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20152026
most citedUncharged and charged anisotropic like--Durgapal stellar model with vanishing complexity

65 citations · 174 across the 8 of their papers we have counts for

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6 papers · 1 filter

gr-qc2026

Zero expansion is not free: the sharp minimum of Eulerian negative energy in Natário warp drives

Nelson Bolívar, Ivaylo Vasilev, Gabriel Abellán

Natário's warp drive replaces the contraction and expansion of the Alcubierre bubble by a divergence-free shift. We determine exactly how much Eulerian negative energy this constru…

gr-qc2026

Boundary Obstructions and Lapse Freedom in Static Spherical Hollow Cores

Nelson Bolívar, Gabriel Abellán, Ivaylo Vasilev

We analyze a sharply delimited comparison problem for a static spherical hollow core: an empty, flat cavity surrounded by a positive matter wall. In the unit-lapse, flat-slice radi…

gr-qc2023★ 11 cited

A Generalized Double Chaplygin Model for Anisotropic Matter: The Newtonian Case

Gabriel Abellán, Angel Rincon, Eduard Sanchez

In this work, we investigate astrophysical systems in a Newtonian regime using anisotropic matter. For this purpose, we considered that both radial and tangential pressures satisfy…

gr-qc2022★ 65 cited

Uncharged and charged anisotropic like--Durgapal stellar model with vanishing complexity

E. Contreras, E. Fuenmayor, G. Abellán

In this work we use the vanishing complexity factor as a supplementary condition to construct uncharged and charged like--Durgapal models. We provide the component of the…

gr-qc2020★ 42 cited

The general relativistic double polytrope for anisotropic matter

G. Abellan, E. Fuenmayor, E. Contreras +1

A general formalism recently proposed to study Newtonian polytropes for anisotropic fluids is here extended to the relativistic regime. Thus, it is assumed that a polytropic equati…

gr-qc2020★ 38 cited

The double polytrope for anisotropic matter: Newtonian Case

G. Abellan, E. Fuenmayor, L. Herrera

A general formalism developed few years ago to model polytropic Newtonian stars with anisotropic pressure is applied to model stars for which, both, radial and tangential pressure…