Lecture 8 - Quantum Theory I

Tuesday, February 6, 2024

7:18 AM

 

 

Class notes can now be found in an alternative location: https://bricejurban.github.io/CHEM111/
I will update this on Tues/Thurs evenings
This is HTML based and compatible with all devices (no more issues!)
Only downside is that hyperlinks do not work.
Assignments due this week:
 ﷟HYPERLINK "https://boisestatecanvas.instructure.com/courses/28699/assignments/990937"HW 4 - Quantum Part 1 (Aktiv Chemistry) (Sun 2/11)
 Finish reading Chapter 4 
 Read Chapter 5
Assignments due next week:
﷟HYPERLINK "https://boisestatecanvas.instructure.com/courses/28699/assignments/990975"HW 5 - Quantum Part 2 (Aktiv Chemistry) (Fri 2/16)
Reading quiz TBD
New Activity TBD
Read Chapter 6, Preview 7
Office Hours: 
Friday 11-1 CIC 
﷟HYPERLINK "https://calendly.com/bricejurban/office-hours"By appointment

Midterm 1:
The first midterm is graded and available for review using the Gradescope software which can be found on Canvas. 
Click through each question's rubric to see how you were graded. 
I recommend printing a copy then reviewing the answer key in the big display case outside SCNC 336 next to the chemistry computer lab. See map for location of answer key.
After reviewing, if you notice any discrepancies you can submit a regrade request through Gradescope.
Statistics:
Mean 73% 
Median 77%
Standard deviation 20%
Top score 106%
Your lowest midterm grade for the semester will be dropped from the gradebook. Midterms amount for 40% of your course grade. If you did not do as well as you would have hoped, you may need to adjust how you study for this class. Here are some ﷟HYPERLINK "https://boisestatecanvas.instructure.com/courses/28698/modules/items/2913696"suggestions.
Today's Schedule:
Tuesday (2/6)
Photoelectric Effect
Wave-Particle Duality of Light and Matter
de Broglie wavelength 
Bohr Model 
Heisenberg Uncertainty Principle

Looking Ahead
Thursday (2/8) Schedule
Quantum Numbers and Orbitals
Electron Configuration
Ground state
Excited State
Transition metals
Atomic Radii

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Equations and Constants to know how to use from last class
Equations and Constants to know how to use from last class
𝜆𝜈=𝑐
wavelength(𝜆)-frequency (𝜈) relation

c = 2.998 × ﷐10﷮8﷯ m∙﷐s﷮−1﷯
speed of light
𝐸=ℎ𝜈  𝑜𝑟 E=﷐hc﷮λ﷯
Planck-Einstein Equation
i.e. Energy of a photon

h = 6.626 × ﷐10﷮−34﷯ J ∙𝑠
Planck constant
Equations to know how to use from today's class
﷐𝐸﷮𝑘﷯=ℎ𝜈−ℎ﷐𝑣﷮0﷯ (when 𝜈> ﷐𝜈﷮0﷯)
﷐𝐸﷮𝑘﷯=ℎ𝜈−𝜑
photoelectric equation
(or in terms of the work function 𝜑)
﷐E﷮k﷯ = ﷐1﷮2﷯m﷐𝓋﷮2﷯
Kinetic energy equation 𝓋 = velocity not frequency
𝜆= ﷐ℎ﷮𝑚𝓋﷯
de Broglie wavelength 
used to find wavelength of electron, particle or anything with mass
﷐𝐸﷮𝑛﷯=﷐−2.1799 𝑎𝐽﷮﷐𝑛﷮2﷯﷯ (𝑛=1, 2, 3…)
Energy levels (n) of hydrogen
﷐𝐸﷮𝑛﷯=−2.1799 𝑎𝐽﷐﷐𝑍﷮2﷯﷮﷐𝑛﷮2﷯﷯ (𝑛=1, 2, 3…)
Energy levels (n) of one-electron ions (Z = atomic number)
﷐𝐸﷮𝑛﷯=2.1799 𝑎𝐽(﷐1﷮﷐﷐𝑛﷮𝑓﷯﷮2﷯﷯−﷐1﷮﷐﷐𝑛﷮𝑖﷯﷮2﷯﷯)
Energy of an emitted photon transitioning from ﷐𝑛﷮𝑖﷯ 𝑡𝑜 ﷐𝑛﷮𝑓﷯
﷐1﷮𝜆﷯=1.097 ×﷐10﷮7﷯ ﷐𝑚﷮−1﷯(﷐1﷮﷐﷐𝑛﷮𝑓﷯﷮2﷯﷯−﷐1﷮﷐﷐𝑛﷮𝑖﷯﷮2﷯﷯)
﷐Wavelength﷮−1﷯ of an emitted photon transitioning from ﷐𝑛﷮𝑖﷯ 𝑡𝑜 ﷐𝑛﷮𝑓﷯
﷐𝐸﷮𝑛﷯=2.1799 𝑎𝐽(﷐1﷮﷐﷐𝑛﷮𝑖﷯﷮2﷯﷯−﷐1﷮﷐﷐𝑛﷮𝑓﷯﷮2﷯﷯)
Energy of an absorbed photon transitioning from ﷐𝑛﷮𝑖﷯ 𝑡𝑜 ﷐𝑛﷮𝑓﷯
(Δ𝑥)(Δ𝑝)≥﷐ℎ﷮4𝜋﷯


