Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction

K. Sonnabend; A. Mengoni; P. Mohr; T. Rauscher; K. Vogt; A. Zilges

doi:10.1016/S0375-9474(03)00835-2

Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction

K. Sonnabend, A. Mengoni, P. Mohr, T. Rauscher, K. Vogt, A. Zilges

Centre for Astrophysics Research (CAR)

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

3 Citations (Scopus)

Abstract

The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 +/- 110) mb.

Original language	English
Pages (from-to)	533C-535C
Number of pages	3
Journal	Nuclear Physics A
Volume	718
DOIs	https://doi.org/10.1016/S0375-9474(03)00835-2
Publication status	Published - 5 May 2003
Event	7th International Symposium on Nuclei in the Cosmos (NIC7) - FUJI, Japan Duration: 8 Jul 2002 → 12 Jul 2002

Keywords

GAMMA

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10.1016/S0375-9474(03)00835-2

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title = "Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction",

abstract = "The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 +/- 110) mb.",

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author = "K. Sonnabend and A. Mengoni and P. Mohr and T. Rauscher and K. Vogt and A. Zilges",

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T1 - Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction

AU - Sonnabend, K.

AU - Mengoni, A.

AU - Mohr, P.

AU - Rauscher, T.

AU - Vogt, K.

AU - Zilges, A.

PY - 2003/5/5

Y1 - 2003/5/5

N2 - The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 +/- 110) mb.

AB - The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 +/- 110) mb.

KW - GAMMA

U2 - 10.1016/S0375-9474(03)00835-2

DO - 10.1016/S0375-9474(03)00835-2

M3 - Article

SN - 0375-9474

VL - 718

SP - 533C-535C

JO - Nuclear Physics A

JF - Nuclear Physics A

T2 - 7th International Symposium on Nuclei in the Cosmos (NIC7)

Y2 - 8 July 2002 through 12 July 2002

ER -

Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction

Abstract

Keywords

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