Experiments on photon - induced reactions for p - process nucleosynthesis ∗

نویسنده

  • K. Sonnabend
چکیده

Photodesintegration rates – like (γ ,n), (γ ,p), and (γ ,α) – play an important role in the nucleosynthesis of the so-called p nuclei. These proton-rich, in general very low-abundant isotopes cannot be produced by neutron capture reactions. Experiments using continuous-energy bremsstrahlung and the activation technique are perfectly suited to carry out systematic surveys on (γ ,n) reactions. In addition, single cases can be studied in more detail using energy-resolved methods as provided by photon sources based on the principle of Laser-Compton backscattering or photon tagging. An overview about current results on photon-induced reactions and recent instrumental developments is given.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Direct Determination of Photodisintegration Cross Sections and the p-process

Photon-induced reactions play a key role in the nucleosynthesis of heavy neutrondeficient nuclei, the so-called p-nuclei. In this paper we review the present status of experiments on photon-induced reactions at energies of astrophysical importance and their relevance to p-process modeling.

متن کامل

Inhomogeneous Primordial Nucleosynthesis: Coupled Nuclear Reactions and Hydrodynamic Dissipation Processes

We present a detailed numerical study of inhomogeneous Big Bang nucleosynthesis where, for the first time, nuclear reactions are coupled to all significant fluctuation dissipation processes. These processes include neutrino heat transport, baryon diffusion, photon diffusive heat transport, and hydrodynamic expansion with photon-electron Thomson drag. Light element abundance yields are presented...

متن کامل

ar X iv : a st ro - p h / 96 12 04 7 v 1 5 D ec 1 99 6 Neutrino - induced nucleosynthesis and the site of the r - process

If the r-process occurs deep within a Type II supernova, probably the most popular of the proposed sites, abundances of r-process elements may be altered by the intense neutrino flux. We point out that the effects would be especially pronounced for 8 isotopes that can be efficiently synthesized by the neutrino reactions following r-process freeze-out. We show that the observed abundances of the...

متن کامل

Summary Report of Working Group on Equipment and Facilities: Stable Beams and Gamma Beams

Stable and photon beam experiments address scientific questions of paramount importance for stellar evolution and nucleosynthesis: Where are the elements produced that life depends on (carbon, nitrogen, oxygen)? How do stars evolve? Where are 50% of the elements beyond iron produced? Are there nuclear signatures to probe the core of stars, e.g., CNO neutrinos for probing the solar core metallic...

متن کامل

Neutrino-induced nucleosynthesis and the site of the r-process

If the r-process occurs deep within a Type II supernova, probably the most popular of the proposed sites, abundances of r-process elements may be altered by the intense neutrino flux. We point out that the effects would be especially pronounced for 8 isotopes that can be efficiently synthesized by the neutrino reactions following r-process freeze-out. We show that the observed abundances of the...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008