Design and Implementation of Models for the Double Precision Trajectory Program (DPTRAJ,;

Total Page:16

File Type:pdf, Size:1020Kb

Design and Implementation of Models for the Double Precision Trajectory Program (DPTRAJ,; II i e NATIONAL AERONAUTIC . AND SPACE ADMINISTRATION Technical Memorandum 33-451 Design and Implementation of Models for the Double Precision Trajectory Program (DPTRAJ,; Gerd W. Spier r N71-25152 tCOD_) (NASA CR OR TN_X _ AD NUMBER) (CAIEG-ORY) JET PROPULSION LABORATORY CALIFOINIA INSTITUTE OF TECNNOLOG-If PASADENA, CALIFORNIA,. April 15, 1971 ':- ........ :,_L." _L :.. i_,%'_''. ' NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Technical Memorandum 33-451 Design and Implementation of Models for the Double Precision Trajectory Program (DPTRAJ) eerd W. Spier 1 _r JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENAp CALIFORNIA April 15, 1971 V_}_C_bIG pAC,_B'_K _IOT_'ILLI_ Preface The work described in this report was performed by the Systems Division of the Jet Propulsion Laboratory. % JPL TECHNICAL MEMORANr_UM 33-451 iii Acknowledgmen_ The author wishes to express his appreciation to Mr. Francis Sturms, group supervisor of the Trajectories and Performance Group, and to Mr. Ahmad Khstib, cognizant engineer of DPTRA], both of the JPL Systems Analysis Section (Section 892), for their efforts and contributions to this paper. In addition, he would like to extend appreciation to Mr. Fred Lesh, supervisor of the Traiectory Group, to Mr. Alva Joseph, cognizant programmer, to Mr. Joseph Witt and Dr. Thomas Talbot, all of the JPL Flight Operations and Deep Space Network Progr._mming Section (Section 315), and to Mr. John Strand of Informatics for e- providing valuable insights into the computer program DPTRA]. _) .,..' Jv dPL TECHNICAL MEMORANDUM 33-451 t Contents h Introduction 1 Ih Time and Coordinate Transformations in General 2 A. Coordinate Conversions 2 B. Rotations 2 1. Space-fixed 2 2. Body-fixed 2 IIh Systemsof Time 2 A. Tropical Year and EphemerisTime 3 B. Atomic Time 3 C. Universal Time 3 D. Transformation Between Time Scales 3 IV. Coordinate Type Transformations 4 A. Spherical to Cartesian Cocrd!nate=- Transformation 4 B. Cartesian to Spherical Coordinates Transformation 5 C. Classical to Cartesian Coordinates Transformation 6 1. Elliptic orbit 7 2. Hyperbolic orbit B 3. Parabolic orbit 9 D. Cartesian to Classical Coordinat,;s Transformation 10 E. Pseudo-Asymptote and Asymptote Coordinates to Cartesian Coordinates Transformation 14 V. Rotations of Coordinate Systems. 19 A. Earth-Related Transformations 19 B. Rotation From Mean Earth Equator of 1950.0 to Mean Equator of Date 19 C. Mean Obliquity of Eclipticand its Time Derivative . 22 D. Earth Mean or True Equatorial Coordinates to EclipticCoordinates Rotation 22 E, Mean Earth Equatorand Equinoxof Date Coordinates to True Earth Equator and Equinox of Date Coordinates Rotations , , 23 F. Rotation Transforming Earth.CenteredTrue Equatorial of Date, Space.Fixed Coordinates to Earth-Fixed Coordinates . 2s i JPL TECHNICAL MEMORANDUM 33.451 V /: Contents (contd) . G. Mars-Related Transformations 27 1. Rotation matrices for position vectors 29 2. Rotation matrices for velocity vectors . 30 H. Moon-Related Transformations 31 I. Rotation From Earth Mean Ecliptic to Moon True Equator Coordinate System 33 J. Rotation From Moon True Equator and Equinox of Date Coordinates to Moon-Fixed Coordinates . 34 VI. Translation of Centers 35 VII. Equations of Motion of a Spacecraft. 35 A. Newtonian Point.Mass Acceleration . 36 1. Center of mass and invariable plane . 36 2. Force function . 38 3. Transfer of origin and perturbing forces . 38 B0 Acceleration Caused by an Oblate Body . 39 C. Acceleration Caused by Solar Radiation Pressure and Operation of Attitude-Control System. 