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5/28/2018 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=
5/28/2018 Chapter 4 Atomic Structure (Pp 96-125)
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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