𝑝=𝑚∙𝓋 

(Δ𝐸)(Δ𝑡)≥﷐ℎ﷮4𝜋﷯
 Heisenberg uncertainty principle
𝛥𝑥=uncertainty in position
Δ𝑝=uncertainty in momentum

Momentum equation


Energy-time uncertainty principle
1 atomic mass unit
mass of an electron (me)
mass of a proton (mp)
mass of a neutron (mn)
1 atomic mass unit
1.6605 × ﷐10﷮−27﷯ kg
mass of an electron (me)
9.1094 × ﷐10﷮−31﷯ kg
mass of a proton (mp)
1.6726 × ﷐10﷮−27﷯ kg
mass of a neutron (mn)
1.6749 × ﷐10﷮−27﷯ kg

Helpful YouTube Videos from Professor Dave Explains that reviews today's material
﷟HYPERLINK "https://www.youtube.com/watch?v=7BXvc9W97iU&list=PLybg94GvOJ9FAFBqQGf5-4YbfKpWbJtGn&index=2"Quantization of Energy Part 1: Blackbody Radiation and the Ultraviolet Catastrophe
﷟HYPERLINK "https://www.youtube.com/watch?v=eU6VqGIc-2Q&list=PLybg94GvOJ9FAFBqQGf5-4YbfKpWbJtGn&index=3"Quantization of Energy Part 2: Photons, Electrons, and Wave-Particle Duality
﷟HYPERLINK "https://www.youtube.com/watch?v=au2HCVn9IJI&list=PLybg94GvOJ9EbbO2RXPWTUNIIE0C7hSfm&index=13"Bohr Model of the Hydrogen Atom
﷟HYPERLINK "https://www.youtube.com/watch?v=O6g-7rUgrdg&list=PLybg94GvOJ9FAFBqQGf5-4YbfKpWbJtGn&index=5"Quantum Mechanics and the Schrödinger Equation
﷟HYPERLINK "https://www.youtube.com/watch?v=7jY5Q6u65uo&list=PLybg94GvOJ9FAFBqQGf5-4YbfKpWbJtGn&index=6"The Heisenberg Uncertainty Principle Part 1: Position/Momentum and Schrödinger's Cat
﷟HYPERLINK "https://www.youtube.com/watch?v=_DXHrp6-LZI&list=PLybg94GvOJ9FAFBqQGf5-4YbfKpWbJtGn&index=7"The Heisenberg Uncertainty Principle Part 2: Energy/Time and Quantum Fluctuation

Photoelectric Effect
Max Planck solved the Ultraviolet Catastrophe by positing that blackbody radiation is emitted in small discrete packets called quanta
An experiment that helped to provide evidence for this novel idea was the photoelectric effect experiment and Albert Einstein's interpretation of the results.
Imagine a sheet of metal with a detector nearby that can monitor the ejection of electrons. Incident to the metal is a light source that can be changed in intensity or in frequency

﷟HYPERLINK "https://phet.colorado.edu/sims/cheerpj/photoelectric/latest/photoelectric.html?simulation=photoelectric"PhET Simulation (colorado.edu) - Try this experiment yourself!