42 D° Acceleration Caused by Finite Motor Burns 45 E. Acceleration Caused by Indirect Oblateness 47 1. Basic equations 47 2. Derivation of_erm__2 48 F. Acceleration Caused by General Relativity 52 1. Relativistic equations of motion 53 2. Heliocentric ephemeris of a planet Cother than earth) 55 3. Heliocentric ephemeris of earth-moon barycente_. 55 4. Geocentric ephemeris of moon 55 5. Equations of motion for generation of a spacecraft ephemeris 56 ! VIII. Numerical Integration of Equations of Motion of a Spacecraft . 56 A. Solution Method 56 B. Backward Differences 56 C. Derivation of Predictor-Corrector Formulas 58 D. Computation of Coefficients a_Cs), b_Cs), c_Cs), d_Cs) . 6O _T vi •If_L TECHNICAL MEMORANDUM 33.451 i Contents (contd) E. Starting Procedures 64 1. Start by Taylor series expansion 64 2. Computation of Taylor series coefficients 66 3. Extrapolative start 69 F. Control of Step Size h 70 1. Step-size control by range list 70 2. Automatic step-size control 71 G. Reverse Integration 72 IX. Differential Correction Process 72 A. Interpolation and Differential Correction of Basic Planetary Ephemerides 73 1. Interpolation ._ 73 2. Differential correction o_ basic ephemerides . 74 B. Partial Derivatives Formulation 75 C. Correction to Ephemeris . 77 X. Summary of Results Obtained From Integrating the Equat!ons of Motion . 77 A. Body Group 77 B. Conic Group . 82 ] C. Angle Group . 94 l.-Clock and cone angles 94 2. Angle iASD and limb angles . 96 3. Hinge and swivel angles . 96 , Appendix A. Proof of Kepler's Laws 98 r_ Appendix B. Kepler's Equation 103 Appendix C. Solution of Kepler's Equation 108 -_ Appendix D. The Vis-Viva Integral 111 l Appendix E. Linearized Flight Time 113 i Glossary 117 1 References . 131 * Bibliography 132 Index 123 JPL TECHNICAL MEMORANDUM 33-451 vii Contents (contd) Table 1. Raddii of relativity spheres 54 Figures 1. Spherical coordinates 4 2. Enlargement of the H-plane ° • ° ° 5 3. Orbital elements . 7 4. Eccentric and true anomalies 7 5. A hyperbolic orbit 8 6. A parabolic orbit . 9 7. Orbit of a spacecraft . 11 8. Spacecraft flight plane 15 9. Launch geometry 16 10. The flight-path angle P 17 11. The radius vector Rm_ 17 12. Mean equator of 1950.0 to mean equator of date 20 13. Rotation about X"-axis 20 14. Rotation about Z'-axis 20 15. Mean obliquity of the ecliptic 22 16. True or mean obliquity . 23 17. Mean and true equinox of date 24 18. Prime meridian of the earth . 25 19. Greenwich hour angle . 26 20. Nutation in longitude, true and mean obliquity 26 21. Martian equator and equinox 27 22. Spherical triangle 1 . 28 23. Spherical triangle 2 29 24. Lunar equator and orbit . 31 25, The orbit of the moon relative to earth . 32 26. Earth mean ecliptic and moon true equatorial coordinate systems . 33 27. Space. and body-fixed lunar' coordinates 34 viii JPL TECHNICAL MEMORANDUM 33.451 .... !ii 2 Contents (contd) Figures (contd) Translation of centers 35 A system of bodies in an inertial coordinate frame . 36 Rectangular coordinate system axes x', y', and zp, relative to body-fixed axes Xb, yb, Zb . 40 The angle K . 44 Orientation of a spacecraft relative to sun, earth, and reference body 45 The parameter D . 45 Spacecraft moving into or out of shadow of body 45 Up-north-east coordinate system 52 Simplified schematic representation of gravity in space-time system 53 Step sizes h and hp 69 Right ascension and declination of a spacecraft 79 The vector II_ 79 Angles P and _ . 79 The vector/'* 80 Angles y and 8O The quantity/_ 82 Sun-shadow parameter d 82 3 Sun-shadow parameter d_ 82 Eccentric anomaly E 84 The quantity F 85 L_ Angles p and vm.... 85 Deflection angle between asymptote vectors 86 A A ^ The vectors W, N, and M 88 ^ A The vectors g, V, ._, and _ 89 i Impact parameter vector B 9O Magnitude of vector B 9O Coordinates of vector B . 90 B vector impact radius 91 Incoming and outgoing asymptote vectors 92 The R, S, T target coordinate system 93 JPL TECHNICAL MEMORANDUM 33-451 Ix Contents (contd) Figures (contd) 58. The vectors Jibe and R_o 93 59. The angle ET_ 0 94 60. The angle XYZ 94 61. Vectors _, and _ . 