Published July 1, 2018 | Version v1
Journal article

Study Of EoS Dependence of SNe via Relic Supernova Neutrino Spectrum

  • 1. Mechanical Engineering Department, Meisei University, 2-1-1 Hodokubo, Hino, Tokyo 191-8506 (Japan)
  • 2. National Astronomical Observatory of Japan 2-21-1 Osawa, Mitaka, Tokyo, 181-8588 (Japan)

Description

The energy spectrum of relic supernova neutrinos (RSNs) tells us valuable information about neutrinos emitted from the core-collapsed SNe and their cosmological evolution. Recent astronomical observations and theoretical studies of SNe give new insights on stellar evolution, which also infuence supernova explosion mechanism. The RSN energy spectrum is an important tool to investigate these Findings. We show the results of the RSN spectrum based on a variety of astronomical scenarios, which include different supernova occurance, the cosmic star formation history, and metallicity dependent initial mass function. They reveal the signature of nuclear EoS dependence, which appears robustly in spite of the different scenarios. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/1056/1/012026

Additional details

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
1056
Journal Issue
1
Journal Page Range
[6 p.]
ISSN
1742-6596

Conference

Title
Conference on Neutrino and Nuclear Physics
Acronym
CNNP2017
Dates
17-21 Oct 2017
Place
Catania (Italy)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
53013564
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
EMISSION; ENERGY SPECTRA; METALLICITY; NEUTRINOS; STAR EVOLUTION
Descriptors DEC
ELEMENTARY PARTICLES; EVOLUTION; FERMIONS; LEPTONS; MASSLESS PARTICLES; SPECTRA