Emission angle dependent HBT at RHIC and beyond

Abstract

We study the geometrical features of non-central heavy ion collisions throughout their dynamical evolution from equilibration to thermal freeze-out within a hydrodynamic picture. We discuss resulting observables, in particular the emission angle dependence of the HBT radii and the relation of these oscillations to the geometry at the final stage.

4 pages, 4 figures, proceedings for Quark Matter 2002

References in corpus (8)

• Radial and elliptic flow at RHIC: further predictions
• Elliptic flow at SPS and RHIC: from kinetic transport to hydrodynamics
• Saturation of Elliptic Flow and the Transport Opacity of the Gluon Plasma at RHIC
• Early thermalization at RHIC
• Partonic effects on the elliptic flow at relativistic heavy ion collisions
• Centrality dependence of multiplicity, transverse energy, and elliptic flow from hydrodynamics
• Is early thermalization achieved only near midrapidity at RHIC ?
• Emission angle dependent pion interferometry at RHIC and beyond

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• Heavy Ion Collisions with Transverse Dynamics from Evolving AdS Geometries
• Scaling of elliptic flow in heavy-ion collisions with the number of constituent quarks in a transport model
• Collective Flow of QCD Matter: a Historical Introduction
• Insight from elliptic flow of open charm mesons using quark coalescence model at RHIC and LHC energies
• Critical Opacity - a possible explanation of the fast thermalisation times seen in RHIC experiments
• Using the $\varphi$-meson elliptic flow to map the strength of partonic interaction
• Early time behavior of spatial and momentum anisotropies in kinetic theory across different Knudsen numbers
• Early time behavior of spatial and momentum anisotropies in a kinetic approach to nuclear collisions
• Relativistic Nucleus-Nucleus Collisions and the QCD Matter Phase Diagram
• Probing the QCD phase diagram with the measurements of $\varphi$-meson production and elliptic flow in the heavy-ion collision at STAR
• Measurements of $D_S^{\pm }$-meson production in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV in STAR