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Example Problems II
Lecture Slides are screen-captured images of important points in the lecture. Students can download and print out these lecture slide images to do practice problems as well as take notes while watching the lecture.
- Intro
- Example I: Find the Term Symbols for the nd² Configuration
- Example II: Find the Term Symbols for the 1s¹2p¹ Configuration
- Example III: Calculate the Separation Between the Doublets in the Lyman Series for Atomic Hydrogen
- Example IV: Calculate the Frequencies of the Lines for the (4d) ²D → (3p) ²P Transition
- Intro 0:00
- Example I: Find the Term Symbols for the nd² Configuration 0:11
- Example II: Find the Term Symbols for the 1s¹2p¹ Configuration 27:02
- Example III: Calculate the Separation Between the Doublets in the Lyman Series for Atomic Hydrogen 41:41
- Example IV: Calculate the Frequencies of the Lines for the (4d) ²D → (3p) ²P Transition 48:53
Physical Chemistry Online Course
Transcription: Example Problems II
Hello and welcome back to www.educator.com, welcome back to Physical Chemistry.0000
Today, we are going to do another set of example problems for the term symbols and for atomic spectra.0004
Let us get started.0011
This next one, find the term symbols for the ND2 configuration.0014
We are doing the same thing that we did before, just more practice.0020
ND2, we know that D orbital has 5 suborbitals.0024
There are 2 spin orbitals for every suborbital, we had a total of 10.0035
ND2 that means 10 and we have 2 electrons, that is going to be 10 choose 2 viable microstates.0041
That is equal to 10!/ 8! is 2!, what you end up with is 90/ 2 = 45.0051
There are 45 microstates, 45 viable microstates.0061
This tends to get very complex very quickly.0066
45 viable microstates but again it is reasonably easy to handle.0071
It is tedious but it is reasonably easy to handle.0077
We have the D which is 12345, m sub l is 2, 1, 0, -1, -2.0080
Remember the quantum numbers represent the locations.0095
The largest ML achievable, we start with the same way.0098
Find the viable microstates and then find the largest ML.0103
The largest ML achievable is ML is equal to 4.0108
1, 2, 3, 4, 5, that is achievable if we put both electrons in the m sub l = 2.0117
Here, because we put them both for the same suborbital, they have to have opposite spin, ½ and -1/2.0125
Here, the largest MS, the largest M sub S is going to equal 0.0137
We have M sub L = 4, M sub S = 0, this implies that L = 4, this implies that S = 0.0147
It implies that 2S + 1 which is the spin multiplicity is equal to 1.0159
The 4 gives us a G term symbol and the 1.0165
We have a singlet G state.0168
The singlet G state, let us go ahead and do our 2L + 1 × 2S + 1.0173
2L + 1 is equal to, L is 4, 2 × 4 is 8, 8 + 1 is 9, 9 × 1.0198
9 × 1, we have 9 microstates that belong to the singlet G state.0204
ML is equal to 4, 3, 2, 1, 0, -1, -2, -3, -4 and MS is equal to 0.0212
We have 4 0, 3 0, 2 0, 1 0, 0 0.0225
That that, that that, that accounts for the 9 microstates.0229
Let us explicitly list what those microstates are.0232
12345, 12345, 12345, 12345, 12345, 12345, 12345, 12345, 12345, there we go.0236
We started off with this and this, let us just run through this entire.0258
This is 4 0, we need to go 3 0, 2 0, 1 0, 0 0, -1 0, -2 0, -3 0, -4 0.0265
We run through them, this is just the beginning.0274
That is there, that is that one, that is that one, that is that one.0278
For example, if I take this one, here the m sub l is 2.0290
Here, the m sub l is -1.0296
2 -1 is 1, up spin downspin is 0.0299
This microstate represents the 1 0 combination.0303
We work our way down this way which is going to be this this, this this, this this, and this this.0312
These are the 10 microstates that have the same energy.0323
The degeneracy of this singlet G is 10.0331
The next largest ML, the next largest M sub L is equal to 3.0340
Mind you, just because I have the next largest ML = 4, the next largest ML = 3, I just do not work my way down.0351
I do, but I still have to be careful because I still might have another state where the ML can be the same.0361
And it is the same if there is another configuration that I can come up with that has not been accounted for.0369
That still gives me that same ML.0375
The next largest ML is equal to 3, achievable as 1, 2, 3, 4, 5.0378
This is achievable as this, 2, 1, 3.0397
This particular microstate has not been accounted for.0406
It was not in the previous 10 that I listed, this is fine.0410
Here, the MS for this is equal to 1 +½ +½.0413
I have an ML equal to 3 and have an MS equal to 1, that implies that L = 3,0420
this implies that S = 1 and implies that 2S + 1 which is the spin multiplicity is equal to 3.0431
L = 3 gives me an F.0439
That was the triplet S state.0442
2L + 1 × 2S + 1, 2 × 3 is 6, 6 + 1 = 7, 2S + 1 that is this, × 3 we have 21 microstates.0446
21 microstates for this level.0463
We have the ML values, ML3 which means 3, 2, 1, 0, -1, -2, -3.0474
MS 1, 0, -1, 3 × 7 = 21.0484
I need to arrange, I need to list 21 microstates that give me0491
all possible combinations 3 1, 2 1, 1 1, 0 1, all the way down 3 0, 2 0, 1 0, all the way down.0496
Here is how it looks.0510
We have 12345, 12345, 12345, 12345, 12345, 12345, 12345, 12345, 12345, 12345, 7.0515
12345, 12345, 12345, 6 7.0537
You see the fact of the matter is one procedure is not necessarily better than another.0558
At some point, you have to list the microstates.0563
I prefer this particular procedure working with the largest ML0565
and with each term symbol that I find will listing the microstates, because I like the list microstates explicitly like this.0568
I do not like that whole 1 + 0 – symbolism, that confuses me after all these years, I still get confused.0577
I’m going to do the next problem like that one because the problem is going to be slightly different.0584
That is a problem that you often see and you probably want to do one of them.0590
Your actual homework assignment but in general I really prefer this particular method.0592
Finding the term symbol based on the largest ML and the largest MS from a basic configuration and0597
then using that basic configuration to generate all the microstates for that particular term symbol.0603
I just think it works out better.0608
It is tedious.0610
12345, 12345, 12345, this is our basic.0614
I think I’m going to go to red here.0627
Let us go up and up, that is that one, that is that one.0633
When we go down up, down up, down up, down up, down up, down up, down up.0649
There is a symmetry when you are listing these microstates, find a pattern, follow that pattern.0663
We have down and down, down and down, down and down, down down, down down, down down, down and down.0670
There we go, those are our 21 microstates here.0684
Let us go back to black.0691
The next largest value of ML is equal to 2 and this is achievable as I can either do a 2 and 0, both up spin.0705
Or I can do a 1 and 1 up spin down spin.0734
This one has been accounted for already.0739
I just need to find one that has not been accounted for as my basis and0744
then use my ML and MS for that one to generate my term symbol.0750
This one has not been accounted for, that is the one that I'm going to use.0755
In this particular case, here MS is equal to 0.0760
I have an ML = 2, I will go ahead and write the MS.0765
MS is equal to 0 and ML = 2 implies the L = 2, implies that S = 0, implies that 2S + 1 is equal to 1.0769
L = 2 gives me the D, the 1.0780
I have a singlet D state.0783
Therefore, my 2L + 1, my degeneracy for this basic term symbol 2S + 1 is equal to 5 × 10786
which is 5 microstates in the singlet D.0796
ML = 2, 1, 0, -1, -2, I hope by now, the basic pattern that I’m doing is what is that0801
we are doing is starting to come together.0810
MS = 0, I'm going to have 12345, 12345, 12345, 12345, 12345.0814
Let us go ahead and go to red.0829
We picked this as our standard, we will go here.0833
The next one is going to go, I will leave 1 and electron here.0837
I will leave an electron here.0841
Notice, in this case my basic is here.0853
I have come over here already, I'm not occupied with the left side anymore and not occupied here.0857
I do not take this over to this, I bring this here.0864
These are the 5 microstates.0873
The individual M sub L is needed to add to these numbers and the individual M sub S need to add to this number.0876
That takes care of that, let us go back to black.0887
The next value of M sub L can take, if you make a mistake in any of this,0897
you will find out because what is going to end up happening is you are going to end up0922
using all your microstates before your term symbols run out.0928
You are going to end up using, you are going to run out of microstates.0933
Where you have too many or not enough, believe me, if you have made a mistake it will show up.0937
It may not show up right away but it will show up eventually.0943
You are going to end up short on either terms symbols or in microstates, that is what is going to happen.0946
Let us see, the next largest value ML can take is ML is equal to 1.0954
And that is achievable 12345, this or,0964
this is achievable as I can put on both up spin like that or I can do up spin down spin like that.0973
This one has already been accounted for.0982
It is already taken care of.0986
This one has not been accounted for, that is the one that I use.0987
Here, MS is equal to 1.0991
I have got ML is equal to 1, I have got MS is equal to 1.0993
That implies that L = 1, that implies that S = 1, that implies that 2S + 1 which is the spin multiplicity = 3.0997
That is going to give me a triplet P state.1012
2L + 1 × 2S + 1 is equal to 3 × 3, I have 9 microstates.1017
ML = 1, 0, -1.1031
MS = 1, 0, -1, 3 × 3 is equal to 9 microstates.1034
I have got 12345, 12345, and 12345, 12345, 12345, 12345, 12345, 12345, 12345.1040
The state that I picked was this and this.1064
I have this this, I have this, I have this.1069
I can go this way, that way, this way, that way, this way, that way.1074
I can go down, this way that way, this way that way, this way this way.1082
M sub L is 1, 1 + 0 is 1.1096
Up spin up spin is 1.1101
1 + 0 is 1 downspin up spin 0.1108
1 + 0 is 1 down spin down spin -1.1114
