Six Easy Pieces

Essentials of Physics Explained by Its Most Brilliant Teacher (Richard P. Feynman)

Bold = new section

Italic = particularly interesting term or phrase

Underline = important vocabulary

Links are included throughout. I have purposefully varied the sources and the format (text, image, audio, video) so that my own notes are not only expanded on, but enriched! The links won’t simply take you to wiki pages that explain concepts by enlisting a wall of words. Instead, I attempted to synthesize different sources that really stretch outside the realm of basic physics and diversify the learning. Partially to aid myself, having a brain that sometimes operates quite slowly and on an elementary level, and also in honor of Feynman himself, most of these sources are far from “academic” or “scholarly”, and might be thought of as childish. I think these types of resources can often be the most illuminating. If you can’t distill something to simpler terms, I would argue you don’t understand it well at all, so why not start learning from the very fundamentals.


Intro

  • Popular misconception that science is an impersonal, dispassionate, and thoroughly objective enterprise

  • The scientific experience and its vast processes are diminished to a result, results are all that count, and the people that produce them are also too often overlooked

  • Science is people-driven (arguably more so than anything else?)

  • Are there not scientific trends and problems that characterize a specific age, just as something like fashion?

  • QED can mean quod erat demonstratum and be placed at the end of a mathematical proof, but it can also mean quantum electrodynamics

  • Quantum theory began with Max Planck in 1900 when the German physicist proposed that light and other electromagnetic radiation behaved like tiny packets of energy known as “quanta”. Prior, light had been regarded as waves

  • These quanta became photons

  • By the early 1930s quantum mechanics had created a mathematical model to describe the emission and absorption of photos by electrically charged particles such as electrons

  • Feynman turned his attention to perfecting the QED Theory; it still suffered from inconsistencies and calculations were known to give strange or infinite answers to reasonable physical questions

  • Making QED a sound theory required 

    1. Consistency with principles of quantum mechanics

    2. Consistency with principles of the theory of relativity 

  • Feynman took a unique and intuitive approach by creating his very own system of diagrams

  • Feynman diagrams are symbolic but powerful way of picturing the interactions between electrons, photons, and other particles

  • Most theoretical physicists rely on careful mathematical calculation to provide a guide into unfamiliar territory. With this in mind, Feynman comes off as cavalier and struts about seemingly reading nature like a book 

  • Feynman displayed a “healthy contempt for rigorous formalisms”

  • Theoretical physics = one of the toughest intellectual exercises… combining abstract concepts that sometimes can’t even be visualized with extreme mathematical complexity?? No thank you

  • Apparently, Feynman was a lifelong prankster who treated authority and academic establishment with the same sort of disrespect he showed for mathematical formalism

  • Particularly Feynman hated “Why” questions 

  • Fun side fascination with the quirky and obscure? Feynman had an obsession with the long-lost country of Tuva in Central Asia which he made a documentary on near his death (he also played, bongo drums, painted, frequented strip clubs, and deciphered Mayan texts)

We love you Dick
  • When he died of cancer in 1988 his students at Caltech made him a banner: “We love you Dick.”

  • Upon being convinced to teach a series of freshmen lectures on physics, they were preserved in book form as The Feynman Lectures on Physics and proved a smashing success around the world

  • Perfect for the less mathematically or physically minded, Feynman is known for his ability to find just the right analogy or everyday illustration to extract the essence of a deep principle

  • Physics is rooted in the notion of laws = the existence of an ordered universe that can be understood by the application of rational reasoning 

  • Laws of physics are not immediately transparent to us in our direct observation of nature

  • Feynman holds the considerable distinction of being one of the few to discover a new law of physics, one that pertains to the way that a weak nuclear force affects the behavior of certain subatomic particles

  • High-energy particle physics was the jewel in the crown of post-war science

  • This physics was glamorous and awesome with huge accelerator machines (check out CERN) and seemingly unending list of newly discovered subatomic particles

  • What unifies particle physicists? The role of symmetry and conservation laws

    1. Symmetry of time: nothing in physics to distinguish one moment of time from the next. The world is “invariant under time translations” because regardless of your starting point (t=0 moment) there is no difference in the description of physical phenomena

      1. The symmetry of time directly implies the most basic laws of physics: The Law of Conservation of Energy = you can move energy around and change its form but it is never created or destroyed

  • Quantum physics has dominated the 20th century

  • The above is indispensable in understanding subatomic particles, atoms, nuclei, molecules, and chemical bonding, the structure of solids, superconductors and superfluids, the electrical and thermal conductivity of metals and semiconductors, the structure of stars, shall I continue??? 

  • “Anybody who is not shocked by the [quantum] theory hasn’t understood it” – Niels Bohr, one of its founders

  • To mess with your brain: an electron cannot have a position in space and a well-defined speed at the same moment

    1. CAN look for the location of an electron and find it

    2. CAN measure its speed and obtain an answer

    3. CANNOT make both observations at once

  • This indeterminism in the nature of atomic particles is encapsulated by Heisenberg’s uncertainty principle 

  • The famous “two-slit” experiment teases out the wave-particle duality 

  • Much easier to imagine an electron traveling directly from A to B, however, in reality it can take an infinite variety of routes and without observing which path is taken, we have to suppose that all possibilities contribute to the arrival point

  • Feynman’s “path-integral” or “sum-over-histories” approach to quantum mechanics

particle comparison
  • “There are 10^11 stars in the galaxy. That used to be a huge number. But that is only a hundred billion… we used to call them astronomical numbers. Now we should call them economical numbers.” – Feynman

  • Feynman scribbled a note to himself in Brazil in 1952: “first figure out why you want the students to learn the subject and what you want them to know, and the method will result more or less by common sense.” – I don’t know about you, but that makes me want to ask my professors and teachers a singular question, not meant with any hostility, but simply curiosity: “why do you want me to know this?”

  • IF you can’t reduce an idea to something more simple THEN you don’t really understand it


Feynman’s Preface

  • “Special problem” of his lectures was to maintain interest of the enthusiastic and smarter high school students entering Caltech

  • Just a side note: stultifying = to cause the loss of enthusiasm and initiative, especially as a result of a tedious or restrictive routine (AKA most high school physics classes)

  • Assumed knowledge of his lectures: geometrical optics and simple chemistry

  • All lectures were given without ever receiving any feedback from the students

  • Solutions to the diffusion equation

  • In more complex applications of quantum mechanics, such as electrical engineering and chemistry, the full machinery of the differential equation approach is not actually used

  • Energy bands = ranges of electron energy in a solid that that are so dense they appear to be continuous 

  • “The power of instruction is seldom of much efficiency except in those happy dispositions where it is almost superfluous.” *superfluous = unnecessary, or being more than enough

  • The best teaching can be done only when there is a direct individual relationship between a student and a good teacher


1: Atoms in Motion

  • Physicists must accept that despite the 200 year accumulation of knowledge and laws, we do not yet know all of them, and there is an expanding frontier of ignorance surrounding physics

  • The correct statement of the laws of physics involves some very unfamiliar ideas which require advanced mathematics for their description; this requires immense amounts of preparatory training to learn what some laws and words even mean.

