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Volumn 75, Issue 5, 2007, Pages 434-458

When action is not least

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EID: 34547379123     PISSN: 00029505     EISSN: None     Source Type: Journal    
DOI: 10.1119/1.2710480     Document Type: Article
Times cited : (60)

References (186)
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    • J. L. Lagrange, Analytical Mechanics (Mécanique Analytique) (Gauthier-Villars, Paris, 1888-89), 2nd ed. (1811) (Kluwer, Dordrecht, 1997), pp. 183 and 219.
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    • The same erroneous statement occurs in work published in 1760-61, ibid, p. xxxiii.
    • The same erroneous statement occurs in work published in 1760-61, ibid, p. xxxiii.
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    • We easily found about two dozen texts using the erroneous term maximum. See, for example, E. Mach, The Science of Mechanics, 9th ed, Open Court, La Salle, IL, 1960, p. 463;
    • We easily found about two dozen texts using the erroneous term "maximum." See, for example, E. Mach, The Science of Mechanics, 9th ed. (Open Court, La Salle, IL, 1960), p. 463;
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    • A similar error occurs in A. J. Hanson, Visualizing Quaternions (Elsevier, Amsterdam, 2006), p. 368, which states that geodesies on a sphere can have maximum length.
    • A similar error occurs in A. J. Hanson, Visualizing Quaternions (Elsevier, Amsterdam, 2006), p. 368, which states that geodesies on a sphere can have maximum length.
  • 24
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    • The number of authors of books and papers using extremum and extremal is endless. Some examples include R. Baierlein, Newtonian Dynamics (McGraw-Hill, New York, 1983), p. 125;
    • The number of authors of books and papers using "extremum" and "extremal" is endless. Some examples include R. Baierlein, Newtonian Dynamics (McGraw-Hill, New York, 1983), p. 125;
  • 26
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    • J. D. Logan, Invariant Variational Principles (Academic, New York, 1977) mentions both extremal and stationary, p. 8;
    • J. D. Logan, Invariant Variational Principles (Academic, New York, 1977) mentions both "extremal" and "stationary," p. 8;
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  • 28
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    • see also their Classical Theory of Fields, 4th ed. (Butterworth Heineman, Oxford, 1999), p. 25;
    • see also their Classical Theory of Fields, 4th ed. (Butterworth Heineman, Oxford, 1999), p. 25;
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    • V. Berry, review of The Optics of Rays, Wavefronts and Caustics by O. N. Stavroudis (Academic, New York, 1972),
    • V. Berry, review of The Optics of Rays, Wavefronts and Caustics by O. N. Stavroudis (Academic, New York, 1972),
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    • The seminal work on second variations of general functionals by Legendre, Jacobi, and Weierstrass and many others is described in the historical accounts of Refs. 19 and 20. Mayer's work (Ref. 19) was devoted specifically to the second variation of the Hamilton action. In our paper, we adapt Culverwell's work (Ref. 21) for the Maupertuis action W to the Hamilton action. Culverwell's work was preceded by that of Jacobi (Ref. 22) and Kelvin and Tait (Ref. 23).
    • The seminal work on second variations of general functionals by Legendre, Jacobi, and Weierstrass and many others is described in the historical accounts of Refs. 19 and 20. Mayer's work (Ref. 19) was devoted specifically to the second variation of the Hamilton action. In our paper, we adapt Culverwell's work (Ref. 21) for the Maupertuis action W to the Hamilton action. Culverwell's work was preceded by that of Jacobi (Ref. 22) and Kelvin and Tait (Ref. 23).
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    • C. G. J. Jacobi, Zür Theorie der Variationensrechnung und der Differential Gleichungen. J. f.Math. XVII, 68-82 (1837). An English translation is given in Ref. 20, p. 243, and a commentary is given in Ref. 19, p. 156.
    • C. G. J. Jacobi, "Zür Theorie der Variationensrechnung und der Differential Gleichungen." J. f.Math. XVII, 68-82 (1837). An English translation is given in Ref. 20, p. 243, and a commentary is given in Ref. 19, p. 156.
  • 52
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    • reprinted as Principles of Mechanics and Dynamics (Dover, New York, 1962), Part I, p. 422.
