Have you ever wondered what light was all about? This video, produced for IB Physics and A-Level students provides you with a clear presentation of the following topics:
Presented by Edouard Reny, PhD in solid state chemistry, and private tutor in physics for international high school students.
You wish to know more about Physics Made Easy, and get access to great resources that will help you with your studies of Physics? Then, visit the Website! https://www.physics-made-easy.com/
Have you ever wondered why the Moon, although attracted by the Earth, never falls on it? Instead, our Moon describes a circular path around it. How come? This course will make you understand why.
Would you like to check it out, feel free to use this link: https://skl.sh/2WIH3rK
This link will direct you to Skillshare and it will give you access to the full course on Gravity as well as thousands of high quality courses on many topics! And if you use this link, you get the first 2 subscription months free (You can cancel your subscription before the 2 months free trial period)!
By taking this class, you will gain an understanding of Orbital Motion. Orbital Motion combines the laws of gravity with the principles of circular motion. This concept is detailed in the first video (5.1) where you will learn what is an orbit and realise how the velocity of an orbiting object can define its orbit.
The three videos that follow are training exercises showing fun stuff you can do with orbital motion equations, like determining the speed of the Earth, calculating the mass of Jupiter or exploring the intricacies of the Saturnian system. This latter exercise will allow you to discover a celestial Law: The 3rd Law of Kepler that links the period of revolution of a body to the distance to the massive object it is orbiting around.
To exemplify this, we will fly far beyond Neptune, deep into the Kuiper belt, where dozens of mysterious draft planets live their frozen lives. We will also play closer to Earth, like calculating the height at which a TV satellite must be launched!
Finally, for those interested in animation, Video 5.8 shows how to use the 3rd law of Kepler to design the motion of a bunch planets orbiting a star.
*** Content of the class ***
Video 5.0: Introduction
Video 5.1: Lesson – Orbital Motion
Video 5.2: Training Exercise – The Speed of the Earth
Video 5.3: Training Exercise – The Mass of Jupiter
Video 5.4: Training Exercise – The Moons of Saturn
Video 5.5: Lesson – The 3rd Law of Kepler
Video 5.6: Training Exercise – Geostationary Orbits
Video 5.7: Training Exercise – A Visit to the Kuiper Belt
Video 5.8: Application Example – the 3rd Law of Kepler at the service of animation
All training exercises are provided as pdf files and formatted so that you can print the exercise and work on them away from the computer. Answers are provided also in a pdf document.
*** This class is part of a larger course named “Gravity, The Basics”.***
“Gravity, The Basics” explores the elementary notions of Newtonian gravity.
Class 1: “Linear Motion” (because being comfortable with this notion will allow you to make the most of the full course). This class presents a step-by-step technique to solve all motion problems when the accelerat
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https://www.youtube.com/watch?v=pscjD0hGtek
Feynman diagrams are a graphical representation of the processes involved in particle physics reactions. This video is the second episode of a series of three that presents what are Feynman diagrams, how to understand and use them, and how to build them.
In this episode you will learn what are the elements you need to know to read Feynman diagrams and build your own: space-time diagrams, particle symbolism and vertices. We will use for this a well-known particle physics reaction as support, electron repulsion. We will also have a look at vertices involving the decay of a gluon into a quark and an anti-quark as well as the transformation of a quark and an anti-quark into a weak force boson.
Feynman diagrams are an insightful tool that puts to light the wonders of particle physics. The reactions occurring in particle physics are a marvel of processes involving the forces of nature (weak force, strong force and electromagnetic force). Writing these like a chemical reaction does not provide information about the processes involved, just what you start up with, and what you end up with.
One can use the Quantum Chromodynamics (QCD) and Quantum Electrodynamics (EOD) to model quite well what is going on, but the mathematics involved is not for everyone! Instead, graphical representation of these reaction, invented by Richard Feynman, allow all to visualize the processes involved easily: Feynman diagrams. He introduced these originally as a graphical aid for visualizing and calculating interactions between electrons and photons. Today, Feynman diagrams are commonly used to depict all types of particle interactions.