  • With an echo of Socrates, we know that we do not know all the laws of physics, so everything we know is only some sort of approximation

  • The principle of science = the test of all knowledge is experiment

  • Believe it or not, imagination is also needed to create accurate generalizations from the hints experiments allow us

  • Division of labor in physics 

    1. Theoretical physicists: imagine, deduce, guess at new laws but do not experiment

    2. Experimental physicists: experiment, imagine, deduce, and guess

  • The “law” that mass is constant is actually inaccurate! Mass is found to increase with velocity, but appreciable increases require velocities near the speed of light. So yes, for ordinary speeds we can approximate mass to be constant, but it is not always true

  • WHAT is our overall picture of the world? Matter is made of atoms

  • The atomic hypothesis or atomic fact = all things are made of atoms – little particles that move around in perpetual motion, attracting each other when they are at a distance but repelling each other upon being squeezed together

  • Atoms in a water molecule are 2x10^-8cm in radius (this is an angstrom)

  • The “jiggling motion” of particles in an object is what we represent as heat and as heat increases, the jiggling increases

  • As demonstrated by classic textbook diagrams of a chamber with piston: when we compress a gas slowly, the temperature of the gas increases

  • In a solid material such as ice, there is a definite place for every atom. This special atomic arrangement in a solid is called a crystalline array

  • Most simple substances – with the exception of water and type metal – EXPAND upon melting because closely packed atoms separate, but an opened structure collapses in the case of water

  • As we decrease temperature, atoms approach a minimum amount of vibration at absolute zero but NOT this ≠ zero 

  • Helium is special, it decreases its atomic motion as much as it can but at absolute zero there is still enough motion to keep it from freezing (unless the pressure is increased to make it solidify) 

  • What happens at the surface of water?

    1. There is always water vapor to be above liquid water

    2. Air consists almost entirely of nitrogen, oxygen, some water vapor, and lesser amounts of carbon dioxide, argon, and other things

    3. Molecules just above the surface of water interact with the liquid water and certain amounts are knocked with enough energy to evaporate

    4. At the same time, some molecules from the vapor in the air stick to the water molecules in the liquid state and condense

    5. Water molecules evaporate because they have more energy than the average, so the ones left have LESS average motion than before. In this way, the liquid also gradually cools if it evaporates

VLE
    1. This process is complicated by stray oxygen or nitrogen molecules which work their way into the process of evaporation. When this occurs, the “air” dissolves into the water and if suddenly all of the air is taken away, they will leave more rapidly than they entered and will make bubbles in the process. This is what is so dangerous for divers!

  • What happens when you dissolve a solid in water?

    1. Take salt (sodium chloride, NaCl) made of ions 

    2. An anion has a negative charge, meaning it has a few extra electrons

    3. A cation has a positive charge, meaning it has lost a few electrons

    4. Water is a polar molecule, meaning different parts have a partially positive or partially negative charge

    5. Na+ and Cl- are then attracted to O2- and H+ ions in water respectively

    6. This results in another dynamic process that is undetectable in diagrams: salt is dissolving in water as it also crystallizes out

    7. More on the chemistry of solution and precipitation – can be complicated to predict which way a reaction will go, depends on the forward and backward reaction rate, and is also subject to the temperature and pressure at the point of the reaction

  • What about when atoms and ions “change partners?”

    1. Atomic rearrangement = a chemical reaction (DISTINCT FROM A PHYSICAL REACTION)

    2. Especially in reactions where large amounts of energy – kinetic energy – is generated, heat can produced from the combination of two atoms and result in burning 

    3. Heat is usually in the form of the molecular motion of the “hot” gas, but sometimes its magnitude generates light which is where our flames come from

    4. Chemists can conclude that every substance is some unique arrangement of atoms

    5. An interesting thought: we smell because a special molecule jostles along into our nose. Chemists can take these molecules (like the odor of a flower) and analyze them to determine the exact arrangement of atoms in space

    6. We cannot picture all that is known about chemical arrangements, because atoms combine in three dimensions while we can only diagram two

    7. Organic chemistry is the finest detective work ever done

  • Brownian motion = the perpetual jiggling of atomic particles

  • A key hypothesis: everything is made of atoms

  • So what follows: everything that animals do, atoms do.

  • This means: there is nothing that living things do that cannot be understood from the point of view that they are made of atoms acting according to the laws of physics


2: Basic Physics

  • Take a moment to appreciate everything occurring around you, as you enjoy (or not) these notes. As the observer you comprehend the words on this screen, this computer is extremely recent, an impressive addition, in the history of everything we know. Wherever you are there is air that you are breathing, of varying levels of moistness depending on where you are in the world. Even these few lines of writing, I have encapsulated more science and physics especially than you could begin to fully understand in a lifetime

  • A question Feynman asks: What common features do different movements have?

  • If we begin to gradually analyze things, we can hope to put together what at first appears different and thus reduce the number of different things thereby understanding them better

  • Scientific method = observation, reason, and experiment

  • What does it mean to understand something?

  • If “the world” (or at least what we believe to constitute it) is a chess game being played by the gods and we are only ever able to watch, maybe catching on to some of the rules along the way, than these rules of the game = fundamental physics

  • At first nature’s phenomena were roughly divided into classes ie heat, electricity, mechanics, magnetism, properties of substances, chemical reactions, light or optics, x-rays, nuclear physics, gravitation, meson phenomena, etc

  • Now the aim is to see complete nature as one set of phenomena

  • The basic problem in theoretical physics: find the laws behind the experiment and amalgamate these classes

  • Constant process of amalgamating a bit and then something new pops up

  • Example: heat and mechanics. Atoms that have more motion mean their system contains more heat, so heat and temperature effects can be represented by the laws of mechanics

  • Amalgamation = the act of unifying into one organization or structure

  • The simplest question becomes what are things made of and how few elements are there?

