Mechanics Mindmap - Comprehensive Visual Guide
Mechanics Mindmap - Comprehensive Visual Guide
π Introduction
This mechanics mindmap provides a visual overview of all classical mechanics concepts, formulas, and problem-solving techniques essential for JEE Advanced preparation. It covers kinematics, dynamics, work-energy, rotational motion, and gravitation.
π― Mechanics Framework
Main Branches:
Mechanics
βββ Kinematics
βββ Newton's Laws of Motion
βββ Work, Energy and Power
βββ Rotational Motion
βββ Gravitation
βββ Properties of Matter
π Kinematics
Kinematics Overview:
Kinematics
βββ Motion in One Dimension
β βββ Position, Displacement, Distance
β βββ Velocity and Speed
β βββ Acceleration
β βββ Equations of Motion
β βββ Graphical Analysis
β βββ Relative Motion
βββ Motion in Two Dimensions
β βββ Vector Representation
β βββ Projectile Motion
β βββ Circular Motion
β βββ Relative Velocity
βββ Motion in Three Dimensions
β βββ Vector Analysis
β βββ Curvilinear Motion
β βββ Angular Motion
βββ Graphical Kinematics
βββ Position-Time Graphs
βββ Velocity-Time Graphs
βββ Acceleration-Time Graphs
βββ Area Under Curves
Kinematics Key Formulas:
Essential Kinematics Formulas:
1. Equations of Motion (Uniform Acceleration):
- v = u + at
- s = ut + Β½atΒ²
- vΒ² = uΒ² + 2as
- s = vt - Β½atΒ²
- s = [(u + v)/2]t
2. Projectile Motion:
- Time of flight: T = 2u sin ΞΈ/g
- Maximum height: H = uΒ² sinΒ²ΞΈ/2g
- Range: R = uΒ² sin 2ΞΈ/g
- At any time t: x = u cos ΞΈΒ·t, y = u sin ΞΈΒ·t - Β½gtΒ²
3. Circular Motion:
- Angular velocity: Ο = v/r
- Centripetal acceleration: a = vΒ²/r = ΟΒ²r
- Period: T = 2Οr/v = 2Ο/Ο
- Frequency: f = 1/T = Ο/2Ο
4. Relative Motion:
- Relative velocity: v_AB = v_A - v_B
- River boat problems: Effective velocity
- Rain drop problems: Relative angles
βοΈ Newton’s Laws of Motion
Newton’s Laws Overview:
Newton's Laws of Motion
βββ First Law (Inertia)
β βββ Concept of Inertia
β βββ Frame of Reference
β βββ Inertial and Non-inertial Frames
β βββ Applications
βββ Second Law (F = ma)
β βββ Force and Acceleration
β βββ Momentum
β βββ Impulse
β βββ Force-Time Graphs
βββ Third Law (Action-Reaction)
β βββ Action-Reaction Pairs
β βββ Examples and Applications
β βββ Common Misconceptions
βββ Free Body Diagrams
β βββ Drawing FBDs
β βββ Identifying Forces
β βββ Force Resolution
β βββ Equilibrium Conditions
βββ Types of Forces
β βββ Contact Forces
β β βββ Normal Force
β β βββ Friction
β β βββ Tension
β β βββ Spring Force
β βββ Non-contact Forces
β β βββ Gravitational Force
β β βββ Electric Force
β β βββ Magnetic Force
β βββ Pseudo Forces
β βββ Centrifugal Force
β βββ Coriolis Force
βββ Applications of Newton's Laws
βββ Connected Bodies
βββ Pulley Systems
βββ Inclined Planes
βββ Circular Motion Dynamics
βββ Banking of Roads
Force Analysis Framework:
Systematic Force Analysis:
1. Draw Free Body Diagram:
- Identify the object
- Draw all forces
- Use proper direction
- Label forces clearly
2. Apply Newton's Second Law:
- Ξ£F = ma (in x-direction)
- Ξ£F = ma (in y-direction)
- Resolve forces if needed
- Consider sign conventions
