Zobrazeno 1 - 8
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pro vyhledávání: '"Kerstin Paech"'
Autor:
Scott Pratt, Kerstin Paech
Publikováno v:
Physical Review C. 93
Publikováno v:
International Journal of Modern Physics E. 16:1957-1963
A vigorous debate has recently concerned the quenching of jets by the expanding hot and dense medium created in high-energy nuclear collisions accompanied by Mach-cone-like structures at STAR and PHENIX.1,2 Large angle (w.r.t. the jet axis) peaks in
Autor:
Stefan Schramm, Jürgen Schaffner-Bielich, D. Zschiesche, Horst Stöcker, Adrian Dumitru, G. Zeeb, Kerstin Paech
Publikováno v:
Acta Physica Hungarica A) Heavy Ion Physics. 21:151-156
The measured particle ratios in central heavy-ion collisions are investigated within a chemical and thermal equilibrium chiral SU(3) σ−ω approach. Contrary to the commonly adopted non-interacting gas calculations, the chiral SU(3) model predicts
Autor:
Kerstin Paech
Publikováno v:
The European Physical Journal C. 33:s627-s629
The dynamical evolution of small systems undergoing a chiral symmetry breaking transition in the course of rapid expansion is discussed. The time evolution of the dynamical correlation length for trajectories passing through a second-order critical p
Autor:
Kerstin Paech
Publikováno v:
Proceedings of Critical Point and Onset of Deconfinement — PoS(CPOD2006).
Autor:
Kerstin Paech, Scott Pratt
Publikováno v:
Physical Review C. 74
A variety of physical phenomena can lead to viscous effects. Several sources of shear and bulk viscosity are reviewed with an emphasis on the bulk viscosity associated with chiral restoration and with chemical nonequilibrium. We show that in linear r
Autor:
Adrian Dumitru, Kerstin Paech
We study the hydrodynamical expansion of a hot and baryon-dense quark fluid coupled to classical real-time evolution of the long wavelength modes of the chiral field. Significant density inhomogeneities develop dynamically when the transition to the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c01b2251cbc068c3ecf27f5060e537bc
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2012:001-001
As an increasing number of well measured type Ia supernovae (SNe Ia) become available, the statistical uncertainty on w has been reduced to the same size as the systematic uncertainty. The statistical error will decrease further in the near future, a