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Solutions Manual for Solid State Physics An Introduction to Theory 1st Edition by Joginder

Page 1

Solution Manual Solid State Physics: An Introduction to Theory


Chapter 1 Problem 1.1: Solution: Operate the operator S ni R n  S mi R n  on the position vector r to write

S

ni

R n  S mi R n  r = S ni R n  (Smi r + R n )

= S ni S mi r + S ni R n + R n = Sni Smi Sni R n + R n 

(S1.1)

Problem 1.2: Solution: Operate the operator S ni R n  on the position vector r to get the transformed vector r  , i.e.,

S

ni

R n  r = r  = S ni r + R n

(S1.2)

It can be written as

S ni r = r  − R n

(S1.3)

Operate the above equation by S −ni1 from the left side to write

S −ni1 S ni r = S −ni1 r  − S −ni1 R n r = S −ni1 r  − S −ni1 R n =

S − S R  r −1 ni

−1 ni

(S1.4)

n

From the definition of the inverse transformation the above equation can also be written as r=

S

R n  r −1

ni

(S1.5)

From Eqs. (S1.4) and (S1.5) one immediately write

S

R n  = S −ni1 − S −ni1 R n −1

ni

(S1.6)

Problem 1.3: Solution: In the bcc structure there are two atoms in a cube with edge a (see Fig. 1.14). Therefore, the volume per atom is a 3 / 2 . Alternately the volume per atom is given by


V0 = a1  a 2  a 3

(S1.7)

For a bcc structure from Eq. (1.37) one can write

a2  a3 =

=

(

)(

1 2 ˆ ˆ ˆ a − i1 + i 2 + i 3  ˆi1 − ˆi 2 + ˆi 3 4

(

1 2 ˆ ˆ a i1 + i 2 2

)

)

Perform the dot product with a1 from the left side to write

a1  a 2  a 3 =

=

(

)(

1 3 ˆ ˆ ˆ ˆ ˆ a i1 + i 2  i1 + i 2 − i 3 4

)

a3 2

Problem 1.4: .Solution: The angle between two primitive vectors a1 and a 2 can be calculated from their dot

product defined as

a1  a 2 = a1 a 2 cos cos =

a1  a 2 a1 a 2

(S1.8) (S1.9)

Here  is the angle between the two vectors a1 and a 2 . From Eq. (1.37) it is straightforward to prove that

a1 = a 2 = 3 a/2

(S1.10)

Substitute the expressions for a1 and a 2 for bcc structure from Eq. (1.37) in Eq. (S1.9) and use Eq. (S1.10) one gets

cos = Hence

− a2 / 4 1 = − = − 0.33 2 3 3a / 4

 = cos − 1 (− 0.33) = 109.47 o or 109 o 28


Problem 1.5: Solution: In the fcc structure there are four atoms in a cube with edge a (see Fig. 1.19a). Therefore, the volume per atom is a 3 / 4 . Alternately the volume per atom is given by

V0 = a1  a 2  a 3

(S1.11)

For fcc structure from Eq. (1.38) one can write

a 2  a3 =

(

)(

1 2 ˆ ˆ a i 2 + i 3  ˆi 3 + ˆi1 4

=

(

1 2 ˆ ˆ ˆ a i1 + i 2 − i 3 4

)

)

Perform the dot product with a1 from the left side to write

V0 = a1  a 2  a 3 =

(

)(

1 3 ˆ ˆ ˆ ˆ ˆ a i1 + i 2  i1 + i 2 − i 3 8

)

= a3 / 4 Problem 1.6: Solution: The angle between two primitive vectors a1 and a 2 can be calculated from the relation

cos =

a1  a 2 a1 a 2

(S1.12)

From Eq. (1.38) it is straightforward to prove that

a1 = a 2 = a/ 2

(S1.13)

Substitute the expressions for a1 and a 2 for fcc structure from Eq. (1.38) in Eq. (S1.12) and use Eq. (S1.13) one gets

cos = Hence

a2 / 4 1 = 2 2 a /2

 = cos − 1 (1 / 2 ) = 60 o


Problem 1.7: Solution: a) Packing fraction in bcc structure In a bcc structure there are two atoms in a cube with side a (see Fig. 1.14). Let r be the radius of an atom in a bcc structure, then in the close packing state three atoms along the diagonal of the cube should touch each other. Therefore, 4r = 3 a

(S1.14)

Hence the volume of an atom becomes V0 =

4 3  3 3 r = a 3 16

(S1.15)

The packing fraction is given by fp =

(

)

