Rotations and Angular Momentum

Total Page:16

File Type:pdf, Size:1020Kb

Rotations and Angular Momentum rotations.nb:11/3/04::13:48:13 1 RotationsandAngularmomentum Á Intro Thematerialheremaybefoundin SakuraiChap3:1-3,(5-6),7,(9-10) MerzbacherChap11,17. Chapter11ofMerzbacherconcentratesonorbitalangularmomentum.Sakurai,andCh17ofMerzbacherfocuson angularmomentuminrelationtothegroupofrotations.Justaslinearmomentumisrelatedtothetranslationgroup, angularmomentumoperatorsaregeneratorsofrotations.Thegoalistopresentthebasicsin5lecturesfocusingon 1.J asthegeneratorofrotations. 2.RepresentationsofSO 3 3.Additionofangularmomentum+ / 4.OrbitalangularmomentumandYlm ' s 5.Tensoroperators. Á Rotations&SO(3) ü Rotationsofvectors Beginwithadiscussionofrotationsappliedtoa3-dimensionalrealvectorspace.Thevectorsaredescribedbythreereal vx numbers,e.g.v = v .ThetransposeofavectorisvT = v , v , v .Thereisaninnerproductdefinedbetweentwo ML y ]\ x y z M ] M vz ] + / T M T ] vectorsbyu ÿ v =Nv ÿ^u = uv cos f,wherefistheanglebetweenthetwovectors.Underarotationtheinnerproduct betweenanytwovectorsispreserved,i.e.thelengthofanyvectorandtheanglebetweenanytwovectorsdoesn't change.Arotationcanbedescribedbya3ä3realorthogonalmatrixRwhichoperatesonavectorbytheusualrulesof matrixmultiplication v'x vx v' = R v and v' , v' , v' = v , v , v RT ML y ]\ ML y ]\ x y z x y z M ] M ] M v'z ] M vz ] + / + / M ]]] M ]]] N ^ N ^ Topreservetheinnerproduct,itisrequirdthatRT ÿ R = 1 u'ÿ v' = uRT ÿ Rv = u1v = u ÿ v Asanexample,arotationbyfaroundthez-axis(orinthexy-plane)isgivenby rotations.nb:11/3/04::13:48:13 2 cos f -sin f 0 R f = sin f cos f 0 z ML ]\ M ] + / M 0 0 1 ] M ]]] N ^ Thesignconventionsareappropriateforarighthandedcoordinatesystem:putthethumbofrighthandalongz-axis, extendfingersalongx-axis,andcurlfingersindirectionofy-axis. z y x Thedirectionofrotationforfiscounter-clockwisewhenlookingdownfromthe+zdirection,i.e.rotatethex-axisinto they-axis.Similarlytherotationsaroundthexandyaxesare cos f 0 sin f 1 0 0 R f = 0 1 0 andR f = 0 cos f -sin f y ML ]\ x ML ]\ M ] M ] + / M -sin f 0 cos f ] + / M 0 sin f cos f ] M ]]] M ]]] N ^ N ^ Thesignofsin finRy isrelatedtothehanded-nessofthecoordinatesystemandthesenseofrotation.For 3-dimensions,itisequivalenttotalkaboutrotationsaroundthez-axis,orrotationsinthexy-plane.Inanyothernumber ofdimensions,thecorrectlanguageistotalkaboutrotationsinthexi x j -plane,wherexi definesoneofthecoordinate directionsofthevectorspace.Thus,whilefor3-dimensionsthereare3independentrotations,inN -dimensions,there willbe ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅN N-1 independentrotations. + 2 / ü Directionkets Tomakethecorrespondencetoquantumstates,justasatranslationwasdefinedbyitsactiononpositioneigenkets,a rotationaroundtheoriginalsocanactonpositioneigenketsby è x ' = R x = R x ? ? ? è whereadistinctionhasbeenmadebetweentheoperatorR,whichactsonthestate,andtherotationmatrixRwhichacts onthecoordinates.Sincetherotationsdon'tchangethelengthofthevector,itispossibletodefinespherical coordinates,r, q, f,andsphericalpositionkets, x Ø r ≈ n` ,whererdeterminestheradialposition,andn` indicates ` thedirectionfromtheorigin.Therotationsactonlyonthe ? ? n ?degreesoffreedom. è ? R r ≈ n` = r ≈ R ÿ n` + ? ?