Comprehensive Study Guide: Work, Power, Energy, Waves, and Electricity

Work, Power, and Energy

  • Newton of Force (NN)

    • Definition: A Newton is the SI unit of force. One Newton is defined as the amount of force required to accelerate a mass of one kilogram (1.0kg1.0\,kg) at a rate of one meter per second squared (1.0m/s21.0\,m/s^2).
    • Problem: Find the force needed to accelerate a 100.0kg100.0\,kg mass to 25.0m/s225.0\,m/s^2.
    • Formula: F=m×aF = m \times a
    • Calculation: F=100.0kg×25.0m/s2=2500NF = 100.0\,kg \times 25.0\,m/s^2 = 2500\,N.
  • Joule of Work (JJ)

    • Definition: A Joule is the SI unit of work and energy. It is defined as the work done when a force of one Newton is applied over a displacement of one meter (1.0J=1.0Nm1.0\,J = 1.0\,N \cdot m).
    • Problem: Find the work done when a 200.0N200.0\,N mass is lifted 30.0m30.0\,m high.
    • Formula: W=F×dW = F \times d
    • Calculation: W=200.0N×30.0m=6000joulesW = 200.0\,N \times 30.0\,m = 6000\,\text{joules}.
  • Power

    • Definition: Power is the rate at which work is performed or energy is transferred. It is measured in Watts (WW), where one Watt is one Joule per second (J/sJ/s).
    • Problem: Find the power expended when a 300kg300\,kg mass is lifted 50.0m50.0\,m in 10.0s10.0\,s.
    • Formula: P=Wt=m×g×htP = \frac{W}{t} = \frac{m \times g \times h}{t}
    • Calculation: P=300kg×9.8m/s2×50.0m10.0sP = \frac{300\,kg \times 9.8\,m/s^2 \times 50.0\,m}{10.0\,s}
    • Step 1 (Work): 300×9.8×50=147000J300 \times 9.8 \times 50 = 147000\,J
    • Step 2 (Power): 147000J/10.0s=14700watts147000\,J / 10.0\,s = 14700\,\text{watts}.
  • Horsepower (hphp)

    • Definition: Horsepower is a non-SI unit of power.
    • Problem: Find the Horsepower (hphp) in the previous problem.
    • Calculation: Given that 1hp746W1\,hp \approx 746\,W, the power is converted: 14700W/74619.7hp14700\,W / 746 \approx 19.7\,hp.
  • Potential Energy (PEPE)

    • Definition: Potential Energy is the stored energy of an object based on its position or configuration. Gravitational Potential Energy depends on an object's mass and its height relative to a reference point.
    • Problem: Find the Potential Energy stored in a 100.00kg100.00\,kg mass raised 60.0m60.0\,m where acceleration due to gravity g=9.8m/s2g = 9.8\,m/s^2.
    • Formula: PE=m×g×hPE = m \times g \times h
    • Calculation: PE=100.00kg×9.8m/s2×60.0m=58800.joulesPE = 100.00\,kg \times 9.8\,m/s^2 \times 60.0\,m = 58800.\,\text{joules}.
  • Kinetic Energy (KEKE)

    • Definition: Kinetic Energy is the energy an object possesses due to its motion.
    • Problem: Find the Kinetic Energy in a 400.kg400.\,kg mass moving at 90m/s90\,m/s.
    • Formula: KE=12mv2KE = \frac{1}{2}m{v}^2
    • Calculation: KE=0.5×400.kg×(90m/s)2=200×8100=1620000joulesKE = 0.5 \times 400.\,kg \times (90\,m/s)^2 = 200 \times 8100 = 1620000\,\text{joules}.
  • Conservation of Energy

    • Formula: PEinitial+KEinitial=PEfinal+KEfinalPE_{initial} + KE_{initial} = PE_{final} + KE_{final}, or effectively mgh=12mv2mgh = \frac{1}{2}m v^2 when converting potential to kinetic energy.
    • Rearranging to solve for velocity (vv):
      • mgh=12mv2mgh = \frac{1}{2}m v^2
      • Divide both sides by mm: gh=12v2gh = \frac{1}{2}v^2
      • Multiply by 22: 2gh=v22gh = v^2
      • Take square root: v=2ghv = \sqrt{2gh}
    • Problem: Find how fast a diver strikes the water when jumping off a 3.00m3.00\,m board (g=9.8m/s2g = 9.8\,m/s^2).
    • Calculation: v=2×9.8×3.00=58.87.7m/sv = \sqrt{2 \times 9.8 \times 3.00} = \sqrt{58.8} \approx 7.7\,m/s.
  • Levers and Simple Machines

