2. Sect. 1.2: Mechanics of a System of Particles Generalization to many (N) particle system: –Distinguish External & Internal Forces. –Newton’s 2 nd Law (eqtn. of motion), particle i: ∑ j F ji + F i (e) = (dp i /dt) = p i F i (e)  Total external force on the i th particle. F ji  Total (internal) force on the i th particle due to the j th particle. Fjj = 0 of course!!

3. ∑ j F ji + F i (e) = (dp i /dt) = p i (1) Assumption: Internal forces F ji obey Newton’s 3 rd Law: F ji = - F ij  The “Weak” Law of Action and Reaction –Original form of the 3 rd Law, but is not satisfied by all forces! Sum (1) over all particles in the system: ∑ i,j(  i) F ji + ∑ i F i (e) = ∑ i (dp i /dt) = d(∑ i m i v i )/dt = d 2 (∑ i m i r i )/dt 2

4. Newton’s 2 nd Law for Many Particle Systems Rewrite as: d 2 (∑ i m i r i )/dt 2 = ∑ i F i (e) + ∑ i,j(  i) F ji (2) ∑ i F i (e)  total external force on system  F (e) ∑ i,j(  i) F ji  0. By Newton’s 3 rd Law: F ji = - F ij  F ji + F ij = 0 (cancel pairwise!) So, (2) becomes (r i  position vector of m i ): d 2 (∑ i m i r i )/dt 2 = F (e) (3)  Only external forces enter Newton’s 2nd Law to get the equation of motion of a many particle system!!

5. d 2 ( ∑ i m i r i )/dt 2 = F (e) (3) Modify (3) by defining R  mass weighted average of position vectors r i. R  (∑ i m i r i )/(∑ i m i )  (∑ i m i r i )/M M  ∑ i m i (total mass of particles in system) R  Center of mass of the system (schematic in Figure)  (3) becomes: M(d 2 R/dt 2 ) = MA = M(dV/dt) = (dP/dt) = F (e) (4) Just like the eqtn of motion for mass M at position R under the force F (e) !

6. M(d 2 R/dt 2 ) = F (e) (4)  Newton’s 2 nd Law for a many particle system: The Center of Mass moves as if the total external force were acting on the entire mass of the system concentrated at the Center of Mass! –Corollary: Purely internal forces (assuming they obey Newton’s 3 rd Law) have no effect on the motion of the Center of Mass (CM). Examples: 1. Exploding shell: Fragments travel AS IF the shell were still in one piece. 2. Jet & Rocket propulsion: Exhaust gases at high v are balanced by the forward motion of the vehicle.

7. Momentum Conservation MR = (∑ i m i r i ). Consider: Time derivative (const M): M(dR/dt) = MV= ∑ i m i [(dr i )/dt]  ∑ i m i v i  ∑ i p i  P (total momentum = momentum of CM)  Using the definition of P, Newton’s 2 nd Law is: (dP/dt) = F (e) (4´) Suppose F (e) = 0:  (dP/dt) = P = 0  P = constant (conserved) Conservation Theorem for the Linear Momentum of a System of Particles: If the total external force, F (e), is zero, the total linear momentum, P, is conserved.

8. Angular Momentum Angular momentum L of a many particle system (sum of angular momenta of each particle): L  ∑ i [r i  p i ] Time derivative: L = (dL/dt) = ∑ i d[r i  p i ]/dt = ∑ i [(dr i /dt)  p i ] + ∑ i [r i  (dp i /dt)] (dr i /dt)  p i = v i  (m i v i ) = 0  (dL/dt) = ∑ i [r i  (dp i /dt)] –Newton’s 2 nd Law: (dp i /dt) = F i (e) + ∑ j(  i) F ji F i (e)  Total external force on the i th particle ∑ j(  i) F ji  Total internal force on the i th particle due to interactions with all other particles (j) in the system  (dL/dt) = ∑ i [r i  F i (e) ] + ∑ i,j(  i) [r i  F ji ]

9. (dL/dt) = ∑ i [r i  F i (e) ] + ∑ i,j(  i) [r i  F ji ] (1) Consider the 2nd sum & look at each particle pair (i,j). Each term r i  F ji has a corresponding term r j  F ij. Take together & use Newton’s 3rd Law:  [r i  F ji + r j  F ij ] = [r i  F ji + r j  (-F ji )] = [(r i - r j )  F ji ] (r i - r j )  r ij = vector from particle j to particle i. (Figure)

10. (dL/dt) = ∑ i [r i  F i (e) ] + (½)∑ i,j(  i) [r ij  F ji ] (1) Assumption: Internal forces are Central Forces: Directed the along lines joining the particle pairs (  The “Strong” Law of Action and Reaction)  r ij || F ji for each (i,j) & [r ij  F ji ] = 0 for each (i,j)!  2 nd term in (1) is (½)∑ i,j(  i) [r ij  F ji ] = 0  To Prevent Double Counting!

