Week 2 Overview

Physics of Motion, Energy, and Pressure

What is Physics?

  • Physics is defined as the study of energy and its interactions.

  • Energy is what enables action to occur, thus physics is foundational to our understanding of everything.

  • Source: Pearson Publishing

Doing Physics

  • Physics elucidates the rules of the universe through mathematical logic.

  • Emphasizes the power of mathematics in understanding physical laws.

  • Source: CBS

Speed and Velocity

  • Speed Equation:
    extdistance=extspeedimesexttimeext{distance} = ext{speed} imes ext{time}
    Or in symbols:
    x=vimestx = v imes t

  • Where:

    • vv = speed (in m/sm/s)

    • xx = distance (in mm)

    • tt = time (in ss)

  • Speed describes how fast something moves.

  • Velocity describes the speed and the direction of the motion.

  • Example: A car traveling at a speed of 30 m/s has a velocity of 30 m/s heading north.

Acceleration

  • Acceleration represents the change in velocity over time.

  • Acceleration Equation:
    extacceleration=racextchangeinspeedexttimeext{acceleration} = rac{ ext{change in speed}}{ ext{time}}

  • Units for acceleration include m/s2m/s^2.

  • A net Force is necessary to initiate acceleration.

  • Force Equation:
    F=extmassimesextacceleration=mimesaF = ext{mass} imes ext{acceleration} = m imes a

  • Force has an International System (SI) unit of kilograms (kg) times meters per second squared (m/s²), which corresponds to one Newton (N).

  • The common unit of force is also recognized as pounds (lb).

Force Example

  • The force of gravity on Earth accelerates objects at 9.8m/s29.8 m/s^2.

  • In a hypothetical scenario, Superman weighs approximately 200 pounds, equivalent to a mass of about 91 kg.

  • To determine the minimum force Superman must exert to ascend:
    F=mimesaF = m imes a
    F=91kgimes9.8m/s2F = 91 kg imes 9.8 m/s^2
    F=892NF = 892 N

  • Source: Warner Brothers

Pressure

  • Pressure is generated by force acting over an area.

  • Pressure Equation:
    extPressure=racextForceextAreaext{Pressure} = rac{ ext{Force}}{ ext{Area}}

  • The SI unit for pressure is Pascals (Pa), while in common usage, pressure is often described in pounds per square inch (psi).

  • Source: New York Post

Types of Energy

  • Energy is measured in Joules (J).

  • Energy Types Include:

    • Potential Energy: energy that is stored.

    • Gravitational Potential Energy: energy due to an object's height, enabling it to fall.

    • Pressure Energy: energy built up to drive fluid flow.

    • Electric Potential Energy: energy stored in batteries.

    • Electrochemical Potential Energy: energy stored in bonds, such as food.

    • Kinetic Energy: energy associated with the motion of an object.

    • Work: the transfer of mechanical energy.

    • Heat: the transfer of thermal energy.

Energy Interactions

  • For an event to occur, a source of potential energy is essential, such as a battery.

  • Movement is achieved through the conversion of potential energy into kinetic energy.

  • In simpler terms, potential energy decreases (e.g., draining a battery), while kinetic energy increases (e.g., speeding up).

  • Energy cannot be created or destroyed; it can only be transformed from one form to another within the universe.

  • Source: Wikipedia

Gravitational Energy (Falling)

  • Gravitational Potential Energy Equation:
    extGravitationalPotentialEnergy=extmassimesgimesextheight=mghext{Gravitational Potential Energy} = ext{mass} imes g imes ext{height} = mg h

  • Kinetic Energy Equation:
    extKineticEnergy=rac12extmassimesextspeed2=rac12mv2ext{Kinetic Energy} = rac{1}{2} ext{mass} imes ext{speed}^2 = rac{1}{2} mv^2

  • The total energy when an object falls is described by:
    extPotentialEnergy+extKineticEnergy=extTotalEnergyext{Potential Energy} + ext{Kinetic Energy} = ext{Total Energy}
    PE+KE=TEPE + KE = TE

  • Specifically, this can be written as:
    mgh+rac12mv2=TEmg h + rac{1}{2} mv^2 = TE

  • Where:

    • mm = mass (kg)

    • hh = height (m)

    • vv = speed (m/s)

    • gg = gravitational acceleration = 9.8m/s29.8 m/s^2

Conservation of Energy Example

  • Consider a 10 kg ball released from a height of 6 meters.

  • Total energy at release is calculated as follows:
    PE+KE=TEPE + KE = TE
    PE+0=TEPE + 0 = TE
    10kgimes9.8m/s2imes6m=TE10 kg imes 9.8 m/s^2 imes 6 m = TE
    TE=588JTE = 588 J

  • During its fall, kinetic energy increases until it reaches the ground while maintaining the total energy at 588 J (ignoring friction).

