{
  "id": "0909.1012",
  "version": "v1",
  "published": "2009-09-05T09:38:19.000Z",
  "updated": "2009-09-05T09:38:19.000Z",
  "title": "Nucleosynthesis in neutrino-driven winds: influence of the nuclear physics input",
  "authors": [
    "Almudena Arcones",
    "Gabriel Martinez-Pinedo"
  ],
  "comment": "Conference proceedings: Nuclear Physics in Astrophysics IV",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We have performed hydrodynamical simulations of the long-time evolution of proto-neutron stars to study the nucleosynthesis using the resulting wind trajectories. Although the conditions found in the present wind models are not favourable for the production of heavy elements, a small enhancement of the entropy results in the production of r-process elements with A $\\approx$ 195. This allows us to explore the sensitivity of their production to the hydrodynamical evolution (wind termination shock) and nuclear physics input used.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-09-05T09:38:19.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "nuclear physics input",
      "neutrino-driven winds",
      "nucleosynthesis",
      "wind termination shock",
      "production"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "publication": {
      "doi": "10.1088/1742-6596/202/1/012007"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 830416
    }
  }
}