Modified gravity revealed along geodesic tracks
arXiv:1811.00046 · doi:10.1140/epjc/s10052-018-6401-0
Abstract
The study of the dynamics of a two-body system in modified gravity constitutes a more complex problem than in Newtonian gravity. Numerical methods are typically needed to solve the equations of geodesics. Despite the complexity of the problem, the study of a two-body system in gravity leads to a new exciting perspective hinting the right strategy to adopt in order to probe modified gravity. Our results point out some differences between the {\em semiclassical} (Newtonian) approach, and the {\em relativistic} (geodesic) one thus suggesting that the latter represents the best strategy for future tests of modified theories of gravity. { Finally, we have also highlighted the capability of forthcoming observations to serve as smoking gun of modified gravity revealing a departure from GR or further reducing the parameter space of gravity}. \keywords{ gravity \and binary system \and geodesics \and precession
arXiv comment7 Pages, 2 figures. Accepted for publication on The European Physics Journal C
References in corpus (51)
- Particle Dark Matter: Evidence, Candidates and Constraints
- f(R) Theories Of Gravity
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- The Confrontation between General Relativity and Experiment
- Extended Theories of Gravity
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- f(T) teleparallel gravity and cosmology
- Testing General Relativity with Present and Future Astrophysical Observations
- Dark Matter Candidates from Particle Physics and Methods of Detection
- Palatini Approach to Modified Gravity: f(R) Theories and Beyond
- Study of the anomalous acceleration of Pioneer 10 and 11
- Indication, from Pioneer 10/11, Galileo, and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range Acceleration
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- An Update on Monitoring Stellar Orbits in the Galactic Center
- The orbit of the star S2 around SgrA* from VLT and Keck data
- A new method for shadow calculations: application to parameterised axisymmetric black holes
- The Current Ability to Test Theories of Gravity with Black Hole Shadows
- Testing General Relativity with stellar orbits around the supermassive black hole in our Galactic center
- Prospects for Probing the Spacetime of Sgr A* with Pulsars
- Modelling clusters of galaxies by f(R)-gravity
- Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
- Detecting massive gravitons using pulsar timing arrays
- Constraining the range of Yukawa gravity interaction from S2 star orbits
- Recognising Axionic Dark Matter by Compton and de-Broglie Scale Modulation of Pulsar Timing
- Analysis of the Yukawa gravitational potential in gravity I: semiclassical periastron advance
- Analysis of the Yukawa gravitational potential in gravity II: relativistic periastron advance
- Constraints on gravity from precession of orbits of S2-like stars
- General relativistic effects on the orbit of the S2 star with GRAVITY
- Constraining gravity by the Large Scale Structure
- Constraining the range of Yukawa gravity interaction from S2 star orbits II: Bounds on graviton mass
- Testing f(R)-theories using the first time derivative of the orbital period of the binary pulsars
- Test-particle dynamics in general spherically symmetric black hole spacetimes
- The Newtonian limit of fourth and higher order gravity
- Probing hybrid modified gravity by stellar motion around Galactic Centre
- The 1919 measurement of the deflection of light
- Constraining the range of Yukawa gravity interaction from S2 star orbits III: improvement expectations for graviton mass bounds
- From Dark Energy and Dark Matter to Dark Metric
- Constraining Extended Gravity Models by S2 star orbits around the Galactic Centre
- Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
- Accelerating universe in scalar tensor models - confrontation of theoretical predictions with observations
- Testing an exact -gravity model at Galactic and local scales
- Testing gravitational theories using Eccentric Eclipsing Detached Binaries
- Conformal Transformations and Weak Field Limit of Scalar-Tensor Gravity
- The Post-Newtonian Limit of f(R)-gravity in the Harmonic Gauge
- A -gravity model of the Sunyaev-Zeldovich profile of the Coma cluster compatible with {\it Planck} data
- Probing the physical and mathematical structure of gravity by PSR
- Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions
- Constraining scalar-tensor quintessence by cosmic clocks
- Decaying dark energy in light of the latest cosmological dataset
- Gravitational Radiation from Compact Binary Pulsars
Cited by in corpus (11)
- Dark matters on the scale of galaxies
- -gravity after the detection of the orbital precession of the S2 star around the Galactic centre massive black hole
- Constraining Non-local Gravity by S2 star orbits
- The Galactic Center as a laboratory for theories of gravity and dark matter
- Testing Born-Infeld teleparallel gravity through Sgr A observations
- Tracing the cosmic history by Gauss-Bonnet gravity
- Estimating the parameters of Hybrid Palatini gravity model with the Schwarzschild precession of S2, S38 and S55 stars: case of bulk mass distribution
- Linearized physics and gravitational-waves polarizations in the Palatini formalism of GBD theory
- Linearized modified gravity theories and gravitational waves physics in the GBD theory
- Einstein-non-linear Maxwell-Yukawa black hole
- Tracking the Local Group Dynamics by Extended Gravity