bohr's theory

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    FOUR QUANTUM NUMBERS

    1. PRINCIPAL QUANTUM NUMBER

    2. ORBITAL QUANTUM NUMBER

    3. SPIN ANGULAR QUANTUM NUMBER

    4. MAGNETIC QUANTUM NUMBER

    PAULIS EXCLUSION PRINCIPLE

    Ref: Perspective of Modern Physics By Beiser

    Modern Physics By Theraja

    Physics of atom By Rajyam

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    The observation of line spectra from rarified

    gases in electrical discharge tubes could also notbe explained by classical physics.

    The only way to explainline spectra was toassume that the electronscould occupy stationarystates in the atom, andthat radiation would onlybe emitted upon atransition between twostationary states at

    different energies

    ATOMIC LINE SPECTRA

    V

    H2 DISCHARGE COLLIMATORS DIFFRAACTION SCREEN

    TUBE GRATING

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    BOHR MODEL OF THE ATOM

    Bohr set out to explain

    location of spectral lines of hydrogen (e.g., Balmer

    series)

    Johann Balmer measured the wavelengths of this

    series of lines from atomic hydrogen and found that theyfit the relation

    1/ = const ( 1/4 - 1/n2).(1)where n = 3, 4, 5, 6.

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    SPECTRAL SERIES OF H ATOM

    1/ = R ( 1/n2- 1/m2)R being the Rydberg const for infinite nuclear mass

    1. Lyman Series (uv region), n=1, m=2, 3, 4

    2. Balmer Series (visible), n=2, m=3, 4, 5 3. Paschen series (IR) n=3, m= 4, 5, 6 4. Brackett Series (IR) n=4, m=5, 6, 7 5. Pfund Series (IR) n=5, m= 6, 7, 8

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    BOHRS POSTULATES

    In 1913, Niels Bohr proposed a model which is

    based on the following three postulates :

    1. The nucleus is considered to be a point masslocated at the center of the atom, while the

    electrons move in circular orbits around it

    The electrostatic attraction between the positivenucleus and negative electron keeps the electron

    in orbit.

    )2..(..........

    4

    12

    22

    r

    e

    r

    mv

    o

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    2. Only those circular orbits of electrons arepermissible for which the angular momentum of

    the atom is an integral multiple of . h/2

    These permissible orbits are 'steady' or 'stationary'..

    )3......(..........2/

    ....,3,2,1;..

    h

    nnmvrei

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    3. Electrons in 'stationary'orbits do not radiate theirenergy; only when the

    electron jumps from a oneorbit to another, thedifference in the energy of

    the orbits is absorbed oremitted depending onwhether the transitioncorresponds to excitation

    or deexcitation. Emissionof energy is in the form ofa photon:

    E2E1 = E = h .(4)

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    Derivation of Quantized Energy States

    The circular orbits postulated for the

    electron requires a balance between the

    centripetal [(4

    o)

    -1q1q2/r

    2

    ]

    and centrifugal(mv2/r) forces.

    (4o)-1q1q2/r2 = (kZe)e/r2=mv2/r (1)

    where for convenience we usek =(4o)-1= 8.99 x109 N m2/C2.

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    Recall that the angular momentum is mvr, and so

    Bohr's postulate about angular momentum is

    mvr = nh/2 (2)Combining equation (1) with (2), we can solve forr, the

    radius of the orbit, as

    m(kZe)e = m2v2r2 /r = n2h2/42ror

    r = n2(h2/42me2kZ) = on2h2/ mZe2 ...........(3)= a

    1n2

    where a1=oh2/ mZe2 =5.29 x 10-11 m is the Bohrradius for the ground state of the hydrogen atom.

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    This equation says that electrons are allowed only

    in orbits of certain (quantized) radii, as n = 1, 2, 3... .

    Associated with these quantized orbits is aquantized energy. Total energy is the sum of kinetic

    energy and potential energy,E = K + U.

    We will take the zero of potential energy at

    infinity. The potential energy difference is just the

    negative of work, or force times the displacement, so the

    potential energy of an electron inside an atom is

    U = dU = kZe2/r2dr =-kZe2/rso that the total energy is K.E. + P.E.

    E =1/2 mv2-kZe2/r

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    and using equations (1), (2) and (3)

    above, after some simple mathematics,we find the quantized energy

    En= -(22me4k2Z2)/n2h2 = -m Z2 e4 /8o 2h2n2

    Note: The total energy is negative, or

    the electron is bound, and that as n ->infinity,E->0. The numbern is called

    the principal quantum number.

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    The quantity (22me4k2Z2)/h2 is a constant that

    depends only on fundamental physical quantities,

    R' =(22me4k2)/h2 = 13.6 eV.The electron-volt (eV) is a unit of energy (the

    energy an electron would gain after acceleration through

    a potential of 1 volt). 1 eV = 1.602 x 10-19

    J.Thus the total energy equation becomes extremely

    simple:

    En=-R' Z2/n2.En=-13.6/n2 eV for H atom.

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    THE BOHR MODEL OF THE HYDROGEN ATOM (Z = 1)

    GAVE US THE FOLLOWING RESULTS:

    The angular momentum, l, was postulated to bequantized according to

    l = mvr= nh/2. where n is the principle quantum

    number.The radii of allowed electron orbits were also quantized

    according

    r = aon2 = n2h2/(42ke2m)where ao= 5.29 x 10

    -11m is theBohr radius.

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    The energies of the orbits were likewise quantized

    according to

    En=-R'[1/n2]whereR' = 13.6 eV is a constant.

    The difference between energy levels (orbits)

    corresponds to a wavelength

    1/ab = ab/c = (Eb- Ea)/ch=RH[1/na2-1/nb2]whereR

    H= 10.96776 mm-1 is the sameRydberg

    constantthat was measured experimentally by

    Rydberg.

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    Here is a scale model of the orbits of the hydrogen

    atom, with the radii getting further apart according to n2:

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    However, despite the orbits getting ever farther apart

    in space, they get closer togetherin energyaccording

    to 1/n2. Any energy level diagram is shown below:

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    K G A

    V Vo

    Hg

    CONFIRMATION OF BOHRS THEORY

    The Franck-Hertz experiment is one of theclassic demonstrations of the quantization ofatomic energy levels. Electrons emitted by thefilament are accelerated through mercury vapor.When the accelerating voltage reaches V1, theelectrons have just enough energy to excite the

    mercury atoms from the ground state to thelowest excited state. Thus, many of theelectrons lose their energy and cannot reach thecollector;

    this is signaled by anabrupt drop in collectorcurrent as theaccelerating voltage isincreased past V1.

    Fi h li i d f ll

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    Figure shows qualitative trend of collector currentvs. accelerating voltage. As the acceleratingvoltage is increased beyond V1, electrons which

    have been brought to rest as a result of excitingmercury atoms are again accelerated until theycan produce another excitation. Thus, a secondpeak occurs at V2, where ideally one expects V2 -

    V1 = V1.

    However, contactpotentials in the system

    displace the first peakat V1 from its expectedvalue, and V1 itself isnot a good measure of

    the excitation potential.

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    The sequence of electron acceleration and atomicexcitation may continue as the accelerating

    voltage is further increased so that a series ofpeaks may be observed.

    Breakdown of the gas in the tube will occur whenthe accelerating voltage becomes too high. Onsetof breakdown may be delayed by increase invapor pressure (higher oven temperature) ordecrease in number of electrons (lower filament

    current).

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