Physics is the study of nature and natural phenomena. It deals with the fundamental principles of the universe and the basic forces of nature.
Force | Relative Strength | Range | Mediator Particle |
---|---|---|---|
Gravitational Force | 10-39 | Infinite | Graviton (hypothetical) |
Electromagnetic Force | 10-2 | Infinite | Photon |
Strong Nuclear Force | 1 | 10-15 m | Gluons |
Weak Nuclear Force | 10-13 | 10-18 m | W± and Z0 bosons |
A physical quantity is a property of a material or system that can be quantified by measurement. It has both numerical magnitude and unit.
Quantity | Unit | Symbol |
---|---|---|
Length | meter | m |
Mass | kilogram | kg |
Time | second | s |
Electric current | ampere | A |
Temperature | kelvin | K |
Amount of substance | mole | mol |
Luminous intensity | candela | cd |
Measurment | Length in Meter |
---|---|
Distance to Andromeda Galexy(from earth) | 2*1022m |
Distance to nearest star(after sun) Proxima century (from earth) | 4*1016m |
Distance to Pluto ( from earth ) | 6*1012m |
Average radius of earth | 6 × 106m |
Height of Mount Everest | 9 × 103m |
Thickness of the paper | 1 × 10-4m |
Length of a typical virus | 1 × 10-8m |
Radius of a Hydrogen Atom | 5 × 10-11m |
Radius of Proton | 1 × 10-15m |
Dimensions of a physical quantity are the powers to which the fundamental units must be raised to represent that quantity.
Example: Force = mass × acceleration = [M][LT-2] = [MLT-2]
Significant figures are the meaningful digits in a measured or calculated quantity that are known reliably.
Absolute Error: The magnitude of the difference between mean value and each individual value is called absolute error.Absolute Error: Δa = |amean - ai|
Mean Absolute ErrorThe arthemetic mean of all the absolute error is called mean absolute error.Mean Absolute Error: Δamean = (ΣΔai)/n
Relative ErrorThe ration of mean absolute error to it's arithematic mean value is called relative errorRelative Error: Δamean/amean
Percentage Error: (Δamean/amean) × 100%
Significant figures are the meaningful digits in a measured or calculated quantity that are known reliably.
It refer to closeness of the observed value to it's true value of the quantity
It refers to closeness between observerd values to the measurement
Defination:It is an instryment to measure to smaller length up to 1/10 mm accuratly
It is defined as difference of value of 1 main scale division and 1 vernier scale division
VC = 1MSD - 1VSDIt is an instrument which is used to measure very small length such as diameter of the thin wire, thickness of the sheet. It can measured 1/100 mm length
PitchIt is defined as the linear distance moved gy screw forward or backward when one complete rotation is given to circular cap
least count of screw gauge = pitch/total number of division of circular scaleIf size of the body is negligible to distance travelled gy body then body can be consider as point mass.
It is point or position from where positive of any object cxan be described
Position:It is address or location of any body from refernce point
RestIf position of an object does not change with respect to tome then object is said to be reat
MotionIf position of an object chamge with respect to time then object is said to be motion
An object is said to be in motion if its position changes with respect to time and its surroundings.
The total length of the path covered by moving object
The shorest distance between final position to initial position
It is defined as rate of change of distance.
Uniform speed :If an object covered gy equal distance in equal time than the speed of an object is called uniform speed.
Nonuniform speed:Ifthe object covered equal distance in unequal time than the speed of an object is called nonuniform speed.
Average speed:It is defined as ration of total distance covered to totaltime teken
v_ = total distance /total tiem taken
Instantenous speed:Speed at any particle time is called instantaneous speed
ds/dt = V
Speedometer:It is a divice which measures instantanrous speed of the vehicle
Rate of change of displacement with respect to time.
V = change in positon / time
Acceleration is defined as the ratio of change of velocity with time
a = change in velocity / time
Term | Definition | Unit (SI) |
---|---|---|
Position | Location of an object with respect to a reference point | meter (m) |
Displacement | Change in position (vector quantity) | meter (m) |
Distance | Total path length (scalar quantity) | meter (m) |
Speed | Distance traveled per unit time (scalar) | m/s |
Velocity | Displacement per unit time (vector) | m/s |
Acceleration | Rate of change of velocity | m/s² |
1. v = u + at
2. s = ut + ½at²
3. v² = u² + 2as
4. s = (u + v)t/2
where:
u = initial velocity,
v = final velocity,
a = acceleration,
t = time,
s = displacement
Slope gives velocity
Curvature indicates acceleration
Slope gives acceleration
Area under curve gives displacement
Motion Type | x-t Graph | v-t Graph | a-t Graph |
---|---|---|---|
At rest | Horizontal line | On time axis | On time axis |
Uniform motion | Straight line with slope | Horizontal line | On time axis |
Uniform acceleration | Parabola | Straight line with slope | Horizontal line |
Relative velocity of A with respect to B: vAB = vA - vB
a = g = 9.8 m/s² (downward)
Equations become:
1. v = u + gt
2. h = ut + ½gt²
3. v² = u² + 2gh
A physical quantity with only magnitude and no direction (e.g., mass, speed, time).
