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Quantum Model of the Hydrogen Atom_Clase Martes_15!10!2013

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    Quantum Model of the

    Hydrogen Atom

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    Simple Harmonic Oscillator

    To explain blackbody radiation Planckpostulated that the energy of a simpleharmonic oscillator is quantized

    In his model vibrating charges act as simpleharmonic oscillators and emit EM radiation

    The quantization of energy of harmonic

    oscillators is predicted by QM

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    Simple Harmonic Oscillator (SHO)

    Lets write down the Schrdinger Equation for SHO

    For SHO the potential energy is

    Time independent Schrdinger Equation for SHO

    in 1D

    mk

    xmkxxU

    22)(

    222

    xEx

    xm

    x

    x

    m

    22

    22

    2

    22

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    Simple Harmonic Oscillator

    Plancks expression for

    energy of SHO

    Energy of SHO obtained

    from the solution of theSchrdinger equation

    Thus, the Planck formulaarises from the Schrdinger

    equation naturally n = 0 is the ground state

    with energy h

    2;2

    ,...3,2,1,0

    2

    1

    2

    1

    h

    n

    hnnE

    nhE

    Term htells usthatquantum SHO always

    oscillates. These are calledzero point vibrations

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    Quantum Model of the

    Hydrogen Atom

    Potential Energy

    Time-independent Schrdinger Equation

    Schrdinger Equation in so-called sphericalor polar coordinates

    2222

    here,)( zyxrr

    ekrU e

    E

    r

    ek

    rrrr

    rrm e

    2

    2

    2

    222

    2

    2

    2

    sin

    1

    sin

    11

    2

    Ezyx

    ek

    zyxm e

    222

    2

    2

    2

    2

    2

    2

    22

    2

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    The wavefunction is the function of three variablesnow and can be written as

    We had one variable (quantum box or simpleharmonic oscillator)one quantum number

    Here we can assume that both wavefunction andenergy should in general depend on threequantum numbers, corresponding to eachcoordinate

    Wavefunction of the

    Hydrogen Atom

    )()()(,, gfrRr

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    Wavefunction of the

    Hydrogen Atom

    The three quantum numbers, corresponding toeach coordinate are

    nis the principal quantum number; it correspondsto coordinate r

    lis the orbital quantum number; associated withthe coordinate , and determines the magnitude of

    the electrons angular momentum, L. mlis the magnetic quantum number; associated

    with the coordinate , and it determines theorientation of Lin the magnetic field

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    The Hydrogen Atom

    Thus we can write in general:

    Quantum numbersdetermine the quantum state Often we say that the electron is in the state (n, l, ml)

    The energy of the particle in a quantum statedepends on all quantum numbers

    ),,(),,( ,, rr lmln

    lmln

    EE ,,

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    The Hydrogen Atom

    An electron in a hydrogen atom only has

    physically reasonable solutions when E, l and mlhave the values given indicated below:

    lm

    nlnln

    a

    ek

    h

    meE

    n

    EE

    rr

    l

    emln

    mln

    l

    l

    ...,,2,1,0

    )i.e.(1...,,2,1,0...,3,2,1

    28,

    ),,(),,(

    0

    2

    20

    4

    020

    ,,

    ,,

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    The Hydrogen Atom

    The electron energy in thehydrogen atom depends only onthe principal quantum number, n

    Same result as in Bohrs model.

    2

    0

    ,, n

    EE

    lmln

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    Hydrogen Atom:

    From Bohr to Schrdinger

    The electron orbital (angular) momentum is

    L is thus quantized This is more general than the Bohrs Postulate 3, since it

    allows for orbits with angular momentum of zero (!!)

    For large values of l(l >> 1):

    )1( llL

    lllLl

    )1(

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    The Hydrogen Atom:

    From Bohr to Schrdinger

    1. Remember:Electrons simply

    exists within the atom, and we canonly know the probability offinding the electron at a certaincoordinate

    2. Bohrs orbits correspond to the

    coordinate, where the probability offinding the electron is the largest1. Moreover, Bohrs theory was limited to

    the states with highest angularmomentum, l = n 1

    The wavefunction gives physical meaning ofthe orbits:

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    The Hydrogen Atom:

    From Bohr to Schrdinger

    There are no orbits!!! We describe the electron through

    the quantum states

    The energy of the electron is

    constant when electron in a givenquantum state

    Thus, no energy can be takenfrom electron by radiation

    Why doesnt the accelerating electron emit EMWwhen in states corresponding to Bohrs Orbits?

