Kinetics of a Particle: Impulse and Momentum Study Notes

Principle of Linear Impulse and Momentum

  • Development of the Principle: The principle is derived by integrating the equation of motion for a particle with respect to time. Starting with Newton’s Second Law: F=ma=mdvdt\sum \mathbf{F} = m\mathbf{a} = m \frac{d\mathbf{v}}{dt}. Rearranging the terms yields Fdt=mdv\sum \mathbf{F} \, dt = m \, d\mathbf{v}. Integrating between the limits v=v1\mathbf{v} = \mathbf{v}_1 at t=t1t = t_1 and v=v2\mathbf{v} = \mathbf{v}_2 at t=t2t = t_2 results in: mv1+t1t2Fdt=mv2m\mathbf{v}_1 + \sum \int_{t_1}^{t_2} \mathbf{F} \, dt = m\mathbf{v}_2.

  • Linear Momentum (L\mathbf{L}): Defined as the vector quantity L=mv\mathbf{L} = m\mathbf{v}.     * Since mass (mm) is a positive scalar, the momentum vector L\mathbf{L} maintains the same direction as the velocity vector (v\mathbf{v}).     * Units: Expressed in units of mass-velocity, such as kgm/s\text{kg} \cdot \text{m/s} or slugft/s\text{slug} \cdot \text{ft/s}.

  • Linear Impulse (I\mathbf{I}): Defined as the integral I=Fdt\mathbf{I} = \int \mathbf{F} \, dt.     * This vector measures the cumulative effect of a force over the duration it acts.     * It acts in the direction of the force.     * Units: Expressed in units of force-time, such as Ns\text{N} \cdot \text{s} or lbs\text{lb} \cdot \text{s}.     * Constant Force: For a force constant in both magnitude and direction (Fc\mathbf{F}_c), the impulse simplifes to: I=Fc(t2t1)\mathbf{I} = \mathbf{F}_c(t_2 - t_1).     * Variable Force: Graphically, the magnitude of the impulse is represented as the area under the force-versus-time curve.

  • Application in Dynamics: The principle Initial Momentum+Sum of Impulses=Final Momentum\text{Initial Momentum} + \text{Sum of Impulses} = \text{Final Momentum} provides a direct method for finding final velocities when forces and time intervals are known. This is a one-step alternative to the two-step process of finding acceleration via F=ma\sum \mathbf{F} = m\mathbf{a} and then integrating a=dv/dta = d\mathbf{v}/dt.

  • Scalar Equations: Resolve the vector equation into three scalar components:     * m(vx)1+t1t2Fxdt=m(vx)2m(v_x)_1 + \sum \int_{t_1}^{t_2} F_x \, dt = m(v_x)_2     * m(vy)1+t1t2Fydt=m(vy)2m(v_y)_1 + \sum \int_{t_1}^{t_2} F_y \, dt = m(v_y)_2     * m(vz)1+t1t2Fzdt=m(vz)2m(v_z)_1 + \sum \int_{t_1}^{t_2} F_z \, dt = m(v_z)_2

Linear Impulse and Momentum for a System of Particles

  • Equation of Motion for Systems: For a collection of particles, the sum of external forces is related to the derivative of the total momentum: Fi=midvidt\sum \mathbf{F}_i = \sum m_i \frac{d\mathbf{v}_i}{dt}. Internal forces (fi\mathbf{f}_i) cancel out due to Newton’s Third Law (equal and opposite collinear pairs).

  • Integrative Principle: The initial total linear momenta plus the sum of external impulses equals the final total linear momenta: mi(vi)1+t1t2Fidt=mi(vi)2\sum m_i(\mathbf{v}_i)_1 + \sum \int_{t_1}^{t_2} \mathbf{F}_i \, dt = \sum m_i(\mathbf{v}_i)_2.

  • Mass Center (GG): The total linear momentum is equivalent to the momentum of a ‘fictitious’ aggregate particle of total mass m=mim = \sum m_i moving at the velocity of the center of mass (vG\mathbf{v}_G). The equation becomes: m(vG)1+t1t2Fidt=m(vG)2m(\mathbf{v}_G)_1 + \sum \int_{t_1}^{t_2} \mathbf{F}_i \, dt = m(\mathbf{v}_G)_2.

Conservation of Linear Momentum for Systems

  • Definition: Linear momentum is conserved when the sum of external impulses acting on a system is zero. Mathematically: mi(vi)1=mi(vi)2\sum m_i(\mathbf{v}_i)_1 = \sum m_i(\mathbf{v}_i)_2.

  • Condition of Zero External Impulse: Occurs when no external forces act or when external forces are nonimpulsive.

