22 research outputs found

    Small-xx evolution of jet quenching parameter

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    Concept of transverse deflection probability of a parton that travels through strongly interacting medium, recently introduced by D'Eramo, Liu and Rajagopal, have been used to derive high energy evolution equation for the jet quenching parameter in stochastic multiple scatterings regime. Jet quenching parameter, q^(x){\hat q}(x), appears to evolve with xx, with an exponent 0.9αˉs0.9{\bar \alpha}_s, which is slightly less than that of xG(x)x {\cal G} (x) where G(x){\cal G} (x) is the gluon distribution function.Comment: Version accepted in Phys. Lett.

    Soft Gluon Radiation off Heavy Quarks beyond Eikonal Approximation

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    We calculate the soft gluon radiation spectrum off heavy quarks (HQs) interacting with light quarks (LQs) beyond small angle scattering (eikonality) approximation and thus generalize the dead-cone formula of heavy quarks extensively used in the literatures of Quark-Gluon Plasma (QGP) phenomenology to the large scattering angle regime which may be important in the energy loss of energetic heavy quarks in the deconfined Quark-Gluon Plasma medium. In the proper limits, we reproduce all the relevant existing formulae for the gluon radiation distribution off energetic quarks, heavy or light, used in the QGP phenomenology

    Soft gluon emission off a heavy quark revisited

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    An improved generalized suppression factor for gluon emission off a heavy quark is derived within perturbative QCD, which is valid for the full range of rapidity of the radiated gluon and also has no restriction on the scaled mass of the quark with its energy. In the appropriate limit it correctly reproduces the usual dead cone factor in the forward rapidity region. On the other hand, this improved suppression factor becomes close to unity in the backward direction. This indicates a small suppression of gluon emission in the backward region, which should have an impact on the phenomenology of heavy quark energy loss in the hot and dense matter produced in ultra-relativistic heavy-ion collisions.Comment: A portion of the discussion and Fig. 3 changed in the text; A little change in the abstract; Version accepted in PR
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