Conservative Principle and Linear Momentum

PHY 101: General Physics

Lecture Topic: Conservative Principles, Conservative Forces, and Conservation of Linear Momentum

Instructors: Dr. H. K. Idu & A. O. Chikwendu
Institution: David Umahi Federal University of Health Sciences, Uburu, Ebonyi State

Conservative Principles

  • Definition:

    • Conservation principles state that certain physical quantities are conserved (remain unchanged) over time in closed or isolated systems, where no external influences act.

  • Conserved Quantities:

    • Includes:

    • Conservation of energy

    • Conservation of momentum

    • Conservation of angular momentum

    • Conservation of mass (in non-relativistic contexts)

  • Significance:

    • Conservation laws simplify problem-solving by providing invariants.


Conservative Forces

  • Definition:

    • A force is conservative if the work done by it on an object moving between two points is independent of the path taken and depends only on the initial and final positions.

  • Mathematical Formulation:

    • For a force FF, the work WW along a path from AA to BB is given by:
      W=racdWds<br>ightarrowextintegratedfromAtoBW = rac{dW}{ds} <br>ightarrow ext{integrated from A to B}

    • If WW is path-independent, then FF is a conservative force.

    • Equivalently:

    • The curl of FF is zero:
      <br>ablaimesF=0<br>abla imes F = 0

    • FF can be expressed as the negative gradient of a scalar potential energy function VV:
      F=<br>ablaVF = -<br>abla V


Examples of Conservative Forces

  • Gravitational Force:

    • Equation: F=mgextbfjF = -mg extbf{j} (considering near Earth's surface)

    • Potential Energy: V=mghV = mgh

  • Electrostatic Force (Coulomb's Law):

    • The work done is path-independent.

  • Spring Force (Hooke's Law):

    • Equation: F=kxextbfiF = -kx extbf{i}

    • Potential Energy: V=rac12kx2V = rac{1}{2}kx^2


Non-Conservative Forces

  • Definition:

    • Forces where work depends on the path taken, such as friction or drag.

  • Work in Non-Conservative Forces:

    • For friction, work dissipates energy as heat, violating path independence.

Relation to Conservation of Mechanical Energy

  • Mechanics of Conservative Forces:

    • The total mechanical energy E=K+VE = K + V (kinetic + potential) is conserved in an isolated system:
      riangleK+riangleV=0<br>ightarrowKf+Vf=Ki+Viriangle K + riangle V = 0 <br>ightarrow K_f + V_f = K_i + V_i

  • Proof:

    • From the Work-Energy Theorem: W=riangleKW = riangle K.

    • For conservative forces: W=riangleVW = - riangle V, so riangleK=riangleVriangle K = - riangle V.

Involvement of Non-Conservative Forces

  • If non-conservative forces act:
    Wnc=riangleK+riangleVW_{nc} = riangle K + riangle V


Applications

  • Pendulum Motion:

    • Energy oscillates between kinetic and potential.

  • Roller Coasters:

    • Design loops using energy conservation to ensure safe speeds.


Conservation of Linear Momentum

  • Definition:

    • Linear momentum pp of a particle is defined as:
      p=mvp = mv

    • For a system of particles, the total momentum PP is:
      P=extstylepiP = extstyle{\bigoplus} p_i

  • Conservation Statement:

    • The conservation of linear momentum states that in any system of mutually interacting or impinging particles, the linear momentum in any fixed direction remains constant unless external forces act on it in that direction.

    • In an isolated system (with no external forces), the total momentum remains constant:
      extTotalmomentum=Pinitial=Pfinalext{Total momentum} = P_{initial} = P_{final}

  • Connection to Newton's Third Law:

    • Internal forces cancel in pairs, thus the net change in momentum is zero.


Types of Collisions

  • Momentum Conservation:

    • Momentum conservation applies to all collisions, but kinetic energy may not be conserved.

  • Elastic Collision:

    • Both momentum and kinetic energy are conserved.

    • For 1D head-on collisions:

    • Masses involved: m1,m2m_1, m_2

    • Momentum before and after:
      m1v1i+m2v2i=m1v1f+m2v2fm_1 v_{1_i} + m_2 v_{2_i} = m_1 v_{1_f} + m_2 v_{2_f}

    • Kinetic energy before and after:
      rac12m1v1i2+rac12m2v2i2=rac12m1v1f2+rac12m2v2f2rac{1}{2} m_1 v_{1_i}^2 + rac{1}{2} m_2 v_{2_i}^2 = rac{1}{2} m_1 v_{1_f}^2 + rac{1}{2} m_2 v_{2_f}^2

    • Solution for final velocities is provided with suitable equations.

  • Inelastic Collision:

    • Momentum is conserved, but kinetic energy is not.

    • Example: Objects stick together post-collision.

    • Coefficient of restitution:
      e < 1

    • Perfectly Inelastic Collision:

    • Final velocity calculation:
      vf=racm1v1i+m2v2im1+m2v_f = rac{m_1 v_{1_i} + m_2 v_{2_i}}{m_1 + m_2}

    • Examples of Applications:

    • Rocket propulsion: Conservation of momentum in exhaust gas and rocket.

    • Recoil of a gun: Bullet and gun momenta equal and opposite.

    • Billiard balls: Elastic collisions approximate momentum conservation.


Applications in Systems with External Forces

  • Approximate Conservation:

    • If external forces are present but impulsive (short duration), momentum is approximately conserved (e.g., explosions).


Conclusion

  • Thank you for your attention!