Comprehensive Physics Study Guide: Forces, Energy Conservation, and Momentum
Fundamentals of Dynamics: Newton's Laws and Types of Forces
Definition and Properties of Force:
A force is defined as a push or a pull acting on an object.
Every force is exerted by an identifiable agent and acts directly on a recipient object.
Force is a vector quantity, possessing both magnitude and direction.
Forces are categorized by interaction type into contact forces (requiring direct physical contact between surfaces) and long-range forces (acting across space without physical contact, such as gravity).
The standard SI unit of force is the Newton (N), defined as the compound unit: 1N=1kg⋅m/s2
English equivalent units include the pound (lb) and slug for mass, where on Earth's surface a mass of 1kg corresponds to approximately 2.2lbs.
Fundamental Forces of Nature:
All known forces in the universe reduce to four fundamental interactions:
Gravitational Force: An attractive force between masses, responsible for weight.
Electromagnetic Force: Responsible for all macroscopic contact forces, including normal force, tension, friction, and spring forces, as well as chemical bonding.
Weak Nuclear Force: Governs subatomic interactions and radioactive decay processes.
Strong Nuclear Force: Binds quarks together inside protons and neutrons, holding atomic nuclei together against electromagnetic repulsion.
Newton's Laws of Motion:
Newton's First Law (Law of Inertia): An object in motion remains in motion at a constant velocity, and an object at rest remains at rest, unless acted upon by a net external force. When the net force is zero (ΣF=0), the acceleration is zero (a=0), maintaining constant velocity.
Newton's Second Law: The net force acting on an object of mass m is directly proportional to its acceleration: ΣF=ma
Mass (m) is an inherent scalar property measuring an object's inertia (resistance to acceleration), with standard SI units of kilograms (kg, where 1000g=1kg).
Broken down into orthogonal Cartesian components: ΣFx=maxΣFy=may
Newton's Third Law (Action-Reaction): For every force exerted on an object by an agent, there is an equal in magnitude and opposite in direction force exerted by the object back on the agent: F1 on 2=−F2 on 1
Pushing against an object with 100N causes the object to exert 100N back on the pusher.
When the Earth exerts a downward gravitational force of 10N on an object, the object exerts an equal upward gravitational force of 10N on the Earth.
Standard Force Classifications in Mechanics:
Weight (Fg or mg): The downward gravitational force exerted on mass m by the Earth: Fg=mg
On Earth's surface, the standard acceleration due to gravity is g=9.81m/s2.
Normal Force (N): The supporting contact force exerted perpendicular to the interface between two contacting surfaces. The normal force must always be solved for using equilibrium equations; it is never automatically assumed equal to mg.
Tension (T): The pulling force transmitted through an ideal string, rope, or cable. Tension always pulls away from the object along the line of the rope. An ideal light string running over an ideal massless, frictionless pulley maintains the same tension throughout its length.
Spring Force (Fs): Governed by Hooke's Law, representing the restoring force exerted by a deformed spring: Fs=kx
k is the spring constant (stiffness) measured in N/m, and x is the displacement from equilibrium.
Drag Force (D): Fluid resistance (air or water) opposing velocity: D=bv2
b represents an aerodynamic drag factor.
Thrust: Driving force generated internally (e.g., rocket or jet exhaust).
Force Problem-Solving Methodology and Incline Plane Analysis
Standardized Systematic Procedure:
Step 1: Read the problem carefully and identify the physical system.
Step 2: Draw a physical diagram showing all interactions.
Step 3: Draw an isolated Free Body Diagram (FBD) for each object, replacing the object with a dot and drawing all external forces as vectors pointing outward from the dot.
Step 4: Establish a Cartesian coordinate system. Identify the direction of acceleration and align axes to maximize the number of forces lying on the axes.
Step 5: Resolve non-aligned force vectors into components: Fx=Fcos(θ)Fy=Fsin(θ)
In general, if angle ϕ is measured relative to the vertical axis: Fx=Fsin(ϕ)Fy=Fcos(ϕ)
Step 6: Write Newton's Second Law component equations: ΣFx=maxΣFy=may
Step 7: List all knowns and unknowns.
