Journal of Physics: Conference Series PAPER • OPEN ACCESS Related content - The Impact of Fission on R-Process The r-process nucleosynthesis during the Calculations M Eichler, A Arcones, R Käppeli et al. decompression of neutron star crust material - Variances in r-process predictions from uncertain nuclear rates Matthew Mumpower, Rebecca Surman To cite this article: S Goriely et al 2016 J. Phys.: Conf. Ser. 665 012052 and Ani Aprahamian - Discovery of a strongly r-process enhanced extremely metal-poor star LAMOST J110901.22plus075441.8 Hai-Ning Li, Wako Aoki, Satoshi Honda et View the article online for updates and enhancements. al. This content was downloaded from IP address 188.184.3.52 on 18/01/2018 at 15:57 Nuclear Physics in Astrophysics VI (NPA6) IOP Publishing Journal of Physics: Conference Series 665 (2016) 012052 doi:10.1088/1742-6596/665/1/012052 The r-process nucleosynthesis during the decompression of neutron star crust material S Goriely1,ABauswein2,H-TJanka2, S Panebianco3, J-L Sida3,J-F Lemaˆıtre3, S Hilaire4, N Dubray4 1 Institut d’Astronomie et d’Astrophysique, ULB, CP226, 1050 Bruxelles, Belgium 2 Max-Planck-Institut f¨urAstrophysik, Postfach 1317, 85741 Garching, Germany 3 CEA Saclay, Irfu/Service de Physique Nuclaire, 91191 Gif-sur-Yvette, France 4 CEA, DAM, DIF, F-91297 Arpajon, France E-mail:
[email protected] Abstract. About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid neutron capture process, or r-process, of nucleosynthesis. The identification of the astrophysics site and the specific conditions in which the r-process takes place remains, however, one of the still-unsolved mysteries of modern astrophysics.