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Extinction of metastable stochastic populations

Source: Phys. Rev. E 81, 021116 (2010); doi:10.1103/PhysRevE.81.021116

Published 9 February 2010

PACS
  • 02.50.Ga
    Markov processes
  • 87.23.Cc
    Population dynamics and ecological pattern formation
  • YEAR: 2010
PUBLICATION DATA
ISSN:
1553-9628 (online)
Publisher:
AIP is a member of CrossRef APS
Michael Assaf and Baruch Meerson
Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
We investigate the phenomenon of extinction of a long-lived self-regulating stochastic population, caused by intrinsic (demographic) noise. Extinction typically occurs via one of two scenarios depending on whether the absorbing state n=0 is a repelling (scenario A) or attracting (scenario B) point of the deterministic rate equation. In scenario A the metastable stochastic population resides in the vicinity of an attracting fixed point next to the repelling point n=0. In scenario B there is an intermediate repelling point n=n1 between the attracting point n=0 and another attracting point n=n2 in the vicinity of which the metastable population resides. The crux of the theory is a dissipative variant of WKB (Wentzel-Kramers-Brillouin) approximation which assumes that the typical population size in the metastable state is large. Starting from the master equation, we calculate the quasistationary probability distribution of the population sizes and the (exponentially long) mean time to extinction for each of the two scenarios. When necessary, the WKB approximation is complemented (i) by a recursive solution of the quasistationary master equation at small n and (ii) by the van Kampen system-size expansion, valid near the fixed points of the deterministic rate equation. The theory yields both entropic barriers to extinction and pre-exponential factors, and holds for a general set of multistep processes when detailed balance is broken. The results simplify considerably for single-step processes and near the characteristic bifurcations of scenarios A and B. ©2010 The American Physical Society
History: Received 1 July 2009; published 9 February 2010
Permalink: http://link.aps.org/abstract/PRE/v81/e021116
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