Step 8: Solve the algebraic system symbolically for the requested variables before substituting numerical values.
Conditions Where ΣF=0:
Static Equilibrium: The object is not moving in the specified coordinate direction (v=0, a=0).
Dynamic Equilibrium: The object is moving with constant velocity in that coordinate direction (v=constant, a=0).
Apparent Weight and Elevator Dynamics:
Apparent weight is defined as the magnitude of the supporting normal force (N) felt by or measured on an object.
Stationary or Constant Velocity Elevator (ay=0):ΣFy=N−mg=0⟹N=mg
Complete apparent weightlessness occurs because both the person and the elevator floor accelerate downward at g.
Inclined Planes (Ramps):
Standard axes are tilted such that the x′-axis is parallel to the incline surface and the y′-axis is perpendicular to the surface.
This alignment ensures that acceleration occurs purely along the x′-axis (ax=a), while acceleration perpendicular to the ramp is zero (ay=0).
Gravity (mg) acts straight down, making an angle θ with the negative y′-axis (where θ is the ramp angle with the horizontal): (mg)x=mgsin(θ)(mg)y=mgcos(θ)
Equilibrium Perpendicular to Ramp:ΣFy=N−mgcos(θ)=0⟹N=mgcos(θ)
Acceleration Down a Frictionless Incline:ΣFx=mgsin(θ)=ma⟹a=gsin(θ)
Friction Mechanics: Static vs. Kinetic Friction
Physical Origin and Properties:
Friction is a resistive electromagnetic contact force arising from microscopic surface irregularities (asperities) interlocking between two contacting bodies.
Direction rules:
Friction always acts parallel to the contacting surface.
Friction always acts in the direction directly opposing relative motion or attempted relative motion.
Kinetic Friction (fk):
Operates when an object is actively sliding relative to the contact surface.
The magnitude of kinetic friction depends solely on the coefficient of kinetic friction (μk) and the normal force (N): fk=μkN
μk is a dimensionless scalar determined by the specific material composition of both contacting surfaces.
Representative material coefficients:
Steel on steel: μk=0.57
Aluminum on steel: μk=0.47
Rubber on concrete: μk=0.8
Ice on ice: μk=0.03
Approximations of zero friction (fk≈0):
Objects on wheels or low-friction bearings.
Smooth ice surfaces.
Explicitly stated "frictionless" conditions.
Static Friction (fs):
Operates when external forces attempt to move an object, but no relative sliding occurs (v=0, a=0).
Static friction matches whatever applied force is necessary to prevent motion up to a threshold: fs≤μsN
Maximum Static Friction (Breakaway Threshold):fs,max=μsN
The coefficient of static friction is almost universally larger than the coefficient of kinetic friction (μs>μk).
Steel on steel: μs=0.74
Aluminum on steel: μs=0.61
Rubber on concrete: μs=1.0
Ice on ice: μs=0.1
Two-Question Protocol for Static Friction Problems:
Question 1: Will the object move?
Calculate normal force N from ΣFy=0.
Calculate the threshold fs,max=μsN.
Calculate the required holding friction fs assuming static equilibrium (ΣFx=0).
If fs≤μsN, the object remains stationary (a=0), and the actual friction force is fs.
If fs>μsN, static friction fails, the object accelerates, and friction immediately transitions to kinetic friction (fk=μkN).
Question 2: What is the minimum force required to initiate motion?
Set applied force equal to fs,max=μsN.
Comprehensive Example: Horizontal Block with Friction:
A block of mass m=1.00kg with initial velocity v0=10.0m/s moves across a surface with μk=0.250. ΣFy=N−mg=0⟹N=mg=1.00(9.81)=9.81NΣFx=−fk=−μkN=−ma⟹a=μkg=0.250(9.81)=2.45m/s2 to the left
A block of mass m=15.0kg sits at rest with μs=0.450 and μk=0.250. An external horizontal force F=150N is applied. N=mg=15.0(9.81)=147.15Nfs,max=μsN=0.450(147.15)=66.2N
Since F=150N>66.2N, the box moves.
