activity
20092013
most citedRelationship Between Gravity and Gauge Scattering in the High Energy Limit

114 citations · 462 across the 9 of their papers we have counts for

collaborators

9 papers

hep-th2013★ 82 cited

Construction of an asymptotic S matrix for perturbative quantum gravity

John Ware, Ryo Saotome, Ratindranath Akhoury

The infrared behavior of perturbative quantum gravity is studied using the method developed for QED by Faddeev and Kulish. The operator describing the asymptotic dynamics is derive…

hep-th2013★ 92 cited

High Energy Scattering in Perturbative Quantum Gravity at Next to Leading Power

Ratindranath Akhoury, Ryo Saotome, George Sterman

We consider the relativistic scattering of unequal-mass scalar particles through graviton exchange in the small-angle high-energy regime. We show the self-consistency of expansion…

hep-th2012★ 114 cited

Relationship Between Gravity and Gauge Scattering in the High Energy Limit

Ryo Saotome, Ratindranath Akhoury

Investigations of high-energy graviton-graviton and gluon-gluon scattering are performed in the leading eikonal approximation for the kinematic regime of large center of mass energ…

hep-th2011★ 9 cited

No Classicalization Beyond Spherical Symmetry

Ratindranath Akhoury, Shinji Mukohyama, Ryo Saotome

We point out that a field theory that exhibits the classicalization phenomenon for perfect spherical symmetry ceases to do so when the spherical symmetry is significantly relaxed.…

hep-th2011★ 108 cited

Collinear and Soft Divergences in Perturbative Quantum Gravity

Ratindranath Akhoury, Ryo Saotome, George Sterman

Collinear and soft divergences in perturbative quantum gravity are investigated to arbitrary orders in amplitudes for wide-angle scattering, using methods developed for gauge theor…

hep-th2011★ 9 cited

Non-Stationary Dark Energy Around a Black Hole

Ratindranath Akhoury, David Garfinkle, Ryo Saotome +1

Numerical simulations of the accretion of test scalar fields with non-standard kinetic terms (of the k-essence type) onto a Schwarzschild black hole are performed. We find a full d…