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Primer on Complex Systems

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Part of the book series: Lecture Notes in Physics ((LNP,volume 943))

Abstract

Complexity has become one of the buzzwords of modern science. It is almost impossible to browse through a recent issue of any scientific journal without running into terms such as complexity, complex behaviour, complex dynamics or complex systems mentioned in one way or another. But what do most scientists actually mean when they use these terms? What does it take for a system to become complex? Why is it important to know if it is complex or not?

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Notes

  1. 1.

    At the same time, it is during these large crashes that new fortunes are more easily made!

  2. 2.

    Many would even go further and claim that there are as many approaches as there are investigators working in this context!

  3. 3.

    In fact, some authors feel that the complex approach is useless to predict the future. We feel that this criticism is however rather unfair since, even if the level of quantitative predictability associated to classical theories is well beyond the capabilities of complexity theory, a certain level of predictability does indeed exist.

  4. 4.

    It is interesting to note that non-determinism is often invoked to differentiate complex systems from chaotic ones. Indeed, chaotic systems are usually deterministic, closed and low-dimensional, while complex systems are often non-deterministic, open and high-dimensional. This distinction also relies on the fact that chaotic systems are usually simplified mathematical models, whilst complex systems are often real systems. It is however worth pointing out that when we simulate complex systems in a computer, nondeterminism disappears since computers are perfectly deterministic. However, we can still observe many emergent features. This is the case, for instance, of any numerical simulation of a fully-developed turbulent system with a large number of degrees of freedom. In the computer, these simulations are driven by a deterministic source (even pseudo-random numbers are deterministic!). However, they still behave like a complex system in many ways. One is the development of a scale-free inertial range; another, the exhibition of long-term correlations and scale-free statistics. This fact suggests that openness and high-dimensionality are probably stronger requirements than non-determinism in order to achieve complex behaviour!

  5. 5.

    The set of partial differential equations that describe the weather system have, in fact, an infinite number of dimensions since N → as the limit of zero parcel size is taken.

  6. 6.

    In contrast, chaotic systems are usually low-dimensional systems defined by a small number of ordinary differential equations, usually N < 10.

  7. 7.

    Nonlinear means that the superposition principle, that states that the any linear combination of solutions of a problem is again a solution of the same problem, is no longer valid.

  8. 8.

    The reader should be aware that this predator-prey model is low-dimensional, closed and deterministic, and does not exhibit complex dynamics. In fact, the version described here is not even chaotic since less than two interacting populations are considered. We feel, however, that thanks to its simplicity, this model works great to illustrate the connection between nonlinearities and feedbacks and feedback loops. It is also great to introduce the concept of threshold, that will be of great importance later on.

  9. 9.

    The attentive reader might complain that we used a nonlinear term to model a similar process in the case of hares. The explanation is based on the fact that hares can live without lynx, quietly feeding on grass, but lynx cannot live without hares to hunt. Therefore, n l should naturally go to zero whenever n h  = 0. This requires the use of the linear term (see Problem 1.1).

  10. 10.

    The phase-space of the predator-prey model is the two-dimensional space that uses n l and n h as coordinates. A point in this phase space represents a possible state of the system, given by a pair of values (n h , n l ). A trajectory in phase space corresponds to the evolution in time of the hare and lynx populations, starting from given initial conditions, as allowed by the equations of the model.

  11. 11.

    The two-dimensional Lotka-Volterra equation does not exhibit either chaotic or complex behaviour. However, if one considers N-order Lotka-Volterra equations, \(\dot n_i = r_i n_i(1 - \sum _{j=1}^N \alpha _{ij}n_j)\), chaotic behaviour ensues for N > 3, where the system, although deterministic, is no longer integrable [38]. For N = 3, limit cycles do appear, to which the trajectories are drawn by the dynamics, but trajectories are not chaotic.

  12. 12.

