Constant Net Force, Kinematics Derivations, and Gravitational Field Principles

Course Methodology and Momentum Principle Review

  • Pedagogical Strategy:

    • Assessment questions focus on applying fundamental principles to new situations rather than memorizing formulas or answers.
    • Problem-solving requires deep conceptual understanding to generate solutions from first principles.
  • Analysis of Discrete Momentum Data:

    • Given data points for an object moving along the x-axis:
      • At t=0 st = 0 \,\text{s}, initial x-momentum px,0=120 kg⋅m/sp_{x,0} = 120 \,\text{kg}\cdot\text{m/s}.
      • At t=1 st = 1 \,\text{s}, x-momentum px,1=100 kg⋅m/sp_{x,1} = 100 \,\text{kg}\cdot\text{m/s}.
      • At t=2 st = 2 \,\text{s}, x-momentum px,2=80 kg⋅m/sp_{x,2} = 80 \,\text{kg}\cdot\text{m/s}.
      • At t=3 st = 3 \,\text{s}, x-momentum px,3=60 kg⋅m/sp_{x,3} = 60 \,\text{kg}\cdot\text{m/s}.
    • Calculating Change in Momentum (Δpx\Delta p_x) and Net Force (Fnet,xF_{\text{net}, x}):
      • From t=0 st = 0 \,\text{s} to t=1 st = 1 \,\text{s}:             Δpx=px,1−px,0=100 kg⋅m/s−120 kg⋅m/s=−20 kg⋅m/s\Delta p_x = p_{x,1} - p_{x,0} = 100 \,\text{kg}\cdot\text{m/s} - 120 \,\text{kg}\cdot\text{m/s} = -20 \,\text{kg}\cdot\text{m/s}
      • Rate of change of momentum over interval Δt=1 s\Delta t = 1 \,\text{s}:             ΔpxΔt=−20 kg⋅m/s1 s=−20 kg⋅m/s2=−20 N\frac{\Delta p_x}{\Delta t} = \frac{-20 \,\text{kg}\cdot\text{m/s}}{1 \,\text{s}} = -20 \,\text{kg}\cdot\text{m/s}^2 = -20 \,\text{N}
      • From t=1 st = 1 \,\text{s} to t=2 st = 2 \,\text{s}:             Δpx=80 kg⋅m/s−100 kg⋅m/s=−20 kg⋅m/s\Delta p_x = 80 \,\text{kg}\cdot\text{m/s} - 100 \,\text{kg}\cdot\text{m/s} = -20 \,\text{kg}\cdot\text{m/s}ΔpxΔt=−20 N\frac{\Delta p_x}{\Delta t} = -20 \,\text{N}
    • Conclusions:
      • The net force acting on the object is constant throughout the entire time interval.
      • By the Momentum Principle, Fnet,x=ΔpxΔt=−20 NF_{\text{net}, x} = \frac{\Delta p_x}{\Delta t} = -20 \,\text{N}.
      • A net force of −20 N-20 \,\text{N} corresponds to a magnitude of 20 N20 \,\text{N} directed in the negative x-direction.
      • If the net force were zero, the change in momentum Δp\Delta p would be zero, resulting in a constant velocity and constant momentum.
  • Curriculum Roadmap:

    • Sections 2.2 to 2.7 & 2.8: Focus on physical systems subjected to a constant net force to derive exact, analytic solutions for predicting future motion.
    • Section 2.3 / 2.4 onward: Returns to examine systems subject to non-constant (varying) net forces.

