Unit 1 Physics: Errors and Uncertainty Study Notes

Unit 1 Physics Notes: Errors and Uncertainty

Types of Errors

  • Every measurement has an associated uncertainty or error.

    • Random Errors

    • Caused by environmental conditions or the person taking measurements.

    • Examples include parallax error and fluctuations in temperature.

    • Measurements are often taken multiple times, and averages are used to reduce the effect of random errors.

    • Systematic Errors

    • Caused by faults in instruments or experimental procedures.

    • Examples include zero error and procedural faults in conducting experiments.

    • These require recalibration of instruments or review of experimental procedures.

Measurement Fundamentals

  • Reading: The value assigned to a measurement when using instruments.

  • Accuracy: The degree to which a series of readings are close to one another.

  • Measurement: A reading taken from an instrument for the size or amount of a base unit.

Error Analysis

  • Definition of Error: The uncertainty in a measured value due to various factors such as wrongly calibrated instruments, incorrect measuring conditions, or failure to follow experiment rules.

  • Accuracy of Measurement: Refers to how well a measured value agrees with the standard value.

    • Example: If a measured weight of a stone is 0.5 kg, while the actual weight is 1 kg, then the measurement is not accurate.

  • Precision: Indicates how closely a set of measurements agree with each other.

    • Example: Measurements of a cord: 2.3m, 2.2m, 2.4m, 2.2m, 2.23m are considered precise because they are closely grouped together.

Error Propagation

  • Errors in Addition:

    • For the equation: y=x+wy = x + w

    • Associated error: extδY=ext±[extδX+extδW].ext{δY} = ext{±}[ ext{δX} + ext{δW}].

  • Errors in Subtraction:

    • For the equation: y=muy = m - u

    • Associated error: extδY=ext±[extδm+extδu].ext{δY} = ext{±}[ ext{δm} + ext{δu}].

  • Errors in Multiplication:

    • For the equation: Y=XimesPY = X imes P

    • Associated error: rac{ ext{δY}}{Y} = ext{±}igg[ rac{ ext{δX}}{X} + rac{ ext{δP}}{P} igg].

  • Errors in Division:

    • For the equation: Y=racXPY = rac{X}{P}

    • Associated error: rac{ ext{δY}}{Y} = ext{±}igg[ rac{ ext{δX}}{X} + rac{ ext{δP}}{P} igg].

  • Errors Involving Powers:

    • For the equation: Y=xn/mkY = x^{n/mk}

    • Associated error: rac{ ext{δY}}{Y} = ext{±} igg[n rac{ ext{δx}}{x} + k rac{ ext{δm}}{m}igg].

  • Percentage Errors:

    • Calculated as:
      ext{Percentage Error} = ext{Fractional Error} imes 100 ext{%}

Forces

  • Force:

    • Defined as anything that keeps a body at rest or in uniform motion in a straight line.

  • Types of Forces:

    1. Contact Force: eg. Reaction forces

    2. Electric Forces

    3. Magnetic Forces

    4. Gravitational Forces

    5. Electrostatic Forces

    6. Nuclear Forces

Diagrammatic Representations

  • Forces at Rest:

    • R=WR = W (At rest the reaction force equals weight)

  • Forces in Motion:

    • An unbalanced force occurs if other conditions change.

Triangle Law of Vector Addition

  • Definition: States that when two vectors are represented as two sides of a triangle, the resultant vector is represented by the third side in magnitude and direction.

Equations of Motion

  • Recall: Speed is defined as distance/time. Average speed is given by the equation: extAverageSpeed=racextTotalDistanceextTotalTimeTakenext{Average Speed} = rac{ ext{Total Distance}}{ ext{Total Time Taken}}

  • Equations:

    • S=rac(V+U)2imestS = rac{(V + U)}{2} imes t

    • a=rac(VU)ta = rac{(V - U)}{t} where acceleration is defined as the rate of change of velocity.

    • Other equations derived from basic definitions include:

      • S=ut+rac12at2S = ut + rac{1}{2} at^2

      • V2=U2+2asV^2 = U^2 + 2 a s

Momentum

  • Definition: The product of an object’s mass and its velocity.

    • p=mvp = mv

  • Newton's Laws of Motion:

    1. 1st Law: A body remains in state of rest or uniform motion unless acted upon by an external force.

    2. 2nd Law: The force acting on an object equals rate of change of momentum, F=rac(mvmu)tF = rac{(mv - mu)}{t} or F=maF = ma.

    3. 3rd Law: For every action, there is an equal and opposite reaction.

Circular Motion

  • Definition of Centripetal Force: The force that keeps a body in circular motion, directed towards the center of the path.

  • Equations:

    • F=racmv2rF = rac{mv^2}{r}

  • Newton's Law of Gravitation:

    • F=Gracm1m2r2F = G rac{m_1 m_2}{r^2}. Here, GG is the universal gravitational constant (6.67imes1011extNm2/extkg26.67 imes 10^{-11} ext{Nm}^2/ ext{kg}^2).

Heat Transfer

  • Heat Flow:

    • Described by their gradient and can be represented as: racextΔQt=KAracextΔθextΔXrac{ ext{ΔQ}}{t} = -K A rac{ ext{Δθ}}{ ext{ΔX}}

    • Where KK is thermal conductivity, AA is cross-sectional area, and racΔθΔXrac{Δθ}{ΔX} is the temperature gradient.

  • First Law of Thermodynamics:

    • Change in internal energy is equal to heat added to the system minus work done by the system.

    • extΔU=QW.ext{ΔU} = Q - W.

Simple Harmonic Motion (SHM)

  • Definition: Motion in which the restoring force is directly proportional to the displacement from the equilibrium position.

  • Equation of SHM:
    F=kxF = -kx

  • Energy in SHM: The total mechanical energy is the sum of kinetic and potential energies. Etotal=KE+PEE_{total} = KE + PE

  • Damping: The reduction in amplitude of oscillations, which can be light, heavy, or critical damping.

Resonance

  • Definition: Occurs when a system is driven at its natural frequency, leading to large amplitude of oscillation.

  • Coherence: When two waves have the same frequency, amplitude, and phase leading to resonance.

Blackbody Radiation

  • Definition: A perfect absorber and emitter of radiation, with its efficiency dependent on temperature.

    • Higher temperatures lead to higher emission intensity.