  • BEFORE 1920: 

    1. The world is a 3D geometrical space as described by Euclid

    2. Things change in a medium called time

    3. The elements on the stage are called particles (atoms for example and some have properties)

    4. Inertia, forces – of molecular attraction (due to charge!) and gravitation

      1. In the short-range, gravity is entirely too weak to impact particle level forces

      2. Electrical force attracts and repels

    1. All matter is a myriad of particles 

    2. Pressure comes from the collision of atoms 

    3. Random internal motions are heat

    4. Waves of excess density are sound

    5. There are 92* different kinds of atoms

*at the time of his lecture, now there are 118 unique atoms on the periodic table (pure elements), however, only 109 are stable.

    1. Atoms contain a positive nucleus at the center which is surrounded by a certain number of electrons which are very light and negatively charged

    2. The nucleus is composed of two kinds of particles: protons and neutrons (nearly the same weight and very heavy) 

    3. Protons are electrically charged while neutrons are neutral

    4. Chemical properties depend on how many electrons are on the outside of the atom

    5. Number of electrons = number of element = number on periodic table

    6. The symbolic nomenclature of elements on the periodic table exists for human convenience 

    7. Complicating the description of electrical forces: the existence of a positive charge creates a condition in space so that when a negative charge is introduced, it feels a force. This is the electric field

    8. The rules of an electric field: 

      1. Charges make a field

      2. Charges in a field have forces on them and move

    1. Electrical fields are complicated by magnetism (having to do with charges in relative motion)

    2. Concepts of local and direct interaction

    3. The concept of the electromagnetic field : carries waves, some waves are light, some are used in radio broadcasts, the general name for all = electromagnetic waves

    4. Oscillatory in nature with various frequencies

    5. Waves are distinctive due to their frequency of oscillation

    6. The usual “pickup” that we get from electric currents in the circuits in the walls of a building has a frequency of ~ 100 cycles per second

  • AFTER 1920/QUANTUM PHYSICS:

    1. At higher frequencies these waves behave more like particles (this behavior is explained by quantum mechanics)

    2. Einstein created a the combination space-time to represent gravitation. It is curved

    3. He changed the rules of particle motion: Newton’s laws of classical mechanics are wrong!

    4. DISCLAIMER: things on a small scale act nothing like things on a large scale

    5. Physics is difficult because human’s have no experience with the way things behave on a small scale – it is unnatural to us and we can only describe it analytically. Ironically, this takes lots of imagination

    6. A particle cannot have a definite location and a definite speed in quantum mechanics

    7. The uncertainty of momentum and the uncertainty of the position are complementary (the product of the two is bounded by a small constant, and written with a law like this: 𝛥x𝛥p ≥ h/2)

    8. Why are atoms so big? How is the nucleus so small in comparison, yet accounts for nearly all the weight of the atom?

    1. Using the uncertainty principle: IF all of the electrons were in the nucleus, we would know their position, but they must have a very large momentum, or kinetic energy which allows them to break away from the nucleus

  1. Quantum mechanics also incited interesting changes in the the ideas and philosophy of science: it is impossible to predict exactly what will happen in any circumstance

  2. Nature’s beauty and horror derives from the fact that it is fundamentally impossible to predict exactly what will happen in any given experiment despite following requisite conditions

  3. Quantum mechanics unifies the idea of the field and its waves, and the particles

  4. When the frequency is low, the field aspect is more evident and a more useful approximate description

  5. When the frequency increases, the particle aspects become more evident

  6. This gives us a new view of electromagnetic interaction and thus a new particle in addition to the electron, proton, and neutron! The photon!

  7. Quantum-mechanically correct relationship between the electrons & photos is called quantum electrodynamics

  8. QED = the fundamental theory of the interaction of light and matter or electrical fields and charges AKA the greatest success so far in physics. The following are all examples of this new law in action: 

    1. Collision of billiard balls

    2. Motions of wires in magnetic fields

    3. Specific heat of carbon monoxide

    4. The color of neon signs

    5. The density of salt

    6. Reaction of hydrogen and oxygen to create water

  1. Consequence of quantum mechanics as it relates to fundamental physics: waves behave like particles and particles behave like waves, there is no distinction between a particle and a wave

  2. QED = the theory of all chemistry and of life (if life is reduced to chemistry and therefore to physics) 

  3. QED also predicts a lot of new things: 

    1. positron, or a particle with the same mass as an electron but of opposite charge. When the two come together they could annihilate each other with the emission of light or gamma rays

    2. For each particle there is an antiparticle

    3. Two numbers are put in and most of the other numbers in the world are supposed to come out (two numbers are the mass of the electron and the charge of the electron) BUT what about the atomic number? AKA how heavy the nuclei are, which is a number on the periodic table

  • Nuclei and Particles: 

  1. Enormous forces hold the nuclei together

  2. When released the energy is HUGE compared to the chemical energy (think of an atomic bomb compared to a TNT explosion: the atomic bomb has to do with changes in the nucleus while TNT explosion has to do with the changes of electrons on the outside of the nucleus)

  3. What forces hold the protons and neutrons together in the nucleus?

    • A field of sorts, when it “jiggles” it behaves like a particle

periodic table
    • Suggests that other particles exist: cosmic rays, muon, pion, 

    • Theory of quantum nucleodynamics is so difficult and complex that no one can work it out and it is left incomplete

  • There are about thirty particles that exist to our knowledge

  • Our inability to connect and understand their relationships with each other represents the amount of unconnected information we have without a good theory

  • QED = lots of knowledge but lots of uncertainty

  • Filling out the Mendeléev chart, and seeking a similar one for new particles

elementary particles
  • Chart of new particles made by Gell-Mann in the USA and in Nishijima, Japan. Basis of their classification is a new number, similar to the electrical charge, that is assigned to each particle called its “strangeness”, S

  • Historical choice: One Mev = 1.782 x 10⁻²⁷ gram

  • Elementary particles

  • What is zero mass? A particle with zero mass cannot be at rest

  • Although there are several different particles, there are four kinds of interactions between them:

    1. Nuclear force (strongest) = between two or more nucleons, for example this force binds together the protons and the neutrons in atomic nuclei

    2. Electrical interactions

    3. The beta-decay interaction

    4. Gravity (weakest)

  • To summarize: outside the nucleus our knowledge of physics seems quite expansive. Inside the nucleus, the principles of quantum mechanics have not been found to fail, but there is much much more we do not know

  • We base all of our knowledge on the premise of relativistic space-time

  • We do not know how the universe got started 

  • There has never been an experiment made to check our ideas of space and time accurately, below a certain tiny distance, so we only really “know” our ideas work above that distance.

