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Solutions to Problems
Solutions to Problems

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Video 3rd Law in Action

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Lesson 2: Work – Kinetic Energy Theorem

Force, Mass, Acceleration, and Friction
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... Newton’s Second Law of Motion – the net force acting on an object causes the object to accelerate in the direction of the net force. The acceleration of an object is determined by the size of the net force and the mass of the object. a = F / m, where F is measured in Newtons (N) and mass is measured ...
Chapter 10 Simple Harmonic Motion and Elasticity continued
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... Machine – a device used to make work easier by adjusting the amount or direction of force applied to the object - purpose is to reduce the amount of work you have to put in - law of conservation of energy: o energy cannot be created nor destroyed, only change form/transferred  machine cannot increa ...
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... 43. According to the Standard Model, a proton is constructed of two up quarks and one down quark (uud) and a neutron is constructed of one up quark and two down quarks (udd). During beta decay, a neutron decays into a proton, an electron, and an electron antineutrino. During this process there is a ...
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... in my experience students are more often distracted by a computer and take poor notes as a result. In addition, we will regularly draw diagrams or pictures, which is very difficult or impossible to do in such a device unless you have a stylus. So while I will allow the use of a laptop or other typin ...
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electric circuits

... A spring with a mass of 2 kg has natural length 0.5 m. A force of 25.6 N is required to maintain it stretched to a length of 0.7 m.  If the spring is stretched to a length of 0.7 m and then released with initial velocity 0, find the position of the mass at any time t. ...
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Classical central-force problem



In classical mechanics, the central-force problem is to determine the motion of a particle under the influence of a single central force. A central force is a force that points from the particle directly towards (or directly away from) a fixed point in space, the center, and whose magnitude only depends on the distance of the object to the center. In many important cases, the problem can be solved analytically, i.e., in terms of well-studied functions such as trigonometric functions.The solution of this problem is important to classical physics, since many naturally occurring forces are central. Examples include gravity and electromagnetism as described by Newton's law of universal gravitation and Coulomb's law, respectively. The problem is also important because some more complicated problems in classical physics (such as the two-body problem with forces along the line connecting the two bodies) can be reduced to a central-force problem. Finally, the solution to the central-force problem often makes a good initial approximation of the true motion, as in calculating the motion of the planets in the Solar System.
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