p-Process simulations with a modified reaction library

I. Dillmann; T. Rauscher; M. Heil; F. Kaeppeler; W. Rapp; F-K Thielemann

doi:10.1088/0954-3899/35/1/014029

p-Process simulations with a modified reaction library

I. Dillmann
, T. Rauscher
, M. Heil
, F. Kaeppeler
, W. Rapp
, F-K Thielemann

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

26 Citations (Scopus)

117 Downloads (Pure)

Abstract

We have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model ('gamma-process') of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.

Original language	English
Article number	014029
Number of pages	5
Journal	Journal of Physics G: Nuclear and Particle Physics
Volume	35
Issue number	1
DOIs	https://doi.org/10.1088/0954-3899/35/1/014029
Publication status	Published - Jan 2008
Event	3rd Europhysics Conference on Nuclear Physics in Astrophysics (NPA3) - Dresden, Germany Duration: 26 Mar 2007 → 31 Mar 2007

Keywords

NUCLEAR
ISOTOPES
STARS
STATISTICAL-MODEL CALCULATIONS
PROCESS NUCLEOSYNTHESIS
CROSS-SECTIONS
ELEMENTS
ASTROPHYSICAL REACTION-RATES
RP-PROCESS
NEUTRON-CAPTURE

Access to Document

10.1088/0954-3899/35/1/014029

0805Accepted author manuscript, 126 KB

Cite this

@article{9f7ceca0cb2240908896972bfcfadaeb,

title = "p-Process simulations with a modified reaction library",

abstract = "We have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model ('gamma-process') of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.",

keywords = "NUCLEAR, ISOTOPES, STARS, STATISTICAL-MODEL CALCULATIONS, PROCESS NUCLEOSYNTHESIS, CROSS-SECTIONS, ELEMENTS, ASTROPHYSICAL REACTION-RATES, RP-PROCESS, NEUTRON-CAPTURE",

author = "I. Dillmann and T. Rauscher and M. Heil and F. Kaeppeler and W. Rapp and F-K Thielemann",

year = "2008",

month = jan,

doi = "10.1088/0954-3899/35/1/014029",

language = "English",

volume = "35",

journal = "Journal of Physics G: Nuclear and Particle Physics",

issn = "0954-3899",

publisher = "IOP Publishing",

number = "1",

note = "3rd Europhysics Conference on Nuclear Physics in Astrophysics (NPA3) ; Conference date: 26-03-2007 Through 31-03-2007",

}

TY - JOUR

T1 - p-Process simulations with a modified reaction library

AU - Dillmann, I.

AU - Rauscher, T.

AU - Heil, M.

AU - Kaeppeler, F.

AU - Rapp, W.

AU - Thielemann, F-K

PY - 2008/1

Y1 - 2008/1

N2 - We have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model ('gamma-process') of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.

AB - We have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model ('gamma-process') of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.

KW - NUCLEAR

KW - ISOTOPES

KW - STARS

KW - STATISTICAL-MODEL CALCULATIONS

KW - PROCESS NUCLEOSYNTHESIS

KW - CROSS-SECTIONS

KW - ELEMENTS

KW - ASTROPHYSICAL REACTION-RATES

KW - RP-PROCESS

KW - NEUTRON-CAPTURE

U2 - 10.1088/0954-3899/35/1/014029

DO - 10.1088/0954-3899/35/1/014029

M3 - Article

SN - 0954-3899

VL - 35

JO - Journal of Physics G: Nuclear and Particle Physics

JF - Journal of Physics G: Nuclear and Particle Physics

IS - 1

M1 - 014029

T2 - 3rd Europhysics Conference on Nuclear Physics in Astrophysics (NPA3)

Y2 - 26 March 2007 through 31 March 2007

ER -

p-Process simulations with a modified reaction library

Abstract

Keywords

Access to Document

Fingerprint

Cite this