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Survival Times of Supramassive Neutron Stars Resulting from Binary Neutron Star Mergers
Paz Beniamini
, Wenbin Lu
Physics discipline
Research output
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Article
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peer-review
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Dive into the research topics of 'Survival Times of Supramassive Neutron Stars Resulting from Binary Neutron Star Mergers'. Together they form a unique fingerprint.
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Keyphrases
Neutron Stars
100%
Binary Neutron Star Mergers
100%
Survival Time
100%
Star Formation
22%
Energy Injection
22%
Energy Distribution
11%
Rotational Energy
11%
Total Mass
11%
Gamma-ray Bursts
11%
Binary Neutron Stars
11%
X-ray
11%
Radio Observations
11%
Short gamma-ray Bursts
11%
Blast Wave
11%
Long-lived
11%
Spin-down
11%
Electromagnetic Counterparts
11%
Radio Surveys
11%
All-sky
11%
Initial Energy
11%
Jet Formation
11%
Collapse Time
11%
Released Energy
11%
Extracted Energy
11%
Remnant Collapse
11%
Radio Transients
11%
Neutron Star Equation of State
11%
Solid Body Rotation
11%
Physics
Neutron Stars
100%
Gamma Ray Burst
12%
Star Formation
12%
Energy Distribution
6%
Transients
6%
Blast Wave
6%
Electromagnetic
6%
Black Holes
6%
Equations of State
6%