A physical quantity with both magnitude and direction (e.g., displacement, velocity, force).
Vector Operation | Mathematical Representation | Graphical Method |
---|---|---|
Addition | R = A + B | Triangle/Parallelogram Law |
Subtraction | R = A - B = A + (-B) | Same as addition with reversed vector |
Dot Product | A·B = ABcosθ | Projection of one vector on another |
Cross Product | A×B = ABsinθ n̂ | Right-hand rule |
An object thrown with some initial velocity that moves under the influence of gravity alone.
For oblique projection (angle θ with horizontal):
Initial velocity components:
ux = ucosθ (horizontal)
uy = usinθ (vertical)
Time of flight: T = 2usinθ/g
Maximum height: H = u²sin²θ/2g
Horizontal range: R = u²sin2θ/g
Equation of trajectory: y = xtanθ - (gx²)/(2u²cos²θ)
Motion of an object along a circular path with constant speed but changing velocity (due to changing direction).
Angular velocity: ω = v/r = 2π/T (rad/s)
Centripetal acceleration: ac = v²/r = ω²r
Centripetal force: Fc = mv²/r = mω²r
Time period: T = 2πr/v = 2π/ω
Frequency: f = 1/T (Hz)
Relative velocity of A with respect to B: vAB = vA - vB
Resultant velocity: vresultant = vboat + vriver
Time to cross river: t = d/vboat,⊥ (where d = width)
Drift: x = vriver × t
Any vector A can be resolved into components:
Ax = Acosθ (x-component)
Ay = Asinθ (y-component)
Magnitude: A = √(Ax² + Ay²)
Direction: θ = tan-1(Ay/Ax)
Work (W): Product of force and displacement in direction of force.
Formula: W = F·d = Fd cosθ
Units: SI – Joule (J), CGS – erg
Positive Work: θ < 90°, Negative Work: θ > 90°, Zero Work: θ = 90°
Work done by variable force:
W = ∫ F(x) dx from x₁ to x₂
Graphically: Area under F-x graph
K.E.: Energy possessed by a body due to motion.
Formula: K.E. = ½mv²
Net work done by all forces = Change in kinetic energy
W = ΔK.E. = ½mv² - ½mu²
P.E.: Energy possessed due to position or configuration
Gravitational P.E.: U = mgh
Elastic P.E. (spring): U = ½kx²
In absence of non-conservative forces (like friction):
Total Mechanical Energy = Constant
K.E. + P.E. = constant
Power: Rate of doing work
Formula: P = W/t = F·v
Units: SI – Watt (W), 1 kW = 1000 W
1 HP (Horsepower) = 746 W
Energy: Capacity to do work
Commercial unit of energy: 1 kWh = 3.6 × 10⁶ J
Conservative Forces | Non-Conservative Forces |
---|---|
Work done is path independent | Work done depends on path |
Mechanical energy conserved | Mechanical energy not conserved |
e.g., Gravitational, electrostatic | e.g., Friction, air resistance |
COM: Point representing the mean position of mass in a system.
Formula (discrete particles): xCOM = (m₁x₁ + m₂x₂ + ...)/(m₁ + m₂ + ...)
For continuous body: xCOM = ∫x dm / ∫dm
Velocity of COM: vCOM = (m₁v₁ + m₂v₂ + ...)/(m₁ + m₂ + ...)
Acceleration of COM: aCOM = (m₁a₁ + m₂a₂ + ...)/(m₁ + m₂ + ...)
Torque (τ): Rotational analogue of force, τ = r × F
Angular Momentum (L): L = r × p = Iω
Newton’s Second Law for Rotation: τ = dL/dt
Translational Equilibrium | Rotational Equilibrium |
---|---|
ΣF = 0 | Στ = 0 |
Couple: Pair of equal and opposite forces with different lines of action causing rotation.