3. Friction Forces:
- Static friction: f_s β€ ΞΌ_s N
- Kinetic friction: f_k = ΞΌ_k N
- Direction: Opposes relative motion
- Maximum static friction: f_max = ΞΌ_s N
4. Pulley Systems:
- Same tension throughout string
- Consider mass of pulley if significant
- Account for friction at pulley
- Multiple pulleys: tension distribution
β‘ Work, Energy and Power
Work-Energy Overview:
Work, Energy and Power
βββ Work
β Definition and Mathematical Expression
β Types of Work
β β βββ Positive Work
β β βββ Negative Work
β β βββ Zero Work
β Work Done by Variable Force
β Work-Energy Theorem
β βββ Conservative and Non-conservative Forces
βββ Energy
β βββ Kinetic Energy
β β βββ Translational KE
β β βββ Rotational KE
β βββ Potential Energy
β β βββ Gravitational PE
β β βββ Elastic PE
β β βββ Electric PE
β βββ Mechanical Energy
β βββ Conservation of Energy
β βββ Energy Transformations
βββ Power
β Definition and Units
β Average and Instantaneous Power
β Power in Circular Motion
β βββ Efficiency
βββ Collisions
β βββ Types of Collisions
β β βββ Elastic Collisions
β β βββ Inelastic Collisions
β β βββ Perfectly Inelastic Collisions
β βββ Conservation Laws in Collisions
β βββ Coefficient of Restitution
β βββ Applications
βββ Applications of Work-Energy
βββ Simple Machines
βββ Projectiles with Air Resistance
βββ Energy Diagrams
βββ Stability and Potential Energy
Energy Conservation Principles:
Energy Conservation Framework:
1. Work Done by Force:
- Constant force: W = FΒ·dΒ·cosΞΈ
- Variable force: W = β«FΒ·ds
- Work by gravity: W = mgh
- Work by spring: W = Β½k(xβΒ² - xβΒ²)
2. Kinetic Energy:
- Translational: KE = Β½mvΒ²
- Rotational: KE = Β½IΟΒ²
- Total: KE = Β½mvΒ² + Β½IΟΒ²
3. Potential Energy:
- Gravitational: PE = mgh
- Spring: PE = Β½kxΒ²
- Electric: PE = kqβqβ/r
4. Conservation of Energy:
- E_total = KE + PE = constant
- ΞKE + ΞPE = 0 (conservative forces only)
- W_nc = ΞKE + ΞPE (with non-conservative forces)
5. Power Calculations:
- Instantaneous: P = dW/dt = FΒ·v
- Average: P = W/t
- Rotational: P = ΟΒ·Ο
π Rotational Motion
Rotational Motion Overview:
Rotational Motion
βββ Rotational Kinematics
β βββ Angular Displacement, Velocity, Acceleration
β βββ Equations of Rotational Motion
β βββ Relation Between Linear and Angular Quantities
β βββ Angular Kinematics Graphs
βββ Rotational Dynamics
β βββ Moment of Inertia
β β βββ Definition
β β βββ Calculation Methods
β β βββ Parallel Axis Theorem
β β βββ Perpendicular Axis Theorem
β βββ Torque
β β βββ Definition and Direction
β β βββ Torque Due to Forces
β β βββ Torque and Angular Acceleration
β βββ Angular Momentum
β β βββ Definition and Conservation
β β βββ Angular Momentum of Rigid Bodies
β β βββ Relation with Linear Momentum
β βββ Rotational Dynamics Equations
βββ Rolling Motion
β βββ Pure Rolling
β βββ Rolling Without Slipping
β βββ Rolling with Slipping
β βββ Energy in Rolling Motion
βββ Angular Momentum Conservation
β βββ Conservation Principles
β βββ Applications
β βββ Gyroscope
β βββ Precession
βββ Applications of Rotational Motion
βββ Figure Skater Effect