11.  (dL/dt) = ∑ i [r i  F i (e) ] (2) Total external torque on particle i: N i (e)  r i  F i (e) (2) becomes: (dL/dt) = N (e) (2´) N (e)  ∑ i [r i  F i (e) ] = ∑ i N i (e) = Total external torque on the system

12. (dL/dt) = N (e) (2´)  Newton’s 2 nd Law (rotational motion) for a many particle system: The time derivative of the total angular momentum is equal to the total external torque. Suppose N (e) = 0:  (dL/dt) = L = 0  L = constant (conserved) Conservation Theorem for the Total Angular Momentum of a Many Particle System: If the total external torque, N (e), is zero, then (dL/dt) = 0 and the total angular momentum, L, is conserved.

13. (dL/dt) = N (e). A vector equation! Holds component by component.  Angular momentum conservation holds component by component. For example, if N z (e) = 0, L z is conserved. Linear & Angular Momentum Conservation Laws: –Conservation of Linear Momentum holds if internal forces obey the “Weak” Law of Action and Reaction: Only Newton’s 3 rd Law F ji = - F ij is required to hold! –Conservation of Angular Momentum holds if internal forces obey the “Strong” Law of Action and Reaction: Newton’s 3 rd Law F ji = - F ij holds, PLUS the forces must be Central Forces, so that r ij || F ji for each (i,j)! Valid for many common forces (gravity, electrostatic). Not valid for some (magnetic forces, etc.). See text discussion.

14. Center of Mass & Relative Coordinates More on angular momentum. Search for an analogous relation to what we had for linear momentum: P = M(dR/dt) = MV Want: Total momentum = Momentum of CM = Same as if entire mass of system were at CM. Start with total the angular momentum: L  ∑ i [r i  p i ] R  CM coordinate (origin O). For particle i define: r i ´  r i - R = relative coordinate vector from CM to particle i (Figure)

15. r i = r i ´ + R Time derivative: (dr i /dt) = (dr i ´/dt) + (dR/dt) or: v i = v i ´ + V, V  CM velocity relative to O v i ´  velocity of particle i relative to CM. Also: p i  m i v i  momentum of particle i relative to O Put this into angular momentum: L = ∑ i [r i  p i ] = ∑ i [(r i ´ + R)  m i (v i ´ +V)] Manipulation: (using m i v i ´= d(m i r i ´)/dt ) L = R  ∑ i (m i )V + ∑ i [r i ´  (m i v i ´)] + ∑ i (m i r i ´)  V + R  d[∑ i (m i r i ´)]/dt Note: ∑ i (m i r i ´) defines the CM coordinate with respect to the CM & is thus zero!! ∑ i (m i r i ´)  0 !  The last 2 terms are zero!

16.  L = R  ∑ i (m i )V + ∑ i [r i ´  (m i v i ´)] (1) Note that ∑ i (m i )  M = total mass & also m i v i ´  p i ´ = momentum of particle i relative to the CM  L = R  (MV)+ ∑ i [r i ´  p i ´] = R  P + ∑ i [r i ´  p i ´] (2) The total angular momentum about point O = the angular momentum of the motion of the CM + the angular momentum of motion about the CM (2)  In general, L depends on the origin O, through the vector R. Only if the CM is at rest with respect to O, will the first term in (2) vanish. Then & only then will L be independent of the point of reference. Then & only then will L = angular momentum about the CM

17. Work & Energy The work done by all forces in changing the system from configuration 1 to configuration 2: W 12  ∑ i ∫F i  ds i (limits: from 1 to 2) (1) As before: F i = F i (e) + ∑ j F ji  W 12 = ∑ i ∫F i (e)  ds i + ∑ i,j(  i) ∫ F ji  ds i (2) Work with (1) first: –Newton’s 2 nd Law  F i = m i (dv i /dt). Also: ds i = v i dt F i  ds i = m i (dv i /dt)  ds i = m i (dv i /dt)  v i dt = m i v i dv i = d[(½)m i (v i ) 2 ]  W 12 = ∑ i ∫ d[(½)m i (v i ) 2 ]  T 2 - T 1 where T  (½)∑ i m i (v i ) 2 = Total System Kinetic Energy