1 + -1 is 0 up spin up spin 1.1122
1 + 1 m sub l + m sub l.1129
1 + -1 is 0 down spin up spin 0, that is 0 0.1133
0 -1 -1 downspin up spin 0, that is it.1142
That is all that is going on here.1148
Let us see what we have got.1153
We just have taken care of 9 + 21 + 5 + 9 = 44 microstates.1158
We have accounted for 44 of the 45 microstates.1171
There is 1 microstate left.1174
The next largest ML is equal to 0.1181
Achievable as that, this state is not an accounted for.1191
Yes, this is the one that we use.1200
And the MS here is equal to 0.1202
We have ML is equal to 0, we have MS is equal to 0.1205
It implies that L is equal to 0, it implies that S is equal to 0.1209
It implies that 2S + 1 is equal to 1.1215
2L + 1 × 2S + 1 is equal to 1 × 1 = to 1 microstate.1224
It corresponds and this particular microstate, we have ML = 0, we have MS = 0.1231
The only way that this is achievable is that.1239
We have singlet G, triplet F, singlet D, triplet P, singlet S.1247
Our singlet G, L + S = 4 + 0 = 4.1264
The absolute value of L - S = the absolute value of 4 -0 = 4.1273
J is equal to 4.1281
What we have is a singlet G 4 state.1284
Let me go ahead and put degeneracy in there.1293
Once again, the degeneracy of the complete term symbol is equal to 2J + 1.1297
This 2L + 1 × the 2S + 1 that is equal to the degeneracy of the basic term symbol without the J value.1305
The degeneracy of the actual full term symbol is 2J + 1.1313
In this particular case, I will put a parentheses, it is equal to 9.1318
Triplet S state, L + S = 3 + 1 = 4.1336
The absolute value of L - S = absolute value of 3 -1 is equal to 2.1345
Therefore, J = 4, 3, 2.1353
Start here and work your way down there by increments of 1.1357
We have a triplet F 4, we have a triplet F 3, and we have a triplet F 2.1361
The degeneracy are 9, 7, and 5.1370
9 + 7 + 5 is 21.1376
We have a singlet D state.1387
L + S is equal to 2 + 0 is equal to 2.1391
The absolute value of L – S, the absolute value of 2 -0 is equal 2.1395
Therefore, the J is equal to 2 so we have a singlet D2 state degeneracy of 5.1402
And we have our triplet P.1411
Let me go ahead do on the next page here.1418
I have a triplet P, L + S = 1 + 1 is equal 2.1426
The absolute value of L - S = 1 -1 = 0.1444
Therefore, J is equal to 2, 1, 0.1451
I have a triplet P2, I have a triplet P1, and I have a triplet P0 state.1455
The degeneracy are 5, 3, and 1 for total of 9.1462
Remember, the total degeneracy, the basic term symbol.1470
The triplet P was 9, these are individual breakdowns.1472
5 microstates in the triplet P2, 3 microstates in the triplet P1, 1 microstate in the triplet P0 state.1475
Final state here, we have singlet S.1485
L +S is equal to 0 + 0 is equal to 0.1492
The absolute of L - S = absolute 0 -0 = 0.1498
J = 0, we have a singlet S0 and the degeneracy is 1.1503
Ground state, we are looking for the one with the largest S value.1512
The largest S is equal to 3.1523
Let us try this again.1537
We have a singlet G, we had a triplet F, we have a singlet D, we had a triplet P, and we had a singlet S.1545
The largest S is going to be 3.1559
The largest S is equal to 3 that means that triplet F or the triplet P.1563
The next is the largest L value.1574
The largest L between F and the P is the F, the triplet F.1577
Because we are talking about the D2 which is less than half filled, we are going to take the smallest J value.1583
Less than half means the smallest J value.1593
We had a triplet F4, triplet F3, triplet F2.1598
Our triplet F2 is our ground state for that particular electron configuration of the D2.1605
Let us see what is next.1623
Find the term symbols for the NS1 ND1 configuration.1625
I am a little bit of a typo here, this should actually the NP1 configuration not ND1 configuration.1639
NS1 NP1 configuration, this is an excited configuration.1650
You have 1 electron in the S and 1 electron in the P.1655
I d o not want to write this.1670
I do not think I wrote this the way that I actually wanted to write this.1671
Let me do this.1674
I’m going to be real specific about it.1679
Let me go ahead and do it this way.1690
Let me go ahead and rewrite this configuration.1692
Let us do it as NS1 and we will do N prime.1695
This is crazy, I’m going to pick a specific one.1705
The 1S1 and 2P1.1709
We had the 1S2 excited, when the electron has been excited to the P level.1714
The primary quantum numbers do not really matter.1719
Ultimately, what we are concerned with is this S1 P1, that is what really matters.1721
For excited states where electrons are in different suborbital, I think it is best to do a table or write out the configuration explicitly.1727
What I have done here, I have actually done a table.1781
However, like I said I'm not a big fan of tables.1797
If I'm going to do the microstates, I much rather just write them all up explicitly.1803
At least that way I can see what it is that I'm actually dealing with.1808
I’m going to go ahead and do that.1811
I’m going to modify what it is that I have done.1811
I’m going to write out the possible microstates, the 1S1, 2P1.1814
First of all, we are going to do the same thing and find out the number of viable microstates here.1821
First of all, let us see what we are looking at.1828
Let me go ahead and do this in blue.1829
We are looking at this, the S and then some P.1832
Because they are in different orbitals, here you have the 1 and here you have the 2, basically the S and P,1837
because they are in separate, you have to treat them differently.1852
Here you have 1 electron has two different ways of being in this S orbital.1855
1 electron in the P has 6 different ways.1861
Basically, here you have 2 choose 1.1864
We are going to multiply that by the 6 choose 1.1867
It is going to be 2 × 6, we are going to end up with 12 viable microstates.1871
Because the electrons are in different orbitals S and P,1877
I have to take the number of ways of finding the electron in one orbital × the number of ways of finding the P in the other orbital,1883
and I have to multiply those numbers.1890
There are 12 viable microstates.1893
I’m going to go ahead and list out those 12 microstates.1897
Maybe I should just use a table.1902
I’m going to go ahead and use a table here.1904
For excited states where electrons are in different suborbitals, the largest ML,1910
the largest M sub L achievable is if you put one here.1923
Here the ML is, the m sub l is 0, here the m sub l is 1, 0, -1.1935
If I do this, the largest M sub L possible is if an electron goes into this orbital and this orbital, that is going to equal 1.1941
The largest M sub S, if they both have an up spin ½ and ½, it is going to be that.1952
Our table, the ML is going to be 1, 0, -1.1960
The MS is going to be 1, 0, -1.1963
We are going to have 1, 0, -1.1968
We would have 1, 0, -1.1971
This is M sub S, this is M sub L.1978
The different ways of getting an ML value of 1 is 0, 1.1986
This is going to be 0 0, this is going to be 0 -1.1995
A spin of ½ are both going to be + ½.1999
This is going to be both + ½ and both + ½.2002
Here, this is going to be 0 0.2011
It is going to be 1, it is going to be 0 1 and this is going to be + and this is going to be -.2018
I can also do it with 0 - and 1 +.2031
I can have an M sub L value of 0 and 1.2036
0 and 1 add to 1, + and - add to 0.2039
0 and 1 add to 1, - and + add to 0.2042
This is going to be 0 + 0 - or 0 -0 +, these are not the same.2048
These are not the same because we are in different orbitals.2056
Because the electrons are in different orbital.2060
1 is in the S and one is in the P, very different.2062
These are not equivalent orbitals.2066
And this is going to be 0 -1 + -, 0 -1 - +.2069
And over here, I will do -1, this is going to be 0 -1, 0 -1.2077
0 0, 0 1, 0 – 1, this is going to be - -, - -, - -.2093
There we go, these are 9 microstates.2105
Yes, these are all the possible microstates that are available.2111
The largest ML is 1 which means 1, 0, -1 and the largest MS that has a viable microstate is 1.2115
It is going to be 1, 0, -1.2123
ML is going to be 1, 0, -1.2131
MS is 1, 0, -1.2135
For every combination, I will knock one out.2138
1 1 knock one out , 1 0 knock one out, 1 -1 knock one out, 0 1, 0 0, 0 -1, 0 1, 0 0, 0 -1 knock them out.2141
And it does not matter which one I choose.2165
-1 1, -1 0, -1 -1, -1 1, -1 0, -1 -1 knock one out.2168
For this ML = 1 MS = 1 that implies that L = 1, that implies that S = 1.2179
It implies that 2S + 1 = 3.2189
Here, I am looking at the triplet P state, I think.2195
Yes, triplet P and that has 9 microstates.2201
I know that already, 9 microstates.2207
And I do not know that is the 2L + 1.2211
Let me go ahead and stick with the same procedure.2212
2L + 1 × 2S + 1 should be 6 microstates.2217
123456789, 9 microstates.2222
2 L + 1 = 3 × 3 is equal to 9 microstates and here they are.2225
The only difference is this is 0 1 symbolism instead of the actual writing out the specific explicit orbital configuration.2236
The triplet P state, after I have done this, the table I'm left with is going to be the following.2249
I still have the 1, 0, and the -1 and I have the 1, 0, and -1, except all I have left now is 0, 1.2256
This is - this is +, this is 0 0 - +, and this is 0 -1 - +.2271
This is what is left over.2280
Here, the largest M sub L with a viable microstate is again, notice 1.2286
Here the largest M sub L is 1.2293
The largest M sub S is 0.2297
You notice in both cases, I ended up with a largest ML possible of 1.2302
I did not just go down to 0.2308
In this case, we have ML = 1, MS = 0.2311
That implies that L = 1, that implies that S = 0, that implies that 2S + 1 is equal to 1.2319
And this is going to be a single P state.2327
2L + 1 × 2S + 1, that is equal to 3 × 1 = 3 microstates.2335
These are your 3 microstates, we knock them out because ML = 1, 0, -1 and MS is equal to 0.2348
1 0, 0 0, -1 0, we knock them out.2362
We are left with that.2373
Let us go ahead and deal with our triplet P state.2375
Triplet P, L + S is equal to 1 + 1 is equal 2.2378
The absolute value of L - S is equal to 1 -1 is equal to 0.2388
Therefore, J is equal to 2, 1, 0.2394
I have a triplet P2, I have a triplet P1, I have a triplet P0.2398
The degeneracies are 5, 3, and 1.2405
I have a singlet P, it is going to be L + S = 1 + 0 is equal to 1.2416