βββ Diving and Gymnastics
βββ Rotational Equilibrium
βββ Rotating Reference Frames
Rotational Motion Key Concepts:
Essential Rotational Formulas:
1. Angular Kinematics:
- Ο = Οβ + Ξ±t
- ΞΈ = Οβt + Β½Ξ±tΒ²
- ΟΒ² = ΟβΒ² + 2Ξ±ΞΈ
- v = rΟ (linear-angular relationship)
- a = rΞ± (linear-angular relationship)
2. Moment of Inertia:
- I = Ξ£mrΒ² (point masses)
- I = β«rΒ²dm (continuous distribution)
- Parallel axis: I = I_cm + MdΒ²
- Perpendicular axis: I_z = I_x + I_y (lamina)
3. Common Moments of Inertia:
- Rod (about center): I = MLΒ²/12
- Rod (about end): I = MLΒ²/3
- Ring: I = MRΒ²
- Disk: I = MRΒ²/2
- Sphere: I = 2MRΒ²/5
4. Torque and Angular Momentum:
- Ο = r Γ F = IΞ±
- L = r Γ p = IΟ
- Ο = dL/dt
- Conservation: L = constant (if Ο = 0)
5. Rolling Motion:
- v_cm = ΟR (pure rolling)
- KE_total = Β½mvΒ² + Β½IΟΒ²
- KE_trans = Β½mvΒ²
- KE_rot = Β½IΟΒ²
π Gravitation
Gravitation Overview:
Gravitation
βββ Universal Law of Gravitation
β βββ Newton's Law of Gravitation
β βββ Gravitational Constant G
β βββ Vector Form of Gravitational Force
β βββ Superposition Principle
βββ Gravitational Field
β βββ Gravitational Field Strength
β βββ Field Due to Various Mass Distributions
β βββ Gravitational Potential
β βββ Equipotential Surfaces
βββ Gravitational Potential Energy
β βββ Binding Energy
β βββ Escape Velocity
β βββ Orbital Energy
βββ Motion of Planets and Satellites
β βββ Kepler's Laws
β β βββ First Law (Law of Ellipses)
β β βββ Second Law (Law of Areas)
β β βββ Third Law (Law of Periods)
β βββ Orbital Velocity
β βββ Orbital Period
β βββ Satellite Motion
βββ Earth's Gravitational Field
β βββ Earth's Shape and Gravity
β βββ Variation of g with Height
β βββ Variation of g with Depth
β βββ Effect of Earth's Rotation
βββ Applications of Gravitation
βββ Geostationary Satellites
βββ GPS Systems
βββ Planetary Motion
βββ Tidal Forces
Gravitation Key Formulas:
Essential Gravitation Formulas:
1. Newton's Law of Gravitation:
- F = G(mβmβ/rΒ²)
- G = 6.67 Γ 10^-11 NΒ·mΒ²/kgΒ²
- Vector form: F = -G(mβmβ/rΒ²)rΜ
2. Gravitational Field:
- Field strength: g = F/m = GM/rΒ²
- Gravitational potential: V = -GM/r
- Field and potential: g = -dV/dr
3. Orbital Motion:
- Orbital velocity: v = β(GM/r)
- Orbital period: T = 2Οβ(rΒ³/GM)
- Escape velocity: v_e = β(2GM/r)
- Binding energy: E = -GMm/(2r)
4. Kepler's Laws:
- First law: Planets move in ellipses
- Second law: dA/dt = L/(2m) = constant
- Third law: TΒ² β aΒ³
- Mathematical form: TΒ² = (4ΟΒ²/GM)aΒ³
5. Variation of g:
- With height: g(h) = g(0)/(1 + h/R)Β²
- With depth: g(d) = g(0)(1 - d/R)
- At Earth's surface: g = 9.8 m/sΒ²
π¬ Properties of Matter
Properties of Matter Overview:
Properties of Matter
βββ Elasticity
β βββ Stress and Strain
β βββ Hooke's Law
β βββ Elastic Moduli
β β βββ Young's Modulus
β β βββ Bulk Modulus
β β βββ Shear Modulus
β β βββ Modulus of Rigidity
β βββ Elastic Potential Energy
β βββ Elastic Limit
βββ Fluids
β βββ Pressure in Fluids
β βββ Buoyancy and Floatation
β βββ Pascal's Law
β βββ Archimedes' Principle
β βββ Fluid Dynamics
β βββ Equation of Continuity