18. Work-Energy Principle W 12 = T 2 - T 1 =  T The total Work done = The change in kinetic energy (Work-Energy Principle or Work-Energy Theorem) Total Kinetic Energy: T  (½)∑ i m i (v i ) 2 –Another useful form: Use transformation to CM & relative coordinates: v i = V + v i ´, V  CM velocity relative to O, v i ´  velocity of particle i relative to CM.  T  (½)∑ i m i (V+ v i ´)  (V + v i ´) T = (½)(∑ i m i )V 2 + (½)∑ i m i (v i ´) 2 + V  ∑ i m i v i ´ Last term: V  d(∑ i m i r i ´)/dt. From the angular momentum discussion: ∑ i m i r i ´ = 0  The last term is zero!  Total KE: T = (½)MV 2 + (½)∑ i m i (v i ´) 2

19. Total KE T = (½)MV 2 + (½)∑ i m i (v i ´) 2 The total Kinetic Energy of a many particle system is equal to the Kinetic Energy of the CM plus the Kinetic Energy of motion about the CM.

20. Work & PE 2 forms for work: W 12 = ∑ i ∫F i  ds i = T 2 - T 1 =  T (just showed!) (1) W 12 = ∑ i ∫F i (e)  ds i + ∑ i,j(  i) ∫F ji  ds i (2) Use (2) with Conservative Force Assumptions: 1. External Forces:  Potential functions V i (r i ) exist such that (for each particle i): F i (e) = - ∇ i V i (r i ) 2. Internal Forces:  Potential functions V ij exist such that (for each particle pair i,j): F ij = - ∇ i V ij 2´. Strong Law of Action-Reaction:  Potential functions V ij (r ij ) are functions only of distance r ij = |r i - r j | between i & j & the forces lie along line joining them (Central Forces!): V ij = V ij (r ij )  F ij = - ∇ i V ij = + ∇ j V ij = -F ji = (r i - r j )f(r ij ) f is a scalar  function!

21. Conservative external forces:  ∑ i ∫F i (e)  ds i = - ∑ i ∫ ∇ i V i  ds i = - ∑ i (V i ) 2 + ∑ i (V i ) 1 Or: ∑ i ∫ F i (e)  ds i = (V (e) ) 1 - (V (e) ) 2 Where: V (e)  ∑ i V i = total PE associated with external forces. Conservative internal forces: Write (sum over pairs)  ∑ i,j(  i) ∫F ji  ds i = (½)∑ i,j(  i) ∫[F ji  ds i + F ij  ds j ] = - (½)∑ i,j(  i) ∫[ ∇ i V ij  ds i + ∇ j V ij  ds j ] Note: ∇ i V ij = - ∇ j V ij = ∇ ij V ij ( ∇ ij  grad with respect to r ij ) Also: ds i - ds j = dr ij  ∑ i,j(  i) ∫F ji  ds i = - (½) ∑ i,j(  i) ∫ ∇ ij V ij  dr ij = - (½) ∑ i,j(  i) (V ij ) 2 + (½) ∑ i,j(  i) (V ij ) 1 do integral!!

22. Conservative internal (Central!) forces: ∑ i,j(  i) ∫F ji  ds i = - (½)∑ i,j(  i) (V ij ) 2 + (½)∑ i,j(  i) (V ij ) 1 or: ∑ i,j(  i) ∫F ji  ds i = (V (I) ) 1 - (V (I) ) 2 Where: V (I)  (½)∑ i,j(  i) V ij = Total PE associated with internal forces. For conservative external forces & conservative, central internal forces, it is possible to define a potential energy function for the system: V  V (e) + V (I)  ∑ i V i + (½)∑ i,j(  i) V ij

23. Conservation of Mechanical Energy For conservative external forces & conservative, central internal forces: –The total work done in a process is: W 12 = V 1 - V 2 = -  V with V  V (e) + V (I)  ∑ i V i + (½)∑ i,j(  i) V ij –In general W 12 = T 2 - T 1 =  T Combining  V 1 - V 2 = T 2 - T 1 or  T +  V = 0 orT 1 + V 1 = T 2 + V 2 or E = T + V = constant E = T + V  Total Mechanical Energy (or just Total Energy)

24. Energy Conservation  T +  V = 0 orT 1 + V 1 = T 2 + V 2 or E = T + V = constant (conserved) Energy Conservation Theorem for a Many Particle System: If only conservative external forces & conservative, central internal forces are acting on a system, then the total mechanical energy of the system, E = T + V, is conserved.

25. Consider the potential energy: V  V (e) + V (I)  ∑ i V i + (½)∑ i,j(  i) V ij 2nd term V (I)  (½)∑ i,j(  i) V ij  Internal Potential Energy of the System. This is generally non-zero & might vary with time. –Special Case: Rigid Body: System of particles in which distances r ij are fixed (do not vary with time). (Chapters 4 & 5!)  dr ij are all  r ij & thus to internal forces F ij  F ij do no work.  V (I) = constant Since V is arbitrary to within an additive constant, we can ignore V (I) for rigid bodies only.