11 research outputs found
Thin accretion disk signatures in hybrid metric-Palatini f(R)-gravity
In the present work, accretion onto a spherically symmetric black hole in the
hybrid metric-Palatini f(R)-gravity is considered. The Novikov-Thorne model for
a relativistic thin accretion disk is used. The energy flux, temperature
distribution, emission spectrum and energy conversion efficiency of accretion
disks around such black holes are numerically calculated. A comparison with the
results for a Schwarzschild black hole is made and conclusions about the
viability of the model are drawn. As a result, it is obtained that the
accretion disks around black holes in hybrid metric-Palatini f(R)-gravity are
colder and less luminous than in general relativity.Comment: 27 pages, 26 figure
Test of hybrid metric-Palatini f(R)-gravity in binary pulsars
We developed the parameterized post-Keplerian formalism for hybrid
metric-Palatini -gravity. We obtained analytical expressions in the
generel eccentric case for four PPK parameters: , ,
and . Using observational data of PSR J0737-3039 and PSR J1903+0327 we
imposed restrictions on the parameters of hybrid f(R)-gravity and showed that
this theory is not ruled out by the observations in strong field regime. In
addition we obtained predictions for masses of systems components and found
that considered astrophysical objects will be heavier than in GR.Comment: 12 pages, 4 figure
Observational Limits on Gauss-Bonnet and Randall-Sundrum Gravities
We discuss the possibilities of experimental search for new physics predicted
by the Gauss-Bonnet and the Randall-Sundrum theories of gravity. The effective
four-dimensional spherically-symmetrical solutions of these theories are
analyzed. We consider these solutions in the weak-field limit and in the
process of the primordial black holes evaporation. We show that the predictions
of discussed models are the same as of General Relativity. So, current
experiments are not applicable for such search therefore different methods of
observation and higher accuracy are required.Comment: 7 pages, accepted to JET
Polarization and speed of gravitational waves in hybrid metric-Palatini f(R)-gravity
The question of the correspondence between the number of degrees of freedom
and the number of polarization states in hybrid metric-Palatini f(R)-gravity is
considered. It is shown that the scalar transverse breathing and longitudinal
modes are a mixture of one polarization state. The speed of gravitational waves
propagation in hybrid f(R)-gravity is calculated.Comment: 6 pages, submitted to JETP. arXiv admin note: text overlap with
arXiv:1907.0691
Tests of f(R)-gravity in binary pulsars
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 obtain restrictions on the parameters of this class of f(R)-models and show that f(R)-gravity is not ruled out by the observations in strong field regime