Published December 2011
| Version v1
Journal article
Viscous photons in relativistic heavy ion collisions
Creators
- 1. Department of Physics, McGill University, 3600 University Street, Montreal, Quebec H3A 2T8 (Canada)
- 2. Physics Department, Bldg. 510A, Brookhaven National Laboratory, Upton, New York 11973 (United States)
Description
Theoretical studies of the production of real thermal photons in relativistic heavy ion collisions at the Relativistic Heavy Ion Collider (RHIC) are performed. The space-time evolution of the colliding system is modelled using music, a 3+1D relativistic hydrodynamic simulation, using both its ideal and viscous versions. The inclusive spectrum and its azimuthal angular anisotropy are studied separately, and the relative contributions of the different photon sources are highlighted. It is shown that the photon v2 coefficient is especially sensitive to the details of the microscopic dynamics like the equation of state, the ratio of shear viscosity over entropy density, η/s, and to the morphology of the initial state.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.84.064901;
- arXiv
- arXiv:1109.4405v3;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 84
- Journal Issue
- 6
- Journal Page Range
- p. 064901-064901.13
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43080229
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ANISOTROPY; BROOKHAVEN RHIC; DENSITY; ENTROPY; EQUATIONS OF STATE; EVOLUTION; FOUR-DIMENSIONAL CALCULATIONS; HEAVY ION REACTIONS; HYDRODYNAMIC MODEL; PHOTONS; RELATIVISTIC RANGE; SIMULATION; SPACE-TIME; SPECTRA
- Descriptors DEC
- ACCELERATORS; BOSONS; ELEMENTARY PARTICLES; ENERGY RANGE; EQUATIONS; HEAVY ION ACCELERATORS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NUCLEAR REACTIONS; PARTICLE MODELS; PHYSICAL PROPERTIES; STATISTICAL MODELS; STORAGE RINGS; THERMODYNAMIC MODEL; THERMODYNAMIC PROPERTIES
Optional Information
- Notes
- (c) 2011 American Institute of Physics