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    The Hydrogen Atom:

    From Bohr to Schrdinger

    Since the energy of electron in a hydrogen doesnot depend on different land ml(in general forother atoms it does), It is naturally to assume

    that photons are only emitted or absorbed withenergies corresponding to the differencebetween various energy sates

    220

    20,,

    11

    ...,3,2,1,

    nk

    EEEh

    nn

    EEE

    knkn

    nmln l

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    The Hydrogen Atom

    Since, the energy depends only on the principal

    quantum number, the energy of an electron indifferent quantum states- with the same n, butdifferent land/or mlis the same

    The different sates having the same energy arecalled Degenerate States

    The number of such states (having the sameenergy or energy level) is referred to as

    degeneracy of the energy level In general, the degeneracy arises from the

    symmetry in a system

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    Degeneracy: The Hydrogen Atom

    Example:n = 3 there are 9 states (describedby different wavefunctions) that have thesame energy

    2,1,02,1,03 lmln

    232322321132320311131310300,,,,,,,,

    2,1,0;2,1,0;3

    lmln

    eV51.1

    9

    6.13

    3

    2

    03

    EE

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    Degeneracy

    Degeneracy can be lifted if additional

    interactions (forces) applied to a system Consider a hydrogen atom in the magnetic field,

    B, applied along z-direction. The energy ofelectron is then

    This energy now depends on ml: we saydegeneracy over mlwas lifted

    How many energy levels with differentdegeneracy are there for n = 3?

    l

    e

    nlm m

    m

    Be

    n

    EE

    l 220

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    More Features of the Atomic

    Wavefunctions

    Electrons in the different quantum states areunlikely to be found in the same spatial regions

    Electrons in the lower angular momentum states

    are more likely to be found closer to the nucleusthan those in states with higher angularmomentum

    In multi-electron atomsthe degeneracy over

    angular momentum is liftedand the sates withthe same nbut different l have slightly differentenergies

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    Space Quantization

    ldetermines the magnitude of the angular

    momentum, L:

    ml

    determines orientation of Lin space when atomis in a magnetic field

    Taking the magnetic field along z-direction, we can showthat

    Thus, not only is the angular momentum quantized, butalso its component in some direction, usually taken tobe the z-direction

    )1( llLl

    lz

    mL

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    Space Quantization

    Therefore, L, in an atom, cannot have anyarbitrary orientation (in magnetic field) withrespect to z-direction, but rather have onlydiscrete orientations:Space Quantization

    However, as long as we do not have apreferred direction (e.g. defined bymagnetic field) space quantization ismeaningless

    lz

    mL

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    Space Quantization: Example, l = 2

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    Space Quantization: Zeeman Effect

    11

    2

    0;0;1

    Em

    m

    BeEE

    mln

    l

    e

    total

    l

    1

    1

    0

    2

    1,0;1,0;2

    2

    e

    total

    l

    m

    BeEE

    mln

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    Space Quantization:

    Stern-Gerlach Experiment

    Silver atoms studied inthe non-uniformmagnetic field with thegradient along z-

    direction (dB/dz) Although the atoms are

    neutral, they possess amagnetic dipole, and

    the inhomogeneousmagnetic field acts onthis dipole with force

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    Stern-Gerlach Experiment

    The atoms are deflected as they travel through the magnet The stronger the force, the greater the deflection, and thus

    the father away from the center of screen the atoms wouldland as detected on the screen

    mdz

    dB

    m

    e

    dz

    Bmm

    ed

    dz

    dU

    Fe

    e

    z

    2

    )2(

    Bmm

    eU

    m

    m

    eL

    m

    e

    BBBU

    e

    ez

    e

    zzz

    2So,

    22

    :atomaninorbitinelelctronanFor

    :zBBfieldmagneticain

    dipolemagneticaofUenergy,potentialMagnetic

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    Stern-Gerlach Experiment

    Only two lines were observed on the screenon which the atoms land: one above and onebelow of the center !! Moreover, there were no central line and the distance

    from the center to each positions was the same

    Stern-Gerlach Experiment

    http://mutuslab.cs.uwindsor.ca/schurko/nmrcourse/animations/stern-gerlach/sgpeng.htmhttp://mutuslab.cs.uwindsor.ca/schurko/nmrcourse/animations/stern-gerlach/sgpeng.htmhttp://mutuslab.cs.uwindsor.ca/schurko/nmrcourse/animations/stern-gerlach/sgpeng.htmhttp://mutuslab.cs.uwindsor.ca/schurko/nmrcourse/animations/stern-gerlach/sgpeng.htm
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    Stern-Gerlach Experiment

    Stern-Gerlach experiment indeed showeddiscrete nature of the momentum, confirmingspace quantization

    However, the result contradict quantitative

    prediction of the Schrdinger The experiment by Phipps and Taylor with

    hydrogen atoms, where ml= 0 (and thus Lz= 0)showed the two emission lines in the spectrum,

    suggesting that the effect is NOT due to OrbitalMomentum

    Thus, there may be a magnetic dipole other thanthe one associated with orbital momentum!

