AP Physics 1 Review

AP Physics Full Review: Past Exam Breakdown

  • Key Topic Breakdown of Exam Content:

    • Energy (25%)

    • Dynamics/Newton's Law (20%)

    • Kinematics (17%)

    • Rotational Motion (16%)

    • Momentum (14%)

    • Circular Motion/Gravitation (5%)

    • Simple Harmonic Motion (3%)

  • Study Tip: Focus on vocabulary, definitions, and formulas as key components for success in physics exams.

Kinematic Equations and Motion Graphs

  • Graphs Understanding:

    • In a position graph, the slope represents velocity.

    • In a velocity graph, the slope indicates acceleration and the area under the curve represents displacement.

    • In an acceleration graph, the area under the line represents velocity.

  • Basic Formulas:

    • Acceleration: a=ΔvΔta = \frac{\Delta v}{\Delta t}

    • Velocity (general): v=dtv = \frac{d}{t}

    • Average Velocity: V1+V2/2

Projectile Motion

  • Basic Principles:

    • Horizontal Motion: characterized by velocity, displacement, and time.

    • Vertical Motion: characterized by initial velocity, final velocity, displacement, time, and acceleration.

    • Key Connection: The horizontal time is equal to the vertical time.

    • Use kinematic equations first to derive vertical quantities, then apply them to find horizontal quantities.

    • At the highest point of a projectile's path, t=Voygt = \frac{-V_{oy}}{-g}.

  • Including Angles:

    • Decompose projectile motion into horizontal and vertical components.

    • Apply kinematics: for projectile motion problems, use the average velocity equation for horizontal quantities, V=dtV = \frac{d}{t}.

    • If launched at an angle, utilize sine for vertical displacement and cosine for horizontal displacement:

    • Horizontal range: R=Voy2sin(2θ)gR = \frac{V_{oy}^2 \sin(2\theta)}{g}, where θ\theta is the launch angle.

Forces and Newton's Laws

  • Newton’s Laws of Motion:

    1. An object at rest will remain at rest unless acted upon by a net force; an object in motion maintains its velocity unless acted upon by a net force.

    2. The acceleration of an object is proportional to the net force acting on it and inversely proportional to its mass: a=Fnetma = \frac{F_{net}}{m}.

    3. For every action, there is an equal and opposite reaction (involves two forces acting on two objects).

  • Equilibrium Concepts:

    • Static Equilibrium: Occurs when the net force is zero for a motionless system.

    • Dynamic Equilibrium: Occurs when the net force is zero for a moving system (no acceleration, constant velocity).

    • If an object is not accelerating, all forces must be balanced.

  • Normal Force and Friction:

    • Normal Force (Fn): Acts perpendicular to the contact surface, calculated typically as Fg=mgF_{g} = mg.

    • Friction Force (Ff): Acts parallel to the contact surface:

    • Static Friction (F<em>sF<em>{s}): Resists the start of motion and is dependent on the applied force until the maximum is reached: Fs < \mus Fn.

    • Kinetic Friction (F<em>kF<em>{k}): Acts on moving objects: F</em>k=μ<em>kF</em>nF</em>k = \mu<em>k F</em>n.

  • Slope Components in Forces:

    • Use sine components to describe sliding motion and cosine components to maintain object proximity to the ramp, coscos into the ramp, and sinsin going downwards.

Atwood Machines and Tension Analysis

  • System Description:

    • Two masses are connected by a massless string over a massless frictionless pulley.

    • Tension is uniform across the string.

    • Both masses will have equal acceleration, Fnet=maF_{net} = ma and tension analysis yields:

    • T=mgmaT = m_{g} - ma.

    • Conditions for equilibrium are indicated when m<em>1+m</em>2m<em>1 + m</em>2 leads to equilibrium; otherwise, acceleration occurs.

  • Key Motion Concepts:

    • For an object sliding down a frictionless ramp, the end velocity can be determined using v=2ghv = \sqrt{2gh}.

Work, Energy, and Power

  • Work Defined:

    • Work (W) is the energy transfer to or from an object by means of force causing a displacement.

    • It is a scalar quantity, defined by the formula: W=Fdcos(θ)W = Fd \cos(\theta) or alternatively W=KE<em>fKE</em>iW = KE<em>f - KE</em>i.

