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Sabetta Talks Math
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Добавлен 16 авг 2021
The wave equation
Harmonic motion is some of the most ubiquitous in all of physics. In this video, we start from a long chain of beads and springs and use it to derive the dynamics for a continuous system with waves propagating through it.
Просмотров: 600
Видео
Physics in non-inertial reference frames
Просмотров 53710 месяцев назад
In this video, we explore what happens when a reference frame is accelerating either linearly or rotationally.
Hidden symmetries and the Runge-Lenz vector
Просмотров 902Год назад
This video examines the role of constants of motion in the symmetries and dimensionality of inverse-square law systems. For more information on these topics, I recommend these posts by: John Baez: math.ucr.edu/home/baez/gravitational.html and Greg Egan: www.gregegan.net/SCIENCE/Ellipse/Ellipse.html Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Orbital Mechanics
Просмотров 1,1 тыс.Год назад
We derive the equation for the shape of an orbit under a central force and solve the specific case of inverse-square-law forces. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Central forces
Просмотров 1,1 тыс.Год назад
In this video, we set up the central force problem according to Lagrangian mechanics and find that an initially six-dimensional system turns into a one-dimensional system. Here is a link to Evgenii Neumerzhitckii's simulation: evgenii.com/blog/two-body-problem-simulator/ Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Phase space & Liouville's Theorem
Просмотров 11 тыс.Год назад
Hamiltonian dynamics exists in phase space a space of formed of all the generalized positions and generalized momenta. We explore ways to solve Hamilton's equations in this space. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Hamiltonian Mechanics
Просмотров 395Год назад
In this video, we derive Hamilton's equations of motion and discuss methods to solve them. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
The Hamiltonian
Просмотров 411Год назад
Starting with Noether's theorem for a continuous time symmetry, we'll examine the Hamiltonian. We compare the "state space" description of Lagrangian mechanics to the "phase space" description of Hamiltonian mechanics. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Conservation of Energy & Conservative Forces
Просмотров 513Год назад
Conservation of energy is one of the main tenets of mechanics. But what does it mean for a force to be conservative? Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Conservation of momentum
Просмотров 435Год назад
Conservation of momentum is a consequence of Newton's second law, when there are no net external forces acting on a system. This is useful for understanding collisions as well as systems, like rockets, which are changing their mass constantly. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Interacting systems
Просмотров 235Год назад
This video is an introduction to interacting systems, sometimes called dynamical systems. Each element of the system has an evolution equation that may depend on the state of the other elements. We explore in depth the Lotke Volterra model of predator-prey ecology and discuss using the slope field method to describe it's dynamics. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Noether's theorem and Conserved Quantities (reupload)
Просмотров 580Год назад
Emmy Noether was one of the most important and influential mathematicians of the 20th century. She contributed greatly to the fields of abstract algebra and theoretical physics. In particular, her theorem relating continuous symmetries of the Lagrangian to conserved quantities is one of the most profound theorems in all of physics. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Constraints and Lagrange multipliers
Просмотров 646Год назад
A lot of systems that we might want to study using in the calculus of variations often have constraints. This video teaches you how to incorporate constraints into your Lagrangian system. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
The Lagrangian
Просмотров 734Год назад
The Lagrangian is the kinetic energy minus the potential energy. It is a functional that lets us solve for the dynamics of many physical systems. Music "Everything" by Vi Hart soundcloud.com/vihartvihart
Damped Oscillators | Classical Mechanics
Просмотров 858Год назад
Damped Oscillators | Classical Mechanics
Newton's laws in polar coordinates | Classical Mechanics
Просмотров 2,7 тыс.Год назад
Newton's laws in polar coordinates | Classical Mechanics
Newton's laws as differential equations | Classical Mechanics
Просмотров 3 тыс.Год назад
Newton's laws as differential equations | Classical Mechanics
Heavy Spinning Tops | Chapter 28 Classical Mechanics 2
Просмотров 1,6 тыс.2 года назад
Heavy Spinning Tops | Chapter 28 Classical Mechanics 2
3D Rotations | Chapter 27 Classical Mechanics 2
Просмотров 3 тыс.2 года назад
3D Rotations | Chapter 27 Classical Mechanics 2
Euler's equations | Chapter 26 Classical Mechanics 2
Просмотров 2 тыс.2 года назад
Euler's equations | Chapter 26 Classical Mechanics 2
The moment of inertia tensor | Chapter 25 Classical Mechanics 2
Просмотров 34 тыс.2 года назад
The moment of inertia tensor | Chapter 25 Classical Mechanics 2
Motion in rotating reference frames | Chapter 24 Classical Mechanics 2
Просмотров 5162 года назад
Motion in rotating reference frames | Chapter 24 Classical Mechanics 2
Review of angular momentum and torque | Chapter 23 Classical Mechanics 2
Просмотров 1,3 тыс.2 года назад
Review of angular momentum and torque | Chapter 23 Classical Mechanics 2
Hidden symmetries and the Runge Lenz vector | Chapter 22 Classical Mechanics 2
Просмотров 3,3 тыс.2 года назад
Hidden symmetries and the Runge Lenz vector | Chapter 22 Classical Mechanics 2
Changes of orbit | Chapter 21 Classical Mechanics 2
Просмотров 7622 года назад
Changes of orbit | Chapter 21 Classical Mechanics 2
Awesome, just the right level of detail to give a decent intuition.
Thanks!
Thanks!
