Pith. sign in

REVIEW

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

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1712.07273 v1 pith:S2SOQ65E submitted 2017-12-20 nucl-th astro-ph.HE

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

S. P. Pattnaik , T. R. Routray , X. Vi\~nas , D. N. Basu , M. Centelles , K. Madhuri , B. Behera This is my paper
classification nucl-th astro-ph.HE
keywords r-modeamplitudeeffectiveequationequilibriumfinite-rangeinfluenceinteraction
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

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.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.