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Kinetic Energy -Work-Kinetic Energy Theorem
Kinetic Energy -Work-Kinetic Energy Theorem

Law of Conservation of Energy
Law of Conservation of Energy

... Even after the diver enters the water, the energy has not disappeared. It is eventually mostly converted into thermal energy which remains in the room, or dissipates out into the environment. Although the above example illustrates several complicated energy transformations, generally it’s only the t ...
2. Work, Energy and Conservation of Energy
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Chapter 2: Basic Concepts of Thermodynamics Thermodynamics
Chapter 2: Basic Concepts of Thermodynamics Thermodynamics

... processes occur in the direction of decreasing quality of energy. Whenever there is an int eraction between energy and matter, ther modynamics is involved. Some examples include heating and air-conditioning systems, refrigerators, water heaters, etc. ...
The gravitational force exerted by the earth on the moon holds the
The gravitational force exerted by the earth on the moon holds the

1. The diagram shows two forces acting at right angles to each other
1. The diagram shows two forces acting at right angles to each other

... 14. A space vehicle of mass 120 kg is falling vertically, towards a planet. The gravitational field strength at this point is 3.5 N/kg. The vehicle fires a rocket engine which applies a steady upward force of 660 N to the vehicle. 11. A mass of 1 kg is pulled along a level bench by a horizontal forc ...
Newton`s Second Law F=ma
Newton`s Second Law F=ma

... second Law using vectors? Warm-up: •Make Entry for “Newton’s Second Law” in your TOC •Answer the following: Imagine you are running from zombies, and the only way you will escape is through a brick wall that is too tall to climb. Next to the wall are these tools to use to break the wall: ...
Linear Impulse and Momentum
Linear Impulse and Momentum

17AP_Physics_C_-_Rotational_Motion_II
17AP_Physics_C_-_Rotational_Motion_II

17AP_Physics_C_-_Rotational_Motion_II
17AP_Physics_C_-_Rotational_Motion_II

... Angular Momentum is also conserved Here is what this says: IF THE NET TORQUE is equal to ZERO the CHANGE ANGULAR MOMENTUM is equal to ZERO and thus the ANGULAR MOMENTUM is CONSERVED. Here is a common example. An ice skater begins a spin with his arms out. His angular velocity at the beginning of th ...
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... GRAVITATIONAL FIELD Field lines are drawn such that - The tangent to the field represents the direction of g. - The number of field lines per unit cross-sectional area is proportional to the magnitude of g. ...
Energy
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17AP_Physics_C_-_Rotational_Motion_II
17AP_Physics_C_-_Rotational_Motion_II

... to ZERO the CHANGE ANGULAR MOMENTUM is equal to ZERO and thus the ANGULAR MOMENTUM is CONSERVED. Here is a common example. An ice skater begins a spin with his arms out. His angular velocity at the beginning of the spin is 2.0 rad/s and his moment of inertia is 6 kgm2. As the spin proceeds he pulls ...
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... combination of units is used so frequently that it has been given a name of its own: the joule (J). ...
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Energy in SHM - Ryerson Department of Physics
Energy in SHM - Ryerson Department of Physics

... of time. We can also describe the system from an energy perspective. In this experiment, you will measure the position and velocity as a function of time for an oscillating mass and spring system, and from those data, plot the kinetic and potential energies of the system. Energy is present in three ...
CBSE Class 9 Work Energy and Power Solved test paper-05
CBSE Class 9 Work Energy and Power Solved test paper-05

... When a satellite moves around the Earth in a circular path, then the force of gravity acts on it directed towards the centre. The motion of the satellite is in the horizontal plane. Therefore, the force of gravity of Earth on the satellite and the direction of motion of satellite are perpendicular t ...
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8.4 Conservation of Energy Part II
8.4 Conservation of Energy Part II

W = ΔK =1/2mv2 f −1/2mv0
W = ΔK =1/2mv2 f −1/2mv0

Rotational Dynamics
Rotational Dynamics

...  Equation: F·r = I·; the units for rotational inertia are kg·m2/rad2.  Rotational inertia and legs: short legs have less rotational inertia than long legs. An animal with shorter legs has a quicker stride than one with long legs (same is true for pendulums). When running, we bend our legs to redu ...
6-2 Energy
6-2 Energy

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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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