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20052025
most citedQuark stars with isotropic matter in Hořava gravity and Einstein-æther theory

13 citations · 14 across the 4 of their papers we have counts for

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gr-qc2025★ 1 cited

Stellar modeling within regularized 4D Einstein-Gauss-Bonnet gravity in light of current astrophysical constraints

G. Panotopoulos, Á. Rincón, I. Lopes

In this study we obtain interior solutions and investigate structural properties of isotropic compact stars in the framework of four-dimensional regularized Einstein-Gauss-Bonnet (…

gr-qc2025

Cosmological implications of Bumblebee theory on an FLRW background

Manuel Gonzalez-Espinoza, Grigorios Panotopoulos, Francisco Tello-Ortiz

We investigate some cosmological implications at background level of the Bumblebee model. The phase-space, the critical points and their stability are analyzed in detail applying w…

gr-qc2025

Compact Stars in Symmetric Teleparallel Scalar-Tensor Gravity

Grigorios Panotopoulos, Andrés Lueiza-Colipí, Nikolaos Dimakis +1

We investigate the existence of static, spherically symmetric compact objects within the framework of symmetric teleparallel scalar-tensor gravity. This theory extends the Brans-Di…

gr-qc2020

Radial oscillations and tidal Love numbers of dark energy stars

Grigoris Panotopoulos, Angel Rincon, Ilidio Lopes

We investigate the properties of relativistic stars made of dark energy. We model stellar structure assuming i) isotropic perfect fluid and ii) a dark energy inspired equation of s…

gr-qc2020★ 13 cited

Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory

Grigoris Panotopoulos, Daniele Vernieri, Ilídio Lopes

We study non-rotating and isotropic strange quark stars in Lorentz-violating theories of gravity, and in particular in Hořava gravity and Einstein-æther theory. For quark matter we…

gr-qc2017

Observational constraints on warm quasi-exponential inflation

Nelson Videla, Grigoris Panotopoulos

In the present work we study a warm inflationary model defined by a quasi-exponential inflaton potential and an inflaton decay rate proportional to the Hubble rate. The model is ch…