Search Results - "de Laurentis, Mariafelicia"
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How to tell an accreting boson star from a black hole
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…The capability of the Event Horizon Telescope (EHT) to image the nearest supermassive black hole candidates at horizon-scale resolutions offers a novel means…”
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Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
Published in The European physical journal. C, Particles and fields (01-02-2021)“…Static and spherically symmetric wormhole solutions can be reconstructed in the framework of curvature based Extended Theories of Gravity. In particular,…”
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Orbital precession of the S2 star in Scalar–Tensor–Vector Gravity
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT We have obtained the first constraint of the parameter space of Scalar–Tensor–Vector Gravity using the motion of the S2-star around the supermassive…”
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Jeans analysis in energy–momentum-squared gravity
Published in The European physical journal. C, Particles and fields (01-02-2020)“…In this paper, we study the Jeans analysis in the context of energy–momentum-squared gravity (EMSG). More specifically we find the new Jeans mass for…”
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Cosmographic Constraints and Cosmic Fluids
Published in Galaxies (01-12-2013)“…The problem of reproducing dark energy effects is reviewed here with particular interest devoted to cosmography. We summarize some of the most relevant…”
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Noether's stars in f(R) gravity
Published in Physics letters. B (10-05-2018)“…The Noether Symmetry Approach can be used to construct spherically symmetric solutions in f(R) gravity. Specifically, the Noether conserved quantity is related…”
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The Accurate Mass Distribution of M87, the Giant Galaxy with Imaged Shadow of Its Supermassive Black Hole, as a Portal to New Physics
Published in The Astrophysical journal (01-04-2022)“…The very careful Event Horizon Telescope estimate of the mass of the supermassive black hole at the center of the giant cD galaxy M87, allied with recent…”
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Response to: Comment on ‘Orbital precession of the S2 star in scalar–tensor–vector gravity’
Published in Monthly notices of the Royal Astronomical Society (02-03-2023)“…ABSTRACT The explicit derivation for the orbital precession of the S2 star in the Galactic Centre in the scalar–tensor–vector gravity is discussed and compared…”
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On the universality of MOG weak field approximation at galaxy cluster scale
Published in Physics letters. B (10-07-2017)“…In its weak field limit, Scalar-tensor-vector gravity theory introduces a Yukawa-correction to the gravitational potential. Such a correction depends on the…”
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The current ability to test theories of gravity with black hole shadows
Published in Nature astronomy (01-07-2018)“…Our Galactic Centre, Sagittarius A*, is believed to harbour a supermassive black hole, as suggested by observations tracking individual orbiting stars 1 , 2 …”
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Modified gravity revealed along geodesic tracks
Published in The European physical journal. C, Particles and fields (01-11-2018)“…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…”
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Testing space–time geometries and theories of gravity at the Galactic centre with pulsar’s time delay
Published in Monthly notices of the Royal Astronomical Society (24-07-2023)“…ABSTRACT We developed a numerical methodology to compute the fully relativistic propagation time of photons emitted by a pulsar in orbit around a massive…”
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Verification of f(R)-gravity in binary pulsars
Published in EPJ Web of conferences (01-01-2016)“…We develop the parameterized post-Keplerian approach for class of analytic f (R)-gravity models. Using the double binary pulsar system PSR J0737-3039 data we…”
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Testing f (R) theories using the first time derivative of the orbital period of the binary pulsars
Published in Monthly notices of the Royal Astronomical Society (01-05-2013)“…In this paper, we use one of the post-Keplerian parameters to obtain constraints on f (R) theories of gravity. Using the Minkowskian limit, we compute the…”
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Quadrupolar gravitational radiation as a test-bed for f( R)-gravity
Published in Astroparticle physics (01-12-2011)“…► We consider quadrupolar gravitational emission for extended theories of gravity. ► In particular, we take into account f( R)-theories where R is the Ricci…”
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On the Parameters of the Spherically Symmetric Parameterized Rezzolla–Zhidenko Spacetime through Solar System Tests, the Orbit of the S2 Star about Sgr A, and Quasiperiodic Oscillations
Published in The Astrophysical journal (01-12-2023)“…In this paper, we find the higher-order expansion parameters α and λ of spherically symmetric parameterized Rezzolla–Zhidenko (PRZ) spacetime by using its…”
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Constraining ƒ(R) Gravity by the Large-Scale Structure
Published in Universe (Basel) (01-09-2015)“…Over the past few decades, general relativity and the concordance ΛCDM model have been successfully tested using several different astrophysical and…”
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Constraining MOdified Gravity with the S2 Star
Published in Universe (Basel) (01-02-2022)“…We have used publicly available kinematic data for the S2 star to constrain the parameter space of MOdified Gravity. Integrating geodesics and using a Markov…”
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Deriving the mass of particles from Extended Theories of Gravity in LHC era
Published in The European physical journal. C, Particles and fields (01-06-2011)“…We derive a geometrical approach to produce the mass of particles that could be suitably tested at LHC. Starting from a 5D unification scheme, we show that all…”
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Massive, massless and ghost modes of gravitational waves from higher-order gravity
Published in Astroparticle physics (01-11-2010)“…We linearize the field equations for higher order theories that contain scalar invariants other than the Ricci scalar. We find that besides a massless spin-2…”
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