Chapter 4 Atomic Structure (Pp 96-125)

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    CHAPTER 4

    ATOMIC STRUCTURE

    BOHRS THEORY OF HYDROGEN ATOMExample 4-1

    Determine the radius of the first orbit of the hydrogen atom.SolutionThe radius of electron in nth orbit of hydrogen atom is given by

    kme

    hnrn 22

    22

    4=

    )10988.8()10602.1)(10109.9(4)10626.6()1(

    9219192

    2342

    1

    =

    r

    53.010287.5 111 = mr

    Example 4-2

    Find the value of quantum number n for a hydrogen atomthat has an orbital radius of 847 pm.SolutionThe radius of in nth orbit of hydrogen atom is given by

    211103.5 nrn

    = in metres

    4103.5

    10847

    103.5 11

    12

    11 =

    =

    =

    nrn the desired quantum

    number.Example 4-3

    Determine the speed of electron in 10th orbit of hydrogen

    atom. B.U. B.Sc. (Hons.) 1984ASolutionThe velocity of electron in nthorbit of hydrogen atom is givenby

    nh

    ekvn

    22=

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    smv /10187.2)10626.6)(10(

    )10602.1)(10988.8(2 534

    2199

    10 =

    =

    the desired speed.

    Example 4-4

    Find the de Broglie wavelength of an electron in the n = 3

    orbit of hydrogen atom. In what region of the spectrumwould a photon of the same wavelength be classified?SolutionThe velocity of electron in nthorbit of hydrogen atom is given

    byhn

    ekvn

    22= or

    h

    ekv

    32 2

    3

    = for n = 3.

    The de Broglie wavelength is defined as

    2

    2

    3 2

    3

    ekm

    h

    vm

    h

    p

    h

    ===

    219931

    234

    )10602.1(10988.8)(10109.9(2

    )10626.6(3

    = 1010977.9 10 = m

    The photon of this wavelength belongs to X-ray region.Example 4-5

    Calculate the frequency of electron in the first Bohr orbit ofhydrogen atom. B.U. B.Sc. 2004ASolutionThe velocity of electron in terms of radius is given by

    rm

    nhv

    2=

    The orbital frequency is given byf = (speed of electron) (circumference of orbit)

    22421

    2 mrnh

    rrm

    nhf

    ==

    Butkme

    hnr

    22

    22

    4= therefore

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    =

    =

    33

    2422

    22

    22

    2

    444 hn

    kme

    hn

    kme

    m

    nhf

    3343

    29419312

    )10626.6()1()10988.8()10602.1)(10109.9(4

    =

    f

    1510577.6 = Hz

    Example 4-6

    On the average, an atom will exist in an excited state for810 second, before it makes a downward transition and

    emits a photon. Assuming that the electron in hydrogen is inthe state n = 2, how many revolutions about the nucleus aremade before the electron jumps to the ground state?SolutionThe time period T of electron in nthorbit is given by

    242

    33

    4

    1

    kme

    hn

    f

    T

    ==

    29419312

    343

    )10988.8()10602.1)(10109.9(4)10626.6()2(

    =

    T

    sT 1510216.1 = Number of revolutions completed by electron is given by

    615

    8

    10224.810216.1

    10=

    =

    periodTime

    stateexcitedinTimeRevolutions

    Example 4-7

    Show that the energy of electron in nthfor hydrogen atom is

    given by 26.13

    nEn = eV.SolutionThe energy of electron in nth orbit is given by

    22

    2422hn

    kmeEn

    = in joules

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    22

    2322

    hn

    kmeEn

    = in eV

    2342

    29319312

    )10626.6()10988.8()10602.1)(10109.9(2

    =

    nEn

    2

    6.13n

    En = in eV

    Example 4-8

    Calculate the binding energy of the hydrogen atom in thefirst excited state.SolutionThe energy of electron in nth orbit is given by

    2

    6.13n

    En = in eV

    For first excited state we substitute n = 2, therefore

    4.3)2(6.1322 ==E eV

    Hence the binding energy of the hydrogen atom in the firstexcited state is 3.4 eV.Example 4-9