  • The rules of our aforementioned chess game are the quantum-mechanical principles which apply – so far as we know – to new particles and old particles

  • Studying the origin of the forces in the nuclei lead us to new particles, but they appear in great profusion (large quantity or abundance) and we don’t have a complete understanding of their interrelationships

  • We are progressing towards an understanding of subatomic particles, but slowly, and with no conception of how far there is to go  


3: The Relation of Physics to Other Sciences

  • Most fundamental and all-inclusive of the sciences

  • Present-day equivalent of what used to be called natural philosophy

  • Physics has remarkable relationships with engineering, industry, society, and war

  • Very special relationship with mathematics… not a science to us, in the sense that experiment doesn’t prove its validity, or it is not a natural science

  • Feynman wants it to be clear: just because something is not a science doesn’t mean that it is bad! His example, love is not a science

  • CHEMISTRY

    1. Arguably the most deeply affected by physics

    2. In the early days, chemistry was almost completely devoted to inorganic chemistry (not associated with living things)

    3. Because the interrelationships of elements and the rules by which substances are combined are ultimately explained by quantum mechanics, in principle, theoretical chemistry is basically physics

    4. There is a branch of physics and chemistry developed by both sciences together: statistical mechanics

    5. Statistical mechanics boils down to the science of heat or thermodynamics

    6. This reduces inorganic chemistry to physical chemistry (to study the rates at which reactions occur and what is happening in detail) & quantum chemistry (to help us understand what happens in terms of the physical laws)

    7. Then there is organic chemistry which studies all of the substances associated with living things

    8. These are the same atoms, just in more complicated arrangements

    9. “Orgo” as it is commonly referred to has a very close relationship to biology

    10. Principles are shared with inorganic chemistry, but the studies and focus of organic chemistry take it more into the direction of biochemistry and molecular biology – with a focus on the analysis and synthesis or the substances formed in biological systems (living things)

  • BIOLOGY

    • As we have heard 1000 times over in our lives: “Biology! The study of living things!”

    • Early days saw biology has a purely descriptive problem of finding out what things were with rudimentary means such as counting limbs and observing the physicality of different organisms

    • Next level was a focus on the machinery inside living bodies 

    • Relationship between physics and biology gets interesting here, as the latter aided the former in discovering conservation of energy (this was first demonstrated by Mayer in connection with the amount of heat taken in and given out by a living creature)

    • Off the top of your head, it is quite easier than you might think to pinpoint physical phenomena in the biology of living animals: circulation of blood, bodily pumps, pressure, nerves, etc

    • Nerves = fine tubes with complex yet very thin walls. Cells pump ions through these walls so that there are positive ions on the outside and negative ions on the inside (similar to a capacitor)

    • If this membrane “discharges” in one place, so that the electric voltage is reduced there, it has a cascading electrical influence on its neighbors and creates a wave of “penetrability” of the membrane that runs down the fiber whenever it is “excited” at a particular place

    • These are how we transmit messages through the body

    • In the nerve cell there are processes that pump the ions slowly out again to get the nerve ready for the next impulse

synapses
    • Anytime electricity is involved, physics is present, and therefore it has a great deal of influence on understanding this signaling

    • Messages that originate in the brain are sent out along nerves

    • Nerves branch out into fine little things that are connected to an endplate structure near a muscle 

    • When the messages reach these areas a chemical release of acetylcholine is triggered to make muscle fibers contract

    • The fundamental processes in the muscle that make mechanical motions are not known because we don’t fully understand the machinery by which the chemical reaction induced by acetylcholine can actually modify the dimensions of the muscle

    • Biology is an enormously wide field (if you didn’t already assume such)

    • What does light do in the eye? 

    • How does hearing work?

    • A really complex one: how does thinking work??

    • To give some perspective, even the biology humans study that is considered pretty fundamental, such as the way nerves work, is not actually so crucial. Living things can exist without nerves… take plants!

    • The most common feature of all living things is that they are made of cells

    • Each cell contains complex machinery for doing things chemically

    • Krebs cycle

    • It is often hard to recreate certain reactions in laboratory settings because of high energy barriers

    • Feynman describes enzymes as very large molecules within cells which in some complicated way hold the smaller molecules just right so that reactions can occur easily

    • Enzymes used to be called ferments because they were discovered in the fermentation of sugar

    • Enzymes are large, unique, reusable, and made of protein

    • Not all proteins are enzymes but all enzymes are proteins

    • They are not directly related to reactions and act solely as the catalyst for one atom to move places (given adequate supply and a proper place to be moved)

    • Just a reminder of why physics is so important in biology and other sciences – the experimental techniques that were developed and all of the classification and labeling of atoms that resulted

    • Point in case: isotopes (having different atomic weights based on differing numbers of neutrons in the nucleus) 

    • Proteins = a chain, or series, of amino acids

    • There are twenty different amino acids, all can combine with each other to form chains with a CO-NH backbone

    • One of the greatest triumphs of Feynman’s time was the discovery of the exact spatial atomic arrangement of certain proteins

    • Hemoglobin

    • How does an enzyme know what to be? The transmission of instructions is done by a substance in the nucleus of the cell called DNA

    • Sperm cells consist mostly of DNA

    • If DNA is thought of as a blueprint – one of the most common analogies used to first teach the concept to anyone – it must be able to do two things: first, reproduce itself and second, instruct the protein 

    • DNA was studied chemically to determine its composition and with the use of x-rays to reveal its pattern in space

    • The DNA molecule is a pair of chains twisted upon each other

    • The backbone of each chain is a series of sugar and phosphate groups

    • Specific series of the DNA = specific genetic instructions it carries and transmits

    • For the sake of the chain analogy, DNA has specific links that attach in specific ways to link the two chains: adenone, thymine, cytosine, and guanine

    • During reproduction, when a chain is split and each goes along with its new cell, the remaining half-chain creates a complementary new chain

    • The central unsolved problem of biology in Feynman’s day was how do the specific arrangements and connections of bases determine our genetic make-up?