    A fixed point of a system of ODEs is a point of phase space where the right-hand-side of the system of ODEs vanishes [39]. Since the right-hand-sides give the time derivatives of all relevant dynamical quantities, the evolution of the system remains unchanged if it starts from any fixed point in phase space, or after it reaches any of them over time. Thus, their name. Fixed points maybe stable, if the solution tends to come back to the fixed point after being perturbed, unstable, if perturbations grow and push the solution away, or neutral, if the perturbation neither grows nor is damped (see Appendix 1 in this chapter).

  13. 13.

    Note that, in the same limit, (B) and (A) coalesce to (n h , n l ) = (0,  0), and remain unstable.

  14. 14.

    Various other names such as non-diffusive transport, anomalous transport, self-similar transport or scale-free transport, are also often used, depending mainly on the specific field and author.

  15. 15.

    This is in contrast to the situation in equilibrium phase transitions, where some physical magnitude, usually temperature, must be finely tuned.

  16. 16.

    Scale-invariance is also apparent in many other quantities of the sandpile. Naturally, the actual value of the exponents and the limits of the mesoscale are different.

  17. 17.

    In an infinite sandpile (in space and time), the mesoscale would extend over all scales. The sandpile would then behave as a true monofractal. In reality, deviations from scale-invariance should be expected at scales that approach any of the finite boundaries. As a result, he monofractal behaviour is only approximate. In particular, the sandpile size (lifespan) must be significantly larger (longer) than the unit cell (one iteration) in order to display SOC dynamics.

  18. 18.

    In fact, Bak’s original formulation (and most analytical studies, such as those that describe SOC dynamics as an absorbing transition [56]) of SOC assume the limit of zero duration, in which avalanches are relaxed instantaneously once excited.

  19. 19.

    In fact, this apparently innocent statement can become pretty important in some cases, such as when trying to confine plasma energy in a tokamak fusion reactor. The determination of whether the confined plasma exhibits SOC or not might cost (or save) the fusion program quite a few millions of additional dollars.

  20. 20.

    Power degradation is not unique to SOC systems. It may also happen in diffusive systems whenever D is a function of the external power. That is the case, for instance, in driven plasmas since D is then a function of the local temperature.

  21. 21.

    It should be noted, however, that SOC could also sustain average supermarginal profiles if the drive is strong enough to keep the profiles above marginal more often than not. SOC would however disappear if the system becomes overdriven, with profiles staying above threshold everywhere, all the time.

  22. 22.

    Finding effective transport models for non-diffusive systems is a very important problem and a very active area of research, particularly in engineering contexts such as the development of magnetic confinement fusion reactors, or the understanding of transport in porous media that has applications in oil extraction or pollutant control, to name a few.

References

  1. Tautz, J.: The Buzz About Bees. Springer, Berlin (2007)

    Google Scholar 

  2. Krugman, P.R.: The Self-organizing Economy. Blackwell Publishers, London (2010)

    Google Scholar 

  3. Dana, K.S., Roy, P.K., Kurths, J. (eds.): Complex Dynamics in Physiological Systems: From Heart to Brain. Springer, Berlin (2009)

    MATH  Google Scholar 

  4. Goertzel, B.: Chaotic Logic: Language, Thought, and Reality from the Perspective of Complex Systems Science. Springer, Boston (1994)

    Book  MATH  Google Scholar 

  5. Larsen-Freeman, D., Cameron, L.: Complex Systems and Applied Linguistics. Oxford University Press, Oxford (2008)

    Google Scholar 

  6. Murray, J.D.: Mathematical Biology. Springer, Heidelberg (1989)

    Book  MATH  Google Scholar 

  7. Kaneko, K.: Life: An Introduction to Complex Systems Biology. Springer, New York (2006)

    Book  MATH  Google Scholar 

  8. Dobson, I., Carreras, B.A., Lynch, V.E., Newman, D.E.: Complex Systems Analysis of Series of Blackouts: Cascading Failure, Critical Points, and Self-organization. Chaos 17, 026103 (2007)