    Calculate the energy of the electron for first two excitedstates of hydrogen atom. What will be the wavelength ofemitted (or absorbed) radiation if an electron makes atransition between these two states?Solution(a) The energy of electron in nth orbit is given by

    2

    6.13

    n

    En = in eV

    The energy of the first two excited states can be calculated bysubstituting n = 2 and n = 3 respectively. Hence

    eVEn 4.3)2(6.13

    ,222

    ===

    eVEn 51.1)3(6.13

    ,323

    ===

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    (b)Now

    hc

    hEE == 23

    )10602.1)}(4.3(51.1{

    )10998.2)(10626.6(19

    834

    23

    =

    =

    EE

    hc

    m710561.6 = or 6561

    Example 4-10

    Calculate the first, second and third excitation energies forhydrogen atom.SolutionThe energy of electron in nth orbit is given by

    2

    6.13n

    En = in eV

    Now ,1=n eVE 6.13)1/()6.13( 21 ==

    ,2=n eVE 4.3)2/()6.13( 22 ==

    ,3=n eVE 51.1)3/()6.13( 23 ==

    ,4=n eVE 85.0)4/()6.13( 24 == Let 1, 2 and 3 be the first, second and third excitationenergies of the hydrogen atom, then

    1= eVEE 2.10)6.13(4.312 == 2= eVEE 09.12)6.13(51.113 == 3= eVEE 75.12)6.13(85.014 ==

    Example 4-11

    Calculate the value of Rydberg constant for hydrogen atom.

    SolutionThe Rydberg constant is defined by

    3

    4222ch

    mekR

    =

    3348

    41931292

    )10626.6)(10998.2()10602.1)(10109.9()10988.8(2

    =

    R

    1710097.1 = mR

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    Example 4-12

    The wavelength of the first line of Lyman series of hydrogenatom is 1216 . Calculate the wavelength of third line.

    B.U. B.Sc. 1990ASolutionThe wavelength of different members of the Lyman series ofhydrogen atom is given by

    =

    22

    1

    1

    11

    nR

    n , n = 2,3,4,.

    For the first member n = 2 , therefore

    43

    21

    11

    12161

    22

    RR =

    =

    )1216)3(4

    =R =9121

    = -1

    For the third member n = 4 and formula for Lyman seriesbecomes

    48645

    9121

    1615

    1615

    41

    111 22

    3

    ===

    = RR

    8.9725

    48643 ==

    Example 4-13

    The wavelength of the first line of Lyman series of hydrogenatom is 1216 . Calculate the wavelength of 5thline.

    B.U. B.Sc. 1992ASolutionThe wavelength of different members of the Lyman series of

    hydrogen atom is given by

    =

    22

    1

    1

    11

    nR

    n , n = 2,3,4,.

    For the first member n = 2 , therefore

    43

    21

    11

    12161

    22

    RR =

    = or

    )1216)3(4

    =R 9121

    = -1

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    For the fifth member n = 6 and formula for Lyman seriesbecomes

    3283235

    9121

    3635

    3635

    61

    111

    223

    ===

    =

    RR

    93835

    328323 ==

    Example 4-14The wavelength of the first member of Balmer series of thehydrogen atom is 6563 . Calculate the wavelength of thefirst member of Lyman series in the same spectrum.

    B.U. B.Sc. 2009ASolutionThe formula for Balmer series of hydrogen atom is

    =

    22

    1

    2

    11

    nR

    , n = 3,4,5, . . .

    For first member of this series we substitute n = 3

    365

    31

    211 22

    1

    RR =

    =

    R536

    1 = (1)

    The Lyman series is given by

    =

    22

    1

    1

    11

    nR

    , n = 2,3,4, . . . .