The friction force becomes kinetic: fk=μkN=0.250(147.15)=36.79N
The minimum force required to keep this 15.0kg block moving without accelerating (a=0) once in motion is: F=fk=μkmg=0.250(15.0)(9.81)=36.8N
The maximum force that can be applied to this block while remaining stationary is: Fmax=μsmg=0.450(15.0)(9.81)=66.2N
Comprehensive Example: Box Pulled at an Angle with Friction:
A 25.0kg box is dragged across a horizontal floor where μk=0.300 by a rope tension T=105N.
Case A: Rope pulled horizontally (θ=0∘):ΣFy=N−mg=0⟹N=mg=25.0(9.81)=245.25Nfk=μkN=0.300(245.25)=73.575NΣFx=T−fk=ma⟹a=25.0105−73.575=1.257m/s2≈1.26m/s2
Case B: Rope pulled at θ=25.0∘ above horizontal:ΣFy=N−mg+Tsin(θ)=0⟹N=mg−Tsin(θ)N=25.0(9.81)−105sin(25.0∘)=245.25−44.375=200.875Nfk=μkN=0.300(200.875)=60.26NΣFx=Tcos(θ)−fk=maa=25.0105cos(25.0∘)−60.26=25.095.163−60.26=1.396m/s2≈1.40m/s2
Pulling upward at an angle decreases the normal force, reducing the kinetic friction and increasing the overall forward acceleration.
Comprehensive Example: Sliding Block on Incline with Friction:
A 2.00kg wooden block sits on an incline set to θ=40.0∘ with μk=0.300. ΣFy=N−mgcos(θ)=0⟹N=mgcos(θ)ΣFx=mgsin(θ)−fk=mamgsin(θ)−μkmgcos(θ)=maa=g(sin(θ)−μkcos(θ))a=9.81(sin(40.0∘)−0.300cos(40.0∘))=9.81(0.6428−0.2298)=4.05m/s2
Coupled Multi-Body Systems and Kinematics Integration
Principles of Connected Systems:
When bodies are connected by an inextensible taut string over an ideal pulley:
All attached bodies share the exact same magnitude of acceleration (a1=a2=a).
The tension in the continuous string is uniform throughout (T1=T2=T).
Half-Atwood Machine (Cart on Table Connected to Hanging Mass):
Consider a frictionless cart (m1=2.30kg) on a horizontal table attached via a light string to a hanging mass (m2=1.50kg), held at rest at height h=0.860m above the floor.
Example: A force F=100N acts horizontally on a 10.0kg cart initially at rest across a distance d=5.00m on a frictionless surface. ΣFx=F=ma⟹a=10.0100=10.0m/s2v=v02+2a(x−x0)=0+2(10.0)(5.00)=100=10.0m/s
Work and Energy Conservation Principles
Energy Fundamentals:
Energy (E) is a scalar quantity representing the capacity to do work or cause physical change.
Units: Joules (J, where 1J=1N⋅m=1kg⋅m2/s2).
Energy can be positive, negative, or zero, but carries no vector direction.
Work (W):
Work is the quantitative transfer of energy across the boundary of a system produced when an external force acts across a displacement: W=Fdcos(θ)
F is the applied force magnitude.
d is the displacement magnitude over which the force acts.
θ is the angle between the force vector and the displacement vector.
Sign Conventions of Work:
Positive Work (W>0, or Win): Occurs when θ<90∘ (force has a component in the direction of motion). Kinetic energy increases.
When θ=0∘, W=+Fd.
Negative Work (W<0, or Wout): Occurs when θ>90∘ (force opposes motion). Kinetic energy decreases.
When θ=180∘, W=−Fd.
