Quantum Mechanics Schaum Series Pdf

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Sueann

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Aug 4, 2024, 9:14:59 PM8/4/24
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Anywayyou might be right that the standard trajectory is semiotics to understanding, but in my case it was stupid grunt work, mixed with useful grunt work. Grad school was grunt work and semiotics. A real mixed bag. It was obvious that it was an ad-hoc collection of approaches, and that it left me with some strengths and not too many weaknesses; I think the grunt work is needed to actually understand things beyond hand wavings.

Let me illustrate. A friend of mine and I got into a lengthy black board discussion about exactly the topic of this blog post. We were contrasting classical and quantum mechanical path integrals (e.g. the sort you see in Onsager-Machlup vs. those you see in non-relativistic quantum mechanics). We were pretty obsessed with the complex phase factor as opposed to the real factor in the classical path integral.


Your hewers of wood and drawers of water madrassa sounds pretty awesome though. I would love to talk to some kids who went through it, I bet they would learn all kinds of useful stuff, unlike some of the kids I interview these days.


I probably learned in some weird order that nobody else gets; I was doing Greens functions and path integrals before I ever quantized anything. I basically had two grown-up courses my sophomore year that put me mathematically ahead of most of my colleagues in grad school who had to work through Arfken when their brains were three or four years more ossified. I also lucked out and Jennie Traschen (a Penrose student, most famous for damning America on public access TV Sept 10, 2001) taught us a bunch of group theory junior year in a 1-credit seminar, also before I was doing any serious QM. Made spin orbit coupling easy-peasy. Also got lucky with an experimental junior year course (probably now reserved for grad students) in applied analysis using Hilbert spaces/orthogonal functions, which should probably be given freshman or sophomore year.


My complex analysis stuff was taught by a bored community college physics prof who still published GR papers, and who sawed off all the unimportant pieces and just taught us the bits that mattered; even conformal mapping got short shrift for being a trivial trick you might use once or twice in an E&M course, but he still taught it well enough I can do it to this day. Only 4 people in the class, and only 2 were serious, so it was practically a personal tutorial. Gave me a taste for what would be possible in a physics madrassa.


In a previous lifetime, I was a PhD student working in computational molecular biophysics. To be succinct, the general physics and modeling problem was as follows: A protein is a very complex molecular system, and as a molecule it undergoes substantial conformational changes. These are associated with its function. Using physical models, can we understand how these occur? Framed physically, we would like to sample pertinent portions of the molecular distribution function. The trouble is that even with immense supercomputing resources and physically oversimplified models, this is a tremendous challenge.


However, the geometric approach was so unintuitive and esoteric that converting an intuitive picture of the molecular dynamics into the mathematics of non-Euclidean geometry was so elusive and challenging that our competitors had to obtain their models algorithmically. Their performance wildly varied relative to ours. Often their methods would just rediscover obvious choices such as the radius of gyration.


In summary, and to be specific, geometry is a very clumsy, abstract language that is often less efficient than dynamical systems. Every time I have taken my work in that direction I have regretted it.


For some reason, people seem to shy away from matrix approaches. I am not sure why. We seem to love using tables of numbers, and while the math involved can get into fiddly realms, the basics are pretty straightforward.


Then we want all divisions to make sense. When integers are not dividable we just call the result of 3/5 a rational number even in reality this is just a pair of (3, 5) with rules how to do operations on pairs.


Then we want all square roots of positive numbers to have a meaning. So we just call sqrt(2) a new irrational number. And nobody complains that if a result of a formula in physics is sqrt(2), it is meaningless as no results of physical experiment can give that. At beast we can record a result of a measurement as an interval between two rational numbers. But properly dealing with intervals is very messy even on computers, so we continue to use sqrt(2) as a nice shorthand and floating point as its approximation even if that leads to numerical instabilities which proper accounting for intervals may often address.


Then we want a revers of a**b to always work. So we call ln(2) a transcendent number. Then we want square roots and in general any function to have a reverse. Then we call sqrt(-1) an imaginary number and the pair of (real number, imaginary number) a complex number and invent a bunch of rules how to apply common operations to such pairs.


And the relevance in physics is that one can treat (phase, amplitude) mathematically as encoding in polar coordinates of a complex number. Sp one can model with complex numbers a lot of phenomenons involving phases and amplitudes.