  • Impulsive vs. Nonimpulsive Forces:     * Impulsive Forces: Large forces acting over a very short time interval (Δt\Delta t) that cause significant momentum changes (e.g., explosions or collisions).     * Nonimpulsive Forces: Small forces relative to impulsive ones, such as weight, air resistance, or low-stiffness springs, whose effect during a very short Δt\Delta t is negligible.

  • Center of Mass Velocity: If linear momentum is conserved, the velocity of the mass center (vG\mathbf{v}_G) remains constant throughout the motion study.

Mechanics of Impact: Central and Oblique

  • Impact Definition: A collision between two bodies over a very short duration, generating large impulsive forces.

  • Types of Impact:     * Central Impact: The directions of motion for both mass centers lie along the line of impact (the line perpendicular to the plane of contact).     * Oblique Impact: The motion of one or both particles occurs at an angle to the line of impact.

  • The Coefficient of Restitution (ee): An experimental value relating the relative separation velocity to the relative approach velocity: e=(vB)2(vA)2(vA)1(vB)1e = \frac{(v_B)_2 - (v_A)_2}{(v_A)_1 - (v_B)_1}.     * Elastic Impact (e=1e = 1): No energy loss; deformation impulse equals restitution impulse.     * Plastic/Inelastic Impact (e=0e = 0): Maximum energy loss; bodies stick together and move at a common velocity.

  • Oblique Impact Analysis Procedure:     1. Establish the xx-axis along the line of impact and the yy-axis along the plane of contact.     2. Conservation of momentum for the system in the xx direction: m(vx)1=m(vx)2\sum m(v_x)_1 = \sum m(v_x)_2.     3. Coefficient of restitution applies along the line of impact (xx direction): e=(vBx)2(vAx)2(vAx)1(vBx)1e = \frac{(v_{Bx})_2 - (v_{Ax})_2}{(v_{Ax})_1 - (v_{Bx})_1}.     4. Conservation of momentum for each individual particle in the yy direction (since no impulse acts perpendicular to the line of impact): (vAy)1=(vAy)2(v_{Ay})_1 = (v_{Ay})_2 and (vBy)1=(vBy)2(v_{By})_1 = (v_{By})_2.

Angular Momentum and Relation to Moment of a Force

  • Scalar Definition: The angular momentum (HOH_O) of a particle about point OO is the moment of its linear momentum: (HO)z=d(mv)(H_O)_z = d \cdot (mv).     * Here, dd is the perpendicular distance (moment arm) from OO to the line of action of mvmv.

  • Vector Definition: Defined via cross product: HO=r×mv\mathbf{H}_O = \mathbf{r} \times m\mathbf{v}.     * Can be evaluated via determinant: HO=(ijkrxryrzmvxmvymvz)\mathbf{H}_O = \begin{pmatrix} \mathbf{i} & \mathbf{j} & \mathbf{k} \\ r_x & r_y & r_z \\ m v_x & m v_y & m v_z \end{pmatrix}.

  • Relation to Moments: The resultant moment about point OO (MO\sum \mathbf{M}_O) equals the time rate of change of the angular momentum (H˙O\dot{\mathbf{H}}_O): MO=H˙O\sum \mathbf{M}_O = \dot{\mathbf{H}}_O.     * For a system of particles: MO=(ri×Fi)=ddt(ri×mivi)\sum \mathbf{M}_O = \sum (\mathbf{r}_i \times \mathbf{F}_i) = \frac{d}{dt} \sum (\mathbf{r}_i \times m_i \mathbf{v}_i).

Principle of Angular Impulse and Momentum

  • The Principle: Integrating the moment equation over time: (HO)1+t1t2MOdt=(HO)2(\mathbf{H}_O)_1 + \sum \int_{t_1}^{t_2} \mathbf{M}_O \, dt = (\mathbf{H}_O)_2.     * Angular Impulse: The integral MOdt=(r×F)dt\int \mathbf{M}_O \, dt = \int (\mathbf{r} \times \mathbf{F}) \, dt.

  • Conservation of Angular Momentum: If the sum of angular impulses about an axis is zero, the angular momentum about that axis is constant: (HO)1=(HO)2(\mathbf{H}_O)_1 = (\mathbf{H}_O)_2.     * Common in central force problems where the force always passes through the center of rotation (moment arm is zero).

Steady Flow of a Fluid Stream

  • Control Volume Logic: Analyzing fluid particles entering and exiting a region. Flow is steady if the rate of mass entering equals the rate exiting.

  • Force Equilibrium: The resultant force F\sum \mathbf{F} on a control volume equals the mass flow rate multiplied by the change in velocity: F=dmdt(voutvin)\sum \mathbf{F} = \frac{dm}{dt}(\mathbf{v}_{out} - \mathbf{v}_{in}).