    • Ribosomes are the tiny particles in the cell in charge of protein synthesis, however, they are not in the nucleus with the DNA

    • Tiny little molecule pieces also come off of DNA, they are not as long or large as the DNA itself, more of a mere section, and known as RNA

    • The RNA carries a message as to what kind of protein to make and travels with this to the ribosome

  • ASTRONOMY

    1. Older than physics

    2. Most remarkable discovery was that the stars are made of atoms of the same kind as those on earth

    3. Using a spectroscope we can analyze the frequencies of the light waves and differentiate atoms in the stars

    4. Two chemical elements were discovered on a star before they were discovered on earth: helium (the sun) and technetium (on certain cool stars)

    5. Because we know about the behavior of atoms under conditions of high temperature and low density, we can analyze via statistical mechanics the behavior of stellar substances

    6. Obviously conditions cannot be reproduced on earth, but physics enables us to make very precise estimates of what will actually happen in different circumstances

    7. Ironically, we understand the distribution of matter in the interior of the sun far better than the interior of the earth

    8. What is the origin of the energy of stars? What makes them able to continue to burn?

    9. Nuclear reactions are occurring in the stars (some man was out walking with his girlfriend when he discovered this)

    10. The nuclear burning of hydrogen supplies the energy of the sun (hydrogen is converted to helium)

    11. The manufacture of carious chemical elements proceeds in the centers of stars, from hydrogen

    12. The elements that created our earth were once “cooked” inside a star and spit out – we know this because of a very important clue: the proportion of different isotopes is never changed by chemical reactions, they are a result of nuclear reactions 

    13. Stellar explosions like the one that made earth are called novae and supernovae

  • GEOLOGY

    1. Known as an earth science

    2. Examples include meteorology and the weather, these sciences have physical instruments (thanks to the development of experimental physics) 

    3. The concept of predicting the condition of our air is scrutinized by physicists (technically we don’t even know exactly what is happening with our air as we speak because it is constantly moving and swirling around us)

    4. The situation of turbulent flow arrises in many fields and remains unanalyzable 

    5. Basic geological question: what makes the earth the way it is? 

    6. An obvious processes is the erosion due to water and air

    7. Processes that counter erosion also occur… otherwise all of our mountains would be gone by now!

    8. Volcanism

    9. Theory that there are currents inside the earth which are circulating due to the difference in temperature inside and outside

    10. If these currents are circulating in opposite directions, matter will collect in the region where they meet and make mountain belts that if unhappily stressed, will produce volcanoes and earthquakes

    11. We know the speed of earthquake waves through the earth and the density distribution of the earth, BUT physicists have been unable to theorize exactly how dense a substance should be at the pressures expected near the center of the earth

    12. AKA we don’t know the properties of matter existing in these circumstances

    13. Feynman seems to think it is only a question of when someone is mathematically gifted enough to work out exactly how matter behaves inside our earth – not if just when

  • PSYCHOLOGY

    1. “Psycho-analysis is not a science: it is at best a medical process, and perhaps even more like witch-doctoring” 

    2. Has a theory for what causes disease

    3. Psychoanalysis has not been carefully checked by experiment, so there is no certainty of the number of cases where it works and where it doesn’t work

    4. Other branches include the physiology of sensation (what happens in the eye, brain, etc)

    5. The central problem of the mind (or nervous system): when an animal learns something, it can do something differently than before and its brain cells must have changed. As these cells are made of atoms, in what way is it different? 

    6. When a fact is learned, a memory stored, or a feeling had, we don’t know where to look or what to look for physically

    7. Analog of the brain and computing machines: elements with a lot of lines similar to the synapse (connection of one nerve to another) 

    8. Feynman seems to be overwhelmed by the mental science of humans, because he concludes that all human beings are “so different” and it will be a long time before we are able to understand the complexity of human behavior. For good measure he adds that dogs are easier to understand, but nobody knows how dogs work yet either.

    9. In my opinion, Feynman doesn’t seem to do this field of science justice. He seems to diminish it to the psychoanalysis of Freud, and doesn’t consider any of the tangible studies done related to the human brain, trauma, addiction, stress, etc

  • Physics is clearly important to other sciences simply in the contribution and invention of instruments 

  • In order for physical theory to be of any use we must know were the atoms are located

  • There is a kind of problem in other sciences that does not exist in physics – a historical question. How did it get that way? 

  • The theory of evolution of the question of the origins of the universe are problems that don’t exactly exist within physics. The laws of physics aren’t questioned – right now.

  • A fundamental problem of physics still being solved: finding new particles

  • The analysis of circulating or turbulent fluids

  • We can predict a lot of things related to fluid dynamics, but when water is really running through a pipe, we can’t quite explain it

  • Feynman believes poets do not write to be understood

  • “The whole universe is in a glass of wine” – the twisting liquid evaporates depending on the wind and weather, the reflections in the glass, the atomic composition and how it got its particular chemical elements to be the way they are through fermentation, a product of the substrates with the help of enzymes

  • All life is fermentation

  • Our minds like the convenience of dividing life into parts that are more manageable for us, like physics vs biology and chemistry and geology, astronomy, and psychology. However, nature doesn’t know this, or behave in accordance. Let’s put everything back together!


4: Conservation of Energy

  • What is energy

  • The conservation of energy governs all natural phenomena that are known to date – with no exception in so far as we know

  • Law states that there is a certain quantity called energy that does NOT change along with the manifold changes in nature

  • The idea is abstract because it is a mathematical principle

  • The energy can be thought of as a numerical quantity which does not change when something happens

  • When calculating the energy of a system, sometimes it leaves and sometimes it enters 

  • Energy has a large number of different forms (eg gravitational, kinetic, heat, elastic, electrical, chemical, radiant, nuclear, mass)

  • In physics today we still have no knowledge of what energy is

  • The complex formulas we have for calculating energy always give us a constant numerical representation for it, but energy is an abstract thing because it does not tell us the mechanisms or the reasons for the various formulas

  • GRAVITATIONAL POTENTIAL ENERGY

    1. Exists near the surface of the earth

    2. GPE = weight x height because it represents the energy which an object has because of its relationship in space, relative to the earth (this formula holds true so long as we are not too far from the earth as the force weakens as we go higher)

    3. The reasoning for this form of energy is beautiful, but it assumes that perpetual motion is not possible. Experimentally it has been checked to be true.

    4. The general name of energy which has to do with its location relative to something else is called potential energy

    5. If it is a question of any other kind of force, take electrical, just tack on “potential” to the end

    6. The general principle for change in energy is: Δenergy = force x (distance force acts through)

    7. The conservation of energy can be used to deduce what happens in a number of circumstances, including the class high school problems and laws about pulleys and levers

    8. Stevinus also discovered a clever way to solve these kinds of problems

    9. The principle of virtual work

  • KINETIC ENERGY

    1. Consider the classic pendulum in its motion, it loses height swinging from side to side. Where does this potential energy go? 

    2. The motion at the bottom of the pendulum must be a quantity of energy that permits it to rise to a certain height, and has nothing to do with the machinery or the path by which it comes up to that height

    3. KE = weight x (velocity)² / 2 x gravity (because of the implication of gravity in the formula, you must consider the relativistic correction at high speeds

  • The existence of energy can be illustrated in many forms

  • Elastic energy – work is required to pull a spring down, and once it is down, it can be used to lift weights (in its stretched condition is has a possibility of doing some work)

  • Elastic energy equations are complicated by the tension the spring is experiencing, and that is why the simple (weight x height) formulas are usually incorrect

  • When you let go of a spring, it passes through an equilibrium point (in mathematics this is the constant solution to a set of differential equations) and is converted to kinetic energy where it goes back and forth between compressing or stretching the string and kinetic energy of motion

  • Eventually the motion stops! Why? Where does the energy go? 

