<?xml version="1.0" encoding="UTF-8"?>
<articles>
<article xmlns:xlink="http://www.w3.org/1999/xlink/">
  <front>
    <journal-meta>
      <journal-title>EPJ Web Conf.</journal-title>
      <abbrev-journal-title>EPJ Web Conf.</abbrev-journal-title>
      <issn/>
    </journal-meta>
    <article-meta>
      <title-group>
        <article-title>Nuclear physics in the N≈126 region relevant for the $r$ process</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <name>
            <surname>Podolyák</surname>
            <given-names>Zsolt</given-names>
          </name>
          <aff>
            <institution>CERN</institution>
          </aff>
          <aff>
            <institution>Surrey U.</institution>
          </aff>
        </contrib>
      </contrib-group>
      <pub-date pub-type="pub">
        <year>2023</year>
      </pub-date>
      <volume>279</volume>
      <fpage/>
      <lpage/>
      <self-uri xlink:href="http://cds.cern.ch/record/2884570"/>
      <self-uri xlink:href="http://cds.cern.ch/record/2884570/files/epjconf_npa-x2023_08001.pdf"/>
    </article-meta>
    <abstract>Understanding how the heavy chemical elements are made in the astrophysical $r$-process requires information on both the properties of the nuclei involved and that of the environment. The availability of experimental information on the neutron-rich N∼126 nuclei is discussed, with emphasis on phenomena specifically relevant to this region: the large role of first-forbidden $\beta$ decays, and that of the $\Delta n = 0$ selection rule in Gamow-Teller decays. The development of nuclear data bases by combining different theoretical approaches is suggested.</abstract>
  </front>
  <article-type>research-article</article-type>
  <ref/>
</article>

</articles>