/ ? ? Directionketswillbeusedmoreextensivelyinthediscussionoforbitalangularmomentumandsphericalharmonics, butfornowtheyareusefulforillustratingthesetofrotations.Thesetofalldirectionkets n` canbevisualizedbythe surfaceofasphere,andtherotationsarethesetofallpossiblewaystoreorientthatsphere. ? rotations.nb:11/3/04::13:48:13 3 ü OrthognalgroupSO(3) Thesetofallpossiblerotationsformagroup.Considerthefourproperties:closure,identity,inverseandassociativity. Usingthepictureofrotationsasreorientationsofasphere,onecanconstructvisualizationstoillustrateeachproperty. Withgreatermathematicalrigor,thesetofallpossiblerotationsformthegroupSO(3),whereOØorthogonal,3Ø3 dimensions,andSØspecial,whichinthiscasemeansthematrixhasadeterminantof1.Therotationsaredescribedby threecontinuous,butbounded,parameters.Fromthematrixpointofview,a3ä3matrixhasninedegreesoffreedom. T Theconstraintthatthematrixisorthogonal,Ri j R j k = di k yields6conditions,i.e.threefori = k andthreefori ∫ k . Thepropertiesofagroupareobeyed: closure: ForanytwoorthogonalmatricesR1 andR2 ,theproductR3 = R1 R2 ,isalsoorthogonal.Thecombination oftworotationsisalsoarotation. identity: The3 ä3unitmatrixactsasanidentityelementforthegroup. 1 R = R 1 = R inverse: EachelementhasaninverseR-1 = RT ,RT R = RRT = 1 associativity: R1 R2 R3 = R1 R2 R3 + / + / UnliketheTranslationgroup,SO(3)isnotabelian,i.e.ingeneralR1 R2 ∫ R2 R1 . ThesignificanceoftheS-condition,Det R = 1,isthatreflectionsarenotincludedinthegroup,i.e.forthreedimensions onecannotturnaright-handedobjectintoaleft-handedobjectbydoingarotation.Ifweallowedreflections,e.g. -1 0 0 0 -1 0 ML ]\ M ] M 0 0 -1 ] M ] N ^ Then,thegroupwouldbeO(3)insteadofSO(3).O(3)iscalled"disconnected"sincenotallelementsofthegroupcan bereachedbyasuccessionofinfinitesimaltransformations.SO(3)isconnected. TherotationmatricesRarejustone"representation"ofthegroupSO(3).Fortwodifferentrepresentations,therehasto bea1 ¨1mappingoftheelementsofonerepresentationtotheother.Themappinghastopreservethecombinationlaw. ConsidertworepresentationsRandS .Labelarotationbyasubscriptwhichrepresentsthethreeparameterstodefinea rotation,andidentifyRa ¨ Sa ,IfR3 = R1 R2 ,thenwemusthaveS3 = S1 S2 topreservethecombinatinlaw. ` ü Fullsetofrotations:+n, f/ Therearetwocommonmethodsforparameterizingrotations.Thefirstistochooseanaxisforrotationandthenperform arotationbyananglebetween0andp.Theaxisofrotationcanbechosenanywhereonthesphere.Whynot0 ¨ 2 p? Thenrotationswithpolesonoppositesidesofthespherewouldberedundant.AnexplicitformforR n`, f willbegiven afterdevelopingthelanguageofinfinitesimalrotations. + / Draw your own picture showing the rotation of a sphere around an off + axis pole. The sphere represents the set of states, n, i.e. the set of direction kets. The rotation reorients the sphere. rotations.nb:11/3/04::13:48:13 4 ü Eulerangles ThesecondparameterizationistogiveEulerangles.Inthismethodonedescribeswherethe"northpole"movesto underarotation,andtheorientationofthesphereafterthepolehasbeenmoved.Thelocationofthepoleisdetermined byfirstchoosingalongitudebyrotatingaroundthez-axis,thenalatitudebyrotatingaroundthenewy-axis.Finally, theorientationofthesphereisgivenbyafinalrotationaroundthenewz-axis.Pictorially, Draw more pictures, showing the sequence of rotations to move the pole, and then reorient the sphere around the new pole. IntheEulerparameterizationtherangeofanglesis a = 0, 2 p , b = 0, p , g = 0, 2 p + / + / + / andanarbitraryrotationisgivenby R a, b, g = Rz' g Ry' b Rz a + / + / + / + / Note thatthez'andy'rotationsarenotdefinedwithrespecttotheoriginalcoordinateaxes,butratherwithrespectto wherethoseaxeshavemovedwiththereorientationofthesphere.Lateritwillbeshownthat Rz' g Ry' b Rz a = Rz a Ry b Rz g + / + / + / + / + / + / wheretheorderhasbeenreversed,butnowallrotationsareconvenientlydefinedaroundtheaxesoftheoriginal coordinatesystem. ü Equivalencyofthetwoparameterizations Thetwoparameterizationsmaynotseemequivalent,buttheyare,ascanbeseenbyapictorialmappingof n`, f to a, b, g .ObservethattherearetwowaystoproducethesamesetofEuleranglesconsistentwiththerestrictionof+ / fto +0, p . / + / This picture didn't make it into the classroom presentation. it's a bit of work Thetwotechniqueshavedifferentuses.Euleranglestendtobemoreusefulforbuildingupactualrotationmatricesina calculation.ThisisbecauseRz andRy aregenerallyfairlyeasytoconstructforarepresentation,andthematrix multiplicationisstraightforward.The n`, f notationhasadvantagesinsomeanalyticmanipulations,aswewillsee below. + / rotations.nb:11/3/04::13:48:13 5 ü J asthegeneratorofinfinitesimalrotations. Inanalogytothediscussionoftranslationsandtimeevolution,itisusefultobuildupthefiniterotationsfrom generatorsofinfinitesimalrotations.Recognizingthatweareeventuallyinterestedinaquantummechanical formulation,itisusefultodevelopthisformalisminawaythatrealizestherotationsasunitaryoperations.Forexample, aninfinitesimalrotationaroundthez-axisisgivenby Rz d = 1 - i d Jz + / whereJz isthegeneratorofinfinitesimalrotationsaroundthez-axis.SinceRisunitary(note:orthogonalmatricesare unitary),J mustbeHermitian.Inthepresentcase,toleadingorderind 1 -d 0 0 -i 0 R d = d 1 0 orJ = i 0 0 z ML ]\ z ML ]\ M ] M ] + / M 0 0 1 ] M 0 0 0 ] M ]]] M ]]] N ^ N ^ Similarly,forthisrepresentation 0 0 0 0 0 i J = 0 0 -i ,J = 0 0 0 x ML ]\ y ML ]\ M ] M ] M 0 i 0 ] M -i 0 0 ] M ]]] M ]]] N ^ N ^ Note thatsincethisisstillaclassicaldiscussionIhaven'tputinanyfactorsof. ü Commutationrelations Thegeneratorsobeythecommutationrelations Ji, J j = i ei jk Jk # ' whereei jk = 1, if i j k is an even permutation of x y z = -1, if +i j k/is an odd permutation of x+ y z / = 0, if any+ two/ of i j k are equal + / + / asausefulasideei jk elmk = dil d jm - dim d jl . Thecommutationrelationsareapropertyofthegroup,notjustaparticularrepresentation.Thecollectionofallthe commutatorrelationsforthegeneratorsissometimescalledthealgebraofthegeneratorsofthegroup,orjustthe algebraofthegroup. ü Finiterotations Forrotationsaroundaparticularaxis,itshouldbeclearthatwecanbuildupanarbitraryrotationbyasequenceof infinitesimalrotations,similartotheprocedureforbuildingupafintetranslationasthelimitingproductofalarge numberofinfinitesimals. rotations.nb:11/3/04::13:48:13 6 R f = Lim P Rz f n nض i + / - + s /1 n = Lim 1 - i Jz f n nض = e-i Jz f+ + s // Itisnowpossibletogiveaformforanarbitraryrotationinthe n`, f parameterization.Theinfinitesimalrotation ` aroundthen-axisisgivenby + / R n`, d = 1 - i d n` ÿ J + / ThereisnoconcernaboutwhichcomponentofJ isoperatedonfirst,sincetheeffectsofcommutationamongstthe
Recommended publications
  • Understanding Euler Angles 1
