activity
20092016
most citedTesting General Relativity with Present and Future Astrophysical Observations

1.5k citations · 1.6k across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2016

Radiation from a D-dimensional collision of shock waves: Two dimensional reduction and Carter-Penrose diagram

Flávio S. Coelho, Marco O. P. Sampaio

We analyse the causal structure of the two dimensional (2D) reduced background used in the perturbative treatment of a head-on collision of two -dimensional Aichelburg-Sexl grav…

hep-th2015★ 1 cited

Radiation from a -dimensional collision of gravitational shock waves

Flávio S. Coelho

Classically, if two highly boosted particles collide head-on, a black hole is expected to form whose mass may be inferred from the gravitational radiation emitted during the collis…

gr-qc2015★ 1.5k cited

Testing General Relativity with Present and Future Astrophysical Observations

Emanuele Berti, Enrico Barausse, Vitor Cardoso +50

One century after its formulation, Einstein's general relativity has made remarkable predictions and turned out to be compatible with all experimental tests. Most of these tests pr…

hep-th2014★ 5 cited

Radiation from a -dimensional collision of shock waves: proof of first order formula and angular factorisation at all orders

Flávio S. Coelho, Carlos Herdeiro, Marco O. P. Sampaio

In two previous papers we have computed the inelasticity in a head-on collision of two -dimensional Aichelburg-Sexl shock waves, using perturbation theory to calculate the g…

gr-qc2013★ 1 cited

PPN expansion and FRW scalar perturbations in n-DBI gravity

Flávio S. Coelho, Carlos Herdeiro, Shinji Hirano +1

n-DBI gravity explicitly breaks Lorentz invariance by the introduction of a unit time-like vector field, thereby giving rise to an extra (scalar) degree of freedom. We look for obs…

gr-qc2013★ 1 cited

n-DBI Gravity in a nutshell

Flavio S. Coelho, Carlos Herdeiro, Shinji Hirano +1

We present a new model of gravity which explicitly breaks Lorentz-invariance by the introduction of a unit time-like vector field, thereby giving rise to an extra (scalar) degree o…

gr-qc2013★ 2 cited

Radiation from a D-dimensional collision of shock waves: an insight allowed by the D parameter

F. S. Coelho, C. Herdeiro, C. Rebelo +1

We consider the radiation emitted in a collision of shock waves, in D-dimensional General Relativity (GR), and describe a remarkably simple pattern, hinting at a more fundamental s…

gr-qc2013★ 4 cited

n-DBI gravity, maximal slicing and the Kerr geometry

Flavio S. Coelho, Carlos Herdeiro, Mengjie Wang

Recently, in arXiv:1110.0832, we have established that solutions of Einstein's gravity admitting foliations with a certain geometric condition are also solutions of n-DBI gravity,…

hep-th2012★ 12 cited

Radiation from a D-dimensional collision of shock waves: higher order set up and perturbation theory validity

Flávio S. Coelho, Carlos Herdeiro, Carmen Rebelo +1

The collision of two D-dimensional, ultra-relativistic particles, described in General Relativity as Aichelberg-Sexl shock waves, is inelastic. In first order perturbation theory,…

hep-th2012★ 10 cited

On the scalar graviton in n-DBI gravity

Flavio S. Coelho, Carlos Herdeiro, Shinji Hirano +1

n-DBI gravity is a gravitational theory which yields near de Sitter inflation spontaneously at the cost of breaking Lorentz invariance by a preferred choice of foliation. We show t…

hep-th2012★ 28 cited

Radiation from a D-dimensional collision of shock waves: a remarkably simple fit formula

Flávio S. Coelho, Carlos Herdeiro, Marco O. P. Sampaio

Recently, in arXiv:1105.2298 [hep-th], we have estimated the energy radiated in the head-on collision of two equal D-dimensional Aichelburg-Sexl shock waves, for even D, by solving…

gr-qc2009★ 13 cited

Relativistic Euler's 3-body problem, optical geometry and the golden ratio

Flavio S. Coelho, Carlos A. R. Herdeiro

A Weyl solution describing two Schwarzschild black holes is considered. We focus on the Z_2 invariant solution, with ADM mass M_{ADM}=2M_K, where M_K is the Komar mass of each blac…