4Forces that win at the macroscale aren’t as important at the nanoscale.
5When you tip a normal-sized teacup, why does the water pour out? Gravity!When you tip a tiny teacup, why doesn’t the water pour out?Properties of water like adhesion, cohesion, polarity & surface tension “defeat” gravity in the miniature version.
7When you throw a ball there are competing forces When you throw a ball there are competing forces. Drag forces are proportional to surface area while inertia, which is proportional to volume, resists changes in velocity. How quickly an object slows down (its deceleration) is given simply by the ratio of the drag force to the inertia (mass).Deceleration = Drag force/Inertia = (C x Surface Area x Velocity)/(Density x Volume)C is a coefficient that depends on the fluid the object is moving through (so it would be the same for both styrofoam balls), we’re assuming the initial velocity & density are the same for both also.Styrofoam has the correct density where we can observe a crossover of the dominance of inertia (for the larger ball) to the dominance of viscous drag (air resistance) for the smaller ball.
8The four important changes at the nanoscale… Gravitational forces become negligible & electromagnetic forces dominate (+ & - charges)Quantum mechanics is used to describe motion rather than classical mechanicsSurface area to volume ratio increasesRandom molecular motion becomes more important
10The Original PhysicsClassical physicsLargely developed by Isaac Newton (late 1600s)Action = reactionStill relevant to our world todayDoesn’t explain observations of atoms, molecules, subatomic particles….
11The Blackbody Radiation Problem In the late 1800s, scientists were unable to use classical physics to explain blackbody radiation (the radiation emitted by solid bodies once they’d been heated).
12The scientist who started to redefine physics… Max Planck was able to explain blackbody radiation with his famous equation:E = hfEnergy is discharged in small packets called quanta. (Before this, physicists believed energy could be discharged in any amount, it was continuous).
13Quantum Mechanics was born! Explains phenomena not explained by Classical Mechanics (early 1900s)Based on probability and statisticsComponents:Electromagnetic WavesPhotoelectric EffectAtomic OrbitalsWave-Particle DualityUncertainty PrincipleQuantization of Energy(Atomic Spectra)
14Electromagnetic Radiation Speed of light = 3.0 x 108 m/s = 670 million mphFrequency (f): number of cycles/secondWavelength ():distance between 2 identical spots on wavecrest to crestwavelength
16Review:Which has more energy—a red wavelength of light or a blue wavelength of light?Answer: Blue!
17Photoelectric Effecte-e-There is a minimum frequency of radiation required for current to flowIt is not based on intensity (ex: it doesn’t matter how much red light you shine on the metal, it still isn’t going to knock electrons off).Current flows when light hits; no time lagThe # of e- emitted depends on intensityPhotons: packets of light energy
18Photoelectric Effect Applications… Digital cameras Night vision Solar cells
19Where are electrons? Atomic Orbital: Cloud around nucleus Each electron is associated with a specific energyAlways some uncertaintyAtomic Orbital:Volume of space where an e- is most likely to be foundEach orbital can hold a maximum of 2 electrons
20Energy States Ground state: lowest E level Excited states: higher E levelsPhoton emitted:e- drops down to lower E statePhoton absorbed:e- jumps up to higher E state
21Atomic SpectraElectrons of gas atoms jump up energy levels (are “excited”) when you put energy in2. Excited electrons drop down to the “ground” stateThe amount of energy lost is equal to the energy of light emitted
22The Double Slit Experiment Waves bend around edges and slitsconstructive interference“in phase”destructive interference“out of phase”
23The Double Slit Experiment Particles do not bend around edges and slitsWhat about electrons? Are they particles?Let’s ask Dr. Quantum….
24Heisenberg Uncertainty Principle Impossible to know exact position and momentum of a particle at same time∆x: uncertainty in positionm: mass∆u: uncertainty in speedh: Planck’s constantMore accurately know position?Why can we be certain about larger particles(i.e. baseball)?
25Overview 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 statesElectrons 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 levelsThe Uncertainty Principle states that the more you know an object’s position, the less you know its momentum (and visa versa).
26SummaryThe laws of physics that are most important to a particular system depend on the size of that system.At the nanoscale, almost all interactions are mediated by surface effects. So forces between objects are often proportional to their surface area.This is why surface-related forces that bond molecules and nano-objects together—such as chemical and intermolecular bonds—are so much more important than gravity!The surface area to volume is dramatically higher—up to a billion times higher—for nano-objects than for human-scale objects (so surface-related effects dominate).