Moment of Inertia: I = Σmr² (discrete), I = ∫r² dm (continuous)
Units: kg·m²
Radius of Gyration (K): I = MK²
Body | Axis | Moment of Inertia (I) |
---|---|---|
Ring | About center | MR² |
Disc | About diameter | ½MR² |
Rod | About center perpendicular | 1/12 ML² |
Solid Sphere | About diameter | 2/5 MR² |
Parallel Axis: I = ICM + Md²
Perpendicular Axis (for planar bodies): Iz = Ix + Iy
K.E.rot = ½Iω²
Rolling without slipping: v = Rω
Total K.E.: K.E. = ½mv² + ½Iω²
Conservation of Angular Momentum: If net torque is zero, L = constant
Applications: Figure skater pulling arms, collapsing star, etc.
Every object attracts every other object with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
F = G·(m₁·m₂) / r²
Where G = 6.674 × 10⁻¹¹ N·m²/kg²
Field due to mass M at distance r: g = G·M / r²
Gravitational field is a vector: direction is toward mass.
Work done per unit mass in bringing a mass from infinity to that point.
V = -G·M / r
Potential Energy of mass m: U = m·V = -G·M·m / r
g = G·M / R² (on Earth’s surface)
At height h: gh = g·(1 - 2h/R)
At depth d: gd = g·(1 - d/R)
Orbital Velocity (vo): Minimum speed needed to orbit Earth close to surface.
vo = √(G·M / R) = √(g·R)
Time Period (T): T = 2π√(r³ / GM)
Geostationary Satellite: Period = 24 hrs, equatorial orbit, same direction as Earth’s rotation.
vesc = √(2·g·R) = √(2GM / R)
For Earth: ~11.2 km/s
Stress: Force applied per unit area.
Stress = F / A (N/m² or Pascal)
Strain: Ratio of change in dimension to original dimension.
Strain = ΔL / L (unitless)
Within elastic limit, Stress ∝ Strain
Stress = E × Strain (E = modulus of elasticity)
Modulus | Formula | Application |
---|---|---|
Young’s Modulus (Y) | Y = (F·L)/(A·ΔL) | Longitudinal stretching |
Shear Modulus (η) | η = (F/A) / (Δx/L) | Shearing deformation |
Bulk Modulus (K) | K = -ΔP / (ΔV/V) | Volume change under pressure |
Poisson’s Ratio (σ) = Lateral strain / Longitudinal strain
Typical values: 0.2 to 0.4
U = ½ × Stress × Strain × Volume
Also: U = ½ × Y × (ΔL)² / L
Pressure = Force / Area (unit: Pascal = N/m²)
In a fluid column: P = h·ρ·g
A change in pressure applied to an enclosed fluid is transmitted undiminished to every portion of the fluid and walls of container.
A body immersed in fluid experiences upward force (buoyant force) equal to weight of fluid displaced.
Fb = V·ρ·g
A1v1 = A2v2
(For incompressible, non-viscous fluids)
P + ½·ρ·v² + ρ·g·h = constant
(Applies to streamline, ideal flow of fluid)
Internal resistance offered by fluid to flow. Measured by coefficient of viscosity (η).
F = η·A·(dv/dx)
SI unit: Pa·s
F = 6·π·η·r·v
Applies to small spherical body falling slowly through fluid.
vt = (2·r²·(ρ - σ)·g) / (9·η)
Where ρ = density of body, σ = fluid density
Property of fluid surface to behave like stretched membrane due to cohesive forces.
T = F / L
SI unit: N/m
h = (2·T·cosθ) / (r·ρ·g)
Rise/fall of liquid in narrow tube due to surface tension
Elasticity is the property of a material to regain its original shape after deforming forces are removed.
Stress: Force applied per unit area (N/m² or Pascal)
Strain: Fractional change in dimension (dimensionless)
Type | Stress | Strain |
---|---|---|
Longitudinal | F/A | ΔL/L |
Volumetric | ΔP | ΔV/V |
Shear | F/A | tanθ ≈ θ (for small angles) |
Stress ∝ Strain
Stress = Elastic Modulus × Strain
Young’s Modulus (Y) = (F·L) / (A·ΔL)
Bulk Modulus (K) = -ΔP / (ΔV/V)
Shear Modulus (η) = (F/A) / (Δx/L)
σ = - (Lateral Strain) / (Longitudinal Strain)
Typically between 0.25 and 0.35 for solids
U = ½·Stress·Strain·Volume
Or: U = ½·Y·(ΔL)²·A / L
When two systems are in thermal contact and no heat flows between them, they are said to be in thermal equilibrium.
