Now showing items 1-5 of 5

    • An approximation for the rp-process 

      Rembges, F.; Freiburghaus, C.; Rauscher, T.; Thielemann, F.K.; Schatz, H.; Wiescher, M. (1997-07-20)
      Hot (explosive) hydrogen burning, or the rapid proton capture process (rp-process), occurs in a number of astrophysical environments. Novae and X-ray bursts are the most prominent ones, but accretion disks around black ...
    • Astrophysics and nuclei far from stabilitys 

      Thielemann, F.K.; Kratz, K.L.; Pfeiffer, B.; Rauscher, T.; van Wormer, L.; Wiescher, M. (1994-03)
      We discuss unstable nuclei on the proton-rich and neutron rich side of stability and their properties of astrophysical relevance. The Coulomb barriers in charged-particle captures lead to a cycle pattern which is not ...
    • The endpoint of the rp-process 

      Schatz, H.; Aprahamian, A.; Brown, B.A.; Gorres, J.; Herndl, H.; Kratz, K.L.; Moller, P.; Pfeiffer, B.; Rauscher, T.; Rembges, J.F.; Thielemann, F.K.; Wiescher, M.; vanWormer, L. (1997-08-04)
    • Production of heavy-elements in inhomogeneous cosmologies 

      Rauscher, T.; Applegate, J.H.; Cowan, J.J.; Thielemann, F.K.; Wiescher, M. (1994-07-10)
      Baryon density inhomogeneities during big bang nucleosynthesis can result from a variety of possible causes (e.g., quantum chromodynamic and electroweak phase transitions; cosmic strings). We present here the consequences ...
    • rp-process nucleosynthesis at extreme temperature and density conditions 

      Schatz, H.; Aprahamian, A.; Gorres, J.; Wiescher, M.; Rauscher, T.; Rembges, J.F.; Thielemann, F.K.; Pfeiffer, B.; Moller, P.; Kratz, K.L.; Herndl, H.; Brown, B.A.; Rebel, H. (1998-02)
      We present nuclear reaction network calculations to investigate the influence of nuclear structure on the rp-process between Ge and Sn in various scenarios. Due to the lack of experimental data for neutron-deficient nuclei ...