dc.date2015
dc.date2016-06-03T20:14:13Z
dc.date2016-06-03T20:14:13Z
dc.date.accessioned2018-03-29T01:33:08Z
dc.date.available2018-03-29T01:33:08Z
dc.identifier
dc.identifierPhysics Letters, Section B: Nuclear, Elementary Particle And High-energy Physics. Elsevier, v. 750, p. 64 - 71, 2015.
dc.identifier3702693
dc.identifier10.1016/j.physletb.2015.08.044
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84940398947&partnerID=40&md5=9bfeab1a4fd779337d5ea720ede553f2
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/238191
dc.identifier2-s2.0-84940398947
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1304852
dc.descriptionThe acceptance-corrected dielectron excess mass spectra, where the known hadronic sources have been subtracted from the inclusive dielectron mass spectra, are reported for the first time at mid-rapidity |yee|<1 in minimum-bias Au+Au collisions at √sNN=19.6 and 200 GeV. The excess mass spectra are consistently described by a model calculation with a broadened ρ spectral function for Mee<1.1 GeV/c2. The integrated dielectron excess yield at √sNN=19.6 GeV for 0.4<Mee<0.75 GeV/c2, normalized to the charged particle multiplicity at mid-rapidity, has a value similar to that in In+In collisions at √sNN=17.3 GeV. For √sNN=200 GeV, the normalized excess yield in central collisions is higher than that at √sNN=17.3 GeV and increases from peripheral to central collisions. These measurements indicate that the lifetime of the hot, dense medium created in central Au+Au collisions at √sNN=200 GeV is longer than those in peripheral collisions and at lower energies. © 2015 The Authors.
dc.description750
dc.description
dc.description64
dc.description71
dc.descriptionAdams, J., (2005) Nucl. Phys. A, 757, p. 102
dc.descriptionArsene, I., (2005) Nucl. Phys. A, 757, p. 1
dc.descriptionAdcox, K., (2005) Nucl. Phys. A, 757, p. 184
dc.descriptionBack, B.B., (2005) Nucl. Phys. A, 757, p. 28
dc.descriptionRapp, R., Wambach, J., (2000) Adv. Nucl. Phys., 25, p. 1
dc.descriptionDavid, G., Rapp, R., Xu, Z., (2008) Phys. Rep., 462, p. 176
dc.descriptionRapp, R., Wambach, J., (1999) Eur. Phys. J. A, 6, p. 415
dc.descriptionBrown, G.E., Rho, M., (1996) Phys. Rep., 269, p. 333
dc.descriptionBrown, G.E., Rho, M., (2002) Phys. Rep., 363, p. 85
dc.descriptionAdamova, D., (2003) Phys. Rev. Lett., 91
dc.descriptionAgakichiev, G., (2005) Eur. Phys. J. C, 41, p. 475
dc.descriptionAdamova, D., (2008) Phys. Lett. B, 666, p. 425
dc.descriptionArnaldi, R., (2006) Phys. Rev. Lett., 96
dc.descriptionArnaldi, R., (2008) Phys. Rev. Lett., 100
dc.descriptionArnaldi, R., (2009) Eur. Phys. J. C, 59, p. 607
dc.descriptionAdare, A., (2010) Phys. Rev. C, 81
dc.descriptionAdamczyk, L., (2014) Phys. Rev. Lett., 113
dc.descriptionAdamczyk, L., (2014) Phys. Rev. Lett., 113. , (Erratum)
dc.descriptionRapp, R., (2001) Phys. Rev. C, 63
dc.descriptionvan Hees, H., Rapp, R., (2006) Phys. Rev. Lett., 97
dc.descriptionvan Hees, H., Rapp, R., (2008) Nucl. Phys. A, 806, p. 339
dc.descriptionRapp, R., (2013) Adv. High Energy Phys., 2013, p. 148253
dc.descriptionLinnyk, O., (2011) Phys. Rev. C, 84
dc.descriptionLinnyk, O., (2012) Phys. Rev. C, 85
dc.descriptionXu, H., (2012) Phys. Rev. C, 85
dc.descriptionBeam, S.T.A.R., Energy Scan II white paper, , https://drupal.star.bnl.gov/STAR/starnotes/public/sn0598
dc.descriptionAngelis, A.L.S., (2000) Eur. Phys. J. C, 13, p. 433
dc.descriptionAbreu, M.C., (1996) Phys. Lett. B, 368, p. 230
dc.descriptionAbreu, M.C., (2000) Eur. Phys. J. C, 14, p. 443
dc.descriptionAckermann, K.H., (2003) Nucl. Instrum. Methods, Sect. A, 499, p. 624
dc.descriptionRapp, R., van Hees, H., arxiv:1411.4612Adams, J., (2004) Phys. Rev. Lett., 92
dc.descriptionAnderson, M., (2003) Nucl. Instrum. Methods, Sect. A, 499, p. 659
dc.descriptionBonner, B., (2003) Nucl. Instrum. Methods, Sect. A, 508, p. 181
dc.descriptionShao, M., (2002) Nucl. Instrum. Methods, Sect. A, 492, p. 344
dc.descriptionWu, J., (2005) Nucl. Instrum. Methods, Sect. A, 538, p. 243
dc.descriptionBichsel, H., (2006) Nucl. Instrum. Methods, Sect. A, 562, p. 154
dc.descriptionAdamczyk, L., (2012) Phys. Rev. C, 86
dc.descriptionhttp://wwwasdoc.web.cern.ch/wwwasdoc/geant_html3/geantall.html, GEANT 3.21, CERN program libraryTang, Z., (2009) Phys. Rev. C, 79
dc.descriptionShao, M., (2010) J. Phys. G, 37
dc.descriptionAlt, C., (2008) Phys. Rev. C, 77
dc.descriptionAbreu, M., (2001) Phys. Lett. B, 499, p. 85
dc.descriptionBeringer, J., (2012) Phys. Rev. D, 86
dc.descriptionSjöstrand, T., (2001) Comput. Phys. Commun., 135, p. 238
dc.descriptionRapp, R., private communicationsAlves, G.A., (1996) Phys. Rev. Lett., 77, p. 2388
dc.descriptionAlves, G.A., (1998) Phys. Rev. Lett., 81, p. 1537. , (Erratum)
dc.descriptionTavernier, S.P.K., (1987) Rep. Prog. Phys., 50, p. 1439. , and references therein
dc.descriptionAdamczyk, L., (2012) Phys. Rev. D, 86
dc.descriptionAdare, A., (2006) Phys. Rev. Lett., 97
dc.descriptionNelson, R., (2013) Phys. Rev. C, 87
dc.descriptionDamjanovic, S., (2007) Nucl. Phys. A, 783, p. 327
dc.descriptionAdamczyk, L., (2015) Phys. Rev. C, , arxiv:1504.01317, submitted for publication
dc.descriptionHohler, P.M., Rapp, R., (2014) Phys. Lett. B, 731, p. 103
dc.descriptionKumar, L., (2014) Nucl. Phys. A, 931, p. 1114
dc.descriptionAbelev, B.I., (2009) Phys. Rev. C, 79
dc.descriptionSpecht, H., (2010) AIP Conf. Proc., 1322, p. 1
dc.description
dc.description
dc.languageen
dc.publisherElsevier
dc.relationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
dc.rightsaberto
dc.sourceScopus
dc.titleEnergy Dependence Of Acceptance-corrected Dielectron Excess Mass Spectrum At Mid-rapidity In Au+au Collisions At √snn=19.6 And 200 Gev
dc.typeArtículos de revistas


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