Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions

P. Chung; N. N. Ajitanand; J. M. Alexander; M. Anderson; D. Best; F. P. Brady; T. Case; W. Caskey; D. Cebra; J. L. Chance; B. Cole; K. Crowe; A. C. Das; J. E. Draper; M. L. Gilkes; S. Gushue; M. Heffner; A. S. Hirsch; E. L. Hjort; W. Holzmann; L. Huo; M. Issah; M. Justice; M. Kaplan; D. Keane; J. C. Kintner; J. Klay; D. Krofcheck; R. A. Lacey; J. Lauret; M. A. Lisa; H. Liu; Y. M. Liu; R. McGrath; Z. Milosevich; G. Odyniec; D. L. Olson; S. Panitkin; N. T. Porile; G. Rai; H. G. Ritter; J. L. Romero; R. Scharenberg; B. Srivastava; N. T.B. Stone; T. J.M. Symons; A. Taranenko; J. Whitfield; R. Witt; L. Wood; W. N. Zhang; D. Brown; S. Pratt; F. Wang; P. Danielewicz

doi:10.1103/PhysRevLett.91.162301

Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions

P. Chung
, N. N. Ajitanand
, J. M. Alexander
, M. Anderson
, D. Best
, F. P. Brady
, T. Case
, W. Caskey
, D. Cebra
, J. L. Chance
, B. Cole
, K. Crowe
, A. C. Das
, J. E. Draper
, M. L. Gilkes
, S. Gushue
, M. Heffner
, A. S. Hirsch
, E. L. Hjort
, W. Holzmann

L. Huo, M. Issah, M. Justice, M. Kaplan, D. Keane, J. C. Kintner, J. Klay, D. Krofcheck, R. A. Lacey, J. Lauret, M. A. Lisa, H. Liu, Y. M. Liu, R. McGrath, Z. Milosevich, G. Odyniec, D. L. Olson, S. Panitkin, N. T. Porile, G. Rai, H. G. Ritter, J. L. Romero, R. Scharenberg, B. Srivastava, N. T.B. Stone, T. J.M. Symons, A. Taranenko, J. Whitfield, R. Witt, L. Wood, W. N. Zhang, D. Brown, S. Pratt, F. Wang, P. Danielewicz

Chemistry

Stony Brook University
University of California at Davis
Lawrence Berkeley National Laboratory
Columbia University
Ohio State University
Brookhaven National Laboratory
Purdue University
Harbin Institute of Technology
Kent State University
Carnegie Mellon University
The University of Auckland
Lawrence Livermore National Laboratory

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

Source images are extracted from two-particle correlations constructed from strange and nonstrange hadrons produced in [Formula presented] [Formula presented] collisions. Very different source images result from [Formula presented] vs [Formula presented] vs [Formula presented] correlations. Scaling by transverse mass can describe the apparent source size ratio for [Formula presented] but not for [Formula presented] or [Formula presented]. These observations suggest important differences in the space-time emission histories for protons, pions, and neutral strange baryons produced in the same events.

Original language	English
Journal	Physical Review Letters
Volume	91
Issue number	16
DOIs	https://doi.org/10.1103/PhysRevLett.91.162301
State	Published - 2003

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10.1103/PhysRevLett.91.162301

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Chung, P., Ajitanand, N. N., Alexander, J. M., Anderson, M., Best, D., Brady, F. P., Case, T., Caskey, W., Cebra, D., Chance, J. L., Cole, B., Crowe, K., Das, A. C., Draper, J. E., Gilkes, M. L., Gushue, S., Heffner, M., Hirsch, A. S., Hjort, E. L., ... Danielewicz, P. (2003). Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions. Physical Review Letters, 91(16). https://doi.org/10.1103/PhysRevLett.91.162301

@article{110fe45db229495481d9f3763c56e9a9,

title = "Comparison of source images for protons, [formula presented]{\textquoteright}s, and [formula presented]{\textquoteright}s in [formula presented] [formula presented] collisions",

abstract = "Source images are extracted from two-particle correlations constructed from strange and nonstrange hadrons produced in [Formula presented] [Formula presented] collisions. Very different source images result from [Formula presented] vs [Formula presented] vs [Formula presented] correlations. Scaling by transverse mass can describe the apparent source size ratio for [Formula presented] but not for [Formula presented] or [Formula presented]. These observations suggest important differences in the space-time emission histories for protons, pions, and neutral strange baryons produced in the same events.",

