Published December 2018 | Version v1
Book

Structural properties of rotating hybrid stars with color - superconducting quarks matter

  • 1. Department of Physics, Himachal Pradesh University, Shimla (India)

Description

We construct the mixed phase of equation of state (EOS) made up of the hadron matter and quark matter by employing the Glendenning construction for hybrid compact star. In order to the properties of a rapidly rotating Hybrid Neutron Star, we should first construct the Equation of State of the star

Part of:
Proceedings of the DAE international symposium on nuclear physics. V. 63

Additional details

Publishing Information

Publisher
Bhabha Atomic Research Centre
Imprint Place
Mumbai (India)
Imprint Title
Proceedings of the DAE international symposium on nuclear physics. V. 63
Imprint Pagination
1300 p.
Journal Page Range
p. 782-783

Conference

Title
63. DAE international symposium on nuclear physics
Dates
10-14 Dec 2018
Place
Mumbai (India)

INIS

Country of Publication
India
Country of Input or Organization
India
INIS RN
50011893
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
EQUATIONS OF STATE; GRAVITATIONAL WAVES; NEUTRON STARS; QUARK MATTER; QUASI PARTICLES
Descriptors DEC
EQUATIONS; MATTER; STARS

Optional Information

Notes
8 refs., 1 fig., 1 tab.