    Article  ADS  MATH  Google Scholar 

  9. Dijkstra, H.A.: Nonlinear Climate Dynamics. Cambridge University Press, Cambridge (2013)

    Book  MATH  Google Scholar 

  10. Hergarten, S.: Self-organized Criticality in Earth Systems. Springer, Heidelberg (2002)

    Book  Google Scholar 

  11. Drossel, B., Schwabl, F.: Self-organized Critical Forest Fire Model. Phys. Rev. Lett. 69, 1629 (1992)

    Article  ADS  Google Scholar 

  12. Sheluhin, O., Smolskiy, S., Osin, A.: Self-similar Processes in Telecommunications. Wiley, New York (2007)

    Book  Google Scholar 

  13. Park, K., Willinger, W.: The Internet as a Large-Scale Complex System. Santa Fe Institute Press, Santa Fe (2002)

    Google Scholar 

  14. Wright, Q.: A Study of War. University of Chicago Press, Chicago (1965)

    Google Scholar 

  15. Allison, M.A., Kelly, S.: The Complexity Advantage: How the Science of Complexity Can Help Your Business Achieve Peak Performance. McGraw Hill, New York (1999)

    Google Scholar 

  16. Chowdhury, D., Santen, L., Schadschneider, A.: Statistical Physics of Vehicular Traffic and Some Related Systems. Phys. Rep. 329, 199 (2000)

    Article  ADS  MathSciNet  Google Scholar 

  17. Binney, J., Tremaine, S.: Galactic Dynamics. Princeton University Press, Princeton, NJ (2008)

    MATH  Google Scholar 

  18. Pietronero, L.: The Fractal Structure of the Universe: Correlations of Galaxies and Clusters. Physica 144A, 257 (1987)

    Article  ADS  MATH  Google Scholar 

  19. Baryshev, Y., Teerikorpi, P.: Discovery of Cosmic Fractals. World Scientific, Singapore (2000)

    Google Scholar 

  20. Frank, J., King, A., Raine, D.: Accretion Power in Astrophysics. Cambridge University Press, Cambridge (2002)

    Book  Google Scholar 

  21. Priest, E.R.: Magnetohydrodynamics of the Sun. Cambridge University Press, Cambridge (2014)

    Google Scholar 

  22. Parker, E.N.: Cosmical Magnetic Fields. Oxford University Press, Oxford (1979)

    Google Scholar 

  23. Crosby, N.B., Aschwanden, M.J., Dennis, B.R.: Frequency Distributions and Correlations of Solar X-ray Flare Parameters. Sol. Phys. 143, 275 (1993)

    Article  ADS  Google Scholar 

  24. Aschwanden, M.J.: Self-organized Criticality in Astrophysics. Springer, New York (2014)

    MATH  Google Scholar 

  25. Moffat, H.K.: Magnetic Field Generation in Electrically Conducting Fluids. Cambridge University Press, Cambridge (1978)

    Google Scholar 

  26. Akasofu, S.I., Chapman, S.: Solar-Terrestrial Physics. Oxford University Press, Oxford (1972)

    Google Scholar 

  27. Heikkila, W.J.: Earth’s Magnetosphere. Elsevier Publishers, Amsterdam (2011)

    Google Scholar 

  28. Lui, A.T.Y., Chapman, S.C., Liou, K., Newell, P.T., Meng, C.I., Brittnacher, M., Parks, G.K.: Is the Dynamic Magnetosphere an Avalanching System? Geophys. Res. Lett. 27, 911 (2000)

    Article  ADS  Google Scholar 

  29. Wesson, J.: Tokamaks. Oxford University Press, Oxford (2008)

    MATH  Google Scholar 

  30. Diamond, P.H., Hahm, T.S.: On the Dynamics of Turbulent Transport Near Marginal Stability. Phys. Plasmas 2, 3640 (1995)

    Article  ADS  Google Scholar 

  31. Sanchez, R., Newman, D.E.: Topical Review: Self-Organized-Criticality and the Dynamics of Near-Marginal Turbulent Transport in Magnetically Confined Fusion Plasmas. Plasma Phys. Controlled Fusion 57, 123002 (2015)