Untitled picture.png Intenslty 
701 nt-n 
0.000 
current: 
o.oov I 
Untitled picture.png Intenslty 
1 00*é 
701 nt-n 
0.000 
current: 
o.oov I
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701 nt-n 
0.000 
current: 
o.oov I 

Untitled picture.png Intenslty 
1 00*é 
701 nt-n 
0.000 
current: 
o.oov I 

Changing the intensity of red light has no effect on the number of electrons ejected
Untitled picture.png Intenslty 
450 nm 
o .020 
current: 
1.00 v I 


Untitled picture.png Intenslty 
100% 
450 nrn 
0.051 
current: 
1.00 v I 

Going to a lower wavelength (higher frequency) of blue allows for the ejection of some electrons
Increasing intensity of blue light produces a greater current
Untitled picture.png Intenslt,' 
current: 0.340 
Untitled picture.png 262 nn- 
current: 
Intenslty 
o .855
Untitled picture.png Intenslt,' 
current: 0.340 

Untitled picture.png 262 nn- 
current: 
Intenslty 
o .855 

Light in the UV results in much more electrons ejected
Additionally the speed (kinetic energy) of the electrons is much greater
If we plot the electron kinetic energy against light frequency we will observe a linear equation that has a x-intercept that does not pass through zero.
This x-intercept is the minimum threshold frequency ﷐𝑣﷮0﷯ 
The work function (𝝋) is the energy ℎ﷐𝑣﷮0﷯
Only if light was quantized would this be possible!
This can be mathematically represented by this equation:
﷐𝐸﷮𝑘﷯=ℎ𝜈−ℎ﷐𝑣﷮0﷯ ﷐when 𝜈> ﷐𝜈﷮0﷯﷯            or           ﷐𝐸﷮𝑘﷯=ℎ𝜈−𝜑
The threshold frequncy of sodium metal is 5.51×﷐10﷮14﷯ Hz, when multiplied by h, it gives 0.341 aJ which is similar to the first ionization energy (0.85 aJ)
We can then use the kinetic energy equation to find the velocity of the ejected electron:
﷐E﷮k﷯ = ﷐1﷮2﷯m﷐𝓋﷮2﷯



Untitled picture.png @ Electron energyvs light frequency 
0.00 0.75 
1.50 2.25 
Frequency (xl onl 5 Hz) 
3.00 

Concept Check
Given that the threshold frequency of caesium metal is 4.38 × 1014 Hz, calculate the velocity of an electron ejected from the surface of caesium metal when it is irradiated with light of wavelength 400.0 nm. The mass of an electron is 9.109 × 10–31 kg

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Light behaves as both a wave and a particle! But so do other particles
In 1924, Louis de Broglie at age 32, proposed that matter under certain conditions could also exhibit wave-particle duality 
de Broglie put forth his idea as a simple equation: 
𝜆= ﷐ℎ﷮𝑚𝓋﷯
where h is the Planck constant, m is mass in kg, and 𝓋 is the velocity in m/s
An electron is one of the smallest subatomic particles and travels at speeds around the nucleus that approach the speed of light. 
It turns out that treating an electron just as a particle is incorrect.
Evidence for this was first observed by J.J. Thomson's son G. P. Thomson by observing electron diffraction patterns
﷟HYPERLINK "https://www.youtube.com/watch?v=LC6WpitQeSo"Electron Diffraction De Broglie Waves and Nucleus Diameter

Electron Diffraction De Broglie Waves and Nucleus Diameter - AQA A Level Physics Press enter to activate

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Concept Check
Calculate the de Broglie wavelength of a hydrogen molecule (H2) traveling at a speed of 2.0 × 103 m·s–1









  
    The wavelength of the molecule is about the radius of an atom


The energy levels in an atom are the result of the wave properties of the electron
de Broglie's interpretation of the wave properties of matter, gave a plausible explanation for Niels Bohr's circular orbit theory of the atom
Only when the wavelength of an electron matched complete revolutions was an orbit stable. 
The allowed energy states of the hydrogen atom are given by the equation:
﷐𝐸﷮𝑛﷯=﷐−2.1799 𝑎𝐽﷮﷐𝑛﷮2﷯﷯ ﷐𝑛=1, 2, 3…﷯