    • reprinted as Principles of Mechanics and Dynamics (Dover, New York, 1962), Part I, p. 422.
  • 53
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    • Gelfand and Fomin (Ref. 25) and other more recent books on calculus of variations are rigorous but rather sophisticated. A previous study (Ref. 26) of the nature of the stationarity of worldline action was based on the Jacobi-Morse eigenfunction method (Ref. 27), rather than on the more geometrical Jacobi-Culverwell-Whittaker approach.
    • Gelfand and Fomin (Ref. 25) and other more recent books on calculus of variations are rigorous but rather sophisticated. A previous study (Ref. 26) of the nature of the stationarity of worldline action was based on the Jacobi-Morse eigenfunction method (Ref. 27), rather than on the more geometrical Jacobi-Culverwell-Whittaker approach.
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    • translated by R. A. Silverman Prentice Hall, Englewood Cliffs, NJ
    • I. M. Gelfand and S. V. Fomin, Calculus of Variations, translated by R. A. Silverman (Prentice Hall, Englewood Cliffs, NJ, 1963),
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    • Russian edition 1961, reprinted (Dover, New York, 2000).
    • Russian edition 1961, reprinted (Dover, New York, 2000).
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    • The sufficient condition for an extremum in the classical action integral as an eigen-value problem
    • M. S. Hussein, J. G. Pereira, V. Stojanoff, and H. Takai, "The sufficient condition for an extremum in the classical action integral as an eigen-value problem," Am. J. Phys. 48, 767-770 (1980).
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    • Hussein et al. make the common error of assuming S can be a true maximum. See also J. G. Papastavridis, An eigenvalue criterion for the study of the Hamiltonian action's extremality, Mech. Res. Commun. 10, 171-179 (1983).
    • Hussein et al. make the common error of assuming S can be a true maximum. See also J. G. Papastavridis, "An eigenvalue criterion for the study of the Hamiltonian action's extremality," Mech. Res. Commun. 10, 171-179 (1983).
  • 59
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    • As we shall see, the nature of the stationary value of Hamilton's action S (and also Maupertuis' action W) depends on the sign of second variations δ2S and δ2W (defined formally in Sec. IV, which in turn depends on the existence or absence of kinetic foci (see Sees. II and VII, The same quantities (signs of the second variations and kinetic foci) are also important in classical mechanics for the question of dynamical stability of trajectories (Refs. 23 and 29-31, and in semiclassical mechanics where they determine the phase loss term in the total phase of the semiclassical propagator due to a particular classical path (Refs. 32 and 33, The phase loss depends on the Morse (or Morse-Maslov) index, which equals the number of kinetic foci between the end-points of the trajectory (see Ref. 34, Further, in devising computational algorithms to find the stationary points of the action either S or W, it is useful to know whether we are seeking a minimum
    • 2W) that determines which case we are considering. Practical applications of the mechanical focal points are mentioned at the end of Ref. 37.
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    • reissued as Stability of Motion, edited by A. T. Fuller (Taylor and Francis, London, 1975).
    • reissued as Stability of Motion, edited by A. T. Fuller (Taylor and Francis, London, 1975).
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    • Toward an extremum characterization of kinetic stability
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    • The principle of least action as a Lagrange variational problem: Stationarity and extremality conditions
    • J. G. Papastavridis, "The principle of least action as a Lagrange variational problem: Stationarity and extremality conditions," Int. J. Eng. Sci. 24, 1437-1443 (1986);
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    • On a Lagrangean action based kinetic instability theorem of Kelvin and Tait, Int. J. Eng. Sci. 24, 1-17 (1986).
