homework 12 solution - university of illinois€¦ · 3. problem 2.4 in the book. this shows how...

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Homework 12 Solution 1. Problem 2.2 in the book. Solution: For the particle in a 1D box, ! = ! ! ! ! !!! ! 1 mole (6.02 x 10 -23 molecules) weighs 28g =0.028 kg. So, 1 N 2 molecule weighs 0.028/(6.02 x 10 -23 ) = 4.65 x 10 -26 kg. So, the energy separation between n=1 and n=2 is, = 2 ! 1 ! ! 8 ! = 3 (!.!"!!" !!" ) ! !!.!"!" !!" !" !! = 3.54 10 !!" J. The average thermal energy is ! ! ! = ! ! 1.38 10 !!" 300 = 2.07 10 !!" J 2.07 10 !!" = ! ! (!.!"!!" !!" ) ! !!.!"!" !!" !" !! , = 4.19 10 ! When we move to very high energy states, quantum effects are no longer observed and classical behavior is recovered. The domain of quantum effects is generally the low temperature (~0 K) region, and at high temperatures statistical effects predominate. Turn in 2. Calculate the probability of finding an electron in the one dimensional box, within L/3 and 2L/3, when its in a) the ground state (n=1) ; and b) 1 st excited state (n=2). What is the difference that you observe, and what can you infer about the shape of the wavefunction at the two different energy levels ? Solution: For the lelctron in a 1D box, the wavefunction is given by = 2 sin

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Homework 12 Solution

1. Problem 2.2 in the book.

Solution: For the particle in a 1D box, 𝐸! =  !!!!

!!!!

1 mole (6.02 x 10-23 molecules) weighs 28g =0.028 kg. So, 1 N2 molecule weighs 0.028/(6.02 x 10-23) = 4.65 x 10-26 kg. So, the energy separation between n=1 and n=2 is,

∆𝐸 = 2! − 1!ℎ!

8𝑚𝐿! = 3   (!.!"!∗!"!!")!

!∗  !.!"∗!"!!"∗!"!!    = 3.54 ∗ 10!!"  J.

The average thermal energy is !

!𝑘!  𝑇 =  

!!  1.38 ∗ 10!!"  300 = 2.07 ∗ 10!!" J

∴ 2.07 ∗ 10!!" =   !

!(!.!"!∗!"!!")!

!∗!.!"∗!"!!"∗!"!!

       𝑜𝑟, 𝑛 = 4.19 ∗ 10! When we move to very high energy states, quantum effects are no longer observed and classical behavior is recovered. The domain of quantum effects is generally the low temperature (~0 K) region, and at high temperatures statistical effects predominate. Turn in 2. Calculate the probability of finding an electron in the one dimensional box, within L/3 and 2L/3, when its in a) the ground state (n=1) ; and b) 1st excited state (n=2). What is the difference that you observe, and what can you infer about the shape of the wavefunction at the two different energy levels ? Solution: For the lelctron in a 1D box, the wavefunction is given by

𝜓 𝑥 =2𝐿 sin

𝑛𝜋𝑥𝐿

So, probability density 𝑃 𝑥 =   𝜓 𝑥 ! =   !

!𝑠𝑖𝑛!(!"#

!)

a) n=1

𝑃𝐿3 →

2𝐿3 =

2𝐿 𝑑𝑥  𝑠𝑖𝑛!(

𝜋𝑥𝐿 )

!!/!

!/!

Now, putting 2𝑠𝑖𝑛!𝑥 = 1− cos(2𝑥) and integrating over the limits, we get

𝑃𝐿3 →

2𝐿3 =

1𝐿𝐿3−

𝐿2𝜋 𝑠𝑖𝑛

2𝜋𝑥𝐿 !

!

!!!

                                                   =  13−

12𝜋 𝑠𝑖𝑛

4𝜋3 − 𝑠𝑖𝑛

2𝜋3

= !

!+ !

