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ALL OF PHYSICS explained in 14 Minutes

Wacky Science • 14:20 minutes • Published 2024-02-17 • YouTube

📚 Chapter Summaries (8)

🤖 AI-Generated Summary:

📚 Video Chapters (8 chapters):

📹 Video Information:

Title: ALL OF PHYSICS explained in 14 Minutes
Channel: Wacky Science
Duration: 14:20
Views: 6,369,067

Overview

This video provides a fast-paced, entertaining overview of foundational concepts in physics, guiding viewers from the basics of classical mechanics to the strange and fascinating world of quantum mechanics. Each chapter focuses on a major domain within physics, building upon previous concepts and weaving together a coherent story of how our universe works, from everyday experiences like gravity and energy, to the mind-bending ideas of relativity and quantum uncertainty. The chapters connect sequentially, introducing more complex principles as the viewer’s understanding deepens.


Chapter-by-Chapter Deep Dive

Classical Mechanics (00:00)

  • Core Concepts & Main Points:
    The chapter opens with the basics of classical mechanics, centering on Newton’s laws and gravity. Mass is explained as both the amount of "stuff" and a measure of inertia. Acceleration is described simply as how quickly velocity changes. The Inverse-Square Law is introduced, emphasizing how gravity decreases rapidly with distance. The nature of planetary orbits is explained—they are not perfectly round, but elliptical due to gravitational forces.
  • Key Insights & Takeaways:
  • Newton’s law (Force = Mass x Acceleration) is foundational.
  • Gravity’s strength diminishes with the square of the distance (Inverse-Square Law).
  • Orbits result from the balance of gravitational pull and the motion of planets.
  • Actionable Strategies or Advice:
  • Use simple definitions to demystify physics (e.g., acceleration as changing speed).
  • Recognize that weight depends on gravity, which varies with location.
  • Important Examples:
  • The apple falling and planetary orbits.
  • Connection to Overall Theme:
    Sets the stage for all physics by explaining motion and force, the basis for more advanced concepts.

Energy (02:33)

  • Core Concepts & Main Points:
    This chapter delves into the concept of energy, measured in Joules. It distinguishes energy from force and explains types of energy (potential, kinetic). The conversion between forms of energy is highlighted—lifting an object transforms chemical energy into gravitational potential energy. The idea of work is clarified: no movement means no work is done, even if effort is expended. Kinetic energy and its conversion to heat (via friction) are explored.
  • Key Insights & Takeaways:
  • Energy is about capacity to do work, not just effort.
  • Energy changes form, such as kinetic to heat.
  • Temperature is the manifestation of particle motion (kinetic energy).
  • Actionable Strategies or Advice:
  • Focus on actual movement when considering work (force x distance).
  • Recognize where energy goes in real-life scenarios (e.g., car braking).
  • Important Examples:
  • Lifting an apple (1 Joule).
  • Car braking—kinetic energy turns to heat.
  • Connection to Overall Theme:
    Builds on mechanics by introducing energy, a key driver of physical processes.

Thermodynamics (04:40)

  • Core Concepts & Main Points:
    Thermodynamics explores heat, temperature, and entropy (disorder). The chapter uses ice and water to illustrate how entropy increases as structure is lost. The Second Law of Thermodynamics is emphasized: the universe tends toward greater disorder. The concept of isolated vs. non-isolated systems is touched upon (e.g., a fridge heating a room overall).
  • Key Insights & Takeaways:
  • Entropy is a measure of disorder; it always increases in isolated systems.
  • Local decreases in entropy (like cooling water) require greater increases elsewhere.
  • Actionable Strategies or Advice:
  • Consider the bigger system when analyzing thermodynamic processes.
  • Important Examples:
  • Structure of ice vs. water; a fridge heating a room.
  • Connection to Overall Theme:
    Expands the idea of energy into how it moves and changes, introducing universal limits.

