Published July 1, 2018
| Version v1
Journal article
Study Of EoS Dependence of SNe via Relic Supernova Neutrino Spectrum
Creators
- 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/10.1088/1742-6596/1056/1/012026Additional details
Identifiers
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