Interplay of shear and bulk viscosity in generating flow in heavy-ion collisions
Creators
- 1. Department of Physics, Ohio State University, Columbus, Ohio 43210 (United States)
Description
We perform viscous hydrodynamic calculations in 2+1 dimensions to investigate the influence of bulk viscosity on the viscous suppression of elliptic flow in noncentral heavy-ion collisions at Relativistic Heavy Ion Collider energies. Bulk and shear viscous effects on the evolution of radial and elliptic flow are studied with different model assumptions for the transport coefficients. We find that the temperature dependence of the relaxation time for the bulk viscous pressure, especially its critical slowing-down near the quark-hadron phase transition at Tc, partially offsets effects from the strong growth of the bulk viscosity itself near Tc and that even small values of the specific shear viscosity η/s of the fireball matter can be extracted without large uncertainties from poorly controlled bulk viscous effects.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.81.024905;
- arXiv
- arXiv:0909.1549v2;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 81
- Journal Issue
- 2
- Journal Page Range
- p. 024905-024905.12
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41115228
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- BROOKHAVEN RHIC; COMPUTERIZED SIMULATION; EVOLUTION; HADRONS; HEAVY ION REACTIONS; HYDRODYNAMIC MODEL; PHASE TRANSFORMATIONS; QUARKS; RELAXATION TIME; SLOWING-DOWN; TEMPERATURE DEPENDENCE; THREE-DIMENSIONAL CALCULATIONS; VISCOSITY
- Descriptors DEC
- ACCELERATORS; ELEMENTARY PARTICLES; FERMIONS; HEAVY ION ACCELERATORS; MATHEMATICAL MODELS; NUCLEAR REACTIONS; PARTICLE MODELS; SIMULATION; STATISTICAL MODELS; STORAGE RINGS; THERMODYNAMIC MODEL
Optional Information
- Notes
- (c) 2010 The American Physical Society