    Welcome Guest View Cart (0 items) Login Home Products Support News About Us Understanding Euler Angles 1. Introduction Attitude and Heading Sensors from CH Robotics can provide orientation information using both Euler Angles and Quaternions. Compared to quaternions, Euler Angles are simple and intuitive and they lend themselves well to simple analysis and control. On the other hand, Euler Angles are limited by a phenomenon called "Gimbal Lock," which we will investigate in more detail later. In applications where the sensor will never operate near pitch angles of +/‐ 90 degrees, Euler Angles are a good choice. Sensors from CH Robotics that can provide Euler Angle outputs include the GP9 GPS‐Aided AHRS, and the UM7 Orientation Sensor. Figure 1 ‐ The Inertial Frame Euler angles provide a way to represent the 3D orientation of an object using a combination of three rotations about different axes. For convenience, we use multiple coordinate frames to describe the orientation of the sensor, including the "inertial frame," the "vehicle‐1 frame," the "vehicle‐2 frame," and the "body frame." The inertial frame axes are Earth‐fixed, and the body frame axes are aligned with the sensor. The vehicle‐1 and vehicle‐2 are intermediary frames used for convenience when illustrating the sequence of operations that take us from the inertial frame to the body frame of the sensor. It may seem unnecessarily complicated to use four different coordinate frames to describe the orientation of the sensor, but the motivation for doing so will become clear as we proceed. For clarity, this application note assumes that the sensor is mounted to an aircraft.
    [Show full text]
  • Rotation and Spin and Position Operators in Relativistic Gravity and Quantum Electrodynamics
    Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 4 December 2019 doi:10.20944/preprints201912.0044.v1 Peer-reviewed version available at Universe 2020, 6, 24; doi:10.3390/universe6020024 1 Review 2 Rotation and Spin and Position Operators in 3 Relativistic Gravity and Quantum Electrodynamics 4 R.F. O’Connell 5 Department of Physics and Astronomy, Louisiana State University; Baton Rouge, LA 70803-4001, USA 6 Correspondence: [email protected]; 225-578-6848 7 Abstract: First, we examine how spin is treated in special relativity and the necessity of introducing 8 spin supplementary conditions (SSC) and how they are related to the choice of a center-of-mass of a 9 spinning particle. Next, we discuss quantum electrodynamics and the Foldy-Wouthuysen 10 transformation which we note is a position operator identical to the Pryce-Newton-Wigner position 11 operator. The classical version of the operators are shown to be essential for the treatment of 12 classical relativistic particles in general relativity, of special interest being the case of binary 13 systems (black holes/neutron stars) which emit gravitational radiation. 14 Keywords: rotation; spin; position operators 15 16 I.Introduction 17 Rotation effects in relativistic systems involve many new concepts not needed in 18 non-relativistic classical physics. Some of these are quantum mechanical (where the emphasis is on 19 “spin”). Thus, our emphasis will be on quantum electrodynamics (QED) and both special and 20 general relativity. Also, as in [1] , we often use “spin” in the generic sense of meaning “internal” spin 21 in the case of an elementary particle and “rotation” in the case of an elementary particle.
