000071329 001__ 71329
000071329 005__ 20170403114019.0
000071329 0247_ $$2DOI$$a10.1140/epja/i2016-16217-8
000071329 035__ $$9INSPIRETeX$$aSenger:2016wfb
000071329 100__ $$aSenger, P.$$uDarmstadt, GSI$$vGSI Helmholtzzentrum f ̈ ur Schwerionenforschung, D-64291 Darmstadt, Germany
000071329 245__ $$aNuclear matter physics at NICA
000071329 260__ $$c2016-08-12
000071329 300__ $$a8
000071329 520__ $$aThe exploration of the QCD phase diagram is one of the most exciting and challenging projects of modern nuclear physics. In particular, the investigation of nuclear matter at high baryon densities offers the opportunity to find characteristic structures such as a first-order phase transition with a region of phase coexistence and a critical endpoint. The experimental discovery of these prominent landmarks of the QCD phase diagram would be a major breakthrough in our understanding of the properties of nuclear matter. Equally important is the quantitative experimental information on the properties of hadrons in dense matter which may shed light on chiral symmetry restoration and the origin of hadron masses. Worldwide, substantial efforts at the major heavy-ion accelerators are devoted to the clarification of these fundamental questions, and new dedicated experiments are planned at future facilities like CBM at FAIR in Darmstadt and MPD at NICA/JINR in Dubna. In this article the perspectives for MPD at NICA will be discussed.
000071329 65017 $$2INSPIRE$$aTheory-Nucl
000071329 65017 $$2INSPIRE$$aExperiment-Nucl
000071329 695__ $$2INSPIRE$$a* Automatic Keywords *
000071329 695__ $$2INSPIRE$$9bibclassify$$aquantum chromodynamics: critical phenomena
000071329 695__ $$2INSPIRE$$9bibclassify$$aaccelerator: heavy ion
000071329 695__ $$2INSPIRE$$9bibclassify$$abaryon: density: high
000071329 695__ $$2INSPIRE$$9bibclassify$$asymmetry: chiral
000071329 695__ $$2INSPIRE$$9bibclassify$$ahadron: mass
000071329 695__ $$2INSPIRE$$9bibclassify$$anuclear matter
000071329 695__ $$2INSPIRE$$9bibclassify$$aNICA
000071329 695__ $$2INSPIRE$$9bibclassify$$anuclear physics
000071329 695__ $$2INSPIRE$$9bibclassify$$aDubna Lab
000071329 695__ $$2INSPIRE$$9bibclassify$$astructure
000071329 695__ $$2INSPIRE$$9bibclassify$$aCBM
000071329 773__ $$c217$$n8$$pEur.Phys.J.$$vA52$$y2016
000071329 909CO $$ooai:inspirehep.net:1517258$$pINSPIRE:HEP
000071329 980__ $$aPublished
000071329 980__ $$aciteable
000071329 980__ $$aHEP
000071329 980__ $$aCORE
000071329 999C5 $$0856295$$hK. Fukushima, T. Hatsuda$$o1$$sRept.Prog.Phys.,74,014001$$y2011
000071329 999C5 $$01206890$$hF. Becattini et al.$$o2$$sPhys.Rev.Lett.,111,082302$$y2013
000071329 999C5 $$0855185$$hS. Borsanyi et al.$$o3$$sJHEP,1009,073$$y2010
000071329 999C5 $$0944699$$hA. Basavov et al.$$o4$$sPhys.Rev.,D85,054503$$y2012
000071329 999C5 $$0731401$$hY. Aoki et al.$$o5$$sNature,443,675$$y2006
000071329 999C5 $$01250016$$hJ. Luecker et al.$$o6$$rarXiv:1308.4509 [hep-ph]
000071329 999C5 $$0753223$$hL. McLerran, R.D. Pisarski$$o7$$sNucl.Phys.,A796,83$$y2007
000071329 999C5 $$hI.C. Arsene et al.$$o8$$sPhys.Rev.,C75,24902$$y2007
000071329 999C5 $$01246889$$hM. Orsaria et al.$$o9$$sPhys.Rev.,C89,015806$$y2014
000071329 999C5 $$01247056$$hJ. Xu et al.$$o10$$sPhys.Rev.Lett.,112,012301$$y2014
000071329 999C5 $$01185269$$hJ. Steinheimer, J. Randrup$$o11$$sPhys.Rev.Lett.,109,212301$$y2012
000071329 999C5 $$01280557$$hL. Adamczyk et al.$$mSTAR Collaboration$$o12$$sPhys.Rev.Lett.,113,092301$$y2014
000071329 999C5 $$0514753$$hF. Antinori et al.$$o13$$sNucl.Phys.,A661,130$$y1999
000071329 999C5 $$01264150$$hP. Hohler, R. Rapp$$o14$$sPhys.Lett.,B731,103$$y2014
000071329 999C5 $$01328529$$hR. Rapp, H. van Hees$$o15$$rarXiv:1411.4612
000071329 999C5 $$0230496$$hT. Matsui, H. Satz$$o16$$sPhys.Lett.,B178,416$$y1986
000071329 999C5 $$0459314$$hM. Abreu et al.$$mNA50 Collaboration$$o17$$sPhys.Lett.,B410,337$$y1997
000071329 999C5 $$0723948$$hA. Adare et al.$$mPHENIX Collaboration$$o18$$sPhys.Rev.Lett.,98,162301$$y2007
000071329 999C5 $$01088222$$cALICE Collaboration$$hB. Abelev et al.$$o19$$sPhys.Rev.Lett.,109,072301$$y2012
000071329 999C5 $$0873073$$hA. Andronic et al.$$o20$$sPhys.Lett.,B697,203$$y2011
000071329 999C5 $$hH. Stoecker et al.$$o21$$sNucl.Phys.,A827,624$$y2009
000071329 999C5 $$01335267$$hA.S. Botvina et al.$$o22$$sPhys.Lett.,B742,7$$y2015
000071329 999C5 $$0496931$$hC. Pinkenburg et al.$$o23$$sPhys.Rev.Lett.,83,1295$$y1999
000071329 999C5 $$0762554$$hC. Alt et al.$$o24$$sPhys.Rev.,C77,024903$$y2008
000071329 999C5 $$hA. Laszlo$$mPoS (CPOD07) 054$$o25$$y2007
000071329 999C5 $$mpublic/sn0598$$o26$$uhttps://drupal.star.bnl.gov/STAR/starnotes/
000071329 999C5 $$msee also this Topical Issue$$o27$$uhttp://nica.jinr.ru/
000071329 999C5 $$h(B. Friman et al. (eds.))$$mThe CBM Physics Book,Lect. Notes Phys. 814$$o28$$y2011
000071329 999C5 $$01413132$$hJ. Th$$m̈ ader for the STAR Collaboration$$o29$$rarXiv:1601.00951 [nucl-ex]
000071329 999C5 $$0716533$$hR. Arnaldi et al.$$mNA60 Collaboration$$o30$$sPhys.Rev.Lett.,96,162302$$y2006
000071329 999C5 $$0811444$$hR. Rapp, J. Wambach, H. van Hees$$o31$$rarXiv:0901.3289 [hepph]
000071329 999C5 $$0787520$$hA. Frawley, T. Ulrich, R. Vogt$$o32$$sPhys.Rept.,462,125$$y2008
000071329 999C5 $$0873073$$hA. Andronic et al.$$o33$$sPhys.Lett.,B697,203$$y2011
000071329 999C6 $$a0-0-1-1-0-0-0$$t2017-03-14 10:55:46$$vInvenio/ refextract/1.5.44