17 citations · 70 across the 17 of their papers we have counts for
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Pulsar timing array results sheds light on Hubble tension during the end of inflation
M. Bousder, E. Salmani, A. Riadsolh +3
Recently, pulsar timing array (PTA) collaborations, including NANOGrav, have reported evidence of a stochastic gravitational wave background within the nHz frequency range.\ It can…
Cosmic acceleration in Lovelock quantum gravity
M. Bousder, A. Riadsolh, M El Belkacemi +1
This paper introduces novel solutions for inflation and late-time cosmic acceleration within the framework of quantum Lovelock gravity, utilizing Friedmann equations. Furthermore,…
A proof of holographic complexity conjecture: wormhole between horizon and singularity
M. Bousder
This letter provides evidence of complexity-volume and complexity-action conjectures by examining the structure of a black hole, which comprises a horizon linked to the singularity…
Implications of the NANOGrav results for primordial black holes and Hubble tension
M. Bousder, A. Riadsolh, A. El Fatimy +2
The purpose of this work is to investigate the formation and evaporation of the primordial black holes in the inflationary scenarios. Thermodynamic parameters such as mass, tempera…
Entropy as logarithmic term of the central charge and modified Friedmann equation in AdS/CFT correspondence
M. Bousder, E. Salmani, H. Ez-Zahraouy
This paper is about the extended thermodynamics of AdS black holes and its relation to CFT thermodynamics. The logarithmic term of the central charge is interpreted as black hole e…
Topological densities in Einstein-scalar-Gauss-Bonnet gravity
M. Bousder, Z Sakhi
The present work is devoted to studying the background dynamical evolution of a scalar field in Einstein-Gauss-Bonnet gravity in maximally symmetric space-time. This study is usefu…
Holographic dark energy satisfying the energy conditions in Lovelock gravity
M. Bousder, E. Salmani, A. El Fatimy +1
In this paper, we show that the holographic dark energy density hides in the solutions of Lovelock gravity for black holes. Using the obtained mass and temperature we find density…