L – S, absolute value is equal to 1 -0 = 1.2427
Therefore, J is equal to 1.2431
Therefore, I have a singlet P1 state and its degeneracy is equal to 3.2434
Which is the ground state?2444
The largest S between the triplet P and the singlet P, it is going to be the triplet P.2450
And then I have the largest L value, that does not matter because they are all P.2459
Triplet P2, triplet P1, triplet P0 and it is less than half filled.2467
Therefore, we are going to pick the smallest J which means we are going to pick the triplet P0 as the ground state.2479
That really is exhausting.2494
Let us do a little bit some of spectra.2500
Use the table below to calculate the separation between the doublet in the Lyman series for atomic hydrogen go up to N = 4.2503
You remember, our discussion a couple of lessons ago2520
when we are talking about the Lyman series and we are talking about the fine structure.2523
We said that the fine structure consist of doublets.2530
Each of those lines actually split into two because the P level, the 2P, 3P, 4P2536
it consists of a doublet P 3/2 and a doublet P ½.2542
We see them right here.2549
For the 2P, we have a doublet P 3/2 so that is a double line, that is a double line, that is a double line.2551
And where is the 4P, that is the double line and so on.2565
I want to go to N = 4.2575
We are going to do N = 2, N = 3, N = 4.2577
I do not want you to find a separation between the doublets.2580
The separation between those doublet, one of those is going to be a transition from here to here.2583
It is going to be a transition from here to here.2591
The separation between those is just the difference in energy between this and this.2595
The difference in energy between this and this.2601
The difference in energy this and this.2605
This can take a higher number and subtract the lower number, that is all.2607
Let us go ahead and write all this out.2614
Recall the Lyman series is for the NP 1 down to 1S1 transition.2623
The table shows NP1 with 2 states, doublet P 3/2 and a doublet P ½.2651
Again, the problem is to find the separation between the two.2676
We just take the difference between energy is higher - the lower.2678
I will write everything.2687
The problem asks us to find a separation between the lines for NP12692
and doublet P 3/2 down to 1S1 which is a doublet S 1/2 and NP1 doublet P 1/2 down to 1S1 doublet S ½.2726
We need to find the difference in energy.2750
For N = 2, we have 82259.28501 - 82258.9191, the difference in energy is 0.3659 wave numbers.2757
For N =3, we have 97.2795
We are just taking that – that, that is all we are doing.2800
97492.3196 - 97482.2112 the δ E = 0.1084 inverse cm.2805
N = 4, we have 102823.8942 - 102823.8486 δ E = 00.0457 inverse cm.2834
This probably is something that I should have told you a little bit earlier, I will go ahead and tell you now, I apologize.2863
I decided to use energy tables that I got off of the NIST web site.2869
They are the most up to date, as far as I know.2873
Very recent, the spectra and energy values were calculated within the last 45 years, if I'm not mistaken the last time I checked.2876
Your book making a different tables, tables that have different values.2887
The values are very close to these, but again as the years go on, as our techniques improve, our values improve.2892
Do not worry about if you will get 0.0457, if you are using different values from different tables.2899
Perhaps, your book was printed a long time ago.2905
You are going to be using table that have different values.2909
Do not worry about it, go with the values in the table you are given.2911
The table itself is not that important.2915
It is the process that is important.2916
I just wan to you to know that.2918
You do not have to get that same numbers I'm getting, you are probably using older tables.2920
The ones that are in your book, that is not a problem at all.2924
They are very minor differences.2929
Let us go ahead and round this out.2933
Using the table below for atomic sodium, this time it is atomic sodium.2936
Calculate the frequencies in inverse cm, all the lines for the 4D transitions.2939
This time we are going to calculate the frequencies of the spectral lines for the transition from the 4D to 3P level.2951
The 4D has a doublet D and the 3P has doublet P.2961
Let us go ahead and we will see what we have got.2968
The 4D, let us look at 4D here for sodium.2970
For sodium, you are looking at 1S2, 2S2, 2P6, 3S1 configuration.2975
This is the grounds state right here, the 2P6 3S1 configuration.2983
Its term symbol is a doublet S ½.2988
We know that, the S1 configuration is always a doublet S ½.2993
The primary quantum number is irrelevant.2999
We are going up to, we are going from 4D to 3P.3003
First of all, let us find the 3P if we can, it is right here.3007
The 3P configuration, we are going to have those two.3013
Let us look for the 4D configuration.3022
For D, we have that.3024
We have two possible levels in the D.3027
We have a doublet D 5/2 and a doublet P 3/2 and it could go down to a doublet a P 1/2 and doublet a P 3/2.3030
This is the transition is taking place.3039
The doublet D to singlet P represents one line.3042
The fine structure of that line shows this one going to this one.3047
The doublet D 5/2 to the doublet P ½.3053
The doublet P 5/2 to the doublet P 3/2.3058
The doublet P 3/2 to the doublet P ½.3063
The doublet P 3/2 to the doublet P 3/2.3066
There are 4 possible transitions.3068
The fine structure could show up to 4 possible lines.3070
Let us see which one of those lines, which of those transitions is actually allowed and which is not allowed.3073
Let us go ahead and do this one.3082
Our doublet D has doublet D 5/2 and it has a doublet D 3/2.3088
Our doublet P has a doublet P 3/2 and a doublet P ½.3101
There are 4 possible transitions.3110
Here to here, here to here, here to here, and here to here.3119
We have the doublet D 5/2 down to the doublet P 3/2.3126
I have got the doublet D 5/2 down to the doublet P ½.3137
I have got the doublet D 3/2 down to the doublet P 3/2.3147
Let me go ahead and put the other one right here.3158
I have got the doublet D 3/2 down to the doublet P ½.3161
Let us calculate some values here.3166
Here our δ L, for this one right here, our δ L = -1 DP.3169
Our δ S, doublet and doublet = 0.3179
Our δ J, 5/2 to 3/2 = -1.3182
This one is allowed.3187
Here we have a δ L = -1, we have a δ S = 0, we have δ J 5/2 to ½, it is -2.3190
This is not allowed.3199
Here we have δ L is equal to -1, δ S = 0 and we have δ J is equal to 0.3202
Yes, this one is allowed.3212
Here we have δ L = D to P-1, δ S = 0, and δ J = 0.3213
This one is allowed.3222
The 4 possibilities that is allowed, that is allowed, and that is allowed.3224
This transition is not allowed.3231
We are going to see 3 lines in the fine structure of this particular transition.3233
The rest is just working out the numbers.3239
I'm going to go ahead and do the doublet D 5/2 down to the doublet P 3/2.3243
That is going to be 34548.729 - 16973.366 = 17575.363 inverse cm.3254
That is where I’m going to see one of my lines.3276
The doublet P 3/2 down to the doublet P 3/2, we are going to have 34548.764 - 16973.366 = 17575.398 inverse cm.3281
That is going to be the second of the 3 lines.3318
Of course, the last one is doublet D 3/2 down to a doublet P ½.3323
That is going to be 34548.764 - 16956.170.3332
I think I hate most about quantum mechanics is the computational part.3344
The theoretical part in quantum mechanics is great, all the symbols not these tedious calculation.3348
But it is a necessity.3354
= 17592.594 inverse cm, this is that line.3357
The fine structure of this particular transition will show 3 unevenly spaced lines, the differences between these numbers.3369
This and this, and this and this, it is not even.3378
You will get something that looks like that, the separation.3383
That is it, there we go.3388
Thank you so much for joining us here at www.educator.com.3391
We will see you next time.3393

Raffi Hovasapian
Example Problems II
Slide Duration:Table of Contents
46m 5s
- Intro0:00
- Course Overview0:16
- Thermodynamics & Classical Thermodynamics0:17
- Structure of the Course1:30
- The Ideal Gas Law3:06
- Ideal Gas Law: PV=nRT3:07
- Units of Pressure4:51
- Manipulating Units5:52
- Atmosphere : atm8:15
- Millimeter of Mercury: mm Hg8:48
- SI Unit of Volume9:32
- SI Unit of Temperature10:32
- Value of R (Gas Constant): Pv = nRT10:51
- Extensive and Intensive Variables (Properties)15:23
- Intensive Property15:52
- Extensive Property16:30
- Example: Extensive and Intensive Variables18:20
- Ideal Gas Law19:24
- Ideal Gas Law with Intensive Variables19:25
- Graphing Equations23:51
- Hold T Constant & Graph P vs. V23:52
- Hold P Constant & Graph V vs. T31:08
- Hold V Constant & Graph P vs. T34:38
- Isochores or Isometrics37:08
- More on the V vs. T Graph39:46
- More on the P vs. V Graph42:06
- Ideal Gas Law at Low Pressure & High Temperature44:26
- Ideal Gas Law at High Pressure & Low Temperature45:16
46m 2s
- Intro0:00
- Math Lesson 1: Partial Differentiation0:38
- Overview0:39
- Example I3:00
- Example II6:33
- Example III9:52
- Example IV17:26
- Differential & Derivative21:44
- What Does It Mean?21:45
- Total Differential (or Total Derivative)30:16
- Net Change in Pressure (P)33:58
- General Equation for Total Differential38:12
- Example 5: Total Differential39:28
1h 6m 45s
- Intro0:00
- Properties of Thermodynamic State1:38
- Big Picture: 3 Properties of Thermodynamic State1:39
- Enthalpy & Free Energy3:30
- Associated Law4:40
- Energy & the First Law of Thermodynamics7:13
- System & Its Surrounding Separated by a Boundary7:14
- In Other Cases the Boundary is Less Clear10:47
- State of a System12:37
- State of a System12:38
- Change in State14:00
- Path for a Change in State14:57
- Example: State of a System15:46
- Open, Close, and Isolated System18:26
- Open System18:27
- Closed System19:02
- Isolated System19:22
- Important Questions20:38
- Important Questions20:39
- Work & Heat22:50
- Definition of Work23:33
- Properties of Work25:34
- Definition of Heat32:16
- Properties of Heat34:49
- Experiment #142:23
- Experiment #247:00
- More on Work & Heat54:50
- More on Work & Heat54:51
- Conventions for Heat & Work1:00:50