    • Three Parts of a Lever:
      1. Effort (Force): The force applied to the lever.
      2. Resistance (Load): The object being moved or the weight being lifted.
      3. Fulcrum: The pivot point around which the lever rotates.
    • Three Classes of Levers:
      1. First Class: The Fulcrum is located between the effort and the resistance (e.g., seesaw).
      2. Second Class: The Resistance is located between the effort and the fulcrum (e.g., wheelbarrow).
      3. Third Class: The Effort is located between the resistance and the fulcrum (e.g., tweezers).
    • Mechanical Advantage (MAMA): The factor by which a machine multiplies the force put into it.
      • IMA (Ideal Mechanical Advantage): The mechanical advantage of an ideal machine with no friction (IMA=input distance/output distanceIMA = \text{input distance} / \text{output distance}).
      • AMA (Actual Mechanical Advantage): The mechanical advantage measured by the actual ratio of forces (AMA=output force/input forceAMA = \text{output force} / \text{input force}), accounting for energy loss due to friction.
    • Identifying MA for Simple Machines:
      • Lever: Ratio of distances from the fulcrum (Leffort/LresistanceL_{effort} / L_{resistance}).
      • Pulley: Count the number of rope segments supporting the load.
      • Incline Plane: Ratio of the slope length to the vertical height (L/hL / h).

Momentum and Collisions

  • Momentum (pp)

    • Definition: Momentum is the quantity of motion of a moving body, measured as a product of its mass and velocity.
    • Problem: Find the momentum of a 2.00kg2.00\,kg water balloon traveling at 10.0m/s10.0\,m/s.
    • Formula: p=m×vp = m \times v
    • Calculation: p=2.00kg×10.0m/s=20kgm/sp = 2.00\,kg \times 10.0\,m/s = 20\,kg \cdot m/s.
  • Impulse (JJ)

    • Definition: Impulse is the change in momentum resulting from a force applied over a specific time interval.
    • Problem: Find the impulse of a 50.0kg50.0\,kg mass acted upon by a 200.0N200.0\,N force for 80.0s80.0\,s.
    • Formula: J=F×ΔtJ = F \times \Delta t
    • Calculation: J=200.0N×80.0s=16000NsJ = 200.0\,N \times 80.0\,s = 16000\,N \cdot s.
  • Impulse-Momentum Theory

    • Theory: The impulse applied to an object is equal to its change in momentum: F×t=m×ΔvF \times t = m \times \Delta v.
    • Rearranging to solve for Force (FF):
      • F×t=m×ΔvF \times t = m \times \Delta v
      • F=m×ΔvtF = \frac{m \times \Delta v}{t}
    • Problem: Find FF when mass is 100.kg100.\,kg, speed is 40m/s40\,m/s, and time is 3.00s3.00\,s.
    • Calculation: F=100.kg×40m/s3.00s1333.33NF = \frac{100.\,kg \times 40\,m/s}{3.00\,s} \approx 1333.33\,N. Adjusted for Significant Digits: 1330N1330\,N.
  • Change in Velocity (Δv\Delta v)

    • Formula: Δv=F×tm\Delta v = \frac{F \times t}{m}
    • Problem: Find Δv\Delta v when Force is 25.0N25.0\,N, Time is 45s45\,s, and Mass is 500kg500\,kg.
    • Calculation: Δv=25.0N×45s500kg=2.25m/s\Delta v = \frac{25.0\,N \times 45\,s}{500\,kg} = 2.25\,m/s.
  • Conservation of Momentum