95 62. Clock and cone angles 95 63. The angle iASD 95 64. The angle xPNi 96 ^ 65. The vector $ . 96 66. Hinge. and swivel angles 96 A-1. Two-body gravitational attraction 98 A-2. Radial component of 100 A-3. Velocities in polar reference frame 101 B-I. An elliptic orbit 103 B-2. A hyperbolic orbit 105 B-:3. A parabolic orbit . 106 C-1. The Method of false position 109 D-1. Velocity components of body b 111 E-1. Trajectory approach geometry 113 i JPL TECHNICAL MEMORANDUM 33-451 '_ ............ i--. " -_'-_._.-_- .; --" " ......... : .............. ' ...... - _ -__ ... - Abstract A common requirement for all lunar and planetary missions is the extremely accurate determination of the trajectory of a spacecraft. The Double Precision Trajectory Program (DPTRAJ) developed by JPL has proved to be a very accurate and dependable tool for the computation of interplanetary trajectories during the Mariner missions in 1969. This report describes the mathematical models that are used in DPTRA] at present, with emphasis on the development of the equations. +! ,+." +, 4 JPL TECHNICAL MEMORANDUM 33-4_I x| Design and Implementation of Models for the Double Precision Trajectory Program (DPTRAJ) I. Introductior, Because the total acc.rleration of a spacecraft cannot be integrated in closed form, recourse must be taken to An important factor in determining high-precision numerical methods. At present, the equatiorts of motion interplanetary trajectories is the computation and sub- of a spacecraft are integrated by a so-called second-sum sequent integrahon of the acceleration of a spa.,2ecraft numerical-integration scheme relaHve to some central that is moving in the solar system and is subject to a body (Cowcll method). variety of forces. The forces acting upon the spacecraft determine its acceleration according to Newton's second law; therefore, knowledge of the forces implies knowledge The equations of motion are solved for the spacecraft of the acceleration of the spacecraft. Integration of the ordy, and ignore the negligible perturbations of the space- total acceleration in some convenient frame of reference craft on celestial bodies (i.e., on the sun, moon, and establishes the ephemeris of the spacecraft, and hence planets); hence, it is sufficient to obtain positions and its trajectory.
Recommended publications
  • The Floating Body in Real Space Forms
    THE FLOATING BODY IN REAL SPACE FORMS Florian Besau & Elisabeth M. Werner Abstract We carry out a systematic investigation on floating bodies in real space forms. A new unifying approach not only allows us to treat the important classical case of Euclidean space as well as the recent extension to the Euclidean unit sphere, but also the new extension of floating bodies to hyperbolic space. Our main result establishes a relation between the derivative of the volume of the floating body and a certain surface area measure, which we called the floating area. In the Euclidean setting the floating area coincides with the well known affine surface area, a powerful tool in the affine geometry of convex bodies. 1. Introduction Two important closely related notions in affine convex geometry are the floating body and the affine surface area of a convex body. The floating body of a convex body is obtained by cutting off caps of volume less or equal to a fixed positive constant δ. Taking the right-derivative of the volume of the floating body gives rise to the affine surface area. This was established for all convex bodies in all dimensions by Schütt and Werner in [62]. The affine surface area was introduced by Blaschke in 1923 [8]. Due to its important properties, which make it an effective and powerful tool, it is omnipresent in geometry. The affine surface area and its generalizations in the rapidly developing Lp and Orlicz Brunn–Minkowski theory are the focus of intensive investigations (see e.g. [14,18, 20,21, 45, 46,65, 67,68, 70,71]).
