Implications from GW170817 and I-Love-Q relations for relativistic hybrid stars

By V. Paschalidis, Kent Yagi, David E. Alvarez-Castillo, David B. Blaschke, Armen Sedrakian. 2017

180 citations recorded by the source corpus.

ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenphysik Darmstadt, Germany; Russian Science Foundation [7-12-01427]; COST Action [MP1304, GWverse CA16104]; Deutsche Forschungsgemeinschaft [SE 1836/3-2]

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/c9239089e0edd48c45e89212872ef73b34a4328e

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In Astronomy and Astrophysics

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3. G. Olmo
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In Geophysics

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Citations in the corpus

• Stellar structure models in modified theories of gravity: Lessons and challenges (2019, background): “ift of the spectral lines emitted from the star’s surface [47] (though it is subject to heavy observational limitations [10]), or via quantities that depend on the star’s tidal deformability,see e.g. [48, 49]. For some reviews of neutron stars structure and their associated astrophysical and observa”
• Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts, and Nucleosynthesis (2018, unknown): “…et al. 2018; De et al. 2018; Drago et al. 2018; Fattoyev et al. 2018; Hinderer et al. 2018; Malik et al. 2018; Most et al. 2018b; Nandi et al. 2018; Paschalidis et al. 2018; Radice et al. 2018c; Rezzolla et al. 2018; Ruiz et al. 2018; Tews et al. 2018; Tsang et al. 2018; Wei et al. 2018), and the…”