A Falling Ball Example

  • The potential energy at the height of 4 meters can be calculated:
    PE=mgh=10kgimes9.8m/s2imes4m=392JPE = mgh = 10 kg imes 9.8 m/s^2 imes 4 m = 392 J

  • The kinetic energy at 4 meters is derived from the total energy:
    PE+KE=TEPE + KE = TE
    392J+KE=588J392 J + KE = 588 J
    KE=588J392J=196JKE = 588 J - 392 J = 196 J

Speed Calculation Before Impact

  • For the falling ball at 6 meters, it has an initial KE of 588 J just before impacting the ground:

  • To calculate the speed right before impact:
    KE=rac12mv2KE = rac{1}{2} mv^2
    Rearranged as:
    2imesKE=mv22 imes KE = mv^2
    v=rac2imesKEmv = rac{2 imes KE}{m}
    v=rac2imes588J10kgv = rac{2 imes 588 J}{10 kg}
    v=117.6racJkgv = 117.6 rac{J}{kg}
    v=10.84m/sv = 10.84 m/s

Pressure in a Balloon

  • Filling a balloon increases the internal pressure.

  • If punctured, the higher internal air pressure causes air to rush out until equilibrium is reached with external air pressure, resulting in a deflated balloon.

  • Pressure acts as a source of energy, similar to a battery; stored pressure allows for a flow of fluid (air, water) when released, converting potential energy to kinetic energy.

Boyle’s Law

  • Boyle's Law Equation:
    P<em>1V</em>1=P<em>2V</em>2P<em>1 V</em>1 = P<em>2 V</em>2

  • Under constant temperature, reducing the volume of a gas increases its pressure as the gas is compressed.

  • Conversely, increasing the volume decreases the pressure as the gas expands.

  • This concept is also applicable in respiratory physiology, illustrating how pressure changes aid in breathing.

    • Source: https://www.criticalcarepractitioner.co.uk/human-physiology/respiratory-system-physiology/

Differential Flow

  • Fluid dynamics demonstrates that fluids move from areas of high pressure to areas of low pressure or from high potential to low potential.

Bernoulli’s Principle

  • States that increasing the speed of a fluid reduces its pressure.

  • Pressure builds up behind an obstruction, converting potential energy into kinetic energy within the flowing fluid.

    • Real-world analogy: Water flowing from a faucet releases pressure and lowers it compared to the pressure behind the valve.

Fluid Dynamics Observations

  • At junctions, narrower channels facilitate faster flow and have lower pressure compared to wider channels.

  • Bernoulli vs. Boyle:

    • Bernoulli's Principle pertains to moving fluids, while Boyle’s Law concerns gas behavior under varying pressure and volume when static.

The Garden Hose Effect

  • Demonstration: Covering the end of a garden hose decreases the cross-sectional area, resulting in higher pressure behind the obstruction, allowing a faster flow of water when released.

Equation of Continuity

  • Equation:
    A<em>1v</em>1=A<em>2v</em>2A<em>1 v</em>1 = A<em>2 v</em>2

  • Where:

    • AA represents cross-sectional area

    • vv signifies fluid speed

Example of Equation of Continuity
  • Given:

    • For Section 1 with a speed of 2 m/s and area of 3 square inches, solve for area of Section 2 with speed of 6 m/s:
      3extin2imes2extm/s=A2imes6extm/s3 ext{ in}^2 imes 2 ext{ m/s} = A_2 imes 6 ext{ m/s}

    • Solve for A<em>2A<em>2 gives: A</em>2=1extin2A</em>2 = 1 ext{ in}^2

The Glottis Mechanism

  • The glottis opens when air from the lungs is forced through it and closes when the airflow reduces pressure sufficiently to shut it closed.

Examples of Bernoulli Effect in Life

  • Observing everyday physical phenomena illustrating Bernoulli's effect, such as flying, which utilizes different pressure distributions over wings to create lift.

Important Formulas

  • All important formulas summarized:

    • extdistance=extspeedimesexttimeext{distance} = ext{speed} imes ext{time}

    • extacceleration=racextchangeinspeedexttimeext{acceleration} = rac{ ext{change in speed}}{ ext{time}}

    • F=maF = ma

    • extPressure=racextForceextAreaext{Pressure} = rac{ ext{Force}}{ ext{Area}}

    • PE+KE=extTotalEnergyPE + KE = ext{Total Energy}

    • PE=mghPE = mgh

    • KE=rac12mv2KE = rac{1}{2} mv^2

    • v=rac2imesKEmv = rac{2 imes KE}{m}

    • A<em>1v</em>1=A<em>2v</em>2A<em>1 v</em>1 = A<em>2 v</em>2