activity
20022022
most citedMarginally stable circular orbits in stationary axisymmetric spacetimes

13 citations · 24 across the 7 of their papers we have counts for

collaborators

9 papers

gr-qc2022★ 2 cited

Future stability of self-gravitating dust balls in an expanding universe

Shabnam Beheshti, Mikael Normann, Juan Valiente Kroon

We consider a system representing self-gravitating balls of dust in an expanding Universe. It is demonstrated that one can prescribe data for such a system at infinity and evolve i…

gr-qc2015★ 13 cited

Marginally stable circular orbits in stationary axisymmetric spacetimes

Shabnam Beheshti, Edgar Gasperin

We derive a necessary condition for the existence of marginally stable circular orbits of test particles in stationary axisymmetric spacetimes which possess a refection symmetry wi…

nlin.SI2013

Dressing with Control: using integrability to generate desired solutions to Einstein's equations

Shabnam Beheshti, A. Shadi Tahvildar-Zadeh

Motivated by integrability of the sine-Gordon equation, we investigate a technique for constructing desired solutions to Einstein's equations by combining a dressing technique with…

nlin.SI2013★ 1 cited

Remarks on Combinatorial Aspects of the KP Equation

Shabnam Beheshti, Amanda Redlich

We survey several results connecting combinatorics and Wronskian solutions of the KP equation, contextualizing the successes of a recent approach introduced by Kodama, et. al. We i…

math.AP2012

Integrability and Vesture for Harmonic Maps into Symmetric Spaces

Shabnam Beheshti, A. Shadi Tahvildar-Zadeh

After giving the most general formulation to date of the notion of integrability for axially symmetric harmonic maps from R^3 into symmetric spaces, we give a complete and rigorous…

math-ph2010

On Generalized Monopole Spherical Harmonics and the Wave Equation of a Charged Massive Kerr Black Hole

Shabnam Beheshti, Floyd L. Williams

We find linearly independent solutions of the Goncharov-Firsova equation in the case of a massive complex scalar field on a Kerr black hole. The solutions generalize, in some sense…