Zero Work (W=0): Occurs when θ=90∘ (force is strictly perpendicular to displacement, e.g., normal force on a horizontal surface or gravity acting on horizontal motion).
Work-Energy Theorem:
The net work done on an object by all acting forces equals the net change in its kinetic energy: Wnet=ΔKE=KEf−KEi
Kinetic energy is defined as: KE=21mv2
Total Energy Conservation Equation:
In an isolated or general system, total energy is strictly conserved: Ei=EfKEi+PEi+Win=KEf+PEf+Eth+∣Wout∣
Alternatively expressed in terms of non-conservative work (Wnc): Wnc=ΔKE+ΔPE
Limitations of Energy Conservation methods:
Vector direction information is lost because kinetic energy depends on speed squared (v2), not directional velocity.
Elapsed time (t) is not an explicit parameter in standard energy equations.
Comprehensive Example: Truck Braking Distance:
A 4000kg truck travels at v0=30.0m/s. The brakes exert a stopping force of 50,000N.
Mechanical energy is dissipated irreversibly into thermal energy (Eth) or transferred in/out as external work (Win, Wout).
Gravitational Potential Energy (PEg):
Represents stored energy due to vertical elevation against gravity: PEg=mgh
The choice of zero datum (h=0) is arbitrary; physical behaviors depend solely on the potential energy difference (ΔPEg):
A 5.00kg block elevated 2.00m above a table that is 3.00m above a floor:
Relative to the table (h=0): at the top PE=5(9.81)(2)=98.1J; at the table PE=0J; at the floor (h=−3m) PE=5(9.81)(−3)=−147.15J.
Relative to the floor (h=0): at the top PE=5(9.81)(5)=245.25J; at the table PE=5(9.81)(3)=147.15J.
In both frameworks, ΔPE between top and table is identically 98.1J, and between table and floor is identically 147.15J.
Free-Fall and Trajectory Independence:
Two balls of mass m=0.0500kg are released from height h=3.00m. Ball 1 travels straight down at 4.00m/s; Ball 2 is projected horizontally at 4.00m/s. KEi=21(0.0500)(4.00)2=0.400JPEi=mgh=0.0500(9.81)(3.00)=1.4715JEtotal=0.400+1.4715=1.8715J
At ground level (PEf=0): KEf=Etotal=1.8715Jv=m2KEf=0.05002(1.8715)=8.65m/s
Both balls impact the ground with the identical speed (8.65m/s) regardless of launch direction, demonstrating that potential energy depends strictly on elevation change, not trajectory shape.
Elastic (Spring) Potential Energy (PEs):
Stored by compressing or stretching an elastic medium from its relaxed equilibrium position (x=0): PEs=21kx2
Dart Gun Example:
A spring gun compresses x=0.0500m (5.00cm) loaded with a m=0.0100kg (10.0g) dart. Upon horizontal release, it fires at v=3.00m/s.
Spring constant: 21kx2=21mv2⟹k=x2mv2=0.050020.0100(3.002)=36.0N/m
If held at height h=1.40m above the floor and discharged horizontally: Ei=mgh+21mv02=KEf=21mv2v=v02+2gh=(3.00)2+2(9.81)(1.40)=9+27.468=6.04m/s
Vertical Spring Oscillations with Coupled Potential Energies:
A 1.50kg box hangs vertically from a spring (k=34.0N/m).
The box is pulled down an additional d=0.500m below equilibrium (xtotal=0.4328+0.500=0.9328m total extension) and released from rest.
Define the low release position as h=0, so the equilibrium height is h=0.500m.
