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20012021
most citedModified Gravity and Cosmology: An Update by the CANTATA Network

242 citations · 1k across the 37 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

gr-qc2019★ 2 cited

Eddington-inspired-Born-Infeld tensorial instabilities neutralized in a quantum approach

Imanol Albarran, Mariam Bouhmadi-López, Che-Yu Chen +1

The recent direct detection of gravitational waves has highlighted the huge importance of the tensorial modes in any extended gravitational theory. One of the most appealing approa…

gr-qc2019★ 33 cited

Annihilation-to-nothing: a quantum gravitational boundary condition for the Schwarzschild black hole

Mariam Bouhmadi-López, Suddhasattwa Brahma, Che-Yu Chen +2

The interior of a static Schwarzschild metric can be written in terms of two functions, similar to some models of anisotropic cosmology. With a suitable choice of canonical variabl…

gr-qc2019★ 13 cited

The classical and quantum fate of the Little Sibling of the Big Rip in cosmology

Teodor Borislavov Vasilev, Mariam Bouhmadi-López, Prado Martín-Moruno

The Little Sibling of the Big Rip is a cosmological abrupt event predicted by some phantom cosmological models that could describe our Universe. When this event is approached the o…

astro-ph.CO2019★ 50 cited

Cosmological constraints of phantom dark energy models

Amine Bouali, Imanol Albarran, Mariam Bouhmadi-López +1

We address three genuine phantom dark energy models where each of them induces the particular future events known as Big Rip, Little Rip and Little Sibling of the Big Rip. The back…

gr-qc2019★ 34 cited

Phantom singularities and their quantum fate: general relativity and beyond

Mariam Bouhmadi-López, Claus Kiefer, Prado Martín-Moruno

Cosmological observations allow the possibility that dark energy is caused by phantom fields. These fields typically lead to the occurrence of singularities in the late Universe. W…

gr-qc2019★ 48 cited

Asymptotic non-flatness of an effective black hole model based on loop quantum gravity

Mariam Bouhmadi-López, Suddhasattwa Brahma, Che-Yu Chen +2

For any non-rotating effective quantum (uncharged) black hole model to be viable, its asymptotic structure of spacetime should reduce to that of a Schwarzschild black hole. After e…