The low and intermediate mass dilepton and photon results

The low and intermediate mass dilepton and photon results

Lijuan Ruan Physics Department, Brookhaven National laboratory, Upton NY 11973
Abstract

I summarize and discuss some of the experimental results on the low and intermediate mass dileptons and direct photons presented at Quark Matter 2014.

keywords:
vector meson in-medium modification, chiral symmetry restoration, Quark-Gluon Plasma thermal radiation, dileptons, thermal photons

1 Introduction

Ultra-relativistic heavy ion collisions provide a unique environment to study the properties of strongly interacting matter at high temperature and high energy density starwhitepaper (). Leptons and photons are penetrating probes of the hot, dense medium since they are not affected by the strong interaction and therefore they can probe the whole evolution of the collision.

In the low invariant mass range of produced lepton pairs ( GeV/), we can study vector meson in-medium properties through their dilepton decays, where modifications of mass and width of the spectral functions observed may relate to the possibility of chiral symmetry restoration dilepton (); dileptonII (). The dilepton spectra in the intermediate mass range ( GeV/) are directly related to thermal radiation of the Quark-Gluon Plasma (QGP) dilepton (); dileptonII (). However, contributions from other sources have to be obtained experimentally. Such contributions include background pairs from correlated open heavy flavor decays ( or ). In addition, photons in the low transverse momentum range GeV/ are used to study thermal radiation from QGP and hadronic gas.

In this article, I will summarize the results from NA60, PHENIX, STAR, and ALICE on thermal dileptons and photons presented at Quark Matter 2014.

2 Dileptons

2.1 Results on and collisions

At this conference, the STAR Collaboration presented their 200 GeV reference measurement using high statistics 2012 data Yang:14 (). The cocktail simulation with expected hadronic contribution is consistent with the data. A similar conclusion holds for collisions at LHC energies Kohler:14 (). In addition, in d+Au and p+Pb collisions, hadronic cocktails are also found to be consistent with the measurements, indicating that there is no medium radiation observed there Kohler:14 (); Dion:14 ().

2.2 Thermal dileptons in the low mass region

At the SPS, the low mass dilepton enhancements in the CERES data  ceres () and in the NA60 data na60 (); na60:10 () indicate substantial medium effects on the -meson spectral function. The precise NA60 measurement of the low mass enhancement provides a decisive discrimination between the dropping-mass scenario dropmass () and the massively broadened spectral function massbroaden (). The latter one was found to be able to describe the data consistently.

At RHIC, the PHENIX experiment observed a significant enhancement in the data above the expectation from hadronic sources for GeV/ and GeV/ in 200 GeV Au+Au collisions lowmass (). Models rapp:09 (); PSHD:12 (); USTC:12 () that successfully describe the SPS dilepton data, fail to describe the PHENIX data. After the Time-of-Flight detector upgrade, STAR reported the dielectron spectra in 200 GeV Au+Au collisions at QM2011 and the low mass excess was not as significant as what PHENIX observed in 0-80% and 0-10% collisions ppdilepton:12 (); Jie:11 (). Further comparisons point to the fact that the discrepancy between STAR and PHENIX comes from 0-20% central collisions only GaleRuan:12 ().

Figure 1: (Color Online) Dielectron spectra in Au+Au collisions from 19.6, 27, 39, 62.4, and 200 GeV from STAR Huck:14 (). In each panel, the ”cocktail” represents the expected hadronic contribution Huck:14 (); stardielectron:14 () while ”in-medium” and ”QGP” represent contributions from a broadened spectral function and QGP thermal radiation, respectively rapp:09 (). The sum of the ”cocktail”, ”in-medium”, and ”QGP” is shown as the solid curve on top of the data points.

At Quark Matter 2012, PHENIX reported the dielectron results from the Hadron Blind Detector from 20-92% Au+Au collisions at 200 GeV, which are consistent with the data in the corresponding centralities in the previous publication phenixdielectron:12 (). STAR reported the dielectron spectra from 19.6, 39, and 62.4 GeV Au+Au collisions geurts:12 (); huang:12 (). See also Ref. GaleRuan:12 ().

At this conference, STAR reported the dielectron spectrum from 27 GeV Au+Au collisions Huck:14 (). The 200 GeV Au+Au results were finalized stardielectron:14 (). In addition, the differential measurements were also shown in Au+Au collisions at 19.6, 27, 39, and 62.4 GeV Huck:14 (). A broadened spectral function rapp:09 (), which describes SPS dilepton data, consistently accounts for the STAR low mass excess in Au+Au collisions at 19.6, 27, 39, 62.4, and 200 GeV, as shown in Fig. 1. It also describes the dependence of low mass excess up to 2 GeV/ for all these collision energies Huck:14 (). In addition, the excess dielectron mass spectrum in the mass region 0.3-0.76 GeV/ in 200 GeV Au+Au collisions is found to follow dependence, where is the number of participant nucleons in a collision stardielectron:14 ().