Impulse and Average Net Force During Collisions

  • Golf Ball Collision Example:

    • A golf ball hit off a driver travels at a high speed of approximately 150 mph150 \,\text{mph}.
    • When the ball collides with a rigid steel plate, contact occurs over a finite time interval Δt\Delta t.
    • During the collision, the ball flattens, compresses, re-expands, and subsequently oscillates.
  • Neglecting Gravitational Force:

    • During high-speed collisions, the contact force exerted by the steel plate on the golf ball far exceeds the force of gravity.
    • Because the gravitational force is negligible in comparison, it is set to zero for the duration of the impact analysis.
    • General Rule: In collision dynamics, internal contact forces between colliding bodies dominate over ambient non-contact forces like gravity.
  • Definition of Time-Average Net Force (FavgF_{\text{avg}}):

    • The measured force F(t)F(t) during impact starts at zero, increases rapidly to a peak, and drops back to zero across interval Δt\Delta t
    • FavgF_{\text{avg}} is not an arithmetic mean of force values.
    • FavgF_{\text{avg}} is defined as a constant force value that produces the exact same integral (area under the curve) over time interval Δt\Delta t as the real time-varying force:         Δpx=∫titfFnet,x(t) dt=Favg,xΔt\Delta p_x = \int_{t_i}^{t_f} F_{\text{net}, x}(t) \, dt = F_{\text{avg}, x} \Delta t
    • The area under a force vs. time graph represents the total change in momentum (Δp\Delta p).
  • Fundamental Principles vs. Approximations:

    • Momentum Principle (General):Δp=FnetΔt\Delta \mathbf{p} = \mathbf{F}_{\text{net}} \Delta t
    • Relativistic Momentum Relation:p=γmv\mathbf{p} = \gamma m \mathbf{v}
    • Low-Speed Approximation: When speed vv is much less than the speed of light cc (v≪cv \ll c), the Lorentz factor γ≈1\gamma \approx 1.
    • Rule of Thumb: γ≈1\gamma \approx 1 can be assumed whenever speed is less than 10%10\% of the speed of light (v<0.10 cv < 0.10 \, c).

Kinematic Equations under Constant Net Force

  • Velocity as a Function of Time:

    • Starting from the Momentum Principle with γ=1\gamma = 1:         pfinal=pinitial+FnetΔt\mathbf{p}_{\text{final}} = \mathbf{p}_{\text{initial}} + \mathbf{F}_{\text{net}} \Delta t
    • Dividing through by constant mass mm yields the velocity update equation:         vfinal=vinitial+FnetmΔt\mathbf{v}_{\text{final}} = \mathbf{v}_{\text{initial}} + \frac{\mathbf{F}_{\text{net}}}{m} \Delta t
    • Under a constant net force, the velocity graph v(t)\mathbf{v}(t) is strictly linear with respect to time.
  • Average Velocity under Constant Net Force:

    • Because the velocity-time relationship is strictly linear for constant forces, the time-average velocity equals the arithmetic mean of the initial and final velocities:         vavg=12(vinitial+vfinal)\mathbf{v}_{\text{avg}} = \frac{1}{2} (\mathbf{v}_{\text{initial}} + \mathbf{v}_{\text{final}})
    • Critical Warning: This arithmetic mean relationship is only valid when net force is constant. It cannot be applied if the net force varies over time.
  • Derivation of Position Update Equation:

    • Definition of Average Velocity (General):rfinal=rinitial+vavgΔt\mathbf{r}_{\text{final}} = \mathbf{r}_{\text{initial}} + \mathbf{v}_{\text{avg}} \Delta t
    • Substituting vfinal=vinitial+FnetmΔt\mathbf{v}_{\text{final}} = \mathbf{v}_{\text{initial}} + \frac{\mathbf{F}_{\text{net}}}{m} \Delta t into the arithmetic average velocity formula:         vavg=12(vinitial+vinitial+FnetmΔt)=vinitial+12FnetmΔt\mathbf{v}_{\text{avg}} = \frac{1}{2} \left( \mathbf{v}_{\text{initial}} + \mathbf{v}_{\text{initial}} + \frac{\mathbf{F}_{\text{net}}}{m} \Delta t \right) = \mathbf{v}_{\text{initial}} + \frac{1}{2} \frac{\mathbf{F}_{\text{net}}}{m} \Delta t
    • Substituting this expression for vavg\mathbf{v}_{\text{avg}} into the general position definition:         rfinal=rinitial+(vinitial+12FnetmΔt)Δt\mathbf{r}_{\text{final}} = \mathbf{r}_{\text{initial}} + \left( \mathbf{v}_{\text{initial}} + \frac{1}{2} \frac{\mathbf{F}_{\text{net}}}{m} \Delta t \right) \Delta t
    • Distributing Δt\Delta t yields the complete analytic position prediction equation for constant net force:         rfinal=rinitial+vinitialΔt+12Fnetm(Δt)2\mathbf{r}_{\text{final}} = \mathbf{r}_{\text{initial}} + \mathbf{v}_{\text{initial}} \Delta t + \frac{1}{2} \frac{\mathbf{F}_{\text{net}}}{m} (\Delta t)^2
  • Summary of Core Constant-Force Equations:

