Oblate effective deformation (D<1) and positive f(R,T) trace coupling systematically raise compact-star maximum masses and radii relative to spherical GR for GM1, MIT Bag, and polytropic equations of state.
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Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
Cosmic Explorer is described as a next-generation gravitational-wave observatory aiming for tenfold sensitivity improvement over Advanced LIGO to observe signals from the edge of the observable universe at z~100.
citing papers explorer
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Deformed Compact Objects in General Relativity and Modified Gravity
Oblate effective deformation (D<1) and positive f(R,T) trace coupling systematically raise compact-star maximum masses and radii relative to spherical GR for GM1, MIT Bag, and polytropic equations of state.
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Nucleosynthesis in the fast ejecta of a neutron star merger
Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
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A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
Cosmic Explorer is described as a next-generation gravitational-wave observatory aiming for tenfold sensitivity improvement over Advanced LIGO to observe signals from the edge of the observable universe at z~100.