6533b82dfe1ef96bd1290963
RESEARCH PRODUCT
Completion of the universal I-Love-Q relations in compact stars including the mass
Raül VeraJosé A. FontBorja ReinaBorja ReinaNicolas Sanchis-gualsubject
High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveFOS: Physical sciencesPerturbation (astronomy)Binary numberAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesUniversal relationGeneral Relativity and Quantum CosmologyStarsTheoretical physicsQuark starSpace and Planetary Science0103 physical sciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsdescription
In a recent paper we applied a rigorous perturbed matching framework to show the amendment of the mass of rotating stars in Hartle's model. Here, we apply this framework to the tidal problem in binary systems. Our approach fully accounts for the correction to the Love numbers needed to obtain the universal $I$-Love-$Q$ relations. We compute the corrected mass vs radius configurations of rotating quark stars, revisiting a classical paper on the subject. These corrections allow us to find a universal relation involving the second-order contribution to the mass $\delta M$. We thus complete the set of universal relations for the tidal problem in binary systems, involving four perturbation parameters, namely $I$, Love, $Q$, and $\delta M$. These relations can be used to obtain the perturbation parameters directly from observational data.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2017-02-15 |