Electromagnetism (06:01)

  • Core Concepts & Main Points:
    This chapter introduces electric charge, current (electron flow), and the basics of electric and magnetic fields. The relationship between electricity and magnetism is discussed—moving magnets induce current, and changing fields generate electromagnetic waves. The unity of electric and magnetic phenomena is emphasized.
  • Key Insights & Takeaways:
  • Electric and magnetic fields are manifestations of the same fundamental force.
  • Electromagnetic waves (like light) arise from oscillating fields.
  • Actionable Strategies or Advice:
  • Use analogies (e.g., field lines) to visualize invisible forces.
  • Experiment with magnets and conductors to see principles in action.
  • Important Examples:
  • Moving a magnet near a wire induces current.
  • Electromagnetic radiation (light).
  • Connection to Overall Theme:
    Continues the story of forces and energy, introducing non-contact forces and the nature of light.

Nuclear Physics 1 (08:30)

  • Core Concepts & Main Points:
    Focuses on the atomic nucleus, composed of protons and neutrons, and the concept of radioactivity. Explains that some nuclei are unstable and decay, releasing particles and energy. Warns against handling radioactive material due to health risks.
  • Key Insights & Takeaways:
  • Atomic nuclei can be unstable, leading to radioactivity.
  • There is a wide range of nuclear stability (some atoms decay quickly, others are stable for eons).
  • Actionable Strategies or Advice:
  • Do not handle radioactive substances.
  • Important Examples:
  • The variety in stability of atomic nuclei.
  • Connection to Overall Theme:
    Introduces the internal structure of matter and the energy locked within atoms.

Relativity (09:28)

  • Core Concepts & Main Points:
    Covers Einstein’s revolutionary ideas: the constant speed of light and the relativity of observation. Discusses the photoelectric effect (light as photons) and the non-intuitive effects of relativity, like time dilation and the curvature of spacetime. Uses analogies (walking north on a globe) to illustrate non-Euclidean geometry.
  • Key Insights & Takeaways:
  • Light’s speed is the same for all observers, regardless of their motion.
  • Gravity is the result of spacetime curvature, not a traditional force.
  • Actionable Strategies or Advice:
  • Use thought experiments to grasp counterintuitive concepts.
  • Important Examples:
  • Photoelectric effect; analogy of walking on a sphere to understand curved space.
  • Connection to Overall Theme:
    Challenges classical views, showing how reality behaves at high speeds and in strong gravity.

Nuclear Physics 2 (11:25)

  • Core Concepts & Main Points:
    Explains mass-energy equivalence (E=mc²), which underpins the energy of nuclear reactions (fission and fusion). The immense energy released by small amounts of mass is highlighted. Discusses two primary ways to release nuclear energy and mentions the concept of "missing mass" being converted to energy.
  • Key Insights & Takeaways:
  • Mass can be converted directly into vast amounts of energy.
  • Nuclear reactions (fission/fusion) are incredibly powerful due to this principle.
  • Actionable Strategies or Advice:
  • Understand the real-world implications (nuclear power and weapons).
  • Important Examples:
  • Atomic bombs; fusion in stars.
  • Connection to Overall Theme:
    Deepens the exploration of matter’s structure and the profound consequences of mass-energy conversion.

Quantum Mechanics (12:13)

  • Core Concepts & Main Points:
    Explores the quantum nature of reality, beginning with the “quantized” nature of light (photons) and energy ("quanta"). Describes superposition (particles existing in multiple states), the probability cloud model of electrons, and the Heisenberg uncertainty principle (limits to knowing position and speed simultaneously). Highlights the weirdness of quantum phenomena (double-slit experiment).
  • Key Insights & Takeaways:
  • Reality at small scales is governed by probabilities, not certainties.
  • Measurement affects quantum systems in fundamental ways.
  • The act of observation changes outcomes (wavefunction collapse).
  • Actionable Strategies or Advice:
  • Accept uncertainty and probability as core to understanding quantum systems.
  • Important Examples:
  • Double-slit experiment; electron probability clouds.
  • Connection to Overall Theme:
    Shows the ultimate limits of classical intuition and the bizarre, foundational rules of the universe.

