Exploring hadron physics in black hole formations: A new promising target of neutrino astronomy

HANDLE オープンアクセス

抄録

The detection of neutrinos from massive stellar collapses can teach us a great deal not only about source objects but also about microphysics working deep inside them. In this study we discuss quantitatively the possibility to extract information on the properties of dense and hot hadronic matter from neutrino signals coming out of black-hole-forming collapses of nonrotational massive stars. Based on our detailed numerical simulations we evaluate the event numbers for SuperKamiokande, with neutrino oscillations fully taken into account. We demonstrate that the event numbers from a Galactic event are large enough not only to detect but also to distinguish one hadronic equation of state from another by our statistical method, assuming the same progenitor model and nonrotation. This means that the massive stellar collapse can be a unique probe into hadron physics and will be a promising target of the nascent neutrino astronomy.

収録刊行物

関連プロジェクト

もっと見る

詳細情報 詳細情報について

  • CRID
    1050282677089667456
  • NII論文ID
    120002314283
  • ISSN
    15507998
  • HANDLE
    2433/123317
  • 本文言語コード
    en
  • 資料種別
    journal article
  • データソース種別
    • IRDB
    • CiNii Articles
    • KAKEN

問題の指摘

ページトップへ