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    • In general, saddle points can be classified (or given an index (Ref. 27)) according to the number of independent directions leading to maximum-type behavior. Thus the point of zero-gradient on an ordinary horse saddle has a Morse index of unity. The Morse index for an action saddle point is equal to the number of kinetic foci between the end-points of the trajectory (Ref. 32, p. 90). Readable introductions to Morse theory are given by R. Forman, How many equilibria are there? An introduction to Morse theory, in Six Themes on Variation, edited by R. Hardt (American Mathematical Society, Providence, RI, 2004), pp. 13-36,
    • In general, saddle points can be classified (or given an index (Ref. 27)) according to the number of independent directions leading to maximum-type behavior. Thus the point of zero-gradient on an ordinary horse saddle has a Morse index of unity. The Morse index for an action saddle point is equal to the number of kinetic foci between the end-points of the trajectory (Ref. 32, p. 90). Readable introductions to Morse theory are given by R. Forman, "How many equilibria are there? An introduction to Morse theory," in Six Themes on Variation, edited by R. Hardt (American Mathematical Society, Providence, RI, 2004), pp. 13-36,
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    • E. T. Whittaker, A Treatise on the Analytical Dynamics of Particles and Rigid Bodies, 4th ed. (originally published in 1904) (Cambridge U. P., Cambridge, 1999), p. 253.
    • E. T. Whittaker, A Treatise on the Analytical Dynamics of Particles and Rigid Bodies, 4th ed. (originally published in 1904) (Cambridge U. P., Cambridge, 1999), p. 253.
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    • The same example was treated earlier by, Braunschweig, Vieweg, reprinted Chelsea, New York, 1969, p. 46
    • The same example was treated earlier by C. G. J. Jacobi, Vorlesungen Über Dynamik (Braunschweig, Vieweg, 1884), reprinted (Chelsea, New York, 1969), p. 46.
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    • A closer mechanics-optics analogy is between a kinetic focus (mechanics) and a caustic point (optics, Ref. 38, The locus of limiting intersection points of pairs of mechanical spatial orbits is termed an envelope or caustic (see Fig. 7 for an example, just as the locus of limiting intersection points of pairs of optical rays is termed a caustic. In optics, the intersection point of a bundle of many rays is termed a focal point; a mechanical analogue occurs naturally in a few systems, for example, the sphere geodesies of Fig. 1 and the harmonic oscillator trajectories of Fig. 3, where a bundle of trajectories recrosses at a mechanical focal point. In electron microscopes (Refs. 39 and 40, mass spectrometers (Ref. 41, and particle accelerators Ref. 42, electric and magnetic field configurations are designed to create mechanical focal points
    • A closer mechanics-optics analogy is between a kinetic focus (mechanics) and a caustic point (optics) (Ref. 38). The locus of limiting intersection points of pairs of mechanical spatial orbits is termed an envelope or caustic (see Fig. 7 for an example), just as the locus of limiting intersection points of pairs of optical rays is termed a caustic. In optics, the intersection point of a bundle of many rays is termed a focal point; a mechanical analogue occurs naturally in a few systems, for example, the sphere geodesies of Fig. 1 and the harmonic oscillator trajectories of Fig. 3, where a bundle of trajectories recrosses at a mechanical focal point. In electron microscopes (Refs. 39 and 40), mass spectrometers (Ref. 41), and particle accelerators (Ref. 42), electric and magnetic field configurations are designed to create mechanical focal points.
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    • Systems with subsequent kinetic foci are discussed in Sees. VIII and IX. For examples with only a single kinetic focus, see Figs. 6 and 7. 46 M. C. Gutzwiller, The origins of the trace formula, in Classical, Semiclassical and Quantum Dynamics in Atoms, edited by H. Friedrich and B. Eckhardt (Springer, New York, 1997), pp. 8-28.
    • Systems with subsequent kinetic foci are discussed in Sees. VIII and IX. For examples with only a single kinetic focus, see Figs. 6 and 7. 46 M. C. Gutzwiller, "The origins of the trace formula," in Classical, Semiclassical and Quantum Dynamics in Atoms, edited by H. Friedrich and B. Eckhardt (Springer, New York, 1997), pp. 8-28.
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    • This type of variation, δx, αφ, δẋ, αφ, where δx and δẋ vanish together for α → 0, is termed a weak variation. See, for example, C. Fox, An Introduction to the Calculus of Variations (Oxford U. P, Oxford, 1950, reprinted Dover, New York, 1987, p. 3
    • This type of variation, δx = αφ, δẋ = αφ, where δx and δẋ vanish together for α → 0, is termed a weak variation. See, for example, C. Fox, An Introduction to the Calculus of Variations (Oxford U. P., Oxford, 1950), reprinted (Dover, New York, 1987), p. 3.