    [Show full text]
  • Matrices for Fenchel–Nielsen Coordinates
    Annales Academi½ Scientiarum Fennic½ Mathematica Volumen 26, 2001, 267{304 MATRICES FOR FENCHEL{NIELSEN COORDINATES Bernard Maskit The University at Stony Brook, Mathematics Department Stony Brook NY 11794-3651, U.S.A.; [email protected] Abstract. We give an explicit construction of matrix generators for ¯nitely generated Fuch- sian groups, in terms of appropriately de¯ned Fenchel{Nielsen (F-N) coordinates. The F-N coordi- nates are de¯ned in terms of an F-N system on the underlying orbifold; this is an ordered maximal set of simple disjoint closed geodesics, together with an ordering of the set of complementary pairs of pants. The F-N coordinate point consists of the hyperbolic sines of both the lengths of these geodesics, and the lengths of arc de¯ning the twists about them. The mapping from these F-N coordinates to the appropriate representation space is smooth and algebraic. We also show that the matrix generators are canonically de¯ned, up to conjugation, by the F-N coordinates. As a corol- lary, we obtain that the TeichmullerÄ modular group acts as a group of algebraic di®eomorphisms on this Fenchel{Nielsen embedding of the TeichmullerÄ space. 1. Introduction There are several di®erent ways to describe a closed Riemann surface of genus at least 2; these include its representation as an algebraic curve; its representation as a period matrix; its representation as a Fuchsian group; its representation as a hyperbolic manifold, in particular, using Fenchel{Nielsen (F-N) coordinates; its representation as a Schottky group; etc. One of the major problems in the overall theory is that of connecting these di®erent visions.
    [Show full text]
  • 19710025511.Pdf
    ORBIT PERTLJFEATION THEORY USING HARMONIC 0SCII;LCITOR SYSTEPE A DISSERTATION SUBMITTED TO THE DEPARTbIEllT OF AJ3RONAUTICS AND ASTROW-UTICS AND THE COMMITTEE ON GRADUATE STUDDS IN PAEMlIAL FULFI-NT OF THE mQUIREMENTS I FOR THE DEGREE OF DOCTOR OF PHILOSOPHY By William Byron Blair March 1971 1;"= * ..--"".-- -- -;.- . ... - jlgpsoijed f~:;c2ilc e distribution unlinl:;&. --as:.- ..=-*.;- .-, . - - I certify that I have read this thesis and that in my opinion it is fully adequate, in scope and quality, as a dissertation for the degree of Doctor of Philosophy. d/c fdd&- (Principal Adviser) I certify that I have read this thesis and that in my opinion it is fully adequate, in scope and quality, as a dissertation for the degree of Doctor of Philosoph~ ., ., I certify that I have read this thesis and that in my opinion it is fully adequate, in scop: and quality, as a dissertation for the degree of Doctor of Philosophy. Approved for the University Cormnittee on Graduate Studies: Dean of Graduate Studies ABSTRACT Unperturbed two-body, or Keplerian motion is transformed from the 1;inie domain into the domains of two ur,ique three dimensional vector harmonic oscillator systems. One harmoriic oscillator system is fully regularized and hence valid for all orbits including the rectilinear class up to and including periapsis passage, The other system is fdly as general except that the solution becomes unbounded at periapsis pas- sage of rectilinear orbits. The natural frequencies of the oscillator systems are related to certain Keplerian orbit scalar constants, while the independent variables are related to well-known orbit angular measurements, or anomalies.