author = "P. Chung and Ajitanand, \{N. N.\} and Alexander, \{J. M.\} and M. Anderson and D. Best and Brady, \{F. P.\} and T. Case and W. Caskey and D. Cebra and Chance, \{J. L.\} and B. Cole and K. Crowe and Das, \{A. C.\} and Draper, \{J. E.\} and Gilkes, \{M. L.\} and S. Gushue and M. Heffner and Hirsch, \{A. S.\} and Hjort, \{E. L.\} and W. Holzmann and L. Huo and M. Issah and M. Justice and M. Kaplan and D. Keane and Kintner, \{J. C.\} and J. Klay and D. Krofcheck and Lacey, \{R. A.\} and J. Lauret and Lisa, \{M. A.\} and H. Liu and Liu, \{Y. M.\} and R. McGrath and Z. Milosevich and G. Odyniec and Olson, \{D. L.\} and S. Panitkin and Porile, \{N. T.\} and G. Rai and Ritter, \{H. G.\} and Romero, \{J. L.\} and R. Scharenberg and B. Srivastava and Stone, \{N. T.B.\} and Symons, \{T. J.M.\} and A. Taranenko and J. Whitfield and R. Witt and L. Wood and Zhang, \{W. N.\} and D. Brown and S. Pratt and F. Wang and P. Danielewicz",

year = "2003",

doi = "10.1103/PhysRevLett.91.162301",

language = "English",

volume = "91",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "16",

}

Chung, P, Ajitanand, NN, Alexander, JM, Anderson, M, Best, D, Brady, FP, Case, T, Caskey, W, Cebra, D, Chance, JL, Cole, B, Crowe, K, Das, AC, Draper, JE, Gilkes, ML, Gushue, S, Heffner, M, Hirsch, AS, Hjort, EL, Holzmann, W, Huo, L, Issah, M, Justice, M, Kaplan, M, Keane, D, Kintner, JC, Klay, J, Krofcheck, D, Lacey, RA, Lauret, J, Lisa, MA, Liu, H, Liu, YM, McGrath, R, Milosevich, Z, Odyniec, G, Olson, DL, Panitkin, S, Porile, NT, Rai, G, Ritter, HG, Romero, JL, Scharenberg, R, Srivastava, B, Stone, NTB, Symons, TJM, Taranenko, A, Whitfield, J, Witt, R, Wood, L, Zhang, WN, Brown, D, Pratt, S, Wang, F & Danielewicz, P 2003, 'Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions', Physical Review Letters, vol. 91, no. 16. https://doi.org/10.1103/PhysRevLett.91.162301

TY - JOUR

T1 - Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions

AU - Chung, P.

AU - Ajitanand, N. N.

AU - Alexander, J. M.

AU - Anderson, M.

AU - Best, D.

AU - Brady, F. P.

AU - Case, T.

AU - Caskey, W.

AU - Cebra, D.

AU - Chance, J. L.

AU - Cole, B.

AU - Crowe, K.

AU - Das, A. C.

AU - Draper, J. E.

AU - Gilkes, M. L.

AU - Gushue, S.

AU - Heffner, M.

AU - Hirsch, A. S.

AU - Hjort, E. L.

AU - Holzmann, W.

AU - Huo, L.

AU - Issah, M.

AU - Justice, M.

AU - Kaplan, M.

AU - Keane, D.

AU - Kintner, J. C.

AU - Klay, J.

AU - Krofcheck, D.

AU - Lacey, R. A.

AU - Lauret, J.

AU - Lisa, M. A.

AU - Liu, H.

AU - Liu, Y. M.

AU - McGrath, R.

AU - Milosevich, Z.

AU - Odyniec, G.

AU - Olson, D. L.

AU - Panitkin, S.

AU - Porile, N. T.

AU - Rai, G.

AU - Ritter, H. G.

AU - Romero, J. L.

AU - Scharenberg, R.

AU - Srivastava, B.

AU - Stone, N. T.B.

AU - Symons, T. J.M.

AU - Taranenko, A.

AU - Whitfield, J.

AU - Witt, R.

AU - Wood, L.

AU - Zhang, W. N.

AU - Brown, D.

AU - Pratt, S.

AU - Wang, F.

AU - Danielewicz, P.

PY - 2003

Y1 - 2003

N2 - Source images are extracted from two-particle correlations constructed from strange and nonstrange hadrons produced in [Formula presented] [Formula presented] collisions. Very different source images result from [Formula presented] vs [Formula presented] vs [Formula presented] correlations. Scaling by transverse mass can describe the apparent source size ratio for [Formula presented] but not for [Formula presented] or [Formula presented]. These observations suggest important differences in the space-time emission histories for protons, pions, and neutral strange baryons produced in the same events.

AB - Source images are extracted from two-particle correlations constructed from strange and nonstrange hadrons produced in [Formula presented] [Formula presented] collisions. Very different source images result from [Formula presented] vs [Formula presented] vs [Formula presented] correlations. Scaling by transverse mass can describe the apparent source size ratio for [Formula presented] but not for [Formula presented] or [Formula presented]. These observations suggest important differences in the space-time emission histories for protons, pions, and neutral strange baryons produced in the same events.

UR - https://www.scopus.com/pages/publications/85038290056

U2 - 10.1103/PhysRevLett.91.162301

DO - 10.1103/PhysRevLett.91.162301

M3 - Article

AN - SCOPUS:85038290056

SN - 0031-9007

VL - 91

JO - Physical Review Letters

JF - Physical Review Letters

IS - 16

ER -

Comparison of source images for protons, [formula presented]’s, and [formula presented]’s in [formula presented] [formula presented] collisions

Abstract

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