BES v3 paper proposal

Title:
Beam Energy Dependence of the Third Harmonic of Azimuthal Correlations in Au+Au Collisions at RHIC

PA's: Paul Sorensen, Niseem Magdy, Yadav Pandit, Navneet Kumar Pruthi, Hui Wang and Liao Song.

Target Journal: PRL

Responses to the referrees: https://drupal.star.bnl.gov/STAR/system/files/BESv3Responses.pdf
Latest Draft for resubmission: 
https://drupal.star.bnl.gov/STAR/system/files/besv3prl_sub_1.pdf
Submitted to the journal: 
https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v8.pdf
Second Draft After Review: 
https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v7.pdf
Draft After Collaboration Review: 
https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v6.pdf
Responses to Insitution Comments: UCLA, RICE, CCNU, LBNL
Draft for Collaboration Review: https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v5.pdf
Previous Drafts: https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v4.pdf
Previous Drafts: https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v3.pdf
Previous Drafts: https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v2.pdf
Previous Drafts: https://drupal.star.bnl.gov/STAR/system/files/besv3prl_v1.pdf

Updated Analysis Note: https://drupal.star.bnl.gov/STAR/system/files/BES_v3_AnalysisNote_2.pdf

Abstract: 

We present results from a harmonic decomposition of two-particle
azimuthal correlations measured in $Au+Au$ collisions for energies
ranging from $\sqrt{s_{NN}}=7.7$ GeV to 200 GeV. The dependence of the
third harmonic $v_3^2\{2\}=\langle cos(\phi_1-\phi_2)\rangle$ is
studied as a function of the longitudinal angle between the particle
pairs $\Delta\eta = \eta_1-\eta_2$. $v_3$ is directly related to the
large $\Delta\eta$ ridge correlations and has been shown in models to
be sensitive to the existence of a low viscosity Quark Gluon Plasma
phase. For sufficiently central collisions, $v_3^2\{2\}$ persist even
down to energies of 7.7 and 11.5 GeV. In peripheral collisions at
these low energies however, no jet-like correlations are observed and
$v_3^2\{2\}$ is consistent with zero. This observation is consistent
with the disappearance of the Quark Gluon Plasma in small systems at
low energies. When scaled by multiplicity, $v_3^2\{2\}$ shows a
minimum near $\sqrt{s_{NN}}=14--20$ GeV, a feature not present in any
current models of heavy-ion collisions.
 

Figure 1:


Figure 2: 

Figure 3:

Figure 4:

Conclusion:

We presented measurements of the collision energy dependence of
\vthree in Au+Au collisions for energies ranging from
$\sqrt{s_{_{NN}}} = $ 7.7 to 200 GeV. Model calculations have shown
that \vthree is particularly sensitive to the presence of a low
viscosity plasma phase in the collision evolution: the smaller scale
geometry fluctuations that lead to \vthree are lost without this phase
while $v_{2}$ can be established over a longer period in a higher
viscosity phase. The conversion of geometry fluctuations in the
initial state have been found to provide a simple explanation for
\vthree and the corresponding ridge structure. By studying the
$\Delta\eta$ dependence of \vthree, we find that for sufficiently
central collisions (\npart $>50$), the ridge and \vthree persists down to
the lowest energies studied. For more peripheral collisions however,
the ridge correlation appears to be entirely abscent for \npart $<50$,
consistent with the disappearance of the Quark Gluon Plasma in small
systems at low energies. When comparing \vthree at RHIC and the LHC,
the much larger multiplicities at the higher energies lead to a much
larger \vthree. When scaled by multiplicity however, $v_3^2\{2\}$
shows a minimum in the range $\sqrt{s_{NN}}=14-20$ GeV. This feature
is not present in any current models of heavy-ion collisions and could
indicate a non-monotonic trend in the pressure of the system. Such a
provacative conclusion however requires a deeper investigation of the
complicated dynamics in that energy range. Such an investigation is
the goal of both major theory and experimental efforts within the
communuity including a second phase of the beam energy scan at RHIC
focusing on collecting larger data samples at energies below 20 GeV.
 

Supporting material:

https://drupal.star.bnl.gov/STAR/system/files/pwc_preview_topics.pdf

https://drupal.star.bnl.gov/STAR/system/files/sorensen_14.5GeV_update.pdf

https://drupal.star.bnl.gov/STAR/system/files/sorensen_bulkcorr_july16_2014.pdf

https://drupal.star.bnl.gov/STAR/system/files/sorensen_bulkcorr_05_28_2014.pdf

https://drupal.star.bnl.gov/STAR/system/files/sorensen_BES_06_23_2014.pdf

A quote from http://arxiv.org/pdf/1310.1764.pdf relevant to this paper:

"the scaled v3 points over several collision energies and centrality classes form an uniform function of the hydro duration thydro, whereas for the elliptic flow the relation is distorted by the transport dynamics. Thus, compared to v2, the triangular flow provides a clearer signal for the formation of (near-)ideal fluid in heavy ion collisions."