A Simulation Study on the Effect of Cavity Shapes on the Penetration of Linear Shaped Charges with Curved Liners

The finite element models of curved-liner shaped charges penetrating aluminum-alloy thin plates were constructed with the ANSYS/LS-DYNA software to analyze the effect of cavity shapes on the charge penetration with curved liners. The cavity height, radius, and spatial dimensions were numerically simulated. Simulation results indicate that these properties are important factors in determining the penetration of curved-liner charges. The penetration depth exhibits an initial increase followed by a decrease with the fixed cavity radius. When the cavity height is fixed, the penetration depth decreases with the cavity radius. When the cavity is semicircular, the penetration depth first increases and then decreases with the cavity radius and height.Построены конечноэлементные модели кумулятивных зарядов со сложнопрофильной облицовкой, проникающих через тонкие пластины из алюминиевого сплава. Использовано программное обеспечение ANSYS/LS-DYNA для анализа влияния формы выемки на их проницаемость. Выполнены численные расчеты высоты, радиуса и пространственных размеров выемки. Показано, что эти характеристики являются важными факторами при определении проницаемости зарядов. Глубина проникновения увеличивается, а затем уменьшается с увеличением высоты выемки при постоянном радиусе. При фиксированной высоте глубина проникновения уменьшается с увеличением радиуса. При полуокружной выемке глубина проникновения увеличивается, затем уменьшается с увеличением ее радиуса и высоты

Effects of different probiotics on the gut microbiome and metabolites in the serum and caecum of weaning piglets

The objective of the study was to determine the effects of antibiotics, yeast culture (YC), and Lactobacillus culture (LC) on the gut microbiome and metabolites in the serum and caecum of weaning piglets. Twenty-four weaning piglets were divided into four treatment groups: control, antibiotic (1% chlortetracycline), 1.8% yeast culture (YC), and 1.6% Lactobacillus culture groups (LC). Each group had six replicated pens with one pig per pen. Feed and water were available ad libitum. Dietary supplementation with antibiotics, YC and LC increased the abundance of phylum, Firmicutes, and decreased the abundance of phylum, Proteobacteria. Beneficial bacteria such as Lactobacillus and Megasphaera in YC and LC groups increased, whereas the proportion of Shigella was decreased. Genera Alloprevotella and Lachnospira were biomarkers in the control and antibiotic groups, respectively. Phylum, Bacteroidetes, and genus, Collinsella, were biomarkers in the YC group, and Mitsuokella, Anaerotruncus, Syntrophococcus and Sharpea were biomarkers in the LC group. Dietary supplementation with different probiotics changed the serum and caecum metabolite profiles too. Antibiotic supplementation increased the levels of D-mannose, D-glucose, and hexadecanoic acid in the serum, and the levels of myo-inositol, D-mannose and benzenepropanoic acid in the caecum. LC increased the concentrations of D-mannose, cis-9-hexadecenoic acid and heptadecanoic acid in caecum compared with the control group. YC and LC supplementation in the weaning diet could improve the abundance of beneficial bacteria by changing the concentrations of some metabolites in the serum and caecum. Therefore, dietary supplementation with YC or LC could be used as additives instead of antibiotics in weaning piglets.Keywords: antibiotic; lactobacillus culture; yeast culture; high-throughput sequencing; gas chromatography mass spectrometr

Revisiting the monopole components of effective interactions for the shell model

International audienceIn this paper, we revisit the monopole components of effective interactions forthe shell model. Without going through specific nuclei or shell gaps, universalroles of central, tensor, and spin–orbit forces can be proved, reflecting theintrinsic features of shell model effective interactions. For monopole matrixelements, even and odd channels of central force often have a canceling effect.However, for the contributions to the shell evolution, its even and oddchannels could have both positive or negative contributions, enhancing therole of central force on the shell structure. Tensor force is generally weakerthan central force. However, for the effect on shell evolutions, tensor force candominate or play a competitive role. A different systematics has been discoveredbetween T = 1 and 0 channels. For example, tensor force, wellestablished in the T = 0 channel, becomes uncertain in the T = 1 channel. Wecalculate the properties of neutron-rich oxygen and calcium isotopes in orderto study T = 1 channel interactions further. It is learned that the mainimprovements of empirical interactions are traced to the central force. For noncentralforces, antisymmetric spin–orbit (ALS) force, originated from manybodyperturbations or three-body force, could also play an explicit role. T = 1tensor forces are less constrained so their effect can differ in differentempirical interactions. The influence of tensor force may sometimes be canceledby many-body effects. For T = 0 channels of effective interactions,which is the main source of neutron–proton correlations, central and tensorforces are the leading components. For T = 1 channels, which can act betweenlike-particles, the request for many-body correlations could be moredemanding, so that the monopole anomaly of the T = 1 channel might be moreserious