    For first member of this series we substitute n = 2

    43

    2

    1

    1

    1122

    1

    RR =

    =

    R34

    1 = (2)

    Divide Eq(2) by Eq(1)

    275

    365

    34

    1

    1=

    =

    R

    R

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    37.121527

    )6563(5275 1

    1 ===

    Example 4-15

    Calculate the longest and shortest wavelength i.e. serieslimit of the Lyman series.Solution

    The Lyman series is given by

    =

    22

    1111

    nR

    , n= 2, 3, 4 . . .

    For longest wavelength, substitute n = 2

    43

    2

    1

    1

    1122

    RR =

    =

    R34

    =

    1215105.121)10097.1(3

    4 97

    ==

    = m

    For series limit, substitute =n

    RRn

    R =

    =

    =

    222 )(

    11

    1

    1

    11

    9121091210097.1

    11 107 ==

    ==

    m

    R

    Example 4-16

    Calculate the longest wavelength in Balmer series. Also findthe value of the shortest wavelength. B.U. B.Sc. 1988SSolution

    The formula for Balmer series of hydrogen atom is

    =

    22

    1

    2

    11

    nR

    , n = 3,4,5,.

    Substitute n = 3

    365

    31

    211

    22

    RR =

    =

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    656310563.6)10097.1(5

    36536 7

    7 ==

    ==

    m

    R

    Substitute =n in above formula

    41

    2

    1122

    RR =

    =

    364610646.310097.1

    44 77 ====

    mR The desired longest and shortest wavelengths are 6563 and3636 respectively.Example 4-17

    Calculate the longest and shortest wavelength i.e. serieslimit of the Paschen series. . B.U. B.Sc. 1991ASolutionThe formula for Paschen series of hydrogen atom is

    =

    22

    1

    3

    11

    nR

    , n =4,5,6, . . .

    Substitute n = 4

    1447

    41

    311

    22

    RR =

    =

    )10097.1(7144

    7144

    7

    ==R

    18750187510875.1 6 === nmm Substitute =n in above formula

    91

    311

    22

    RR =

    =

    710097.199

    ==R

    82044.82010204.8 7 === nmm The desired longest and shortest wavelengths are 1875 nm and820.4 nm respectively.

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    Example 4-18

    Determine the largest wavelength when excited electronmake transition to n = 4level. K.U. B.Sc. 2001SolutionThe wavelength of the emitted photon will; be the longest whenelectron jumps from n = 5 to n = 4. Hence

    400951411 22 RR =

    =

    )10097.1(9400

    9400

    7

    ==R

    nmm 405110051.4 6 == Note that this is the longest wavelength in Brackett series ofHydrogen atom.Example 4-19

    Compute the first three wavelengths for the Paschen seriesof hydrogen. In what region of the spectrum do the lines of

    Paschen series lie?SolutionThe formula for Paschen series of hydrogen atom is

    =

    22

    1

    3

    11

    nR

    , n =4,5,6, . . .

    Substitute n = 4 ,1447

    41

    311

    221

    RR =

    =

    R7144

    1 = )10097.1(7144

    7

    =

    nmm 187510875.1 61

    ==

    Substitute n = 5 ,22516

    51

    311

    222

    RR =

    =

    nmm

    R

    128210282.1

    )10097.1(16225

    16225

    62

    72

    ==

    ==

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    Substitute n = 6 ,126

    1311

    223

    RR =

    =

    nmmR

    109410094.110097.1

    1212 673 ==

    ==

    The wavelengths of desired lines are 1875 nm, 1282 nm and1094 nm. These lines lie in the infrared region of the spectrum.

    Example 4-20Find the wavelength of the spectral line corresponding tothe transition in hydrogen atom from n = 6 to n = 3 statewhere 710097.1 =R m-1. B.U. B.Sc. 1991SSolutionThe desired line is the third line in Paschen series. The Paschenseries is given by

    =

    22

    1

    3

    11

    nR

    , n =4,5,6, . . .