    [Show full text]
  • The Rolling Ball Problem on the Sphere
    S˜ao Paulo Journal of Mathematical Sciences 6, 2 (2012), 145–154 The rolling ball problem on the sphere Laura M. O. Biscolla Universidade Paulista Rua Dr. Bacelar, 1212, CEP 04026–002 S˜aoPaulo, Brasil Universidade S˜aoJudas Tadeu Rua Taquari, 546, CEP 03166–000, S˜aoPaulo, Brasil E-mail address: [email protected] Jaume Llibre Departament de Matem`atiques, Universitat Aut`onomade Barcelona 08193 Bellaterra, Barcelona, Catalonia, Spain E-mail address: [email protected] Waldyr M. Oliva CAMGSD, LARSYS, Instituto Superior T´ecnico, UTL Av. Rovisco Pais, 1049–0011, Lisbon, Portugal Departamento de Matem´atica Aplicada Instituto de Matem´atica e Estat´ıstica, USP Rua do Mat˜ao,1010–CEP 05508–900, S˜aoPaulo, Brasil E-mail address: [email protected] Dedicated to Lu´ıs Magalh˜aes and Carlos Rocha on the occasion of their 60th birthdays Abstract. By a sequence of rolling motions without slipping or twist- ing along arcs of great circles outside the surface of a sphere of radius R, a spherical ball of unit radius has to be transferred from an initial state to an arbitrary final state taking into account the orientation of the ball. Assuming R > 1 we provide a new and shorter prove of the result of Frenkel and Garcia in [4] that with at most 4 moves we can go from a given initial state to an arbitrary final state. Important cases such as the so called elimination of the spin discrepancy are done with 3 moves only. 1991 Mathematics Subject Classification. Primary 58E25, 93B27. Key words: Control theory, rolling ball problem.
    [Show full text]
  • Vectors, Matrices and Coordinate Transformations
    S. Widnall 16.07 Dynamics Fall 2009 Lecture notes based on J. Peraire Version 2.0 Lecture L3 - Vectors, Matrices and Coordinate Transformations By using vectors and defining appropriate operations between them, physical laws can often be written in a simple form. Since we will making extensive use of vectors in Dynamics, we will summarize some of their important properties. Vectors For our purposes we will think of a vector as a mathematical representation of a physical entity which has both magnitude and direction in a 3D space. Examples of physical vectors are forces, moments, and velocities. Geometrically, a vector can be represented as arrows. The length of the arrow represents its magnitude. Unless indicated otherwise, we shall assume that parallel translation does not change a vector, and we shall call the vectors satisfying this property, free vectors. Thus, two vectors are equal if and only if they are parallel, point in the same direction, and have equal length. Vectors are usually typed in boldface and scalar quantities appear in lightface italic type, e.g. the vector quantity A has magnitude, or modulus, A = |A|. In handwritten text, vectors are often expressed using the −→ arrow, or underbar notation, e.g. A , A. Vector Algebra Here, we introduce a few useful operations which are defined for free vectors. Multiplication by a scalar If we multiply a vector A by a scalar α, the result is a vector B = αA, which has magnitude B = |α|A. The vector B, is parallel to A and points in the same direction if α > 0.
    [Show full text]
  • Chapter 5 ANGULAR MOMENTUM and ROTATIONS
    Chapter 5 ANGULAR MOMENTUM AND ROTATIONS In classical mechanics the total angular momentum L~ of an isolated system about any …xed point is conserved. The existence of a conserved vector L~ associated with such a system is itself a consequence of the fact that the associated Hamiltonian (or Lagrangian) is invariant under rotations, i.e., if the coordinates and momenta of the entire system are rotated “rigidly” about some point, the energy of the system is unchanged and, more importantly, is the same function of the dynamical variables as it was before the rotation. Such a circumstance would not apply, e.g., to a system lying in an externally imposed gravitational …eld pointing in some speci…c direction. Thus, the invariance of an isolated system under rotations ultimately arises from the fact that, in the absence of external …elds of this sort, space is isotropic; it behaves the same way in all directions. Not surprisingly, therefore, in quantum mechanics the individual Cartesian com- ponents Li of the total angular momentum operator L~ of an isolated system are also constants of the motion. The di¤erent components of L~ are not, however, compatible quantum observables. Indeed, as we will see the operators representing the components of angular momentum along di¤erent directions do not generally commute with one an- other. Thus, the vector operator L~ is not, strictly speaking, an observable, since it does not have a complete basis of eigenstates (which would have to be simultaneous eigenstates of all of its non-commuting components). This lack of commutivity often seems, at …rst encounter, as somewhat of a nuisance but, in fact, it intimately re‡ects the underlying structure of the three dimensional space in which we are immersed, and has its source in the fact that rotations in three dimensions about di¤erent axes do not commute with one another.
