Chapter 3 Why Properties Change on the Nanoscale: An Introduction to Nanoscale Physics NANO 101 Introduction to Nanotechnology 1 The Original Physics • Classical physics • Largely developed by Isaac Newton (late 1600s) • Action = reaction • Still relevant to our world today • Doesn’t explain observations of atoms, molecules, subatomic particles…. 2 http://www.colsterworth.lincs.sch.uk/_includes/images/design/home/footer_newton.jpg Quantum Mechanics “I think I can safely say that nobody understands quantum mechanics” - Richard Feynman, The Character of Physical Law (1965) “For those who are not shocked when they first come across quantum theory cannot possibly have understood it.” - Nils Bohr 3 Quantum Mechanics • Explains phenomena not explained by Classical Mechanics (early 1900s) • Based on probability and statistics • Correspondence Principle – not one or the other Components: • • • • • Electromagnetic Waves Photoelectric Effect Atomic Orbitals Wave-Particle Duality Uncertainty Principle 4 Electromagnetic Radiation • Speed of light = 3.0 x 108 m/s = 670 million mph • Frequency (f): number of cycles/second (s-1 = Hz) • Wavelength (): • distance between 2 identical spots on wave • crest to crest c wavelength f c 5 http://www.andor.com/library/ 6 Light is a Wave Waves can interfere constructively or destructively Double slit experiment shows wave like nature 7 Photoelectric Effect e- e- e- e- e- • Light as a wave: – Energy of emitted electrons should be proportional to intensity of incident light – An electron should be emitted eventually if light of a low frequency is shone at a high intensity for a long period of time – There should be a lag time associated with lights of lower frequency 8 Photoelectric Effect e- e- e- e- e- • Einstein - Light as a particle: – Energy of light is proportion to its frequency – Light of a lower frequency will never have enough energy to eject an electron – Increasing intensity increases amount of electrons ejected but not their energy – No lag time associated with transfer of energy from particle to electron 9 Light is a Particle: Photons Light “particles” Discrete (not continuous) fixed quantity bundles of energy E photon hf h Planck' s constant 6.626 10 34 J s What is the E of one photon of microwave radiation with a wavelength of 1.20 cm? c f c C = 3 x 108 m/s 10 The Double Slit Experiment 11 Wavelength of an Electron h mv h = 6.626 x 10-34 J s m = mass v = velocity What is the wavelength of : Usain Bolt (m = 94 kg) running the 100 meter dash at avg speed of 25 mph 1 mile = 1.61 km An electron (m = 9.1x10-31 kg) in a TEM accelerated at 3 x 108 m/s 12 Heisenberg Uncertainty Principle Impossible to know exact position and momentum of a particle at same time h x mu 4 ∆x: uncertainty in position m: mass ∆u: uncertainty in speed h: Planck’s constant Why can we be certain about larger particles (i.e. baseball)? 13 Heisenberg Uncertainty Principle 14 h x mu 4 • A radar gun measures Felix Hernandez’s fastball at 94 mph ± 0.1 mph, what is the uncertainty in position? – A baseball weights ~ 145 g – 1 mile = 1.61 km • What is the uncertainty in position of one of the electrons that make up the baseball? – An electron weight 9.1 x 10-31 kg 15 • Reminder: HW#2: 2.1, 3.8, 3.10abd, 3.20, 3.21 • Electrons have particle and wave like properties • Atoms are the building blocks - > Chemistry and Nanotechnology 16 Models of the Atom J.J. Thomson Rutherford Proton Neutron Current model Electron Charge Mass (kg) Location ~1.673*10-27 ~1.675*10-27 ~9.11*10-31 nucleus nucleus “clouds” 17 Schrodinger Equation • Electrons as standing waves 18 Where are electrons? • Cloud around nucleus • Each e- is associated with a specific energy • Always some uncertainty Atomic Orbital: • volume of space where an e- is most likely to be found • each orbital can hold a maximum of 2 e• orbitals closer to the nucleus have lower energy 19 Quantum Numbers Each atomic orbital can be described by three numbers: (n, l, ml) 1. Principal quantum number (n) • Energy level, shells • Probable distance from nucleus 2. Angular momentum quantum number (l) • • Subshells, sublevels Shape 3. Magnetic quantum number (ml) • Orientation 20 Orbital Shapes p orbitals s orbitals http://www.800mainstreet.com/33/0003-004b-location-electron.htm http://library.tedankara.k12.tr/chemistry/vol3/Wave%20 functions%20 and%20probability%20distributions/z51.htm 21 More Orbital Shapes d orbitals f orbitals http://int.ch.liv.ac.uk/Lanthanide/Ln_Chemistry_folder/ Miscellaneous%20folder/Miscellaneous.html#f_orbitals http://www.geo.arizona.edu/xtal/geos306/fall06-1.htm 22 Quantization of Energy Atoms can only contain certain amount of energy (discrete values – not continuous) White light is a continuous spectrum 23 Quantization of Energy Atoms can only contain certain amount of energy (discrete values – not continuous) E nhf Electrons in an atom move between energy states 24 Quantization of Energy Atoms can only contain certain amount of energy (discrete values – not continuous) E nhf Electrons in an atom move between energy states 25 26 Chapter 3 Overview • Electrons in atoms are found in orbitals. • Each orbital has an energy level and sublevel (shape) • The closest energy level to the nucleus is the ground state; higher levels are excited states • Electrons can act like particles or waves (double-slit expt) • Radiation can act like energy or waves (photoelectric effect; photons are packets of light energy) • Atoms emit or absorb photons when their electrons change energy levels • The Uncertainty Principle states that the more you know an object’s position, the less you know its momentum (and visa versa). 27 Langmuir Film/Self Assembled Monolayer 28 Langmuir-Blodgett Technique 29 Fatty Acids Lauric acid Stearic acid Pentadecanoic acid 30 Lycopodium Powder -Very hydrophobic -Help to see the monolayer -Very fine powder Primary use of lycopodium powder (not in this lab) 31 For Thursday • No food or drink in lab • Bring a print out of lab sheet • Record all significant figures from measurements • Potential for lab based question on quiz 32