1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engNuclear matter with hyperon in neutron star under nuclear physics with double strangeness - KMI - Nagoya Universityrich600338<blockquote class="wp-embedded-content" data-secret="rAJy5xHP4c"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/947/">Nuclear matter with hyperon in neutron star under nuclear physics with double strangeness</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/947/embed/#?secret=rAJy5xHP4c" width="600" height="338" title="“Nuclear matter with hyperon in neutron star under nuclear physics with double strangeness” — KMI - Nagoya University" data-secret="rAJy5xHP4c" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
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Mixing of hyperons was strongly suggested in neutron stars to support their masses (typically ~1.4 M◎ , where M◎ is a solar mass). Although three body forces with nucleon(N) and hyperon are introduced to support the recent observed massive neutron star with (1.97 +/- 0.04)M◎, some other theorists claim that almost all model under hyperon or boson condensate can be ruled out. Appearance of hyperon around the core in neutron star is supposed to be naïve concept due to a …