Published December 2017
| Version v1
Book
Correlation in the properties of static and rotating compact star within extended relativistic mean field model
- 1. Department of Physics, Rajkiya Kanya Mahavidyalaya, Shimla (India)
- 2. Department of Physics, Himachal Pradesh University, Shimla (India)
- 3. Department of Physics, Government College, Karsog (India)
Description
The efforts have been made to establish the empirical relationship between observable properties of static star with uniformly rotating star. Many correlations have been calculated which correlate the static properties with the keplerian properties of star. In present work we tried to correlate the static mass with the mass of star rotating with some frequency
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. 722-723
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
- 49014659
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- MEAN-FIELD THEORY; MESON-NUCLEON INTERACTIONS; NEUTRON STARS; OMEGA PARTICLES; SU-6 GROUPS
- Descriptors DEC
- BARYONS; ELEMENTARY PARTICLES; FERMIONS; HADRON-HADRON INTERACTIONS; HADRONS; HYPERONS; INTERACTIONS; LIE GROUPS; MESON-BARYON INTERACTIONS; OMEGA BARYONS; PARTICLE INTERACTIONS; STARS; STRANGE PARTICLES; SU GROUPS; SYMMETRY GROUPS
Optional Information
- Notes
- 3 refs., 2 figs.