𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Data needs for the astrophysical p-process

✍ Scribed by Zs. Fülöp; Gy. Gyürky; E. Somorjai


Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
365 KB
Volume
758
Category
Article
ISSN
0375-9474

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Nuclear structure studies for the astrop
✍ B. Pfeiffer; K.-L. Kratz; F.-K. Thielemann; W.B. Walters 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 767 KB

The production of the heaviest elements in nature occurs via the r-process, i.e. a combination of rapid neutron captures, the inverse photodisintegrations, and slower β --decays, β-delayed processes as well as fission and possibly interactions with intense neutrino fluxes. A correct understanding an

Radiative cooling in numerical astrophys
✍ Allard Jan van Marle; Rony Keppens 📂 Article 📅 2011 🏛 Elsevier Science 🌐 English ⚖ 917 KB

Energy loss through optically thin radiative cooling plays an important part in the evolution of astrophysical gas dynamics and should therefore be considered a necessary element in any numerical simulation. Although the addition of this physical process to the equations of hydrodynamics is straight

DISCUSSION on Data Needs for Molecular H
✍ U. Fantz; P. T. Greenland 📂 Article 📅 2002 🏛 John Wiley and Sons 🌐 English ⚖ 74 KB

A discussion on data needs for molecular hydrogen modelling and spectroscopy formed part of the WHYPE workshop. Greenland and Fantz led the discussion, and stressed: 1. All the data mentioned below are needed for D 2 , D + 2 , HD, HD + as well as H 2 , H + 2 etc. In fact in many cases, for fusion p