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Studying compact star equation of st...
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Studying compact star equation of states with general relativistic initial data approach
Record Type:
Electronic resources : Monograph/item
Title/Author:
Studying compact star equation of states with general relativistic initial data approachby Enping Zhou.
Author:
Zhou, Enping.
Published:
Singapore :Springer Singapore :2020.
Description:
xviii, 78 p. :ill., digital ;24 cm.
Contained By:
Springer eBooks
Subject:
Compact objects (Astronomy)Mathematical models.
Online resource:
https://doi.org/10.1007/978-981-15-4151-3
ISBN:
9789811541513$q(electronic bk.)
Studying compact star equation of states with general relativistic initial data approach
Zhou, Enping.
Studying compact star equation of states with general relativistic initial data approach
[electronic resource] /by Enping Zhou. - Singapore :Springer Singapore :2020. - xviii, 78 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Backgrounds -- Tidal deformability of strange star -- Maximum mass of rotating strange star -- Triaxially rotating strange star -- Conclusion and Discussion.
This book focuses on the equation of state (EoS) of compact stars, particularly the intriguing possibility of the "quark star model." The EoS of compact stars is the subject of ongoing debates among astrophysicists and particle physicists, due to the non-perturbative property of strong interaction at low energy scales. The book investigates the tidal deformability and maximum mass of rotating quark stars and triaxially rotating quark stars, and compares them with those of neutron stars to reveal significant differences. Lastly, by combining the latest observations of GW170817, the book suggests potential ways to distinguish between the neutron star and quark star models.
ISBN: 9789811541513$q(electronic bk.)
Standard No.: 10.1007/978-981-15-4151-3doiSubjects--Topical Terms:
860203
Compact objects (Astronomy)
--Mathematical models.
LC Class. No.: QB843.N4 / Z468 2020
Dewey Class. No.: 523.8874
Studying compact star equation of states with general relativistic initial data approach
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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.
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Physics and Astronomy (Springer-11651)
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EB QB843.N4 Z63 2020 2020
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https://doi.org/10.1007/978-981-15-4151-3
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