182 research outputs found
Coulomb suppression of the stellar enhancement factor
It is commonly assumed that reaction measurements for astrophysics should be
preferably performed in the direction of positive Q value to minimize the
impact of the stellar enhancement factor, i.e. the difference between the
laboratory rate and the actual stellar rate. We show that the stellar effects
can be minimized in the charged particle channel, even when the reaction Q
value is negative. As a demonstration, the cross section of the astrophysically
relevant 85Rb(p,n)85Sr reaction has been measured by activation between 2.16 <
Ec.m. < 3.96 MeV and the astrophysical reaction rate for (p,n) as well as (n,p)
is directly inferred from the data. The presented arguments are also relevant
for other alpha and proton-induced reactions in the p and rp processes.
Additionally, our results confirm a previously derived modification of a global
optical proton potential.Comment: submitted to PR
Precise half-life measurement of the 10 h isomer in 154Tb
The precise knowledge of the half-life of the reaction product is of crucial
importance for a nuclear reaction cross section measurement carried out with
the activation technique. The cross section of the 151Eu(alpha,n)154Tb reaction
has been measured recently using the activation method, however, the half-life
of the 10 h isomer in 154Tb has a relatively high uncertainty and ambiguous
values can be found in the literature. Therefore, the precise half-life of the
isomeric state has been measured and found to be 9.994 h +- 0.039 h. With
careful analysis of the systematic errors, the uncertainty of this half-life
value has been significantly reduced.Comment: Accepted for publication in Nuclear Physics
70Ge(p,gamma)71As and 76Ge(p,n)76As cross sections for the astrophysical p process: sensitivity of the optical proton potential at low energies
The cross sections of the 70Ge(p,gamma)71As and 76Ge(p,n)76As reactions have
been measured with the activation method in the Gamow window for the
astrophysical p process. The experiments were carried out at the Van de Graaff
and cyclotron accelerators of ATOMKI. The cross sections have been derived by
measuring the decay gamma-radiation of the reaction products. The results are
compared to the predictions of Hauser-Feshbach statistical model calculations
using the code NON-SMOKER. Good agreement between theoretical and experimental
S factors is found. Based on the new data, modifications of the optical
potential used for low-energy protons are discussed.Comment: Accepted for publication in Phys. Rev.
High precision half-life measurement of Ru, Tc and Tc with -spectroscopy
The precise knowledge of the half-life of the reaction product is of crucial
importance for a nuclear reaction cross section measurement carried out with
the activation technique. The cross section of the
Mo(,n)Ru reaction was measured recently using this
experimental approach. The preliminary results indicated that the literature
half-life of Ru, derived about half a century ago, is overestimated.
Therefore, the half-lives of Ru and its daughter isotope Tc and
Tc have been measured with high precision using -spectroscopy.
The results are t=1.6033 0.0044 h for Ru, t =
19.258 0.026 h for Tc and t = 61.96 0.24 d for
Tc. The precision of the half-life values has been increased,
consequently the recently measured Mo(,n)Ru activation
cross section will become more precise
Direct study of the alpha-nucleus optical potential at astrophysical energies using the 64Zn(p,alpha)61Cu reaction
In the model calculations of heavy element nucleosynthesis processes the
nuclear reaction rates are taken from statistical model calculations which
utilize various nuclear input parameters. It is found that in the case of
reactions involving alpha particles the calculations bear a high uncertainty
owing to the largely unknown low energy alpha-nucleus optical potential.
Experiments are typically restricted to higher energies and therefore no direct
astrophysical consequences can be drawn. In the present work a (p,alpha)
reaction is used for the first time to study the alpha-nucleus optical
potential. The measured 64Zn(p,alpha)61Cu cross section is uniquely sensitive
to the alpha-nucleus potential and the measurement covers the whole
astrophysically relevant energy range. By the comparison to model calculations,
direct evidence is provided for the incorrectness of global optical potentials
used in astrophysical models.Comment: Accepted for publication in Physical Review C as a Rapid
Communicatio
Cross section measurement of the astrophysically important 17O(p,gamma)18F reaction in a wide energy range
The 17O(p,g)18F reaction plays an important role in hydrogen burning
processes in different stages of stellar evolution. The rate of this reaction
must therefore be known with high accuracy in order to provide the necessary
input for astrophysical models.
The cross section of 17O(p,g)18F is characterized by a complicated resonance
structure at low energies. Experimental data, however, is scarce in a wide
energy range which increases the uncertainty of the low energy extrapolations.
The purpose of the present work is therefore to provide consistent and precise
cross section values in a wide energy range.
The cross section is measured using the activation method which provides
directly the total cross section. With this technique some typical systematic
uncertainties encountered in in-beam gamma-spectroscopy experiments can be
avoided.
The cross section was measured between 500 keV and 1.8 MeV proton energies
with a total uncertainty of typically 10%. The results are compared with
earlier measurements and it is found that the gross features of the 17O(p,g)18F
excitation function is relatively well reproduced by the present data.
Deviation of roughly a factor of 1.5 is found in the case of the total cross
section when compared with the only one high energy dataset. At the lowest
measured energy our result is in agreement with two recent datasets within one
standard deviation and deviates by roughly two standard deviations from a third
one. An R-matrix analysis of the present and previous data strengthen the
reliability of the extrapolated zero energy astrophysical S-factor.
Using an independent experimental technique, the literature cross section
data of 17O(p,g)18F is confirmed in the energy region of the resonances while
lower direct capture cross section is recommended at higher energies. The
present dataset provides a constraint for the theoretical cross sections.Comment: Accepted for publication in Phys. Rev. C. Abstract shortened in order
to comply with arxiv rule
- …