SCOPUS 정보 검색 플랫폼

Physical Review C - Nuclear Physics

Volumn 86, Issue 2, 2012, Pages

Decomposition of flow and nonflow in relativistic heavy-ion collisions

(6) Xu, Lingshan a Yi, Li a Kikola, Daniel a Konzer, Joshua a Wang, Fuqiang a Xie, Wei a

a PURDUE UNIVERSITY (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84865589781 PISSN: 05562813 EISSN: 1089490X Source Type: Journal
DOI: 10.1103/PhysRevC.86.024910 Document Type: Article

Times cited : (16)

References (33)

1
- 85026345669
- e-print arXiv: 0809.2949.
- S. A. Voloshin, A. M. Poskanzer, and R. Snellings, e-print arXiv: 0809.2949.
- Voloshin, S.A.¹ Poskanzer, A.M.² Snellings, R.³

2
- 24544479590
- PRVDAQ 1550-7998 10.1103/PhysRevD.46.229
- J. Y. Ollitrault, Phys. Rev. D PRVDAQ 1550-7998 10.1103/PhysRevD.46.229 46, 229 (1992).
- (1992) Phys. Rev. D , vol.46 , pp. 229
- Ollitrault, J.Y.¹

3
- 0035911702
- PT azimuthal asymmetry in noncentral A + A at RHIC
- DOI 10.1103/PhysRevLett.86.2537
- M. Gyulassy, I. Vitev, and X.-N. Wang, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.86.2537 23, 2537 (2001). (Pubitemid 32286697)
- (2001) Physical Review Letters , vol.86 , Issue.12 , pp. 2537-2540
- Gyulassy, M.¹ Vitev, I.² Wang, X.-N.³

4
- 12944331357
- PRVCAN 0556-2813 10.1103/PhysRevC.62.034902
- N. Borghini, P. M. Dinh, and J. Y. Ollitrault, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.62.034902 62, 034902 (2000).
- (2000) Phys. Rev. C , vol.62 , pp. 034902
- Borghini, N.¹ Dinh, P.M.² Ollitrault, J.Y.³

5
- 0001449146
- PRVCAN 0556-2813 10.1103/PhysRevC.44.1091
- S. Wang, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.44.1091 44, 1091 (1991).
- (1991) Phys. Rev. C , vol.44 , pp. 1091
- Wang, S.¹

6
- 0032388094
- Methods for analyzing anisotropic flow in relativistic nuclear collisions
- DOI 10.1103/PhysRevC.58.1671
- A. M. Poskanzer and S. A. Voloshin, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.58.1671 58, 1671 (1998). (Pubitemid 128129634)
- (1998) Physical Review C - Nuclear Physics , vol.58 , Issue.3 , pp. 1671-1678
- Poskanzer, A.M.¹ Voloshin, S.A.²

7
- 85026393635
- e-print arXiv: nucl-ex/0312008.
- M. Miller and R. Snellings, e-print arXiv: nucl-ex/0312008.
- Miller, M.¹ Snellings, R.²

9
- 68549098081
- PRVCAN 0556-2813 10.1103/PhysRevC.80.014904
- J. Y. Ollitrault, A. M. Poskanzer, and S. A. Voloshin, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.80.014904 80, 014904 (2009).
- (2009) Phys. Rev. C , vol.80 , pp. 014904
- Ollitrault, J.Y.¹ Poskanzer, A.M.² Voloshin, S.A.³

10
- 58149252088
- PRVCAN 0556-2813 10.1103/PhysRevC.78.064908
- T. A. Trainor, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.78.064908 78, 064908 (2008).
- (2008) Phys. Rev. C , vol.78 , pp. 064908
- Trainor, T.A.¹

11
- 14344279262
- PRVCAN 0556-2813 10.1103/PhysRevC.63.054906
- N. Borghini, P. M. Dinh, and J. Y. Ollitrault, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.63.054906 63, 054906 (2001).
- (2001) Phys. Rev. C , vol.63 , pp. 054906
- Borghini, N.¹ Dinh, P.M.² Ollitrault, J.Y.³

12
- 14344281807
- PRVCAN 0556-2813 10.1103/PhysRevC.64.054901
- N. Borghini, P. M. Dinh, and J. Y. Ollitrault, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.64.054901 64, 054901 (2001).
- (2001) Phys. Rev. C , vol.64 , pp. 054901
- Borghini, N.¹ Dinh, P.M.² Ollitrault, J.Y.³

13
- 34548176740
- PRVCAN 0556-2813 10.1103/PhysRevC.76.024907
- G. Wang, D. Keane, A. Tang, and S.A. Voloshin, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.76.024907 76, 024907 (2007).
- (2007) Phys. Rev. C , vol.76 , pp. 024907
- Wang, G.¹ Keane, D.² Tang, A.³ Voloshin, S.A.⁴

14
- 38849181035
- PRVCAN 0556-2813 10.1103/PhysRevC.77.014906
- B. Alver, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.77.014906 77, 014906 (2008).
- (2008) Phys. Rev. C , vol.77 , pp. 014906
- Alver, B.¹

15
- 77950923946
- (PHOBOS Collaboration), PRVCAN 0556-2813 10.1103/PhysRevC.81.034915
- B. Alver (PHOBOS Collaboration), Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.81.034915 81, 034915 (2010).
- (2010) Phys. Rev. C , vol.81 , pp. 034915
- Alver, B.¹

16
- 34547461211
- (STAR Collaboration), JPGPED 0954-3899 10.1088/0954-3899/34/8/S121
- P. Sorensen (STAR Collaboration), J. Phys. G JPGPED 0954-3899 10.1088/0954-3899/34/8/S121 34, S897 (2007).
- (2007) J. Phys. G , vol.34 , pp. 897
- Sorensen, P.¹