  • Heat energy

  • The kinetic energy of atoms is constantly happening in the background, we just lose track of it because it is not visible

  • So how to be certain that the kinetic energy is still there? Use a thermometer

  • If something is warmer –> there is an increase of kinetic energy by a definite amount

  • In this way, heat energy is just kinetic energy on an invisible scale, or internal motion

  • An issue with our experiments with matter on a large scale: we cannot fully demonstrate the conservation of energy because every time we move a “large clump of stuff” the atoms do not remain absolutely undisturbed and a certain amount of random motion goes into the atomic system. This cannot be seen. But it can be measured using change in temperature!

  • Many many forms of energy

  • Electrical energy has to do with pushing and pulling electric charges

  • Radiant energy is the energy of light, and we know it as a form of electrical energy because the light can be represented as wiggles in the electromagnetic field

  • The energy that is released in chemical reactions is known as chemical energy

  • Chemical energy is understood to have two parts: kinetic energy of the electrons inside the atoms, and the electrical energy of the interaction between electrons and protons inside the atoms

  • Nuclear energy is involved with the arrangement of particles inside the nucleus (for which we have formulas but no fundamental laws)

  • Associated with the relativity theory is a modification of the laws of kinetic energy – it is combined with another thing called mass energy

  • Basically, anything has energy from its sheer existence!

  • This all might be more familiar with Einstein’s equation: E = mc² 

  • You might be wondering, like me, if there are any other conservation laws in physics…

  • Conservation of linear momentum

  • Conservation of angular momentum

  • We don’t understand any of these laws deeply; we do not understand energy as a certain number of little blobs

  • The energy of a photon is Planck’s constant x frequency

  • As we presently understand, there can be any amount of energy

  • In quantum mechanics it gets even more interesting because it turns out the conservation of energy is very closely related to another important property of the world, things do not depend on the absolute time

  • This basically means that you can set up an experiment one moment and then later on do the exact same experiment and have it behave the exact same way, regardless of the different start times. We don’t know if this is strictly true though

  • The conservation of charge (merely counting how many positive – how many negative electrical charges you have, and the number is never changed)

  • The conservation of baryons – baryons encompass a number of strange particles like the neutron and proton. In any reaction, it appears that counting the number of baryons coming into a process will result in the same number coming out *if you count anti baryons as -1 baryon

  • The conservation of leptons (electrons, mu mesons, and neutrinos, and positrons, as anti-electrons, are -1 leptons)

  • Of the six conservation laws, three subtly involving space and time and three are simple in the sense that they count something

  • With regard to conservation of energy, note that available energy is another matter (we know energy is conserved, but the energy available for human utility is not so easily conserved)

  • The laws which govern how much energy is available are called Laws of Thermodynamics and involve the concept of entropy for irreversible thermodynamic processes

  • So where can we get our supplies of energy today? From the sun, rain, coal, uranium, and hydrogen – but mostly from the sun because it makes the rain and the coal.

  • Nature liberates a lot of energy from the sun, but only one part in two billion falls on the earth

  • The energy from hydrogen comes at explosive and dangerous conditions and can only be controlled in thermonuclear reactions

  • Get this: the energy that can be obtained from 10 quarts of water per second is equal to all of the electrical power generated in the United States *at least it was in Feynman’s time 5: The Theory of Gravitation

    • Apparently this chapter will discuss some of the most far-reaching generalizations of the human mind

    • Is it not quite elegant and impressive that nature follows with such completeness the simple principle of the law of gravitation?

    • Every object in the universe attracts every other object with a force that (for any two bodies) is proportional to the mass of each and varies inversely with the square of the distance between them

    • Mathematically: F = G x mm’/r²

    • An object responds to a force by accelerating in the direction of the force by an amount that is inversely proportional to the mass of the object

    • The story of this law and its two important principles begins with the ancients observing the motions of the planets among the stars, and finally deducing that they went around the sun (a fact later discovered by Copernicus)

    • Tycho Brahe had a different idea, he proposed that the debates about the motions of the planets would best be resolved if the actual positions of the planets in the sky were measured sufficiently accurately

    • Kepler was a mathematician that succeeded Brahe and from his data, discovered more simple and beautiful laws regarding planetary motion

    • Kepler’s laws: 

      • Each planet goes around in the sun in a curve called an ellipse with the sun at a focus

      • Ellipses are not just ovals, but very specific and precise curves that can be obtained using two tracks, one at each focus, a loop of string, and a pencil. Mathematically: it is the locus of all points the sum of whose distances from the two fixed foci points is a constant

      • He also observed that the planets do not go around the sun at a uniform speed, but move faster when they are nearer the sun and more slowly when they are farther from the sun

      • Radius vector = a line drawn from the sun to any point in a planet’s orbit

      • If the planets went in circles, which they nearly do, the time required to go around the circle would be proportional to the 3/2 power of the diameter

    1. Each planet moves around the sun in an ellipse, with the sun at one focus

    2. The radius vector from the sun to the planet sweeps out equal areas in equal intervals of time

    3. The squares of the periods of any two planets are proportional to the cubes of the semi major axes of their respective orbits: T ∝ a³∕²

    • While Kepler was discovering his laws, Galileo was studying the laws of motion

    • In these times, people theorized that planets orbited because invisible angels were behind them beating their wings

    • The principle of inertia aided the process of refining this theory – if something is moving, with nothing touching it and if left completely undisturbed it will go on forever, coasting at a uniform speed in a straight line

    • Newton modified the above with his forces that are able to change the motion of a body

    • If a body speeds up, a force must be applied in the direction of motion

    • If a motion is changed to a new direction, a force must have been applied sideways

    • F = ma

    • Thus, the more massive something is, the stronger the force required to produce a given acceleration

    • The idea resulting from all of these considerations of forces is that no tangential force is needed to keep a planet in its orbit

    • Inertia means that the force needed to control the motion of a planet around the sun is not a force around the sun but a force towards the sun (if undisturbed the planet would go off in a straight line, so there must be a force acting perpendicularly towards the sun so the resulting path is this circular orbit)

    • NEWTON’S LAW OF GRAVITATION

      • Newton appreciated that the sun could be the organization of forces that govern the motion of the planets

      • His observations inspired the idea that all forces are directed exactly towards the sun 

      • Using Kepler’s third law, it is possible to show that the farther away the planet, the weaker the forces

      • Newton was a man of “considerable feeling for generalities”

