Pycnonuclear fusion in the curst of accreting neutron stars

ORAL

Abstract

Pycnonuclear fusion processes take place at extreme density conditions of $\rho >$10$^{10}$ g/cm$^{3}$, anticipated for the core of white dwarfs or the crust of neutron stars. A formalism was developed for predicting pycnonuclear reaction rates for neutron rich nuclei in the carbon to magnesium range. The reaction rates have been used to simulate pycnonuclear burning in the deeper crust of an accreting neutron star. The pycnonuclear reaction rates will be presented and the results of the nucleosynthesis simulations will be discussed.

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Authors

  • Mary Beard

    University of Notre Dame

  • Edward Brown

    Michigan State University

  • Leandro Gasques

    University of Lisbon, Portugal

  • Rita Lau

    Michigan State University

  • Hendrik Schatz

    Michigan State University, NSCL, Michigan State University, Michigan State University, National Superconducting Cyclotron Laboratory, and Joint Institute for Nuclear Astrophysics

  • Michael Wiescher

    University of Notre Dame

  • Dimitrji Yakovlev

    University of St. Petersburg, Russia