Nuclear Structure Studied from Weak and Related Processes
نویسندگان
چکیده
منابع مشابه
Nuclear Matter in Intense Magnetic Field and Weak Processes
We study the effect of magnetic field on the dominant neutrino emission processes in neutron stars.The processes are first calculated for the case when the magnetic field does not exceed the critical value to confine electrons to the lowest Landau state.We then consider the more important case of intense magnetic field to evaluate the direct URCA and the neutronisation processes. In order to es...
متن کاملAstrophysical Weak-interaction Processes and Nuclear Effective Field Theory
Low-energy nuclear weak-interaction processes play important roles in many astrophysical contexts, and effective field theory is believed to be a highly useful framework for describing these processes in a model-independent manner. I present a brief account of the basic features of the nuclear effective theory approach, and some examples of actual calculations carried out in this method. Invite...
متن کاملNuclear Structure Functions and Cumulative Processes
The authors’s point of view, based on QCD, on the nuclear quark structure is presented. Different models for explaining the EMC–effect are considered. It is also shown that cumulative production data are very useful for a better understanding of the EMC–effect and give some evidence in favor of its multiquark nature. Discovery of the EMC–effect [2] has drawn attention of the world–wide communit...
متن کاملWeak decay of uniformly accelerated protons and related processes
We investigate the weak interaction emission of spin-1/2 fermions from accelerated currents. As particular applications, we analyze the decay of uniformly accelerated protons and neutrons, and the neutrino-antineutrino emission from uniformly accelerated electrons. The possible relevance of our results to astrophysics is also discussed. 13.30.-a, 04.62.+v, 14.20.Dh, 95.30.Cq Typeset using REVTEX 1
متن کاملProjected shell model for nuclear structure and weak interaction rates
The knowledge on stellar weak interaction processes is one of the most important ingredients for resolving astrophysical questions. Study of these rates is essentially a nuclear structure problem, in which the actual decay rates are determined by the microscopic inside of nuclear many-body systems. For many astrophysically-interested questions, information on detailed nuclear level structure at...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Progress of Theoretical Physics Supplement
سال: 2013
ISSN: 0375-9687
DOI: 10.1143/ptp.48.41