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Studying Compact Star Equation of States with General Relativistic Initial Data Approach: Springer Theses

Autor Enping Zhou
en Limba Engleză Paperback – 4 apr 2021
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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Specificații

ISBN-13: 9789811541537
ISBN-10: 9811541531
Ilustrații: XVIII, 78 p. 23 illus., 22 illus. in color.
Dimensiuni: 155 x 235 mm
Greutate: 0.15 kg
Ediția:1st ed. 2020
Editura: Springer Nature Singapore
Colecția Springer
Seria Springer Theses

Locul publicării:Singapore, Singapore

Cuprins

Backgrounds.- Tidal deformability of strange star.- Maximum mass of rotating strange star.- Triaxially rotating strange star.- Conclusion and Discussion.

Notă biografică

Dr. Enping Zhou received his Ph.D. degree from Peking University. His research interests include pulsar observation and pulsar science, compact star physics, numerical relativity, strange quark star models, and building initial data for binary quark stars. He received “The Excellent Doctoral Dissertation” award from Peking University in 2018. 

Textul de pe ultima copertă

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. 


Caracteristici

Nominated as an outstanding Ph.D. thesis by Peking University Studies the equation of state (EoS) of compact stars with the aid of gravitational wave observations Discusses the possibility of a quark star model Presents significant differences between quark stars and neutron stars