Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction

• Autor: Pattnaik, Sanjay P ; Routray, T. R ; Viñas Gausí, Xavier ; Basu, D. N ; Centelles Aixalà, Mario ; Madhuri, K ; Behera, B
• Assuntos: Cosmologia ; Cosmology ; Neutrons
• Notas: Articles publicats en revistes (Física Quàntica i Astrofísica)
  679954
  http://hdl.handle.net/2445/156042
  Versió postprint del document publicat a: https://doi.org/10.1088/1361-6471/aab7c5
  https://doi.org/10.1088/1361-6471/aab7c5
  0954-3899
  Journal of Physics G: Nuclear and Particle Physics, 2018, vol. 45, num. 5, p. 055202
  
• Descrição: The characteristic physical properties of rotating neutron stars under the r-mode oscillation are evaluated using the finite-range simple effective interaction. Emphasis is given on examining the influence of the stiffness of both the symmetric and asymmetric parts of the nuclear equation of state on these properties. The amplitude of the r-mode at saturation is calculated using the data of particular neutron stars from the considerations of 'spin equilibrium' and 'thermal equilibrium'. The upper limit of the r-mode saturation amplitude is found to lie in the range 10−8-10−6, in agreement with the predictions of earlier work.
  
• Editor: Institute of Physics (IOP)
  
• Data de criação/publicação: 2018-04
  
• Idioma: Inglês