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2023

Tidal properties of neutron stars in scalar-tensor theories of gravity

Creci, Gastón, Hinderer, Tanja, Steinhoff, Jan

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A major science goal of gravitational-wave (GW) observations is to probe the nature of gravity and constrain modifications to General Relativity.

An established class of modified gravity theories are scalar-tensor models, which introduce an extra scalar degree of freedom.
This affects the internal structure of neutron stars (NSs), as well as their dynamics and GWs in binary systems, where distinct novel features can arise from the appearance of scalar condensates in parts of the parameter space.
To improve the robustness of the analyses of such GW events requires advances in modeling internal-structure-dependent phenomena in scalar-tensor theories.

Tidal properties of neutron stars in scalar-tensor theories of gravity · Around

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