Matriculation Physics Bohrs Model of Hydrogen Atom.pdf

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    1

    PHYSICS CHAPTER 11

    CHAPTER 11:CHAPTER 11:

    Bohrs model of hydrogen atomBohrs model of hydrogen atom(3 Hors!(3 Hors!

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    PHYSICS CHAPTER 11

    2

    At the end of this chapter, students should be able to:At the end of this chapter, students should be able to:

    ExplainExplainBohrs postulates of hydrogen atom.Bohrs postulates of hydrogen atom.

    Learning Outcome:

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    PHYSICS CHAPTER 11

    4

    "utherfords model of atom"utherfords model of atom

    In 1*11+ Ernest Rtherford %erformed a r&t&al e%er&ment that

    sho"ed the Thomsons model &s not orret and %ro%osed h&sne" atom& model $no"n as Rtherfords %lanetary model of the

    atom as sho"n &n /&gre 11#2a#

    Aord&ng to Rtherfords model+ the atom "as %&tred as

    eletrons or.&t&ng arond a entral nles "h&h onentrated

    of %os&t&-e harge#

    The eletrons are aelerat&ng .ease the&r d&ret&ons are

    onstantly hang&ng as they &rle the nles#

    nles

    eletron

    !igure 11.#a!igure 11.#a

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    PHYSICS CHAPTER 11

    5

    Based on the "a-e theory+ an aelerat&ng harge em&ts energy#

    Hene the eletrons mst em&t the E rad&at&on as they re-ol-e

    arond the nles# As a reslt of the ont&nos loss of energy+ the rad&& of the

    eletron or.&ts "&ll .e dereased stead&ly#

    Th&s "old lead the eletrons s%&ral and falls &nto the nles+

    hene the atom "old olla%se as sho"n &n /&gre 11#2.#

    !igure 11.#b!igure 11.#b

    ++Ze ee

    0%lo%

    energy loss

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    PHYSICS CHAPTER 11

    6

    +e

    ev

    r

    eF

    In 1*13+ 4e&ls Bohr %ro%osed a ne" atom& model .ased onhydrogen atom#

    Aord&ng to Bohrs odel+ he assmes that each electroneach electron

    mo$es in a circular orbit %hich is centred on the nucleusmo$es in a circular orbit %hich is centred on the nucleus+

    the neessary centripetal force being pro$ided by thecentripetal force being pro$ided by the

    electrostatic force of attraction bet%een the positi$elyelectrostatic force of attraction bet%een the positi$elycharged nucleus and the negati$ely charged electroncharged nucleus and the negati$ely charged electronas

    sho"n &n /&gre 11#3#

    11.1.# Bohrs model of hydrogen atom

    !igure 11.&!igure 11.&

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    PHYSICS CHAPTER 11

    7

    5n th&s .as&s he "as a.le to sho" that the energy of anenergy of an

    orbiting electron depends on the radius of its orbitorbiting electron depends on the radius of its orbit#

    Th&s model has se-eral featres "h&h are desr&.ed .y the%ostlates (assm%t&ons! stated .elo" :

    1# The electronselectronsmo-e only &n erta&n &rlar or.&ts+ alled

    'A(O)A"* 'AE''A(O)A"* 'AE'or E)E"+* LEEL'E)E"+* LEEL'# 6hen &t &s

    &n one of these or.&ts+ &t does not radiate energydoes not radiate energy#

    2# The only permissible orbits arepermissible orbits arethose &n the d&srete setfor "h&h the angular momentum of the electronangular momentum of the electronLL

    e-uals an integer timese-uals an integer times h/h/22# athemat&ally+

    2

    nhL=

    2

    nhmvr= 11.1/11.1/

    and mvrL=

    "here

    orbittheofradius:r electrontheofmass:m

    ,...,,n 321numberquantumprincipal: =

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    PHYSICS CHAPTER 11

    8

    3# Emission or absorptionEmission or absorptionof rad&at&on ors only "hen an

    electron ma0es a transition from one orbit to anotherelectron ma0es a transition from one orbit to another#