These videos are intended to help high school students with their physics studies as well as high school physics teachers wondering how to approach the topic with their students.
**** Access to the Videos ****
Introduction: Content review of the Feynman Diagram mini-series:
https://youtu.be/O9ihGuK53Ww
Episode 1: What is a Feynman Diagram? (brief overview of Feynman diagrams, using as support a very well-known reaction, beta decay):
https://youtu.be/TLBXrMixcu8
Episode 3: Feynman Diagrams, Let’s build some! (Learning how to build Feynman diagrams by example, using particle physics reactions like muon decay, pion decay, Kaon decay etc.:
https://youtu.be/vgk2aJRlBcg
SUPER USEFUL - The table of particles: https://www.physics-made-easy.com/Standard-Model-of-Particle-Physics
If you are not familiar with Particle physics, I recommend you start by viewing the series of videos that deals in detail with particle physics reactions:
_ Introduction: https://youtu.be/gy-durcAhJ4
_ Elementary and composite particles of the standard model: https://youtu.be/AJSL39hVVPw
_ Quantum numbers of particles: https://youtu.be/3SVMrLmGHWQ
_ Conservation laws
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https://www.youtube.com/watch?v=JScJjZ9zW7A
This video is aimed at IB (SL or HL) or A-Level students preparing for their exams .
In this episode, we will be working on an exercise inspired by past papers that deal with calculations in regards to atomic energy levels and emission spectra.
An exercise will appear on the screen. Pause the video and work it out by yourself. Then, we will review the exercise together.
The text of the exercise can be consulted here:
Page 1 (questions a & b): https://s26.postimg.org/5ky5f77nt/Page1_C.jpg
Page 2 (question c):
https://s26.postimg.org/bxdap1aq1/Page2_B.jpg
Page 3: (questions d,e and f)
https://s26.postimg.org/e4hjcyg09/Page3_B.jpg
This video is the fifth episode of the Atomic Physics Series. It is a direct application of the knowledge compiled in the first 4 episodes:
You can get free access to tons of free resources that will help you with your studies of high school physics by visiting the website:
https://www.physics-made-easy.com
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View the 4 first episodes if you haven't done so yet:
Episode 1: "Energies in an atom". This episode introduces the series by reminding the viewer of the concepts of energy (Kinetic, potential, internal and mechanical). Within this context, it discusses the energies involved in an atom of Hydrogen.
https://youtu.be/g9ieCabz_PI
Episode 2: "What is light", that describes how an atom can gain or lose energy.
https://youtu.be/XwNsi1vzjTs
Episode 3: "Energy levels of an atom", that explains that the energy of an atom can only take specific values. This shows why atoms can be characterized by their emission or absorbtion spectra.
https://youtu.be/MHJO6pm-hoM
Episode 4 (IB Physics High Level): "Deriving Energy Levels of the Hydrogen Atom". It presents how to derive the energy levels of a Hydrogen atom from scratch in 6 easy steps! It is a beautiful demonstration that reminds us that art and science are really not that far apart (this derivation is to be known for the exam).
https://youtu.be/YW_g3dy0HOg
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This video is produced and presented by Edouard Reny, Ph.D. in materials sciences and private tutor in Physics.
Edouard provides one-on-one private tuition in Physics (face to face or by Skype). If you wish to contact him, visit his website: https://www.physics-tutor.nl/
If you enjoy these videos and / or find them useful for your studies, please like and subscribe!
I wish you a productive study!
Edouard Reny
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Credits:
Music: Edouard Andre Reny (http://www.synaptic-machines.com)
Background image for thumbnail: Pixabay.com
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https://www.youtube.com/watch?v=XS8xQzCDT3k
Particles are the Lego bricks of nature. Their interaction with each other constructs all matter that is present in our universe. Particle Physics studies how particles interact with each other .
In this lesson, divided into separate 3 videos, you will learn about fundamental particles, about the quantum numbers associated with each of them, and how to predict and write particle physics reactions .
In this video (PART 2/3), we get a detailed look at some of the properties of elementary and composite particles, which are expressed as quantum numbers (Baryon number, Electric Charge, Lepton number, Strangeness).
