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Erratum to: A study of vorticity formation in high energy nuclear collisions

  • F. Becattini
  • G. Inghirami
  • V. Rolando
  • A. Beraudo
  • L. Del Zanna
  • A. De Pace
  • M. Nardi
  • G. Pagliara
  • V. Chandra
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Erratum
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1 Erratum to: Eur. Phys. J. C (2015) 75:406  https://doi.org/10.1140/epjc/s10052-015-3624-1

Due to an oversight of ours in proofreading and a communication problem with the publisher, the figures published in F. Becattini et al. Eur. Phys. J. C (2015) 75:406 were not correct. This Erratum contains the correct figures (Figs. 2, 3, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15) as in arXiv:1501.04468 [v2], submitted on March 12 2015, and the post-publication version arXiv:1501.04468 [v3], submitted on August 17 2015.
Fig. 2

Mean of the absolute value of T-vorticity components, divided by \(T^2\), at the freeze-out as a function of the grid resolution

Fig. 3

Contour plot of \(\varOmega _{x\eta }/\tau T^2\) at the freeze-out hypersurface at \(y=0\)

Fig. 5

Mean of the absolute values of \(\varOmega _{\mu \nu }/T^2\) components at the freeze-out hypersurface as a function of \(\eta /s\). Note that the \(\varOmega _{x\eta },\varOmega _ {y\eta },\varOmega _{\tau \eta }\) have been multiplied by \(1/\tau \). Upper panel: log scale. Lower panel: magnification of the region around zero viscosity

Fig. 6

Directed flow of pions for different values of \(\eta _m\) parameter with \(\eta /s=0.1\) compared with STAR data [1]

Fig. 7

Directed flow of pions for different values of \(\eta /s\) with \(\eta _m=2.0\) compared with STAR data [1]

Fig. 8

Directed flow of pions at \(\eta /s=0.1\) and \(\eta _m=2.0\) compared with STAR data [1]

Fig. 9

Angular momentum (in \(\hbar \) units) of the plasma with Bjorken initial conditions as a function of the parameter \(\eta _m\)

Fig. 10

Estimated angular momentum (in \(\hbar \) units) of the overlap region of the two colliding nuclei (solid line) and total angular momentum of the plasma according to the parametrization of the initial conditions (dashed line), as a function of the impact parameter

Fig. 11

Mean of the absolute value of thermal vorticity covariant components at the freeze-out as a function of \(\eta /s\). Note that the \({\varpi }_{x\eta },{\varpi }_{y\eta }, {\varpi }_{\tau \eta }\) have been multiplied by \(1/\tau \)

Fig. 12

Mean values of thermal vorticity components at the freeze-out as a function of \(\eta /s\). Note that the \({\varpi }_{x\eta },{\varpi }_{y\eta },{\varpi }_{\tau \eta }\) have been multiplied by \(1/\tau \)

Fig. 13

Contour plot of \(1/\tau \)-scaled \(\eta x\) covariant component of the thermal vorticity, \({\varpi }_{\eta x}/\tau \) over the freeze-out hypersurface for \(y=0\), \(\eta /s=0.1\), \(\eta _m=2.0\)

Fig. 14

Magnitude (a) and components (bd) of the polarization vector of the \(\Lambda \) hyperon in its rest frame

Fig. 15

Directed flow of pions at \(\eta /s=0.1\) and \(\eta _m=2.0\) and with initial \(u^\eta =\frac{1}{\tau } \tanh Ax \; \sinh (y_\mathrm{beam} -|\eta |)\) as in the eq. (36) of the amended paper (Eur. Phys. J. C (2015) 75:406) compared with STAR data [1]

Reference

  1. 1.
    B.I. Abelev et al. (STAR Collaboration), Phys. Rev. Lett. 101, 252301 (2008)Google Scholar

Copyright information

© The Author(s) 2018

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Funded by SCOAP3

Funded by SCOAP3

Authors and Affiliations

  • F. Becattini
    • 1
    • 2
  • G. Inghirami
    • 1
    • 3
  • V. Rolando
    • 4
    • 5
  • A. Beraudo
    • 6
  • L. Del Zanna
    • 1
    • 2
    • 7
  • A. De Pace
    • 6
  • M. Nardi
    • 6
  • G. Pagliara
    • 4
    • 5
  • V. Chandra
    • 8
  1. 1.Dipartimento di Fisica e AstronomiaUniversità di FirenzeSesto F.no (Firenze)Italy
  2. 2.INFN, Sezione di FirenzeSesto F.no (Firenze)Italy
  3. 3.Frankfurt Institute for Advanced Studies (FIAS)Johann Wolfgang Goethe UniversityFrankfurt am MainGermany
  4. 4.Dipartimento di Fisica e Scienze della TerraUniversitá di FerraraFerraraItaly
  5. 5.INFN, Sezione di FerraraFerraraItaly
  6. 6.INFN, Sezione di TorinoTurinItaly
  7. 7.INAF, Osservatorio Astrofisico di ArcetriFlorenceItaly
  8. 8.Indian Institute of Technology GandhinagarAhmedabadIndia

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