  • Work Classifications:

    • Positive Work: Adds mechanical energy when the force and displacement are in the same direction (0° < Θ < 90°).

    • Negative Work: Extracts mechanical energy when the force and displacement are in opposite directions (90° < Θ < 180°).

    • Zero Work: Occurs when force is perpendicular to the direction of motion.

  • Energy Types:

    • Kinetic Energy (KE): Energy of motion, given by KE=12mv2KE = \frac{1}{2}mv^2 (if KE is doubled, velocity increases by 2\sqrt{2}).

    • Potential Energy (PE): Energy based on position, specifically gravitational potential energy: Ug=mghU_g = mgh.

    • Gravitational PE relates to height, where 12v2=gh\frac{1}{2}v^2 = gh due to mass cancelling out when frictionless.

    • Elastic Potential Energy is defined as: Us=12kx2U_s = \frac{1}{2}kx^2 where k is spring constant.

  • Conservation Laws:

    • Total energy in an isolated system remains constant; mechanical energy is conserved absent friction.

    • Work is required to change the total mechanical energy of a system.

  • Power Defined:

    • Power (P) measures the rate of energy change or working: P=WtP = \frac{W}{t} (measured in watts, with $1 W = 1 J/s$).

    • Extended calculations: P=Fvcos(θ)P = Fv \cos(\theta) can connect force, velocity, and angle to power interpretation.

Momentum and Impulse

  • Momentum (p): Defined as the tendency for an object to remain in motion, momentum is conserved in isolated systems. Momentum is related by:

    • p=mvp = mv.

  • Impulse (J): Change in momentum of an object, defined by:

    • J=FΔt=Δ(mv)J = F \Delta t = \Delta (mv).

  • Impulse is represented graphically as the area under a force vs. time graph.

  • Collision Types:

    • Elastic Collisions: Both momentum and kinetic energy conserved; often seen in hard collisions where objects bounce off.

    • Conservation Law: P<em>1i+P</em>2i=P<em>1f+P</em>2fP<em>{1i} + P</em>{2i} = P<em>{1f} + P</em>{2f}.

    • Inelastic Collisions: Only momentum is conserved; objects may stick together post-collision but kinetic energy is not conserved.

    • Explosions: Begin as a single object and split into parts without conserving kinetic energy but do conserve momentum.

Center of Mass, Systems

  • Center of Mass (CM): Balance point in a system, mathematically determined by:

    • Establish a coordinate point ($x=0$) and for each component multiply its mass by its distance, summing these and dividing by total mass.

  • System Types:

    • Open systems swap energy up/down with surroundings.

    • Closed systems conserve energy without external energy change; friction indicates an open system, while mechanical energy is conserved when friction is absent.

Circular Motion and Gravitation

  • Uniform Circular Motion Characteristics:

    • It's where an object moves in a circular path at constant tangential speed, while continuously changing its direction.

    • Tangential Speed (v): Remains consistent; tangential velocity varies due to direction change.

  • Centripetal Motion Dynamics:

    • Centripetal Acceleration (Aₙ): Always directed towards the center: Ac=v2rA_c = \frac{v^2}{r}.

    • Centripetal Force (F_c): Required to maintain circular motion and is given by:

    • F<em>c=mv2rF<em>c = m \frac{v^2}{r} or F</em>c=mw2rF</em>c = mw^2r for circular motion on a string.

    • For planetary orbits, gravitational force acts as centripetal force.

  • Gravitation Principles:

    • Newton’s Law of Universal Gravitation:

    • F<em>g=Gm</em>1m2r2F<em>g = \frac{G m</em>1 m_2}{r^2}, where G is the gravitational constant (6.67 x 10^-11).

    • Gravitational Field Strength (g): Field strength defined as g=GMr2g = \frac{GM}{r^2} (9.81 m/s² at Earth's surface).

    • Gravitational Potential Energy (Ug): Potential energy between two masses given by U<em>g=Gm</em>1m2rU<em>g = \frac{G m</em>1 m_2}{r}.

Rotational Motion Basics

  • Rotational Dynamics and Quantities:

    • Translational vs. Angular Motion:

    • Translational: moves across space; Angular: rotates.

    • Rotational motion combines aspects of both.

