Unit 6: Linear Momentum, Impulse, and Collisions

Unit 6: Linear Momentum, Impulse and Collisions

Introduction

  • Quote by Neil deGrasse Tyson: "Physics is the only profession in which prophecy is not only accurate but routine."

Before We Begin

Power
  • Definition:
    • Power is the rate of energy transfer.
  • Mathematical Representation:
    • Average power ($ar{P}$) is given by:
      ar{P} = rac{W}{ riangle t}
    • Applying the definition of work:
      ar{P} = rac{W}{ riangle t} = rac{F riangle x}{ riangle t} = F ar{v} ext{cos} heta
  • Units:
    • The unit of power is the Watt ($W$):
      1W = rac{J}{s} = kg rac{m^2}{s^3}
    • In the U.S. customary system, power is measured in horsepower ($hp$):
      1hp=746W1hp = 746W
    • Important Note: Do not confuse $[W]$ from Watts with “$W$” from work!
    • For electric power generation, the customary unit is kilowatt-hour ($kWh$) as a measure of energy:
      1kWh=3.60imes106J1 kWh = 3.60 imes 10^6 J

Example Problem

  • Problem Statement:
    • A $1.00 imes 10^3 kg$ elevator car carries a maximum load of $8.00 imes 10^2 kg$. A constant frictional force of $4.00 imes 10^3 N$ retards its motion upward.
    • Question: What minimum power, in kilowatts, must the motor deliver to lift the fully loaded elevator car at a constant speed ($v = 3.00 m/s$)?

Definition of Momentum

  • Momentum is defined as the tendency to continue moving in some direction.
  • Importance: Relevant in isolated systems, where two or more objects interact through collisions.
  • Types of Momentum:
    1. Linear Momentum:
    • Movement in a straight line or the same direction (e.g., running at speed with direction).
    1. Angular Momentum:
    • Movement radially about an axis (e.g., ballerina spinning or tetherball moving around a pole).
  • Focus: This unit concentrates on linear momentum.

Linear Momentum ($p$)

Mathematical Description
  • Definition:
    • Linear Momentum ($p$) is mathematically described as:
      p=mimesvp = m imes v
    • Where:
    • $m$ = Mass of an object in kilograms
    • $v$ = Velocity in meters per second
  • SI Unit:
    • The unit for momentum is $kg imes m/s$ (kilogram-meter per second).
Proportional Relationships
  • Momentum is directly proportional to both mass and velocity:
    • If velocity is constant, then momentum increases with increasing mass:
      pextincreasesasmextincreases,givenvextisconstant.p ext{ increases as } m ext{ increases, given } v ext{ is constant.}
    • If mass is constant, then momentum increases with increasing velocity:
      pextincreasesasvextincreases,givenmextisconstant.p ext{ increases as } v ext{ increases, given } m ext{ is constant.}
Sample Problem
  • Problem Statement: What velocity would a smaller mass ($m1$) need to achieve the same momentum as a bigger mass ($m2$) traveling at some speed ($v_2$)?
  • Step 1: Set momentum of $m1$ equal to that of $m2$:
    • p<em>1=p</em>2p<em>1 = p</em>2
    • Thus,
      m<em>1v</em>1=m<em>2v</em>2m<em>1 v</em>1 = m<em>2 v</em>2
  • To find $v_1$:
    • v1 = v2 rac{m2}{m1}
Example Calculation
  • Given:
    • $m1 = 5 kg$, $m2 = 10 kg$, $v_2 = 30 m/s$
  • Calculation:
    • v1 = v2 rac{m2}{m1} = 30 m/s imes rac{10 kg}{5 kg} = 60 m/s

Momentum-Force Relation

Changing Momentum
  • Definition: The momentum ($p$) of an object can be changed ($ riangle p$) only when an external force ($F$) is applied to the object over a duration of time ($ riangle t = t{final} - t{initial}$).
  • Change in momentum mathematically expressed:
    • rianglep=mimesrianglevriangle p = m imes riangle v
  • Taking the ratio of momentum change and time gives:
    • rac{ riangle p}{ riangle t} = m imes rac{ riangle v}{ riangle t}
  • By definition, acceleration ($a$) is given by:
    • a = rac{ riangle v}{ riangle t}
  • This leads to:
    • racriangleprianglet=mimesarac{ riangle p}{ riangle t} = m imes a
  • Note: The symbol $ riangle$ signifies “The change in [something] …” and is pronounced “delta [something].”
Newton's Second Law and Impulse Definition
  • Newton’s second law states that the force exerted on an object is equal to the mass times acceleration:
    • F=mimesaF = m imes a
  • Thus, we can express:
    • F = rac{ riangle p}{ riangle t}
  • The impulse ($I$) can be defined as:
    • I=Fau=rianglep=m(v<em>fv</em>i)I = F au = riangle p = m(v<em>f - v</em>i)
Example Problem
  • Problem Statement: A runaway train car with mass $15000 kg$ is moving at a velocity of $5.4 m/s$. Determine the time required for a force of $1500 N$ to bring the car to rest.
Impulse Calculation
  • Definition of Impulse:
    • I=rianglep=FimesriangletI = riangle p = F imes riangle t
  • Change in momentum equals the average net external force multiplied by the time this force is applied.
  • Example Problem:
    • Calculate the final speed of a $110 kg$ rugby player initially running at $8.00 m/s$ who collides head-on with a padded goalpost and experiences a backward force of $1.76 imes 10^4 N$ for $5.50 imes 10^{-2} s$.

