scholarly journals Nuclear modification of full jet energy and jet structure at the LHC energies

2021 ◽  
Author(s):  
NingBo Chang ◽  
Guang-You Qin ◽  
Yasuki Tachibana
2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
A. Andronic ◽  
J. Honermann ◽  
M. Klasen ◽  
C. Klein-Bösing ◽  
J. Salomon

Abstract In this paper we present a study of in-medium jet modifications performed with JEWEL and PYTHIA 6.4, focusing on the uncertainties related to variations of the perturbative scales and nuclear parton distribution functions (PDFs) and on the impact of the initial and crossover temperature variations of the medium. The simulations are compared to LHC data for the jet spectrum and the nuclear modification factor. We assess the interplay between the choice of nuclear PDFs and different medium parameters and study the impact of nuclear PDFs and the medium on the jet structure via the Lund plane.


1991 ◽  
Author(s):  
ELLEN LONGMIRE ◽  
JOHN EATON ◽  
CHRISTOPHER ELKINS
Keyword(s):  

2020 ◽  
Vol 15 (S359) ◽  
pp. 280-282
Author(s):  
Gustavo Amaral Lanfranchi ◽  
Anderson Caproni ◽  
Jennifer F. Soares ◽  
Larissa S. de Oliveira

AbstractThe gas evolution of a typical Dwarf Spheroidal Galaxy is investigated by means of 3D hydrodynamic simulations, taking into account the feedback of type II and Ia supernovae, the outflow of an Intermediate Massive Black Hole (IMBH) and a static cored dark matter potential. When the IMBH’s outflow is simulated in an homogeneous medium a jet structure is created and a small fraction of the gas is pushed away from the galaxy. No jet structure can be seen, however, when the medium is disturbed by supernovae, but gas is still pushed away. In this case, the main driver of the gas removal are the supernovae. The interplay between the stellar feedback and the IMBH’s outflow should be taken into account.


2008 ◽  
Vol 5 (5) ◽  
pp. 447-455 ◽  
Author(s):  
I. A. Golutvin ◽  
A. V. Zarubin ◽  
O. L. Kodolova ◽  
V. F. Konoplyanikov ◽  
A. L. Ul’yanov ◽  
...  

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