A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process

Gy. Gyurky; Zs. Fulop; G. Kiss; Z. Mate; E. Somorjai; J. Gorres; A. Palumbo; M. Wiescher; D. Galaviz; A Kretschmer; K. Sonnabend; A. Zilges; T. Rauscher

doi:10.1016/j.nuclphysa.2005.05.094

A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process

Gy. Gyurky, Zs. Fulop, G. Kiss, Z. Mate, E. Somorjai, J. Gorres, A. Palumbo, M. Wiescher, D. Galaviz, A Kretschmer, K. Sonnabend, A. Zilges, T. Rauscher

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

8 Citations (Scopus)

Abstract

In order to test the reliability of reaction rate calculations in the framework of the Hauser-Feshbach statistical model, the cross sections of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined in the energy range close to the Gamow window for the astrophysical p-process scenario. In addition, to reduce the errors in the predictions of the statistical model calculations, the relevant optical potential parameters are to be determined from the angular distribution measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering reaction at low energies.

Original language	English
Pages (from-to)	517C-520C
Number of pages	4
Journal	Nuclear Physics A
Volume	758
DOIs	https://doi.org/10.1016/j.nuclphysa.2005.05.094
Publication status	Published - 25 Jul 2005
Event	8th International Symposium on Nucle in the Cosmos (NIC8) - Vancouver, Canada Duration: 19 Jul 2004 → 23 Jul 2004

Keywords

CROSS-SECTION

Access to Document

10.1016/j.nuclphysa.2005.05.094

Cite this

@article{17384b8031db41faa4dfdb751dc97523,

title = "A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process",

abstract = "In order to test the reliability of reaction rate calculations in the framework of the Hauser-Feshbach statistical model, the cross sections of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined in the energy range close to the Gamow window for the astrophysical p-process scenario. In addition, to reduce the errors in the predictions of the statistical model calculations, the relevant optical potential parameters are to be determined from the angular distribution measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering reaction at low energies.",

keywords = "CROSS-SECTION",

author = "Gy. Gyurky and Zs. Fulop and G. Kiss and Z. Mate and E. Somorjai and J. Gorres and A. Palumbo and M. Wiescher and D. Galaviz and A Kretschmer and K. Sonnabend and A. Zilges and T. Rauscher",

year = "2005",

month = jul,

day = "25",

doi = "10.1016/j.nuclphysa.2005.05.094",

language = "English",

volume = "758",

pages = "517C--520C",

journal = "Nuclear Physics A",

issn = "0375-9474",

publisher = "Elsevier",

note = "8th International Symposium on Nucle in the Cosmos (NIC8) ; Conference date: 19-07-2004 Through 23-07-2004",

}

TY - JOUR

T1 - A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process

AU - Gyurky, Gy.

AU - Fulop, Zs.

AU - Kiss, G.

AU - Mate, Z.

AU - Somorjai, E.

AU - Gorres, J.

AU - Palumbo, A.

AU - Wiescher, M.

AU - Galaviz, D.

AU - Kretschmer, A

AU - Sonnabend, K.

AU - Zilges, A.

AU - Rauscher, T.

PY - 2005/7/25

Y1 - 2005/7/25

N2 - In order to test the reliability of reaction rate calculations in the framework of the Hauser-Feshbach statistical model, the cross sections of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined in the energy range close to the Gamow window for the astrophysical p-process scenario. In addition, to reduce the errors in the predictions of the statistical model calculations, the relevant optical potential parameters are to be determined from the angular distribution measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering reaction at low energies.

AB - In order to test the reliability of reaction rate calculations in the framework of the Hauser-Feshbach statistical model, the cross sections of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined in the energy range close to the Gamow window for the astrophysical p-process scenario. In addition, to reduce the errors in the predictions of the statistical model calculations, the relevant optical potential parameters are to be determined from the angular distribution measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering reaction at low energies.

KW - CROSS-SECTION

U2 - 10.1016/j.nuclphysa.2005.05.094

DO - 10.1016/j.nuclphysa.2005.05.094

M3 - Article

SN - 0375-9474

VL - 758

SP - 517C-520C

JO - Nuclear Physics A

JF - Nuclear Physics A

T2 - 8th International Symposium on Nucle in the Cosmos (NIC8)

Y2 - 19 July 2004 through 23 July 2004

ER -

A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process

Abstract

Keywords

Access to Document

Fingerprint

Cite this