Heavy Element Nucleosynthesis

This contribution deals with the important subject of the nucleosynthesis of heavy elements in the Galaxy. After an overview of several observational features, the physical processes responsible mainly for the formation of heavy elements will be described and linked to possible stellar sites and to...

Full description

Bibliographic Details
Main Author: El Eid Mounib F.
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201818401007
_version_ 1819137062295568384
author El Eid Mounib F.
author_facet El Eid Mounib F.
author_sort El Eid Mounib F.
collection DOAJ
description This contribution deals with the important subject of the nucleosynthesis of heavy elements in the Galaxy. After an overview of several observational features, the physical processes responsible mainly for the formation of heavy elements will be described and linked to possible stellar sites and to galactic chemical evolution. In particular, we focus on the neutron-capture processes, namely the s-process (slow neutron capture) and the r-process (rapid neutron capture) and discuss some problems in connection with their sites and their outcome. The aim is to give a brief overview on the exciting subject of the heavy element nucleosynthesis in the Galaxy, emphasizing its importance to trace the galactic chemical evolution and illustrating the challenge of this subject.
first_indexed 2024-12-22T10:44:54Z
format Article
id doaj.art-49ab83a4a6b7474d90669099f4fe636e
institution Directory Open Access Journal
issn 2100-014X
language English
last_indexed 2024-12-22T10:44:54Z
publishDate 2018-01-01
publisher EDP Sciences
record_format Article
series EPJ Web of Conferences
spelling doaj.art-49ab83a4a6b7474d90669099f4fe636e2022-12-21T18:28:57ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011840100710.1051/epjconf/201818401007epjconf_ena2018_01007Heavy Element NucleosynthesisEl Eid Mounib F.This contribution deals with the important subject of the nucleosynthesis of heavy elements in the Galaxy. After an overview of several observational features, the physical processes responsible mainly for the formation of heavy elements will be described and linked to possible stellar sites and to galactic chemical evolution. In particular, we focus on the neutron-capture processes, namely the s-process (slow neutron capture) and the r-process (rapid neutron capture) and discuss some problems in connection with their sites and their outcome. The aim is to give a brief overview on the exciting subject of the heavy element nucleosynthesis in the Galaxy, emphasizing its importance to trace the galactic chemical evolution and illustrating the challenge of this subject.https://doi.org/10.1051/epjconf/201818401007
spellingShingle El Eid Mounib F.
Heavy Element Nucleosynthesis
EPJ Web of Conferences
title Heavy Element Nucleosynthesis
title_full Heavy Element Nucleosynthesis
title_fullStr Heavy Element Nucleosynthesis
title_full_unstemmed Heavy Element Nucleosynthesis
title_short Heavy Element Nucleosynthesis
title_sort heavy element nucleosynthesis
url https://doi.org/10.1051/epjconf/201818401007
work_keys_str_mv AT eleidmounibf heavyelementnucleosynthesis