    • Definition: In a closed system with no external forces, the total momentum remains constant: Pinitial=PfinalP_{initial} = P_{final}.
    • Tennis Ball Problem: A 55kg55\,kg machine fires a 0.057kg0.057\,kg ball at 36m/s36\,m/s to the right.
      • pinitial=0p_{initial} = 0
      • 0=(mmachine×vmachine)+(mball×vball)0 = (m_{machine} \times v_{machine}) + (m_{ball} \times v_{ball})
      • 0=(55kg×vmachine)+(0.057kg×36m/s)0 = (55\,kg \times v_{machine}) + (0.057\,kg \times 36\,m/s)
      • vmachine=0.057×36550.037m/sv_{machine} = -\frac{0.057 \times 36}{55} \approx -0.037\,m/s.
  • Collision Types

    • Elastic Collision: Objects bounce off each other without loss of Kinetic Energy.
    • Inelastic Collision: Objects bounce but some Kinetic Energy is lost (transformed into heat/sound).
    • Perfectly Inelastic Collision: Objects stick together after colliding. Total mass becomes (m1+m2)(m_1 + m_2).
    • Problem 6 (Sticking Together): 4.0kg4.0\,kg cart (5.0m/s5.0\,m/s) vs 3.0kg3.0\,kg cart (4.0m/s4.0\,m/s in opposite direction).
      • m1v1+m2v2=(m1+m2)Vfinalm_1 v_1 + m_2 v_2 = (m_1 + m_2)V_{final}
      • (4.0×5.0)+(3.0×4.0)=(7.0)Vfinal(4.0 \times 5.0) + (3.0 \times -4.0) = (7.0)V_{final}
      • 2012=7Vfinal20 - 12 = 7V_{final}
      • 8=7Vfinal    Vfinal1.14m/s8 = 7V_{final} \implies V_{final} \approx 1.14\,m/s. This is a Perfectly Inelastic Collision.
    • Problem 7 (Elastic Marble Collision): Marble A (0.015kg0.015\,kg, 0.225m/s0.225\,m/s right) hits Marble B (0.030kg0.030\,kg, 0.180m/s0.180\,m/s left). A becomes 0.315m/s0.315\,m/s left.
      • (0.015×0.225)+(0.030×0.180)=(0.015×0.315)+(0.030×VB2)(0.015 \times 0.225) + (0.030 \times -0.180) = (0.015 \times -0.315) + (0.030 \times V_{B2})
      • 0.0033750.0054=0.004725+0.030VB20.003375 - 0.0054 = -0.004725 + 0.030V_{B2}
      • 0.002025=0.004725+0.030VB2-0.002025 = -0.004725 + 0.030V_{B2}
      • 0.0027=0.030VB2    VB2=0.09m/s(to the right)0.0027 = 0.030V_{B2} \implies V_{B2} = 0.09\,m/s\,(\text{to the right}).

Harmonic Motion & Wave Properties

  • Simple Harmonic Motion (SHM)

    • Description: Periodic motion where the restoring force is proportional to the displacement from equilibrium.
    • Examples:
      1. A swinging pendulum.
      2. A mass bouncing on a spring.
      3. A vibrating guitar string.
  • Wave Definitions

    • Amplitude: The maximum displacement from the equilibrium position.
    • Frequency (ff): The number of oscillations or cycles per second (measured in Hertz, HzHz).
    • Period (TT): The time required for one complete cycle (T=1/fT = 1/f).
  • Transverse Wave Components

    • Crest: The highest point of the wave.
    • Trough: The lowest point of the wave.
    • Wavelength (\lambda): Distance between successive crests or troughs.
    • Amplitude: Height from equilibrium to crest.
  • The Pendulum

    • Galileo's Laws of the Pendulum: The period of a pendulum is independent of the mass and independent of the amplitude (for small angles). It depends only on the length of the pendulum and gravity.
    • Formula for Period (TT): T=2πLgT = 2\pi\sqrt{\frac{L}{g}}
      • TT = Period
      • LL = Length of the pendulum
      • gg = Acceleration due to gravity (9.8m/s29.8\,m/s^2)
    • Problem 5: Period of a pendulum with L=10.0mL = 10.0\,m.
      • T=2π10.09.86.28×1.026.3sT = 2\pi\sqrt{\frac{10.0}{9.8}} \approx 6.28 \times \sqrt{1.02} \approx 6.3\,s.
    • Problem 6: Length of a pendulum with T=5.0sT = 5.0\,s.
      • 5=2πL9.8    52π=L9.85 = 2\pi\sqrt{\frac{L}{9.8}} \implies \frac{5}{2\pi} = \sqrt{\frac{L}{9.8}}
      • 0.7952=L9.8    0.633=L9.8    L6.2m0.795^2 = \frac{L}{9.8} \implies 0.633 = \frac{L}{9.8} \implies L \approx 6.2\,m.
  • Wave Types and Properties

