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Motion Study Guide
Motion Study Guide

... 16. A steel ball whose mass is 2.0 kg is rolling at a rate of 2.8 m/s. What is its momentum? p = mv = (2.0 kg)(2.8 m/s) = 5.6 kg*m/s 17. A race car leaves the starting line and travels 36000 m in the first 600 seconds of the race. They are then forced to take a pit stop and don’t go anywhere for 250 ...
Slide 1
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FAQ- Generating Representative Inputs to a Model Under Construction
FAQ- Generating Representative Inputs to a Model Under Construction

Newton`s Laws - Cobb Learning
Newton`s Laws - Cobb Learning

... Push and Pull ...
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Solving Momentum Problems
Solving Momentum Problems

Lecture13-10
Lecture13-10

... ball at the elephant with a speed of 7.81 m/s. When the ball bounces back toward you, what is its speed? Our simplest formulas for speed after an elastic collision relied on one body being initially at rest. So lets try a frame where one body (the ball) is at rest! What is the speed of the elephant ...
APPLICATION OF FORCES
APPLICATION OF FORCES

... • The forces that might act on a rotating body are air resistance or friction. • ICE SKATING example in revision pack… • Skaters spin on the ice with arms out = SLOW spin as air resistance acts on arms • Bring their arms into ‘streamline position’ = FASTER spin as less air resistance • This is becau ...
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Document

... 1- Chemical Energy: Energy from an objects position. (Potential Energy) 2- Electrical Energy: Energy that flows through a wire (Kinetic Energy) 3- Energy: The ability to do work. 4- Internal Energy: Energy to the particles that make it up. 5- Joule: Metric Unit for energy. ...
Get Notes - Mindset Learn
Get Notes - Mindset Learn

... Two blocks of masses 20 kg and 5 kg respectively are connected by a light inextensible string, P. A second light inextensible string Q, attached to the 5 kg block, runs over a light frictionless pulley. A constant horizontal force of 250 N pulls the second string as shown in the diagram below. The m ...
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Energy Forms Notes

Chapter 21 Rigid Body Dynamics: Rotation and Translation
Chapter 21 Rigid Body Dynamics: Rotation and Translation

... gravitational force does not contribute to the torque because it is acting at the center of mass. We draw a torque diagram in Figure 21.7a showing the location of the point of application of the forces, the point we are computing the torque about (which in this case ...
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Chapter 4

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Chapter 4 Energy and Stability

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Conservation of Energy

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Momentum

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M1.4 Dynamics

... The impulse on a body is defined as its change in momentum. Impulse = change in momentum = mv – mu where u is the initial velocity and v is the final velocity. Impulse is denoted by the vector I. Note that the impulse I that a body A exerts on a body B is equal to the magnitude of the impulse that B ...
Problem 6C - Cobb Learning
Problem 6C - Cobb Learning

Conservation of Energy
Conservation of Energy

...  As the apple falls to the ground, its height decreases. Therefore, its GPE decreases.  The potential energy is not lost… it is converted into kinetic energy as the velocity of the apple increases.  What happens to the mechanical energy? ...
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Conservation of Energy

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Chapter 5 Work and Friction

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Conservation of Energy

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Energy Unit Concept Review Questions

Space Time and Gravity - Florida State University
Space Time and Gravity - Florida State University

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141S13-NotesCh6a-June04

< 1 ... 229 230 231 232 233 234 235 236 237 ... 437 >

Relativistic mechanics

In physics, relativistic mechanics refers to mechanics compatible with special relativity (SR) and general relativity (GR). It provides a non-quantum mechanical description of a system of particles, or of a fluid, in cases where the velocities of moving objects are comparable to the speed of light c. As a result, classical mechanics is extended correctly to particles traveling at high velocities and energies, and provides a consistent inclusion of electromagnetism with the mechanics of particles. This was not possible in Galilean relativity, where it would be permitted for particles and light to travel at any speed, including faster than light. The foundations of relativistic mechanics are the postulates of special relativity and general relativity. The unification of SR with quantum mechanics is relativistic quantum mechanics, while attempts for that of GR is quantum gravity, an unsolved problem in physics.As with classical mechanics, the subject can be divided into ""kinematics""; the description of motion by specifying positions, velocities and accelerations, and ""dynamics""; a full description by considering energies, momenta, and angular momenta and their conservation laws, and forces acting on particles or exerted by particles. There is however a subtlety; what appears to be ""moving"" and what is ""at rest""—which is termed by ""statics"" in classical mechanics—depends on the relative motion of observers who measure in frames of reference.Although some definitions and concepts from classical mechanics do carry over to SR, such as force as the time derivative of momentum (Newton's second law), the work done by a particle as the line integral of force exerted on the particle along a path, and power as the time derivative of work done, there are a number of significant modifications to the remaining definitions and formulae. SR states that motion is relative and the laws of physics are the same for all experimenters irrespective of their inertial reference frames. In addition to modifying notions of space and time, SR forces one to reconsider the concepts of mass, momentum, and energy all of which are important constructs in Newtonian mechanics. SR shows that these concepts are all different aspects of the same physical quantity in much the same way that it shows space and time to be interrelated. Consequently, another modification is the concept of the center of mass of a system, which is straightforward to define in classical mechanics but much less obvious in relativity - see relativistic center of mass for details.The equations become more complicated in the more familiar three-dimensional vector calculus formalism, due to the nonlinearity in the Lorentz factor, which accurately accounts for relativistic velocity dependence and the speed limit of all particles and fields. However, they have a simpler and elegant form in four-dimensional spacetime, which includes flat Minkowski space (SR) and curved spacetime (GR), because three-dimensional vectors derived from space and scalars derived from time can be collected into four vectors, or four-dimensional tensors. However, the six component angular momentum tensor is sometimes called a bivector because in the 3D viewpoint it is two vectors (one of these, the conventional angular momentum, being an axial vector).
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