Dissipative processes in relativistic fluids are known to be important in the
analyses of the hot QCD matter created in high-energy heavy-ion collisions. In
this work, I consider dissipative corrections to energy and conserved charge
densities, which are conventionally assumed to be vanishing but could be
finite. Causal dissipative hydrodynamics is formulated in the presence of those
dissipative currents. The relation between hydrodynamic stability and transport
coefficients is discussed. I then study their phenomenological consequences on
the observables of heavy-ion collisions in numerical simulations. It is shown
that particle spectra and elliptic flow can be visibly modified.Comment: 10 pages, 5 figures; title changed, references added, conclusions
unchange