Cross-Chapter Synthesis

Recurring Themes & Progressive Learning:
- Building from the Familiar to the Abstract:
The video starts with everyday experiences (gravity, energy) and moves stepwise into more abstract and counterintuitive realms (relativity, quantum mechanics).
- Unifying Concepts:
- Conservation laws (energy, mass-energy equivalence) bridge chapters from classical to nuclear physics.
- The shift from deterministic (classical mechanics) to probabilistic (quantum mechanics) descriptions illustrates the evolution of scientific understanding.
- The interplay between forces (gravity, electromagnetism) is woven throughout.
- Visualization & Analogy:
- The use of analogies (apples, cars, walking on a globe) makes complex ideas accessible and memorable.
- Warning Against Oversimplification:
- Several chapters (Energy, Thermodynamics, Nuclear Physics 1) caution against naive or careless interpretations—e.g., not all effort equals work, and radioactive materials are dangerous.

Learning Journey:
- The video guides viewers from the macroscopic (motion, energy, heat) to the microscopic and fundamental (atoms, relativity, quantum uncertainty).
- Each chapter introduces new terms and phenomena, but consistently ties them back to earlier principles, helping viewers see the interconnectedness of physics.

Most Important Points Across Chapters:
- Newton’s Laws & Gravity (Classical Mechanics)
- Energy Transformation and Conservation (Energy, Thermodynamics, Nuclear Physics 2)
- Entropy and Irreversibility (Thermodynamics)
- Electromagnetic Unification (Electromagnetism)
- Atomic Structure and Radioactivity (Nuclear Physics 1)
- Relativity and the Nature of Spacetime (Relativity)
- Quantum Uncertainty and Probability (Quantum Mechanics)


Actionable Strategies by Chapter

Classical Mechanics (00:00):
- Use clear, simple definitions when learning or teaching new concepts.
- Remember that gravity and weight depend on location and mass.

Energy (02:33):
- When calculating work, only consider movement (force x distance).
- Track energy transformation in real-world systems to understand outcomes.

Thermodynamics (04:40):
- Always consider the system’s boundaries when analyzing energy and entropy changes.

Electromagnetism (06:01):
- Use field lines and hands-on experiments (e.g., magnets and wires) to visualize concepts.
- Relate electric/magnetic phenomena to real-life devices and technologies.

Nuclear Physics 1 (08:30):
- Avoid handling potentially dangerous materials; respect safety warnings.

Relativity (09:28):
- Use thought experiments to challenge and expand your intuition about motion and space.

Nuclear Physics 2 (11:25):
- Recognize the practical consequences of mass-energy conversion (e.g., in nuclear power and weapons).

Quantum Mechanics (12:13):
- Embrace uncertainty and the probabilistic nature of quantum outcomes.
- Accept that observing a system can change what you measure.

Warnings & Pitfalls:
- Don’t mistake effort for work (Energy).
- Do not handle radioactive atoms (Nuclear Physics 1).
- Beware of oversimplifying complex systems—context matters (Thermodynamics, Quantum Mechanics).

Resources, Tools, or Next Steps:
- The video suggests using analogies and simple experiments to deepen understanding.
- Encourages further study of foundational experiments (photoelectric effect, double-slit) to grasp advanced concepts.


Chapter Structure for Reference:
- Classical Mechanics (00:00)
- Energy (02:33)
- Thermodynamics (04:40)
- Electromagnetism (06:01)
- Nuclear Physics 1 (08:30)
- Relativity (09:28)
- Nuclear Physics 2 (11:25)
- Quantum Mechanics (12:13)


This structured summary allows readers to easily revisit key ideas by chapter, understand how each section connects to the broader narrative, and apply the advice and insights in their own learning or teaching of physics.