    Article  ADS  Google Scholar 

  32. Wagner, F., Stroth, U.: Transport in Toroidal Devices-the Experimentalist’s View. Plasma Phys. Controlled Fusion 35, 1321 (1993)

    Article  ADS  Google Scholar 

  33. Terry, P.W.: Suppression of Turbulence and Transport by Sheared Flow. Rev. Mod. Phys. 72, 109 (2000)

    Article  ADS  Google Scholar 

  34. Boffetta, G., Cencini, M., Falcioni, M., Vulpiani, A.: Predictability: A Way to Characterize Complexity. Phys. Rep. 356, 367 (2002)

    Article  ADS  MathSciNet  MATH  Google Scholar 

  35. Prigogine, I., Nicolis, G.: Self-organization in Non-Equilibrium Systems. Wiley, New York (1977)

    MATH  Google Scholar 

  36. Chaisson, E.J.: Cosmic Evolution: The Rise of Complexity in Nature. Harvard University Press, Harvard (2002)

    Google Scholar 

  37. Lotka, A.J.: Elements of Physical Biology. Williams and Wilkins, London (1925)

    MATH  Google Scholar 

  38. Vano, J.A., Wildenberg, J.C., Anderson, M.B., Noel, J.K., Sprott, J.C.: Chaos in Low-Dimensional Lotka-Volterra Models of Competition. Nonlinearity 19, 2391 (2006)

    Article  ADS  MathSciNet  MATH  Google Scholar 

  39. Tenenbaum, M., Pollard, H.: Ordinary Differential Equations. Dover, New York (1985)

    MATH  Google Scholar 

  40. Chandrasekhar, S.: Hydrodynamic and Hydromagnetic Stability. Dover, New York (1981)

    MATH  Google Scholar 

  41. Mandelbrot, B.B.: Fractals: Form, Chance and Dimension. W H Freeman, New York (1977)

    MATH  Google Scholar 

  42. Feder, J.: Fractals. Plenum Press, New York (1988)

    Book  MATH  Google Scholar 

  43. Bassingthwaighte, J.B., Liebovitch, L.S., West, B.J.: Fractal Physiology. Oxford University Press, New York (1994)

    Book  Google Scholar 

  44. Gutenberg, B., Richter, C.F.: Magnitude and Energy of Earthquakes. Ann. Geofis. 9, 1 (1956)

    Google Scholar 

  45. Roberts, D.C., Turcotte, D.L.: Fractality and Self-organized Criticality of Wars. Fractals 6, 351 (1998)

    Article  Google Scholar 

  46. Frisch, U.: Turbulence: The Legacy of A. N. Kolmogorov. Cambridge University Press, Cambridge (1996)

    MATH  Google Scholar 

  47. Ma, S.K.: Modern Theory of Critical Phenomena. W.A. Benjamin, Inc., Reading (1976)

    Google Scholar 

  48. Bak, P., Tang, C., Wiesenfeld, K.: Self-organized Criticality: An Explanation of the 1/f Noise. Phys. Rev. Lett. 59, 381 (1987)

    Article  ADS  Google Scholar 

  49. Jensen, H.J.: Self-organized Criticality: Emergent Complex Behaviour in Physical and Biological Systems. Cambridge University Press, Cambridge (1998)

    Book  MATH  Google Scholar 

  50. Chang, T.: Self-organized Criticality, Multi-fractal Spectra, Sporadic Localized Reconnections and Intermittent Turbulence in the Magnetotail. Phys. Plasmas 6, 4137 (1999)

    Article  ADS  Google Scholar 

  51. Fick, A.: Uber Diffusion. Ann. Phys. 170, 59 (1885)

    Article  Google Scholar 

  52. Einstein, A.: Investigations on the Theory of Brownian Movement. Dover, New York (1956)

    MATH  Google Scholar 

  53. Metzler, R., Klafter, J.: The Random Walk’s Guide to Anomalous Diffusion: A Fractional Dynamics Approach. Phys. Rep. 339, 1 (2000)

