stable arran!ement of electrons

    in subshells is the one with the !reatest

    number of parallel spins (Hunds rule).

    3 #s66s66p6

    M " electrons

    M #s66s66p+

    K * electrons

    K #s66s66p/

    L ; electrons

    L #s66s66p0

    Me #- electrons

    Me #s66s66p

    "."

    Krder of orbitals (fillin!) in multi electron atom

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    Krder of orbitals (fillin!) in multi=electron atom

    #s N 6s N 6p N +s N +p N /s N +d N /p N 0s N /d N 0p N s"."

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    Electron configurationis how the electrons are

    distributed amon! the various atomic orbitals in an

    atom.

    #s#

    principal 2uantumnumber n an!ular momentum2uantum number l

    number of electrons

    in the orbital or subshell

    rbital diagram

    $

    #s#

    ".*

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    What is the electron confi!uration of !5

    ! #6 electrons

    #s N 6s N 6p N +s N +p N /s#s66s66p+s6 6 C 6 C C 6 & #6 electrons

    ".*

    Abbreviated as OMe+s6 OMe #s66s66p

    What are the possible 2uantum numbers for the

    last (outermost) electron in 3l5

    3l #" electrons #s N 6s N 6p N +s N +p N /s#s66s66p+s6+p0 6 C 6 C C 6 C 0 & #" electrons

    @ast electron added to +p orbital

    n & + l& # ml& =#, -, or C# ms& I or =I

    Kutermost subshell bein! filled with electrons

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    Kutermost subshell bein! filled with electrons

    ".*

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    ".*

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    Paramagneticunpaired electrons

    6p

    !iamagneticall electrons paired

    6p".*

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    Chemistry Mystery: %isco&ery of 'eli$m

    Gn #**, Pierre >anssen detected a new dar line in the solar

    emission spectrum that did not match nown emission lines

    Gn #*;0, William 1amsey discovered helium in a mineral of

    uranium (from alpha decay).

    ystery element was named $elium