Speaker
Mauricio Hippert
(Brazilian Center for Research in Physics)
Description
We clarify how the weak-interaction-driven bulk viscosity ζ and the bulk relaxation time $\tau_\Pi$ of neutrino-transparent $npe$ matter depend on the nuclear symmetry energy. We show that, at saturation density, the equation-of-state dependence of these transport quantities is fully determined by the experimentally constrained nuclear symmetry energy S and its slope L. Variations of L within current experimental uncertainties can change the bulk viscosity by orders of magnitude. This suggests that dissipative effects encoded in the gravitational-wave signatures of binary neutron star inspirals may help constrain nuclear symmetry energy properties.
Author
Mauricio Hippert
(Brazilian Center for Research in Physics)