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    • As discussed in Sec. VI, for a true worldline x0(t) or PQ, where Q is the (first) kinetic focus, we have β2S=0 for one special variation (and δ2S > 0 for all other variations) as well as δS=0 for all variations. Further, we show that δ3S, etc, all vanish for the special infinitesimal variation for which δ2S vanishes, and that S-S0=0 to second-order for larger such variations. In the latter case, typically δ3S is nonvanishing due to a single coalescing alternative worldline. In atypical (for one dimension Ref. 58, cases, more than one coalescing alternative worldline occurs, and the first nonvanishing term is δ4S or higher order, see Ref. 32, pp. 122-127. The harmonic oscillator is a limiting case where δk5=0 for all k for the special variation around worldline PQ, which reflects the infinite number of true worldlines which connect P to
    • k5=0 for all k for the special variation around worldline PQ, which reflects the infinite number of true worldlines which connect P to Q, and which can all coalesce by varying the amplitude (see Fig. 3). In Morse theory (Refs. 27 and 34) the worldline PQ is referred to as a degenerate critical (stationary) point.
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    • This statement and the corresponding one in Ref. 52 must be qualified. It is in general not simply a matter of the time interval (tR-t P) being short. The spatial path of the worldline must be sufficiently short. When, as usually happens, more than one actual worldline can connect a given position xP to a given position xR in the given time interval (tR-tP, for short time intervals only the spatially shortest worldline will have the minimum action. For example, the repulsive power-law potentials U(x) C/xn (including the limiting case of a hard-wall potential at the origin for C → 0) and the repulsive exponential potential U(x, U0exp(-x/a) have been studied (Ref. 53, No matter how short the time interval tR, tP, two different worldlines can connect given position xP to given position xR. The fact that two different true worldlines can connect th
    • P). Only for the shortest of these worldlines is S a minimum. The situation is different in 2D (see Appendix B).
  • 95
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    • 2 → ẋ.
    • 2 → ẋ.
  • 96
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    • L. I. Lolle, C. G. Gray, J. D. Poll, and A. G. Basile, Improved short-time propagator for repulsive inverse power-law potentials, Chem. Phys. Lett. 177, 64-72 (1991, In Sec. X and Ref. 54 further analytical and numerical results are given for the inverse-square potential, U(x)=C/x 2. For given end positions xP and xR, there are two actual worldlines (xP,tP) → (x R,tR) for given short times (tR-tP, There is one actual worldline for tR=tQ when the two worldlines have coalesced into one, and there is no actual worldline for longer times remember xP and x are fixed
    • P and x are fixed).
  • 97
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    • A relaxation algorithm for classical paths as a function of end points: Application to the semiclassical propagator for far-from-caustic and near-caustic conditions
    • A. G. Basile and C. G. Gray, "A relaxation algorithm for classical paths as a function of end points: Application to the semiclassical propagator for far-from-caustic and near-caustic conditions," J. Comput. Phys. 101, 80-93 (1992).
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    • Better estimates can be found using the Sturm and Sturm-Liouville theories; see Papastavridis, Refs. 26 and 66.
    • Better estimates can be found using the Sturm and Sturm-Liouville theories; see Papastavridis, Refs. 26 and 66.
  • 99
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    • This argument can be refined. In Sec. 8 we show that δ2S becomes script O sign(α3) for R → Q but is still larger in magnitude than the δ3S term, which is also script O sign(α3, See Ref. 60 for δ2S and Eq, 40a) for δ3S
    • 3S.
  • 100
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    • 2=0 [see Eq. (19)], so that kinetic foci do not exist.
    • 2=0 [see Eq. (19)], so that kinetic foci do not exist.
  • 101
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    • 2S =0 is called the multiplicity of the kinetic focus (Van Brunt, Ref. 34, p. 254; Ref. 32, p. 90). If the mulitplicity is different from unity, Morse's theorem is modified from the statement in Ref. 34 to read as follows; The Morse index of the saddle point in action of worldline PR is equal to the number of kinetic foci between P and R, with each kinetic focus counted with its multiplicity.
    • 2S =0 is called the multiplicity of the kinetic focus (Van Brunt, Ref. 34, p. 254; Ref. 32, p. 90). If the mulitplicity is different from unity, Morse's theorem is modified from the statement in Ref. 34 to read as follows; The Morse index of the saddle point in action of worldline PR is equal to the number of kinetic foci between P and R, with each kinetic focus counted with its multiplicity.
