Litcius/Paper detail

Plausible presence of new state in neutron stars with masses above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si40.svg"> <mml:mrow> <mml:mn>0.98</mml:mn> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">TOV</mml:mi> </mml:mrow> </mml:msub> </mml:mrow> </mml:math>

Mingzhe Han, Yong-Jia Huang, Shao-Peng Tang, Yi-Zhong Fan

2023Science Bulletin61 citationsDOI

Topics & Concepts

PhysicsNeutron starEquation of stateParticle physicsStarsStrangenessAstrophysicsHadronNuclear physicsQuantum mechanicsPulsars and Gravitational Waves ResearchGamma-ray bursts and supernovaeHigh-pressure geophysics and materials
Plausible presence of new state in neutron stars with masses above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si40.svg"> <mml:mrow> <mml:mn>0.98</mml:mn> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">TOV</mml:mi> </mml:mrow> </mml:msub> </mml:mrow> </mml:math> | Litcius