2  3 / 16 a 3  3 = = 0.68 8 a3

(S1.16)

b) Packing fraction in fcc structure In a fcc structure there are four atoms in a cube with side a (see Fig. 1.19a). Let r be the radius of an atom in a fcc structure, then in the close packing state three atoms along the diagonal of the basal plane of the cube should touch each other. Therefore, 4r = 2 a

(S1.17)

Hence the volume of an atom becomes V0 =

4 3  r = a3 3 12 2

(S1.18)

The packing fraction is given by

fp =

(

)

4  / 12 2 a 3  = = 0.74 3 a 3 2

(S1.19)


Problem 1.8: Solution: From Eq. (1.40) one can write  1 3 ˆ  ˆ a 2  a 3 =  − a ˆi1 + a i 2   c i 3 2 2   =

ac ˆ i2 + 2

(S1.20)

3ac ˆ i1 2

The volume per atom becomes ac V0 = a1  a 2  a 3 = a ˆi1   ˆi 2 +  2 =

3acˆ  i1  2 

3a2 c 2

(S1.21)

The same result can be obtained from the lattice vectors of the hexagonal structure given by Eq. (1.41). Problem 1.9: Solution: In the hcp structure there are 6 atoms in the unit cell shown in Fig. 1.23b. The volume of the unit cell of hcp structure V (Fig.1.23b) is three times the volume of the primitive cell, i.e., V=

3 3 2 a c 2

(S1.22)

In the close packing the atoms in the basal plane of the unit cell touch each other. Therefore, twice the radius of an atom must be equal to the lattice vector in the basal plane, i.e.,

2r = a

(S1.23)

4 3 a r = 8   =  a 3 3 2 3

Volume of six atoms in the unit cell = 6

Packing fraction f p =

 a3 2

3 3 a c/2

In an ideal hcp structure

=

2 a 3 3c

(S1.24)


Here x 1 and x 2 are the distances moved by the positively and negatively charged ions having masses M1 and M 2 , respectively. Z is the valency of both the negatively and positively charged ions (assumed to be the same). The net dipole moment per unit cell becomes

p I = p I1 − p I2 = Z e (x 1 + x 2 )

(S15.42)

Let  F1 and  F2 are the force constants for the positively and negatively charged ions then the forces acting on the ions are given by Z e E 0 = F1 =  F1 x 1 = M1 02 x 1

(S15.43)

− Z e E 0 = F2 = −  F2 x 2 = − M 2 02 x 2

(S15.44)

Here  0 is the natural frequency of vibration. From the above equations x1 =

Ze E0 M1  02

(S15.45)

x2 =

Ze E0 M 2  02

(S15.46)

Substitute Eqs. (S15.45) and (S15.46) in Eq. (S15.42) we write

pI =

Z2e2 E 0

  02

(S15.47)

where  is the reduced mass defined as 1

=

1 1 + M1 M 2

(S15.48)

The ionic polarizability is given by

 Ia =

pI Z2 e2 = E0   02

(S15.49)


Chapter 17 Problem 17.1: Solution: Fig. 17.4 shows the propagation of a plane wave from one medium into the other where the polarization of the wave is parallel to the interface. The four boundary conditions are defined by Eqs. (17.37) to (17.40) or by Eqs. (17.43) to (17.46). From the Fig. 17.4 it is evident that the magnetic field is parallel to the interface separating the two media. Therefore, there is no component of magnetic field B perpendicular to the interface and hence the boundary condition (17.42) becomes redundant. The boundary condition (17.45) can be written as

E 0 sin (/2 − i ) − E 0 sin (/2 − i ) = E 0 sin (/2 − r ) which can be written as

(E 0 − E 0 ) cos i = E 0 cos r

(S17.1)

The boundary conditions (17.37) and (17.40) become the same. Eq. (17.40) can be written as

1

(B 0 + B0 )  nˆ = 1 B0  nˆ

(S17.2)

(B 0 + B0 ) = 1 B0

(S17.3)



 1



Substitute the value of B 0 from Eq. (17.22) in the above equation we write

 ( E 0 + E0 ) = 

 E 0 

(S17.4)

Eqs. (S17.1) and (S17.4) can be solved for E 0 / E 0 and E 0 / E 0 to yield

E 0 =2 E0

 sin 2i    sin 2r +  sin 2i 

 sin 2i − sin 2r E 0  =  E0 sin 2r + sin 2i  For  =   the above equations reduce to

(S17.5)

(S17.6)