    The fre7enyfof the em&tted (a.sor.ed! rad&at&on &sg&-en .y

    if EEhfE == 11.#/11.#/

    "here

    constantsPlanck':hstateenergyfinal:fE

    energyofchange:E

    stateenergyinitial:iE)ote:)ote:

    IfEf>E

    i

    IfEf

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    PHYSICS CHAPTER 11

    9

    At the end of this chapter, students should be able to:At the end of this chapter, students should be able to: eri$eeri$eBohrs radius and energy le$el in hydrogen atom.Bohrs radius and energy le$el in hydrogen atom. 2se2se

    efineefine

    ground state energy, excitation energy andground state energy, excitation energy and

    ionisation energy.ionisation energy.

    Learning Outcome:

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    11#2 Energy le-el of hydrogen atom (1hor!

    ==

    22

    2

    2

    ! mkehnanrn

    andand

    =

    2

    2 1

    2 na

    keEn

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    PHYSICS CHAPTER 11

    10

    11.#.1 Bohrs radius in hydrogen atom

    Cons&der one eletron of hargeeand mass mmo-es &n a

    &rlar or.&t of rad&s rarond a %os&t&-ely harged nles

    "&th a -elo&ty vas sho"n &n /&gre 11#3# The electrostatic force bet%een electron and nucleuselectrostatic force bet%een electron and nucleus

    contributes the centripetal forcecontributes the centripetal forceas "r&te &n the relat&on .elo":

    11.# Energy le$el of hydrogen atom

    ce FF = entr&%etal foreeletrostat& fore

    r

    mv

    r

    QQ 2

    2

    21

    !

    1

    =

    and eQQ == 21

    r

    emv

    22

    ! = 11.&/11.&/

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    PHYSICS CHAPTER 11

    11

    /rom the Bohrs seond %ostlate:

    By ta$&ng s7are of .oth s&de of the e7at&on+ "e get

    By d&-&d&ng the e7s# (11#8! and (11#3!+ ths

    2

    nh

    mvr=

    11.3/11.3/2

    22222

    !

    hnrvm =

    =

    re

    hn

    mv

    rvm

    2

    2

    22

    2

    222

    !

    !

    2

    22

    me

    hnr= and

    k

    !

    1=

    electrostaticelectrostatic

    constantconstant

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    PHYSICS CHAPTER 11

    12

    "h&h rn&s radii of the permissible orbitsradii of the permissible orbitsfor the Bohrs atom# E7# (11#9! an also .e "r&tten as

    "here a&s alled the Bohrs radiusBohrs radiusof hydrogen atom#

    =kme

    hnr

    !

    12

    22

    11.4/11.4/"""3#2#1$! 22

    22 =

    = n

    mke

    hnrn

    2anrn=

    22

    2

    ! mke

    ha

    =

    11.5/11.5/

    and

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    PHYSICS CHAPTER 11

    13

    The Bohrs rad&s &s def&ned as the radius of the most stablethe radius of the most stable

    lo%est/ orbit or ground state lo%est/ orbit or ground state nn=1=1//in the hydrogen atomin the hydrogen atom

    and &ts -ale &s

    n&t on-ers&on:

    The rad&& of the or.&ts asso&ated "&th allo"ed or.&ts or states

    n % 2#3#&are !a,'a,+ ths the orbits radii areorbits radii are-uanti6ed-uanti6ed#

    ( )( )( )( )21''312

    23!

    1("11"'111"'!

    1(3"(

    =

    a

    m131") 11 =a 5R ")31 * (angstrom!