Law of Conservation of Momentum

  • Momentum is a conserved quantity stated as:
    • extΣp<em>i=extΣp</em>fext{Σ}p<em>i = ext{Σ}p</em>f
  • The change in momentum for all agents can be expressed:
    • For object 1:
      rianglep<em>1=F</em>1riangletriangle p<em>1 = F</em>1 riangle t
    • For object 2:
      rianglep<em>2=F</em>2riangletriangle p<em>2 = F</em>2 riangle t
  • According to Newton’s third law:
    • F<em>1=F</em>2F<em>1 = -F</em>2
  • This means:
    • rianglep<em>1=rianglep</em>2riangle p<em>1 = - riangle p</em>2, leading to:
    • p<em>f1p</em>i1=(p<em>f2p</em>i2)p<em>f1 - p</em>i1 = -(p<em>f2 - p</em>i2)
  • Rearranging gives:
    • p<em>f1p</em>i1=p<em>i2p</em>f2p<em>f1 - p</em>i1 = p<em>i2 - p</em>f2
    • Thus:
      p<em>f1+p</em>f2=p<em>i2+p</em>i1p<em>f1 + p</em>f2 = p<em>i2 + p</em>i1
    • This establishes the law of conservation of momentum true in isolated systems where net external force is zero:
    • F<em>1+F</em>2++FN=0F<em>1 + F</em>2 + … + F_N = 0

Collisions

Types of Collisions
  1. Elastic Collisions:

    • A collision that conserves kinetic energy:
      K<em>i=K</em>fK<em>i = K</em>f
    • Expressed mathematically:
      rac{1}{2}m1v{1i}^2 + rac{1}{2}m2v{2i}^2 = rac{1}{2}m1v{1f}^2 + rac{1}{2}m2v{2f}^2
    • Objects bounce off one another after impact:
      p<em>1i+p</em>2i=p<em>1f+p</em>2fp<em>{1i} + p</em>{2i} = p<em>{1f} + p</em>{2f}
  2. Inelastic Collisions:

    • A collision that does not conserve kinetic energy
    • Objects stick together after impact, sharing final velocity:
      m<em>1v</em>1i+m<em>2v</em>2i=(m<em>1+m</em>2)vfm<em>1v</em>{1i} + m<em>2v</em>{2i} = (m<em>1 + m</em>2)v_f
Strategic Steps for Solving Collision Problems
  1. Coordinates:
    • Choose a coordinate axis that aligns with the direction of motion.
  2. Diagram:
    • Sketch the problem to visualize forces and motion.
  3. Conservation of Momentum:
    • Write expressions for total momentum in the initial and final states for both types of collisions.
  4. Conservation of Energy:
    • Write total energy conservation expressions only for elastic collisions.
  5. Solve Equations:
Example Problem (Elastic Collision)
  • A block of mass $1.60 kg$ moves right at $4 m/s$ on a frictionless track and collides with a massless spring attached to a second block of mass $2.10 kg$ moving left at $-2.50 m/s$.
  • Questions:
    1. Determine the velocity of the second block when the first block is moving at $3.00 m/s$.
    2. Find the compression of the spring at that moment.
Example Problem (Inelastic Collision)
  • Problem Statement:
    • Two objects move in the same direction with velocities $v1 = 5 m/s$ and $v2 = 10 m/s$. Given $m1 = 10 kg$ and $m2 = 20 kg$, what is their final velocity after a perfectly inelastic collision?
  • Solution Approach:
    • Inelastic objects stick together post-impact:
      m<em>1v</em>1i+m<em>2v</em>2i=(m<em>1+m</em>2)vfm<em>1v</em>{1i} + m<em>2v</em>{2i} = (m<em>1 + m</em>2)v_f
Final Velocity Calculation
  • Substitute and solve:
    • vf = rac{m1 v{1i} + m2 v{2i}}{m1 + m_2} = rac{10 kg imes 5 m/s + 20 kg imes 10 m/s}{10 kg + 20 kg} = 8.3 m/s

Collisions and Kinetic Energy

  • In all systems, energy is conserved if all energy transfer mechanisms are considered.
  • Kinetic Energy Formula:
    • ext{Total } K.E.: ext{Σ} rac{1}{2} mi vi^2 = ext{Σ} rac{1}{2} mf vf^2
  • For elastic collisions:
    • K<em>K</em>i=K<em>K</em>fK<em>{K</em>i} = K<em>{K</em>f}
  • For inelastic collisions:
    • K<em>K</em>i<br/>eqK<em>K</em>fK<em>{K</em>i} <br /> eq K<em>{K</em>f}
    • Energy conservation may involve other forms:
    • K<em>E</em>i=K<em>E</em>f+extΣUotherK<em>E</em>i = K<em>E</em>f + ext{Σ} U_{other}
  • Additional Energy Forms: Heat, sound, etc.