Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156

I. Dillmann; C. Domingo-Pardo; M. Heil; F. Kaeppeler; S. Walter; S. Dababneh; T. Rauscher; Friedrich-Karl Thielemann

doi:10.1103/PhysRevC.81.015801

Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156

I. Dillmann
, C. Domingo-Pardo
, M. Heil
, F. Kaeppeler
, S. Walter
, S. Dababneh
, T. Rauscher
, Friedrich-Karl Thielemann

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

24 Citations (Scopus)

135 Downloads (Pure)

Abstract

We have investigated the (n,gamma) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the Li-7(p, n) Be-7 source for simulating a Maxwellian neutron distribution of kT = 25 keV. Stellar cross section measurements are reported for the light p-process isotopes Pd-102, Te-120, Ba-130,Ba-132, and Dy-156. In a following paper the cross sections of Yb-168, W-180, Os-184, Pt-190, and Hg-196 will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.

Original language	English
Article number	015801
Number of pages	13
Journal	Physical Review C (nuclear physics)
Volume	81
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevC.81.015801
Publication status	Published - Jan 2010

Keywords

STARS
ATOMIC WEIGHTS
STATISTICAL-MODEL CALCULATIONS
NUCLEAR-DATA LIBRARY
ELEMENTS
ASTROPHYSICAL REACTION-RATES
NUCLEOSYNTHESIS
RP-PROCESS
DATA SHEETS
TELLURIUM

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title = "Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156",

abstract = "We have investigated the (n,gamma) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the Li-7(p, n) Be-7 source for simulating a Maxwellian neutron distribution of kT = 25 keV. Stellar cross section measurements are reported for the light p-process isotopes Pd-102, Te-120, Ba-130,Ba-132, and Dy-156. In a following paper the cross sections of Yb-168, W-180, Os-184, Pt-190, and Hg-196 will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.",

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author = "I. Dillmann and C. Domingo-Pardo and M. Heil and F. Kaeppeler and S. Walter and S. Dababneh and T. Rauscher and Friedrich-Karl Thielemann",

year = "2010",

month = jan,

doi = "10.1103/PhysRevC.81.015801",

language = "English",

volume = "81",

journal = "Physical Review C (nuclear physics)",

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T1 - Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156

AU - Dillmann, I.

AU - Domingo-Pardo, C.

AU - Heil, M.

AU - Kaeppeler, F.

AU - Walter, S.

AU - Dababneh, S.

AU - Rauscher, T.

AU - Thielemann, Friedrich-Karl

PY - 2010/1

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N2 - We have investigated the (n,gamma) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the Li-7(p, n) Be-7 source for simulating a Maxwellian neutron distribution of kT = 25 keV. Stellar cross section measurements are reported for the light p-process isotopes Pd-102, Te-120, Ba-130,Ba-132, and Dy-156. In a following paper the cross sections of Yb-168, W-180, Os-184, Pt-190, and Hg-196 will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.

AB - We have investigated the (n,gamma) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the Li-7(p, n) Be-7 source for simulating a Maxwellian neutron distribution of kT = 25 keV. Stellar cross section measurements are reported for the light p-process isotopes Pd-102, Te-120, Ba-130,Ba-132, and Dy-156. In a following paper the cross sections of Yb-168, W-180, Os-184, Pt-190, and Hg-196 will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.

KW - STARS

KW - ATOMIC WEIGHTS

KW - STATISTICAL-MODEL CALCULATIONS

KW - NUCLEAR-DATA LIBRARY

KW - ELEMENTS

KW - ASTROPHYSICAL REACTION-RATES

KW - NUCLEOSYNTHESIS

KW - RP-PROCESS

KW - DATA SHEETS

KW - TELLURIUM

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DO - 10.1103/PhysRevC.81.015801

M3 - Article

SN - 2469-9985

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JO - Physical Review C (nuclear physics)

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M1 - 015801

ER -

Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156

Abstract

Keywords

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