Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: Comparing high-resolution and large-eddy simulations-Reference-Cited by-同舟云学术

Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: Comparing high-resolution and large-eddy simulations

Published:2020-11-06 Issue:10 Volume:102 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Aguilera-Miret Ricard^ORCID,Viganò Daniele^ORCID,Carrasco Federico^ORCID,Miñano Borja,Palenzuela Carlos^ORCID

Funder

Ministerio de Economía y Competitividad

H2020 European Research Council

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.102.103006/fulltext

Reference69 articles.

1. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2. Multi-messenger Observations of a Binary Neutron Star Merger

3. An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi -GBM Detection of GRB 170817A

4. INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational-wave Event GW170817

5. Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

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