- Convention for Heat1:02:40
- Convention for Work1:04:24
- Schematic Representation1:05:00
1h 6m 33s
- Intro0:00
- The First Law of Thermodynamics0:53
- The First Law of Thermodynamics0:54
- Example 1: What is the Change in Energy of the System & Surroundings?8:53
- Energy and The First Law II, cont.11:55
- The Energy of a System Changes in Two Ways11:56
- Systems Possess Energy, Not Heat or Work12:45
- Scenario 116:00
- Scenario 216:46
- State Property, Path Properties, and Path Functions18:10
- Pressure-Volume Work22:36
- When a System Changes22:37
- Gas Expands24:06
- Gas is Compressed25:13
- Pressure Volume Diagram: Analyzing Expansion27:17
- What if We do the Same Expansion in Two Stages?35:22
- Multistage Expansion43:58
- General Expression for the Pressure-Volume Work46:59
- Upper Limit of Isothermal Expansion50:00
- Expression for the Work Done in an Isothermal Expansion52:45
- Example 2: Find an Expression for the Maximum Work Done by an Ideal Gas upon Isothermal Expansion56:18
- Example 3: Calculate the External Pressure and Work Done58:50
1h 2m 17s
- Intro0:00
- Compression0:20
- Compression Overview0:34
- Single-stage compression vs. 2-stage Compression2:16
- Multi-stage Compression8:40
- Example I: Compression14:47
- Example 1: Single-stage Compression14:47
- Example 1: 2-stage Compression20:07
- Example 1: Absolute Minimum26:37
- More on Compression32:55
- Isothermal Expansion & Compression32:56
- External & Internal Pressure of the System35:18
- Reversible & Irreversible Processes37:32
- Process 1: Overview38:57
- Process 2: Overview39:36
- Process 1: Analysis40:42
- Process 2: Analysis45:29
- Reversible Process50:03
- Isothermal Expansion and Compression54:31
- Example II: Reversible Isothermal Compression of a Van der Waals Gas58:10
- Example 2: Reversible Isothermal Compression of a Van der Waals Gas58:11
1h 4m 39s
- Intro0:00
- Recall0:37
- State Function & Path Function0:38
- First Law2:11
- Exact & Inexact Differential2:12
- Where Does (∆U = Q - W) or dU = dQ - dU Come from?8:54
- Cyclic Integrals of Path and State Functions8:55
- Our Empirical Experience of the First Law12:31
- ∆U = Q - W18:42
- Relations between Changes in Properties and Energy22:24
- Relations between Changes in Properties and Energy22:25
- Rate of Change of Energy per Unit Change in Temperature29:54
- Rate of Change of Energy per Unit Change in Volume at Constant Temperature32:39
- Total Differential Equation34:38
- Constant Volume41:08
- If Volume Remains Constant, then dV = 041:09
- Constant Volume Heat Capacity45:22
- Constant Volume Integrated48:14
- Increase & Decrease in Energy of the System54:19
- Example 1: ∆U and Qv57:43
- Important Equations1:02:06
16m 50s
- Intro0:00
- Joule's Experiment0:09
- Joule's Experiment1:20
- Interpretation of the Result4:42
- The Gas Expands Against No External Pressure4:43
- Temperature of the Surrounding Does Not Change6:20
- System & Surrounding7:04
- Joule's Law10:44
- More on Joule's Experiment11:08
- Later Experiment12:38
- Dealing with the 2nd Law & Its Mathematical Consequences13:52
43m 40s
- Intro0:00
- Changes in Energy & State: Constant Pressure0:20
- Integrating with Constant Pressure0:35
- Defining the New State Function6:24
- Heat & Enthalpy of the System at Constant Pressure8:54
- Finding ∆U12:10
- dH15:28
- Constant Pressure Heat Capacity18:08
- Important Equations25:44
- Important Equations25:45
- Important Equations at Constant Pressure27:32
- Example I: Change in Enthalpy (∆H)28:53
- Example II: Change in Internal Energy (∆U)34:19
32m 23s
- Intro0:00
- The Relationship Between Cp & Cv0:21
- For a Constant Volume Process No Work is Done0:22
- For a Constant Pressure Process ∆V ≠ 0, so Work is Done1:16
- The Relationship Between Cp & Cv: For an Ideal Gas3:26
- The Relationship Between Cp & Cv: In Terms of Molar heat Capacities5:44
- Heat Capacity Can Have an Infinite # of Values7:14
- The Relationship Between Cp & Cv11:20
- When Cp is Greater than Cv17:13
- 2nd Term18:10
- 1st Term19:20
- Constant P Process: 3 Parts22:36
- Part 123:45
- Part 224:10
- Part 324:46
- Define : γ = (Cp/Cv)28:06
- For Gases28:36
- For Liquids29:04
- For an Ideal Gas30:46
39m 15s
- Intro0:00
- General Equations0:13
- Recall0:14
- How Does Enthalpy of a System Change Upon a Unit Change in Pressure?2:58
- For Liquids & Solids12:11
- For Ideal Gases14:08
- For Real Gases16:58
- The Joule Thompson Experiment18:37
- The Joule Thompson Experiment Setup18:38
- The Flow in 2 Stages22:54
- Work Equation for the Joule Thompson Experiment24:14
- Insulated Pipe26:33
- Joule-Thompson Coefficient29:50
- Changing Temperature & Pressure in Such a Way that Enthalpy Remains Constant31:44
- Joule Thompson Inversion Temperature36:26
- Positive & Negative Joule-Thompson Coefficient36:27
- Joule Thompson Inversion Temperature37:22
- Inversion Temperature of Hydrogen Gas37:59
35m 52s
- Intro0:00
- Adiabatic Changes of State0:10
- Adiabatic Changes of State0:18
- Work & Energy in an Adiabatic Process3:44
- Pressure-Volume Work7:43
- Adiabatic Changes for an Ideal Gas9:23
- Adiabatic Changes for an Ideal Gas9:24
- Equation for a Fixed Change in Volume11:20
- Maximum & Minimum Values of Temperature14:20
- Adiabatic Path18:08
- Adiabatic Path Diagram18:09
- Reversible Adiabatic Expansion21:54
- Reversible Adiabatic Compression22:34
- Fundamental Relationship Equation for an Ideal Gas Under Adiabatic Expansion25:00
- More on the Equation28:20
- Important Equations32:16
- Important Adiabatic Equation32:17
- Reversible Adiabatic Change of State Equation33:02
42m 40s
- Intro0:00
- Fundamental Equations0:56
- Work2:40
- Energy (1st Law)3:10
- Definition of Enthalpy3:44
- Heat capacity Definitions4:06
- The Mathematics6:35
- Fundamental Concepts8:13
- Isothermal8:20
- Adiabatic8:54
- Isobaric9:25
- Isometric9:48
- Ideal Gases10:14
- Example I12:08
- Example I: Conventions12:44
- Example I: Part A15:30
- Example I: Part B18:24
- Example I: Part C19:53
- Example II: What is the Heat Capacity of the System?21:49
- Example III: Find Q, W, ∆U & ∆H for this Change of State24:15
- Example IV: Find Q, W, ∆U & ∆H31:37
- Example V: Find Q, W, ∆U & ∆H38:20
1h 23s
- Intro0:00
- Example I0:11
- Example I: Finding ∆U1:49
- Example I: Finding W6:22
- Example I: Finding Q11:23
- Example I: Finding ∆H16:09
- Example I: Summary17:07
- Example II21:16
- Example II: Finding W22:42
- Example II: Finding ∆H27:48
- Example II: Finding Q30:58
- Example II: Finding ∆U31:30
- Example III33:33
- Example III: Finding ∆U, Q & W33:34
- Example III: Finding ∆H38:07
- Example IV41:50
- Example IV: Finding ∆U41:51
- Example IV: Finding ∆H45:42
- Example V49:31
- Example V: Finding W49:32
- Example V: Finding ∆U55:26
- Example V: Finding Q56:26
- Example V: Finding ∆H56:55
44m 34s
- Intro0:00
- Example I0:15
- Example I: Finding the Final Temperature3:40
- Example I: Finding Q8:04
- Example I: Finding ∆U8:25
- Example I: Finding W9:08
- Example I: Finding ∆H9:51
- Example II11:27
- Example II: Finding the Final Temperature11:28
- Example II: Finding ∆U21:25
- Example II: Finding W & Q22:14
- Example II: Finding ∆H23:03
- Example III24:38
- Example III: Finding the Final Temperature24:39
- Example III: Finding W, ∆U, and Q27:43
- Example III: Finding ∆H28:04
- Example IV29:23
- Example IV: Finding ∆U, W, and Q25:36
- Example IV: Finding ∆H31:33
- Example V32:24
- Example V: Finding the Final Temperature33:32
- Example V: Finding ∆U39:31
- Example V: Finding W40:17
- Example V: First Way of Finding ∆H41:10
- Example V: Second Way of Finding ∆H42:10
59m 7s
- Intro0:00
- Example I: Find ∆H° for the Following Reaction0:42
- Example II: Calculate the ∆U° for the Reaction in Example I5:33
- Example III: Calculate the Heat of Formation of NH₃ at 298 K14:23
- Example IV32:15
- Part A: Calculate the Heat of Vaporization of Water at 25°C33:49
- Part B: Calculate the Work Done in Vaporizing 2 Mols of Water at 25°C Under a Constant Pressure of 1 atm35:26
- Part C: Find ∆U for the Vaporization of Water at 25°C41:00
- Part D: Find the Enthalpy of Vaporization of Water at 100°C43:12
- Example V49:24
- Part A: Constant Temperature & Increasing Pressure50:25
- Part B: Increasing temperature & Constant Pressure56:20
49m 16s
- Intro0:00
- Entropy, Part 10:16
- Coefficient of Thermal Expansion (Isobaric)0:38
- Coefficient of Compressibility (Isothermal)1:25
- Relative Increase & Relative Decrease2:16
- More on α4:40
- More on κ8:38
- Entropy, Part 211:04
- Definition of Entropy12:54
- Differential Change in Entropy & the Reversible Path20:08
- State Property of the System28:26
- Entropy Changes Under Isothermal Conditions35:00
- Recall: Heating Curve41:05
- Some Phase Changes Take Place Under Constant Pressure44:07
- Example I: Finding ∆S for a Phase Change46:05
33m 59s
- Intro0:00
- Math Lesson II0:46
- Let F(x,y) = x²y³0:47
- Total Differential3:34
- Total Differential Expression6:06
- Example 19:24
- More on Math Expression13:26
- Exact Total Differential Expression13:27
- Exact Differentials19:50
- Inexact Differentials20:20
- The Cyclic Rule21:06
- The Cyclic Rule21:07
- Example 227:58
54m 37s
- Intro0:00
- Entropy As a Function of Temperature & Volume0:14
- Fundamental Equation of Thermodynamics1:16
- Things to Notice9:10
- Entropy As a Function of Temperature & Volume14:47
- Temperature-dependence of Entropy24:00
- Example I26:19
- Entropy As a Function of Temperature & Volume, Cont.31:55
- Volume-dependence of Entropy at Constant Temperature31:56
- Differentiate with Respect to Temperature, Holding Volume Constant36:16
- Recall the Cyclic Rule45:15
- Summary & Recap46:47
- Fundamental Equation of Thermodynamics46:48
- For Entropy as a Function of Temperature & Volume47:18
- The Volume-dependence of Entropy for Liquids & Solids52:52
31m 18s
- Intro0:00
- Entropy as a Function of Temperature & Pressure0:17
- Entropy as a Function of Temperature & Pressure0:18
- Rewrite the Total Differential5:54
- Temperature-dependence7:08
- Pressure-dependence9:04
- Differentiate with Respect to Pressure & Holding Temperature Constant9:54
- Differentiate with Respect to Temperature & Holding Pressure Constant11:28
- Pressure-Dependence of Entropy for Liquids & Solids18:45
- Pressure-Dependence of Entropy for Liquids & Solids18:46
- Example I: ∆S of Transformation26:20
23m 6s
- Intro0:00
