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IIT Energy Materials Group
United States
เข้าร่วมเมื่อ 30 ต.ค. 2017
The Illinois Institute of Technology (IIT) Energy Materials Group is led by Prof. Carlo Segre from the Department of Physics (Duchossois Leadership Professor) and Dr. Elena Timofeeva, Research Professor in the Department of Chemistry. The complementary expertise enables scientific pursuits in cutting edge interdisciplinary projects. We develop and investigate of new functional materials for battery cathodes and anodes, catalysts for fuel cells, nanofluid flow batteries and other functional nanocomposites. We use in situ and ex situ x-ray absorption spectroscopy (XAS) and x-ray diffraction (XRD) techniques to study material’s structure and transformations, revealing the reaction mechanisms and ways to improve the performance.
The purpose of this TH-cam channel is to share our research with the broader community and to engage in discussion and collaborations with other research groups and interested individuals. Contact us: segre@iit.edu, etimofee@iit.edu.
The purpose of this TH-cam channel is to share our research with the broader community and to engage in discussion and collaborations with other research groups and interested individuals. Contact us: segre@iit.edu, etimofee@iit.edu.
Practical application of radiolysis to flow battery charging
The phenomenon of radiolysis charging is described and experimentally verified. On practical application is briefly discussed.
มุมมอง: 252
วีดีโอ
Coin Cell Assembly
มุมมอง 7422 ปีที่แล้ว
Otavio Marques, a Ph.D. student in our group demonstrates the assembly of a Li-ion coin cell.
Electrode Casting
มุมมอง 2.3K2 ปีที่แล้ว
Otavio Marques, a Ph.D. student in the group explains how we cast electrodes for Li-ion battery testing.
11.01 Time dependent perturbation theory
มุมมอง 4.3K3 ปีที่แล้ว
11.01 Time dependent perturbation theory
10.04 The integral Schrödinger equation
มุมมอง 2.6K3 ปีที่แล้ว
10.04 The integral Schrödinger equation
9.02 The WKB solution for the non-classical region
มุมมอง 3.5K3 ปีที่แล้ว
9.02 The WKB solution for the non-classical region
7.06 The intermediate field Zeeman effect
มุมมอง 2.8K3 ปีที่แล้ว
7.06 The intermediate field Zeeman effect
7.05 The Zeeman effect for weak and strong fields
มุมมอง 6K3 ปีที่แล้ว
7.05 The Zeeman effect for weak and strong fields
7.03 The hydrogen relativistic correction
มุมมอง 4K3 ปีที่แล้ว
7.03 The hydrogen relativistic correction
7.04 The hydrogen spin-orbit correction
มุมมอง 3.3K3 ปีที่แล้ว
7.04 The hydrogen spin-orbit correction
Aliya Meadow
99006 Bernhard Highway
Theoretical physicists keep telling each other (and their students) that these corrections are very important. Unfortunately, nobody else thinks so ;-)
Than you, good explanation, can you send a pdf of this lecture please 🙏🏼 i need it
Thank you. If you want the slides you will hve to send me an email.
@@iitenergymaterialsgroup4816 can you send your email so i can messaging you
@@iitenergymaterialsgroup4816 can you send your email so i can message you 🙏🏼
perfect
99464 Beier Underpass
Why a particle in box? Why not mention that it comes close to an electron bound in an atom that is hit by some perturbation from outside? It makes the scene described a bit more realistic (for me).
Always start with the simplest problem, a spherical horse. Then you can move to something more complex, like the fine structure and Zeeman effect.
@@iitenergymaterialsgroup4816 But if your simplest model is far from reality (= too abstract, so there is no recognition). then it might not feel so simple anymore ;-)
@@jacobvandijk6525 Zeeman effect is not simple nor is it unphysical. Start simple end up with a real system and the student can understand all the way through. Believe me a 20 year old student will not get the idea if the spin-orbit couple is the first example. YYMV
@@iitenergymaterialsgroup4816 Haha, I agree with you on that last statement. P.S. I know the YMCA, but what is YYMV?