    • Longitudinal Wave: A wave where the vibration of the medium is parallel to the direction of wave travel. Parts include Compressions (high density) and Rarefactions (low density).
    • Properties:
      • Reflection: The bouncing back of a wave when it hits a boundary (e.g., Echo).
      • Refraction: The bending of a wave as it passes from one medium to another and changes speed (e.g., Straw appearing bent in water).
      • Diffraction: The bending of waves around an edge or through an opening (e.g., Hearing sound around a corner).
      • Interference: The meeting of two waves that combine to form a resultant wave (Constructive or Destructive).
  • Standing Waves and Resonance

    • Standing Wave: A wave pattern that results from the interference of two waves of the same frequency and amplitude traveling in opposite directions. It appears stationary.
      • Nodes: Points of zero displacement.
      • Antinodes: Points of maximum displacement.
    • Wave Equation Problem: Find frequency with Wavelength = 25m25\,m and Speed = 350m/s350\,m/s.
      • v=f×λ    f=vλv = f \times \lambda \implies f = \frac{v}{\lambda}
      • f=35025=14Hz(cycles/sec)f = \frac{350}{25} = 14\,Hz\,\text{(cycles/sec)}.
    • Resonance: Occurs when a vibrating object forces another object to vibrate at its natural frequency, increasing amplitude.
    • Examples of Resonance:
      1. Tacoma Narrows Bridge collapse.
      2. Shattering a wine glass with a specific vocal pitch.
      3. The body of an acoustic guitar amplifying the string's sound.

Sound

  • Definitions

    • Physics definition of Sound: A mechanical longitudinal wave produced by vibrating objects that travels through a medium.
    • Tone: A sound with a regular, periodic frequency.
    • Noise: Irregular, non-periodic sound vibrations.
    • Pitch: The human perception of frequency (high pitch = high frequency).
  • Sound Characteristics

    • Longitudinal Nature: Sound waves consist of molecules bumping into one another, creating regions of compression and expansion along the direction of travel.
    • Intensity vs Loudness: Intensity is the physical power per area (W/m2W/m^2), whereas Loudness is the subjective human perception of that intensity.
    • Inverse Square Law: Intensity decreases with the square of the distance: I1d2I \propto \frac{1}{d^2}.
      • Examples: Sound, Light, Gravitational pull.
    • The Decibel (dBdB): A logarithmic unit used to measure sound intensity. Examples include a whisper (20dB20\,dB), conversation (60dB60\,dB), or a jet engine (140dB140\,dB).
  • Wave Interference and Mechanics

    • Beat Frequency: The periodic variation in volume heard when two sound waves of slightly different frequencies interfere (fbeat=f1f2f_{beat} = |f_1 - f_2|). Example: Tuning a musical instrument against a reference note.
    • Doppler Effect: The change in received frequency due to the motion of the source or the observer. Example: The sound of a siren changing pitch as a fire truck passes by.
    • Speed of Sound Problems:
      • Find speed (vv) if f=100.0Hzf = 100.0\,Hz and λ=5.00m\lambda = 5.00\,m: v=100.0×5.00=500m/sv = 100.0 \times 5.00 = 500\,m/s.
      • Organ Pipes: For a closed tube organ pipe (L=2.0mL = 2.0\,m), the fundamental wavelength is approximately λ=4L=8.0m\lambda = 4L = 8.0\,m.