A short revisit to Kuo-Brown effective interactions

International audienceThis paper is a short revisit to Kuo-Brown effective interaction derived from the Hamada-Johnston nucleon-nucleon potential, doneby Gerry Brown and Tom Kuo. This effective interaction, derived in year 1966, is the first attempt to describe nuclear structureproperties from the free nucleon-nucleon potential. Nowadays much progress has been achieved for the effective interactions inshell model. We would compare the effective interactions obtained in the 1966 paper with up-to-date shell-model interactions insd-shell and pf-shell model space. Recent knowledge of effective interactions on nuclear structure, can also be traced in the Kuo-Brown effective interaction, i.e., the universal roles of central and tensor forces, which reminds us that such discovery should benoticed much earlier

Systematic study of shell-model effective interaction in

The spin-tensor decomposition method has been used to analyse the shell model effective interactions in sd shell systematically. Almost all the interactions have been studied, including the microscopic interactions and phenomenological ones. It can be noticed that the discrepancies between the central force of microscopic interactions with the ones of empirical interactions are remarkable

Systematic study of shell-model effective interaction in sd shell

The spin-tensor decomposition method has been used to analyse the shell model effective interactions in sd shell systematically. Almost all the interactions have been studied, including the microscopic interactions and phenomenological ones. It can be noticed that the discrepancies between the central force of microscopic interactions with the ones of empirical interactions are remarkable

Gamow shell model description of the radiative capture reaction 8^8B(p,γ)(p,\gamma)9^9C

In low metallicity supermassive stars, the hot $pp$ chain can serve as an alternative way to produce the CNO nuclei. In the astrophysical environment of high temperature, the proton capture of $^8$B can be faster than its beta decay, thus $^8$B$(p,\gamma)$$^9$C reaction plays an important role in the hot $pp$ chain. Due to the unstable nature of $^8$B and the lack of the $^8$B beam, the measurement of $^8$B$(p,\gamma)$$^9$C reaction can only be achieved by the indirect method, and large uncertainties exist. The Gamow shell model in the coupled-channel representation (GSM-CC) is applied to study the proton radiative capture reaction $^8$B$(p,\gamma)$$^9$C. For the calculation of the $^8$B$(p,\gamma)$$^9$C astrophysical factors, all E1, M1, and E2 transitions from the initial continuum states to the final bound states ${3/2}_1^-$of $^9$C are considered. The resonant capture to the first resonant state ${1/2}_1^-$ of $^{9}$C is also calculated. The experimental low-energy levels and the proton emission threshold in $^9$C are reproduced by the GSM-CC. The calculated astrophysical factors agrees with the existed experimental data from the indirect measurements. The reaction rates from the direct capture and resonant capture are calculated for the temperature range of astrophysical interest. The calculated total astrophysical $S$ factor is dominated by the E1 transition to the ground state of $^9$C. The GSM-CC calculations suggest that $S$ first increase with the energy of the center of mass $E_{\rm c.m.}$, and then decrease with the energy. This agrees with the existing data, which has smaller values at around zero energy and larger value in the energy range of 0.2 MeV $\leq E_{\rm c.m.} \leq$ 0.6 MeV

Gamow shell model description of the radiative capture reaction 8^8Li(n,γ)(n,\gamma) 9^9Li

International audienceThe $^8$Li$(n,\gamma)$$^9$Li reaction plays a critical role in several reaction chains leading to the nucleosynthesis of $A>12$ nuclei. Due to unstable nature of $^8$Li and the unavailability of neutron targets, direct measurements of this reaction are exceedingly difficult. Only upper limits of this cross section, provided by the indirect experiments, have been obtained so far. In this work, we use the Gamow shell model (GSM) in the coupled-channel representation (GSM-CC) to study the properties of $^9$Li and the radiative capture reaction $^8$Li$(n,\gamma)$$^9$Li. In GSM-CC calculations, a translationally invariant Hamiltonian is used with a finite-range two-body interaction tuned to reproduce the low-energy spectra of $^{8-9}$Li. In the calculation of $^8$Li$(n,\gamma)$$^9$Li cross section, all relevant E1, M1, and E2 transitions from the initial continuum states to the final bound states ${3/2}_1^-$, ${1/2}_1^-$ and the resonance ${5/2}_1^-$ of $^9$Li are included. The GSM-CC approach reproduces the experimental low-energy spectrum, neutron emission threshold, and spectroscopic factors in $^9$Li. The calculated reaction rate is consistent with the experimental upper limit of the reaction rate obtained in the indirect measurements at stellar energies. The GSM-CC calculations suggest that the $^8$Li$(n,\gamma)$$^9$Li reaction does not reduce significantly heavy-element production via the main chain $^7$Li($n,\gamma$)$^8$Li($\alpha,n$)$^{11}$B($n,\gamma$)$^{12}$B($\beta^+$)$^{12}$C. Major contribution to the calculated cross section is given by the direct E1 transition to the ground state of $^8$Li. The contribution of excited states to the reaction rate does not exceed $\sim$20% of the total reaction rate