NP Explaining Light-Nuclei Produ... | U.S. DOE Office of Science(SC)
Researchers now suggest a microscopic mechanism that might explain why the nuclei survive these harsh conditions. Knowing how energetic heavy-ion collisions produce light atomic nuclei (with just a few protons and neutrons) will help to find a sought-after critical point.
TUNL Nuclear Data Project
2021年11月18日 · Live Chart of Nuclides - IAEA: Allows to search and plot nuclear structure and nuclear decay data interactively. AME-Viewer: Java utility for interacting and comparing atomic mass data from the Atomic Mass Data Center 2020 mass evaluation. Vesrion: 17-November-2023, Date updated: 27-November-2023.
Light-nuclei production in collisions at GeV within a …
2024年1月31日 · We present results of simulations of light-nuclei production in collisions at a collision energy of GeV within the updated Three-fluid Hydrodynamics-based Event Simulator Extended by UrQMD (ultrarelativistic quantum molecular dynamics) final State interactions (THESEUS). The results are compared with recent STAR data.
The Light Nuclei - SpringerLink
The light nuclei with mass number A = 5 to 20 have been widely studied during the past 30 years. Each year over 1,000 papers are published reporting theoretical and experimental studies of these nuclei. Why is so much attention paid to the nuclei with A = 5 – 20?
Light Nuclei - Physics of Atomic Nuclei - Wiley Online Library
2017年2月3日 · The shell-model configurations are the simplest in light nuclei. Only for the ground states of doubly-magic nuclei and adjacent nuclei with one valence particle or one hole, the shell model is capable of predicting the ground state unambiguously.
Overview of light nuclei production in relativistic heavy-ion ...
2021年1月1日 · We briefly overview motivations, some recent results and challenges in studying light nuclei production in relativistic heavy ion collisions.
major goal in nuclear physics is to understand nuclear structure and dynamics in terms of un-derlying interactions occurring between individual nucleons. Studies grounded on this basic picture of the nucleus are referred to as ab initio.
Solving for nuclear structure in light nuclei
2020年11月19日 · Her recent publication, “Weak Transitions in Light Nuclei,” in November’s Frontiers in Physics, contributes to a body of increasingly accurate, descriptive calculations of nuclear structure and reactions.
The lessons learned from ephemeral nuclei | Physics Today | AIP …
2 天之前 · For light nuclei, particle emission dominates over beta decay. But for the heavier elements—and deep in the proton metastable region, especially when Z is even—weak decays can prevail. On the neutron-rich side, nuclei heavier than 24 O (N = 16) strain the definition of a nucleus. Only the presence of finite angular momentum, which generates ...
In order to construct the models to predict the s isotope productions, it is necessary to know the neutron-capture cross sections of various nuclei at stellar neutron energy. The reaction cross section is also playing an important role in the inhomogeneous big bang models.
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