Related papers: R-process in Low Entropy Neutrino Driven Winds
This paper has been withdrawn since a trivial proof of the result has been pointed out to the author.
During the first 20 seconds of its life, the enormous neutrino luminosity of a neutron star drives appreciable mass loss from its surface. This neutrino-driven wind has been previously identified as a likely site for the r-process. Qian &…
This paper has been withdrawn by the authors.
We explore neutrino capture during r-process nucleosynthesis in neutrino-driven ejecta from nascent neutron stars. We focus on the interplay between charged-current weak interactions and element synthesis, and we delineate the important…
Current understanding of the r-process is summarized in terms of the astrophysical sites, the yield patterns, and the role of neutrinos. The importance of observational and experimental tests is emphasized. A number of future tests…
This paper has been withdrawn by the author.
This paper has been withdrawn by the author(s),
This paper has been withdrawn by the authors because the authors excluded the paper from electronic proceedings of the conference.
We use results from long-time core-collapse supernovae simulations to investigate the impact of the late time evolution of the ejecta and of the nuclear physics input on the calculated r-process abundances. Based on the latest…
This paper has been withdrawn.
After a successful core-collapse supernova, a neutrino-driven wind develops where it is possible to synthesize lighter heavy elements ($30<Z<45$). In the early galaxy, the origin of these elements is associated to the r-process and to an…
The paper has been withdrawn because the research work is still in progress.
Neutrino-driven wind from young hot neutron star, which is formed by supernova explosion, is the most promising candidate site for r-process nucleosynthesis. We study general relativistic effects on this wind in Schwarzschild geometry in…
This paper has been withdrawn by the author.
This paper has been withdrawn.
The neutrino-driven wind cooling phase of proto-neutron stars (PNSs) follows successful supernovae. Wind models without magnetic fields or rotation fail to achieve the necessary conditions for production of the third $r-$process peak, but…
This paper has been withdrawn by the authors.
This paper has been withdrawn by the authors, due to issues concerning the use of unpublished experimental data.
This paper has been withdrawn Abstract: This paper has been withdrawn by the author due to the publication.
The paper is being withdrawn. A new submission will follow.