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  1. AP Physics C Mechanics
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Glossary

C

Conservative Force

Criticality: 3

A force for which the work done on an object is independent of the path taken, depending only on the initial and final positions.

Example:

Gravity is a conservative force; the work done by gravity on a ball thrown upwards and caught at the same height is zero, regardless of its trajectory.

D

Dissipative Forces

Criticality: 2

Forces that cause mechanical energy to be lost from a system, typically converting it into other forms like heat.

Example:

When a car brakes, the dissipative forces of friction between the brake pads and rotors convert kinetic energy into heat.

E

Elastic Potential Energy

Criticality: 3

The energy stored in a deformable elastic object, such as a spring, when it is stretched or compressed from its equilibrium position.

Example:

A toy dart gun stores elastic potential energy in its spring when cocked, which is then converted to kinetic energy to propel the dart.

Equilibrium

Criticality: 2

A state where the net force acting on an object is zero, often identified on a potential energy graph where the slope is zero.

Example:

A ball resting at the bottom of a bowl is in a stable equilibrium position, as any small displacement results in a restoring force.

F

Force as Negative Gradient of Potential Energy

Criticality: 3

A mathematical relationship stating that a conservative force can be found by taking the negative derivative (or gradient) of the potential energy function with respect to position (F = -dU/dr).

Example:

By analyzing a potential energy graph for a particle, you can determine the force as the negative gradient of potential energy at any point, indicating the direction and magnitude of the force.

G

Gravitational Force

Criticality: 3

The attractive force between any two objects with mass, which is a fundamental conservative force.

Example:

The gravitational force keeps satellites in orbit around Earth and causes objects to fall downwards.

Gravitational Potential Energy (General Case / Large Distances)

Criticality: 3

The potential energy of a system of two masses due to their mutual gravitational attraction, defined as U = -Gm1m2/r, with zero potential energy at infinite separation.

Example:

Calculating the energy required to launch a rocket into deep space involves considering the gravitational potential energy (general case / large distances) between the rocket and Earth.

Gravitational Potential Energy (Near Earth)

Criticality: 3

The potential energy an object possesses due to its position in a uniform gravitational field near the Earth's surface, given by ΔU = mgΔh.

Example:

Lifting a book from the floor to a shelf increases its gravitational potential energy (near Earth).

H

Hooke's Law

Criticality: 3

A principle stating that the force needed to extend or compress a spring by some distance is proportional to that distance, given by F_s = -kΔx.

Example:

When you pull back the string of a bow, the force exerted by the bowstring follows Hooke's Law, storing energy for the arrow's launch.

N

Newton's Law of Universal Gravitation

Criticality: 2

A law stating that every particle attracts every other particle in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

Example:

The orbit of the Moon around the Earth is governed by Newton's Law of Universal Gravitation.

P

Path Independence

Criticality: 2

A characteristic of conservative forces where the work done by the force on an object moving between two points does not depend on the specific path taken.

Example:

When climbing a mountain, the work done by gravity on you depends only on your change in vertical height, demonstrating path independence.

Potential Energy Wells

Criticality: 2

Local minimums on a potential energy versus position graph, representing stable equilibrium points where a particle can oscillate.

Example:

An atom in a molecule can be thought of as sitting in a potential energy well, oscillating around its stable bond length.

R

Restoring Force

Criticality: 2

A force that always acts to bring a system back to its equilibrium position, often seen in springs.

Example:

The force that pulls a pendulum bob back towards its lowest point after being displaced is a restoring force.

S

Spring Constant (k)

Criticality: 3

A measure of the stiffness of a spring, indicating how much force is required to stretch or compress it by a unit distance.

Example:

A car's suspension system uses springs with a specific spring constant to absorb shocks and provide a smooth ride.

Spring Force

Criticality: 3

The force exerted by a spring when it is compressed or stretched, acting to restore the spring to its equilibrium length.

Example:

The spring force in a pogo stick pushes the rider upwards after the spring is compressed.

T

Total Mechanical Energy

Criticality: 3

The sum of the kinetic energy and all forms of potential energy within a system, which is conserved in the absence of non-conservative forces.

Example:

In a frictionless roller coaster, the total mechanical energy of the car remains constant, converting between kinetic and gravitational potential energy.

W

Work-Potential Energy Relationship

Criticality: 3

The principle that the work done by a conservative force is equal to the negative change in the system's potential energy (W = -ΔU).

Example:

As a roller coaster car descends, the work done by gravity is positive, and its gravitational potential energy decreases, illustrating the work-potential energy relationship.

Z

Zero Work in Closed Path

Criticality: 2

A property of conservative forces where the total work done by the force on an object moving along any closed loop is zero.

Example:

If you push a box around a complete circle on a frictionless surface, the net work done by the spring force (if attached) would be zero work in a closed path.