@@jacobvandijk6525 I mean YMMV (Your Mileage May Vary)
shouldn't we have g_e in H'_hf (around 1:52)?
It is assumed to be 2 and thus cancels out a 2 in the denominator.
At 11:25 Its (-i)^l+1 instead of (-1)^l+1 in the second line
You are correct, it is a typographical error but the line below is correct.
Psi = e^(ig)Psi' not= -ihbar*e^(ig)grad(Psi'), so how can you apply the operator again to -ihbar*e^(ig)grad(Psi')?
Time stamp?
4:36, but I see now the operator got squared so it isn't replacing phi with -hbar*e^(ig)grad(Psi').
@@willemesterhuyse2547 That is correct.
thank you so much
Thank you so much
Glad you find them useful.
Thank you
Glad you find them useful.
Do you have any video on Bell's theorem? TIA
this playlist is amazing! thank you
nice
sir what is (al) that you used to expand cl
al, is the partial wave coefficient. To have the solution to a problem of scattering, we need to find those coefficients. I believe, not sure tho, we find those coefficients by aplying the proper bound condiditions of our problem to the general solution, that's derived here.
thaks a lot for this
You are very welcome
Agreed, very useful for exam prep. Wish there were more example problems available online though.
Not having the problems in the videos is deliberate.
where does the iota go in the equation for cb from 7:23 to 7:50 ?
It is not an iota. It is the "i" for a complex number and it can be removed as it is a global phase factor that cancels when computing the probability.
oh okay, i was wondering where my calculations went wrong. thank you.@@iitenergymaterialsgroup4816
Thank You Sir for teaching this in a very simple way. 🙏
I'm glad it was useful!
Lmao my prof put "solve for the normalized molecular wave function of a hydrogen molecule" homework when we had a single lecture on molecular hydrogen ion and it didn't provide half of the concepts I just learned watching this video.
I'm glad you found it useful.
Hace pocos días conocí este experimento. Solo conozco algo de la teoría clásica del electromagnetismo. Pero noto algo extraño en el fenómeno que se trata de explicar con operaciones matemáticas muy complejas, para mi modesta formación matemática. No logro ver en qué parte del estudio se considera el propio campo magnético de la partícula en movimiento. Si se considera el propio campo magnético de la partícula, se entiende mejor que es dicho campo el que llega hasta el espacio donde está confinado el otro campo. De esta manera, se ve claramente que sí hay un área de interacción de ambos campos, y por supuesto una fuerza que cambia la trayectoria de la partícula.
Brilliant competition
I always like ur videos
Thanks!
Very hepful thank you! Great presentation.
You very welcome.
Thank you 🙏
You are very welcome
11:42 , Podría explicar como obtener la constante de normalización?
Normalization is performed in the usual way but integrating the probability density and setting it equal to 1. WHile the Griffiths book does not do the integral explicitly, I am sure you can find a book which has it done.
clear cut stuff!!! Hatsoff!!!
Thank you!
What x quantity of NMP did you use for y quantity of total powder ? I want to achieve same slurry viscosity as you ! Thanks
These details should be in our publication: doi.org/10.1016/j.jpowsour.2023.232852 and doi.org/10.3390/batteries9020115
This is a fine example of the fact that with math you can create any unphysical situation you like. Here (11:48) in first approximation the lower state is unchanged, but somehow (not physically explained, of course) the higher state in this two-state system is changed! This is truly an amazing system, haha.
I think you’re misunderstanding something here
@@gi99hf60 Could be. But it seems to me you can't explain it either.
@@jacobvandijk6525there was a global phase common factor taken out initially, now imbedded in the w_0. This is just an artifact of that. Due to normalization, it doesn’t matter what the absolute magnitude of c_a or c_b is, but the ratio of their squares. That’s why the initial global phase factor was taken out initially, to keep one coefficient at unity and just keep all the evolution info in the other. Then we only solve one equation, it was intentionally set up that way to simplify the calculation
@@jacobvandijk6525 physically, the probability of being in the lower state is still decreasing just by the coefficient of the other changing. You’ll have to normalize at the end anyways
What will be the energy for bound state of a particle in a square well? Is E<0 or E>0?
