409 research outputs found
Gamma-Ray Bursts Black hole accretion disks as a site for the vp-process
We study proton rich nucleosynthesis in windlike outflows from gamma-ray
bursts accretion disks with the aim to determine if such outflows are a site of
the vp-process. The efficacy of this vp-process depends on thermodynamic and
hydrodynamic factors. We discuss the importance of the entropy of the material,
the outflow rate, the initial ejection point and accretion rate of the disk. In
some cases the vp-process pushes the nucleosynthesis out to A~100 and produces
light p-nuclei. However, even when these nuclei are not produced, neutrino
induced interactions can significantly alter the abundance pattern and cannot
be neglected.Comment: 9 pages, 16 figures, accepted for publication in Phys. Rev.
Neutron Capture in the r-Process -- Do We Know Them And Does It Make Any Difference?
The r-process involves neutron-rich nuclei far off stability for which no
experimental cross sections are known. Therefore, one has to rely on theory
which might be prone to considerable uncertainties far off stability. To
investigate the impact of such uncertainties, nucleosynthesis in hot bubble
models followed completely from high-temperature NSE to low-temperature neutron
capture freeze-out were calculated with largely varied rates. Due to the
(n,gamma)-(gamma,n) equilibrium established at the onset of the r-process, only
late-time neutron captures are important which mainly modify the abundances
around the third r-process peak.Comment: 4 pages, 4 figures; contribution to Nuclei In The Cosmos VIII, to
appear in Nucl. Phys.
Changes in r-process abundances at late times
We explore changes in abundance patterns that occur late in the r process. As
the neutrons available for capture begin to disappear, a quasiequilibrium
funnel shifts material into the large peaks at A=130 and A=195, and into the
rare-earth "bump" at A=160. A bit later, after the free-neutron abundance has
dropped and beta-decay has begun to compete seriously with neutron capture, the
peaks can widen. The degree of widening depends largely on neutron-capture
rates near closed neutron shells and relatively close to stability. We identify
particular nuclei the capture rates of which should be examined experimentally,
perhaps at a radioactive beam facility.Comment: 8 pages, 14 figures included in tex
The Influence Of Neutron Capture Rates On The Rare Earth Region Of The r-Process Abundance Pattern
We study the sensitivity of the r-process abundance pattern to neutron
capture rates along the rare earth region (A~150 to A~180). We introduce the
concepts of large nuclear flow and flow saturation which determine the neutron
capture rates that are influential in setting the rare earth abundances. We
illustrate the value of the two concepts by considering high entropy conditions
favorable for rare earth peak production and identifying important neutron
capture rates among the rare earth isotopes. We also show how these rates
influence nuclear flow and specific sections of the abundance pattern.Comment: 14 pages, 7 figures, submitted to PR
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