  • 103
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    • The fact that δ2S0→0 for α→0 is not surprising because δ2S0 is proportional to α2. The surprising fact is that here δ2S 0 vanishes as α3 as α → 0 because the integral involved in the definition, Eq, 36a, of δ2S 0 is itself script O sign(α, We can see directly that δ2S0 becomes script O sign(α3) for R near Q for this special variation αφ by integrating the φ term by parts in Eq, 36a) and using φ=0 at the end-points. The result is δ2S0, α2/2)∫P Rφ[mφ +U″(x0)φ] dt. Because x 0 and x1=x0+αφ are both true worldlines, we can apply the equation of motion mẍ+U′(x)=0 to both. We then subtract these tw
    • 0.
  • 104
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    • 2S<0, in agreement with Morse's general theory (Ref. 34).
    • 2S<0, in agreement with Morse's general theory (Ref. 34).
  • 105
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    • If we use L(x,ẋ)=pẋ-H(x,p, we can rewrite the Hamilton action as a phase-space integral, that is, S=∫PR[pẋ, H(x, p)]dt. We set δS=0 and vary x(t) and p(t) independently and find (Ref. 63) the Hamilton equations of motion ẋ=∂H/∂p, ṗ=-∂H/∂x. We can then show (Ref. 64) that in phase space, the trajectories x(t, p(t) that satisfy the Hamilton equations are always saddle points of 5, that is, never a true maximum or a true minimum. In the proof it is assumed that H has the normal form H(x,p)=p2/2m+Ux
    • 2/2m+U(x).
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    • Reference 48, p. 353
    • Reference 48, p. 353.
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    • C. W. Misner, K. S. Thorne, and J. A. Wheeler, Gravitation (Freeman, San Francisco, 1973, p. 318. These authors use the Rayleigh-Ritz direct variational method (see Ref. 12 for a detailed discussion of this method) with a two-term trial trajectory x(t, a1 sin (ωt/2)+a 2 sin (ωt, where ω =2π/tR and a 1 and a2 are variational parameters, to study the half-cycle (tR=T0/2) and one-cycle (tR=T 0) trajectories. Because the kinetic focus time TQ > T0/2 for this oscillator, they find, in agreement with our results, that S is a minimum for the half-cycle trajectory (with a1 ≠ 0, a2, 0) and a saddle point for the one-cycle trajectory (with a 1, 0, a2 ≠ 0, However, in the figure accompanying their calculation, which shows the stationary points in (a1,a 2) space, they lab
    • 2)=(0,0) represents the equilibrium trajectory x(t)=0. As we have seen, a true maximum in S cannot occur, so that other "directions" in function space not considered by the authors must give minimum-type behavior of S, leading to an overall saddle point.
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    • The two-incline oscillator potential has the form U(x)=C|x|, with C = mg sin α cos α and α the angle of inclination. Here x is a horizontal direction. A detailed discussion of this oscillator is given by B. A. Sherwood, Notes on Classical Mechanics (Stipes, Champaign, Il, 1982), p. 157.
    • The two-incline oscillator potential has the form U(x)=C|x|, with C = mg sin α cos α and α the angle of inclination. Here x is a horizontal direction. A detailed discussion of this oscillator is given by B. A. Sherwood, Notes on Classical Mechanics (Stipes, Champaign, Il, 1982), p. 157.
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    • 2|x|, the bouncing ball (Ref. 71), and for x ≥ 0 the constant force spring (Ref. 72).
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    • Nearly pure quartic potentials have been found in molecular physics for ring-puckering vibrational modes (Ref. 75) and for the caged motion of the potassium ion K+ in the endohedral fullerene complex K, C60 (Ref. 76, where the quadratic terms in the potential are small. Ferroelectric soft modes in solids are also sometimes approximately represented by quartic potentials Refs. 77 and 78
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    • In two dimensions with x=(x1,x2) and v 0=(v01,v02, our analytic condition (4) for the kinetic focus of worldline x(t, v0) becomes det(∂x i/∂v0j, 0, where det(Aij) denotes the determinant of matrix Aij. The generalization to other dimensions is obvious. This condition (in slightly different form) is due to Mayer, Ref. 19, p. 269
    • ij. The generalization to other dimensions is obvious. This condition (in slightly different form) is due to Mayer, Ref. 19, p. 269.