    • Angular Velocity (ω): defined as the angle/time period.

  • Angular Acceleration (α): Rate of change in angular velocity; defined through:

    • α=Δωtα = \frac{\Delta \omega}{t}.

  • Torque (T): Defined as the force that causes rotational motion, given by:

    • T=Frsin(θ)T = F r \sin(θ) where θ is the angle between lever arm and applied force. The unit is Newton-meters (N·m).

  • Equilibrium in Rotational Mechanics:

    • Rotational equilibrium occurs when net torque is zero, analyzed similarly to net force considerations in translational equilibrium.

Simple Harmonic Motion (SHM)

  • Foundational Concepts:

    • SHM is characterized by a restoring force proportional to displacement from equilibrium.

    • Key definitions include:

    • Amplitude (A): Maximum displacement.

    • Period (T): Time for one full cycle, given as T=2π(m/k)T = 2π√(m/k) for mass-spring systems.

    • Frequency (f): Cycles per time: f=1Tf = \frac{1}{T}.

  • Hooke's Law: Describes restoring force in terms of displacement and spring constant:

    • Fs=kxF_s = kx.

    • Restoring Forces: These forces bring the system back to equilibrium point.

Waves and Sound

  • Parts of Transverse Waves:

    • Crests and Troughs: Maximum displacements above and below equilibrium, respectively.

    • Wavelength (λ): Distance between successive crests or troughs.

    • Amplitude and Frequency: Key features defining wave properties.

  • Wave Speed: Described by:

    • v=fλv = fλ and v=dtv = \frac{d}{t}.

    • Constant wave speeds depend on medium characteristics, independent of frequency.

  • Superposition and Interference:

    • When two waves overlap, their displacements combine algebraically.

    • Constructive and Destructive Interference: Describes how waves interact and form new wave patterns.

  • Doppler Effect: Observed when a wave source moves relative to an observer, altering perceived frequency:

    • Higher frequency when moving closer, lower when moving apart.

Electric Forces and Fields

  • Basic Concepts of Charge:

    • Atoms contain protons, neutrons and electrons; charge is conserved.

    • Ionic Charge: Produced by imbalance in protons and electrons (adding/removing electrons changes total charge).

  • Coulomb’s Law: Governs the interaction of charged particles:

    • F<em>E=kq</em>1q2r2F<em>E = k \frac{|q</em>1 q_2|}{r^2}.

    • States that electric force is attractive for unlike charges and repulsive for like charges.

  • Electric Field (E): Related to the charge and force experienced by a test charge:

    • E=FqE = \frac{F}{q},

    • Field strength inversely correlates with the distance from the charge, with denser field lines indicating stronger fields.

  • Superposition Principle: The resultant electric field is the vector sum of all individual fields.

Direct Current Circuits

  • Electric Current Concept: Defined as the flow of electric charge:

    • Measure of charge crossing a plane per time: Iavg=QtI_{avg} = \frac{∆Q}{∆t} (1 A = 1 C/s).

    • Current direction conventionally taken as flow of positive charge.

  • Resistance is analogous to flow obstruction, defined by Ohm’s Law:

    • R=VIR = \frac{V}{I} and also reducible via R=ρLAR = \frac{\rho L}{A} with ρ\rho as resistivity.

  • Electric Circuit Elements:

    • Emf represents work per charge; voltage provides energy to charges.

  • Circuit Analysis and Kirchhoff's Rules:

    • Momentum through junctions must balance, total potential must sum to zero in closed loops.

    • Analyze volts dropped/increased across components based on current direction and resistive properties.

In physics, the magnitude of a vector quantity refers to its size or strength without regard to its direction. To solve for the magnitude of a vector, you typically apply the Pythagorean theorem if you have the vector's components. The basic formula for finding magnitude is:
V=V<em>x2+V</em>y2|V| = \sqrt{V<em>x^2 + V</em>y^2}
where:

  • V|V| is the magnitude of the vector V.

  • VxV_x is the horizontal component of the vector.

  • V<em>yV<em>y is the vertical component of the vector. For three-dimensional vectors, the formula extends to: V=V</em>x2+V<em>y2+V</em>z2|V| = \sqrt{V</em>x^2 + V<em>y^2 + V</em>z^2}
    where VzV_z is the vertical component in three dimensions.