    Article  ADS  MathSciNet  MATH  Google Scholar 

  54. Hunt, A., Ewing, R.: Percolation Theory for Flow in Porous Media. Springer, New York (2009)

    MATH  Google Scholar 

  55. Hwa, T., Kardar, M.: Avalanches, Hydrodynamics and Discharge Events in Models of Sand Piles. Phys. Rev. A 45, 7002 (1992)

    Article  ADS  Google Scholar 

  56. Dickman, R., Muñoz, M.A., Vespignani, A., Zapperi, S.: Paths to Self-organized Criticality. Braz. J. Phys. 30, 27 (2000)

    Article  ADS  Google Scholar 

  57. Boffetta, G., Carbone, V., Giuliani, P., Veltri, P., Vulpiani, A.: Power Laws in Solar Flares: Self-organized Criticality or Turbulence? Phys. Rev. Lett. 83, 4662 (1999)

    Article  ADS  Google Scholar 

  58. Sanchez, R., Newman, D.E., Carreras, B.A.: Waiting-Time Statistics of Self- Organized-Criticality Systems. Phys. Rev. Lett. 88, 068302 (2002)

    Article  ADS  Google Scholar 

  59. Sattin, F., Baiesi, M.: Self-Organized-Criticality Model Consistent with Statistical Properties of Edge Turbulence in a Fusion Plasma. Phys. Rev. Lett. 96, 105005 (2006)

    Article  ADS  Google Scholar 

  60. Mier, J.A., Sanchez, R., Newman, D.E.: Characterization of a Transition in the Transport Dynamics of a Diffusive Sandpile by Means of Recurrence Quantification Analysis. Phys. Rev. E 94, 022128 (2016)

    Article  ADS  Google Scholar 

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Appendices

Appendix 1: Fixed Points of a Dynamical System

A dynamical system is usually defined by a system of N ordinary differential equations (or simply, ODEs) that, written in matrix form, becomes:

$$\displaystyle \begin{aligned} \dot{\mathbf{x}} = \mathbf{F}(\mathbf{x}), \end{aligned} $$
(1.12)

where F is an arbitrary N-dimensional non-linear function. The fixed points of the system are given by the solutions of F(x fp) = 0, that correspond to all the time-independent solutions of the problem. At most, N different fixed points may exist. Each fixed-point can be either stable, unstable or neutral, depending on whether a small perturbation away from the fixed point is attracted back to it (i.e., stable), diverges away from it (i.e., unstable) or remains close to the fixed point without either being attracted or ejected from it (i.e., neutral).

To determine their type [39], one needs to linearize the system of ODEs in the neighbourhood of each fixed point, x fp;k , where the index k = 1, 2, ⋯ , N p , being N p  ≤ N the number of fixed points of the system. To do this, one writes x = x fp;k  + y and assumes that the norm of the perturbation |y| remains small. The behaviour of the perturbation, when advanced in time, will tell the type of the fixed point. A linear advance is sufficient. Thus, one proceeds by inserting x = x fp;k  + y into Eq. 1.12, that yields the linear evolution equation of y:

$$\displaystyle \begin{aligned} \dot{\mathbf{y}} = \left. \frac{\partial\mathbf{F}}{\partial \mathbf{x}}\right|{}_{\mathbf{ x}= \mathbf{x}_{\mathrm{fp};k}} \cdot \mathbf{y}. \end{aligned} $$
(1.13)

The matrix formed by taking partial derivatives of F and evaluating them at the fixed point is called the jacobian matrix at the fixed point. The solution of this equation is given by the exponential of the jacobian,

$$\displaystyle \begin{aligned} \mathbf{y}(t) = \exp\left( \left. \frac{\partial\mathbf{F}}{\partial \mathbf{ x}}\right|{}_{\mathbf{x}= \mathbf{x}_{\mathrm{fp};k}} (t - t_0) \right) \cdot \mathbf{ y}(t_0). \end{aligned} $$
(1.14)