    Substitute n = 6

    1261

    311

    22RR =

    =

    710097.11212

    ==R

    109399.1093100939.1 6 === nmm

    Example 4-21

    In the hydrogen atom, an electron experiences a transitionfrom a state whose binding energy is 0.54 eV to anotherstate whose excitation energy is 12.2 eV. (a) What are the

    quantum numbers for these states? (b) Compute thewavelength of the emitted photon. (c) To what series doesthis line belong? K.U. B.Sc. 2008SolutionThe binding energy of the electron is given by

    2

    6.13n

    En = in eV

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    (a)The above equation can be rewritten as

    nEn

    6.13=

    Now 54.0=nE eV, therefore 554.06.13==n .

    The binding energy 0.54 eV corresponds to the state n = 5. Notethat the binding energy of the state n = 1 is 13.6 eV. As theexcitation energy is given as 10.2 eV, therefore

    eVEn 4.32.106.13 ==

    Hence 24.36.13==n

    i.e. the given excitation energy corresponds to state n = 2.

    (b)

    hceVEE === 86.254.04.352

    eV

    hc

    86.2

    =

    m7

    19

    834

    10336.4)10602.1)(86.2(

    )10998.2)(10626.6(

    =

    =

    4336= the wavelength of the emitted photon.(c) As the wavelength of the emitted photon is in the visibleregion, therefore it belongs to Balmer series of the hydrogenatom.

    Example 4-22

    A collection of hydrogen atoms in the ground state isilluminated with ultraviolet light of wavelength

    59.0 nm.

    Find the kinetic energy of the emitted electron.SolutionThe energy of the incident photon is given by

    Jch

    E 189

    834

    10367.3100.59

    )10998.2)(10626.6(

    =

    ==

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    eVeVE 0.2110602.110367.3

    19

    18

    =

    =

    The energy needed to separate the electron from hydrogen atomis given by

    eVE 6.131 =

    The kinetic energy of the emitted electron will beeVEEK 4.76.130.211 ===

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    4-2 HYDROGEN-LIKE ATOMSExample 4-23

    How much energy is required to remove the electron from asingly ionized helium atom (He+1) in its ground state?Solution

    The energy of electron in nth

    orbit for hydrogen-like atom isgiven by

    eVinn

    Z

    hn

    ZkmeEn 2

    2

    22

    2242 )6.13(2==

    Now n = 1 and Z = 2, therefore the desired energy is

    eVE 4.54)1(

    )2)(6.13(2

    2

    1 ==

    Example 4-24

    Apply the Bohrs theory to He+and calculate for n = 1(a) the radius, (b) the frequency of revolution, (c) the linear

    speed of the electron, (d) the total energy of the electron, (d)the angular momentum and (e) the ratio v/c, and (f) decidewhether the classical treatment can be used or not.

    Solution(a) The radius of nthorbit of electron in hydrogen-like atom isgiven by

    Z

    n

    eZmk

    hnrn

    211

    22

    22 )10287.5(4

    ==

    Substitute n = 1, Z = 2 in above equation

    mr11

    211

    1 10644.2

    2

    )1)(10287.5(

    =

    =

    (b) The orbital frequency of the electron in hydrogen-like atomis given by

    33

    42224

    hn

    eZkmfn

    =

    )10626.6()1()10602.1()2)(10988.8)(10109.9(4

    343

    41929312

    1

    =

    f

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    Hz1610631.2 = the desired frequency.(c) The velocity of electron in nthorbit of hydrogen-like atom isgiven by

    nh

    eZkvn

    22=

    )10626.6)(1(

    )10602.1)(2)(10988.8(234

    2199

    1

    =

    v sm/10375.4 61 =

    (d) The energy of electron in nth orbit for hydrogen-like atom isgiven by

    eVinn

    Z

    hn

    ZkmeEn 2

    2

    22

    2242 )6.13(2==

    eVE 4.54)1(

    )2)(6.13(2

    2

    1 ==

    (e) The angular momentum of electron in first orbit is given by

    )10644.2)(10375.4)(10109.9( 11631111

    == rvmL 123410054.1 = smkg

    (f) 015.010998.2

    10375.48

    6

    =

    =

    c

    v As the ratio (v/c) is small i.e. v

    is very small as compared with c, therefore classical treatment isapplicable.Example 4-25

