Imitation and contrarian behaviour: hyperbolic bubbles, crashes and chaos

Authors: Corcos, A1; Eckmann, J-P2; Malaspinas, A3; Malevergne, Y2; Sornette, D2

Source: Quantitative Finance, Volume 2, Number 4, August 2002 , pp. 264-281(18)

Publisher: Routledge, part of the Taylor & Francis Group

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Abstract:

Imitative and contrarian behaviours are the two typical opposite attitudes of investors in stock markets. We introduce a simple model to investigate their interplay in a stock market where agents can take only two states, bullish or bearish. Each bullish (bearish) agent polls m ‘friends' and changes her opinion to bearish (bullish) if (i) at least m rgr hb ( m rgr bh ) among the m agents inspected are bearish (bullish) or (ii) at least m rgr hh > m rgr hb ( m rgr bb > m rgr bh ) among the m agents inspected are bullish (bearish). The condition (i) ((ii)) corresponds to imitative (antagonistic) behaviour. In the limit where the number N of agents is infinite, the dynamics of the fraction of bullish agents is deterministic and exhibits chaotic behaviour in a significant domain of the parameter space {rgr hb ,rgr bh ,rgr hh ,rgr bb , m }. A typical chaotic trajectory is characterized by intermittent phases of chaos, quasi-periodic behaviour and super-exponentially growing bubbles followed by crashes. A typical bubble starts initially by growing at an exponential rate and then crosses over to a nonlinear power-law growth rate leading to a finite-time singularity. The reinjection mechanism provided by the contrarian behaviour introduces a finite-size effect, rounding off these singularities and leads to chaos. We document the main stylized facts of this model in the symmetric and asymmetric cases. This model is one of the rare agent-based models that give rise to interesting non-periodic complex dynamics in the ‘thermodynamic' limit (of an infinite number N of agents). We also discuss the case of a finite number of agents, which introduces an endogenous source of noise superimposed on the chaotic dynamics.

Document Type: Research article

DOI: http://dx.doi.org/10.1088/1469-7688/2/4/303

Affiliations: 1: CRIISEA, Université de Picardie, BP 2716, 80027, Amiens, France 2: Institute of Geophysics and Planetary Physics and Department of Earth and Space Science, University of California, Los Angeles, CA, 90095, USA 3: Dépt. de Physique Théorique, Université de Genève, CH-1211 Genève 4, Switzerland

Publication date: 2002-08-01

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