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

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. 722-723

Conference

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

Optional Information

Notes
3 refs., 2 figs.