      • Knowing that there was a force holding us to the earth, he proposed that this was a universal force that everything pulls everything else

      • The radius of the moon’s orbit = ~240,000 miles

      • It takes ~ 29 days for the moon to go around the earth… a month

      • This messes with my brain: the moon ‘falls’ in the sense that it falls away from the straight line it would pursue if there were no forces 

      • Again: if you shoot a bullet faster and faster, because the earth’s surface is curved, when the bullet falls its standard 16ft due to gravity & forces, it may be at just the same height above the ground as it was before because it is traveling “around” the curved earth

      • A handy geometry theorem says that a tangent to a circle is the mean proportional between the two parts of the diameter cut by an equal chord

      • “Any discovery of a new law is useful only if we can take more out than we put in” – Feynman

      • The pull of the moon on earth causes the tides (they go up and down in 12 hours)

      • What is a centrifugal force

      • Gravity is responsible for the earth being round (they are nearly spheres, but should technically be elliptical)

      • Jupiter’s moons and their inability to be on schedule almost caused the death of Newton’s laws of gravitation. If a law does not work in even one place then it is simply wrong.

      • Jupiter’s moons were ahead of schedule when it was close to the earth, and they were behind schedule when Jupiter was further from the earth. Why?

      • The time it takes for us to see the moons of Jupiter differs because of the time it takes light to travel from Jupiter to earth depending on their distance from each other

      • So, light does not travel instantaneously

      • This also allowed for the first estimate of the speed of light in 1656

      • Do stars experience gravitational attractions as planet’s do? Yes thanks to a double-star system

      • One of the most beautiful things in the sky is a globular star cluster

      • When you inspect an entire galaxy there is an obvious tendency for its matter to agglomerate (cluster together around a common center)

      • That does not mean it is just a ball of matter because everything is spinning and has angular momentum

      • Galaxies have a scale of perhaps 50,000 to 100,000 light-years

      • The earth’s distance from the sun is 8 1/3 light-minutes 

      • Galaxies also cluster together most likely due to gravitational forces just as stars cluster within galaxies

      • The law of gravitation also gives some ideas on the origin of the stars: if a big cloud of gas and dust exists, the attraction of tiny pieces together causes clumps to form. These clumps are basically fetus stars

    • CAVENDISH’S EXPERIMENT

      • Performing simple experiments to observe forces of gravitation is actually quite difficult because of all the confounding variables you must address like keeping all air out, making sure nothing is electrically charged, etc

      • Cavendish designed an apparatus that did just that and first demonstrated the direct force between two large, fixed balls of lead and two smaller balls of lead on the ends of an arm supported by very fine torsion fiber

      • He measured how much the fiber twisted to indirectly measure the strength of the force and verify that is was indeed inversely proportional to the square of the distance

      • This allows one to accurately determine the coefficient G in the formula F = Gmm’/r²

      • His experiment allowed us to discover the mass of the earth by rearranging the equation!

    • GRAVITY

      • What is the machinery of gravity? 

      • Even though Newton created these laws on gravity, he never explored what created the forces, only that they existed. 

      • It is quite characteristic of many physical laws to have this abstract character: someone makes an amazing and beautiful discovery, does enough math and experimentation to ensure it can become a fundamental law, and continues along

      • No one knows why we are able to use mathematics to describe nature without a tangible mechanism behind it

      • Although gravitation and other forces are similar, there is no explanation of it in terms of other forces

      • The unified field theory is an elegant attempt to combine the forces of gravitation and electricity as they behave rather similarly (the forces are constant, and vary inversely as the square of the distance, they also behave in the opposite direction as ‘likes repel’)

      • Nature’s universal charge = the repulsion of two electrons due to electricity and the attraction of two electrons due to their masses

      • Can measure the ratio of electron repulsion: gravitational attraction

      • The above ratio is independent of the distance and is a fundamental constant of nature (1 / 4.17 x 10⁴²) 

      • It has been proposed that the gravitational constant is related to the age of the universe, but the fact that standard measurements of time (such as years) were created by humans complicates the ability to make further calculations

      • Is it possible that the gravitational constant is changing with time? This would be a fairly logical deduction if it is indeed related to the aging of the universe… BUT that would mean that at the time of the earliest records of life on earth that we have, the earth would’ve been much closer to the sun, so close that temperatures would have been 100ºC hotter and therefore the aforementioned life wouldn’t have existed. So no, probably not related to age

      • For all substances tested thus far on record, masses and weights are exactly proportional within 1 part in 1,000,000,000 or less

    • GRAVITY AND RELATIVITY

      • Einstein modified Newton’s law of gravitation

      • This modification corrected it (yes Newton was wrong!) to take the theory of relativity into account

      • Anything which has energy has mass (mass in the sense that it is attracted gravitationally)

      • This includes light!

      • When a light beam, which has an energy, passes the sun, there is an attraction and thus it does not travel straight but is deflected

      • Quantum-mechanical aspects of nature also fail to explain gravitation 

      • When the scale is so small that quantum effects become relevant, gravitational effects become irrelevant

      • Newton’s law was modified to Einstein’s law which really should be further modified with the uncertainty principle, however, this has yet to be done

    ______________________________________________________________________

    6: Quantum Behavior

    • ATOMIC MECHANICS

      • The theory of the index of dense materials and total internal reflection 

      • The “classical theory” of electric waves turns out to be a completely adequate description of nature for a large number of effects

      • Light energy comes in lumps called photons

      • Classical and older theories tend to fail to describe the behavior of larger pieces of matter because they are really made up of atomic-sized particles

      • Quantum mechanics is the description of the behavior of matter in all its details – in particular things happening on an atomic scale

      • These things on a very small scale do not behave like anything we have experience with: not particles, not clouds, not balls, weights on springs, etc

      • Newton thought light was made up of particles, then it was discovered that it behaves like a wave, later then again it was found to sometimes behave like a particle and so now we roughly conclude it isn’t exactly either

      • There is some generalization to be made: electrons behave just like light because the quantum behavior of atomic objects is all the same (electrons, protons, neutrons, photons ‘of light’, etc)

      • The accumulation of info about atomic and small-scale behavior was gradual, and the increasing confusion was resolved in 1926-27 by Schrodinger, Heisenberg, and Born when they obtained a consistent description for matter

      • Just like trying to picture things in four dimensions is nearly impossible for humans, atomic behavior is so unlike ordinary experience that it is very difficult to get used to

    • AN EXPERIMENT WITH BULLETS

      • Behavior of bullets = particle like, behavior of water waves = wave like

      • Set up a wall with two holes in it and backstops to determine where bullets that are sprayed out of a machine gun land, and collect them