The integers n =1, 2, 3 . . . are allowed stationary states

n = 1 is the ground state (lowest energy and most stable state)

n = 2 is the first excited state

n = 3 is the second excited state

n = ∞ is when the atom is ionized and the electron is no longer bound



Untitled picture.png 0 
-2.00 
n=6 
n=5 
n=3 
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Untitled picture.png 0 
-2.00 
n=6 
n=5 
n=3 
 Absorption of electromagnetic radiation of only specific energy differences will result in the promotion of an electron to a higher energy level
Atoms can emit or absorb electromagnetic radiation to transition from one stationary state to another
In lab this week you will be using a spectroscope to measure the emission spectra of various elements.
You will also be observing the characteristic flame color of a variety of elements
These spectral lines are the result of the difference in energy levels. For the data analysis you should be familiar with these three equations

﷐𝐸﷮𝑛﷯=2.1799 𝑎𝐽(﷐1﷮﷐﷐𝑛﷮𝑓﷯﷮2﷯﷯−﷐1﷮﷐﷐𝑛﷮𝑖﷯﷮2﷯﷯) 
Energy of photon emitted
﷐1﷮𝜆﷯=1.097 ×﷐10﷮7﷯ ﷐𝑚﷮−1﷯(﷐1﷮﷐﷐𝑛﷮𝑓﷯﷮2﷯﷯−﷐1﷮﷐﷐𝑛﷮𝑖﷯﷮2﷯﷯)
E=﷐hc﷮λ﷯

The visible lines are known as the Balmer series are the transitions to the n = 2 energy level
Untitled picture.png Brackett series 
Paschen series 
Balmer series 
Lyman series 

Concept Check
A line in the Brackett series (En ⟶ E4) of hydrogen has a wavelength of 2626 nm. From what state (ni) did the electron originate? 
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A line in the Brackett series (En ⟶ E4) of hydrogen has a wavelength of 2626 nm. From what state (ni) did the electron originate? 
In what region of the spectrum is this line observed?





































Difference between Emission and Absorption Spectra
Untitled picture.png 400 nm 
Sodium emission spectrum 
Sodium absorption spectrum 
750 nm 
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Untitled picture X-Rays 
Ix 10 12 
1 x 10 14 
Wavelength (in meters) 
4 x 107 
High Energy 
Gamma 
Rays 
1 x 10 
Ultraviolet 
Rays 
Ix108 
5 x 107 
Infrared 
Rays 
Visible Light 
6 x 107 
Radar 
-4 
FM 
I x 102 
TV 
Shortwave AM 
I x 102 
7 x 107 
Low Energy 
I x 104 
Wavelength (in meters) 
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Untitled picture.png 400 nm 
Sodium emission spectrum 
Sodium absorption spectrum 
750 nm 
The Bohr Model is inconsistent with the Uncertainty Principle
Werner Heisenberg showed that is not possible to accurately measure both the position (x) and momentum (p) of a particle simulatenously.
When we try to observe a particle, we must use a photon.
By very act of this observation, we manipulate the particle and this therefore results in some uncertainty in its momentum
This is not a problem with our technique, but rather a fundamental limitation on accuracy.
Heisenberg's discovery led to the quantum revolution a period during the 1920s to 1930s when our understanding of the atom changed dramatically. We will study this starting on Thursday.
Here is Heisenberg's equation and a related one (note the inequality)
(Δ𝑥)(Δ𝑝)≥﷐ℎ﷮4𝜋﷯


𝑝=𝑚∙𝓋 

(Δ𝐸)(Δ𝑡)≥﷐ℎ﷮4𝜋﷯
 Heisenberg uncertainty principle
𝛥𝑥=uncertainty in position
Δ𝑝=uncertainty in momentum

Momentum equation


Energy-time uncertainty principle



Concept Check
What is the uncertainty in the velocity of an electron whose position is known to within 2 × 10–8 meters? 





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If the electron is moving at a speed of 5.0 ×105 m·s–1, what fraction of this speed does the uncertainty represent?









Consider a spectroscopic transition in a molecule that occurs within a very short time frame 1.0 × 10-15 seconds. This transition is due to an electron moving between two energy states in the molecule.

(a) Calculate the minimum uncertainty in the energy (ΔE) of this transition.














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(b) Discuss might this uncertainty affect the results of spectroscopic measurements

        This will result in a broadening of the spectral line.

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