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Access to the table of particles:
https://www.physics-made-easy.com/Standard-Model-of-Particle-Physics
This lecture is structured in three sections that follow a general introduction:
INTRODUCTION: https://youtu.be/gy-durcAhJ4
SECTION 1: The standard Model of Particle Physics
https://youtu.be/AJSL39hVVPw
SECTION3: Conservation laws and particle physics reactions
https://youtu.be/E4JGzQjBgHg
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PART 1 is a reminder of the standard model of particle physics. It presents the elementary particles (fermions, like quarks and leptons, and bosons, like the photon or the gluon). It shows how combining quarks lead to composite particles (hadrons like the proton, the neutron, the pion and the kaon). Antimatter is also discussed in this section.
This first section is a brief overview, so if you wish to view a lesson on the standard model of particles with more details and at a slower pace head on to these two videos:
Elementary particles: https://youtu.be/guYfayO3ESI
Composite particles: https://youtu.be/e-oyDDnI348
PART 2 is a detailed look at some of the properties of these particles, which are expressed as quantum numbers (Baryon number, Electric Charge, Lepton number, Strangeness).
PART 3: In nature there are some symmetries that need to be respected in all interactions. These lead to the existence of conservation laws (via Noether's theorem). Quantum numbers need to follow these conservation laws. This idea is central. After viewing this section, you will be able to determine if a particle physics reaction is possible or not. For that, we will work on many examples of reactions including Beta decay, muon decay into a positron, and more.
This video has a lot of information, it’s a real course in itself. I hope you enjoy it and that it helps in giving you a clearer idea about the reactions between particles.
If you are a high school teacher, feel free to use anything you see fit in this video for your own students .
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This video is produced and presented by Edouard Reny, Ph.D. in solid state chemistry and private tutor in Physics.
For access to g
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https://www.youtube.com/watch?v=3SVMrLmGHWQ
Welcome to the Course ”Gravity, The Basics”: 50 videos, 6 sections, 4.5 hours that explore the Basics of Newtonian gravity.
Hopefully you have watched the video, and you are here reading these lines to know more… But first, as promised in the video here are the promotional actions for Youtube Viewers:
You can purchase the full course on Udemy by using this link
https://www.udemy.com/course/gravity-the-basics/?referralCode=91F294FF9D2454F6CEE5
You can also view this course as part of a subscription program on Skillshare (On skillshare, the course is cut into 6 classes - each class corresponds to a section of the course-. By using the link below, which will bring you to the first section of the course, you can benefit of your first 2 months of subscription for free!:
https://skl.sh/2UTpsI0
*** What you will learn ***
“Gravity, The Basics” teaches the elementary notions you need to understand and apply Newtonian gravity:
_ Solving 1-dimensional motion problems (Linear Kinematics),
_ Newton’s Universal Law of Gravitation,
_ What are fields,
_ Gravitational fields and gravitational field strength,
_ Gravitational field lines,
_ Circular motion: angular velocity, centripetal acceleration and force, how to apply these notions to solve questions in physics,
_ Orbital motion and the third law of Kepler.
*** Who is this course for? ***
This course is suited for high school students studying Physics (from grade 10 to 12).
The content of this course complies with Chapter 6 of the IB Physics Program and Topics 6.2 and 11 of the A-Level Curriculum.
It contains many exercises in all sections as well as exam inspired questions (especially section 6). This course is a very valuable tool for preparing any upcoming physics exam that may have questions related to gravity.
This course is also suited as a refresher for early university students that wish to solidify their understanding on Newtonian gravity.
And of course, any person interested in physics and in how the world works will also enjoy the voyage: I often invite my students on adventures beyond the academic…
*** Structure of the course ***
“Gravity, The Basics” explores the elementary notions of Newtonian gravity.
Section1: “Linear Motion” (because being comfortable with this notion will allow you to make the most of the full course). This class presents a step-by-step technique to solve all motion problems when the acceleration is constant. This Section can be taken by itself.
Section 2: “Newton’s Universal Law of Gravitation”, which you can be seen as a doorway to the deeper dive we carry out in the next classes.
