Published December 2017 | Version v1
Book

Boson star under Cornell potential

  • 1. Department of Physics and Astrophysics, University of Delhi, Delhi (India)

Description

Signals coming from Quark Gluon Plasma (QGP) at high density and temperature can give information about evolution of the early universe expansion. Supernova explosion of universe expansion represents the phase transition in the early universe. There is formation of the compact stars after the supernova explosion. Neutron stars are one of the probable signals of early universe formation in which the quark and gluons are defined in free degree of freedom. Like neutron star, a boson star (BS) may have been formed through gravitational collapse during the primordial stages of the big bang. For these type of stars to exist there must be a stable type of BS that possesses a small mass of magnitude. However, it may possibly detect them by the gravitational radiation emitted by a pair of co-orbiting boson stars

Part of:
Proceedings of the DAE-BRNS symposium on nuclear physics. V. 62

Additional details

Publishing Information

Publisher
Bhabha Atomic Research Centre
Imprint Place
Mumbai (India)
Imprint Title
Proceedings of the DAE-BRNS symposium on nuclear physics. V. 62
Imprint Pagination
[1220 p.]
Journal Page Range
p. 846-847

Conference

Title
62. DAE-BRNS symposium on nuclear physics
Dates
20-24 Dec 2017
Place
Patiala (India)

INIS

Country of Publication
India
Country of Input or Organization
India
INIS RN
49014718
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
NEUTRON STARS; QUARK MATTER; QUARK-ANTIQUARK INTERACTIONS; SUPERNOVAE; WAVE FUNCTIONS
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; FUNCTIONS; INTERACTIONS; MATTER; PARTICLE INTERACTIONS; STARS; VARIABLE STARS

Optional Information

Notes
8 refs., 3 figs.