Boson star under Cornell potential
Creators
- 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
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.