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picture1_Dynamics Of Rigid Bodies Lecture Notes Pdf 158170 | Chap11


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File: Dynamics Of Rigid Bodies Lecture Notes Pdf 158170 | Chap11
lecture notes for phy 405 classical mechanics from thorton marion s classical mechanics prepared by dr joseph m hahn saint mary s university department of astronomy physics november 21 2004 ...

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                  Lecture Notes for PHY 405
                      Classical Mechanics
               From Thorton & Marion’s Classical Mechanics
                              Prepared by
                           Dr. Joseph M. Hahn
                          Saint Mary’s University
                       Department of Astronomy & Physics
                            November 21, 2004
                         Problem Set #6
                     due Thursday December 1
                        at the start of class
                 late homework will not be accepted
    text problems 10–8, 10–18, 11–2, 11–7, 11-13, 11–20, 11–31
                            Final Exam
                       Tuesday December 6
                       10am-1pm in MM310
                      (note the room change!)
               Chapter 11: Dynamics of Rigid Bodies
    rigid body = a collection of particles whose relative positions are fixed.
    Wewill ignore the microscopic thermal vibrations occurring among a ‘rigid’
    body’s atoms.
                                 1
                                    The inertia tensor
      Consider a rigid body that is composed of N particles.
      Give each particle an index α = 1...N.
      The total mass is M = Pαmα.
      This body can be translating as well as rotating.
      Place your moving/rotating origin on the body’s CoM:
                                         Fig. 10-1.
                                               1 X        ′
                      the CoM is at    R = M         mαrα
                                                   α
                              where r′    = R+r =α’sposition wrt’ fixed origin
                                        α           α
      note that this implies   Xmr = 0
                                     α α
                                α
      Particle α has velocity vf,α = dr′α/dt relative to the fixed origin,
      and velocity vr,α = drα/dt in the reference frame that rotates about axis ω~.
      Then according to Eq. 10.17 (or page 6 of Chap. 10 notes):
         vf,α = V+vr,α+ω~ ×rα = α’s velocity measured wrt’ fixed origin
      and V = dR/dt = velocity of the moving origin relative to the fixed origin.
      What is vr,α for the the particles that make up this rigid body?
                                             2
        Thus vα = V+ω~ ×rα after dropping the f subscript
         and T = 1m v2 = 1m (V+ω~ ×r )2 is the particle’s KE
                α    2  α α    2  α          α
                      N
            so T = XTα thesystem’stotal KE is
                     α=1
                  = 1MV2+XmαV·(ω~ ×rα)+1Xmα(ω~ ×rα)2
                     2         α                  2 α
                     1     2           X ! 1X                       2
                  = 2MV +V· ω~ ×           mαrα +2       mα(ω~ ×rα)
                                        α              α
     where M = Pαmα = the system’s total mass.
     Recall that P m r = 0, so
                  α  α α
             thus T = Ttrans +Trot
        where T      = 1MV2=KEduetosystem’stranslation
                trans   2
           and Trot = 1Xmα(ω~ ×rα)2 = KE due to system’s rotation
                        2 α
     Now focus on Trot,
     and note that (A ×B)2 = A2B2 −(A·B)2 ← see text page 28 for proof.
     Thus
                       Trot = 1Xmα[ω2r2 −(ω~ ·rα)2]
                              2           α
                                 α
                                      3
         In Cartesian coordinates,
                                                      ω~   = ωxxˆ+ωyyˆ+ωzˆz
                                                                                              3
                                             so     ω2 = ω2+ω2+ω2≡Xω2
                                                                   x        y        z               i
                                                                                             i=1
                                                                   3
                                           and rα = Xxα,ixˆi
                                                                 i=1
                                                                   3
                                        so     ω~ · rα = Xωixα,i
                                                                 i=1
         Thus
                                         3             !  3                !   3                       ! 3                    
                       1 X                   X 2               X 2                     X                       X
         Trot = 2 α mα i=1 ωi                                 k=1 xα,k         − i=1 ωixα,i                j=1 ωjxα,j
         Wecan also write
                                                                                       3
                                                                          ωi = Xωjδi,j
                                                                                      j=1
                                                           where δi,j =  1 i = j
                                                                                         0     i 6= j
                                                                                            3                   3
                                                                  so     ω2 = ωiXωjδi,j = Xωiωjδi,j
                                                                            i
                                                                                          j=1                  j=1
                                                         !                !
              and also note that                Xai              Xbi = XXaibi≡Xaibi
                                                  i                i                   i      j                i,j
                                                                       4
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...Lecture notes for phy classical mechanics from thorton marion s prepared by dr joseph m hahn saint mary university department of astronomy physics november problem set due thursday december at the start class late homework will not be accepted text problems final exam tuesday am pm in mm note room change chapter dynamics rigid bodies body a collection particles whose relative positions are xed wewill ignore microscopic thermal vibrations occurring among atoms inertia tensor consider that is composed n give each particle an index total mass p this can translating as well rotating place your moving origin on com fig x r where sposition wrt implies xmr has velocity vf dt to and vr reference frame rotates about axis then according eq or page chap v measured what make up thus after dropping f subscript t ke so xt thesystem stotal mv xm system recall ttrans trot keduetosystem stranslation trans rotation now focus b ab see proof cartesian coordinates xx yy z y i ix k j jx wecan also write xai...

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