    [Show full text]
  • Euler Quaternions
    Four different ways to represent rotation my head is spinning... The space of rotations SO( 3) = {R ∈ R3×3 | RRT = I,det(R) = +1} Special orthogonal group(3): Why det( R ) = ± 1 ? − = − Rotations preserve distance: Rp1 Rp2 p1 p2 Rotations preserve orientation: ( ) × ( ) = ( × ) Rp1 Rp2 R p1 p2 The space of rotations SO( 3) = {R ∈ R3×3 | RRT = I,det(R) = +1} Special orthogonal group(3): Why it’s a group: • Closed under multiplication: if ∈ ( ) then ∈ ( ) R1, R2 SO 3 R1R2 SO 3 • Has an identity: ∃ ∈ ( ) = I SO 3 s.t. IR1 R1 • Has a unique inverse… • Is associative… Why orthogonal: • vectors in matrix are orthogonal Why it’s special: det( R ) = + 1 , NOT det(R) = ±1 Right hand coordinate system Possible rotation representations You need at least three numbers to represent an arbitrary rotation in SO(3) (Euler theorem). Some three-number representations: • ZYZ Euler angles • ZYX Euler angles (roll, pitch, yaw) • Axis angle One four-number representation: • quaternions ZYZ Euler Angles φ = θ rzyz ψ φ − φ cos sin 0 To get from A to B: φ = φ φ Rz ( ) sin cos 0 1. Rotate φ about z axis 0 0 1 θ θ 2. Then rotate θ about y axis cos 0 sin θ = ψ Ry ( ) 0 1 0 3. Then rotate about z axis − sinθ 0 cosθ ψ − ψ cos sin 0 ψ = ψ ψ Rz ( ) sin cos 0 0 0 1 ZYZ Euler Angles φ θ ψ Remember that R z ( ) R y ( ) R z ( ) encode the desired rotation in the pre- rotation reference frame: φ = pre−rotation Rz ( ) Rpost−rotation Therefore, the sequence of rotations is concatentated as follows: (φ θ ψ ) = φ θ ψ Rzyz , , Rz ( )Ry ( )Rz ( ) φ − φ θ θ ψ − ψ cos sin 0 cos 0 sin cos sin 0 (φ θ ψ ) = φ φ ψ ψ Rzyz , , sin cos 0 0 1 0 sin cos 0 0 0 1− sinθ 0 cosθ 0 0 1 − − − cφ cθ cψ sφ sψ cφ cθ sψ sφ cψ cφ sθ (φ θ ψ ) = + − + Rzyz , , sφ cθ cψ cφ sψ sφ cθ sψ cφ cψ sφ sθ − sθ cψ sθ sψ cθ ZYX Euler Angles (roll, pitch, yaw) φ − φ cos sin 0 To get from A to B: φ = φ φ Rz ( ) sin cos 0 1.
    [Show full text]
  • Theory of Angular Momentum and Spin
    Chapter 5 Theory of Angular Momentum and Spin Rotational symmetry transformations, the group SO(3) of the associated rotation matrices and the 1 corresponding transformation matrices of spin{ 2 states forming the group SU(2) occupy a very important position in physics. The reason is that these transformations and groups are closely tied to the properties of elementary particles, the building blocks of matter, but also to the properties of composite systems. Examples of the latter with particularly simple transformation properties are closed shell atoms, e.g., helium, neon, argon, the magic number nuclei like carbon, or the proton and the neutron made up of three quarks, all composite systems which appear spherical as far as their charge distribution is concerned. In this section we want to investigate how elementary and composite systems are described. To develop a systematic description of rotational properties of composite quantum systems the consideration of rotational transformations is the best starting point. As an illustration we will consider first rotational transformations acting on vectors ~r in 3-dimensional space, i.e., ~r R3, 2 we will then consider transformations of wavefunctions (~r) of single particles in R3, and finally N transformations of products of wavefunctions like j(~rj) which represent a system of N (spin- Qj=1 zero) particles in R3. We will also review below the well-known fact that spin states under rotations behave essentially identical to angular momentum states, i.e., we will find that the algebraic properties of operators governing spatial and spin rotation are identical and that the results derived for products of angular momentum states can be applied to products of spin states or a combination of angular momentum and spin states.