    [Show full text]
  • Some Applications of the Spectral Theory of Automorphic Forms
    Academic year 2009-2010 Department of Mathematics Some applications of the spectral theory of automorphic forms Research in Mathematics M.Phil Thesis Francois Crucifix Supervisor : Doctor Yiannis Petridis 2 I, Francois Nicolas Bernard Crucifix, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. SIGNED CONTENTS 3 Contents Introduction 4 1 Brief overview of general theory 5 1.1 Hyperbolic geometry and M¨obius transformations . ............. 5 1.2 Laplaceoperatorandautomorphicforms. ......... 7 1.3 Thespectraltheorem.............................. .... 8 2 Farey sequence 14 2.1 Fareysetsandgrowthofsize . ..... 14 2.2 Distribution.................................... 16 2.3 CorrelationsofFareyfractions . ........ 18 2.4 Good’sresult .................................... 22 3 Multiplier systems 26 3.1 Definitionsandproperties . ...... 26 3.2 Automorphicformsofnonintegralweights . ......... 27 3.3 Constructionofanewseries. ...... 30 4 Modular knots and linking numbers 37 4.1 Modularknots .................................... 37 4.2 Linkingnumbers .................................. 39 4.3 TheRademacherfunction . 40 4.4 Ghys’result..................................... 41 4.5 SarnakandMozzochi’swork. ..... 43 Conclusion 46 References 47 4 Introduction The aim of this M.Phil thesis is to present my research throughout the past academic year. My topics of interest ranged over a fairly wide variety of subjects. I started with the study of automorphic forms from an analytic point of view by applying spectral methods to the Laplace operator on Riemann hyperbolic surfaces. I finished with a focus on modular knots and their linking numbers and how the latter are related to the theory of well-known analytic functions. My research took many more directions, and I would rather avoid stretching the extensive list of applications, papers and books that attracted my attention.
    [Show full text]
  • Hilbert Geometry of the Siegel Disk: the Siegel-Klein Disk Model
    Hilbert geometry of the Siegel disk: The Siegel-Klein disk model Frank Nielsen Sony Computer Science Laboratories Inc, Tokyo, Japan Abstract We study the Hilbert geometry induced by the Siegel disk domain, an open bounded convex set of complex square matrices of operator norm strictly less than one. This Hilbert geometry yields a generalization of the Klein disk model of hyperbolic geometry, henceforth called the Siegel-Klein disk model to differentiate it with the classical Siegel upper plane and disk domains. In the Siegel-Klein disk, geodesics are by construction always unique and Euclidean straight, allowing one to design efficient geometric algorithms and data-structures from computational geometry. For example, we show how to approximate the smallest enclosing ball of a set of complex square matrices in the Siegel disk domains: We compare two generalizations of the iterative core-set algorithm of Badoiu and Clarkson (BC) in the Siegel-Poincar´edisk and in the Siegel-Klein disk: We demonstrate that geometric computing in the Siegel-Klein disk allows one (i) to bypass the time-costly recentering operations to the disk origin required at each iteration of the BC algorithm in the Siegel-Poincar´edisk model, and (ii) to approximate fast and numerically the Siegel-Klein distance with guaranteed lower and upper bounds derived from nested Hilbert geometries. Keywords: Hyperbolic geometry; symmetric positive-definite matrix manifold; symplectic group; Siegel upper space domain; Siegel disk domain; Hilbert geometry; Bruhat-Tits space; smallest enclosing ball. 1 Introduction German mathematician Carl Ludwig Siegel [106] (1896-1981) and Chinese mathematician Loo-Keng Hua [52] (1910-1985) have introduced independently the symplectic geometry in the 1940's (with a preliminary work of Siegel [105] released in German in 1939).
    [Show full text]
  • Travelling Randomly on the Poincar\'E Half-Plane with a Pythagorean Compass
    Travelling Randomly on the Poincar´e Half-Plane with a Pythagorean Compass July 29, 2021 V. Cammarota E. Orsingher 1 Dipartimento di Statistica, Probabilit`ae Statistiche applicate University of Rome `La Sapienza' P.le Aldo Moro 5, 00185 Rome, Italy Abstract A random motion on the Poincar´ehalf-plane is studied. A particle runs on the geodesic lines changing direction at Poisson-paced times. The hyperbolic distance is analyzed, also in the case where returns to the starting point are admitted. The main results concern the mean hyper- bolic distance (and also the conditional mean distance) in all versions of the motion envisaged. Also an analogous motion on orthogonal circles of the sphere is examined and the evolution of the mean distance from the starting point is investigated. Keywords: Random motions, Poisson process, telegraph process, hyperbolic and spherical trigonometry, Carnot and Pythagorean hyperbolic formulas, Cardano for- mula, hyperbolic functions. AMS Classification 60K99 1 Introduction Motions on hyperbolic spaces have been studied since the end of the Fifties and most of the papers devoted to them deal with the so-called hyperbolic Brownian motion (see, e.g., Gertsenshtein and Vasiliev [4], Gruet [5], Monthus arXiv:1107.4914v1 [math.PR] 25 Jul 2011 and Texier [9], Lao and Orsingher [7]). More recently also works concerning two-dimensional random motions at finite velocity on planar hyperbolic spaces have been introduced and analyzed (Orsingher and De Gregorio [11]). While in [11] the components of motion are supposed to be independent, we present here a planar random motion with interacting components. Its coun- terpart on the unit sphere is also examined and discussed.