Initial energy at release point (vi=0): Ei=21kxtotal2+0+0=21(34.0)(0.9328)2=14.792J
Final energy as it passes through equilibrium: Ef=21kx02+mgh+21mv2Ef=21(34.0)(0.4328)2+1.50(9.81)(0.500)+21(1.50)v214.792=3.184+7.3575+0.75v214.792−10.542=0.75v2⟹4.250=0.75v2v=0.754.250=2.38m/s
Non-Conservative Forces, Thermal Dissipation, and Power
Thermal Energy Generated by Friction:
Kinetic friction removes mechanical energy from a system, transforming it into internal thermal energy (Eth): Wfk=fkdcos(180∘)=−fkd=−μkNdEth=∣Wfk∣=μkNd
On a horizontal surface where N=mg: Eth=μkmgd
On an inclined plane where N=mgcos(θ), with displacement d along the ramp: Eth=μk(mgcos(θ))d
Comprehensive Example: Sled on Frictionless Hill with Rough Run-Out:
A child and sled (m=38.0kg) start from rest atop a frictionless hill of height h=2.30m. At the bottom, the sled encounters horizontal snow with μk=0.100.
(b) Speed at the Foot of the Hill:mgh=21mv2⟹v=2gh=2(9.81)(2.30)=6.716m/s≈6.72m/s
(c) Stopping Distance across Rough Snow:
The total initial mechanical energy converts entirely into thermal dissipation: PEi=Eth=μkmgdmgh=μkmgd⟹d=μkh=0.1002.30=23.0m
Power (P):
Power is defined as the time rate of doing work or transferring energy: P=ΔtW=ΔtΔE
SI Unit: Watt (W), where 1W=1J/s.
Imperial Unit: Horsepower (hp): 1hp=746W
Power Delivered at Constant Velocity:
When an applied force F moves an object at constant speed v against resistance: P=Fv
Example: An object of mass m=5.00kg moved at v=5.00m/s where μk=0.300: F=fk=μkmg=0.300(5.00)(9.81)=14.715NP=Fv=14.715(5.00)=73.6W
Automobile Power Calculation:
A 1500kg automobile accelerates from 0 to 26.8m/s (60mph) in 5.30s.
Work required: W=ΔKE=21(1500)(26.8)2=538,680J
Average power output: P=5.30538,680=101,638W≈102kW
In horsepower: P=746101,638=136.2hp≈136hp
Commercial Energy Billing (Kilowatt-Hour):
The kilowatt-hour (kWh) is a unit of energy, not power: 1kWh=(1000W)(3600s)=3.60×106J=3,600,000J
Momentum, Impulse, and Conservation in Collisions
Linear Momentum (Vector p):
Defined as the product of mass and velocity: p=mv
SI Units: kg⋅m/s or Newton-seconds (N⋅s).
Direction strictly follows the velocity vector. Momentum is directional, so opposite directions require opposing algebraic signs (+v vs −v).
Mathematical link to kinetic energy: KE=2mp2
Newton's Second Law in Terms of Momentum:
Net force equals the instantaneous rate of change of linear momentum: ΣF=ΔtΔp
Impulse (J or I):
Impulse is the integrated effect of a force over an elapsed time interval: J=FavgΔt=Δp=mvf−mvi
Baseball Impact Example:
A 0.100kg baseball approaches home plate horizontally at vi=−20.0m/s and is struck by a bat, rebounding at vf=+40.0m/s. The impact duration is Δt=0.100s.
Initial and final momentum: pi=mvi=0.100(−20.0)=−2.00kg⋅m/spf=mvf=0.100(40.0)=+4.00kg⋅m/s
Average contact force: Favg=ΔtΔp=0.1006.00=60.0N
Law of Conservation of Linear Momentum:
In an isolated system experiencing zero net external force (ΣFext=0): Pi=Pf
Internal interaction forces between colliding bodies form Newton's third law action-reaction pairs (F12=−F21). The internal impulses cancel identically (Δp1+Δp2=0), conserving total momentum.
Taxonomy of Collision Types:
Completely (Perfectly) Inelastic Collisions:
Colliding bodies stick together, moving with a single shared final velocity (v3=v4=vf).
Momentum is fully conserved; mechanical kinetic energy is maximally lost to deformation and thermal energy.
Governing equation: m1v1+m2v2=(m1+m2)vf
Inelastic Collisions (General):
Colliding bodies rebound independently.
Momentum is conserved, but kinetic energy is not conserved (KEf<KEi).