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    • For a clear discussion, see J. G. Papastavridis, Analytical Mechanics (Oxford U. P., Oxford, 2002), p. 1061.
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    • For multidimensions a caustic becomes in general a surface in space-time. The analogous theory for multidimensional spatial caustics, relevant for the action W, is discussed in Ref. 105. A simple example of a 2D surface spatial caustic is obtained by revolving the pattern of Fig. 7 about the vertical axis, thereby generating a paraboloid of revolution surface caustic/envelope. Due to axial symmetry, the caustic has a second (linear) branch, that is, the symmetry axis from y=0 to y=Y. An analogous optical example is discussed by M. V. Berry, Singularities in waves and rays, in Physics of Defects, Les Houches Lectures XXXIV, edited by R. D. Balian, M. Kleman, and J.-P. Poirier (North Holland, Amsterdam, 1981). pp. 453-543.
    • For multidimensions a caustic becomes in general a surface in space-time. The analogous theory for multidimensional spatial caustics, relevant for the action W, is discussed in Ref. 105. A simple example of a 2D surface spatial caustic is obtained by revolving the pattern of Fig. 7 about the vertical axis, thereby generating a paraboloid of revolution surface caustic/envelope. Due to axial symmetry, the caustic has a second (linear) branch, that is, the symmetry axis from y=0 to y=Y. An analogous optical example is discussed by M. V. Berry, "Singularities in waves and rays," in Physics of Defects, Les Houches Lectures XXXIV, edited by R. D. Balian, M. Kleman, and J.-P. Poirier (North Holland, Amsterdam, 1981). pp. 453-543.
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    • A dynamics problem can be formulated as an initial value problem. For example, find x(t) from Newton's equation of motion with initial conditions (xP,ẋP, It can also be formulated as a boundary value problem; for example, find x(t) from Hamilton's principle with boundary conditions (xP,tP) and (xR,tR, Solving a boundary value problem with initial value problem methods (for example, the shooting method) is standard (Ref. 82, Solving an initial value problem with boundary value problem methods is much less common (Ref. 83, For an example of a boundary value problem with mixed conditions (prescribed initial velocities and final positions) for about 107 particles, see A. Nusser and E. Branchini, On the least action principle in cosmology, Mon. Not. R. Astron. Soc. 313, 587-595 2000
    • R). Solving a boundary value problem with initial value problem methods (for example, the shooting method) is standard (Ref. 82). Solving an initial value problem with boundary value problem methods is much less common (Ref. 83). For an example of a boundary value problem with mixed conditions (prescribed initial velocities and final positions) for about 107 particles, see A. Nusser and E. Branchini, "On the least action principle in cosmology," Mon. Not. R. Astron. Soc. 313, 587-595 (2000).
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    • The converse effect cannot occur: a time-dependent potential U(x, t) with U″ < 0 at all times always has δ2>0 as seen from Eq, 19, If U(x,t) is such that U″ alternates in sign with time, kinetic foci (and hence trajectory stability) may occur. An example is a pendulum with a rapidly vertically oscillating support point. In effect the gravitational field is oscillating. The pendulum can oscillate stably about the (normally unstable) upward vertical direction (Ref. 85, Two- and three-dimensional examples of this type are Paul traps (Ref. 86) and quadrupole mass filters (Ref. 85, which use oscillating quadrupole electric fields to trap ions. The equilibrium trajectory x(f)=0 at the center of the trap is unstable for purely electrostatic fields but is stabilized by using time-dependent electric fields. Focusing by alternating-gradients (also known as strong focus ing) in particle accelerators and storage rings is based on the same idea Ref. 42
    • 2>0 as seen from Eq. (19). If U(x,t) is such that U″ alternates in sign with time, kinetic foci (and hence trajectory stability) may occur. An example is a pendulum with a rapidly vertically oscillating support point. In effect the gravitational field is oscillating. The pendulum can oscillate stably about the (normally unstable) upward vertical direction (Ref. 85). Two- and three-dimensional examples of this type are Paul traps (Ref. 86) and quadrupole mass filters (Ref. 85), which use oscillating quadrupole electric fields to trap ions. The equilibrium trajectory x(f)=0 at the center of the trap is unstable for purely electrostatic fields but is stabilized by using time-dependent electric fields. Focusing by alternating-gradients (also known as strong focus ing) in particle accelerators and storage rings is based on the same idea (Ref. 42).
