Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers-Reference-Cited by-同舟云学术

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Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

Published:2015-12-16 Issue:12 Volume:92 Page:
ISSN:1550-7998
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Kiuchi Kenta,Cerdá-Durán Pablo,Kyutoku Koutarou,Sekiguchi Yuichiro,Shibata Masaru

Funder

European Research Council

Grant-in-Aid for Scientific Research

Scientific Research on Innovative Area

MEXT/JSPS

RIKEN iTHES

local Spanish funds

Publisher

American Physical Society (APS)

Subject

Nuclear and High Energy Physics

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.92.124034/fulltext

Reference43 articles.

1. Calibration of the LIGO gravitational wave detectors in the fifth science run

2. Calibration and sensitivity of the Virgo detector during its second science run

3. Calibration and sensitivity of the Virgo detector during its second science run

4. Status of LCGT

5. Gamma-ray bursts as the death throes of massive binary stars

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