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In a series of works by two of us, various characteristics of the glasma fromthe earliest phase of relativistic heavy-ion collisions have been studied usinga proper time expansion. These characteristics include: energy density,longitudinal and transverse pressures, collective flow, angular momentum andparameters of jet quenching. In this paper we extend the proper time intervalwhere our results are reliable by working at higher order in the expansion. Wealso generalize our previous study of jet quenching by extending ourcalculations to consider inhomogeneous glasma. Inhomogeneities are an importantaspect of physically realistic systems that are difficult to include incalculations and are frequently ignored.

Glasma properties in small proper time expansion