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Insights on Skyrme parameters from GW170817
Published 2019-09-01“…The binary neutron-star merger event, GW170817, has cast a new light on nuclear physics research. …”
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On the Progenitor of Binary Neutron Star Merger GW170817
Published 2018“…On 2017 August 17 the merger of two compact objects with masses consistent with two neutron stars was discovered through gravitational-wave (GW170817), gamma-ray (GRB 170817A), and optical (SSS17a/AT 2017gfo) observations. …”
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Properties of the Binary Neutron Star Merger GW170817
Published 2019“…The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. …”
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Properties of the Binary Neutron Star Merger GW170817
Published 2021“…The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. …”
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Symmetry energy constraints from GW170817 and laboratory experiments
Published 2019-08-01“…The LIGO-Virgo collaboration detection of the binary neutron-star merger event, GW170817, has expanded efforts to understand the Equation of State (EoS) of nuclear matter. …”
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Non-minimal derivative coupling theories compatible with GW170817
Published 2024-03-01“…Due to the fact that the Universe is classical during and in the post-inflationary epoch, there is no fundamental reason for the graviton to change its mass, the GW170817 event severely constrained these theories. …”
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Shortcut in codimension-2 brane cosmology in light of GW170817
Published 2023-03-01“…We also study the time delay between a GW signal and an electromagnetic (EM) wave signal in the low-redshift limit by combining with the joint observations of GW170817 and GRB 170817A, which gives an upper limit to the $$\text {AdS}_{6}$$ AdS 6 radius as $$\ell ^{2}_{~} \lesssim 3.84\,\text {Mpc}^{2}_{~}$$ ℓ 2 ≲ 3.84 Mpc 2 . …”
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Rectifying Einstein-Gauss-Bonnet inflation in view of GW170817
Published 2020-09-01“…The main requirement is that the Einstein-Gauss-Bonnet theory has to be compatible with the GW170817 event, so the gravitational wave speed cT2 is required to be cT2≃1 in natural units. …”
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Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
Published 2018“…The source of the gravitational-wave (GW) signal GW170817, very likely a binary neutron star merger, was also observed electromagnetically, providing the first multi-messenger observations of this type. …”
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GW170817: Measurements of Neutron Star Radii and Equation of State
Published 2018“…The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. …”
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GW170817A as a hierarchical black hole merger
Published 2020“…Here we show that the recently reported gravitational-wave candidate, GW170817A, could be the result of such a hierarchical merger. …”
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Constraining Palatini–Horndeski theory with gravitational waves after GW170817
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GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
Published 2020-04-01“…Most of the obtained results are located within the constraints of the tidal deformabilities extracted from the GW170817 detection. Keywords: Equation of state, Finite-range interactions, Neutron star, Tidal deformability, Moment of inertia…”
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GW170817 and GW190425 as hybrid stars of dark and nuclear matter
Published 2022-04-01“…These hybrid stars could provide alternative interpretations to the LIGO/Virgo events GW170817 and GW190425. To demonstrate our proposal, we solve the Tolman–Oppenheimer–Volkoff configurations of hybrid stars by using the SLy4, APR4, and SKb equations of state (EoS) for nuclear matter, and an EoS for a bosonic self interacting dark matter (SIDM) proposed by Colpi et al. …”
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Neutron Star Binary Mergers: The Legacy of GW170817 and Future Prospects
Published 2022-09-01Subjects: Get full text
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Short Duration Gamma-Ray Bursts and Their Outflows in Light of GW170817
Published 2020-11-01“…All together, the incomparable richness of the data from GW170817 has allowed us to paint a fairly detailed picture of at least one SGRB. …”
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Swampland implications of GW170817-compatible Einstein-Gauss-Bonnet gravity
Published 2020-06-01“…We revisit the Einstein-Gauss-Bonnet theory in view of the GW170817 event, which compels that the gravitational wave speed is equal to cT2=1 in natural units. …”
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Constraining the p-Mode–g-Mode Tidal Instability with GW170817
Published 2020“…We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the binary to internal modes of the stars, accelerating the gravitational-wave driven inspiral. …”
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