103 research outputs found
Neutrino reactions on La and Ta via charged and neutral currents by the Quasi-particle Random Phase Approximation (QRPA)
Cosmological origins of the two heaviest odd-odd nuclei, La and
Ta, are believed to be closely related to the neutrino-process. We
investigate in detail neutrino-induced reactions on the nuclei. Charged current
(CC) reactions, BaLa and HfTa, are calculated by the standard Quasi-particle Random Phase
Approximation (QRPA) with neutron-proton pairing as well as neutron-neutron,
proton-proton pairing correlations. For neutral current (NC) reactions,
La{La} and TaTa, we generate ground and excited states of odd-even target nuclei,
La and Ta, by operating one quasi-particle to even-even nuclei,
Ba and Hf, which are assumed as the BCS ground state. Numerical
results for CC reactions are shown to be consistent with recent semi-empirical
data deduced from the Gamow-Teller strength distributions measured in the
(He, t) reaction. Results for NC reactions are estimated to be smaller by
a factor about 4 5 rather than those by CC reactions. Finally, cross
sections weighted by the incident neutrino flux in the core collapsing
supernova are presented for further applications to the network calculations
for relevant nuclear abundances
Neutrino induced reactions related to the -process nucleosynthesis of Nb and Tc
It has recently been proposed that Nb and Tc may
have been formed in the -process. We investigate the neutrino induced
reactions related to the -process origin of the two odd-odd nuclei. The
main neutrino reactions for Nb are the charged-current (CC)
Zr()Nb and the neutral-current (NC) Nb( n)Nb reactions. The main
reactions for Tc, are the CC reaction
Mo()Tc and the NC reaction Ru( p)Tc. Our calculations are carried
out using the quasi-particle random phase approximation. Numerical results are
presented for the energy and temperature dependent cross sections. Since charge
exchange reactions by neutrons may also lead to the formation of
Nb and Tc, we discuss the feasibility of the
Mo(n,p)Nb and Ru(n,p)Tc reactions to produce these
nuclei.Comment: 21 pages, 8 figure
Neutrino self-interaction and MSW effects on the supernova neutrino-process
We calculate the abundances of Li, B, Nb, Tc,
La, and Ta produced by neutrino induced reactions in a
core-collapse supernova explosion. We consider the modification by
self-interaction (-SI) near the neutrinosphere and the
Mikheyev-Smirnov-Wolfenstein effect in outer layers for time-dependent neutrino
energy spectra. Abundances of Li and heavy isotopes Nb, Tc
and La are reduced by a factor of 1.5-2.0 by the -SI. In contrast,
B is relatively insensitive to the -SI. We find that the abundance
ratio of heavy to light nucleus, La/B, is sensitive to the
neutrino mass hierarchy, and the normal mass hierarchy is more likely to be
consistent with the solar abundances
Comprehensive Analyses of the Neutrino-Process in the Core-collapsing Supernova
We investigate the neutrino flavor change effects due to neutrino
self-interaction, shock wave propagation as well as matter effect on the
neutrino process of the core-collapsing supernova. For the hydrodynamics, we
use two models: a simple thermal bomb model and a specified hydrodynamic model
for SN1987A. As a pre-supernova model, we take an updated model adjusted to
explain the SN1987A employing recent development of the reaction
rates for nuclei near the stability line . As for the neutrino
luminosity, we adopt two different models: equivalent neutrino luminosity and
non-equivalent luminosity models. The latter is taken from the synthetic
analyses of the CCSN simulation data which involved quantitatively the results
obtained by various neutrino transport models. Relevant neutrino-induced
reaction rates are calculated by a shell model for light nuclei and a
quasi-particle random phase approximation model for heavy nuclei. For each
model, we present abundances of the light nuclei (Li, Be, B and
C) and heavy nuclei (Nb, Tc, La and Ta)
produced by the neutrino-process. The light nuclei abundances turn out to be
sensitive to the Mikheyev-Smirnov-Wolfenstein region around ONeMg region while
the heavy nuclei are mainly produced prior to the MSW region. Through the
detailed analyses of the numerical abundances, we find that neutrino
self-interaction becomes a key ingredient in addition to the MSW effect for
understanding the neutrino process and the relevant nuclear abundances.
However, the whole results are shown to depend on the adopted neutrino
luminosity scheme. Detailed evaluations of the nuclear abundances for the two
possible neutrino mass hierarchies are performed with the comparison to the
available meteorite analyses data. The normal mass hierarchy is shown to be
more compatible with the meteoritic data
Pseudo scalar contributions to light-by-light correction of muon g-2 in AdS/QCD
We have performed a holographic calculation of the hadronic contributions to
the anomalous magnetic moment of the muon, using the gauge/gravity duality. We
study a model of holographic QCD in the five dimensional AdS background with a
hard-wall cutoff. Both 5D SU(2) and U(3) flavor gauge symmetries are considered
for the neutral pion, eta and eta' contributions to the hadronic corrections.
We find the total light-by-light contributions of pseudo scalars to the muon
anomalous magnetic moment, a_mu=10.7 x 10^(-10), which is consistent with
previous estimates, based on other approaches.Comment: v3. 13 pages, 6 figures, slightly expanded and reorganized for
clarit
Modelling the Effect of Temperature on Respiration Rate of Fresh Cut Papaya (Carica papaya L.) Fruits.
A respiration rate (RR) model based on Peleg’s equation was developed for predicting RRs of fresh cut papaya. Respiration data for fresh cut papaya at 3/4 maturity were generated at temperatures 5, 10, 15, 20, 25 and 30°C using a closed system. RRs was found to be significantly influenced by storage temperature and increased from 0.021 to 0.289 mL[O2]/kg·h and 0.063 to 0.393 mL[CO2]/kg·h as a function of O2 and CO2 gas concentrations, respectively. Peleg’s constant K 1 and K 2 were obtained from linear regression analysis using GraphPad Prism 5.0 software and regression coefficients have good fit with values close to unity. The model was verified to assess the capability of its predictability of the RRs over the temperatures. There was good agreement with the experimentally estimated RRs. Information derived from the model can contribute in the design of successful modified atmospheric systems for storage of fresh cut papaya
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