    [Show full text]
  • Solving the Geodesic Equation
    Solving the Geodesic Equation Jeremy Atkins December 12, 2018 Abstract We find the general form of the geodesic equation and discuss the closed form relation to find Christoffel symbols. We then show how to use metric independence to find Killing vector fields, which allow us to solve the geodesic equation when there are helpful symmetries. We also discuss a more general way to find Killing vector fields, and some of their properties as a Lie algebra. 1 The Variational Method We will exploit the following variational principle to characterize motion in general relativity: The world line of a free test particle between two timelike separated points extremizes the proper time between them. where a test particle is one that is not a significant source of spacetime cur- vature, and a free particles is one that is only under the influence of curved spacetime. Similarly to classical Lagrangian mechanics, we can use this to de- duce the equations of motion for a metric. The proper time along a timeline worldline between point A and point B for the metric gµν is given by Z B Z B µ ν 1=2 τAB = dτ = (−gµν (x)dx dx ) (1) A A using the Einstein summation notation, and µ, ν = 0; 1; 2; 3. We can parame- terize the four coordinates with the parameter σ where σ = 0 at A and σ = 1 at B. This gives us the following equation for the proper time: Z 1 dxµ dxν 1=2 τAB = dσ −gµν (x) (2) 0 dσ dσ We can treat the integrand as a Lagrangian, dxµ dxν 1=2 L = −gµν (x) (3) dσ dσ and it's clear that the world lines extremizing proper time are those that satisfy the Euler-Lagrange equation: @L d @L − = 0 (4) @xµ dσ @(dxµ/dσ) 1 These four equations together give the equation for the worldline extremizing the proper time.
    [Show full text]
  • Geodetic Position Computations
    GEODETIC POSITION COMPUTATIONS E. J. KRAKIWSKY D. B. THOMSON February 1974 TECHNICALLECTURE NOTES REPORT NO.NO. 21739 PREFACE In order to make our extensive series of lecture notes more readily available, we have scanned the old master copies and produced electronic versions in Portable Document Format. The quality of the images varies depending on the quality of the originals. The images have not been converted to searchable text. GEODETIC POSITION COMPUTATIONS E.J. Krakiwsky D.B. Thomson Department of Geodesy and Geomatics Engineering University of New Brunswick P.O. Box 4400 Fredericton. N .B. Canada E3B5A3 February 197 4 Latest Reprinting December 1995 PREFACE The purpose of these notes is to give the theory and use of some methods of computing the geodetic positions of points on a reference ellipsoid and on the terrain. Justification for the first three sections o{ these lecture notes, which are concerned with the classical problem of "cCDputation of geodetic positions on the surface of an ellipsoid" is not easy to come by. It can onl.y be stated that the attempt has been to produce a self contained package , cont8.i.ning the complete development of same representative methods that exist in the literature. The last section is an introduction to three dimensional computation methods , and is offered as an alternative to the classical approach. Several problems, and their respective solutions, are presented. The approach t~en herein is to perform complete derivations, thus stqing awrq f'rcm the practice of giving a list of for11111lae to use in the solution of' a problem.