📝 Transcript Chapters (8 chapters):

📝 Transcript (329 entries):

## Classical Mechanics [00:00] [00:00] Hi! You’re on a rock. Floating in space. Surrounded by more rocks. [00:04] And gas. And a bunch of nothing, mainly. Oh hey, look at that, the rocks are going around the gas. Hold on, what the heck, is going on here? [00:11] To understand, let’s look a little bit of Physics. Wait, did I say a little bit? To find out what kind of magic this is, we’ll have to go back in time. Okay, not that far. [00:23] Stop! Yeah. That’s perfect. This is gravity guy. [00:27] But most people call him “Isaac Newton”. One important thing he said is that Force equals mass times acceleration. Now what do all these words even mean? Force is just a push or pull on something, in a certain direction. [00:36] Mass tells you how much of something there is, and it’s also a measure of inertia, [00:39] but we’ll get to that later, and acceleration is the derivative of velocity with respect [00:43] to time, but that’s too many big words for my taste, so let’s just say it’s how fast [00:47] velocity is changing. The key takeaway is that if you apply a Force to a fixed mass, you get a predictable amount of acceleration. If you know all the forces acting on a basketball mid-air, you can predict with 100% certainty if the ball will go in the hoop or your neighbours windshield. “Whoa, did an apple just fall on my head?” [01:05] Yes Newton, it did. “That must have happened for a reason” said Newton, as he discovered that two masses attract one another, making the apple fall. Yes, even you, no matter how ugly you think you are, attract pretty much the whole universe, at least a little bit. Hey, can you put that on paper? [01:19] “yup” said Newton, who gave us the Law of Universal Gravitation. In other words, how much two bodies pull on each other, given their mass and distance, times a constant. Bigger mass? Bigger Pull. [01:29] Bigger distance? Smaller pull. Actually, a lot smaller pull. You see, the as the distance increases, the Force gets smaller by the square. [01:36] That my friends, is the Inverse-Square Law. Gravity is also the reason why the planets in our solar system orbit the sun. They got their initial velocity when the solar system formed out of spinning gas, and since there’s nothing in space to stop them from moving, they’ll keep moving. Hey, that’s Newton’s first Law. [01:51] The sun is so massive, that the force of gravity keeps pulling the planets towards the sun, [01:55] but the planets are fast enough to essentially fall towards the sun but miss it, and this [01:59] goes on forever, creating a round orbit. Actually, that’s kind of a lie. Most orbits orbits are not perfectly round but more egg-shaped and pluto’s orbit is just…a complete mess. But you get the idea. [02:09] In this case, the gravity is what we call a centripetal force. One thing many people confuse is mass and weight, and no, they are not the same. Mass tells you how much of this blob there is, and Weight is the force of Gravity the blob would feel. To make things clear, your mass would be the same on the earth and on the moon, but the “weight” you would perceive, is different, because the moon has a weaker gravitational pull, meaning, a weaker force acting on your mass. [02:31] So really, you’re not overweight, you’re just on the wrong planet. ## Energy [02:33] [02:34] Aight, enough about Newton, let’s break some stuff. If you ever dropped your phone, it might look like this: What the hell ground, why’d you do that? The answer is Energy. You know, the thing kids have after eating gummy bears. [02:45] Energy has the unit Joule. And it’s not like Force, it’s doesn’t have a direction, it’s just a number, that’s kind of chilling there, as a property of a thing. You see, there’s two main kinds of energy: Kinetic energy, and potential energy. In plain English, energy of movement, and stored energy due to some circumstance. [02:59] For example, when you held your phone, it stored gravitational potential energy, due [03:02] to being held above the ground, at a certain height. Once you dropped it, the potential energy was converted into kinetic energy, as the phone fell. Then it smashed into the ground, and the phone absorbed some of the energy making the screen go boom. Work is defined as Force applied over distance. [03:17] For example: If you lift an apple by 1 meter, you would [03:19] have done about 1 Joule of work. This happened by converting chemical energy stored in your body to gravitational potential energy stored in the apple. As you may have noticed, Energy and Work have the same unit “Joule”. So they must be the same thing? [03:31] Uhhh, No. Energy is the total amount of work that a thing could possibly do. Work is just the stuff that actually happened