!!≈ 0.61 or about 61%

b) n=2

𝑃𝐿3 →

2𝐿3 =

2𝐿 𝑑𝑥  𝑠𝑖𝑛!(

2𝜋𝑥𝐿 )

!!/!

!/!

                                                           =1𝐿𝐿3−

𝐿4𝜋 𝑠𝑖𝑛

4𝜋𝑥𝐿 !

!

!!!

                                                               =  13−

14𝜋 𝑠𝑖𝑛

8𝜋3 − 𝑠𝑖𝑛

4𝜋3

 = !

!− !

!!≈ 0.19 or about 19%

You can see that the probability of finding the electron between L/3 and 2L/3 is higher in the ground state (n=1) than the first excited state n=2. This is a reflection of the corresponding wavefunctions, which has a maximum at L/2 for n=1, and has a node (zero probability) at L/2 for n=2.

                   

3. Problem 2.4 in the book. This shows how ‘electron in a box’ wavefunctions can be applied to calculate energy levels of a conjugated molecule like carotene. We’ll talk about benzene and other such molecules later.

Solution:

a) For 22 C atoms, there are 22 energy levels. The first 11 are occupied, and the last 11 are unoccupied. So, the highest occupied level is n=11, and lowest unoccupied level is n=12. (You know about filling in 2 electrons per energy level due to spin; we’ll discuss this in detail soon in the lectures.)

∴ 𝐸!" − 𝐸!! = 12! − 11!ℎ!

8𝑚𝐿!

                                                                                                       = 23 ∗  (6.626 ∗ 10!!")!

8 ∗ 9.1 ∗ 10!!" ∗ (3.17 ∗ 10!!)!  𝐽

= 1.38 ∗ 10!!"𝐽

b) ∆𝐸 =   !!

!,        𝜆 = !!

∆!= !.!"!∗!!!!"∗!∗!!!

!.!"∗!!!!"= 1.44 ∗ 10!!  𝑚

b) To find the average number of electrons between C11 and C12 , we proceed by taking

the average value of probability density at the center of these C atoms, over ALL the occupied states (remember that occupancy in each state is 2). Probability of finding one electron in this region is given by

𝑃 =  2𝐿 𝑑𝑥  𝑠𝑖𝑛!(𝑛𝜋𝑥/𝐿

!!"

!!!

)  ≈  2𝐿 𝑠𝑖𝑛

! 𝑛𝜋𝑥𝐿  (𝐶!" − 𝐶!!)  

where we assumed the wavefunction to be constant in this small region, and C11 and C12 are the distances between the 12th and 11th carbon atoms.

0.5 1.0 1.5 2.0 2.5 3.0x

0.2

0.4

0.6

0.8

1.0

ψ(x)n = 1

1 2 3 4 5 6x

-1.0

-0.5

0.5

1.0

ψ(x)n = 2

Thus, to find the average number o electrons between C11 and C12 , we sum from n=1 to n=12, with 2 electrons in each energy level (this IS the ground state !).

𝑁 = 2 ∗  2𝐿 ∗ 𝑠𝑖𝑛!

𝑛𝜋(𝐶!! + 𝐶!")/2𝐿 ∗ (𝐶!" − 𝐶!!)

!!

!!!

Now, 𝐿 = 3.17 ∗ 10!!𝑚 (length of the box),

𝐶!! = 10.5 ∗ 144 ∗ 10!!"𝑚, 𝑎𝑛𝑑                𝐶!" = 11.5 ∗ 144 ∗ 10!!"  𝑚 Plugging in the values, we get 𝑁 = 1.09. This is the average number of electrons between 11th and 12th carbon atoms in the ground state. d) The bond order is basically a measure of the number of bonds. You also know that 2 paired electrons nominally make up one bond (we have yet to prove this formally – soon!). So, the number of Pi bonds afforded by 1.09 Pi electrons is, 1.09/2 = 0.545. There is also one Sigma bond already present between the two carbon atoms, that we haven’t dealt with (we were just talking about Pi electrons). Thus, the total bond order between C11 and C12 is 1+0.545 = 1.545.