You can always set the potential of the bottom of the well to whatever you like. If you set it at zero, as conventionally is done for the infinite well, all the energies are positive. Things are different with the finite well. There we generally set the bottom of the well to -V and all the energies are negative. However, you could just as well set the bottom of the well to zero and the "outside" to V. The solutions are thus shifted by V.
Thanks I have been trying to describe the “U” shape wave that is produced in my model that is produced as the loading increases/ just before the wave function shifts to the next higher energy level. Your viewers might be interested in watching the test video of my model see the load verse deflection graph. th-cam.com/video/wrBsqiE0vG4/w-d-xo.htmlsi=waT8lY2iX-wJdjO3
Thanks, I'll take a look
you saved my life thanks
Happy to help!
@ 3:40 He calls it a potential, but it really is a potential energy: H' = P . E = (e . z) . E = e . (z . E) = e . V = PE (11:06). And, as you can see from H = (e . z) . E, it is also the energy of an electric dipole in an oscillating E-field.
Saying “potential” can mean both “electric potential” and “potential energy”
@@gi99hf60 When you are teaching, you must be clear about concepts.
Thank you sir...
You are very welcome!
I dont understand how we take the expectation value of 1/J^2 mathematically and also have a <J> outside as if it was distributive under multiplication
Pleae tell me the time or slide number and I can better respond
Thank you sir 😊
You are welcome
absolute fire 🔥
Thank you, glad you found it helpful
Very helpful, thank you very much!
You are welcome!
Amazing what the internet can find for me! I got my chem degree 40 yrs ago i only had 3 or 4 books now i can find multiple sources excellently presented explaing what I want. My son got stuck with his qm module in his astrophysics degree and I found this for him and he is much happier!
Couldn't agree more. It's a wonderful source of knowledge. Hope your son does well.
You are very welcome, I hope your son does well.
reference please?
Reference for what in particular? Give me a time stamp and slide number.
can you pls tell me why in l equal to 0 the first term is "null"
If you give me a time stamp I can answer your question.
This effort of yours is commendable. Don't know how to thank you!
7:37 why does this L-L+(ft) term vanish? Can you please explain
ft is the topmost angular momentum eigenfunction. If you apply L+ to raise it it just gives zero because you cannot go above the top function.
@@iitenergymaterialsgroup4816 Yep... absolutely... later realized myself.
Hello professor Thank you for the great lecture.I have a doubt at 5:48 How can we say that the value of integral is 1 or the function u(r) is normalised?
If comes directly from the normalization of the entire 3D wavefunction. Recall that in the radial normalization integral you have |R|^2r^2 in the integrand. This is exactly |u|^2.
May l ask, what exactly are r_1 and r_2? Are these positions in the same coordinate space from the same origin? If so, how do the gradients differ? Do they differ only by their actions on the wavefunctions?
It helps if you tell me at what time in the video you are raising the question. I presume that you mean the part on two identical particles. In this case r_1 and r_2 are the positions of the two identical particles with respect to a common origin.
I find your online lectures to be accessible, to the point, well-informed and well-presented.
@peterchindove7146 Sorry about the delay, thanks!
14:30 I guess n^2 term is missing from the expectation value of 1/r.
You are correct
Sir can you please elaborate on how you've obtained this c_j+1 = (2^j/j!)*(c_0) timestamp: 10:44
In order to get c_j in terms of c_0, you need to apply the recursion j time. Each time you get a power of 2 in the numerator and one higher value in the denominator, starting with 1 and ending with j. This is simply j!.
@@iitenergymaterialsgroup4816ok 👍🏻
Thank you so much professor! Can't imagine how much this helped.
You are welcome!