“…[3] The introduction of a governing law guarantees a finite energy flux at the rupture tip and makes it possible to simulate the traction evolution on the fault surface as it results from the inclusion of the various chemical and physical mechanisms which can strongly affect the traction evolution and ultimately the earthquake dynamics; the thermal weakening [Rice, 2006;Bizzarri, 2009], the pore fluid pressurization [Lachenbruch and Sass, 1980;Bizzarri and Cocco, 2006;Brantut et al, 2010], the powder lubrication due to nanograins [Han et al, 2010Reches and Lockner, 2010], the silica gel formation [Goldsby and Tullis, 2002], the thermal decomposition [Han et al, 2007;Brantut et al, 2008], the frictional melting [e.g., Jeffreys, 1942;Sibson, 1975;Bizzarri, 2011a], the acoustic fluidization [Melosh, 1996], the normal interface vibrations [Brune et al, 1993], etc. The relative importance of these different dissipative mechanisms can depend on the presence of fluids in the seismic structure, its hydraulic properties and its maturity, the level of development of the fault fabric, the rock type, etc.…”