    [Show full text]
  • ' ~ !Iifi.;Tf(I',A Memi~ Well/A41 All ~! GAIL NGA: (301) 320-3621 for De
    . ':...',. ~ if ~OO ~ National Capital Astronomers.l/J ~..i9j~'Y Wilshin!ltlln. DC (301) 320- 3621 Volume XLVill Number 4 December 1989 ISSN 0898-7548 Ryan: Quasar S, VLBJ Track Earth Crust Shifts --~ Cap;ital A~tronomers colloquium in t~e "... NatIonal Air and Space Museum. He will descn"be the joint NASA/NOAA use of Very Long Baseline Interferometry (VIBD with quasars, the farthest known objects in the universe, for tracking tectonic plate motions in the Earth within a centimeter. He will present latest results from the San Francisco and Alaska earthquakes, and measurement of a 9-cm per year motion of Hawaii towaro Japan. He will also discuss measurements of nutation and various other components of polar motion, and the techniques with which the effects of atmospheric refraction and ionospheric dispersion are compensated. James W. Ryan received his B.S. from John Carroll University in Cleveland and his M.S. in mathematics from George MR. RYAN Washington University. In 1963 he joined I~ /;'Ir. James W. Ryan, of the new Space NASA Goddaro Space Flight Center, where ltWGeodesy Branch, NASA GOOdaro Space he calculated Apollo orbits for the next Flight Center, will discuss a decade. Since the Apollo program he has currently active, effective application of been engaged in the VLBI Program, the astronomy to an important, down-to-Earth basis of the current Space Geodesy problem at the December 2 National program which he will descuss. DECEMBmt CALBNDAR- The EXlblic is welcome. Friday, Decembeer 1, 8, 15, 22, 29, 7:30 pm -Telescope-making classes at American University, McKinley Hall basement.
    [Show full text]
  • 19720023166.Pdf
    /~~~~~~~ ~'. ,;/_ ., i~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~f', k· ' S 7. 0 ~ ~~~~~ ·,. '''':'--" ""-J' x ' ii 5 T/~~~~~~~~~' q z ?p~ ~ ~ ~~~~'-'. -' ' 'L ,'' "' I ci~~~'""7: .... ''''''~ 1(oI~~~~~~~~~~~~~~~~~~~~nci"~~~~~~~~~~~~~' ;R --,'~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~j. DTERSMINAT ION,SUBSYSTEM I i~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~, ;' '~/ ',\* i ' /,i~~·EM'AI-At1' - ' ' ' ' . , .. SPECQIFICA~TIONS'` .i ~~~~~~~-- r ~. i .t +-% ~.- V~~~~~~~r~_' " , ' ''~v N .·~~~~~,·' : z' '% - '::' "~'' ' ·~''-,z '""·' -... '"' , ......?.':; ,,<" .~:iI ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~-.. L /' ' ) .. d~' 1.- il · ) · 'i. i L i i; j~~~~~~~~~~l^ ' .1) ~~~~~~~~~~~~Y~~~~~~~~~~ .i · ~ .i -~.,,-~.~~ ' / (NASA-TM-X-65984 ) GODDARD TRAJECTORY N 72- 30O816 , .,-Q: ... DETERMlINATION SUBSY STEM: M9ATHEMATICAL k_ % SP E CIFTC AT IONS W.E. Wagner, et al (NASA) -_/3.· ~ar. 1972 333 CSCL 22C Uca i-- ~·--,::--..:- ~~~~~~~~~ ~~~~~~~ : .1... T~T· r~ ~~~~~~~~~~~~I~~~~~~~~~~ ~ ~ ~ ~ ~ I~-' ~~~~~~~ x -'7 ' ¥' .;'. ,( .,--~' I "-, /. ·~.' 'd , %- ~ '' ' , , ' ~,- - . '- ' :~ ' ' ' ". · ' ~ . 'I - ... , ~ ~ -~ /~~~~~~~~~~~~~~~~~~.,. ,.,- ,~ , ., ., . ~c ,x. , -' ,, ~ ~ -- ' ' I/· \' {'V ,.%' -- -. '' I ,- ' , -,' · '% " ' % \ ~ 2 ' - % ~~: ' - · r ~ %/, .. I : ,-, \-,;,..' I '.-- ,'' · ~"I. ~ I· , . ...~,% ' /'-,/.,I.~ .,~~~-~, ",-->~-'."-,-- '''i" - ~' -,'r ,I r .'~ -~~~'-I ' ' ;, ' r-.'', ":" I : " " ' -~' '-", '" I~~ ~~~~~i ~ ~~~~~~~~'"'% ~'. , ' ',- ~-,' - <'/2 , -;'- ,. 'i , 7-~' ' ,'z~, , '~,'ddz ~ "% ' ~',2; ; ' · -o ,-~ ' '~',.,~~~~.~,~,,,:.i? -":,:-,~-
    [Show full text]