- Summary of Entropy So Far0:43
- Defining dS1:04
- Fundamental Equation of Thermodynamics3:51
- Temperature & Volume6:04
- Temperature & Pressure9:10
- Two Important Equations for How Entropy Behaves13:38
- State of a System & Heat Capacity15:34
- Temperature-dependence of Entropy19:49
25m 42s
- Intro0:00
- Entropy Changes for an Ideal Gas1:10
- General Equation1:22
- The Fundamental Theorem of Thermodynamics2:37
- Recall the Basic Total Differential Expression for S = S (T,V)5:36
- For a Finite Change in State7:58
- If Cv is Constant Over the Particular Temperature Range9:05
- Change in Entropy of an Ideal Gas as a Function of Temperature & Pressure11:35
- Change in Entropy of an Ideal Gas as a Function of Temperature & Pressure11:36
- Recall the Basic Total Differential expression for S = S (T, P)15:13
- For a Finite Change18:06
- Example 1: Calculate the ∆S of Transformation22:02
43m 39s
- Intro0:00
- Entropy Example Problems I0:24
- Fundamental Equation of Thermodynamics1:10
- Entropy as a Function of Temperature & Volume2:04
- Entropy as a Function of Temperature & Pressure2:59
- Entropy For Phase Changes4:47
- Entropy For an Ideal Gas6:14
- Third Law Entropies8:25
- Statement of the Third Law9:17
- Entropy of the Liquid State of a Substance Above Its Melting Point10:23
- Entropy For the Gas Above Its Boiling Temperature13:02
- Entropy Changes in Chemical Reactions15:26
- Entropy Change at a Temperature Other than 25°C16:32
- Example I19:31
- Part A: Calculate ∆S for the Transformation Under Constant Volume20:34
- Part B: Calculate ∆S for the Transformation Under Constant Pressure25:04
- Example II: Calculate ∆S fir the Transformation Under Isobaric Conditions27:53
- Example III30:14
- Part A: Calculate ∆S if 1 Mol of Aluminum is taken from 25°C to 255°C31:14
- Part B: If S°₂₉₈ = 28.4 J/mol-K, Calculate S° for Aluminum at 498 K33:23
- Example IV: Calculate Entropy Change of Vaporization for CCl₄34:19
- Example V35:41
- Part A: Calculate ∆S of Transformation37:36
- Part B: Calculate ∆S of Transformation39:10
56m 44s
- Intro0:00
- Example I0:09
- Example I: Calculate ∆U1:28
- Example I: Calculate Q3:29
- Example I: Calculate Cp4:54
- Example I: Calculate ∆S6:14
- Example II7:13
- Example II: Calculate W8:14
- Example II: Calculate ∆U8:56
- Example II: Calculate Q10:18
- Example II: Calculate ∆H11:00
- Example II: Calculate ∆S12:36
- Example III18:47
- Example III: Calculate ∆H19:38
- Example III: Calculate Q21:14
- Example III: Calculate ∆U21:44
- Example III: Calculate W23:59
- Example III: Calculate ∆S24:55
- Example IV27:57
- Example IV: Diagram29:32
- Example IV: Calculate W32:27
- Example IV: Calculate ∆U36:36
- Example IV: Calculate Q38:32
- Example IV: Calculate ∆H39:00
- Example IV: Calculate ∆S40:27
- Example IV: Summary43:41
- Example V48:25
- Example V: Diagram49:05
- Example V: Calculate W50:58
- Example V: Calculate ∆U53:29
- Example V: Calculate Q53:44
- Example V: Calculate ∆H54:34
- Example V: Calculate ∆S55:01
57m 6s
- Intro0:00
- Example I: Isothermal Expansion0:09
- Example I: Calculate W1:19
- Example I: Calculate ∆U1:48
- Example I: Calculate Q2:06
- Example I: Calculate ∆H2:26
- Example I: Calculate ∆S3:02
- Example II: Adiabatic and Reversible Expansion6:10
- Example II: Calculate Q6:48
- Example II: Basic Equation for the Reversible Adiabatic Expansion of an Ideal Gas8:12
- Example II: Finding Volume12:40
- Example II: Finding Temperature17:58
- Example II: Calculate ∆U19:53
- Example II: Calculate W20:59
- Example II: Calculate ∆H21:42
- Example II: Calculate ∆S23:42
- Example III: Calculate the Entropy of Water Vapor25:20
- Example IV: Calculate the Molar ∆S for the Transformation34:32
- Example V44:19
- Part A: Calculate the Standard Entropy of Liquid Lead at 525°C46:17
- Part B: Calculate ∆H for the Transformation of Solid Lead from 25°C to Liquid Lead at 525°C52:23
54m 35s
- Intro0:00
- Entropy & Probability0:11
- Structural Model3:05
- Recall the Fundamental Equation of Thermodynamics9:11
- Two Independent Ways of Affecting the Entropy of a System10:05
- Boltzmann Definition12:10
- Omega16:24
- Definition of Omega16:25
- Energy Distribution19:43
- The Energy Distribution19:44
- In How Many Ways can N Particles be Distributed According to the Energy Distribution23:05
- Example I: In How Many Ways can the Following Distribution be Achieved32:51
- Example II: In How Many Ways can the Following Distribution be Achieved33:51
- Example III: In How Many Ways can the Following Distribution be Achieved34:45
- Example IV: In How Many Ways can the Following Distribution be Achieved38:50
- Entropy & Probability, cont.40:57
- More on Distribution40:58
- Example I Summary41:43
- Example II Summary42:12
- Distribution that Maximizes Omega42:26
- If Omega is Large, then S is Large44:22
- Two Constraints for a System to Achieve the Highest Entropy Possible47:07
- What Happened When the Energy of a System is Increased?49:00
35m 5s
- Intro0:00
- Volume Distribution0:08
- Distributing 2 Balls in 3 Spaces1:43
- Distributing 2 Balls in 4 Spaces3:44
- Distributing 3 Balls in 10 Spaces5:30
- Number of Ways to Distribute P Particles over N Spaces6:05
- When N is Much Larger than the Number of Particles P7:56
- Energy Distribution25:04
- Volume Distribution25:58
- Entropy, Total Entropy, & Total Omega Equations27:34
- Entropy, Total Entropy, & Total Omega Equations27:35
28m 42s
- Intro0:00
- Reversible & Irreversible0:24
- Reversible vs. Irreversible0:58
- Defining Equation for Equilibrium2:11
- Defining Equation for Irreversibility (Spontaneity)3:11
- TdS ≥ dQ5:15
- Transformation in an Isolated System11:22
- Transformation in an Isolated System11:29
- Transformation at Constant Temperature14:50
- Transformation at Constant Temperature14:51
- Helmholtz Free Energy17:26
- Define: A = U - TS17:27
- Spontaneous Isothermal Process & Helmholtz Energy20:20
- Pressure-volume Work22:02
34m 38s
- Intro0:00
- Transformation under Constant Temperature & Pressure0:08
- Transformation under Constant Temperature & Pressure0:36
- Define: G = U + PV - TS3:32
- Gibbs Energy5:14
- What Does This Say?6:44
- Spontaneous Process & a Decrease in G14:12
- Computing ∆G18:54
- Summary of Conditions21:32
- Constraint & Condition for Spontaneity21:36
- Constraint & Condition for Equilibrium24:54
- A Few Words About the Word Spontaneous26:24
- Spontaneous Does Not Mean Fast26:25
- Putting Hydrogen & Oxygen Together in a Flask26:59
- Spontaneous Vs. Not Spontaneous28:14
- Thermodynamically Favorable29:03
- Example: Making a Process Thermodynamically Favorable29:34
- Driving Forces for Spontaneity31:35
- Equation: ∆G = ∆H - T∆S31:36
- Always Spontaneous Process32:39
- Never Spontaneous Process33:06
- A Process That is Endothermic Can Still be Spontaneous34:00
30m 50s
- Intro0:00
- The Fundamental Equations of Thermodynamics0:44
- Mechanical Properties of a System0:45
- Fundamental Properties of a System1:16
- Composite Properties of a System1:44
- General Condition of Equilibrium3:16
- Composite Functions & Their Differentiations6:11
- dH = TdS + VdP7:53
- dA = -SdT - PdV9:26
- dG = -SdT + VdP10:22
- Summary of Equations12:10
- Equation #114:33
- Equation #215:15
- Equation #315:58
- Equation #416:42
- Maxwell's Relations20:20
- Maxwell's Relations20:21
- Isothermal Volume-Dependence of Entropy & Isothermal Pressure-Dependence of Entropy26:21
34m 6s
- Intro0:00
- The General Thermodynamic Equations of State0:10
- Equations of State for Liquids & Solids0:52
- More General Condition for Equilibrium4:02
- General Conditions: Equation that Relates P to Functions of T & V6:20
- The Second Fundamental Equation of Thermodynamics11:10
- Equation 117:34
- Equation 221:58
- Recall the General Expression for Cp - Cv28:11
- For the Joule-Thomson Coefficient30:44
- Joule-Thomson Inversion Temperature32:12
39m 18s
- Intro0:00
- Properties of the Helmholtz & Gibbs Energies0:10
- Equating the Differential Coefficients1:34
- An Increase in T; a Decrease in A3:25
- An Increase in V; a Decrease in A6:04
- We Do the Same Thing for G8:33
- Increase in T; Decrease in G10:50
- Increase in P; Decrease in G11:36
- Gibbs Energy of a Pure Substance at a Constant Temperature from 1 atm to any Other Pressure.14:12
- If the Substance is a Liquid or a Solid, then Volume can be Treated as a Constant18:57
- For an Ideal Gas22:18
- Special Note24:56
- Temperature Dependence of Gibbs Energy27:02
- Temperature Dependence of Gibbs Energy #127:52
- Temperature Dependence of Gibbs Energy #229:01
- Temperature Dependence of Gibbs Energy #329:50
- Temperature Dependence of Gibbs Energy #434:50
19m 40s
- Intro0:00
- Entropy of the Universe & the Surroundings0:08
- Equation: ∆G = ∆H - T∆S0:20
- Conditions of Constant Temperature & Pressure1:14
- Reversible Process3:14
- Spontaneous Process & the Entropy of the Universe5:20
- Tips for Remembering Everything12:40
- Verify Using Known Spontaneous Process14:51
54m 16s
- Intro0:00
- Example I0:11
- Example I: Deriving a Function for Entropy (S)2:06
- Example I: Deriving a Function for V5:55
- Example I: Deriving a Function for H8:06
- Example I: Deriving a Function for U12:06
- Example II15:18
- Example III21:52
- Example IV26:12
- Example IV: Part A26:55
- Example IV: Part B28:30
- Example IV: Part C30:25
- Example V33:45
- Example VI40:46
- Example VII43:43
- Example VII: Part A44:46
- Example VII: Part B50:52
- Example VII: Part C51:56
31m 17s
- Intro0:00
- Example I0:09
- Example II5:18
- Example III8:22
- Example IV12:32
- Example V17:14
- Example VI20:34
- Example VI: Part A21:04
- Example VI: Part B23:56
- Example VI: Part C27:56
45m
- Intro0:00
- Example I0:10
- Example II15:03
- Example III21:47
- Example IV28:37
- Example IV: Part A29:33
- Example IV: Part B36:09
- Example IV: Part C40:34
58m 5s
- Intro0:00
- Example I0:41
- Part A: Calculating ∆H3:55
- Part B: Calculating ∆S15:13
- Example II24:39
- Part A: Final Temperature of the System26:25
- Part B: Calculating ∆S36:57
- Example III46:49
25m 20s
- Intro0:00
- Work, Heat, and Energy0:18
- Definition of Work, Energy, Enthalpy, and Heat Capacities0:23
- Heat Capacities for an Ideal Gas3:40
- Path Property & State Property3:56
- Energy Differential5:04
- Enthalpy Differential5:40
- Joule's Law & Joule-Thomson Coefficient6:23
