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From Plancks Constant to Qu Quant antum Mec um Mechanics hanics Mat atteo eo M Mas ascolo olo Dont be afraid ... ... you are in good company ! I think I can safely say that nobody understands quantum mechanics (R. P.


  1. From Planck’s Constant to Qu Quant antum Mec um Mechanics hanics Mat atteo eo M Mas ascolo olo

  2. Don’t be afraid ... ... you are in good company ! “I think I can safely say that nobody understands quantum mechanics “ (R. P. FEYNMAN)

  3. If you don’t understand QM ...

  4. Let’s start from the very beginning Physics before Galileo Galiei (1622). According to Aristotele.... A constant force produces a uniform motion F = F = m v m v The speed of a body in vacuum is infinity

  5. Something thing is evid vident ently ly wr wrong ng

  6. No way ay to un understand derstand it t !! !! Two easy observations can show the lacks of Aristotelian mechanics It hardly explains how an arrow keeps on 1) flying after being shot (Aristotele tried with the theories of “natural places” and the “horror vacui” ) Trajectories can be easily disproved 2) through a simple experiment (throwing an arrow and looking its motion!!)

  7. Ar Aris istotel elia ian n physi ysics cs is is WR WRONG! G!

  8. One ne mo more re easy asy thi hing ng .. ... SCIENTIFIC METHOD (1622) - Observation of phenomenon - Hypothesis and prediction - Experiment - Write a law using the “ language of mathematics ” - Falsifiability of the law - Prediction capabilities

  9. The best “EPIC FAIL” ever ... “ The task of physics is nearly completed. There are a few minor things left to do: measure some quantities with higer precision and find a theoretical justification for the emission and absoprtion spectra , the photoelectric effect and the black body radiation ...” 18 1874 74 1643-1727 1831-1879

  10. Bu But . ... we we kn knowk wk wh what ca came aft fter r !

  11. Than han the he questi uestions ons are are: • Is classical mechanics as wrong as Aristotelian mechanics? • How can classical mechanics, relativity, and quantum mechanics to reconcile? Every theory has its own scope of validity, one has to know its limits! For example, how is the atom made?

  12. The he Thomson homson mo model el Also kwown as ‘ Plum Pudding ’ model “The atoms […] consist of a number of negatively electrified corpuscles enclosed in a sphere of uniform positive electrification…” [J.J. Thomson]

  13. The he limits imits of Thomson homson mo model del • The electron is the only charged particle having mass, thus every atom should contain a very huge number of particles • It does not explain the different attitude of chemical elements to ionize and combine together • It does not explain absorption and emission lines of elements • It does not explain the results coming from scattering experiments 3 out of 4 points solved by the Thomson’s pupil : prof . ‘Crocodile’

  14. The e Ge Geige iger-Ma Marsde rsden n exp xper erim iment ent (aka a the e Ruthe herf rfor ord d exper perimen iment t ) a -particles (nuclei of Helium) on a thin foil of gold : scattering effects were evaluated ‘’by eye’’, working in absolute dark and assuming drugs that dilated the pupila

  15. Tho homson mson vs vs Ru Ruthe herford rford THOMSON ATOM RUTHERFORD ATOM

  16. Ru Rutherfor rford d mode deli ling ng of t f the atomù (Nob Nobel l Prize ze 1908) 08) Negatively-charged electrons orbit around a positively charged nucleus (no neutrons yet!)

  17. Ho How big ig is s an an atom tom ?? ?? 1 1 q q     2 1 2 E T V mv  2 4 r 0 The total energy is the kinetic energy of the α -particle T plus the Coulomb-energy V due to the repulsion between charges of the same sign. When the particle turns back T = V . 1 q 1 q 2 T  4  0 r 1 q 1 q 2 r  4  0 T ฀

  18. Ho How big ig is s an an atom tom ?? ?? Z a Z Au e 2 1 r  4  0 T Given the elementary charge e , the dielectric constant of vacuum ε 0 and the kinetic energy T   2 ฀ 1 z z e e  1.6  10  19 C  a Au r =  4 T  0  8.85  10 -12 m -3 kg -1 s 4 A 2 0 T  5 MeV  5  10 6  1.6  10  19 J    - 15 45.5 10 m 4 5 . 5 fm At that time, the radius of the atom of gold was well ฀ known: 150’000 fm. It is 3000 times larger!

  19. 3000 00 times larger it’s a lot !!!

