English

# Item

ITEM ACTIONSEXPORT
Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission

Vincent, T., Foucart, F., Duez, M. D., Haas, R., Kidder, L. E., Pfeiffer, H. P., et al. (2020). Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission. Physical Review D, 101: 044053. doi:10.1103/PhysRevD.101.044053.

Item is

### Basic

show hide
Genre: Journal Article

### Files

show Files
hide Files
:
1908.00655.pdf (Preprint), 6MB
Name:
1908.00655.pdf
Description:
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
-
-

show

### Creators

show
hide
Creators:
Vincent, Trevor, Author
Foucart, Francois, Author
Duez, Matthew D., Author
Haas, Roland, Author
Kidder, Lawrence E., Author
Pfeiffer, Harald P.1, Author
Scheel, Mark A., Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290

### Content

show
hide
Free keywords: General Relativity and Quantum Cosmology, gr-qc,
Abstract: We present twelve new simulations of unequal mass neutron star mergers. The simulations were preformed with the SpEC code, and utilize nuclear-theory based equations of state and a two-moment gray neutrino transport scheme with an improved energy estimate based on evolving the number density. We model the neutron stars with the SFHo, LS220 and DD2 equations of state (EOS) and we study the neutrino and matter emission of all twelve models to search for robust trends between binary parameters and emission characteristics. We find that the total mass of the dynamical ejecta exceeds \$0.01M_\odot\$ only for SFHo with weak dependence on the mass-ratio across all models. We find that the ejecta have a broad electron fraction (\$Y_e\$) distribution (\$\approx 0.06-0.48\$), with mean \$0.2\$. \$Y_e\$ increases with neutrino irradiation over time, but decreases with increasing binary asymmetry. We also find that the models have ejecta with a broad asymptotic velocity distribution (\$\approx 0.05-0.7c\$). The average velocity lies in the range \$0.2c - 0.3c\$ and decreases with binary asymmetry. Furthermore, we find that disk mass increases with binary asymmetry and stiffness of the EOS. The \$Y_e\$ of the disk increases with softness of the EOS. The strongest neutrino emission occurs for the models with soft EOS. For (anti) electron neutrinos we find no significant dependence of the magnitude or angular distribution or neutrino luminosity with mass-ratio. The heavier neutrino species have a luminosity dependence on mass-ratio but an angular distribution which does not change with mass-ratio.

### Details

show
hide
Language(s):
Dates: 2019-08-012020
Publication Status: Published in print
Pages: 23 pages, 15 figures
Publishing info: -
Rev. Method: -
Identifiers: arXiv: 1908.00655
URI: http://arxiv.org/abs/1908.00655
DOI: 10.1103/PhysRevD.101.044053
Degree: -

show

show

show

### Source 1

show
hide
Title: Physical Review D
Other : Phys. Rev. D.
Source Genre: Journal
Creator(s):
Affiliations:
Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 101 Sequence Number: 044053 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: https://pure.mpg.de/cone/journals/resource/111088197762258