      • Can then find the probability that a bullet which passes through the holes in the wall will arrive at the backstop at a certain distance, x, from the center

      • Must mention probability because there is no way to be definite about where each bullet will go

      • Take the ratio of (no of bullets which arrive at the detecter in a certain time: total no of bullets that hit the backstop during the same time) 

      • The bullet experiment observations reveal that probability of arrival shows no interference (P₁₂ = P₁ + P₂)

    • AN EXPERIMENT WITH WAVES

      • A small object that creates waves jiggles around in a shallow trough of water to make circular waves

      • There is another wall with two holes in it and something to absorb the waves so there is no reflection 

      • Need a detector of sorts that measures the energy being carried by the wave

      • The detector picks up the wave motion and calculates the proportional intensity at the rate in which waves approach it – regardless of the magnitude

      • As holes are covered or opened, a very different relationship is discovered between interference and intensity

      • When intensity has its maxima, the waves are in phase (peaks of the waves add together to give a large amplitude and subsequently, a large intensity)

      • Constructive interference

      • If two waves arrive with a phase difference of pi they are out of phase and the resulting motion is the difference of the two amplitudes

      • Destructive interference

      • For waves: I₁ = |h₁|² , I₂ = |h₂|² , I₁₂ = |h₁ + h₂|²

      • |h₁ + h₂|² = |h₁|² + |h₂|² + cosδ, where δ is the phase difference between h₁ and h₂ 

      • One last way to write is would be: I₁₂ = I₁ + I₂ + 2√ I₁ I₂cosδ which is the “interference term” – intensity of these water waves can have any value and it shows interference

    • AN EXPERIMENT WITH ELECTRONS

      • Same set up as before, where an electron gun of sorts is shot through two holes in a wall and the ones that make it through are intercepted by a detector of sorts

      • a geiger counter is recognizable by its erratic clicking sounds

      • The rate at which the “clicks” of the detector may change, but the size or loudness of each click is always the same

      • Electrons always arrive in identical lumps

      • What is the relative probability that an electron ‘lump’ will arrive at the backstop at various distances, x, from the center? 

      • The probability distribution is the same as was found for waves!

      • Because each electron either goes through hole 1 or through hole 2, the observed curve to map their probability must be a sum of the electrons that come through both, and we can conclude that there is interference

      • The mathematics for describing the electron probability distribution curb is the exact same as for describing waves BUT what actually goes on, or how it happens remains an inexplicable mystery

      • The electrons arrive in discrete lumps, like particles, and the probability of their arrival is distributed like that distribution intensity of a wave – hence the particle-wave duality of electrons

      • In quantum mechanics, it turns out that the amplitudes HAVE to be represented by complex numbers because the real parts alone are not sufficient

      • Modify the experiment by adding a very strong light source because we know that electron charges scatter light

      • This means that when an electron passes we will be able to detect it because it will scatter light in a way that is visible to us

      • This modification to the experiment allows us to conclude that when we look at the electrons, the distribution is different than when we do not look

      • Why?! How? Well, the light source is strong enough to disturb the delicate electrons. The electric field of light acting on a charge will exert a force on it

      • It becomes a catch-22: if you turn down the brightness of the light source, the waves will be weaker and will not disturb the electrons as much, but we will not be able to observe the negligible effect anymore

      • However, using a dimmer light source does reveal some interesting things: the flash of light scatter from the electrons as they pass does NOT get weaker (it is always the same size). Sometimes electrons will pass through without a visible flash!

      • This really means that the light also acts like electrons… it arrives in a scattered manner of lumps as well, called photons

      • As the intensity of light is turned down, it doesn’t change the size of the photons, only the rate at which they are emitted 

      • Further analyzing the experiment, if the electrons are not seen (ie they are not disturbed by a bright light source), interference occurs

      • Remember that the momentum carried by a “photon” of light is inversely proportional to its wavelength (p = h/λ)

      • If you want to disturb electrons only slightly try lowering the frequency of the light instead of its intensity

      • This would mean using light with a more red color, or infrared, or radio-waves/radar

      • Using these longer waves, we see a big fuzzy flash when light is scattered by electrons and can no longer tell which hole it went through because the wavelength itself was longer than the distance between holes

      • In conclusion, it is impossible to arrange light in such a way that we can tell which hole the electron went through and still not disturb the pattern

      • This led to Heisenberg’s suggestion that these laws of nature could only be consistent if there were some basic limitation on our experimental capabilities – the uncertainty principle explains that “it is impossible to design an apparatus to determine the path an electron takes that will not at the same time disturb the electrons enough to destroy the interference pattern”

      • The complete theory of quantum mechanics which we use to describe atoms and all matter depends on the correctness of this uncertainty principle

      • Returning to the bullets, we didn’t see any interference patterns there, so does that mean they don’t confine to these constructs for describing the behavior of nature? No. 

      • The bullets just had wavelengths that were so tiny we didn’t detect the interference and the curve appeared smooth

      • A kind of average = the classical curve (of distribution by Maxwell-Boltzmann)

    • FIRST PRINCIPLES OF QUANTUM MECHANICS

      • A summary of findings based on an ideal experiment: 

    1. The probability of an event is given by the square of the absolute value of a complex number Φ which is called the probability amplitude

      1. P = probability

      2. Φ = probability amplitude

      3. P = |Φ|²

    2. When an event can occur in several alternative ways, the probability amplitude is the sum of the probability amplitudes for each separate event and there is interference

      1. Φ = Φ₁ + Φ₂

      2. P = |Φ₁ + Φ₂|²

    3. If an experiment is performed which is capable of determining whether one or another alternative is actually taken, the probability of the event is the sum of the probabilities for each alternative and the interference is lost

      1. P = P₁ + P₂

    • If you ask how it works exactly you will be disappointed because no one has discovered the machinery behind the law

    • A very important difference between classical and quantum mechanics: it is impossible to predict exactly what would happen, you can only predict the odds!!!

    • So has physics given up? This recognition that only the prediction of the probability of different events occurring, and not the prediction of the events themselves seems a retrenchment, but it is unavoidable

    • This puzzle is the way that nature is

    • THE UNCERTAINTY PRINCIPLE

      • Heisenberg originally stated: If you make the measurement on any object, and you can determine the x-component of its momentum with an uncertainty of 𝛥p you cannot, at the same time, know its x-position more accurately than 𝛥x ≥ h/2𝛥p

      • In other words, the uncertainties in the position and the momentum at any instant must have their product greater than half the reduced Planck constant

      • Basically, the uncertainty principle protects quantum mechanics by confirming and perpetuating our inability to accurately know where something is (position) and how fast it is traveling (momentum) at exactly the same time


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