activity
20032022
most citedPossibility of Catastrophic Black Hole Growth in the Warped Brane-World Scenario at the LHC

20 citations · 82 across the 9 of their papers we have counts for

collaborators

9 papers

gr-qc2022★ 7 cited

Cosmic acceleration in Regge-Teitelboim gravity

S. Fabi, A. Stern, Chuang Xu

The Regge-Teitelboim formulation of gravity, which utilizes dynamical embeddings in a background space, effectively introduces source terms in the standard Einstein equations that…

math-ph2013★ 5 cited

On the gauge features of gravity on a Lie algebroid structure

S. Fabi, B. Harms, S. Hou

We present the geometric formulation of gravity based on the mathematical structure of a Lie Algebroid. We show that this framework provides the geometrical setting to describe the…

hep-th2011★ 1 cited

On the equation of motion for test particles in an ambient gravitational field as the Wong equation for a generalized gauge theory

S. Fabi, G. S. Karatheodoris

In this note we demonstrate the equation of motion for test particles in an ambient gravitational field for the teleparallel theory of gravity, considered as a generalized gauge th…

hep-th2009★ 17 cited

Theoretical survey of tidal-charged black holes at the LHC

Roberto Casadio, Sergio Fabi, Benjamin Harms +1

We analyse a family of brane-world black holes which solve the effective four-dimensional Einstein equations for a wide range of parameters related to the unknown bulk/brane physic…

hep-ph2009★ 20 cited

Possibility of Catastrophic Black Hole Growth in the Warped Brane-World Scenario at the LHC

Roberto Casadio, Sergio Fabi, Benjamin Harms

In this paper we present the results of our analysis of the growth and decay of black holes possibly produced at the Large Hadron Collider, based on our previous study of black hol…

hep-th2008★ 16 cited

Noncommutative Corrections to the Robertson-Walker metric

S. Fabi, B. Harms, A. Stern

Upon applying Chamseddine's noncommutative deformation of gravity we obtain the leading order noncommutative corrections to the Robertson-Walker metric tensor. We get an isotropic…