Subtleties in constraining gravity theories with mass-radius data
arXiv:2303.01910 · doi:10.1103/PhysRevD.108.024028
Abstract
Simultaneous measurements of neutron star masses and radii can be used to constrain deviations from general relativity (GR) as was recently demonstrated for the spontaneous scalarization model of Damour and Esposito-Farèse (DEF). Here, we investigate the general applicability of the same procedure beyond this single example. We first show that a simple variation of the DEF model renders the same mass-radius measurements ineffective for obtaining constraints. On the other hand, a recently popular and distinct model of scalarization that arises in scalar-Gauss-Bonnet theory can be constrained similarly to the original DEF model, albeit due to a slightly different underlying mechanism. These establish that using the mass-radius data can potentially constrain various theories of gravity, but the method also has limitations.
arXiv comment18 pages, 11 figures. Published version. A larger dataset was used in the analysis and a chapter explaining the effect of the dataset size is added in this version
References in corpus (43)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- The Confrontation between General Relativity and Experiment
- Testing General Relativity with Present and Future Astrophysical Observations
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Massive Gravity
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Black holes, gravitational waves and fundamental physics: a roadmap
- Tests of General Relativity with GW170817
- Spontaneous scalarization of black holes and compact stars from a Gauss-Bonnet coupling
- Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability
- New Gauss-Bonnet black holes with curvature induced scalarization in the extended scalar-tensor theories
- PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star
- Neutron-star radius constraints from GW170817 and future detections
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- The Dense Matter Equation of State from Neutron Star Radius and Mass Measurements
- Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory
- Measuring the neutron star equation of state with gravitational wave observations
- Approximate Universal Relations for Neutron Stars and Quark Stars
- Spontaneous Scalarization with Massive Fields
- Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-ray Data Set
- Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star
- Neutron stars in scalar-tensor theories of gravity and catastrophe theory
- Dynamics of spontaneous black hole scalarization and mergers in Einstein-scalar-Gauss-Bonnet gravity
- Slowly rotating neutron stars in scalar-tensor theories with a massive scalar field
- Neutron Star Mass-Radius Constraints of the Quiescent Low-mass X-ray Binaries X7 and X5 in the Globular Cluster 47 Tuc
- Spontaneous growth of vector fields in gravity
- Highly compact neutron stars in scalar-tensor theories of gravity: Spontaneous scalarization versus gravitational collapse
- Neutron star solutions with curvature induced scalarization in the extended Gauss-Bonnet scalar-tensor theories
- Nonlinear studies of binary black hole mergers in Einstein-scalar-Gauss-Bonnet gravity
- Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
- Closing a spontaneous-scalarization window with binary pulsars
- New class of quasinormal modes of neutron stars in scalar-tensor gravity
- On the possibility of setting a new constraint to scalar-tensor theories
- Constraining scalar-tensor theories of gravity from the most massive neutron stars
- Spontaneous scalarization: asymmetron as dark matter
- What does a measurement of mass and/or radius of a neutron star constrain: Equation of state or gravity?
- Spontaneous nonlinear scalarization of Kerr black holes
- Instability of vectorized stars
- Structure of neutron stars in massive scalar-tensor gravity
- Regularization of instabilities in gravity theories