E 0 2 cos i sin r → E0 sin (i + r ) + cos (i − r )

(S17.7)

E 0 tan (i - r ) → E0 tan (i + r )

(S17.8)

Problem 17.2: Solution: Eqs. (17.84) and (17.85) of the text can be written here for completeness as

1.

n 2 − n 22 = n 12 − n 22 =  1

(S17.9)

2 n n 2 = 2 n1 n 2 =  2

(S17.10)

(n + n ) = (n − n ) + 4 n n

n 2 + n 22 =

2

2 2 2

2

2 2 2

2

2 2

=  12 +  22

(S17.11)

2. Add Eqs.(S17.9) and (S17.11) we get

2 n 2 =  12 +  22 +  1

(S17.12)

(S17.13)

1  12 +  22 +  1 2 3. Subtract Eq. (S17.9) from Eq. (S17.11) we get n2 =

2 n 22 =  12 +  22 −  1

1  12 +  22 −  1 2 4. One can write n 22 =

(

2 n = 4 n 2 = 2 n 2 + n 22 + n 2 − n 22 =

(

2  12 +  22 +  1

)

) (S17.14)

Problem 17.3: Solution: According to Eq. (17.99) the reflection coefficient is given by

R=

(n − 1)2 + n 22 (n + 1)2 + n 22

(S17.15)


n 2 + n 22 + 1 − 2 n R= 2 n + n 22 + 1 + 2 n

(S17.16)

Substitute for n 2 + n 22 and 2 n from Eqs. (S17.11) and (S17.14) in the above equation one gets

) ( 1 +  +  + 2(  +  +  ) 1 +  12 +  22 −

R=

2 1

2 2

2  12 +  22 +  1 2 1

2 2

(S17.17)

1

Problem 17.4: Solution: The equation of motion of the electron is given by Eq. (17.154) and is written as

me

d2x dx + = e E = e E 0 e  t 2 dt dt

(S17.18)

The electrons collide with the atoms and ultimately acquire a small constant velocity called drift velocity under the influence of a steady and slowly varying electric field. The constant drift velocity yield zero acceleration, i.e.

d2x =0 dt 2 Therefore, the equation of motion given by Eq. (S17.18) reduces to

dx = e E = e E 0 e  t dt

(S17.19)

The above equation gives

 =

eE vd

(S17.20)

where the drift velocity v d = dx/dt . The current density j is defined as

J = n ee vd Or

vd =

 J = 0 E n ee n ee

Substitute Eq. (S17.22) for v d in Eq. (S17.20) we get

(S17.21) (S17.22)


 =

n ee2

(S17.23)

0

Problem 17.5: Eq. (17.177) is written as

 Pi2  ( ) =  ( ) − 2  −  02

(S17.24)

From the above equation for  = 0 we get

 (0) −  ( ) =

 Pi2  02

(S17.25)

Now Eq. (S17.24) can be written as

 ( ) −  ( ) =

 Pi2 1 2  0 1 −  2 /  02

(S17.26)

With the help of Eq. (S17.25) one gets

 ( ) −  ( ) =  (0 ) −  ( )

 ( ) −  ( ) =  (0) −  ( )

1 1 −  2 /  02

 02  02 −  2

(S17.27)

Problem 17.6: Eq. (S17.27) can be written as

 ( ) =  ( ) +  (0) −  ( )

 ( ) =

 ( ) =

 02  02 −  2

( −  )  () +   (0) −  () 2 0

2

2 0 2

 02 − 

 02  (0) −  2  ( )  02 −  2   (0 ) − 2  ( )   2 2 0 − 

 ( ) =

 ( )  02

Using Eq. (17.186) the above equation becomes

(S17.28)


 L2 −  2  ( ) =  ( ) 2 T −  2 Or

2 − 2  ( ) = L2  ( )  T −  2

(S17.29)

Problem 17.7: The equation of motion of an electron in the presence of finite mean free path is given by

me

m dx d2x + e = − eE 2  e dt dt

(S17.30)

In terms of velocity the above equation can be written as me

m dv + e v = − eE dt e

(S17.31)

The current density due to the flow of electrons is defined as

J = − ne e v

(S17.32)

Multiply Eq. (S17.31) by − n e e , we write me

m d (− n e e v) + e (− n e e v) = n e e 2 E dt e

n e2 dJ 1 + J= e E dt  e me Rearrange the terms we write

 me dJ n e e 2   E − = J  2 dt me  ne e  e  n e e2  dJ J   E −  = dt me   0 

(S17.33)


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