In the RF domain, we can look at an antenna and see the voltage climb up and down in time as the passing E-field pushes on things. In optics, the best we can do is interferometry, because we have no 10THz measuring devices. (though I may be out of date on this with all the ultra-short-pulse laser stuff)


Al termine del corso l'allievo deve aver acquisito i fondamentali concetti di relativit, fisica atomica e fisica nucleare che verranno richiamati ed utilizzati in altri insegnamenti della Laurea Magistrale in Ingegneria Nucleare.


At the end of the course the student must have acquired the fundamental concepts of relativity, atomic physics and nuclear physics that will be required and applied in other courses of the Master Degree in Nuclear Engineering.


Lezioni frontali in lingua inglese con ausilio di slide ed esercitazioni in laboratorio a gruppi o con dimostrazioni per tutti da parte del docente. Il materiale didattico disponibile sul sito di elearning del Polo di Ingegneria dell'Universit di Pisa ( ) o chiedendo direttamente al docente.


Frontal lessons in English language with slide presentations and laboratory exercises in groups or with teacher demonstration for all students. The lesson material is available on the e-learning site of the Engineering School of the University of Pisa ( ) or directly asking to the teacher.


L'insegnamento si articola sui seguenti argomenti: relativit ristretta; fisica atomica con elementi di meccanica quantistica e struttura della materia; fisica nucleare, decadimento radioattivo e sorgenti di radiazione; interazioni delle radiazioni con la materia; introduzione alla statistica; semplici esperienze di laboratorio. Gli argomenti del corso sono illustrati in dettaglio di seguito.


Relativit: basi sperimentale della teoria della relativit speciale, esperimento di Michelson-Morley, postulati della teoria della relativit speciale. Relativit della simultaneit e sincronizzazione degli orologi. Trasformazioni di Lorentz e loro conseguenze. Velocit relativistiche e trasformazioni dell'accelerazione. Dinamica relativistica ed equivalenza tra massa ed energia. Trasformazioni di Lorentz del momento angolare, dell'energia, della massa e della forza.


Fisica atomica: struttura atomica della materia, leggi dei gas perfetti e leggi fondamentali della chimica. Teoria cinetica dei gas, moto browniano, distribuzione di Maxwell-Boltzmann. Radiazione di corpo nero e ipotesi del fotone. Effetto fotoelettrico ed effetto Compton. Carica e massa dell'elettrone. Modelli atomici di Thomson e Rutherford, teoria di Bohr dell'idrogeno e degli atomi idrogenoidi. Dualit onda-particella e principio di indeterminazione di Heisenberg. Equazione di Schrdinger e sua applicazione all'atomo di idrogeno, numeri quantici, principio di esclusione di Pauli. Principio di sovrapposizione in meccanica quantistica.


Laboratorio: vari tipi di radiazioni ionizzanti, esempi di radioattivit naturale, natura probabilistica del decadimento radioattivo. Misurazione della radioattivit con un rivelatore Geiger e con un rivelatore a scintillazione, statistica di conteggio. Attivazione neutronica di indio e oro.


The course is based on the following topics: special relativity; atomic physics with elements of quantum mechanics and structure of matter; nuclear physics, radioactive decay and radiation sources; interactions of radiation with matter; introduction to statistics; simple laboratory exercises. In the following the arguments of the course are listed in more detail.


Relativity: experimental basis of the special relativity theory, experiment of Michelson-Morley, postulates of the special relativity theory. Relativity of simultaneity and clocks synchronization. Lorentz coordinate transformations and their consequences. Relativistic velocity and acceleration transformations. Relativistic dynamics and equivalence between mass and energy. Lorentz transformations of the momentum, energy, mass, and force.


Nuclear physics: Definition of a nuclear species, chart of the nuclides, isotopy and isotope separation. Radioactive decay law and natural radioactive decay chains. Properties of atomic nuclei, nuclear models, formula of Weizscker, energy levels of the nucleus. Alpha decay, beta decay, gamma decay. Nuclear reactions and artificial radioactivity. Nuclear fission, neutron interactions with matter, neutron sources and neutron cross sections. Interaction of electromagnetic radiation and charged particles with matter. Short description of fission nuclear power plants. Introduction to statistics.


Laboratory: Different types of ionizing radiations, examples of natural radioactivity, probabilistic character of the radioactive decay. Measurement of the radioactivity with a Geiger and scintillator detector, counting statistics. Neutron activation of indium and gold.

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