and required energy. You know, force applied over a distance, which most often implies converting energy from one form to another. [03:40] If you try to lift a weight that’s too heavy for you, you’d feel like that took a bunch [03:42] of work, right? Well, yes, but your feelings are invalid in the face of Physics! Mathematically, no work has been done! Because, work is a force applied over a distance. [03:51] And since you didn’t move the weight at all, no distance means no work. The key thing to remember about energy is that it cannot be created or destroyed, only converted. Aka, the conservation of energy. Okay, but a car, that’s moving has kinetic energy. [04:04] When the car stops, assuming the car doesn’t smash into a wall, where does that energy [04:09] go? When you apply the brakes, there’s friction between the brakes and the wheels, causing the car to slow down, and creating heat as a byproduct. That heat is then dissipated to the surrounding air. And that makes the molecules in the air move faster. [04:21] And things that move have kinetic energy. So ultimately, the kinetic energy is transferred from the car to the air. With this knowledge, we can define that Temperature is just the average kinetic energy of atoms in a system. You see, all atoms, not just molecules in the air, wiggle. [04:34] Like this. The faster they move, the hotter things get. That is temperature. All that talk about hot stuff, I think it’s time we talk about Thermodynamics. ## Thermodynamics [04:40] [04:42] It tells us that jumping in lava is probably a bad idea, but more importantly, the absolute [04:47] mess that is entropy. Literally, it tells you how much disorder there is in a system, indicating the number of possible states a system can be in. For example, get an ice cube, no not that one, yes that’s perfect, and put it in the sun. The sun will obliterate the ice cube and turn it into water. [05:03] Looking at the structure of ice and water, we can see that ice is more neatly organized [05:06] than water, which just kind of goes all over the place. Also, the water could look like this, or this, or even this, but the ice will always look a little something like this. In total, the system went from low entropy to high entropy, meaning more disorder and more possible microstates. This trend applies everything. [05:22] The whole universe is on an unstoppable path to higher entropy. It’s also the reason why time seems to go only forwards, or at least, that’s what we believe at this point. Practically, entropy tells us that some forms of energy are more useful for doing work than others. Burn some gasoline, and your car will move, spitting out heat and gas. [05:37] That heat and gas is pretty much gasoline, just in the form of higher entropy. And as you can imagine, this stuff won’t really make your car move, and the gas won’t spontaneously turn back into liquid gasoline. Meaning, the form of gasoline with lower entropy is more useful for doing work. Okay, but if you put some water in the freezer, will it not decrease in entropy? [05:55] Yes, BUT the fridge is not an isolated system and will heat up the room more than it will [06:00] cool down the water, increasing the total entropy. ## Electromagnetism [06:01] [06:02] Wanna see some magic? Woah, what just happened? Some electrons apparently moved through some wires and let there be light. What is going on here? [06:13] Objects have a fancy something called a charge. It can be positive or negative. Or, if you have the same amount of both, an object is neutral. Electrons have a single negative charge. [06:20] The flow of electrons is called electric current. To describe it, we use three parameters: Current, Voltage, and Resistance. Current is the amount of electrons passing through a wire in a given amount of time, Voltage is what pushes the electrons to move, but simply put, it’s a difference in electric potential, so you can imagine it as a slope that goes from high potential to low potential, where the flow of current goes downhill, and resistance is pretty self explanatory. This is Coulomb’s Law. [06:43] Wait a minute, this is just Newton’s Law of Gravitation in disguise! This tells us that electric charges attract each other in a similar way masses do. Opposites want to cuddle, while like charges literally couldn’t think of a more disgusting thing than to be with one another. These four equations explain pretty much all of electromagnetism. [06:59] But don’t be scared just because they look scary! I mean, yeah, they do, but it’s simpler than it seems at first. The first one states that if there is an electric charge, there will be an Electric field, or this big E, emerging form it. Add another and you have an electrostatic field. [07:12] These lines tell us in which