activity
20152020
most citedGauge fixing and regularity of axially symmetric and axistationary second order perturbations around spherical backgrounds

6 citations · 10 across the 2 of their papers we have counts for

collaborators

6 papers

gr-qc2020★ 4 cited

Existence and uniqueness of compact rotating configurations in GR in second order perturbation theory

Marc Mars, Borja Reina, Raül Vera

Existence and uniqueness of rotating fluid bodies in equilibrium is still poorly understood in General Relativity (GR). Apart from the limiting case of infinitely thin disks, the o…

gr-qc2020★ 6 cited

Gauge fixing and regularity of axially symmetric and axistationary second order perturbations around spherical backgrounds

Marc Mars, Borja Reina, Raül Vera

Perturbation theory in geometric theories of gravitation is a gauge theory of symmetric tensors defined on a Lorentzian manifold (the background spacetime). The gauge freedom makes…

gr-qc2018

First order perturbations of hypersurfaces of arbitrary causal character

Brien C. Nolan, Borja Reina, Kepa Sousa

In this work we study the problem of first order perturbations of a general hypersurface, i.e. with arbitrary causal character at each point. We extend the framework by Mars (Class…

gr-qc2017

Completion of the universal I-Love-Q relations in compact stars including the mass

Borja Reina, Nicolas Sanchis-Gual, Raül Vera +1

In a recent paper we applied a rigorous perturbed matching framework to show the amendment of the mass of rotating stars in Hartle's model. Here, we apply this framework to the tid…

gr-qc2015

Junction conditions in quadratic gravity: thin shells and double layers

Borja Reina, José M. M. Senovilla, Raül Vera

The junction conditions for the most general gravitational theory with a Lagrangian containing terms quadratic in the curvature are derived. We include the cases with a possible co…

gr-qc2015

On the mass of rotating stars in Newtonian gravity and GR

Borja Reina, Raül Vera

We show how the correction to the calculation of the mass in the original relativistic model of a rotating star by Hartle [6], found recently [10], appears in the Newtonian limit,…