- Coefficient of Thermal Expansion & Coefficient of Compressibility7:01
- Enthalpy of a Substance at Any Other Temperature7:29
- Enthalpy of a Reaction at Any Other Temperature8:01
- Entropy8:53
- Definition of Entropy8:54
- Clausius Inequality9:11
- Entropy Changes in Isothermal Systems9:44
- The Fundamental Equation of Thermodynamics10:12
- Expressing Entropy Changes in Terms of Properties of the System10:42
- Entropy Changes in the Ideal Gas11:22
- Third Law Entropies11:38
- Entropy Changes in Chemical Reactions14:02
- Statistical Definition of Entropy14:34
- Omega for the Spatial & Energy Distribution14:47
- Spontaneity and Equilibrium15:43
- Helmholtz Energy & Gibbs Energy15:44
- Condition for Spontaneity & Equilibrium16:24
- Condition for Spontaneity with Respect to Entropy17:58
- The Fundamental Equations18:30
- Maxwell's Relations19:04
- The Thermodynamic Equations of State20:07
- Energy & Enthalpy Differentials21:08
- Joule's Law & Joule-Thomson Coefficient21:59
- Relationship Between Constant Pressure & Constant Volume Heat Capacities23:14
- One Final Equation - Just for Fun24:04
34m 25s
- Intro0:00
- Complex Numbers0:11
- Representing Complex Numbers in the 2-Dimmensional Plane0:56
- Addition of Complex Numbers2:35
- Subtraction of Complex Numbers3:17
- Multiplication of Complex Numbers3:47
- Division of Complex Numbers6:04
- r & θ8:04
- Euler's Formula11:00
- Polar Exponential Representation of the Complex Numbers11:22
- Example I14:25
- Example II15:21
- Example III16:58
- Example IV18:35
- Example V20:40
- Example VI21:32
- Example VII25:22
59m 57s
- Intro0:00
- Probability & Statistics1:51
- Normalization Condition1:52
- Define the Mean or Average of x11:04
- Example I: Calculate the Mean of x14:57
- Example II: Calculate the Second Moment of the Data in Example I22:39
- Define the Second Central Moment or Variance25:26
- Define the Second Central Moment or Variance25:27
- 1st Term32:16
- 2nd Term32:40
- 3rd Term34:07
- Continuous Distributions35:47
- Continuous Distributions35:48
- Probability Density39:30
- Probability Density39:31
- Normalization Condition46:51
- Example III50:13
- Part A - Show that P(x) is Normalized51:40
- Part B - Calculate the Average Position of the Particle Along the Interval54:31
- Important Things to Remember58:24
42m 5s
- Intro0:00
- Schrӧdinger Equation & Operators0:16
- Relation Between a Photon's Momentum & Its Wavelength0:17
- Louis de Broglie: Wavelength for Matter0:39
- Schrӧdinger Equation1:19
- Definition of Ψ(x)3:31
- Quantum Mechanics5:02
- Operators7:51
- Example I10:10
- Example II11:53
- Example III14:24
- Example IV17:35
- Example V19:59
- Example VI22:39
- Operators Can Be Linear or Non Linear27:58
- Operators Can Be Linear or Non Linear28:34
- Example VII32:47
- Example VIII36:55
- Example IX39:29
30m 26s
- Intro0:00
- Schrӧdinger Equation as an Eigenvalue Problem0:10
- Operator: Multiplying the Original Function by Some Scalar0:11
- Operator, Eigenfunction, & Eigenvalue4:42
- Example: Eigenvalue Problem8:00
- Schrӧdinger Equation as an Eigenvalue Problem9:24
- Hamiltonian Operator15:09
- Quantum Mechanical Operators16:46
- Kinetic Energy Operator19:16
- Potential Energy Operator20:02
- Total Energy Operator21:12
- Classical Point of View21:48
- Linear Momentum Operator24:02
- Example I26:01
21m 34s
- Intro0:00
- The Plausibility of the Schrӧdinger Equation1:16
- The Plausibility of the Schrӧdinger Equation, Part 11:17
- The Plausibility of the Schrӧdinger Equation, Part 28:24
- The Plausibility of the Schrӧdinger Equation, Part 313:45
56m 22s
- Intro0:00
- Free Particle in a Box0:28
- Definition of a Free Particle in a Box0:29
- Amplitude of the Matter Wave6:22
- Intensity of the Wave6:53
- Probability Density9:39
- Probability that the Particle is Located Between x & dx10:54
- Probability that the Particle will be Found Between o & a12:35
- Wave Function & the Particle14:59
- Boundary Conditions19:22
- What Happened When There is No Constraint on the Particle27:54
- Diagrams34:12
- More on Probability Density40:53
- The Correspondence Principle46:45
- The Correspondence Principle46:46
- Normalizing the Wave Function47:46
- Normalizing the Wave Function47:47
- Normalized Wave Function & Normalization Constant52:24
45m 24s
- Intro0:00
- Free Particle in a Box0:08
- Free Particle in a 1-dimensional Box0:09
- For a Particle in a Box3:57
- Calculating Average Values & Standard Deviations5:42
- Average Value for the Position of a Particle6:32
- Standard Deviations for the Position of a Particle10:51
- Recall: Energy & Momentum are Represented by Operators13:33
- Recall: Schrӧdinger Equation in Operator Form15:57
- Average Value of a Physical Quantity that is Associated with an Operator18:16
- Average Momentum of a Free Particle in a Box20:48
- The Uncertainty Principle24:42
- Finding the Standard Deviation of the Momentum25:08
- Expression for the Uncertainty Principle35:02
- Summary of the Uncertainty Principle41:28
48m 43s
- Intro0:00
- 2-Dimension0:12
- Dimension 20:31
- Boundary Conditions1:52
- Partial Derivatives4:27
- Example I6:08
- The Particle in a Box, cont.11:28
- Operator Notation12:04
- Symbol for the Laplacian13:50
- The Equation Becomes…14:30
- Boundary Conditions14:54
- Separation of Variables15:33
- Solution to the 1-dimensional Case16:31
- Normalization Constant22:32
- 3-Dimension28:30
- Particle in a 3-dimensional Box28:31
- In Del Notation32:22
- The Solutions34:51
- Expressing the State of the System for a Particle in a 3D Box39:10
- Energy Level & Degeneracy43:35
46m 18s
- Intro0:00
- Postulate I0:31
- Probability That The Particle Will Be Found in a Differential Volume Element0:32
- Example I: Normalize This Wave Function11:30
- Postulate II18:20
- Postulate II18:21
- Quantum Mechanical Operators: Position20:48
- Quantum Mechanical Operators: Kinetic Energy21:57
- Quantum Mechanical Operators: Potential Energy22:42
- Quantum Mechanical Operators: Total Energy22:57
- Quantum Mechanical Operators: Momentum23:22
- Quantum Mechanical Operators: Angular Momentum23:48
- More On The Kinetic Energy Operator24:48
- Angular Momentum28:08
- Angular Momentum Overview28:09
- Angular Momentum Operator in Quantum Mechanic31:34
- The Classical Mechanical Observable32:56
- Quantum Mechanical Operator37:01
- Getting the Quantum Mechanical Operator from the Classical Mechanical Observable40:16
- Postulate II, cont.43:40
- Quantum Mechanical Operators are Both Linear & Hermetical43:41
39m 28s
- Intro0:00
- Postulate III0:09
- Postulate III: Part I0:10
- Postulate III: Part II5:56
- Postulate III: Part III12:43
- Postulate III: Part IV18:28
- Postulate IV23:57
- Postulate IV23:58
- Postulate V27:02
- Postulate V27:03
- Average Value36:38
- Average Value36:39
35m 32s
- Intro0:00
- The Postulates & Principles of Quantum Mechanics, Part III0:10
- Equations: Linear & Hermitian0:11
- Introduction to Hermitian Property3:36
- Eigenfunctions are Orthogonal9:55
- The Sequence of Wave Functions for the Particle in a Box forms an Orthonormal Set14:34
- Definition of Orthogonality16:42
- Definition of Hermiticity17:26
- Hermiticity: The Left Integral23:04
- Hermiticity: The Right Integral28:47
- Hermiticity: Summary34:06
29m 55s
- Intro0:00
- The Postulates & Principles of Quantum Mechanics, Part IV0:09
- Operators can be Applied Sequentially0:10
- Sample Calculation 12:41
- Sample Calculation 25:18
- Commutator of Two Operators8:16
- The Uncertainty Principle19:01
- In the Case of Linear Momentum and Position Operator23:14
- When the Commutator of Two Operators Equals to Zero26:31
54m 25s
- Intro0:00
- Example I: Three Dimensional Box & Eigenfunction of The Laplacian Operator0:37
- Example II: Positions of a Particle in a 1-dimensional Box15:46
- Example III: Transition State & Frequency29:29
- Example IV: Finding a Particle in a 1-dimensional Box35:03
- Example V: Degeneracy & Energy Levels of a Particle in a Box44:59
46m 58s
- Intro0:00
- Review0:25
- Wave Function0:26
- Normalization Condition2:28
- Observable in Classical Mechanics & Linear/Hermitian Operator in Quantum Mechanics3:36
- Hermitian6:11
- Eigenfunctions & Eigenvalue8:20
- Normalized Wave Functions12:00
- Average Value13:42
- If Ψ is Written as a Linear Combination15:44
- Commutator16:45
- Example I: Normalize The Wave Function19:18
- Example II: Probability of Finding of a Particle22:27
- Example III: Orthogonal26:00
- Example IV: Average Value of the Kinetic Energy Operator30:22
- Example V: Evaluate These Commutators39:02
44m 11s
- Intro0:00
- Example I: Good Candidate for a Wave Function0:08
- Example II: Variance of the Energy7:00
- Example III: Evaluate the Angular Momentum Operators15:00
- Example IV: Real Eigenvalues Imposes the Hermitian Property on Operators28:44
- Example V: A Demonstration of Why the Eigenfunctions of Hermitian Operators are Orthogonal35:33
35m 33s
- Intro0:00
- The Harmonic Oscillator0:10
- Harmonic Motion0:11
- Classical Harmonic Oscillator4:38
- Hooke's Law8:18
- Classical Harmonic Oscillator, cont.10:33
- General Solution for the Differential Equation15:16
- Initial Position & Velocity16:05
- Period & Amplitude20:42
- Potential Energy of the Harmonic Oscillator23:20
- Kinetic Energy of the Harmonic Oscillator26:37
- Total Energy of the Harmonic Oscillator27:23
- Conservative System34:37
43m 4s
- Intro0:00
- The Harmonic Oscillator II0:08
- Diatomic Molecule0:10
- Notion of Reduced Mass5:27
- Harmonic Oscillator Potential & The Intermolecular Potential of a Vibrating Molecule7:33
- The Schrӧdinger Equation for the 1-dimensional Quantum Mechanic Oscillator14:14
- Quantized Values for the Energy Level15:46
- Ground State & the Zero-Point Energy21:50
- Vibrational Energy Levels25:18
- Transition from One Energy Level to the Next26:42
- Fundamental Vibrational Frequency for Diatomic Molecule34:57
- Example: Calculate k38:01
26m 30s
- Intro0:00
- The Harmonic Oscillator III0:09
- The Wave Functions Corresponding to the Energies0:10
- Normalization Constant2:34
- Hermite Polynomials3:22
- First Few Hermite Polynomials4:56
- First Few Wave-Functions6:37
- Plotting the Probability Density of the Wave-Functions8:37
- Probability Density for Large Values of r14:24
- Recall: Odd Function & Even Function19:05
- More on the Hermite Polynomials20:07
- Recall: If f(x) is Odd20:36
- Average Value of x22:31