    1. vfinal=vinitial+FnetmΔt\mathbf{v}_{\text{final}} = \mathbf{v}_{\text{initial}} + \frac{\mathbf{F}_{\text{net}}}{m} \Delta t
    2. vavg=12(vinitial+vfinal)\mathbf{v}_{\text{avg}} = \frac{1}{2} (\mathbf{v}_{\text{initial}} + \mathbf{v}_{\text{final}}) (Constant force only)
    3. rfinal=rinitial+vavgΔt\mathbf{r}_{\text{final}} = \mathbf{r}_{\text{initial}} + \mathbf{v}_{\text{avg}} \Delta t
    4. rfinal=rinitial+vinitialΔt+12Fnetm(Δt)2\mathbf{r}_{\text{final}} = \mathbf{r}_{\text{initial}} + \mathbf{v}_{\text{initial}} \Delta t + \frac{1}{2} \frac{\mathbf{F}_{\text{net}}}{m} (\Delta t)^2

Analytical Application: Fan Cart vs. Fan Truck

  • System Setup:

    • A fan cart (car) has mass mcar=mm_{\text{car}} = m.
    • A fan truck has double the mass mtruck=2mm_{\text{truck}} = 2m.
    • Both objects experience the exact same constant forward pushing force Fnet,x=+FF_{\text{net}, x} = +F generated by pushing air backwards.
    • Both objects start from rest: vinitial,x=0v_{\text{initial}, x} = 0
    • Both objects travel the exact same linear distance dd: Δx=d\Delta x = d
  • Derivation of Travel Time (Δt\Delta t):

    • Using the 1D position equation:         Δx=vinitial,xΔt+12Fnet,xm(Δt)2\Delta x = v_{\text{initial}, x} \Delta t + \frac{1}{2} \frac{F_{\text{net}, x}}{m} (\Delta t)^2
    • Substitute known values (Δx=d\Delta x = d, vinitial,x=0v_{\text{initial}, x} = 0, Fnet,x=FF_{\text{net}, x} = F):         d=12Fm(Δt)2d = \frac{1}{2} \frac{F}{m} (\Delta t)^2
    • Solving for Δt\Delta t:         (Δt)2=2mdF  ⟹  Δt=2mdF(\Delta t)^2 = \frac{2 m d}{F} \implies \Delta t = \sqrt{\frac{2 m d}{F}}
    • Proportionality Analysis for Time:Δt∝m\Delta t \propto \sqrt{m}
    • Evaluating the truck (2m2m) relative to the car (mm):         Δttruck=2⋅Δtcar\Delta t_{\text{truck}} = \sqrt{2} \cdot \Delta t_{\text{car}}
    • Conclusion: The car reaches the finish line first because it has a smaller time interval. The truck takes a factor of 2\sqrt{2} longer.
  • Derivation of Final Velocity (vfinal,xv_{\text{final}, x}):