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    • For example, the equilibrium position can be modulated. A somewhat similar system is a ball bouncing on a vertically oscillating table. The motion can be chaotic. See, for example, Springer, New York
    • For example, the equilibrium position can be modulated. A somewhat similar system is a ball bouncing on a vertically oscillating table. The motion can be chaotic. See, for example, J. Guckenheimer and P. Holmes, Nonlinear Oscillations, Dynamical Systems and Bifurcations of Vector Fields (Springer, New York, 1983), p. 102;
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    • 0 cos ωt is studied in Ref. 30. For k=0 the Duffing oscillator reduces to the quartic oscillator.
    • 0 cos ωt is studied in Ref. 30. For k=0 the Duffing oscillator reduces to the quartic oscillator.
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    • 0 cos ωt (note the sign change in C compared to Ref. 92), and the Henon-Heiles oscillator with the potential in Eq. (83).
    • 0 cos ωt (note the sign change in C compared to Ref. 92), and the Henon-Heiles oscillator with the potential in Eq. (83).
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    • In Ref. 54 the harmonic potential U(x, t, 1/2)k[x, x c(t)]2 with an oscillating equilibrium position x c(t) is studied. The worldlines for this system are all nonchaotic
    • c(t) is studied. The worldlines for this system are all nonchaotic.
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    • The situation is complicated because, as Eq. (A1) shows, there are two forms for W, that is, the time-independent (first) form and the time-dependent (last) form. Spatial kinetic foci (discussed in Appendix B) occur for the time-independent form of W. Space-time kinetic foci occur for the time-dependent form of W, as for S. Typically the kinetic foci for the two forms for W differ from each other (Refs. 30 and 98) and from those for S.
    • The situation is complicated because, as Eq. (A1) shows, there are two forms for W, that is, the time-independent (first) form and the time-dependent (last) form. Spatial kinetic foci (discussed in Appendix B) occur for the time-independent form of W. Space-time kinetic foci occur for the time-dependent form of W, as for S. Typically the kinetic foci for the two forms for W differ from each other (Refs. 30 and 98) and from those for S.
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    • Families of Keplerian orbits
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    • We assume that we are dealing with bound orbits. Similar comments apply to scattering orbits (hyperbolas, Just as for the orbits in the linear gravitational potential discussed in the preceding paragraph, here too there are restrictions and special cases (Ref. 19, p. 164; Ref. 103, p. 122, If the second point (xR,yR) lies within the ellipse of safety (the envelope (French, Ref. 101, of the elliptical trajectories of energy E originating at (xP,yP, then two ellipses with energy E can connect (xP,yP) to (xR,y R, If (xR,yR) lies on the ellipse of safety, then one ellipse of energy E can connect (xP,yP) to (xR,yR, and if (xR,yR) lies outside the ellipse of safety, then no ellipse of energy E can connect the two points. Usually the initial and final points (xP,yP) and x R
    • P) to (0,0), a third kinetic focus arises for elliptical periodic orbits in three dimensions (see Ref. 33, p. 29).
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    • For the repulsive 1/r potential, the hyperbolic spatial orbits have a (parabolic shaped) caustic/envelope (French, Ref. 101).
    • For the repulsive 1/r potential, the hyperbolic spatial orbits have a (parabolic shaped) caustic/envelope (French, Ref. 101).