β βββ Bernoulli's Equation
β βββ Applications
βββ Surface Tension
β βββ Surface Tension Force
β βββ Surface Energy
β βββ Capillarity
β βββ Angle of Contact
β βββ Applications
βββ Viscosity
β βββ Viscous Force
β βββ Poiseuille's Equation
β βββ Stokes' Law
β βββ Terminal Velocity
β βββ Reynolds Number
βββ Mechanical Properties of Solids
βββ Stress-Strain Relationships
βββ Elastic Behavior
βββ Plastic Deformation
βββ Fracture
Mechanical Properties Key Formulas:
Essential Properties of Matter Formulas:
1. Stress and Strain:
- Stress: Ο = F/A
- Strain: Ξ΅ = ΞL/L (linear strain)
- Volumetric strain: Ξ΅_v = ΞV/V
- Shear strain: Ξ³ = Ξx/h
2. Elastic Moduli:
- Young's modulus: Y = Ο/Ξ΅ = FL/(AΒ·ΞL)
- Bulk modulus: K = -P/Ξ΅_v = -PΒ·ΞV/V
- Shear modulus: Ξ· = F/(AΒ·Ξ³)
- Relation: Y = 9KG/(3K + G)
3. Fluid Statics:
- Pressure: P = Οgh
- Buoyant force: F_b = ΟΒ·VΒ·g
- Pascal's law: P = F/A (transmitted equally)
4. Bernoulli's Equation:
- P + Β½ΟvΒ² + Οgh = constant
- Applications: Venturi meter, airplane wing
5. Viscosity:
- Viscous force: F = Ξ·A(dv/dy)
- Terminal velocity: v_t = (2/9)(rΒ²g/Ξ·)(Ο_s - Ο_f)
- Poiseuille's equation: Q = ΟPrβ΄/(8Ξ·L)
6. Surface Tension:
- Surface tension force: F = Ξ³L
- Surface energy: U = Ξ³A
- Capillary rise: h = 2Ξ³cosΞΈ/(Οgr)
π― Problem-Solving Strategies
Mechanics Problem-Solving Framework:
Systematic Approach:
1. Understand the Problem
- Identify the system
- Determine given quantities
- Identify what needs to be found
- Note the constraints
2. Draw Free Body Diagrams
- Isolate the object
- Draw all forces
- Use proper directions
- Label all quantities
3. Apply Physical Laws
- Newton's laws (F = ma)
- Conservation laws
- Kinematic equations
- Energy principles
4. Solve Mathematically
- Choose coordinate system
- Resolve vectors if needed
- Apply equations
- Solve systematically
5. Check and Verify
- Check units
- Verify reasonableness
- Consider special cases
- Confirm physical sense
Common Problem Types:
Mechanics Problem Categories:
1. Kinematics Problems:
- Projectile motion
- Relative motion
- Circular motion
- Graphical analysis
2. Dynamics Problems:
- Connected bodies
- Inclined planes
- Pulley systems
- Circular dynamics
3. Energy Problems:
- Work-energy theorem
- Conservation of energy
- Power calculations
- Collision analysis
4. Rotational Problems:
- Moment of inertia
- Torque and angular acceleration
- Angular momentum
- Rolling motion
5. Gravitation Problems:
- Orbital motion
- Escape velocity
- Gravitational potential
- Kepler's laws
π Performance Tips
Exam Success Strategies:
- Master vector analysis for force problems
- Practice free body diagrams extensively
- Memorize all kinematic equations with conditions
- Understand energy conservation deeply
- Practice moment of inertia calculations
- Focus on conceptual understanding over rote memorization
Use this comprehensive mechanics mindmap to master all JEE Advanced mechanics concepts! Systematic practice with these visual aids will significantly enhance your problem-solving abilities. π―