Published December 2022
| Version v1
Book
Study of r-mode spin down features of new born neutron star pulsars using KDE0v1 interaction
- 1. School of Physics, Sambalpur University, Jyotivihar-768 019 (India)
Description
The r-modes are the neutral circular currents on the surface of Neutron Stars (NSs) that couple to gravitational radiation where the Coriolis force provides the true dynamics. In this work we focus mainly on the spin down features of new born NS pulsars using KDE0v1 interaction by using the method proposed by Owen et al. Here we have limit ourselves to the case of npeμ matter. The r-mode spin-down feature provides a probable explanation for the low rotational frequency for the young NS pulsars
Additional details
Publishing Information
- Publisher
- Cotton University
- Imprint Place
- Guwahati (India)
- Imprint Title
- Proceedings of the DAE-BRNS symposium on nuclear physics. V. 66
- Imprint Pagination
- [1318 p.]
- Journal Page Range
- [2 p.]
Conference
- Title
- 66. DAE-BRNS symposium on nuclear physics
- Dates
- 1-5 Dec 2022
- Place
- Guwahati (India)
INIS
- Country of Publication
- India
- Country of Input or Organization
- India
- INIS RN
- 54037878
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CORIOLIS FORCE; GRAVITATIONAL COLLAPSE; NEUTRON STARS; NUCLEAR MATTER; NUCLEOSYNTHESIS; R PROCESS
- Descriptors DEC
- EVOLUTION; MATTER; STAR EVOLUTION; STARS; SYNTHESIS
Optional Information
- Notes
- Article No. C26