17
- 54749103829
- (STAR Collaboration), JPGPED 0954-3899 10.1088/0954-3899/35/10/104102
- P. Sorensen (STAR Collaboration), J. Phys. G JPGPED 0954-3899 10.1088/0954-3899/35/10/104102 35, 104102 (2008).
- (2008) J. Phys. G , vol.35 , pp. 104102
- Sorensen, P.¹

18
- 37549040230
- PYLBAJ 0370-2693 10.1016/j.physletb.2007.11.043
- S. A. Voloshin, Phys. Lett. B PYLBAJ 0370-2693 10.1016/j.physletb.2007. 11.043 659, 537 (2008).
- (2008) Phys. Lett. B , vol.659 , pp. 537
- Voloshin, S.A.¹

19
- 77954076212
- PRVCAN 0556-2813 10.1103/PhysRevC.81.064905
- Q. Wang and F. Wang, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.81. 064905 81, 064905 (2010).
- (2010) Phys. Rev. C , vol.81 , pp. 064905
- Wang, Q.¹ Wang, F.²

20
- 79961159319
- (ALICE Collaboration), PRLTAO 0031-9007 10.1103/PhysRevLett.107.032301
- K. Aamodt (ALICE Collaboration), Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.107.032301 107, 032301 (2011).
- (2011) Phys. Rev. Lett. , vol.107 , pp. 032301
- Aamodt, K.¹

21
- 85026432588
- e-print arXiv: 1101.4646.
- L. Yi, F. Wang, and A. Tang, e-print arXiv: 1101.4646.
- Yi, L.¹ Wang, F.² Tang, A.³

22
- 84864400384
- PRVCAN 0556-2813 10.1103/PhysRevC.86.014901
- D. Kikola, L. Yi, S. I. Esumi, F. Wang, and W. Xie, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.86.014901 86, 014901 (2012).
- (2012) Phys. Rev. C , vol.86 , pp. 014901
- Kikola, D.¹ Yi, L.² Esumi, S.I.³ Wang, F.⁴ Xie, W.⁵

24
- 84862313330
- (CMS Collaboration), EPCFFB 1434-6044 10.1140/epjc/s10052-012-2012-3
- S. Chatrchyan (CMS Collaboration), Eur. Phys. J. C EPCFFB 1434-6044 10.1140/epjc/s10052-012-2012-3 72, 2012 (2012).
- (2012) Eur. Phys. J. C , vol.72 , pp. 2012
- Chatrchyan, S.¹

25
- 84913599963
- (ATLAS Collaboration), PRVCAN 0556-2813 10.1103/PhysRevC.86.014907
- G. Aad (ATLAS Collaboration), Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.86.014907 86, 014907 (2012).
- (2012) Phys. Rev. C , vol.86 , pp. 014907
- Aad, G.¹

26
- 85026346659
- (STAR Collaboration), e-print arXiv: 1010.0690.
- H. Agakishiev (STAR Collaboration), e-print arXiv: 1010.0690.
- Agakishiev, H.¹

27
- 33244482549
- Multiphase transport model for relativistic heavy ion collisions
- DOI 10.1103/PhysRevC.72.064901
- Z. W. Lin, C. M. Ko, B. A. Li, B. Zhang, and S. Pal, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.72.064901 72, 064901 (2005). (Pubitemid 43272833)
- (2005) Physical Review C - Nuclear Physics , vol.72 , Issue.6 , pp. 064901
- Lin, Z.-W.¹ Ko, C.M.² Li, B.-A.³ Zhang, B.⁴ Pal, S.⁵

28
- 0348064082
- PRVCAN 0556-2813 10.1103/PhysRevC.65.034904
- Z.-W. Lin and C. M. Ko, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.65.034904 65, 034904 (2002).
- (2002) Phys. Rev. C , vol.65 , pp. 034904
- Lin, Z.-W.¹ Ko, C.M.²

29
- 18244403158
- Dissipation and elliptic flow at relativistic energies
- DOI 10.1103/PhysRevLett.94.012302, 012302
- D. Molnar and P. Huovinen, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94.012302 94, 012302 (2005). (Pubitemid 40629818)
- (2005) Physical Review Letters , vol.94 , Issue.1 , pp. 1-4
- Molnar, D.¹ Huovinen, P.²

30
- 0028695052
- CPHCBZ 0010-4655 10.1016/0010-4655(94)90057-4
- M. Gyulassy and X.-N. Wang, Comput. Phys. Commun. CPHCBZ 0010-4655 10.1016/0010-4655(94)90057-4 83, 307 (1994).
- (1994) Comput. Phys. Commun. , vol.83 , pp. 307
- Gyulassy, M.¹ Wang, X.-N.²

31
- 79960636917
- PRLTAO 0031-9007 10.1103/PhysRevLett.106.162301
- G. L. Ma and X.-N. Wang, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.106.162301 106, 162301 (2011).
- (2011) Phys. Rev. Lett. , vol.106 , pp. 162301
- Ma, G.L.¹ Wang, X.-N.²

32
- 78649340857
- PRVCAN 0556-2813 10.1103/PhysRevC.82.041901
- H. Petersen, G. Y. Qin, S. A. Bass, and B. Muller, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.82.041901 82, 041901 (2010).
- (2010) Phys. Rev. C , vol.82 , pp. 041901
- Petersen, H.¹ Qin, G.Y.² Bass, S.A.³ Muller, B.⁴

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.