- Average Value of Momentum23:56
41m 10s
- Intro0:00
- Possible Confusion from the Previous Discussion0:07
- Possible Confusion from the Previous Discussion0:08
- Rotation of a Single Mass Around a Fixed Center8:17
- Rotation of a Single Mass Around a Fixed Center8:18
- Angular Velocity12:07
- Rotational Inertia13:24
- Rotational Frequency15:24
- Kinetic Energy for a Linear System16:38
- Kinetic Energy for a Rotational System17:42
- Rotating Diatomic Molecule19:40
- Rotating Diatomic Molecule: Part 119:41
- Rotating Diatomic Molecule: Part 224:56
- Rotating Diatomic Molecule: Part 330:04
- Hamiltonian of the Rigid Rotor36:48
- Hamiltonian of the Rigid Rotor36:49
30m 32s
- Intro0:00
- The Rigid Rotator II0:08
- Cartesian Coordinates0:09
- Spherical Coordinates1:55
- r6:15
- θ6:28
- φ7:00
- Moving a Distance 'r'8:17
- Moving a Distance 'r' in the Spherical Coordinates11:49
- For a Rigid Rotator, r is Constant13:57
- Hamiltonian Operator15:09
- Square of the Angular Momentum Operator17:34
- Orientation of the Rotation in Space19:44
- Wave Functions for the Rigid Rotator20:40
- The Schrӧdinger Equation for the Quantum Mechanic Rigid Rotator21:24
- Energy Levels for the Rigid Rotator26:58
35m 19s
- Intro0:00
- The Rigid Rotator III0:11
- When a Rotator is Subjected to Electromagnetic Radiation1:24
- Selection Rule2:13
- Frequencies at Which Absorption Transitions Occur6:24
- Energy Absorption & Transition10:54
- Energy of the Individual Levels Overview20:58
- Energy of the Individual Levels: Diagram23:45
- Frequency Required to Go from J to J + 125:53
- Using Separation Between Lines on the Spectrum to Calculate Bond Length28:02
- Example I: Calculating Rotational Inertia & Bond Length29:18
- Example I: Calculating Rotational Inertia29:19
- Example I: Calculating Bond Length32:56
33m 48s
- Intro0:00
- Equations Review0:11
- Energy of the Harmonic Oscillator0:12
- Selection Rule3:02
- Observed Frequency of Radiation3:27
- Harmonic Oscillator Wave Functions5:52
- Rigid Rotator7:26
- Selection Rule for Rigid Rotator9:15
- Frequency of Absorption9:35
- Wave Numbers10:58
- Example I: Calculate the Reduced Mass of the Hydrogen Atom11:44
- Example II: Calculate the Fundamental Vibration Frequency & the Zero-Point Energy of This Molecule13:37
- Example III: Show That the Product of Two Even Functions is even19:35
- Example IV: Harmonic Oscillator24:56
46m 43s
- Intro0:00
- Example I: Harmonic Oscillator0:12
- Example II: Harmonic Oscillator23:26
- Example III: Calculate the RMS Displacement of the Molecules38:12
40m
- Intro0:00
- The Hydrogen Atom I1:31
- Review of the Rigid Rotator1:32
- Hydrogen Atom & the Coulomb Potential2:50
- Using the Spherical Coordinates6:33
- Applying This Last Expression to Equation 110:19
- Angular Component & Radial Component13:26
- Angular Equation15:56
- Solution for F(φ)19:32
- Determine The Normalization Constant20:33
- Differential Equation for T(a)24:44
- Legendre Equation27:20
- Legendre Polynomials31:20
- The Legendre Polynomials are Mutually Orthogonal35:40
- Limits37:17
- Coefficients38:28
35m 58s
- Intro0:00
- Associated Legendre Functions0:07
- Associated Legendre Functions0:08
- First Few Associated Legendre Functions6:39
- s, p, & d Orbital13:24
- The Normalization Condition15:44
- Spherical Harmonics20:03
- Equations We Have Found20:04
- Wave Functions for the Angular Component & Rigid Rotator24:36
- Spherical Harmonics Examples25:40
- Angular Momentum30:09
- Angular Momentum30:10
- Square of the Angular Momentum35:38
- Energies of the Rigid Rotator38:21
36m 18s
- Intro0:00
- The Hydrogen Atom III0:34
- Angular Momentum is a Vector Quantity0:35
- The Operators Corresponding to the Three Components of Angular Momentum Operator: In Cartesian Coordinates1:30
- The Operators Corresponding to the Three Components of Angular Momentum Operator: In Spherical Coordinates3:27
- Z Component of the Angular Momentum Operator & the Spherical Harmonic5:28
- Magnitude of the Angular Momentum Vector20:10
- Classical Interpretation of Angular Momentum25:22
- Projection of the Angular Momentum Vector onto the xy-plane33:24
33m 55s
- Intro0:00
- The Hydrogen Atom IV0:09
- The Equation to Find R( r )0:10
- Relation Between n & l3:50
- The Solutions for the Radial Functions5:08
- Associated Laguerre Polynomials7:58
- 1st Few Associated Laguerre Polynomials8:55
- Complete Wave Function for the Atomic Orbitals of the Hydrogen Atom12:24
- The Normalization Condition15:06
- In Cartesian Coordinates18:10
- Working in Polar Coordinates20:48
- Principal Quantum Number21:58
- Angular Momentum Quantum Number22:35
- Magnetic Quantum Number25:55
- Zeeman Effect30:45
51m 53s
- Intro0:00
- The Hydrogen Atom V: Where We Are0:13
- Review0:14
- Let's Write Out ψ₂₁₁7:32
- Angular Momentum of the Electron14:52
- Representation of the Wave Function19:36
- Radial Component28:02
- Example: 1s Orbital28:34
- Probability for Radial Function33:46
- 1s Orbital: Plotting Probability Densities vs. r35:47
- 2s Orbital: Plotting Probability Densities vs. r37:46
- 3s Orbital: Plotting Probability Densities vs. r38:49
- 4s Orbital: Plotting Probability Densities vs. r39:34
- 2p Orbital: Plotting Probability Densities vs. r40:12
- 3p Orbital: Plotting Probability Densities vs. r41:02
- 4p Orbital: Plotting Probability Densities vs. r41:51
- 3d Orbital: Plotting Probability Densities vs. r43:18
- 4d Orbital: Plotting Probability Densities vs. r43:48
- Example I: Probability of Finding an Electron in the 2s Orbital of the Hydrogen45:40
51m 53s
- Intro0:00
- The Hydrogen Atom VI0:07
- Last Lesson Review0:08
- Spherical Component1:09
- Normalization Condition2:02
- Complete 1s Orbital Wave Function4:08
- 1s Orbital Wave Function4:09
- Normalization Condition6:28
- Spherically Symmetric16:00
- Average Value17:52
- Example I: Calculate the Region of Highest Probability for Finding the Electron21:19
- 2s Orbital Wave Function25:32
- 2s Orbital Wave Function25:33
- Average Value28:56
- General Formula32:24
34m 29s
- Intro0:00
- The Hydrogen Atom VII0:12
- p Orbitals1:30
- Not Spherically Symmetric5:10
- Recall That the Spherical Harmonics are Eigenfunctions of the Hamiltonian Operator6:50
- Any Linear Combination of These Orbitals Also Has The Same Energy9:16
- Functions of Real Variables15:53
- Solving for Px16:50
- Real Spherical Harmonics21:56
- Number of Nodes32:56
43m 49s
- Intro0:00
- Example I: Angular Momentum & Spherical Harmonics0:20
- Example II: Pair-wise Orthogonal Legendre Polynomials16:40
- Example III: General Normalization Condition for the Legendre Polynomials25:06
- Example IV: Associated Legendre Functions32:13
1h 1m 57s
- Intro0:00
- Example I: Normalization & Pair-wise Orthogonal0:13
- Part 1: Normalized0:43
- Part 2: Pair-wise Orthogonal16:53
- Example II: Show Explicitly That the Following Statement is True for Any Integer n27:10
- Example III: Spherical Harmonics29:26
- Angular Momentum Cones56:37
- Angular Momentum Cones56:38
- Physical Interpretation of Orbital Angular Momentum in Quantum mechanics1:00:16
48m 33s
- Intro0:00
- Example I: Show That ψ₂₁₁ is Normalized0:07
- Example II: Show That ψ₂₁₁ is Orthogonal to ψ₃₁₀11:48
- Example III: Probability That a 1s Electron Will Be Found Within 1 Bohr Radius of The Nucleus18:35
- Example IV: Radius of a Sphere26:06
- Example V: Calculate <r> for the 2s Orbital of the Hydrogen-like Atom36:33
48m 33s
- Intro0:00
- Example I: Probability Density vs. Radius Plot0:11
- Example II: Hydrogen Atom & The Coulombic Potential14:16
- Example III: Find a Relation Among <K>, <V>, & <E>25:47
- Example IV: Quantum Mechanical Virial Theorem48:32
- Example V: Find the Variance for the 2s Orbital54:13
48m 33s
- Intro0:00
- Example I: Derive a Formula for the Degeneracy of a Given Level n0:11
- Example II: Using Linear Combinations to Represent the Spherical Harmonics as Functions of the Real Variables θ & φ8:30
- Example III: Using Linear Combinations to Represent the Spherical Harmonics as Functions of the Real Variables θ & φ23:01
- Example IV: Orbital Functions31:51
59m 18s
- Intro0:00
- Quantum Numbers Specify an Orbital0:24
- n1:10
- l1:20
- m1:35
- 4th Quantum Number: s2:02
- Spin Orbitals7:03
- Spin Orbitals7:04
- Multi-electron Atoms11:08
- Term Symbols18:08
- Russell-Saunders Coupling & The Atomic Term Symbol18:09
- Example: Configuration for C27:50
- Configuration for C: 1s²2s²2p²27:51
- Drawing Every Possible Arrangement31:15
- Term Symbols45:24
- Microstate50:54
34m 54s
- Intro0:00
- Microstates0:25
- We Started With 21 Possible Microstates0:26
- ³P State2:05
- Microstates in ³P Level5:10
- ¹D State13:16
- ³P State16:10
- ²P₂ State17:34
- ³P₁ State18:34
- ³P₀ State19:12
- 9 Microstates in ³P are Subdivided19:40
- ¹S State21:44
- Quicker Way to Find the Different Values of J for a Given Basic Term Symbol22:22
- Ground State26:27
- Hund's Empirical Rules for Specifying the Term Symbol for the Ground Electronic State27:29
- Hund's Empirical Rules: 128:24
- Hund's Empirical Rules: 229:22
- Hund's Empirical Rules: 3 - Part A30:22
- Hund's Empirical Rules: 3 - Part B31:18
- Example: 1s²2s²2p²31:54
38m 3s
- Intro0:00
- Spin Quantum Number: Term Symbols III0:14
- Deriving the Term Symbols for the p² Configuration0:15
- Table: MS vs. ML3:57
- ¹D State16:21
- ³P State21:13
- ¹S State24:48
- J Value25:32
- Degeneracy of the Level27:28
- When Given r Electrons to Assign to n Equivalent Spin Orbitals30:18
- p² Configuration32:51
- Complementary Configurations35:12
57m 49s
- Intro0:00
- Lyman Series0:09
- Spectroscopic Term Symbols0:10
- Lyman Series3:04
- Hydrogen Levels8:21
- Hydrogen Levels8:22
- Term Symbols & Atomic Spectra14:17
- Spin-Orbit Coupling14:18
- Selection Rules for Atomic Spectra21:31
- Selection Rules for Possible Transitions23:56
- Wave Numbers for The Transitions28:04
- Example I: Calculate the Frequencies of the Allowed Transitions from (4d) ²D →(2p) ²P32:23
- Helium Levels49:50
- Energy Levels for Helium49:51
- Transitions & Spin Multiplicity52:27
- Transitions & Spin Multiplicity52:28
1h 1m 20s
- Intro0:00
- Example I: What are the Term Symbols for the np¹ Configuration?0:10
- Example II: What are the Term Symbols for the np² Configuration?20:38
- Example III: What are the Term Symbols for the np³ Configuration?40:46
56m 34s
- Intro0:00
