Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817

Keyphrases

• Afterglow 20%
• Allowed Regions 20%
• Binary Neutron Star Mergers 20%
• Current Constraint 20%
• Disk Wind 20%
• Ejecta 100%
• Electromagnetic Counterparts 20%
• Electromagnetic Observation 20%
• Electromagnetic Signal 20%
• Electromagnetic Waves 20%
• Equation of State 20%
• Gamma-ray Bursts 40%
• Gravitational Waves 40%
• GW170817 100%
• High Density 20%
• Jet Power 20%
• Kilonova 60%
• Lanthanides 20%
• Likelihood Probability 20%
• Maximum Mass 100%
• Mmax 100%
• Model-dependent 20%
• Multi-messenger Observations 100%
• Neutron Star Equation of State 20%
• Neutron Star Radii 20%
• Neutron Stars 100%
• Parameter Space 20%
• Radio Emission 20%
• Radioactive Decay 20%
• Rotational Energy 20%
• Shock 20%
• Synchrotron 20%
• Tight 20%
• X-ray 20%

Physics

• Afterglow 20%
• Black Holes 20%
• Earth Observing System 20%
• Ejecta 100%
• Electromagnetic Radiation 20%
• Electromagnetism 60%
• Equations of State 40%
• Gamma Ray Burst 40%
• Gravitational Wave 40%
• Neutron Star Mergers 20%
• Neutron Stars 100%
• Radio Emission 20%
• Radioactive Decay 20%
• Rare Earth Element 20%
• Synchrotron 20%

Medicine and Dentistry

• Lanthanide 100%
• Shock (Circulatory) 100%
• Synchrotron 100%