[PDF] Top 20 Neutron properties from light nuclei

... We have also addressed the issue of the uncertainty quantification of our results due to the truncation of the chiral expansion at a given order. In particular, we have argued that the standard procedure for error ... See full document

... exotic nuclei which will have a direct impact on the modelling of compact ...of neutron-rich isotopes with mass numbers between 80 and 160 would reduce the uncertainties in the composition of the outer ... See full document

... of nuclei starting from the constituent nucleons and the fundamental interactions among them has been a long-standing goal in nuclear ...derives from the combination of the ab initio no-core shell ... See full document

... In light nuclei the number of protons and neutrons is the same ( N = Z ) but the number of neutrons increases fast as go up to balance the repulsive force between positively charges protons so that the ... See full document

... The theoretical analysis of (p,pN ) reactions has been traditionally performed within the distorted-wave impulse approximation (DWIA) [3,19]. Nowadays, there are different models to study this type of reactions using ... See full document

... with light beam probes such as protons, deuterons or al- phas since the dawn of the first ...radioactive nuclei produced as beams has proven to be a significant experi- mental ...the light probe ... See full document

... Another difference between the (p,pn) and (p,2p) cases, that favors (p,pn) over (p,2p), stems from the difference between the p-n and p-p interactions. Between 400 MeV and 500 MeV, the np scattering cross section ... See full document

... predicted properties, noise that, thanks to the Central Limit Theorem ...ranging from quantum chemistry [12, 13] to condensed matter [14, 15], and nuclear physics ...for light nuclei and ... See full document

... have been presented with the aim of extracting neutron polarizabilities. Our results show that most of the observ- ables are quite sensitive to the polarizabilities. The elec- tric and magnetic polarizabilities ... See full document

... of light particles, in systems of various neutron-proton asymme- tries, is expected to be a probe of nuclear matter properties such as the density dependence of the symmetry energy and the ... See full document

... the properties of hot and dense nuclear matter which can be probed experimentally by measuring particle composition, longitudinal and transverse momentum distributions of different ...of light nuclei ... See full document

... cles from other direct process, which would give the same reaction products with similar energies. A complete understanding of the reaction mechanism would require coincidence measurements of the charged ... See full document

... Core-collapse supernovae are believed to be neutrino driven explosions of massive stars. At the end of its life a massive star (M > 8 M , where M is the solar mass) presents a typical onion-like structure with layers ... See full document

... closed neutron shell N = 126 – the so called last “wait- ing point” for the r-process – is located in the region of heavy neutron rich nuclei, “north-east” part of the nuclide chart, which is very ... See full document

... both nuclei and neutron stars based on the above model interaction: We study possible coexistence of K − mesons and hyperons in nuclei as the ground state of multi-strangeness nuclei ...in ... See full document

... the properties of odd-Z nuclei in the region of the most neutron-rich isotopes of elements 105 to 117 is significantly expanded by our eleven newly identified isotopes which have increased stability ... See full document

... of light nuclei having additional neutrons (compared to the N = Z ones) show a different type of clustering, with extra neutrons acting as valence particles in molecule-like ... See full document

... on neutron-rich nuclei as well as other light ...the neutron capture reactions practi- cally, we must solve the problems about the use of arti- ficial resonance parameters, the phase problem, ... See full document

... p relative motion and the obtained FWHMs for the con- sidered three cases. Due to the uncertainty principle the widths become smaller with the increase of the distance between the two clusters. We note the good agreement ... See full document

... the nuclei involved in the relation: most of the differences seen between them can be attributed to the deviations of the MSMME fit from the measured m a ... See full document