    1 * % 1" 11 m

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    PHYSICS CHAPTER 11

    14

    &s def&ned as a fixed energy corresponding to the orbits ina fixed energy corresponding to the orbits in%hich its electrons mo$e around the nucleus%hich its electrons mo$e around the nucleus#

    The energy le-els of atoms are -uanti6ed-uanti6ed#

    The total energy le$eltotal energy le$elEEof the hydrogen atomof the hydrogen atom&s g&-en .y

    7otential energy7otential energy UUof the electronof the electron &s g&-en .y

    11.#.# Energy le$el in hydrogen atom

    KUE += 11.8/11.8/9inetic energy of the electron9inetic energy of the electron

    7otential energy of the electron7otential energy of the electron

    r

    QkQ

    U21

    = eQeQ == 21 $"here 2

    anr=and

    2

    2

    an

    keU = 11./11./

    nucleusnucleus electronelectron

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    PHYSICS CHAPTER 11

    15

    9inetic energy9inetic energyKKof the electronof the electron &s g&-en .y

    Therefore the e7# (11#;! an .e "r&tten as

    2

    2

    1mvK=

    11.;/11.;/

    .t r

    emv

    22

    ! =

    =

    r

    eK

    2

    !2

    1

    "here k=

    !

    1

    =

    2

    2

    2

    1

    an

    keK

    +=

    2

    2

    2

    2

    21

    anke

    ankeEn

    and 2anr=

    =2

    2 1

    2 na

    keEn 11.1

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    PHYSICS CHAPTER 11

    16

    In general+ the total energy le-elEfor the atom&s

    s&ng nmer&al -ale of k+ eand a+ ths the e7# (11#1

    "r&tten as

    = 2

    2

    2

    2 n

    Z

    a

    ke

    En 11.11/11.11/

    ( )( )( )

    =

    211

    21'' 1

    131")2

    1("11"'

    nEn

    =

    21'

    1+ 1e,

    1("1

    11-"2

    n

    1#2#3#"""e,$("132

    == nn

    En 11.1#/11.1#/

    )ote:)ote:

    E-s. 11.1

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    PHYSICS CHAPTER 11

    17

    The negati$e signnegati$e sign&n the e7# (11#12! &nd&ates that %or0 has to%or0 has to

    be done to remo$e the electron from the bound of the atombe done to remo$e the electron from the bound of the atom

    to infinityto infinity+ "here &t &s ons&dered to ha-e 6ero energy6ero energy# The energy le-els of the hydrogen atom are "hen

    n=1+ the ground stateground state(the state of the lo%est energy le$ello%est energy le$el! >

    n=2+ the first excited statefirst excited state>

    n=3+ the second excited statesecond excited state>

    n=8+ the third excited statethird excited state>

    n=+ the energy le-el &s

    ( )

    e,(13e,

    1

    ("1321 .E ==

    ( )e,!3e,

    2

    ("1322 .E ==

    ( )

    e,("132

    =

    =E

    ( )e,)11e,

    3

    ("1323 .E ==

    ( )e,+)e,

    !

    ("132! .E ==

    electron is completelyelectron is completely

    remo$ed from the atomremo$ed from the atom#

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    PHYSICS CHAPTER 11

    19

    The eletron &n the hydrogen atom ma$es a trans&t&on from the

    energy state of

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    PHYSICS CHAPTER 11

    20

    The lo"est energy state for hydrogen atom &s 13# e@# eterm&ne

    the fre7eny of the %hoton re7&red to &on&De the atom#

    (?&-en the s%eed of l&ght &n the -am+ c=3#

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    PHYSICS CHAPTER 11

    21

    /or an eletron &n a hydrogen atom harater&Ded .y the %r&n&%al

    7antm nm.er n=2+ allatea# the or.&tal rad&s+.# the s%eed+

    # the $&net& energy#

    (?&-en c=3#

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    PHYSICS CHAPTER 11

    22

    'olution :'olution :

    .# By a%%ly&ng the Bohrs 2nd%ostlate+ ths

    # The $&net& energy of the or.&t&ng eletron &s g&-en .y

    ( ) ( )

    3!131 1(3"(112"2111" = v

    1( sm1"1 =v

    2nhmvrn=

    2=n

    2

    22

    hmvr =

    2

    21 mvK=

    ( )( )2(31 1"1111"2

    1=

    1!1")1

    =K

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    PHYSICS CHAPTER 11

    23

    A hydrogen atom em&ts rad&at&on of "a-elengths 221#9 nm and

    2

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    PHYSICS CHAPTER 11

    24

    'olution :'olution :

    a# The energy of the %hoton de to trans&t&on from 2nde&ted state

    to the grond state &s

    .#

    Therefore the "a-elength of the em&tted %hoton de to the

    trans&t&on from 2nde&ted state to the 1ste&ted state &s

    m1!"22m$1)"221 2

    1 ==

    ( )( )

    +3!