    Determine the radius of the second Bohr orbit for doublyionized Lithium.Solution

    The radius of nthorbit for Hydrogen-like atom is given by

    Z

    rnrn

    12

    =

    where 53.01 =r is the radius of the first Bohr orbit ofHydrogen atom. Hence

    706.03

    )53.0()2( 22 ==r

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    Example 4-26

    How much energy is required to remove the electron from adoubly ionized lithium atom (Li+2) in its ground state?SolutionThe energy of electron in nth orbit for hydrogen-like atom isgiven by

    eVinn

    Zhn

    ZkmeEn 2

    2

    22

    2242

    )6.13(2 ==

    Now n = 1 and Z = 3, therefore the desired energy is

    eVE 4.122)1(

    )3)(6.13(2

    2

    1 ==

    Example 4-27

    (a) Compute the first and second excitation potentials forsingly ionized helium atom. (b) What wavelengths areemitted when the He+ returns to the ground state from theseexcited states?

    SolutionThe energy of electron in nth orbit for hydrogen-like atom isgiven by

    eVinn

    Z

    hn

    ZkmeEn 2

    2

    22

    2242 )6.13(2==

    eVnn

    22

    2 4.54)2)(6.13(== for He+

    Now n = 1 , eVE 4.54)1(

    4.5421

    ==

    n = 2 , eVE 6.13)2(

    4.5422 ==

    n = 3 , eVE 04.6)3(

    4.5423

    ==

    Let 1 and2be the first and second excitation energies of theHe+atom, then

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    1= eVEE 8.40)4.54(6.1312 == 2= eVEE 46.48)4.54(04.613 ==

    The desired excitation potentials are 40.8 V and 48.46 V.

    (b) Now 11

    hc= or

    )10602.1)(8.40()10998.2)(10626.6(

    19

    834

    11

    ==

    hc

    30410039.3 81 = m

    22

    hc= or

    )10602.1)(46.48()10998.2)(10626.6(

    19

    834

    212

    ==

    hc

    25610559.2 81 = m

    Example 4-28

    Determine the wavelength of the first two lines of singlyionized helium that corresponds to the first two lines of theBalmer series.SolutionThe formula for Balmer series of hydrogen-like atom is

    =

    222 1

    2

    11

    nZR

    , n = 3,4,5,..

    For singly ionized helium Z = 2 and above equation becomes

    =

    22

    1

    2

    14

    1

    nR

    , n = 3,4,5,..

    The desired wavelengths are calculated by substituting n = 3and n = 4 respectively in above relation. Now

    95

    31

    21

    41

    221

    RR =

    =

    164110641.1)10097.1(5

    959 7

    71 ==

    ==

    mR

    43

    4

    1

    2

    14

    122

    2

    RR =

    =

    121510215.1)10097.1(3

    434 7

    72 ==

    ==

    mR

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    Example 4-29

    Calculate the wavelengths of first two lines of the Balmerseries of triply ionized Beryllium (Z = 4).SolutionThe formula for Balmer series of Hydrogen-like atom is

    =

    222 1

    2

    11

    n

    ZR

    , n = 3,4,5,..

    For present case Z = 4 , therefore

    = 22

    2 121

    161

    nZ

    , n = 3,4,5,..

    Now n = 3,9

    2031

    21

    161

    221

    RR =

    =

    nmmR

    0.411010.4)10097.1(20

    920

    9 871 ==

    ==

    n = 4, RR 34

    1

    2

    116

    1

    222

    =

    =

    nmmR

    4.301004.3)10097.1(3

    13

    1 872 ==

    ==

    Hence the wavelengths of the first two lines of the Balmerseries of triply ionized Beryllium are 41.0 nm and 30.4 nmrespectively.Example 4-30

