New results on Coulomb effects in meson production in relativistic heavy ion collisions
We propose a new method of investigating the space-time evolution of meson production in heavy ion collisions, by making use of spectator-induced electromagnetic (“Coulomb”) effects. The presence of two nuclear remnants (“spectator systems”) in the non-central collision generates a strong Coulomb f...
Main Authors: | , , |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2014-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20148105024 |
id |
doaj-0e5608f2fca540f2865d03982f7c561c |
---|---|
record_format |
Article |
spelling |
doaj-0e5608f2fca540f2865d03982f7c561c2021-08-02T18:36:15ZengEDP SciencesEPJ Web of Conferences2100-014X2014-01-01810502410.1051/epjconf/20148105024epjconf_meson2014_05024New results on Coulomb effects in meson production in relativistic heavy ion collisionsRybicki Andrzej0Szczurek AntoniKłusek-Gawenda Mariola1H.Niewodniczański Institute of Nuclear Physics, Polish Academy of SciencesH.Niewodniczański Institute of Nuclear Physics, Polish Academy of Sciences We propose a new method of investigating the space-time evolution of meson production in heavy ion collisions, by making use of spectator-induced electromagnetic (“Coulomb”) effects. The presence of two nuclear remnants (“spectator systems”) in the non-central collision generates a strong Coulomb field, which modifies the trajectories of charged final state hadrons. This results in charge-dependent azimuthal anisotropies in final state meson emission. In our approach, this effect can be computed numerically by means of a high-statistics Monte Carlo simulation, using the distance between the meson formation zone and the spectator system as free parameter. Our simulation correctly describes the electromagnetic effect on azimuthal anisotropies observed for π+ and π−mesons in Au+Au collisions at lower RHIC energy, known from data recently reported by the STAR Collaboration. Similarly to our earlier studies of spectator-induced electromagnetic effects, also in the present study we find that these effects offer sensitivity to the position of the meson formation zone with respect to the spectator system. Therefore, we conclude that they can serve as a new tool to investigate the space-time evolution of meson production, and the dynamics of the heavy ion collision. http://dx.doi.org/10.1051/epjconf/20148105024 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Rybicki Andrzej Szczurek Antoni Kłusek-Gawenda Mariola |
spellingShingle |
Rybicki Andrzej Szczurek Antoni Kłusek-Gawenda Mariola New results on Coulomb effects in meson production in relativistic heavy ion collisions EPJ Web of Conferences |
author_facet |
Rybicki Andrzej Szczurek Antoni Kłusek-Gawenda Mariola |
author_sort |
Rybicki Andrzej |
title |
New results on Coulomb effects in meson production in relativistic heavy ion collisions |
title_short |
New results on Coulomb effects in meson production in relativistic heavy ion collisions |
title_full |
New results on Coulomb effects in meson production in relativistic heavy ion collisions |
title_fullStr |
New results on Coulomb effects in meson production in relativistic heavy ion collisions |
title_full_unstemmed |
New results on Coulomb effects in meson production in relativistic heavy ion collisions |
title_sort |
new results on coulomb effects in meson production in relativistic heavy ion collisions |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2014-01-01 |
description |
We propose a new method of investigating the space-time evolution of meson production in heavy ion collisions, by making use of spectator-induced electromagnetic (“Coulomb”) effects. The presence of two nuclear remnants (“spectator systems”) in the non-central collision generates a strong Coulomb field, which modifies the trajectories of charged final state hadrons. This results in charge-dependent azimuthal anisotropies in final state meson emission. In our approach, this effect can be computed numerically by means of a high-statistics Monte Carlo simulation, using the distance between the meson formation zone and the spectator system as free parameter. Our simulation correctly describes the electromagnetic effect on azimuthal anisotropies observed for π+ and π−mesons in Au+Au collisions at lower RHIC energy, known from data recently reported by the STAR Collaboration. Similarly to our earlier studies of spectator-induced electromagnetic effects, also in the present study we find that these effects offer sensitivity to the position of the meson formation zone with respect to the spectator system. Therefore, we conclude that they can serve as a new tool to investigate the space-time evolution of meson production, and the dynamics of the heavy ion collision.
|
url |
http://dx.doi.org/10.1051/epjconf/20148105024 |
work_keys_str_mv |
AT rybickiandrzej newresultsoncoulombeffectsinmesonproductioninrelativisticheavyioncollisions AT szczurekantoni newresultsoncoulombeffectsinmesonproductioninrelativisticheavyioncollisions AT kłusekgawendamariola newresultsoncoulombeffectsinmesonproductioninrelativisticheavyioncollisions |
_version_ |
1721227923570032640 |