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This book focuses on the equation of state (EoS) of compact stars,
particularly the intriguing possibility of the "quark star model."
The EoS of compact stars is the subject of ongoing debates among
astrophysicists and particle physicists, due to the
non-perturbative property of strong interaction at low energy
scales. The book investigates the tidal deformability and maximum
mass of rotating quark stars and triaxially rotating quark stars,
and compares them with those of neutron stars to reveal significant
differences. Lastly, by combining the latest observations of
GW170817, the book suggests potential ways to distinguish between
the neutron star and quark star models.
This book focuses on the equation of state (EoS) of compact stars,
particularly the intriguing possibility of the "quark star model."
The EoS of compact stars is the subject of ongoing debates among
astrophysicists and particle physicists, due to the
non-perturbative property of strong interaction at low energy
scales. The book investigates the tidal deformability and maximum
mass of rotating quark stars and triaxially rotating quark stars,
and compares them with those of neutron stars to reveal significant
differences. Lastly, by combining the latest observations of
GW170817, the book suggests potential ways to distinguish between
the neutron star and quark star models.
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