Nuclear astrophysics with radioactive ions at FAIR

Type: Article

Publication Date: 2016-01-05

Citations: 8

DOI: https://doi.org/10.1088/1742-6596/665/1/012044

Abstract

The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process, β-decay chains. These nuclei are attributed to the p and rp process.

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Works Cited by This (12)

Action Title Year Authors
+ PDF Chat Nuclear weak-interaction processes in stars 2003 K. Langanke
G. Martı́nez-Pinedo
+ PDF Chat Sensitivity of<i>r</i>‐Process Nucleosynthesis to Light‐Element Nuclear Reactions 2005 Takahiro Sasaqui
Toshitaka Kajino
Grant J. Mathews
Kaori Otsuki
T. Nakamura
+ PDF Chat The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>s</mml:mi></mml:math>process: Nuclear physics, stellar models, and observations 2011 F. Käppeler
R. Gallino
S. Bisterzo
Wako Aoki
+ Astrophysical constraints from gamma-ray spectroscopy 2005 R. Diehl
Nikos Prantzos
P. von Ballmoos
+ PDF Chat Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments 2000 K. Langanke
G. Martı́nez-Pinedo
+ X-ray binaries 2005 H. Schatz
K. E. Rehm
+ PDF Chat CONVECTIVE-REACTIVE PROTON-<sup>12</sup>C COMBUSTION IN SAKURAI'S OBJECT (V4334 SAGITTARII) AND IMPLICATIONS FOR THE EVOLUTION AND YIELDS FROM THE FIRST GENERATIONS OF STARS 2011 Falk Herwig
M. Pignatari
Paul R. Woodward
David H. Porter
Gabriel Rockefeller
Chris L. Fryer
Michael Bennett
Raphaël Hirschi
+ PDF Chat New Nuclear Reaction Flow during<i>r</i>‐Process Nucleosynthesis in Supernovae: Critical Role of Light, Neutron‐rich Nuclei 2001 M. Terasawa
Kohsuke Sumiyoshi
Toshitaka Kajino
Grant J. Mathews
I. Tanihata
+ PDF Chat Nuclear astrophysics with radioactive beams 2009 C. A. Bertulani
A. Gade
+ PDF Chat Probing the Neutron‐Capture Nucleosynthesis History of Galactic Matter 2002 James W. Truran
J. J. Cowan
C. A. Pilachowski
C. Sneden