    An atom of tungsten has all of its electrons removed exceptone. (a) Calculate the ground-state energy for this oneremaining electron. (b) Calculate the energy and wavelength

    of the radiation emitted when this electron makes adownward transition from n = 2to n = 1. (c) In what portionof the electromagnetic spectrum is this photon?Solution(a)The energy of electron in nth orbit for hydrogen-like atom isgiven by

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    eVinn

    Z

    hn

    ZkmeEn 2

    2

    22

    2242 )6.13(2==

    For tungsten Z = 74, therefore

    keVn

    eVnn

    En 22

    4

    2

    2 5.741044736.7)74)(6.13(

    ==

    keVE 5.741 = the desired ground state energy.(b) When electron makes a downward transition from n = 2 ton = 1, the energy E of the emitted photon is given by

    keVkeVkeVEEE 9.55875.5511

    21

    5.742212 =

    ==

    The wavelength of the emitted photon is calculated from therelation

    )10602.1)(10875.55()10998.2)(10626.6(

    193

    834

    ==

    E

    hc

    222.010219.211

    =

    m (c) The emitted photon belongs to X-rays.

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    4-3 THE FRANK-HERTZ EXPERIMENTExample 4-31

    In Franck-Hertz experiment the ionization potential ofsodium is 5.13 V. Calculate the velocity of the electron.Solution

    The kinetic energy of the electron is given byVevm =

    2

    21

    1631

    19

    10343.1)10109.9(

    )10602.1)(13.5(22

    =

    == sm

    m

    Vev

    Example 4-32

    What will be the minimum energy of electron to excite2536 spectral line of mercury in a Franck-Hertzexperiment?

    SolutionThe minimum kinetic energy of electron to excite a spectral lineof wavelength is given by

    10

    934

    min 102536

    )10998.2)(10626.6(.).(

    ==

    hcEK

    eVorJ 890.410833.7 19=

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    4-4 ANGULAR MOMENTUMExample 4-33

    Calculate the value of Bohr magneton.SolutionThe Bohr magneton is defined as

    ee

    Bm

    eorm

    eh24

    h

    =

    12431

    3419

    10273.9)10109.9(4

    )10626.6)(10602.1(

    =

    = TJB

    The accepted value of Bohr magneton is 12410274.9 TJ or

    .10778.5 15 TeV Example 4-34

    Calculate the magnitude of the orbital angular momentumof an electron in a state with 4=l .

    SolutionThe magnitude of orbital angular momentum is given by

    sJL3434 10718.4)10055.1()14(4)1( =+=+= hll

    Example 4-35

    Write down the quantum numbers for all the hydrogenatom states belonging to subshells for which 4=n and 3=l .SolutionNow 4=n and 3=l . As

    ll

    = ..,.........2,1,0m therefore the desired magnetic quantum numbers are

    3,2,1,0,1,2,3 =lm

    The spin quantum number is given by21

    =Sm .

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    Example 4-36

    A hydrogen state is known to have the quantumnumber 3=l . What are possible n,

    lm and Sm .

    SolutionThe principal quantum number n must be greater than l which is 3 for present case. Hence n = 4 and the magnetic

    quantum number lm value are as under3,2,1,0,1,2,3 =

    lm

    The spin quantum number is given by21

    =Sm .

    Example 4-37

    If an electron in a hydrogen atom is in a state with 5=l ,what is the smallest possible angle between L and ZL .Solution

    The minimum angle occurs when ll =m and is given by

    [ ] )1()1(cos min

    +=

    +==

    ll

    l

    hll

    hl

    LLZ

    [ ] 91287.0)15(5

    5cos min =

    +=

    245241.24 00min = or

    Example 4-38

    Calculate and tabulate for a hydrogen atom in a state 3=l ,

    the allowed values of ZL , Z and. Find the magnitude of L and.Solution

    The corresponding values of magnetic quantum numberl

    m for

    3=l are 3,2,1,0,1,2,3 =l

    m .The desired values arecalculated and tabulated below. Here we have employed thefollowing values

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    sJ3410055.1 =h and TJB /10274.924