direction a charged particle would feel a force at any given point. The second one tells us the same for magnetic fields, AND, even though electric charges are cool and can be alone, magnetic poles, are not. They’re very lonely. There will always be a north pole together with a south pole, and a single pole can never be alone. [07:29] Okay now here’s where things get kind of freaky. You know how electric charges only act on other charges, and magnets only affect other magnets? Well that’s only true if they’re not moving. The third and fourth maxwell equations tell us that a moving magnet creates an electric field, and a moving charge or electric field creates a magnetic field. [07:45] One consequence of this is that current can seemingly come “out of nowhere” by moving [07:49] a magnet next to a conductor. The moving magnet creates and electric field, which makes the electrons inside the conductors go crazy. That is called induction. It’s the reason why your phone charges when you put in on the charging pad, even though it is not directly connected to a cable. [07:59] In other words, electric and magnetic fields are so tightly linked that they are the two [08:00] parts of the same bigger thing. Let’s say we have a charge. Since it doesn’t move, it has a static electric field. If we accelerate the charge, there will be a magnetic field around it. [08:09] That magnetic field interacts with the electric field, which again changes the magnetic field, [08:13] and this is a sort of chain reaction that makes the electromagnetic field radiate outwards [08:17] into space as an electromagnetic wave. Depending on the frequency, the human eye can actually see this, it’s called light, but most of the spectrum is invisible to the human eye and is used for things such as Bluetooth, wireless charging and confusing human apes into thinking magic is real. ## Nuclear Physics 1 [08:30] [08:31] Hey, can we go back to the water and look at those molecules? Yeah, those, what are they made of? The molecules are made of Atoms. Atoms are made of a core and some electrons. [08:39] The core is made of protons and neutrons, both of which are made of quarks. They’re strange yet charming, from up top down to the bottom. Oh yeah there’s some more stuff, like for example the overweight brothers of the electron. All of this together makes up the standard model, which we believe to be the smallest things in the universe. [08:55] At least that’s the excuse we have for not knowing what quarks are made of. Fun Fact! Depending on the number of protons in the core, you get different elements. Depending on the number of Neutrons in the core, you get different Isotopes of the same element. [09:06] Most of which are a little overweight and very unstable. So they fall apart, into smaller atoms. That releases ionizing radiation. Not so fun fact: That stuff will kill you. [09:15] Do not play with radioactive atoms. If you have a large group of atoms, you can predict when half of those will have fallen apart. That’s the halflife. Depending on how unstable an isotope is, it will survive a certain amount of time. [09:23] Some don’t want to live, some really don’t want to live, but some will live far longer [09:27] than you probably will. ## Relativity [09:28] [09:28] Oh yeah, did I mention that light is like the fastest thing in the universe? To be exact, 299, 792, 458 meters per second in a vacuum. “That is pretty fast” said everyone. Also, “Light is a wave” said everyone. [09:43] Why? If you shoot it through two teeny tiny slits it creates a fancy pattern due to interference, which is just a wave thing. You see, when two waves cross, they can add up, or cancel each other out. These gaps, are the spots where they cancel each other out, so in this case, light behaves like a wave. [09:57] “Nah, screw that, everything you know is wrong” said Albert Einstein, probably smoking [10:02] crack, after hearing about the photoelectric effect and discovering that light comes in [10:05] tiny packets called photons. I sure hope that doesn’t unravel a whole new area of phyiscs, haha. “Anyway” he said, as he continued to casually drop an absolute bomb on the entire field of physics with his theory of relativity: He assumed the speed of light is constant because it arises from two other constants. He also assumed the laws of physics are the same for everyone, regardless if moving or at rest. [10:27] Now think about it: If two people turn on a flashlight, but one person is standing still, [10:30] while the other person is on a moving train, wouldn’t the person standing still see the [10:34] other person’s light as going faster than the speed of light? The reality is: NO! It would be the same as their own flashlight. That’s impossible, except if time passes slower for