Classical Mechanics Quiz

Definition: Branch of physics dealing with the motion of bodies under the influence of forces.
Fundamental Principles:
- Newton's Laws of Motion.
- Conservation Laws.
- Energy and Work.

First Law (Inertia):
- An object at rest remains at rest and an object in motion continues in motion at constant velocity unless acted upon by a net external force.
Second Law (F=ma):
- The acceleration (a) of an object is directly proportional to the net force (F) acting on it and inversely proportional to its mass (m).
- Formula: F = ma.
Third Law (Action-Reaction):
- For every action, there is an equal and opposite reaction.

Types of Motion:
- Linear (straight line).
- Circular (movement along a circular path).
- Projectile (motion of an object thrown into the air).
- Rotational (motion around an axis).
Equations of Motion (for uniformly accelerated motion):
- ( v = u + at )
- ( s = ut + \frac{1}{2}at^2 )
- ( v^2 = u^2 + 2as )
where:
- ( v ) = final velocity
- ( u ) = initial velocity
- ( a ) = acceleration
- ( s ) = displacement
- ( t ) = time

Types of Forces:
- Gravitational (attraction between masses).
- Normal (perpendicular support force).
- Frictional (opposes motion).
- Tension (force in strings or ropes).
- Applied (external force).
Net Force: The vector sum of all forces acting on an object. Determines motion according to Newton’s Second Law.

Kinetic Energy (KE): Energy of motion.
- Formula: ( KE = \frac{1}{2} mv^2 )
Potential Energy (PE): Stored energy based on position.
- Gravitational PE formula: ( PE = mgh )
Conservation of Energy: The total mechanical energy (KE + PE) in a closed system remains constant.

Definition: Work is done when a force causes a displacement.
Formula:
- ( W = Fd \cos(\theta) )
- Where ( W ) = work, ( F ) = force, ( d ) = displacement, ( \theta ) = angle between force and displacement direction.

Definition: The product of an object's mass and its velocity.
Formula: ( p = mv )
Conservation of Momentum: In a closed system, the total momentum before an interaction is equal to the total momentum afterward.

Reference Frames: The perspective from which motion is observed (inertial vs. non-inertial).
Closed Systems: No external forces acting.

Projectile Motion: Analyzing objects moving in two dimensions under gravity.
Circular Motion: Understanding forces and energy in systems like satellites and rotating objects.

Classical mechanics is a fundamental branch of physics that studies the motion of objects under the influence of forces.
It is built on the principles of Newton's Laws of Motion, Conservation Laws, Energy and Work.

First Law (Inertia): An object at rest will remain at rest or in motion unless it is acted upon by an external force.
Second Law (F=ma): The acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass. This is represented by the equation: F = ma, where F is force, m is mass, and a is acceleration.
Third Law (Action-Reaction): For every action, there is an equal and opposite reaction.

Motion is the change in position of an object over time. It can be linear, circular, projectile, rotational, or a combination.
Linear motion occurs in a straight line.
Circular motion describes movement along a circular path.
Projectile motion is the motion of an object thrown into the air, influenced by gravity and an initial velocity.
Rotational motion describes movement around an axis.
Uniformly Accelerated Motion is when an object's acceleration is constant. There are three important equations of motion:
- ( v = u + at ): Final velocity (v) is the initial velocity (u) plus acceleration (a) multiplied by time (t)
- ( s = ut + \frac{1}{2}at^2 ): Displacement (s) is the initial velocity (u) multiplied by time (t) plus half of the acceleration (a) multiplied by the square of time (t).
- ( v^2 = u^2 + 2as ): The square of the final velocity (v) is equal to the square of the initial velocity (u) plus twice the acceleration (a) multiplied by the displacement (s)

Forces are interactions that can cause a change in motion.
Types of forces:
- Gravitational force: The force of attraction between any two objects with mass.
- Normal force: A perpendicular force that a surface exerts on an object in contact with it.
- Frictional force: A force that opposes motion between two surfaces in contact.
- Tension force: The force transmitted through a string, rope, or cable when pulled taut.
- Applied force: An external force applied to an object.
Net force: The vector sum of all forces acting on an object. The net force determines the acceleration of an object according to Newton's Second Law.

Kinetic energy (KE): The energy of motion. It is calculated using the formula ( KE = \frac{1}{2} mv^2 ), where m is mass and v is velocity.
Potential energy (PE): Stored energy based on an object's position. Gravitational potential energy is calculated using ( PE = mgh ), where m is mass, g is the acceleration due to gravity, and h is the height.
Conservation of energy: States that the total mechanical energy (KE + PE) in a closed system remains constant.

Work is done when a force causes a displacement. It is calculated using ( W = Fd \cos(\theta) ). Where W is work, F is force, d is displacement, and (\theta) is the angle between force and displacement direction.

Momentum: The product of an object's mass and its velocity. It is calculated using ( p = mv ), where p is momentum, m is mass, and v is velocity.
Conservation of momentum: In a closed system, the total momentum before an interaction is equal to the total momentum afterward.

Reference frames: The perspective from which motion is observed. Inertial reference frames are those where Newton's laws of motion are directly applicable. Non-inertial reference frames are those that are accelerating.
Closed systems: Systems that have no external forces acting on them and no exchange of energy with the surroundings.

Projectile motion: The analysis of objects moving in two dimensions under the influence of gravity.
Circular motion: Understanding forces and energy in systems like satellites, rotating objects, and amusement park rides.

Identify known and unknown variables: Determine what information is given and what needs to be calculated.
Draw free-body diagrams: Illustrate all the forces acting on an object.
Apply relevant equations of motion and conservation principles: Use the appropriate equations and principles to solve the problem.