    =

    lm

    smkg

    mLZ

    /2h

    l=

    TJ

    m BZ

    /

    l

    =

    +=

    )1(cos 1

    ll

    lm

    -3 3410165.3 2310782.2 00.150-2 3410110.2 2310855.1 03.125

    -1 3410055.1

    2410274.9

    08.106 0 0 0 00.90 1 3410055.1 2410274.9 02.73 2 3410110.2 2310855.1 07.54 3 3410165.3 2310782.2 00.30 The magnitude of orbital angular momentum is given by

    sJL 3434 10655.3)10055.1()13(3)1( =+=+= hll The magnitude of dipole moment is given by

    TJB /10213.3))13(3)(10274.9()1(2324

    =+=+=

    ll

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    4-5 THE ZEEMAN EFFECTExample 4-39

    A hydrogen atom gas is placed in intense magnetic field of0.8 tesla. Compute the separation between two consecutivestates (Normal Zeeman Effect) when = 5000 .

    SolutionThe wavelength separation is given by

    hc

    B

    cm

    eB B

    e

    22

    4

    == where

    ee

    Bm

    eor

    m

    eh

    24h

    =

    )10998.2)(10626.6(

    )105000)(8.0)(10274.9(834

    21024

    =

    0937.010337.9 12 orm=

    Example 4-40

    What will be the separation, in , due to normal Zeemansplitting of 4916 line in the mercury spectrum in amagnetic field of 0.5 tesla?SolutionThe wavelength separation is given by

    )10998.2)(10626.6(

    )104916)(5.0)(10274.9(834

    10242

    ==

    hc

    BB

    212 1064.51064.5 == m

    Example 4-41

    Calculate the wavelengths of the normal Zeeman Effecttriplet of a spectral line 5500 placed in a magnetic field of10 tesla.SolutionThe wavelength separation is given by

    )10998.2)(10626.6(

    )105500)(10)(10274.9(834

    210242

    ==

    hc

    BB

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    412.110412.1 10 == m The wavelengths of Zeeman triplet are

    588.5498412.155001 === 55002 ==

    412.5501412.155003 =+=+= Example 4-42

    The Zeeman components of a 500 nm spectral line are0.0116 nm apart when the magnetic field is 1.00 tesla. Findthe ratio of e/mof the electron from this data.SolutionThe wavelength separation is given by

    cm

    eB

    e

    4

    2

    =

    or2

    )(4

    B

    c

    m

    e

    e

    =

    29

    98

    )10500)(1( )100116.0)(10998.2(4

    =

    eme

    kgCm

    e

    e

    /10733.1 11=

    Example 4-43

    A spectral line having a wavelength of 5500 shows anormal Zeeman splitting of 2101.1 . What is themagnitude of the magnetic field causing the splitting?Solution

    The wavelength separation is given by

    hc

    BB2

    =

    or21024

    102834

    2 )105500)(10274.9()}10)(101.1){(10998.2)(10626.6()(

    =

    =

    B

    hcB

    teslaB 078.0=

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    Example 4-44

    Find the minimum magnetic field needed for the ZeemanEffect to be observed in a spectral line of 400 nmwavelengthwhen a spectrometer whose resolution is 0.010 nmis used.SolutionThe wavelength separation is given by

    hcBB

    2

    =

    or 2)(

    B

    hcB

    =

    2924

    9834

    )10400)(10274.9()}10010.0){(10998.2)(10626.6(

    =B

    teslaB 339.1=

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    CONCEPTUAL QUESTIONS(1) What is meant by a stationary orbit in Bohrs theory ofHydrogen atom?Answer: - A stationary or allowed orbit is one in which electrondoes not radiate any energy i.e. the total energy of the electronremains constant.(2) What should be the angular momentum of the electronmoving in an allowed orbit?Answer: - The angular momentum of an electron should be anintegral multiple of )2/( h=h while moving in an allowed

    orbit i.e. hnL = .(3) How many electronic orbits are there in a Hydrogenatom?Answer: - Theoretically there are an infinite number of orbits ina Hydrogen atom. As there is only one electron in the Hydrogenatom, therefore one of these orbits will be occupied at one time.

