A probabilistic analysis of the Fermi paradox in terms of the Drake
  formula: the role of the L factor
  In evaluating the number of technological civilizations N in the Galaxy
through the Drake formula, emphasis is mostly put on the astrophysical and
biotechnological factors describing the emergence of a civilization and much
less on its the lifetime, which is intimately related to its demise. It is
argued here that this factor is in fact the most important regarding the
practical implications of the Drake formula, because it determines the maximal
extent of the "sphere of influence" of any technological civilization. The
Fermi paradox is studied in the terms of a simplified version of the Drake
formula, through Monte Carlo simulations of N civilizations expanding in the
Galaxy during their space faring lifetime L. In the framework of that scheme,
the probability of "direct contact" is determined as the fraction of the
Galactic volume occupied collectively by the "spheres of influence" of N
civilizations. The results of the analysis are used to determine regions in the
parameter space where the Fermi paradox holds. It is argued that in a large
region of the diagram the corresponding parameters suggest rather a "weak"
Fermi paradox. Future research may reveal whether a "strong" paradox holds in
some part of the parameter space. Finally, it is argued that the value of N is
not bound by N=1 from below, contrary to what is usually assumed, but it may
have a statistical interpretation.