    21!"22

    1"31(3"(

    =E

    1+3" 12=E

    4E1 4E2

    4E3

    ?rond state

    1st e&ted state

    2nd e&ted state

    123 EEE =11

    3 1+"+1+3" =E

    1)"+2

    3

    =E

    3

    3

    hcE =

    ( )( )

    3

    +3!2 1"31(3"(1)"+

    =

    m13!"2 (3 =

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    PHYSICS CHAPTER 11

    25

    At the end of this chapter, students should be able to:At the end of this chapter, students should be able to:

    ExplainExplainthe emission of line spectrum by using energythe emission of line spectrum by using energy

    le$el diagram.le$el diagram.

    'tate'tatethe line series of hydrogen spectrum.the line series of hydrogen spectrum. 2se2seformula,formula,

    Learning Outcome:

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    PHYSICS CHAPTER 11

    26

    The em&ss&on l&nes orres%ond to the %hotons of d&sreteenerg&es that are em&tted "hen e&ted atom& states &n the gasma$e trans&t&ons .a$ to lo"er energy le-els#

    /&gre 11#9 sho"s l&ne s%etra %roded .y em&ss&on &n the-&s&.le range for hydrogen (H!+ merry (Hg! and neon (4e!#

    11.& Line spectrum

    !igure 11.4!igure 11.4

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    PHYSICS CHAPTER 11

    27

    Em&ss&on %roesses &n hydrogen g&-e r&se to ser&es+ "h&h are

    se7enes of l&nes orres%ond&ng to atom& trans&t&ons# The ser&es &n the hydrogen em&ss&on l&ne s%etrm are

    Lyman seriesLyman series&n-ol-eselectron transitionselectron transitions thatend at theend at the

    ground state of hydrogen atomground state of hydrogen atom# It &s &n the ltra$ioletltra$iolet

    2/ range2/ range#

    Balmer seriesBalmer series&n-ol-eselectron transitionselectron transitions that end atend atthe 1the 1ststexcited state of hydrogen atomexcited state of hydrogen atom# It &s &n the $isible$isible

    light rangelight range#

    7aschen series7aschen series&n-ol-eselectron transitionselectron transitions thatend atend at

    the #the #ndndexcited state of hydrogen atomexcited state of hydrogen atom# It &s &n the infraredinfrared

    ("/ range("/ range# Brac0ett seriesBrac0ett series&n-ol-eselectron transitionselectron transitions that end atend at

    the &the &rdrdexcited state of hydrogen atomexcited state of hydrogen atom# It &s &n the ("("

    rangerange#

    7fund series7fund series &n-ol-eselectron transitionselectron transitions that end at theend at the

    33thth

    excited state of hydrogen atomexcited state of hydrogen atom# It &s &n the (" range(" range#

    11.&.1 =ydrogen emission line spectrum

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    PHYSICS CHAPTER 11

    29

    /&gre 11#; sho"s F%erm&ttedG or.&ts of an eletron &n the Bohrmodel of a hydrogen atom#

    !igure 11.5: not to scale!igure 11.5: not to scale

    P&tre 11#1

    http://opt/scribd/conversion/tmp/scratch2594/G:/P&P/Semester1/Latest/p11_01_01_01a.swfhttp://opt/scribd/conversion/tmp/scratch2594/G:/P&P/Semester1/Latest/p11_01_01_01a.swfhttp://balmer_series.jpg/
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    PHYSICS CHAPTER 11

