Anomalous mass dependence of radiative quark energy loss in a finite-size quark-gluon plasma
arXiv:0907.1918 · doi:10.1134/S0021364009160048
Abstract
We demonstrate that for a finite-size quark-gluon plasma the induced gluon radiation from heavy quarks is stronger than that for light quarks when the gluon formation length becomes comparable with (or exceeds) the size of the plasma. The effect is due to oscillations of the light-cone wave function for the in-medium transition. The dead cone model by Dokshitzer and Kharzeev neglecting quantum finite-size effects is not valid in this regime. The finite-size effects also enhance the photon emission from heavy quarks.
8 pages, 3 figures
References in corpus (7)
- Heavy flavor in heavy-ion collisions at RHIC and RHIC II
- Parton energy loss in an expanding quark-gluon plasma: Radiative vs collisional
- Jet quenching with running coupling including radiative and collisional energy losses
- High-energy gluon bremsstrahlung in a finite medium: harmonic oscillator versus single scattering approximation
- A new correlation method to identify and separate charm and bottom production processes at RHIC
- Failure of the collinear expansion in calculation of the induced gluon emission
- Collinear Photon Emission from the Quark-Gluon Plasma: The Light-Cone Path Integral Formulation
Cited by in corpus (6)
- The quark-gluon medium
- Dead-cone searches in heavy-ion collisions using the jet tree
- Updated analysis of jet quenching at RHIC and LHC within the light cone path integral approach
- Heavy Quark Energy Loss in the Quark-Gluon Plasma in the Moller theory
- Heavy Quark Radiation in the Quark-Gluon Plasma in the Moliere Theory: Angular Distribution of the Radiation
- Jet quenching for heavy flavors in and collisions