  • Moment Equilibrium: MO=dmdt(rout×voutrin×vin)\sum \mathbf{M}_O = \frac{dm}{dt}(\mathbf{r}_{out} \times \mathbf{v}_{out} - \mathbf{r}_{in} \times \mathbf{v}_{in}).

  • Mass Flow Rate (dmdt\frac{dm}{dt}): Related to fluid density (ρ\rho), velocity (vv), and cross-sectional area (AA): dmdt=ρvA\frac{dm}{dt} = \rho v A.

  • Discharge/Volumetric Flow (QQ): Q=vAQ = v A. Measured in dm3/sdm^3/s or ft3/sft^3/s.

Propulsion and Variable Mass Mechanics

  • Control Volumes with Changing Mass: Used for rockets (losing mass) or scoops (gaining mass).

  • Losing Mass (Rocket Propulsion): The equation of motion is: Fcv=mdvdtvD/edmedt\sum \mathbf{F}_{cv} = m \frac{d\mathbf{v}}{dt} - \mathbf{v}_{D/e} \frac{dm_e}{dt}.     * Fcv\sum \mathbf{F}_{cv}: External forces (drag, weight).     * mdvdtm \frac{d\mathbf{v}}{dt}: Mass of the device times its acceleration (mam \cdot a).     * vD/edmedt\mathbf{v}_{D/e} \frac{dm_e}{dt}: The thrust (TT), where vD/e\mathbf{v}_{D/e} is the velocity of the ejected mass relative to the device.

  • Gaining Mass: The equation of motion is: Fcv=mdvdt+vD/idmidt\sum \mathbf{F}_{cv} = m \frac{d\mathbf{v}}{dt} + \mathbf{v}_{D/i} \frac{dm_i}{dt}.     * vD/i\mathbf{v}_{D/i}: Velocity of the injected mass relative to the device.     * The term vD/idmidt\mathbf{v}_{D/i} \frac{dm_i}{dt} represents the retarding force (RR) resisting motion as mass is gathered.

Questions & Discussion

  • Example 15.1: 100-kg stone with constant force:     * Initial state: at rest. F=200N\mathbf{F} = 200 \, \text{N} at 4545^{\circ}, time t=10st = 10 \, \text{s}, μk=0\mu_k = 0.     * Using m(vx)1+Fxdt=m(vx)2\sum m(v_{x})_1 + \sum \int F_x \, dt = m(v_{x})_2:         0+200cos(45)10=100v2    v2=14.1m/s0 + 200 \cos(45^{\circ}) \cdot 10 = 100 \cdot v_2 \implies v_2 = 14.1 \, \text{m/s}.     * Normal force calculation (Fy=0\sum F_y = 0): Nc(10)981(10)+200sin(45)10=0    Nc=840NN_c(10) - 981(10) + 200 \sin(45^{\circ}) \cdot 10 = 0 \implies N_c = 840 \, \text{N}.

  • Example 15.4: Boxcar and Tank Car Collision:     * Boxcar A (15Mg15 \, \text{Mg}, 1.5m/s1.5 \, \text{m/s}, +x+x) and Tank car B (12Mg12 \, \text{Mg}, 0.75m/s0.75 \, \text{m/s}, x-x).     * Coupling means v2v_2 is shared.     * Conservation of momentum: (15000)(1.5)(12000)(0.75)=(27000)v2    v2=0.5m/s(15000)(1.5) - (12000)(0.75) = (27000)v_2 \implies v_2 = 0.5 \, \text{m/s}.     * Average Force (FavgF_{avg}) over 0.8s0.8 \, \text{s}: (15000)(1.5)Favg(0.8)=(15000)(0.5)    Favg=18.8kN(15000)(1.5) - F_{avg}(0.8) = (15000)(0.5) \implies F_{avg} = 18.8 \, \text{kN}.

  • Example 15.14: Ball on a Cord with constant radial speed:     * Initially: r1=1.75ftr_1 = 1.75 \, \text{ft}, v1=4ft/sv_1 = 4 \, \text{ft/s}. Cord pulled at vc=6ft/sv_c = 6 \, \text{ft/s}.     * Final: r2=0.6ftr_2 = 0.6 \, \text{ft}.     * Conservation of angular momentum: r1mv1=r2mvθ    (1.75)v1=(0.6)vθr_1 m v_1 = r_2 m v_{\theta} \implies (1.75)v_1 = (0.6)v_{\theta}.     * (1.75)(4)=(0.6)vθ    vθ=11.67ft/s(1.75)(4) = (0.6)v_{\theta} \implies v_{\theta} = 11.67 \, \text{ft/s}.     * Total final speed: v2=11.672+62=13.1ft/sv_2 = \sqrt{11.67^2 + 6^2} = 13.1 \, \text{ft/s}.