A Tale of Tails: Photon Rates and Flow in Ultra-Relativistic Heavy Ion Collisions
arXiv:1504.07223 · doi:10.1016/j.nuclphysa.2015.11.008
Abstract
We consider the possibility that quark and gluon distributions in the medium created in high energy heavy ion collisions may be modified by a power law tail at energies much higher than the temperature. We parametrize such a tail by Tsallis distributions with an exponent motivated by phenomenology. These distributions are characterized by an effective temperature scale that we assume to evolve in time like the temperature for thermal distributions. We find that including such a tail increases the rates for photon production and significantly delays the emission times for photons of a fixed energy. We argue that these effects are sufficiently large that they should be able to account for photon yields and flow patterns seen in LHC and RHIC experiments.
18 pages, 6 figures, references added and corrected
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- Beam-energy and centrality dependence of direct-photon emission from ultra-relativistic heavy-ion collisions
- Ellipticity of photon emission from strongly magnetized hot QCD plasma
- Thermal photon radiation in high multiplicity p+Pb collisions at the Large Hadron Collider
- Prompt photon yield and elliptic flow from gluon fusion induced by magnetic fields in relativistic heavy-ion collisions
- Holographic Photon Production in Heavy Ion Collisions
- Holography for Heavy Ions Collisions at LHC and NICA
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- Impact of residual contamination on inclusive and direct photon flow
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- Prompt photon yield and coefficient from gluon fusion induced by magnetic field in heavy-ion collision