Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes

B. K. Srivastava; S. Albergo; F. Bieser; F. P. Brady; Z. Caccia; D. A. Cebra; A. D. Chacon; J. L. Chance; Y. Choi; S. Costa; P. Danielewicz; J. B. Elliott; M. L. Gilkes; J. A. Hauger; A. S. Hirsch; E. L. Hjort; A. Insolia; M. Justice; D. Keane; J. C. Kintner; V. Lindenstruth; M. A. Lisa; H. S. Matis; M. McMahan; C. McParland; W. F.J. Müller; D. L. Olson; M. D. Partlan; N. T. Porile; R. Potenza; G. Rai; J. Rasmussen; H. G. Ritter; J. Romanski; J. L. Romero; G. V. Russo; H. Sann; R. P. Scharenberg; A. Scott; Y. Shao; T. J.M. Symons; M. Tincknell; C. Tuvé; S. Wang; P. Warren; H. H. Wieman; T. Wienold; K. Wolf

doi:10.1103/PhysRevC.60.064606

Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes

B. K. Srivastava, S. Albergo, F. Bieser, F. P. Brady, Z. Caccia, D. A. Cebra, A. D. Chacon, J. L. Chance, Y. Choi, S. Costa, P. Danielewicz, J. B. Elliott, M. L. Gilkes, J. A. Hauger, A. S. Hirsch, E. L. Hjort, A. Insolia, M. Justice, D. Keane, J. C. KintnerV. Lindenstruth, M. A. Lisa, H. S. Matis, M. McMahan, C. McParland, W. F.J. Müller, D. L. Olson, M. D. Partlan, N. T. Porile, R. Potenza, G. Rai, J. Rasmussen, H. G. Ritter, J. Romanski, J. L. Romero, G. V. Russo, H. Sann, R. P. Scharenberg, A. Scott, Y. Shao, T. J.M. Symons, M. Tincknell, C. Tuvé, S. Wang, P. Warren, H. H. Wieman, T. Wienold, K. Wolf

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

Abstract

The properties of the remnant resulting from the emission of prompt particles in the interaction of [Formula Presented] interactions have been compared with intranuclear cascade and Boltzmann-Uehling-Uhlenback transport calculations. The number of first-stage particles and the energy spectra of first-stage protons are also compared. Both models can fit the general but not the detailed features of the data.

Original language	English (US)
Pages (from-to)	7
Number of pages	1
Journal	Physical Review C - Nuclear Physics
Volume	60
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevC.60.064606
State	Published - 1999
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1103/PhysRevC.60.064606

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Srivastava, B. K., Albergo, S., Bieser, F., Brady, F. P., Caccia, Z., Cebra, D. A., Chacon, A. D., Chance, J. L., Choi, Y., Costa, S., Danielewicz, P., Elliott, J. B., Gilkes, M. L., Hauger, J. A., Hirsch, A. S., Hjort, E. L., Insolia, A., Justice, M., Keane, D., ... Wolf, K. (1999). Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes. Physical Review C - Nuclear Physics, 60(6), 7. https://doi.org/10.1103/PhysRevC.60.064606

Srivastava, BK, Albergo, S, Bieser, F, Brady, FP, Caccia, Z, Cebra, DA, Chacon, AD, Chance, JL, Choi, Y, Costa, S, Danielewicz, P, Elliott, JB, Gilkes, ML, Hauger, JA, Hirsch, AS, Hjort, EL, Insolia, A, Justice, M, Keane, D, Kintner, JC, Lindenstruth, V, Lisa, MA, Matis, HS, McMahan, M, McParland, C, Müller, WFJ, Olson, DL, Partlan, MD, Porile, NT, Potenza, R, Rai, G, Rasmussen, J, Ritter, HG, Romanski, J, Romero, JL, Russo, GV, Sann, H, Scharenberg, RP, Scott, A, Shao, Y, Symons, TJM, Tincknell, M, Tuvé, C, Wang, S, Warren, P, Wieman, HH, Wienold, T & Wolf, K 1999, 'Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes', Physical Review C - Nuclear Physics, vol. 60, no. 6, pp. 7. https://doi.org/10.1103/PhysRevC.60.064606

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abstract = "The properties of the remnant resulting from the emission of prompt particles in the interaction of [Formula Presented] interactions have been compared with intranuclear cascade and Boltzmann-Uehling-Uhlenback transport calculations. The number of first-stage particles and the energy spectra of first-stage protons are also compared. Both models can fit the general but not the detailed features of the data.",

author = "Srivastava, {B. K.} and S. Albergo and F. Bieser and Brady, {F. P.} and Z. Caccia and Cebra, {D. A.} and Chacon, {A. D.} and Chance, {J. L.} and Y. Choi and S. Costa and P. Danielewicz and Elliott, {J. B.} and Gilkes, {M. L.} and Hauger, {J. A.} and Hirsch, {A. S.} and Hjort, {E. L.} and A. Insolia and M. Justice and D. Keane and Kintner, {J. C.} and V. Lindenstruth and Lisa, {M. A.} and Matis, {H. S.} and M. McMahan and C. McParland and M{\"u}ller, {W. F.J.} and Olson, {D. L.} and Partlan, {M. D.} and Porile, {N. T.} and R. Potenza and G. Rai and J. Rasmussen and Ritter, {H. G.} and J. Romanski and Romero, {J. L.} and Russo, {G. V.} and H. Sann and Scharenberg, {R. P.} and A. Scott and Y. Shao and Symons, {T. J.M.} and M. Tincknell and C. Tuv{\'e} and S. Wang and P. Warren and Wieman, {H. H.} and T. Wienold and K. Wolf",

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doi = "10.1103/PhysRevC.60.064606",

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T1 - Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes

AU - Srivastava, B. K.

AU - Albergo, S.

AU - Bieser, F.

AU - Brady, F. P.

AU - Caccia, Z.

AU - Cebra, D. A.

AU - Chacon, A. D.

AU - Chance, J. L.

AU - Choi, Y.

AU - Costa, S.

AU - Danielewicz, P.

AU - Elliott, J. B.

AU - Gilkes, M. L.

AU - Hauger, J. A.

AU - Hirsch, A. S.

AU - Hjort, E. L.

AU - Insolia, A.

AU - Justice, M.

AU - Keane, D.

AU - Kintner, J. C.

AU - Lindenstruth, V.

AU - Lisa, M. A.

AU - Matis, H. S.

AU - McMahan, M.

AU - McParland, C.

AU - Müller, W. F.J.

AU - Olson, D. L.

AU - Partlan, M. D.

AU - Porile, N. T.

AU - Potenza, R.

AU - Rai, G.

AU - Rasmussen, J.

AU - Ritter, H. G.

AU - Romanski, J.

AU - Romero, J. L.

AU - Russo, G. V.

AU - Sann, H.

AU - Scharenberg, R. P.

AU - Scott, A.

AU - Shao, Y.

AU - Symons, T. J.M.

AU - Tincknell, M.

AU - Tuvé, C.

AU - Wang, S.

AU - Warren, P.

AU - Wieman, H. H.

AU - Wienold, T.

AU - Wolf, K.

PY - 1999

Y1 - 1999

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AB - The properties of the remnant resulting from the emission of prompt particles in the interaction of [Formula Presented] interactions have been compared with intranuclear cascade and Boltzmann-Uehling-Uhlenback transport calculations. The number of first-stage particles and the energy spectra of first-stage protons are also compared. Both models can fit the general but not the detailed features of the data.

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Comparison of the 1A [Formula Presented]Au+C interaction with first-stage transport codes

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