Kinetic Energy: Example Problems
This video gives an explanation of kinetic and contains several examples for calculating kinetic energy, mass and velocity using the kinetic energy equation. Kinetic energy is the energy an object possesses due to its motion. If an object is in motion then it has kinetic energy. It is als
From playlist Kinetic Energy, Potential Energy, Work, Power
Energy, Work, & Power, (1 of 31) Kinetic Energy, An Explanation
Explanation of kinetic energy, the units and the relationship of the kinetic energy of an object to its mass and velocity. Kinetic energy is the energy that an object has due to its motion. It is defined as the work needed to accelerate an object from rest to a specific velocity. The same
From playlist Kinetic Energy, Potential Energy, Work, Power
Energy, Work & Power (4 of 31) Kinetic Energy, Its Relationship to the Square of the Velocity
Explains the relationship between the increasing velocity of an object and its kinetic energy. The kinetic energy is proportional to the square of the velocity. Kinetic energy is the energy that an object has due to its motion. It is defined as the work needed to accelerate an object fro
From playlist Kinetic Energy, Potential Energy, Work, Power
Energy, Work & Power (2 of 31) Kinetic Energy, Example No. 1
This video shows you how to calculate the kinetic energy of an object in motion and the relationship between kinetic energy and work. Kinetic energy is the energy that an object has due to its motion. It is defined as the work needed to accelerate an object from rest to a specific velocit
From playlist Kinetic Energy, Potential Energy, Work, Power
Energy, Work & Power (7 of 31) Gravitational Potential Energy, Example No. 1
Show you how to calculate changes in gravitational potential energy. Gravitational potential energy is the energy that an object has due to its position relative to other objects. Potential energy is often referred to as stored energy. Gravitational potential energy is dependent on the ma
From playlist Kinetic Energy, Potential Energy, Work, Power
Energy, Work & Power (6 of 31) Gravitational Potential Energy, Work Done By an External Force
Explains the relationship between the change in gravitational potential energy and the work done by an external force. Gravitational potential energy is the energy that an object has due to its position relative to other objects. Potential energy is often referred to as stored energy. Gra
From playlist Kinetic Energy, Potential Energy, Work, Power
Like the video https://youtu.be/E-8P4nJqfVQ , this simulation shows how a sonic boom is created when an aircraft accelerates beyond the speed of sound, or when a boat accelerates to become faster than the speed of surface waves. Instead of the wave height and time-averaged energy, it shows
From playlist Wave equation
Energy and momentum in elastic collisions: from fizzics.org
In elastic collisions both momentum and energy are conserved. The tutorial demonstrates and simulates a number of different collisions and explains some of the mathematics used to analyse the outcomes.
From playlist Momentum energy and collisions
Turbulence: Arrow of time & equilibrium-nonequilibrium behaviour by Mahendra Verma
PROGRAM THERMALIZATION, MANY BODY LOCALIZATION AND HYDRODYNAMICS ORGANIZERS: Dmitry Abanin, Abhishek Dhar, François Huveneers, Takahiro Sagawa, Keiji Saito, Herbert Spohn and Hal Tasaki DATE : 11 November 2019 to 29 November 2019 VENUE: Ramanujan Lecture Hall, ICTS Bangalore How do is
From playlist Thermalization, Many Body Localization And Hydrodynamics 2019
Energy, Work & Power (5 of 31) Gravitational Potential Energy, An Explanation
Explains the what gravitational potential energy is. Also shows how to calculate changes in potential energy and explains the relationship between potential energy and work. Gravitational potential energy is the energy that an object has due to its position relative to other objects. Pot
From playlist Kinetic Energy, Potential Energy, Work, Power
Computational prediction technologies for turbulent flows by Charles Meneveau
