Experimental cross section of 144 Sm ( α , γ ) 148 Gd and implications for the p - process

نویسندگان

  • H. P. Trautvetter
  • U. Greife
  • M. Junker
  • S. Goriely
  • M. Arnould
  • H. Oberhummer
چکیده

The cross section of the Sm(α, γ)Gd reaction has been measured at bombarding energies in the 10.513.4MeV range using an activationmethod based on the off-line α-activity measurement of the Gd residual nucleus. The long measuring time of the α-decay has required the use of etched track detectors. The resulting cross sections and astrophysical S-factors are compared to new statistical model calculations. The measured data at low energies reflect the strong energy dependence of the optical potential which is found to affect significantly our predictions of the α-capture rate.

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

Reaction Rates for 146Sm Production in Supernovae

Correlations of the 142 Nd/ 144 Nd ratio with the Sm/Nd ratio in some meteorites have been previously explained by the-decay of long-lived 146 Sm. In order to account for these observations, a necessary production ratio for 146 Sm/ 144 Sm in the-process of 0.1{0.7 was deduced. The ratio (148 Gd(,n) 147 Gd)/(148 Gd(,) 144 Sm), which plays the dominant role in the production of 146 Sm/ 144 Sm, ha...

متن کامل

Study of Radiative Capture Reactions in the Astrophysical P-process

The cross sections of 70 Ge(;) 74 Se and 144 Sm(;) 148 Gd reactions have been measured over the bombarding energy ranges of 5.05 MeV<E <7.80 MeV and 10.5 MeV<E <13.4 MeV, respectively. The results are compared to statistical model calculations. The importance of further reaction studies is emphasized.

متن کامل

Measurement of lifetimes and absolute cross-sections in the region of heavy mass p – nuclei (part II)

Scientific motivation: The proton-rich nuclei heavier than Fe (the so-called p – nuclei) are produced by a combination of the (γ, n), (γ, p) and (γ, α) reactions on existing s or r nuclei at temperatures around a few GK, characteristic of explosive environments. To adequately describe the p – process nucleosynthesis, one needs reliable information on the thousands of reactions involved, but als...

متن کامل

A simple radionuclide-driven single-ion source.

We describe a source capable of producing single barium ions through nuclear recoils in radioactive decay. The source is fabricated by electroplating (148)Gd onto a silicon α-particle detector and vapor depositing a layer of BaF(2) over it. (144)Sm recoils from the alpha decay of (148)Gd are used to dislodge Ba(+) ions from the BaF(2) layer and emit them in the surrounding environment. The simu...

متن کامل

Solution of the α-potential mystery in the γ process and its impact on the Nd/Sm ratio in meteorites.

The 146Sm/144Sm ratio in the early solar system has been constrained by Nd/Sm isotope ratios in meteoritic material. Predictions of 146Sm and 144Sm production in the γ process in massive stars are at odds with these constraints, and this is partly due to deficiencies in the prediction of the reaction rates involved. The production ratio depends almost exclusively on the (γ,n)/(γ,α) branching at...

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 1998