Zeroth Law: If A is in thermal equilibrium with B, and B with C, then A is in thermal equilibrium with C.
Internal Energy (U): The total energy (kinetic + potential) of all molecules in a system.
Heat (Q): Energy transferred due to temperature difference.
Work (W): Energy transferred when the system expands or compresses.
dU = Q - W
(First Law of Thermodynamics)
W = ∫ P dV (area under P-V curve)
Isothermal: W = nRT ln(V₂/V₁)
Adiabatic: W = (P₂V₂ - P₁V₁)/(1 - γ)
Where γ = Cp / Cv
γ = Cp / Cv
For monoatomic gas: γ = 5/3
For diatomic gas: γ ≈ 1.4
No process is possible whose sole result is the transfer of heat from a colder body to a hotter one (Kelvin-Planck statement).
Efficiency (η): η = W / QH = 1 - QC / QH
Carnot Efficiency: ηmax = 1 - TC / TH
(Temperatures in Kelvin)
P = (1/3)ρ⟨v²⟩ = (1/3)(Nm/V)⟨v²⟩
Where ρ = mass density, ⟨v²⟩ = mean square speed
Eavg = (3/2)kT
K.E. ∝ T
Total K.E. = (3/2)nRT for n moles
vrms = √(3kT/m) = √(3RT/M)
Where M = molar mass, R = universal gas constant
Each degree of freedom contributes (1/2)kT to average energy per molecule.
For monoatomic gas: (3/2)kT
For diatomic gas: (5/2)kT (includes rotational)
For polyatomic gas: ≈ (6/2)kT = 3kT
λ = 1 / (√2 π d² n)
Where d = molecular diameter, n = number density
Periodic Motion: A motion that repeats itself at regular intervals of time.
Oscillatory Motion: To and fro motion about a mean position (e.g., pendulum, spring).
Motion in which restoring force is directly proportional to displacement and acts towards mean position.
F = -kx (Hooke’s law)
Equation of SHM: x(t) = A sin(ωt + φ)
v(t) = dx/dt = Aω cos(ωt + φ)
a(t) = d²x/dt² = -Aω² sin(ωt + φ)
ω = √(k/m), T = 2π√(m/k), f = 1/T
Kinetic Energy: K = (1/2)mv² = (1/2)mA²ω² cos²(ωt + φ)
Potential Energy: U = (1/2)kx² = (1/2)mA²ω² sin²(ωt + φ)
Total Energy: E = K + U = (1/2)kA² (constant)
T = 2π√(l/g)
Only valid for small angle approximation (θ < 15°)
ω = √(k/m), T = 2π√(m/k)
Total mechanical energy = (1/2)kA²
Damping: Gradual loss of energy due to friction/resistance.
Forced Oscillation: External periodic force applied. Leads to resonance when driving frequency = natural frequency.
Mechanical Waves: Require a medium to travel (e.g., sound, water waves).
Electromagnetic Waves: Do not require a medium, can travel in a vacuum (e.g., light, radio waves).
Transverse Waves: Particles of the medium oscillate perpendicular to the direction of wave propagation (e.g., light, waves on a string).
Longitudinal Waves: Particles of the medium oscillate parallel to the direction of wave propagation (e.g., sound waves).
Amplitude (A): Maximum displacement from the equilibrium position.
Wavelength (λ): The distance between two consecutive crests or troughs.
Frequency (f): Number of oscillations per second. f = 1/T
Wave Speed (v): v = fλ
Time Period (T): Time taken for one complete oscillation.
y(x, t) = A sin(kx - ωt + φ)
Where:
k = 2π/λ (Wave number), ω = 2πf (Angular frequency), φ = phase constant.
The resultant displacement at any point due to two or more waves is the algebraic sum of the displacements due to each wave.
Constructive Interference: When the displacements of two waves are in the same direction.
Destructive Interference: When the displacements of two waves are in opposite directions.
When two waves of the same frequency and amplitude traveling in opposite directions superpose, they form a standing wave. These waves do not propagate but oscillate in place.
The general equation for a standing wave is:
y(x,t) = 2A sin(kx) cos(ωt)
Resonance: Occurs when an external force frequency matches the natural frequency of the system, causing the amplitude of oscillation to increase significantly.
v = √(B/ρ)
Where B is the bulk modulus and ρ is the density of the medium.