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Effect of Time Delay and Age Structure

The inclusion of age structure in RD equations has its origin in the generalization of population growth models. Age-structured models take explicitly into account that population growth is due only to adult individuals. The oldest such model is described by the McKendrick-von Foerster equation [447]  [Pg.146]

Here p, a, t) is the per capita mortality rate for individuals of age a at time t, and J(a, t) is the flux of individuals of age a at time t. Dividing by Aa and taking the limit Aa 0, we obtain the conservation equation for the density of individuals  [Pg.146]

The flux J is not a flux in space, but rather the movement of individuals in age. We assume that it is proportional to the density of individuals and some characteristic velocity of aging, J a, t) = p a, t)v(a, t). Aging is simply the passage of time V = da/dt =, and we obtain (4.107). If we also include the flux in the space due to the motion of individuals, then we obtain Metz-Diekman model [295]  [Pg.146]

Almost parallel to McKendrick, Hutchinson [215], a well-known ecologist, proposed a time-delayed version for the logistic growth equation, where the nonlinear term was delayed in time. The diffusive Hutchinson equation, also known as the delayed Fisher equation. [Pg.147]

Under certain conditions, this equation has front solutions. However, as for (4.111), loss of monotonicity occurs as the delay is increased and the front develops a prominent hump [167]. [Pg.147]


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