    The remaining orbits will be vacant.(4) How is the spacing of adjacent electronic energy levels ofan atom affected by the value of n?Answer: - The spacing of adjacent electronic energy levels ofan atom decreases as n increases.(5) What is indicated by the existence of sharp lines in thespectrum of Hydrogen atom?Answer: - It indicates that the electron is moving in a givenorbit with certain frequency only.

    ORIt indicates the presence of discrete energy levels in the

    Hydrogen atom.(6) Which transition of the electron in Hydrogen atom willemit highest energy photon?Answer: - The transition of the electron from =n to

    1=n will emit maximum energy photon. The energy of thisphoton is eVeVEE 6.13)6.13()0(1 == .

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    (7) The total energy of the electron in Hydrogen atom isnegative. What is the physical significance of negative sign?Answer: - It reflects the fact that the electron is bound to thenucleus. An energy of 13.6 eV is needed to separate the electronfrom the nucleus of hydrogen atom.(8) Can a Hydrogen atom absorb a photon whose energyexceeds its biding energy?

    Answer: - Yes. The excess energy will appear as kinetic energyof the detached electron of Hydrogen atom.(9) Which series in the emission spectrum of Hydrogen atomhas the highest frequencies? In what part of the spectrumare these lines?Answer: - Lyman series. The spectral lines of Lyman series arein the ultraviolet region.(10) Any series of atomic Hydrogen yet to be discoveredwill probably found to be in what region of the spectrum?Answer: - In infrared region of the spectrum.(11) If an electron moves to a larger orbit, does its total

    energy increase or decrease? Does its kinetic energyincrease or decrease?Answer: - The total energy of an orbiting electron is given by

    r

    eZkE

    2

    2

    =

    As rincreasesEbecomes less negative and therefore increases.The orbital kinetic energy of the electron is given by

    r

    eZkK

    2

    2

    =

    It is clear that Kdecreases with increase in r.

    (12) Under what conditions an electron moving in the orbitwill have de Broglie wavelength?Answer: -The electron orbit (i.e. the circumference of circularorbit) must contain an integral number of de Brogliewavelengths.

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    (13) What are two essential features of the vector atommodel?Answer: - (a) Space quantization and (b) Hypothesis ofspinning electron.(14) What is minimum energy needed to create an Electron -positron pair?Answer: - The minimum energy needed to create an electron-

    positron pair is given by MeVcm 022.12 20 = .(15) What is the wavelength of the photon corresponding tothe threshold energy needed to produce electron-positronpair i.e. 1.022 MeV?Answer: - 0.012

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    ADDITIONAL PROBLEMS(1)Compute the first three wavelengths of the Bracket

    series of hydrogen.(2)The binding energy of electron in a certain state of

    hydrogen atom is 0.85 eV. What is the correspondingquantum number?

    (3)A photon of energy 12.1 eVabsorbed by a hydrogenatom, originally in the ground state, raises the atomto an excited state. What is the quantum number ofthis state?

    (4)Determine the speed of electron in the n = 8orbit ofhydrogen atom. Use this value to find thecorresponding de Broglie wavelength.

    (5)The lifetime of an excited state is about 810 second.Compute how many revolutions an electron ofhydrogen atom in the excited state n = 4will make

    before jumping in the ground state?(6)Which of the spectral lines of the Bracket series isclosest in wavelength to the first spectral line of thePaschen series of hydrogen atom? What is differencein their wavelengths?

    (7)Find the radius of the smallest Bohr orbit in doublyionized lithium ( ++Li ). What will be the energy ofelectron in this orbit?

    Answers

    (1) mandmm 666 10166.210625.2,10051.4

    (2) 4 (3) 3 (4) 1510734.2 sm , 2661 (5) 71004.1 Revolutions (6) Fifth line (n = 9)(7) 0.18 , -122 eV