activity
20052026
most citedThe geodesic motion of S2 and G2 as a test of the fermionic dark matter nature of our galactic core

57 citations · 405 across the 35 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.HE20161 cited

Theoretical and observational constraints on the mass-radius relations of neutron stars

Kuantay Boshkayev, Jorge A. Rueda, Marco Muccino

We investigate theoretical and observational constraints on the mass-radius relations for neutron stars. For that purpose we consider the model of neutron stars taking into conside…

gr-qc2016

What can we really infer from GW 150914? (II)

J. F. Rodriguez, J. A. Rueda, R. Ruffini

In a recent letter we have outlined some issues on GW 150914, we hereby give additional details. We analyze the event GW 150914 announced by the Advanced Laser Interferometer Gravi…

gr-qc2016

What can we really infer from GW 150914?

J. F. Rodriguez, J. A. Rueda, R. Ruffini

We analyze the event GW 150914 announced by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) as the gravitational-wave emission of a black-hole binary merger…

astro-ph.HE2016

Main parameters of neutron stars from quasi-periodic oscillations in low mass X-ray binaries

Kuantay Boshkayev, Jorge A. Rueda, Marco Muccino

We investigate the kilohertz quasi-periodic oscillations of low-mass X-ray binaries within the Hartle-Thorne spacetime. On the basis the relativistic precession model we extract th…

astro-ph.SR2016

Induced Compression of White Dwarfs by Angular Momentum Loss

Kuantay Boshkayev, Jorge A. Rueda, Remo Ruffini +1

We investigate isolated sub- and super-Chandrasekhar white dwarfs which lose angular momentum through magnetic dipole braking. We construct constant rest mass sequences by fulfilli…

astro-ph.SR2016

Mass-radius relations of white dwarfs at finite temperatures

Kuantay Boshkayev, Jorge A. Rueda, Remo Ruffini +3

We construct mass-radius relations of white dwarfs taking into account the effects of rotation and finite temperatures. We compare and contrast the theoretical mass-radius relation…