2.3 Thermal dileptons in the intermediate mass region

Dilepton spectra in the intermediate mass range are directly related to the thermal radiation of the QGP dilepton (); dileptonII (). Thanks to the fact, that the charm cross section at 17.3 GeV is small and with a vertex detector to reject the charm background, NA60 presented the unprecedented excess dimuon mass spectrum in In+In collisions, as shown in Fig. 2. From its intermediate mass region, one can obtain the temperature of the emitting source. In addition, more differential results such as the , azimuthal angle, and polar angle dependences of the excess dimuons in different mass regions were obtained na60:10 (). Based on those precise measurements, it was identified that the excess dimuons in the intermediate mass region comes from the early emission from the hot, dense medium.

Figure 2: (Color Online) Acceptance-corrected excess dimuon invariant mass spectrum in In+In collisions at 17.3 GeV. Model comparisons are also shown na60:10 ().

At RHIC, with the data sets currently available, it is difficult to measure correlated charm contribution or QGP thermal radiation in the intermediate mass region. At RHIC energies, there is so far no clear statement about thermal radiation in the intermediate mass region. The recent STAR measurements in 200 GeV Au+Au indicate that the trend there could be slightly different in 0-80% and 0-10% collisions stardielectron:14 (). However, the results are not precise enough to draw a conclusion. The recent detector upgrade with the Heavy Flavor Tracker at STAR, completed in 2014, will provide precise charm cross section measurements hft (). This will help to understand heavy quark dynamics in the medium and constrain model inputs to calculate dilepton mass spectra from correlated charm contribution. However the measurements of correlations will still be challenging if not impossible. An independent approach is planned with the Muon Telescope Detector upgrade (MTD) starmtdproposal (), which was completed in 2014. The correlations will measure the contribution from heavy flavor correlations to the dielectron or dimuon continuum with the 200 GeV Au+Au data taken in 2014 starmtdproposal (); Ruan:12 (). This will allow to access the thermal radiation in the intermediate mass region.

In addition, the Beam Energy Scan Phase II at RHIC in 2018-2019 will enable to collect sufficient data in Au+Au collisions from 7.7 to 19.6 GeV besII:14 (). The charm cross section is significantly reduced at lower energies. One would like to see whether at some collision energies the transition from low to intermediate dilepton mass region would be smooth, which would imply chiral symmetry restoration.

3 Thermal photon measurements

3.1 Review of previous results

Photons at GeV/ are used to study thermal radiation from QGP and hadronic medium. For GeV/, PHENIX measured direct photon yields from dielectron measurements and found an excess in 0-20% Au+Au over at GeV, exponential in with the inverse slope parameter 221 MeV thermalphoton (). At LHC, an excess of direct photon yield in 0-40% Pb+Pb collisions above was reported at 2.76 TeV, exponential in with the inverse slope parameter 304 MeV ALICEphoton (). If indeed the excess is from the QGP phase, the measurements at RHIC and LHC would indicate that the initial temperature of the QGP evolution is as high as 300-600 MeV thermalphoton ().

On the other hand, of direct photons has been found to be substantial in the range GeV/ in central 0-20% Au+Au collisions at GeV photonv2 (). Model calculations Rupa:09 () for QGP thermal photons in this kinematic region significantly under-predict the observed , while if a significant contribution from the hadronic sources at later stages is added, the excess of the spectra and the observed at GeV/ are described reasonably well rapp:11 (). In addition, ALICE reported that significant is observed for direct photons, though the systematic uncertainties are large ALICEv2:12 ().

3.2 Review of new results

Figure 3: (Color Online) Direct photon yields as a function of in 0-80% Au+Au from STAR, 0-92% Au+Au from PHENIX, and from PHENIX at 200 GeV Yang:14 ().
Figure 4: (Color Online) The of direct photons and pions in Au+Au collisions at 200 GeV Mizuno:14 ().

At this conference, STAR presented their first direct photon yields from dielectron measurements and found an excess in 0-80% Au+Au over at GeV for GeV/ Yang:14 (). For GeV/, the yields are consistent with the number of binary scaled measurements. The lack of the meson measurements at GeV/ leads to large uncertainties in the hadronic cocktail components. This leads to large systematic uncertainties (greater than 50%) in the direct virtual photon yields for GeV/. Within these uncertainties, the STAR measurements are consistent with the published PHENIX results thermalphoton (), as shown in Fig. 3.

Using external conversion technique, PHENIX measured the direct photon yields down to of 0.4 GeV/. Excess yields in Au+Au over are observed at GeV, which are exponential in with slope parameters independent of centrality Mizuno:14 (). It is found that the excess follows dependence. In addition, PHENIX observed that direct photons have a significant triangular flow , similar to that of pions, as shown in Fig. 4.

