316 research outputs found
Experimental Be production cross section from the Li(p,n)Be reaction at E MeV
The Li(p,n)Be reaction is widely used as neutron source for neutron
induced reaction cross section measurements, and for Be radioactive source
production. There are two prominent structures in the excitation function, a
narrow resonance between MeV, and a broad peak, around
MeV. There are tension between the experimental data sets
both in the position and the width of this latter structure, as well as in the
absolute scale of the data. In the present work the Li(p,n)Be reaction
is investigated using the activation technique, with the aim of providing
comprehensive cross section data covering the second structure and connecting
prior literature data sets. The irradiations were performed with the Atomki
cyclotron accelerator with pairs of thin foil targets, thus with precisely
controlled reaction energy in the range of E MeV. After
the irradiations the activity of the samples was measured using a high-purity
germanium detector. The energy uncertainty of the new data points is much
smaller than in any of the previous works, while the cross section uncertainty
is comparable with the most precise literature data. A consistent data set was
obtained connecting the most recent and most precise literature data sets. With
the new data the absolute magnitude of the Li(p,n)Be reaction cross
section is constrained and became more precise.Comment: typos correcte
Investigation of alpha-induced reactions on 130Ba and 132Ba and their importance for the synthesis of heavy p nuclei
Captures of alpha particles on the proton-richest Barium isotope, 130Ba, have
been studied in order to provide cross section data for the modeling of the
astrophysical gamma process. The cross sections of the 130Ba(alpha,gamma)134Ce
and 130Ba(alpha,n)133Ce reactions have been measured with the activation
technique in the center-of mass energy range between 11.6 and 16 MeV, close
above the astrophysically relevant energies. As a side result, the cross
section of the 132Ba(alpha,n)135Ce reaction has also been measured. The results
are compared with the prediction of statistical model calculations, using
different input parameters such as alpha+nucleus optical potentials. It is
found that the (alpha,n) data can be reproduced employing the standard
alpha+nucleus optical potential widely used in astrophysical applications.
Assuming its validity also in the astrophysically relevant energy window, we
present new stellar reaction rates for 130Ba(alpha,gamma)134Ce and
132Ba(alpha,gamma)136Ce and their inverse reactions calculated with the SMARAGD
statistical model code. The highly increased 136Ce(gamma,alpha)132Ba rate
implies that the p nucleus 130Ba cannot directly receive contributions from the
Ce isotopic chain. Further measurements are required to better constrain this
result.Comment: Accepted for publication in Phys. Rev.
Chaotic Phase Synchronization in Bursting-neuron Models Driven by a Weak Periodic Force
We investigate the entrainment of a neuron model exhibiting a chaotic
spiking-bursting behavior in response to a weak periodic force. This model
exhibits two types of oscillations with different characteristic time scales,
namely, long and short time scales. Several types of phase synchronization are
observed, such as 1 : 1 phase locking between a single spike and one period of
the force and 1 : l phase locking between the period of slow oscillation
underlying bursts and l periods of the force. Moreover, spiking-bursting
oscillations with chaotic firing patterns can be synchronized with the periodic
force. Such a type of phase synchronization is detected from the position of a
set of points on a unit circle, which is determined by the phase of the
periodic force at each spiking time. We show that this detection method is
effective for a system with multiple time scales. Owing to the existence of
both the short and the long time scales, two characteristic phenomena are found
around the transition point to chaotic phase synchronization. One phenomenon
shows that the average time interval between successive phase slips exhibits a
power-law scaling against the driving force strength and that the scaling
exponent has an unsmooth dependence on the changes in the driving force
strength. The other phenomenon shows that Kuramoto's order parameter before the
transition exhibits stepwise behavior as a function of the driving force
strength, contrary to the smooth transition in a model with a single time
scale
Cross section measurements for γ-process studies using a LEPS detector
T Szücs, GG Kiss, T Rauscher1, Zs Török, Z Halász, Zs Fülöp, Gy Gyürky and E Somorjai, 'Cross section measurements for Y-process studies using a LEPS detector', Journal of Physics: Conference Series, Vol 665(1), 012041, Jan 2016, Published under licence by IOP Publishing Ltd. The version of record is available online via doi: 10.1088/1742-6596/665/1/012041 Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence.In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studies. These studies are intended to enlarge the limited experimental database from α-induced reactions on nuclei in the heavier mass range of the γ -process. In all presented cases the activation method was used. The details of the cross section measurements and preliminary results on115In(α,n)118mSb, 115In(α,γ)119Sb; 162Er(α,n)165Yb, 162Er(α,γ)166Yb, 164Er(α,n)167Yb, 166Er(α,n)169Yb; 191Ir(α,n)194Au, 191Ir(α,γ)195Au, 193Ir(α,n)196mAu, 193Ir(α,n)196Au reactions are presented.Peer reviewedFinal Published versio
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
Alpha induced reaction cross section measurements on 162Er for the astrophysical γ process
Funding Details: NSF, National Science Foundation. ©2014 Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/3.0/). Funded by SCOAP3The cross sections of the Er162(α,γ)Yb166 and Er162(α,n)Yb165 reactions have been measured for the first time. The radiative alpha capture reaction cross section was measured from Ec.m.=16.09MeV down to Ec.m.=11.21MeV, close to the astrophysically relevant region (which lies between 7.8 and 11.48 MeV at 3 GK stellar temperature). The Er162(α,n)Yb165 reaction was studied above the reaction threshold between Ec.m.=12.19 and 16.09MeV. The fact that the Er162(α,γ)Yb166 cross sections were measured below the (α,n) threshold at first time in this mass region opens the opportunity to study directly the α-widths required for the determination of astrophysical reaction rates. The data clearly show that compound nucleus formation in this reaction proceeds differently than previously predicted. © 2014 Elsevier B.V.Peer reviewedFinal Published versio
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