- Example I: Find the Term Symbols for the nd² Configuration0:11
- Example II: Find the Term Symbols for the 1s¹2p¹ Configuration27:02
- Example III: Calculate the Separation Between the Doublets in the Lyman Series for Atomic Hydrogen41:41
- Example IV: Calculate the Frequencies of the Lines for the (4d) ²D → (3p) ²P Transition48:53
18m 24s
- Intro0:00
- Quantum Mechanics Equations0:37
- De Broglie Relation0:38
- Statistical Relations1:00
- The Schrӧdinger Equation1:50
- The Particle in a 1-Dimensional Box of Length a3:09
- The Particle in a 2-Dimensional Box of Area a x b3:48
- The Particle in a 3-Dimensional Box of Area a x b x c4:22
- The Schrӧdinger Equation Postulates4:51
- The Normalization Condition5:40
- The Probability Density6:51
- Linear7:47
- Hermitian8:31
- Eigenvalues & Eigenfunctions8:55
- The Average Value9:29
- Eigenfunctions of Quantum Mechanics Operators are Orthogonal10:53
- Commutator of Two Operators10:56
- The Uncertainty Principle11:41
- The Harmonic Oscillator13:18
- The Rigid Rotator13:52
- Energy of the Hydrogen Atom14:30
- Wavefunctions, Radial Component, and Associated Laguerre Polynomial14:44
- Angular Component or Spherical Harmonic15:16
- Associated Legendre Function15:31
- Principal Quantum Number15:43
- Angular Momentum Quantum Number15:50
- Magnetic Quantum Number16:21
- z-component of the Angular Momentum of the Electron16:53
- Atomic Spectroscopy: Term Symbols17:14
- Atomic Spectroscopy: Selection Rules18:03
50m 2s
- Intro0:00
- Spectroscopic Overview: Which Equation Do I Use & Why1:02
- Lesson Overview1:03
- Rotational & Vibrational Spectroscopy4:01
- Frequency of Absorption/Emission6:04
- Wavenumbers in Spectroscopy8:10
- Starting State vs. Excited State10:10
- Total Energy of a Molecule (Leaving out the Electronic Energy)14:02
- Energy of Rotation: Rigid Rotor15:55
- Energy of Vibration: Harmonic Oscillator19:08
- Equation of the Spectral Lines23:22
- Harmonic Oscillator-Rigid Rotor Approximation (Making Corrections)28:37
- Harmonic Oscillator-Rigid Rotor Approximation (Making Corrections)28:38
- Vibration-Rotation Interaction33:46
- Centrifugal Distortion36:27
- Anharmonicity38:28
- Correcting for All Three Simultaneously41:03
- Spectroscopic Parameters44:26
- Summary47:32
- Harmonic Oscillator-Rigid Rotor Approximation47:33
- Vibration-Rotation Interaction48:14
- Centrifugal Distortion48:20
- Anharmonicity48:28
- Correcting for All Three Simultaneously48:44
59m 47s
- Intro0:00
- Vibration-Rotation0:37
- What is Molecular Spectroscopy?0:38
- Microwave, Infrared Radiation, Visible & Ultraviolet1:53
- Equation for the Frequency of the Absorbed Radiation4:54
- Wavenumbers6:15
- Diatomic Molecules: Energy of the Harmonic Oscillator8:32
- Selection Rules for Vibrational Transitions10:35
- Energy of the Rigid Rotator16:29
- Angular Momentum of the Rotator21:38
- Rotational Term F(J)26:30
- Selection Rules for Rotational Transition29:30
- Vibration Level & Rotational States33:20
- Selection Rules for Vibration-Rotation37:42
- Frequency of Absorption39:32
- Diagram: Energy Transition45:55
- Vibration-Rotation Spectrum: HCl51:27
- Vibration-Rotation Spectrum: Carbon Monoxide54:30
46m 22s
- Intro0:00
- Vibration-Rotation Interaction0:13
- Vibration-Rotation Spectrum: HCl0:14
- Bond Length & Vibrational State4:23
- Vibration Rotation Interaction10:18
- Case 112:06
- Case 217:17
- Example I: HCl Vibration-Rotation Spectrum22:58
- Rotational Constant for the 0 & 1 Vibrational State26:30
- Equilibrium Bond Length for the 1 Vibrational State39:42
- Equilibrium Bond Length for the 0 Vibrational State42:13
- Bₑ & αₑ44:54
29m 24s
- Intro0:00
- The Non-Rigid Rotator0:09
- Pure Rotational Spectrum0:54
- The Selection Rules for Rotation3:09
- Spacing in the Spectrum5:04
- Centrifugal Distortion Constant9:00
- Fundamental Vibration Frequency11:46
- Observed Frequencies of Absorption14:14
- Difference between the Rigid Rotator & the Adjusted Rigid Rotator16:51
- Adjusted Rigid Rotator21:31
- Observed Frequencies of Absorption26:26
30m 53s
- Intro0:00
- The Anharmonic Oscillator0:09
- Vibration-Rotation Interaction & Centrifugal Distortion0:10
- Making Corrections to the Harmonic Oscillator4:50
- Selection Rule for the Harmonic Oscillator7:50
- Overtones8:40
- True Oscillator11:46
- Harmonic Oscillator Energies13:16
- Anharmonic Oscillator Energies13:33
- Observed Frequencies of the Overtones15:09
- True Potential17:22
- HCl Vibrational Frequencies: Fundamental & First Few Overtones21:10
- Example I: Vibrational States & Overtones of the Vibrational Spectrum22:42
- Example I: Part A - First 4 Vibrational States23:44
- Example I: Part B - Fundamental & First 3 Overtones25:31
- Important Equations27:45
- Energy of the Q State29:14
- The Difference in Energy between 2 Successive States29:23
- Difference in Energy between 2 Spectral Lines29:40
1h 1m 33s
- Intro0:00
- Electronic Transitions0:16
- Electronic State & Transition0:17
- Total Energy of the Diatomic Molecule3:34
- Vibronic Transitions4:30
- Selection Rule for Vibronic Transitions9:11
- More on Vibronic Transitions10:08
- Frequencies in the Spectrum16:46
- Difference of the Minima of the 2 Potential Curves24:48
- Anharmonic Zero-point Vibrational Energies of the 2 States26:24
- Frequency of the 0 → 0 Vibronic Transition27:54
- Making the Equation More Compact29:34
- Spectroscopic Parameters32:11
- Franck-Condon Principle34:32
- Example I: Find the Values of the Spectroscopic Parameters for the Upper Excited State47:27
- Table of Electronic States and Parameters56:41
33m 47s
- Intro0:00
- Example I: Calculate the Bond Length0:10
- Example II: Calculate the Rotational Constant7:39
- Example III: Calculate the Number of Rotations10:54
- Example IV: What is the Force Constant & Period of Vibration?16:31
- Example V: Part A - Calculate the Fundamental Vibration Frequency21:42
- Example V: Part B - Calculate the Energies of the First Three Vibrational Levels24:12
- Example VI: Calculate the Frequencies of the First 2 Lines of the R & P Branches of the Vib-Rot Spectrum of HBr26:28
1h 1m 5s
- Intro0:00
- Example I: Calculate the Frequencies of the Transitions0:09
- Example II: Specify Which Transitions are Allowed & Calculate the Frequencies of These Transitions22:07
- Example III: Calculate the Vibrational State & Equilibrium Bond Length34:31
- Example IV: Frequencies of the Overtones49:28
- Example V: Vib-Rot Interaction, Centrifugal Distortion, & Anharmonicity54:47
33m 31s
- Intro0:00
- Example I: Part A - Derive an Expression for ∆G( r )0:10
- Example I: Part B - Maximum Vibrational Quantum Number6:10
- Example II: Part A - Derive an Expression for the Dissociation Energy of the Molecule8:29
- Example II: Part B - Equation for ∆G( r )14:00
- Example III: How Many Vibrational States are There for Br₂ before the Molecule Dissociates18:16
- Example IV: Find the Difference between the Two Minima of the Potential Energy Curves20:57
- Example V: Rotational Spectrum30:51
1h 1m 15s
- Intro0:00
- Statistical Thermodynamics: The Big Picture0:10
- Our Big Picture Goal0:11
- Partition Function (Q)2:42
- The Molecular Partition Function (q)4:00
- Consider a System of N Particles6:54
- Ensemble13:22
- Energy Distribution Table15:36
- Probability of Finding a System with Energy16:51
- The Partition Function21:10
- Microstate28:10
- Entropy of the Ensemble30:34
- Entropy of the System31:48
- Expressing the Thermodynamic Functions in Terms of The Partition Function39:21
- The Partition Function39:22
- Pi & U41:20
- Entropy of the System44:14
- Helmholtz Energy48:15
- Pressure of the System49:32
- Enthalpy of the System51:46
- Gibbs Free Energy52:56
- Heat Capacity54:30
- Expressing Q in Terms of the Molecular Partition Function (q)59:31
- Indistinguishable Particles1:02:16
- N is the Number of Particles in the System1:03:27
- The Molecular Partition Function1:05:06
- Quantum States & Degeneracy1:07:46
- Thermo Property in Terms of ln Q1:10:09
- Example: Thermo Property in Terms of ln Q1:13:23
47m 23s
- Intro0:00
- Lesson Overview0:19
- Monatomic Ideal Gases6:40
- Monatomic Ideal Gases Overview6:42
- Finding the Parition Function of Translation8:17
- Finding the Parition Function of Electronics13:29
- Example: Na17:42
- Example: F23:12
- Energy Difference between the Ground State & the 1st Excited State29:27
- The Various Partition Functions for Monatomic Ideal Gases32:20
- Finding P43:16
- Going Back to U = (3/2) RT46:20
54m 9s
- Intro0:00
- Diatomic Gases0:16
- Diatomic Gases0:17
- Zero-Energy Mark for Rotation2:26
- Zero-Energy Mark for Vibration3:21
- Zero-Energy Mark for Electronic5:54
- Vibration Partition Function9:48
- When Temperature is Very Low14:00
- When Temperature is Very High15:22
- Vibrational Component18:48
- Fraction of Molecules in the r Vibration State21:00
- Example: Fraction of Molecules in the r Vib. State23:29
- Rotation Partition Function26:06
- Heteronuclear & Homonuclear Diatomics33:13
- Energy & Heat Capacity36:01
- Fraction of Molecules in the J Rotational Level39:20
- Example: Fraction of Molecules in the J Rotational Level40:32
- Finding the Most Populated Level44:07
- Putting It All Together46:06
- Putting It All Together46:07
- Energy of Translation51:51
- Energy of Rotation52:19
- Energy of Vibration52:42
- Electronic Energy53:35
48m 32s
- Intro0:00
- Example I: Calculate the Fraction of Potassium Atoms in the First Excited Electronic State0:10
- Example II: Show That Each Translational Degree of Freedom Contributes R/2 to the Molar Heat Capacity14:46
- Example III: Calculate the Dissociation Energy21:23
- Example IV: Calculate the Vibrational Contribution to the Molar heat Capacity of Oxygen Gas at 500 K25:46
- Example V: Upper & Lower Quantum State32:55
- Example VI: Calculate the Relative Populations of the J=2 and J=1 Rotational States of the CO Molecule at 25°C42:21
57m 30s
- Intro0:00
- Example I: Make a Plot of the Fraction of CO Molecules in Various Rotational Levels0:10
- Example II: Calculate the Ratio of the Translational Partition Function for Cl₂ and Br₂ at Equal Volume & Temperature8:05
- Example III: Vibrational Degree of Freedom & Vibrational Molar Heat Capacity11:59
- Example IV: Calculate the Characteristic Vibrational & Rotational temperatures for Each DOF45:03
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