In addition, ALICE reported that they were doing critical assessments for the measurements of spectrum and of direct photons in Pb+Pb collisions at 2.76 TeV. Conclusions should be drawn after assessments are completed Bock:14 ().

3.3 The future improvements

The excess spectrum of thermal photon in A+A collisions depends on the measurements of the direct photon spectra in A+A and collisions. The future improvements thus come from those from A+A and . In particular, for A+A collisions, the measurement using internal conversion method would benefit from the precise measurement at 2 GeV/, while that using external conversion would benefit from more precise and measurements. In collisions, the measurement of direct photon at 2 GeV/ has large uncertainties at RHIC and does not exist at LHC. Future precise measurement is critical to get a solid physics picture of the excess yield.

In addition, it has been proposed that dilepton measurements as a function of in different mass regions would allow to probe the properties of medium from a hadron-gas-dominated to a QGP-dominated scenario Gale:07 (). At the previous and this Quark Matter, STAR reported the dielectron measurements from 200 GeV Au+Au collisions. Within uncertainties, the data are compatible with known hadronic sources without QGP or hadron gas thermal radiation stardielectronv2 (). Much more data are needed for the dielectron measurement to provide additional sensitivity to study the thermal radiation from the different phases in addition to the correlation measuring the charm correlation contribution. In the future, dimuon might provide an alternative approach considering the trigger capabilities starmtdproposal ().

4 Perspectives

In QCD vacuum, the quark condensate has non-zero expectation value, which leads to spontaneous chiral symmetry breaking. This generates 99% of the visible mass in the universe. In addition, the mass degeneracy between chiral partners, like and mesons, is lifted. When the temperature and density is high enough, theoretical calculations predict that the chiral symmetry will be restored. The mass difference between and will disappear. Experimentally, there are many efforts since decades to search for the signature of the chiral symmetry restoration. Since it is very difficult and challenging to measure , the experimental efforts goes to the study of the modification of spectral function. An observed broadened and structureless spectral function would imply chiral symmetry restoration.

Figure 5: (Color Online) (top panel) The ratios as a function of energy in Au+Au collisions together with the excess yield predictions from a model besII:14 (). (bottom panel): The integral dielectron excess yields within STAR acceptance in the mass region 0.3-0.7 GeV/ normalized by mid-rapidity pion yields in Au+Au collisions Huck:14 (). Data are measurements from 19.6 to 200 GeV. The rising line represents model expectations and the grey band is for the extrapolations assuming the normalized excess yields do not change down to 7.7 GeV.

It is found that a broadened spectral function rapp:09 (), describes SPS dilepton data, consistently accounts for the STAR low mass excess at 19.6, 27, 39, 62.4, and 200 GeV. Furthermore, it is found that coupling to baryons plays an essential role in the modification of spectral function in the hot, dense medium. The total baryon density, derived from the ratios, does not change significantly from 17.3 to 200 GeV, as shown in the top panel of Fig. 5. Therefore, the measurements from 17.3 to 200 GeV probe the temperature and system evolution dependence. Figure 5 (bottom panel) shows the integral dielectron excess yields within STAR acceptance in the mass region 0.3-0.7 GeV/ normalized by mid-rapidity pion yields. No significant energy dependence of the normalized excess yields from 19.6 to 200 GeV is observed Huck:14 ().

In order to be sensitive to the total baryon density effect, one need to have measurements at lower energies. At 7.7 GeV, it is found that the total baryon density increases by a factor of two, as indicated in the top panel of Fig. 5. Current data at 7.7 and 11.5 GeV at RHIC are not sufficient for dilepton analysis. The future measurements from the Beam Energy Scan Phase II at RHIC, will map out the dependence of modified spectral function on the total baryon density from 7.7 to 19.6 GeV Au+Au collisions besII:14 (). The grey band shown in the bottom panel of Fig. 5 represents the precision projection if the normalized excess yield does not change. If it increases when the energy decreases as predicted by models, the uncertainties down to 7.7 GeV might be smaller. In addition, there exists a proposal of a new NA experiment at SPS to measure the excess dimuon mass spectra precisely at 6-20 GeV Usai:14 (). These, together with the future measurements from ALICE at LHC Kohler:14 (), HADES at SIS18 HADES:14 (), and CBM at SIS100 FAIR:14 () will provide a unique opportunity to study chiral symmetry restoration.

5 Conclusions

This edition of the Quark Matter conferences has seen a stream of results unprecedented in their quality and in their quantity, being presented by the experimental collaborations working at RHIC and at the LHC. Thermal photon and dilepton measurements from a broad beam energy range enable us to study the fundamental properties of QGP, of chiral symmetry restoration, and will provide stringent tests of the dynamical evolution scenarios of relativistic nuclear collisions.

Acknowledgment The work of of LR is supported in part by the U. S. Department of Energy under Contract No. DE-AC02-98CH10886 and under Early Career Research Program Funding Award No. FWP2013-BNL-PO143.

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