Light

  • Sources and Concepts

    • Eight Sources of Light: Common sources include the Sun, Stars, Fire, Incandescent Bulbs, LEDs, Lasers, Bioluminescence, and Chemical reactions (Chemiluminescence).
    • Light Terms:
      • Luminous: Objects that produce their own light (e.g., The Sun).
      • Illuminated: Objects that reflect light from other sources (e.g., The Moon).
      • Opaque: Does not let light through.
      • Transparent: Allows light to pass through clearly.
  • Refraction and Illumination

    • Illumination (EE): The amount of light falling on a surface.
    • Equation: E=Id2E = \frac{I}{d^2}
    • Problem: Intensity (II) is 500.00candelas500.00\,candelas, Distance (dd) is 200.00meters200.00\,meters.
    • Calculation: E=500.00(200.00)2=500.0040000=0.0125Result given: 0.125lumens/m2E = \frac{500.00}{(200.00)^2} = \frac{500.00}{40000} = 0.0125 \rightarrow \text{Result given: } 0.125\,\text{lumens}/m^2 (Note: Standard calculation gives 0.01250.0125; transcript provides 0.1250.125).
    • Snell’s Law: Describes how light bends when entering a new medium (n1sin(θ1)=n2sin(θ2)n_1 \sin(\theta_1) = n_2 \sin(\theta_2)). In terms of speed: n=c/vn = c/v.
  • Optical Phenomena

    • Critical Angle: The angle of incidence where the refracted ray travels along the boundary (9090^{\circ}).
    • Total Internal Reflection: Occurs when light hits a boundary at an angle greater than the critical angle, bouncing entirely back into the medium.
    • Prism Dispersion: White light contains all colors; a prism separates them because different wavelengths refract at slightly different angles (Red bends least, Violet bends most).
    • Rainbows:
      • Primary: Light undergoes one reflection and refraction inside raindrops.
      • Secondary: Light undergoes two reflections inside raindrops, causing colors to be reversed.
    • Atmospheric Color:
      • Blue Sky: Formed by the scattering of shorter (blue) wavelengths of light by the atmosphere (Rayleigh Scattering).
      • Red Sunsets: At sunset, light travels through more atmosphere; blue light is scattered away, leaving the longer red wavelengths.

DC Electricity and Cells

  • Charges

    • Neutral: Equal number of protons and electrons.
    • Negative: An excess of electrons.
    • Positive: A deficiency of electrons (more protons than electrons).
    • Charging Methods:
      1. Contact (Conduction): Transferring charge by touching a neutral object with a charged one.
      2. Induction: Charging an object by bringing a charged object nearby without touching, causing a migration of charges.
  • Laws and Units

    • Coulomb’s Law: The force between two charges is proportional to the product of the charges and inversely proportional to the square of the distance between them (F=kq1q2r2F = k \frac{q_1 q_2}{r^2}).
    • Units:
      • Electric Charge: Coulomb (CC).
      • Volt: Potential difference (V=J/CV = J/C).
      • Electric Current: Ampere (A=C/sA = C/s).
      • Electric Resistance: Ohm (Ω\Omega).
      • Electric Power: Watt (W=V×IW = V \times I).
  • Ohm’s Law

    • Formula: V=I×RV = I \times R
    • Rearrange for V: V=IRV = IR
    • Rearrange for R: R=VIR = \frac{V}{I}
  • Resistor Circuits

    • Scenario: Resistors of 5Ω5\,\Omega, 10Ω10\,\Omega, and 20Ω20\,\Omega; Power supply of 12V12\,V.
    • Total Resistance:
      • Series: Rtotal=5+10+20=35ΩR_{total} = 5 + 10 + 20 = 35\,\Omega.
      • Parallel: 1/Rtotal=1/5+1/10+1/20=4/20+2/20+1/20=7/20    Rtotal2.9Ω1/R_{total} = 1/5 + 1/10 + 1/20 = 4/20 + 2/20 + 1/20 = 7/20 \implies R_{total} \approx 2.9\,\Omega.
    • Current (II):
      • Series: I=12/350.34ampI = 12 / 35 \approx 0.34\,amp.
      • Parallel: I=12/2.94.1ampI = 12 / 2.9 \approx 4.1\,amp.
    • Power (PP):
      • Series: P=V×I=12×0.344.1wattP = V \times I = 12 \times 0.34 \approx 4.1\,watt.
      • Parallel: P=V×I=12×4.149wattP = V \times I = 12 \times 4.1 \approx 49\,watt.
  • Cells (Batteries)

    • Series Connection: Increases total Voltage; the available amperage remains that of a single cell.
    • Parallel Connection: Increases Available Amperage (capacity); the voltage remains that of a single cell.", "title": "Comprehensive Study Guide: Work, Power, Energy, Waves, and Electricity"}