  • Life in the Rindler Reference Frame: Does an Uniformly Accelerated Charge Radiates? Is There a Bell ‘Paradox’? Is Unruh Effect Real?
    Life in the Rindler Reference Frame: Does an Uniformly Accelerated Charge Radiates? Is there a Bell `Paradox'? Is Unruh Effect Real? Waldyr A. Rodrigues Jr.1 and Jayme Vaz Jr.2 Departamento de Matem´aticaAplicada - IMECC Universidade Estadual de Campinas 13083-859 Campinas, SP, Brazil Abstract The determination of the electromagnetic field generated by a charge in hyperbolic motion is a classical problem for which the majority view is that the Li´enard-Wiechert solution which implies that the charge radi- ates) is the correct one. However we analyze in this paper a less known solution due to Turakulov that differs from the Li´enard-Wiechert one and which according to him does not radiate. We prove his conclusion to be wrong. We analyze the implications of both solutions concerning the validity of the Equivalence Principle. We analyze also two other is- sues related to hyperbolic motion, the so-called Bell's \paradox" which is as yet source of misunderstandings and the Unruh effect, which accord- ing to its standard derivation in the majority of the texts, is a correct prediction of quantum field theory. We recall that the standard deriva- tion of the Unruh effect does not resist any tentative of any rigorous mathematical investigation, in particular the one based in the algebraic approach to field theory which we also recall. These results make us to align with some researchers that also conclude that the Unruh effect does not exist. Contents 1. Introduction 2 2. Rindler Reference Frame 4 2.1. Rindler Coordinates . 5 arXiv:1702.02024v1 [physics.gen-ph] 7 Feb 2017 2.2.
    [Show full text]
  • Observations of Disintegrating Long-Period Comet C/2019 Y4 (ATLAS) – a Sibling of C/1844 Y1 (Great Comet)
    Draft version June 17, 2020 Typeset using LATEX twocolumn style in AASTeX62 Observations of Disintegrating Long-Period Comet C/2019 Y4 (ATLAS) { A Sibling of C/1844 Y1 (Great Comet) Man-To Hui (1文韜)1 and Quan-Zhi Ye (I泉志)2 1Institute for Astronomy, University of Hawai`i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA 2Department of Astronomy, University of Maryland, College Park, MD 20742, USA (Received 2020; Revised June 17, 2020; Accepted 2020) ABSTRACT We present a study of C/2019 Y4 (ATLAS) using Sloan gri observations from mid-January to early April 2020. During this timespan, the comet brightened with a growth in the effective cross-section of (2:0 ± 0:1) × 102 m2 s−1 from the beginning to ∼70 d preperihelion in late March 2020, followed by a brightness fade and the comet gradually losing the central condensation. Meanwhile, the comet became progressively bluer, and was even bluer than the Sun (g − r ≈ 0:2) when the brightness peaked, likely due to activation of subterranean fresh volatiles exposed to sunlight. With the tailward-bias corrected −7 astrometry we found an enormous radial nongravitational parameter, A1 = (+2:25 ± 0:13) × 10 au d−2 in the heliocentric motion of the comet. Taking all of these finds into consideration, we conclude that the comet has disintegrated since mid-March 2020. By no means was the split new to the comet, as we quantified that the comet had undergone another split event around last perihelion ∼5 kyr ago, during which its sibling C/1844 Y1 (Great Comet) was produced, with the in-plane component of the −1 separation velocity &1 m s .