    • Substitute the time equation Δt=2mdF\Delta t = \sqrt{\frac{2 m d}{F}} into the velocity update formula:         vfinal,x=0+Fm(2mdF)v_{\text{final}, x} = 0 + \frac{F}{m} \left( \sqrt{\frac{2 m d}{F}} \right)
    • Bringing the factor Fm\frac{F}{m} inside the radical:         vfinal,x=(Fm)2(2mdF)=2Fdmv_{\text{final}, x} = \sqrt{\left( \frac{F}{m} \right)^2 \left( \frac{2 m d}{F} \right)} = \sqrt{\frac{2 F d}{m}}
    • Proportionality Analysis for Final Velocity:vfinal,x∝1mv_{\text{final}, x} \propto \frac{1}{\sqrt{m}}
    • Evaluating the truck (2m2m) relative to the car (mm):         vtruck=12vcarv_{\text{truck}} = \frac{1}{\sqrt{2}} v_{\text{car}}
    • Conclusion: The car attains a higher final velocity at the finish line by a factor of 2\sqrt{2} compared to the truck.

Gravitational Field and Gravitational Force

  • Gravitational Field Definition:

    • Near Earth's surface, the gravitational force exerted on an object of mass mm is given by:         Fgrav=mg\mathbf{F}_{\text{grav}} = m \mathbf{g}
    • g\mathbf{g} represents the gravitational field produced by surrounding objects (e.g., Earth).
    • Magnitude near Earth's surface: g≈9.8 N/kgg \approx 9.8 \,\text{N/kg} (or 9.8 m/s29.8 \,\text{m/s}^2).
    • Direction: Directed vertically downward toward the center of Earth.
  • Pedagogical Clarification on Terminology:

    • Referring to gg as "acceleration due to gravity" is physically imprecise.
    • The correct term is the gravitational field of the source object.
    • An object only accelerates at gg if gravity is the sole force acting on it (free fall in a vacuum).
  • Conceptual Application Questions:

    • Question 1: Comparing gravitational forces on Ball A (mass mm) and Ball B (mass 2m2m):
      • Fgrav,A=mg\mathbf{F}_{\text{grav}, A} = m \mathbf{g}
      • Fgrav,B=2mg\mathbf{F}_{\text{grav}, B} = 2 m \mathbf{g}
      • Result: Ball B experiences twice as much gravitational force as Ball A.
    • Question 2: Dropping Ball A (mm) and Ball B (2m2m) from rest over distance dd:
      • While the force on Ball B is double (2mg2mg vs. mgmg), its inertia/mass is also double (2m2m vs. mm).
      • The resulting acceleration for both objects in free fall is identical:             a=Fnetm=mgm=ga = \frac{F_{\text{net}}}{m} = \frac{m g}{m} = g

Questions & Discussion

  • Question: What is the net force acting on an object if its momentum changes from 120 kg⋅m/s120 \,\text{kg}\cdot\text{m/s} to 100 kg⋅m/s100 \,\text{kg}\cdot\text{m/s} and then to 80 kg⋅m/s80 \,\text{kg}\cdot\text{m/s} in equal 1-second intervals?

    • Response: The change in momentum per second is −20 kg⋅m/s2-20 \,\text{kg}\cdot\text{m/s}^2. Therefore, the net force is constant at −20 N-20 \,\text{N} (directed in the negative x-direction).
  • Question: If force is constant, is net force zero?

    • Response: No. A constant non-zero net force causes a constant rate of change in momentum (ΔpΔt=Fnet\frac{\Delta p}{\Delta t} = F_{\text{net}}). If the net force were zero, the momentum would remain entirely unchanged over time.
  • Question: Is gravitational force on a heavier ball larger, and does it fall faster?

    • Response: The gravitational force Fgrav=mgF_{\text{grav}} = mg is twice as large on a ball of mass 2m2m compared to mass mm. However, because force scales linearly with mass, the acceleration a=Fm=ga = \frac{F}{m} = g remains identical for both balls in the absence of air resistance.