output
20062026
most citedSolar system constraints on f(T) gravity

266 citations

Showing 2022Show all

7 papers · 1 filter

gr-qc2022★ 10 cited

Frame-Dragging in Extrasolar Circumbinary Planetary Systems

Lorenzo Iorio

Extrasolar circumbinary planets are so called because they orbit two stars instead of just one; to date, an increasing number of such planets have been discovered with a variety of…

physics.gen-ph2022

Non-cosmological, Non-Doppler Relativistic Frequency Shift over Astronomical Distances

Germano D'Abramo

We investigate in detail an apparently unnoticed consequence of special relativity. It consists in time dilation/contraction and frequency shift for emitted light affecting acceler…

physics.gen-ph2022★ 7 cited

Mass-energy connection without special relativity

Germano D'Abramo

In 1905, Einstein carried out his first derivation of the mass-energy equivalence by studying in different reference frames the energy balance of a body emitting electromagnetic ra…

gr-qc2022★ 5 cited

Effect of some modified models of gravity on the radial velocity of binary systems

Lorenzo Iorio, Matteo Luca Ruggiero

For many classes of astronomical and astrophysical binary systems, long observational records of their radial velocity , which is their directly observable quantity, are availab…

gr-qc2022★ 12 cited

Post-Newtonian effects on some characteristic timescales of transiting exoplanets

Lorenzo Iorio

Some measurable characteristic timescales of transiting exoplanets are investigated in order to check preliminarily if their cumulative shifts over…

astro-ph.EP2022

Impact of Lorentz violation models on exoplanets dynamics

Antonio Gallerati, Matteo Luca Ruggiero, Lorenzo Iorio

Many exoplanets were detected thanks to the radial velocity method, according to which the motion of a binary system around its center of mass can produce a periodical variation of…

gr-qc2022★ 4 cited

Why the mean anomaly at epoch is not used in tests of non-Newtonian gravity?

Lorenzo Iorio

The mean anomaly at epoch is one of the standard six Keplerian orbital elements in terms of which the motion of the two-body problem is parameterized. Along with the argument o…