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    • If the orbit equation has the explicit form y=y(x, θ0, or the implicit form f(x, y, θ0)=0, the spatial kinetic focus is found from ∂y/∂θ0=0 or ∂f/ ∂θ0=0, respectively. Here θ0 is the launch angle at (xP,yP, see Fig. 15 for an example, The derivation of these spatial kinetic focus conditions is similar to the derivation of the space-time kinetic focus condition of Eq, 4, see Ref. 106, p. 59, In contrast, if the orbit equation is defined parametrically by the trajectory equations x=x(t, θ0) and y=y(t, θ0, the spatial kinetic focus condition is ∂(x, y)/∂(t, θ0)=0. This Jacobian determinant condition is similar to that of Ref. 80 for the space-time kinetic focus see Ref. 106, p. 73 for a derivation, As an example, consider a family of figure-eight-like harmonic oscillator orbits of Fig. 16, laun
    • 2)|x|, which is a parabolic shaped curve with two cusps on the y-axis.
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    • The finding of the two elliptical (or hyperbolic or parabolic) shaped trajectories from observations giving the two end-positions and the time interval is a famous problem of astronomy and celestial mechanics, solved by Lambert (1761), Gauss (1801-1809), and others (Ref. 108).
    • The finding of the two elliptical (or hyperbolic or parabolic) shaped trajectories from observations giving the two end-positions and the time interval is a famous problem of astronomy and celestial mechanics, solved by Lambert (1761), Gauss (1801-1809), and others (Ref. 108).
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    • P. R. Escobal, Methods of Orbit Determination (Wiley, New York, 1965), p. 187. For the elliptical orbits, more than two trajectories typically become possible at sufficiently large time intervals; these additional trajectories correspond to more than one complete revolution along the orbit (Ref. 109).
    • P. R. Escobal, Methods of Orbit Determination (Wiley, New York, 1965), p. 187. For the elliptical orbits, more than two trajectories typically become possible at sufficiently large time intervals; these additional trajectories correspond to more than one complete revolution along the orbit (Ref. 109).
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    • It is clear from Fig. 13 that a kinetic focus occurs after time T 0. To show rigorously that this focus is the first kinetic focus (unlike for W where it is the second, we can use a result of Gordon (Ref. 111) that the action S is a minimum for time t=T0. If one revolution corresponds to the second kinetic focus, the trajectory P → P would correspond to a saddle point. The result tQ, T0 can also be obtained algebraically by applying the general relation (4) to the relation r, r(t, L) for the radial distance, where we use angular momentum L as the parameter labeling the various members of the family in Fig. 13. We obtain tQ from (∂r/∂L)t=0. The latter equation implies that (∂t/∂L)r=0, because (∂r/∂L) t, ∂r/∂t)L(∂t/∂L)r. At fixed energy E or fixed major axis 2a, the period T0 is independent of L for the attra
    • Q.
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    • Note that for the actual 2D trajectories in the potential U(x, y)=mgy, kinetic foci exist for the spatial paths of the Maupertuis action W, but do not exist for the space-time trajectories of the Hamilton action S. This result illustrates the general result stated in Appendix A that the kinetic foci for W and S differ in general.
    • Note that for the actual 2D trajectories in the potential U(x, y)=mgy, kinetic foci exist for the spatial paths of the Maupertuis action W, but do not exist for the space-time trajectories of the Hamilton action S. This result illustrates the general result stated in Appendix A that the kinetic foci for W and S differ in general.
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    • The four variational principles of mechanics
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    • Gray, C.G.1    Karl, G.2    Novikov, V.A.3
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    • From Maupertuis to Schrödinger. Quantization of classical variational principles
    • C. G. Gray, G. Karl, and V. A. Novikov, "From Maupertuis to Schrödinger. Quantization of classical variational principles," Am. J. Phys. 67, 959-961 (1999).
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    • Gray, C.G.1    Karl, G.2    Novikov, V.A.3
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    • Quantisierung als eigenwert problem I
    • E. Schrödinger, "Quantisierung als eigenwert problem I," Ann. Phys. 79, 361-376 (1926),
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    • translated in E. Schrödinger, Collected Papers on Wave Mechanics (Blackie, London, 1928),
    • translated in E. Schrödinger, Collected Papers on Wave Mechanics (Blackie, London, 1928),
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    • Chelsea reprint 1982. For modern discussions and applications, see, for example, E. Merzbacher, Quantum Mechanics, 3rd ed. (Wiley, New York, 1998), p. 135;
    • Chelsea reprint 1982. For modern discussions and applications, see, for example, E. Merzbacher, Quantum Mechanics, 3rd ed. (Wiley, New York, 1998), p. 135;


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.