Published December 2018
| Version v1
Book
Mass and radius of rotating protoneutron star with in extended relativistic mean field model and their correlation with frequency
- 1. Department of Physics, Government College, Karsog (India)
- 2. Department of Physics, Rajkiya Kanya Mahavidyalya, Shimla (India)
- 3. Department of Physics, Himachal Pradesh University, Shimla (India)
Description
This parameterization is selected for this study as this parameterization produces a canonical mass (1.4M⊙) at rest when composition is assumed to possess hyperon. We plotted mass as a function of frequency for BSR15 parameterization at different temperatures
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. 804-805
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
- 50011904
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- MEAN-FIELD THEORY; NEUTRON STARS; OMEGA PARTICLES; PULSARS; SU-6 GROUPS
- Descriptors DEC
- BARYONS; COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYPERONS; LIE GROUPS; OMEGA BARYONS; STARS; STRANGE PARTICLES; SU GROUPS; SYMMETRY GROUPS
Optional Information
- Notes
- 4 refs., 2 figs., 2 tabs.