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    The Spin

    The Spin is a [quantum] property of the electron.

    Spin quantum number is always there

    Other quantum numbers can change depending onthe specifics of the potential the electron is in.

    For instance: In hydrogen, in addition to the spin, an electron is

    characterized by three quantum numbers n, l, ml In a 1D Infinite potential well, in addition to the spin, an

    electron is characterized by only one quantum number n

    The spin is intrinsic to the electron!

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    The Hydrogen Atom Wavefunction:

    Revisited

    Now we need to add another quantumnumber, associated with the electron spin

    2

    1

    ...,,2,1,0

    )i.e.(1...,,2,1,0

    ...,3,2,1),,(),,( ,,,

    s

    l

    mmln

    m

    lm

    nlnl

    nrr sl

    G S f

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    The Ground State of the

    Hydrogen Atom

    For the hydrogen ground state we have

    Reminder: The hydrogen atom is unusual since

    states with the same lhave the same energy.

    21or

    21;0;0;1

    ),,(),,( ,,,

    sl

    mmln

    mmln

    rrsl

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    The Ground State of Atoms other

    than Hydrogen

    As soon as an atom contains more than oneelectron, the states with different lno longer havethe same energy, and degeneracy over orbital

    quantum number is lifted What is the ground sate of a multi-electron system?

    Perhaps in the lowest energy state all electrons in theatom have the same four quantum numbers

    NO!!!

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    Paulis Exclusion Principle

    NO TWO ELECTRONS IN A SYSTEM CAN BEIN THE SAME QUANTUMS STATE

    In other words, no two electrons can have thesame values of the quantum numbers

    For atoms these are:

    This allows us to understand the Periodic Table The electron configuration of any atom must

    satisfy the Paulis exclusion principle

    sl mmln ;;;

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    Paulis Exclusion Principle: Atoms

    Definitions:

    a shell is the set of states with the same n(thusdifferent l, mland ms)

    a sub-shell the set of states with the same n and

    l(thus different mland ms) Using the rules for the atomic quantum

    numbers, we determine that the number of

    electrons in a sub-shell is 2(2l+1)

    a shell is 2n2

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    Additional Rules for Determining

    the Ground State-Configuration

    1. The total energy of the electron increases with increasing n(energy less negative)

    2. Within a given shell (a given n), the l = 0states alwayshave

    the lowest energy3. The energy of the sub-shells generally increases with l :

    El=0< El=1< El=2< El=3

    since electron with lowest value of lcan be closer tonucleus and does not feel shielding of (+)nuclear charge by () electron cloud

    El i C fi i f h

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    Electronic Configuration of the

    Atomic Ground State: Examples

    We shall use letters instead of numbers to denote the orbitalquantum number:

    l = 0s; l = 1p;

    l = 2d; l = 3f We shall use superscript above the letter to indicate the

    number of electrons in a given sub-shell

    Hydrogen (1): 1s1

    Lithium (3): 1s22s1

    Nitrogen (7): 1s22s2p3

    Argon (18): 1s22s2p63s2p6

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    Electronic Configuration of the

    Atomic Ground State: Examples

    Potassium (19): 1s22s2p63s2p64s1

    Calcium (20): 1s22s2p63s2p64s2

    Scandium (21): 1s22s2p63s2p6 d14s2 Note that 3d sub-shell starts to fill in after 4s

    sub-shell is filled up

    The same is true for 4d vs 5s sub-shells

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    Electronic Configuration of the

    Atomic Ground State: Examples

    Nickel (28): 1s22s2p63s2p6d84s2

    Copper (29): 1s22s2p63s2p6d104s1

    Silver (47): 1s22s2p63s2p6d84s2p6d105s1 Note that there is no nd9 state for either Cu, Ag,

    or Au (they loose one s-electron from the nextshell)

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    www.webelements.com

    http://www.webelements.com/http://www.webelements.com/
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    Bees This should be a learning experience. So lets discuss your

    project before the due date After ~ 600 seconds some bees have reached the boundary

    and escaped

    Up to this time would expect that the variance of the averagethat variance begins to approach the diffusion relation derivedby Einstein,

    D is the diffusion coefficient, is the mean free path, and isthe mean free time

    Could you describe one characteristic of the bees motion thatyou choose. For example, you could consider the timedependence of the number of bees escaping per unit time or

    2

    22

    3

    1,inces,

    3

    1

    0case,thisinsince,6)()var(

    vDvvD

    xDtxxxx