Thank you
Great ❤❤❤ please videos on textbook recommendations 🙏 🙏🙏 thanks !
Brilliant
8:43 why the off-diagonal term (integral von xy) measure the distance to lines x=y??? there is not even an z component here!
so well constructed and so well spoken!! tysm
Didn’t need to read out the whole expression 😭 LMAO
1:56 "Euclidean space, dual spaces are isomorphic." WHAT? Repeated this a million times and still don't know what she means.
When using the einstein summation convention, we usually sum over equal indices when one index is lowered, while the other index is raised. The lowered index represents a covariant component, and a raised index represents a covariant component. For convenience, let’s say that the tensor is uniquely defined by a singular index, meaning that it can be thought of as a vector. Let’s also say that the vector lives in a vector space (let’s call that vector space V), and can be written as a linear combination of basis vectors that has contravariant components (raised index). The covariant (lowered index) components can then be found by finding the corresponding dual vector. The dual vector lives in another vector space, called the dual space of V. The dual space is often denoted as V^*. However, for a eucledian space V, it’s dual space V^* will be isomorphic, essentialy meaning that these to vectors spaces are the same, just represented with different basis vectors. When this is the case, there is no real use to distinguish between covariant and contravariant components. Thus, we do not need to have one raised, and one lowered index for the einstein summation convention. Hence, the inner product between two vectors a and b can be written ass a • b = a_i*b_i. Hopes this helps to clear some confusion.
@mathiasfjsne8854 Name checks out Math-ius. Thank you fellow traveler of this universe. When and why would the dual space be different? Why are we using Euclidian space?
That accent 😶
why is the velocity v_i in the direction of r? (4:38)
Can you please make more videos?
1:52 "Euclidean space, dual spaces are isomorphic." WHAT?
私も実験していますが、回転体の向きを変えると、表向き裏向きの慣性力が働くようです。
Beautiful animations, but too much text to read while listening you you talk really fast at the same time.
This channel is a gem for physics students. Subscribed.
Hello! May I ask a question? If I want to transform moment inertia tensor from Cartesian to spherical coordinate, how to do it? Thanks!
Amazing videos!, Saving fellow undergrads like us who just need a little push in the right direction of math🙌🔥
2:53 You meant as n goes to infinity didn't you?
Nice explanation!
My hair is so beautiful and luxurious😉.
I assume you are already famous but trust me you deserve to be more famous. Thanks for sharing your knowledge.
Love your videos !!
Thanks for all the amazing works! This is such an underrated channel.
amazing video
I wish I'd never heard of 'vocal fry' because the narrator has it to the max & I cant ignore it.
For which standard this topic is for??
This is taught in college/university. Or maybe you can do this for JEE Advanced (Indian entrance exam for engineering).
@@absolutedesi5899 Yes I'm preparing for JEE only but this is not in our syllabus we have only scalars and vectors
these are great
why didn't rotated about x-axis ?
Is this the 3b1b animation engine? So beautiful. I know how to numerically solve ODEs but couldn't be bothered to listen to a PDE lecture, so this video was perfect for me.
I don't think this was any more valuable than just reading it in any text book, this doesn't help develop my understanding further as it's just regurgitating the same old "stuff".
Very helpful, currently studying for physics quals
Enjoyed this...at (e.g.) 9:10, why do you use cursive delta in the integral? At 8:17 also, dA = Int (n.v dt)dg and all the d's are cursive, like variational notation?
You deserve so many more subscribers. Each of your videos is a divulgation masterpiece.
Why do the best video have the least views, this channel is so underrated. Great video as usual!
3B1B vibes
The "proof" given at 6:36 doesn't seem too convincing, at least visually I can imagine a lot of points outside A(t) where the trayectorias do not cross. Besides that, great video and a very good topic
Sehr gut
Wonderlful explanation. Very much appreciated!
I like calculus of variations but i dont know how to learn it. What books do you recommend?
One point of critique, you show a phase space plot with spiralling motion. However, Hamiltonian systems never have a sink or source at a singularity. Great video nonetheless!
Work on that sound quality
it's a very cool video and I'm sorry to point that out, but are you sure about the last poisson bracket at 14:43 ? I think that it should be equal to the angular momentum, at least in QM.
Thanks!
Linear algebra has only orthogonalization process to get orthogonal polynomials but there are faster ways to get these polynomials
Very nice and clear derivation!
I can't figure out the logic behind the calculation of the residues when the imaginary unit is involved: using the Matlab calculator, the final result of the last integral in the video would be pi/2i -pi/(2sqrt(3)). I tried to do the calculation using the residue theorem arriving at the same conclusions as Matlab. Instead, if I traditionally solve this integral with substitutions and simplifications, I arrive at the correct result, pi/sqrt(3). The point is this: I don't get the reason Res(f, i) = -1/2 and Res(f,-i)=e^(-i2*pi/3)/2, as you say. From my calculations, Res(f, i)= i^(1/3)/(2*i)= e^(i*pi/6)/(2*i) = (-i/2)*e^ (i*pi/6) = (-1/2)*e^(i*pi/2)*e^(i*pi/6) = (-1/2)*e^(i*2*pi /3). Similarly, Res(f,-i) = (-i)^(1/3)/(2*(-i)) = e^(-i*pi/6)/(2*(-i)) = (i/2)*e^(-i*pi/6) = (1/2)*e^(i*pi/2)*e^(-i*pi/6) = (1/2)* e^(i*pi/3). Why is this not correct?