that person from the perspective of this person. [10:46] In other words, if the speed of light is constant, time must be relative. Also, gravity is not actually a Force, sorry Newton, but rather a consequence of masses bending spacetime. Einstein thought that the universe is a mesh of space and time, and anything with a mass bends this fabric. Also, all objects move freely on a straight line when moving through space. [11:04] Gravitation is simply the result of objects following these bent lines, which appear straight [11:07] to them. If you have a hard time understanding this, you can imagine two people on earth, walking in parallel, straight lines. On a short distance, the straight lines will never meet. Now imagine one standing on the east cost, and one the west coast of the US. [11:16] If they both walk north, eventually, they will meet at the north pole. Because of the curvature of the earth, they ended up at the same point even though they both walked “straight” relative to themselves. ## Nuclear Physics 2 [11:25] [11:25] “Oh yeah by the way Energy and mass are kind of the same thing” he added, which [11:28] explains why atom bombs are so frickin powerful. According to this formula, even just tiny atoms can release a humongous amount of energy by giving up just a fraction of their mass during fission. What is Fission? It’s the same thing Oppenheimer used to make this thing go boom. [11:42] You see, there’s two main ways to gain energy from changing nuclei: Fission and Fusion. Fission aims to split the nucleus of an atom into two or more smaller nuclei, which is most often achieved by blasting the core with neutrons. Fusion is the opposite, where you combine two smaller nuclei to get one bigger one. The energy came from something we call a “mass defect” where the resulting nucleus is lighter than the starting nuclei. [12:02] This “missing” mass is what was converted to energy during Fusion. Fission and Fusion are cool, but you have got to be careful or you might just blow up the planet. That totally didn’t almost happen before…multiple times. ## Quantum Mechanics [12:13] [12:13] Hey remember when Einstein said light is a particle? He accidentally discovered a whole new field of physics which he though is just a giant hoax: Quantum Mechanics. This stuff is crazy. Another german guy called Max Planck said “yes, Einstein, you’re right. [12:26] Light does come in tiny packets. Actually, all energy comes in tiny packets”. Or “Quanta”. He is the daddy of Quantum Mechanics. [12:32] Wanna know where an electron is inside an atom? It’s here! And there! And everywhere, at the same time, actually! [12:36] That’s a superposition. It’s not in one state, it’s in multiple states at once - at least until you measure it. Then it chooses one cozy spot to be in. Schrödinger gave us an equation that gives you a probabilistic model of where you can find it if you were to measure. [12:49] You can imagine this as a cloud, and the denser it is, the more likely it is for an electron [12:53] to be there. But still, where exactly it will end up once you measure it, is random. Speaking of observing particles, they’re also super sensitive about their private data. Look at these two images of a flying ball: in one, you can clearly see where the ball is, but not in which direction it’s moving, and in the other you can see where it’s moving and approximately how fast, but not where exactly it is at the moment. [13:12] That is essentially Heisenberg’s uncertainty principle: You can never know both the exact [13:16] position and the exact speed of a quantum particle at the same time. Okay, let’s recap, a small thing can be a particle and a wave at the same time, and when we try to look at them, weird stuff happens. But you know what, it gets even weirder. Think back to the double slit experiment: We know that a light beam acts as a bunch of waves and we get interference. [13:31] But here’s the weird thing: Even if you send individual photons, after sending enough [13:36] of them and detecting where they end up, you get interference. Like, how can that be? What did a single particle interfere with? Well, we think it interfered with itself, because it acted as a wave and went through both slits at the same time. [13:48] That’s a superposition. “Okay, well let’s just measure which slit it goes through”. Uh, yeah, that’s not going to happen. Once you start measuring which slit the photon goes through, it stops acting like a wave and the interference pattern disappears, as every particle chooses just one of the slits to go through. [14:01] Sounds kinda suspicious to me. Anyways, all this knowledge is going to cost you one subscribe and a thumbs up, thank you very much, and you can decide if maybe you’d want to tip with a comment, perhaps?