  20. A A new ew mo model del of f the he atom tom “ It was quite the most incredible event that has ever happened to me in my life. It was almost as if you fired a 15-inch shell into a piece of tissue paper and it came back and hit you […] [ … ] this scattering backward must be the result of a single collision, and when I made calculations I saw that it was impossible to get anything of that order of magnitude unless you took a system in which the greater part of the mass of the atom was concentrated in a minute nucleus. It was then that I had the idea of an atom with a minute massive center, carrying a charge. “ [E. Rutherford]

  21. The he limits imits of the he Ru Ruthe herford rford mo model del 1. Electrons are charges in motion and they should lose energy by emitting radiation (Maxwell - Hertz “The great tragedy of Science: the 1888) slaying of a beautiful hypothesis by an ugly fact” They should fall on the nucleus in 10 -10 seconds 2. [T. Huxley] 3. The puzzle of spectral lines is still unsolved !

  22. The he emission mission of radi radiation ation • Every object at a given temperature emits energy in the form of electromagnetic radiation (the common “heat”) • An object emits radiation at all the wavelengths ( l ), but the distribution of the emitted energy as a function of l changes with the temperature ( T ).

  23. So Some e emis mission sion spec pectra tra

  24. The “Black Body” • A body is composed of many oscillating charges. The oscillations increase if temperature T increases • Oscillating charge emit radiation and slow down. That is how bodies cool down • All bodies at equilibrium have emissivity equal to absorption e = a for every value of T and l • A body at high temperature T that absorb all the energy that is able to emit (at equilibrium) e = a = 1 is called a “ black body” (it radiates not reflects radiation, that’s why it was called a black body!)

  25. Why the “Black Body” question?? The answer is absolutely disappointing: TRIVIAL INDUSTRIAL NEEDS (i.e. measure very the very high temperature of devices from their luminosity!) ns mens Sieme W. Si W.

  26. Why hy physicists hysicists ?? ?? The spectrum of a hot body was already measurable with very high precision, but there was no way to connect it with theoretical predictions !!! W. Herschel (1800)

  27. Ki Kirchhof rchhoff f and and the he black lack body dy A black body is a cavity (e.g. an oven) with a tiny hole, kept at a constant temperature The radiation entering the black body is reflected by the inner walls a huge number of times before getting out

  28. The he black lack body dy spectrum pectrum All black bodies at the same temperature emit thermal radiation with the same spectrum (regardless of shape, dimensions and material) From spectra observation: l max T = constant Wien’s law M tot a T 4 Stefan (1879) From theoretical calculation: M tot  s T 4 Boltzmann (1879)

  29. The black body “puzzle” The flux of the radiation within the cavity in every direction is zero, but there is energy transfer everywhere This transfer is given by the density of radiated energy in the wavelength range ( l , l +d l ) : Y l d l ( Y l  is also called emission power )  The calculation of Y l  giving the shape of expected experimental spectrum, was very difficult from th theoretical point of view C  l  Firs rst t Attempt tempt ... by by Wi Wien l 5 e C '/ l T First “empirical” forumla (similar to Maxwell velocity distribution) ฀

  30. The black body “puzzle” Wien’s Y l does not work! It fits data at low l not at high l . Constants C e C’ are completely arbitrary!  l  8  Second Se nd Attempt tempt ... l 4 kT by by R Rayleigh leigh-Je Jeans ans Model with stationary waves inside the cavity. The energy density is evaluated as the density of modes with mean kinetic energy kT ฀ It does not work! It fits data only at high l . Smaller is l greater is the number of possible stationary waves! But everything was calculated correctly…

  31. The “ultraviolet catastrophe”  l  8  l 4 kT ฀ • Wien: empirical formula, correct only for small values of l AN AND NOW OW?!?!  • Rayleigh-Jeans: consistent formula, correct for big l

  32. Sp Spectroscopy ctroscopy at t that hat time ime .. ... H. Kayser (5000 spectra!) H. Rubens “A triumph of observation, in a theoretical desert!” [Unknown]

  33. PLanck’s lucky solution OCTOBER 1900 Max Planck solves the puzzle of the spectrum of black body radiation. With a new empirical formula: C  l  l 5 ( e C '/ l T  1) • What are the constants C and C’ !?  • It works for every value of l! ฀ Yeah bu but ... WH WHY?!?! !?! 1858-1947

  34. PLanck’s lucky solution C  l  l 5 ( e C '/ l T  1) ฀ The agreement with Rubens’ experimental data is striking . Nevertheless Planck can’t find a physical explanation...

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