3rd Italian-Sino Italian Participants |
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Nakia Carlevaro
I.C.R.A.Net- International Center for Relativistic
Astrophysics Network, University of Rome "La Sapienza"
Title: Viscosity effects on gravitational collapse
Authors: Nakia Carlevaro, Giovanni Montani
Speaker: Nakia Carlevaro
Abstract: We analyze the effects induced by the bulk
viscosity on the dynamics associated to the extreme gravitational collapse. Aim
of the
work is to investigate whether the presence of viscous corrections to the evolution of a collapsing gas
cloud influence the top-down fragmentation process. To this end, we
generalize the approach presented by C. Hunter to include in the dynamics
of the (uniform and spherically symmetric) cloud the negative pressure
contribution associated to the bulk
viscosity phenomenology. Within the framework of a Newtonian approach, we
extend to the viscous case either the Lagrangian,
either the Eulerian
motion of the system and we treat the asymptotic evolution in correspondence to
a viscosity coefficient of the form $\zeta=\zeta_0\rho^{5/6}$
($\rho$ being the cloud density and $\zeta_0=const.$).
We show how the adiabatic-like behavior of the gas is deeply influenced by
viscous correction when its collapse reaches the extreme regime toward the
singularity. In fact, for sufficiently large viscous contributions, density
contrasts associated to a given scale of the fragmentation process acquire,
asymptotically, a vanishing behavior which prevents the formation of
sub-structures. Since in the non-dissipative case density contrasts diverge, we
can conclude that in the adiabatic-like collapse the top down mechanism of
structures formation is suppressed as soon as enough strong viscous effects are
taken into account. Such a feature is not present in the isothermal-like collapse
because the sub-structures formation is yet present and outlines the same
behavior as in the non-viscous case. We emphasize that in the adiabatic-like collapse the bulk
viscosity is also responsible for the appearance of a threshold scale beyond
which perturbations begin to increase; this issue, absent in the non-viscous
case, is equivalent to deal with a Jeans length.
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