Section 3: “Gravitational Fields”, the core of this course: This class teaches first what is a field, and then dives into a deep description of gra
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https://www.youtube.com/watch?v=UsZqX812E2s
Tip 4: Take advantage of Kirschhoff laws !
This video is the fourth of a series of 5 tips that will help you understand electric circuits. It is aimed at IB Physics, A-level physics and AP Physics students.
Check out the other tips for a more complete picture :
Tip 1: Consider charges circulating in a circuit as carriers of energy. Getting grips with this concept will allow you to have a more intuitive approach in solving circuit problems.
https://youtu.be/p-z-o2n61fs
Tip 2: When relevant, think in potentials at a point instead of voltages (voltage = potential difference).
https://youtu.be/GVmZ-72Efkw
Tip 3: Prepare the analysis of a circuit by drawing first arrows for potential differences and currents.
https://youtu.be/_M8HIeArqR4
Tip 5: Calculate equivalent resistance of two resistors in parallel in seconds!
https://youtu.be/WD5u-wrwBpY
I am also uploading some exam preparation exercises that will give you a very practical methodology to solve circuits with a minimum of effort!
Exercise 1: for circuits with a single battery.
https://youtu.be/H0gyq3284x4
Exercise 2: for circuits with multiple batteries.
https://youtu.be/CpYryUtMdcw
Have fun and good luck!
Edouard
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Edouard Reny, Ph.D. in materials science, is a private physics tutor for international IB, A-level and AP students.
Need more info?
Visit www.physics-tutor.nl.
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https://www.youtube.com/watch?v=EERWWUlAwoE
Dark matter accounts for more than 80% of all matter that populates the spacetime of our Universe. What is dark matter, is one of the most troubling mysteries in astrophysics and cosmology.
But... how do we know that dark matter even exists?
*=*=*=*=*=* Please support the channel, donate (see below) *=*=*=*=*=*
Many cosmological observations show that there is more gravity than there should be if we only account for matter we can see directly. There must be some kind of invisible matter out there. its gravitational effect gives astronomers many opportunities to study it indirectly: The rotational dynamics of galaxies, the strength of gravitational lensing, The weak intensity of CMB fluctuations and many more, are phenomena that require dark matter…
In this video, we create a model of a spiral galaxy, and from that predict its velocity curve (speed of stars vs the distance from the central supermassive black hole). Then, we compare this prediction to observations, and realise there is a serious glitch! A huge amount of mass appears to be missing: Dark Matter. Without it, out galaxy would evaporate, with a large fraction of its stars ejected into inter-galactic space!
We stay open however to other explanations that do not require dark matter by briefly looking into the an alternative explanation, the MOND theory: it does work well in justifying the shape of galactic velocity curves without introducing any dark stuff, but it doesn’t match other astronomical observations.
Now, enough reading: it is time for you to tighten you seat belts and join me for a ride in a Dark Universe!
= = = = = = = = = = Support the Channel : Donate ! = = = = = = = = = =
You may have noticed… there were no ads in this video. That means that I am creating these videos entirely for free…
If you enjoy them, please consider making a donation to support me. In addition to encouraging me, donation allow me to create new education videos on physics, that all can enjoy…
To make a one-time donation, please visit:
https://www.physics-made-easy.com/donate
Thank you!
= = = = = = = = = = The Presenter = = = = = = = = = =
This video is produced and presented by Edouard Reny, Ph.D. in solid state chemistry and private tutor in Physical Sciences.
For access to great resources that will help you with your studies of high school Physics, visit and subscribe to the "Physics Made Easy" website:
https://www.physics-made-easy.com/
Edouard provides one-on-one private tuition in Physics (face to face or by Skype). If you wish to contact him, visit his website: https://www.physics-tutor.nl/
= = = = = = = = = = Footage and Image credits = = = = = = = = = =
_ Picture of Galaxy in Intro and at 12:40, Star and Planet (Intro): by NASA/JPL-Caltech
_ Artist view of Nebulae, St
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https://www.youtube.com/watch?v=EKUy1dD1nSM