Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-04-02
Phys.Rev.D81:083009,2010
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
7 pages, 3 figures, accepted for publication in PRD
Scientific paper
10.1103/PhysRevD.81.083009
The detection of neutrinos from massive stellar collapses can teach us a lot 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 non-rotational massive stars. Based on our detailed numerical simulations we evaluate the event numbers for SuperKamiokande with neutrino oscillations being fully taken into account. We demonstrate that the event numbers from a Galactic event are large enough not only to detect it but also to distinguish one hadronic equation of state from another by our statistical method assuming the same progenitor model and non-rotation. 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.
Nakazato Ken'ichiro
Sumiyoshi Kohsuke
Suzuki Hideyuki
Yamada Shoichi
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