    30

    If an eletron ma$es a trans&t&on from an oter or.&t of le-el nito

    an &nner or.&t of le-el nf+ ths the energy &s rad&ated#

    The energy radiatedenergy radiated&n form of E> radiation photon/form of E> radiation photon/"here

    the "a-elength &s g&-en .y

    /rom the Bohrs 3rd%ostlate+ the e7# (11#13! an .e "r&tten as

    11.&.# ?a$elength of hydrogen emission line

    spectrum

    hcE=hcE=

    1 11.1&/11.1&/

    if11 nn EEhc ="here

    = 2

    f

    2

    12f nakeEn

    and

    =

    2

    i

    2 1

    2i na

    keEn

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    PHYSICS CHAPTER 11

    31

    =

    2

    i

    2

    2

    f

    2 1

    2

    1

    2

    11

    na

    ke

    na

    ke

    hc

    =

    2

    i

    2

    f

    2 11

    2

    1

    nna

    ke

    hc

    =

    2

    i

    2

    f

    2 11

    2 nnhca

    keand HR

    hca

    ke=

    2

    2

    = 2i2

    f

    111

    nnRH 11.13/11.13/

    "here1- m1-"1constants5ydberd': =HR

    nn of0aluefinal:f

    nn of0alueinitial:i

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    PHYSICS CHAPTER 11

    32

    )ote:)ote:

    /or the hydrogen l&ne s%etrm+

    LymanLyman ser&es(nnff=1=1!

    BalmerBalmer ser&es(nnff=2=2!

    7aschen7aschen ser&es(nnff=3=3!

    Brac0ettBrac0ett ser&es(nnff=4=4!

    7fund7fund ser&es(nnff=5=5!

    To allate the shortest %a$elength in any seriesshortest %a$elength in any series+ ta$e nnii== #

    = 2i21

    1

    11

    nR

    H

    =

    2

    i

    2

    1

    2

    11

    nRH

    =

    2

    i

    21

    311

    nRH

    =

    2

    i

    2

    1

    !

    11

    nRH

    =

    2

    i

    2

    1

    )

    11

    nRH

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    PHYSICS CHAPTER 11

    33

    The Bohrs model of hydrogen atom

    %red&ts sessflly the energy le-els of the hydrogen atom.t fails to explain the energy le$els of more complexfails to explain the energy le$els of more complexatomsatoms#

    an e%la&n the s%etrm for hydrogen atom .t somedeta&ls of the s%etrm cannot be explained especiallycannot be explained especially%hen the atom is placed in a magnetic field%hen the atom is placed in a magnetic field#

    annot e%la&n the eeman effet (/&gre 11#;!# @eeman effect@eeman effect&s def&ned as the splitting of spectralthe splitting of spectral

    lines %hen the radiating atoms are placed in alines %hen the radiating atoms are placed in amagnetic field.magnetic field.

    11.&.& Limitation of Bohrs model of hydrogen atom

    agnet& f&eld

    Trans&t&ons

    4o magnet& f&eld

    11

    ##Energy e-els

    S%etra!igure 11.8!igure 11.8

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    PHYSICS CHAPTER 11

    34

    The Balmer ser&es for the hydrogen atom orres%onds to eletron&

    trans&t&ons that term&nate at energy le-el n=2 as sho"n &n the/&gre 11#)#

    Callatea# the longest "a-elength+ and

    .# the shortest "a-elength of the %hoton em&tted &n th&s ser&es#

    (?&-en the s%eed of l&ght &n the -am c=3#

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    PHYSICS CHAPTER 11

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    PHYSICS CHAPTER 11

    37

    eterm&ne the "a-elength for a l&ne s%etrm &n yman ser&es

    "hen the eletron ma$es a trans&t&on from n=3 le-el#

    (?&-en Ryd.ergs onstant +RH= 1#

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    PHYSICS CHAPTER 11

    38

    Eer&se 11#1 :?&-en c=3#

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    39

    PHYSICS CHAPTER 11

    Next ChapterCHAPTER 12 :

    JKrays