Therefore, it is the eigenvalues of the jacobian at the fixed point that define the type of the fixed point. If there is any eigenvalue with a positive real part, the perturbation will grow and the solution will move away from the fixed point, and the fixed point is unstable. If all eigenvalues have negative real parts, the amplitude of the perturbation will eventually vanish, and the solution will come back to the fixed point, which is stable. If, on the other hand, all eigenvalues are purely imaginary, the norm of the perturbation remains constant over time and, although the solution never gets back to the fixed point, it does not run away from it. The fixed point is then neutral.

Problems

1.1

Predator-Prey Model: Definition

Prove that, if a term like \(\gamma n_l - \nu n_l^2\) had been used in Eq. 1.2 of the predator-prey model to account for lynx mating and overpopulation, a finite number of lynx might exist in the absence of hares, which would make no sense in the context of the model.

1.2

Lotka-Volterra Model: Periodic Orbits

  1. (a)

    Prove that the predator-prey model, if 𝜖 = 0, admits the conserved quantity:

    $$\displaystyle \begin{aligned} K(n_l, n_h):= \alpha \log(n_l) + \gamma \log(n_h) - \beta n_l - \delta n_h \end{aligned} $$
    (1.15)
  2. (b)

    Write a numerical code to plot the orbits K(n l , n h ) = K 0, for arbitrary K 0.

1.3

Predator-Prey Model: Fixed Points

With the help of the techniques discussed in Appendix 1 in this chapter,

  1. (a)

    prove that all the fixed points of the PP model are given by Eqs. 1.31.5.

  2. (b)

    show that the jacobians at the fixed points are given by:

    $$\displaystyle \begin{aligned} A: \left(\begin{array}{cc} \alpha & 0 \\ 0 & -\gamma\end{array}\right),~~~ B: \left(\begin{array}{cc} -\alpha & -\beta\alpha/\epsilon \\ 0 & \delta\alpha/\epsilon-\gamma\end{array}\right),~~ C: \left(\begin{array}{cc} -\epsilon\gamma/\delta & -\beta\gamma/\delta \\ \left(\delta\alpha - \epsilon \gamma\right)/\beta & 0 \end{array}\right) \end{aligned} $$
    (1.16)
  3. (c)

    find the eigenvalues of each jacobian.

  4. (d)

    classify the type of each fixed point.

1.4

Predator-Prey Model: Phase Space

Write a computer code that numerically integrates the dynamical system given by Eqs. 1.11.2, starting from appropriate initial conditions. Use the code to reproduce all the phase space plots shown in Fig. 1.5.

1.5

The Running Sandpile: Building of a Cellular Automata

Write a computer program that evolves in time the one-dimensional running sandpile described in Sect. 1.3.1. The output of the program should include at least the time record of the state of each cell of the sandpile (stable or unstable), its height, the total mass confined and the outflux coming out of the bottom of the pile. This program will be the basis of several exercises proposed in later chapters.

1.6

Diffusive Equation: Global Confinement Scaling

Assume a one-dimensional system of size L driven by a source density S, uniform both in time and space. If transport in the system takes place according to the diffusive equation (Eq. 1.7) with boundary conditions: n(L) = dn/dx(0) = 0, show that:

  1. (a)

    profiles are not stiff by finding the steady-state profile as a function of S and D;

  2. (b)

    the scaling of the global confinement time, τ CF , defined as the ratio of the total mass contained to the total drive strength, is τ CF  ∝ L 2;

  3. (c)

    there is no power degradation if D is independent of the external source S.

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Sánchez, R., Newman, D. (2018). Primer on Complex Systems. In: A Primer on Complex Systems. Lecture Notes in Physics, vol 943. Springer, Dordrecht. https://doi.org/10.1007/978-94-024-1229-1_1

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