    [Show full text]
  • 8 Surfaces Invariant by One-Parameter Group of Hyperbolic Isometries Having Constant Mean Curvature in ˜ PSL2(R,Τ)
    8 Surfaces invariant by one-parameter group of hyperbolic isometries having constant mean curvature in PSL2(R,τ) g On (3) Ricardo Sa Earp gave explicit formulas for parabolic and hyper- bolic screw motions surfaces immersed in H2 R. There, they gave several × examples. In this chapter we only consider surfaces invariant by one-parameter group of hyperbolic isometries having constant mean curvature immersed in P] SL (R, τ). Since for τ 0 we are in H2 R then we have generalized the result 2 ≡ × obtained by Ricardo Sa Earp when the surface is invariant by one-parameter group of hyperbolic isometries having constant mean curvature. In this chapter we focus our attention on surfaces invariant by one- parameter group of hyperbolic isometries. To study this kind of surfaces, we take M 2 = H2 that is the half plane model for the hyperbolic space. Thus, the metric of M 2 is given by: 1 dσ2 = λ2(dx2 + dy2), λ = . y From Proposition 5.1.1, we know that to obtain a hyperbolic motion on ] P SL2(R, τ), it is necessary consider a hyperbolic motion (hyperbolic isometry) on H2. 8.1 Surfaces invariant by one-parameter group of hyperbolic isometries main lemma The idea to obtain a surface invariant by one-parameter group of hyper- bolic isometries is simple, we will take a curve in the xt plane and we will apply ] one-parameter group Γ of hyperbolic isometries on P SL2(R, τ). We denote by α(x)=(x, 1,u(x)) the curve in the xt plane and by S = Γ(α), the surface invariant by one-parameter group of hyperbolic isometries generate by α.
    [Show full text]
  • The Automorphic Universe
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Università degli Studi di Napoli Federico Il Open Archive Università di Napoli Federico II - Dipartimento di Scienze Fisiche Dottorato di Ricerca in Fisica Fondamentale e Applicata - XX Ciclo Anno Accademico 2007-2008 The Automorphic Universe Coordinatore Candidato Prof. G. Miele Luca Antonio Forte Supervisore prof. A. Sciarrino On the cover: Gravity, M. C. Escher, Lithograph and watercolor (1952) Property of the M. C. Escher Company B. V. - http://www.mcescher.com/ a mammà a papà a peppe Contents Introduction 2 Why the automorphic universe . 3 Plan of the thesis . 3 I Mathematical Structures 5 1 Chaotic Dynamical Systems 6 1.1 Ergodicity, Mixing, Hyperbolicity and All that . 6 1.1.1 The Gauss map . 18 1.1.2 Geodesic Flows and Billiards . 21 1.2 Quantum chaology, not quantum chaos . 25 1.3 The Gutzwiller Trace Formula . 28 1.4 Hyperbolic Geometry and Fuchsian Groups . 31 1.4.1 The regular octagon . 42 1.4.2 The modular group and some of its distinguished sub- groups . 42 1.5 Maass automorphic forms and the Selberg Trace Formula . 47 1.6 The geodesic flow on the hyperbolic plane . 54 1.6.1 Artin modular billiard . 56 1.7 Quantum Unique Ergodicity . 59 1.8 Notes and Comments on Chapter 1 . 62 2 Kac-Moody Algebras 67 2.1 Overview of Kac-Moody Algebras . 68 2.1.1 On Kac-Moody groups: A remark on terminology . 73 2.2 Classification of Kac-Moody Algebras . 74 2.2.1 Affine Kac-Moody Algebras .
    [Show full text]