Governing equation: m1v1+m2v2=m1v3+m2v4
Perfectly Elastic Collisions:
Colliding bodies rebound without permanent deformation or thermal dissipation.
Both total momentum and total kinetic energy are conserved simultaneously: m1v1+m2v2=m1v3+m2v421m1v12+21m2v22=21m1v32+21m2v42
Relative Velocity Theorem (1D Elastic Collision):
Combining the momentum and kinetic energy conservation laws yields the relative velocity condition: v1−v2=−(v3−v4)=v4−v3
The relative speed of approach equals the relative speed of separation.
Explosions:
A unified body at initial velocity vi separates into multiple fragments: (m1+m2)vi=m1v3+m2v4
Kinetic energy increases dramatically (KEf>KEi), converted from internal chemical or mechanical potential energy.
One-Dimensional and Two-Dimensional Collision Dynamics
One-Dimensional Inelastic Collision Examples:
Two Carts Sticking Together:
A 2.30kg cart moving at 4.50m/s collides with a stationary 3.50kg cart on a frictionless track: m1v1+m2(0)=(m1+m2)vfvf=2.30+3.502.30(4.50)=5.8010.35=1.78m/s
Opposing Motion (Mouse Jumping onto Cart):
A 0.980kg mouse runs at +1.20m/s toward an oncoming 2.30kg cart traveling at −2.50m/s. The mouse jumps onto the cart: vf=m1+m2m1v1+m2v2=0.980+2.300.980(1.20)+2.30(−2.50)=3.281.176−5.75=−1.39m/s
The combined unit moves at 1.39m/s in the cart's initial direction of travel.
One-Dimensional Elastic Collisions between Equal Masses (m1=m2=1.30kg, v1=3.40m/s):
Case A: Cart 2 initially at rest (v2=0):
Using v4=v1−v2+v3 into momentum equation: v3=m1+m2(m1−m2)v1+2m2v2=2.600+0=0m/sv4=v1+v3=3.40+0=+3.40m/s
Hunter on Ice: A 99.0kg hunter standing motionless (v0=0) on frictionless ice fires a 0.0220kg bullet at 305m/s. 0=m1v1+m2v2⟹v1=−m1m2v2=−99.00.0220(305)=−0.0678m/s
Ice Skater Throwing a Weight: A 60.0kg skater moving at 5.00m/s on ice throws a 0.500kg snowball forward at 25.0m/s. (m1+m2)vi=m1v3+m2v4v3=60.0(60.0+0.500)(5.00)−0.500(25.0)=60.0302.5−12.5=4.83m/s
Two-Dimensional Collisions:
Total linear momentum is independently conserved along each orthogonal axis: ΣPxi=ΣPxf⟹m1v1x+m2v2x=m1v3x+m2v4xΣPyi=ΣPyf⟹m1v1y+m2v2y=m1v3y+m2v4y
A 25.0kg child running at v1=3.00m/s jumps horizontally onto a stationary 10.0kg sled on frictionless snow. The sled then coasts up a frictionless embankment until stopping.
Stage 1: Momentum Conservation during Jump:m1v1+m2(0)=(m1+m2)v2v2=25.0+10.025.0(3.00)=35.075.0=2.1429m/s≈2.14m/s
Stage 2: Sled Impulse and Average Force:
Impulse imparted to sled alone: Δpsled=m2v2−0=10.0(2.1429)=21.4kg⋅m/s
If the landing process takes Δt=0.250s, the average horizontal force exerted by child on sled is: Favg=ΔtΔp=0.25021.43=85.7N
Stage 3: Energy Conservation Ascending Embankment:21(m1+m2)v22=(m1+m2)ghh=2gv22=2(9.81)(2.1429)2=19.624.592=0.234m
Multi-Stage Sledding and Incline Problem:
A 60.0kg person running at v1=5.00m/s jumps onto a stationary 2.00kg sled at the top of a slope, and the combination slides down a vertical drop of h=4.00m.