    [Show full text]
  • Rotation Matrix - Wikipedia, the Free Encyclopedia Page 1 of 22
    Rotation matrix - Wikipedia, the free encyclopedia Page 1 of 22 Rotation matrix From Wikipedia, the free encyclopedia In linear algebra, a rotation matrix is a matrix that is used to perform a rotation in Euclidean space. For example the matrix rotates points in the xy -Cartesian plane counterclockwise through an angle θ about the origin of the Cartesian coordinate system. To perform the rotation, the position of each point must be represented by a column vector v, containing the coordinates of the point. A rotated vector is obtained by using the matrix multiplication Rv (see below for details). In two and three dimensions, rotation matrices are among the simplest algebraic descriptions of rotations, and are used extensively for computations in geometry, physics, and computer graphics. Though most applications involve rotations in two or three dimensions, rotation matrices can be defined for n-dimensional space. Rotation matrices are always square, with real entries. Algebraically, a rotation matrix in n-dimensions is a n × n special orthogonal matrix, i.e. an orthogonal matrix whose determinant is 1: . The set of all rotation matrices forms a group, known as the rotation group or the special orthogonal group. It is a subset of the orthogonal group, which includes reflections and consists of all orthogonal matrices with determinant 1 or -1, and of the special linear group, which includes all volume-preserving transformations and consists of matrices with determinant 1. Contents 1 Rotations in two dimensions 1.1 Non-standard orientation
    [Show full text]
  • Hamilton Equations, Commutator, and Energy Conservation †
    quantum reports Article Hamilton Equations, Commutator, and Energy Conservation † Weng Cho Chew 1,* , Aiyin Y. Liu 2 , Carlos Salazar-Lazaro 3 , Dong-Yeop Na 1 and Wei E. I. Sha 4 1 College of Engineering, Purdue University, West Lafayette, IN 47907, USA; [email protected] 2 College of Engineering, University of Illinois at Urbana-Champaign, Urbana, IL 61820, USA; [email protected] 3 Physics Department, University of Illinois at Urbana-Champaign, Urbana, IL 61820, USA; [email protected] 4 College of Information Science and Electronic Engineering, Zhejiang University, Hangzhou 310058, China; [email protected] * Correspondence: [email protected] † Based on the talk presented at the 40th Progress In Electromagnetics Research Symposium (PIERS, Toyama, Japan, 1–4 August 2018). Received: 12 September 2019; Accepted: 3 December 2019; Published: 9 December 2019 Abstract: We show that the classical Hamilton equations of motion can be derived from the energy conservation condition. A similar argument is shown to carry to the quantum formulation of Hamiltonian dynamics. Hence, showing a striking similarity between the quantum formulation and the classical formulation. Furthermore, it is shown that the fundamental commutator can be derived from the Heisenberg equations of motion and the quantum Hamilton equations of motion. Also, that the Heisenberg equations of motion can be derived from the Schrödinger equation for the quantum state, which is the fundamental postulate. These results are shown to have important bearing for deriving the quantum Maxwell’s equations. Keywords: quantum mechanics; commutator relations; Heisenberg picture 1. Introduction In quantum theory, a classical observable, which is modeled by a real scalar variable, is replaced by a quantum operator, which is analogous to an infinite-dimensional matrix operator.
    [Show full text]
  • Coordinate Transformation
    Coordinate Transformation Coordinate Transformations In this chapter, we explore mappings – where a mapping is a function that "maps" one set to another, usually in a way that preserves at least some of the underlyign geometry of the sets. For example, a 2-dimensional coordinate transformation is a mapping of the form T (u; v) = x (u; v) ; y (u; v) h i The functions x (u; v) and y (u; v) are called the components of the transforma- tion. Moreover, the transformation T maps a set S in the uv-plane to a set T (S) in the xy-plane: If S is a region, then we use the components x = f (u; v) and y = g (u; v) to …nd the image of S under T (u; v) : EXAMPLE 1 Find T (S) when T (u; v) = uv; u2 v2 and S is the unit square in the uv-plane (i.e., S = [0; 1] [0; 1]). Solution: To do so, let’s determine the boundary of T (S) in the xy-plane. We use x = uv and y = u2 v2 to …nd the image of the lines bounding the unit square: Side of Square Result of T (u; v) Image in xy-plane v = 0; u in [0; 1] x = 0; y = u2; u in [0; 1] y-axis for 0 y 1 u = 1; v in [0; 1] x = v; y = 1 v2; v in [0; 1] y = 1 x2; x in[0; 1] v = 1; u in [0; 1] x = u; y = u2 1; u in [0; 1] y = x2 1; x in [0; 1] u = 0; u in [0; 1] x = 0; y = v2; v in [0; 1] y-axis for 1 y 0 1 As a result, T (S) is the region in the xy-plane bounded by x = 0; y = x2 1; and y = 1 x2: Linear transformations are coordinate transformations of the form T (u; v) = au + bv; cu + dv h i where a; b; c; and d are constants.
    [Show full text]