Turbulence from Angstroms to light years DATE:20 January 2018 to 25 January 2018 VENUE:Ramanujan Lecture Hall, ICTS, Bangalore The study of turbulent fluid flow has always been of immense scientific appeal to engineers, physicists and mathematicians because it plays an important role acr
From playlist Turbulence from Angstroms to light years
Turbulence Closure Models: Reynolds Averaged Navier Stokes (RANS) & Large Eddy Simulations (LES)
Turbulent fluid dynamics are often too complex to model every detail. Instead, we tend to model bulk quantities and low-resolution approximations. To remain physical, these reduced approximations of the Navier-Stokes equations must be "closed", and turbulence closure modeling is one of t
From playlist Fluid Dynamics
Windfarm turbulence at 10^13 Angstroms, 10^-13 Lightyears by Charles Meneveau
Turbulence from Angstroms to light years DATE:20 January 2018 to 25 January 2018 VENUE:Ramanujan Lecture Hall, ICTS, Bangalore The study of turbulent fluid flow has always been of immense scientific appeal to engineers, physicists and mathematicians because it plays an important role acr
From playlist Turbulence from Angstroms to light years
Turbulence Energy Spectrum by Jayanta K. Bhattacharjee
Program Turbulence: Problems at the Interface of Mathematics and Physics (ONLINE) ORGANIZERS: Uriel Frisch (Observatoire de la Côte d'Azur and CNRS, France), Konstantin Khanin (University of Toronto, Canada) and Rahul Pandit (Indian Institute of Science, Bengaluru) DATE: 07 December 202
From playlist Turbulence: Problems at The Interface of Mathematics and Physics (Online)
Kinetic and Chemical Equilibration at Zero and Finite Density by Xiaojian Du
DISCUSSION MEETING EXTREME NONEQUILIBRIUM QCD (ONLINE) ORGANIZERS: Ayan Mukhopadhyay (IIT Madras) and Sayantan Sharma (IMSc Chennai) DATE & TIME: 05 October 2020 to 09 October 2020 VENUE: Online Understanding quantum gauge theories is one of the remarkable challenges of the millennium
From playlist Extreme Nonequilibrium QCD (Online)
Horizontal convection: ocean energetics, heat flux,... - Young - Workshop 1 - CEB T3 2019
Young (Scripps Institution of Oceanography, UC, San Diego) / 10.10.2019 Horizontal convection: ocean energetics, heat flux, upper-bounds and scaling I’ll begin by surveying the current understanding of the mechanical energy balance of the ocean i.e., the identification of the main s
From playlist 2019 - T3 - The Mathematics of Climate and the Environment
Lagrangian flows and turbulent irreversibility by Jeremie Bec
Turbulence from Angstroms to light years DATE:20 January 2018 to 25 January 2018 VENUE:Ramanujan Lecture Hall, ICTS, Bangalore The study of turbulent fluid flow has always been of immense scientific appeal to engineers, physicists and mathematicians because it plays an important role acr
From playlist Turbulence from Angstroms to light years
Energy Spectra and Fluxes in Buoyant Flows by Mahendra Kumar Verma
DISCUSSION MEETING WAVES, INSTABILITIES AND MIXING IN ROTATING AND STRATIFIED FLOWS (ONLINE) ORGANIZERS: Thierry Dauxois (CNRS & ENS de Lyon, France), Sylvain Joubaud (ENS de Lyon, France), Manikandan Mathur (IIT Madras, India), Philippe Odier (ENS de Lyon, France) and Anubhab Roy (IIT M
From playlist Waves, Instabilities and Mixing in Rotating and Stratified Flows (ONLINE)
Turbulence and non-thermal pressure in the intracluster medium by Xun Shi
Program Cosmology - The Next Decade ORGANIZERS : Rishi Khatri, Subha Majumdar and Aseem Paranjape DATE : 03 January 2019 to 25 January 2019 VENUE : Ramanujan Lecture Hall, ICTS Bangalore The great observational progress in cosmology has revealed some very intriguing puzzles, the most i
From playlist Cosmology - The Next Decade
Teach Astronomy - Kinetic Energy
http://www.teachastronomy.com/ Kinetic energy is the energy of motion. It depends on both mass and velocity and is defined mathematically as a half times the mass times the velocity squared. Thus, kinetic energy increases linearly with mass but as the square of the velocity. A small obj
From playlist 04. Chemistry and Physics