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20152026
most citedElectromagnetic Emission from Supermassive Binary Black Holes Approaching Merger

106 citations · 642 across the 22 of their papers we have counts for

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gr-qc2023

Ameliorating the Courant-Friedrichs-Lewy condition in spherical coordinates: A double FFT filter method for general relativistic MHD in dynamical spacetimes

Liwei Ji, Vassilios Mewes, Yosef Zlochower +5

Numerical simulations of merging compact objects and their remnants form the theoretical foundation for gravitational wave and multi-messenger astronomy. While Cartesian-coordinate…

gr-qc2020★ 16 cited

Spontaneous creation of circularly polarized photons in chiral astrophysical systems

Adrian del Rio, Nicolas Sanchis-Gual, Vassilios Mewes +3

This work establishes a relation between chiral anomalies in curved spacetimes and the radiative content of the gravitational field. In particular, we show that a flux of circularl…

gr-qc2020★ 38 cited

Numerical relativity in spherical coordinates: A new dynamical spacetime and general relativistic MHD evolution framework for the Einstein Toolkit

Vassilios Mewes, Yosef Zlochower, Manuela Campanelli +4

We present SphericalNR, a new framework for the publicly available Einstein Toolkit that numerically solves the Einstein field equations coupled to the equations of general relativ…

gr-qc2018★ 31 cited

Numerical relativity in spherical coordinates with the Einstein Toolkit

Vassilios Mewes, Yosef Zlochower, Manuela Campanelli +3

Numerical relativity codes that do not make assumptions on spatial symmetries most commonly adopt Cartesian coordinates. While these coordinates have many attractive features, sphe…

gr-qc2015★ 28 cited

Quasistationary solutions of self-gravitating scalar fields around collapsing stars

Nicolas Sanchis-Gual, Juan Carlos Degollado, Pedro J. Montero +2

Recent work has shown that scalar fields around black holes can form long-lived, quasistationary configurations surviving for cosmological timescales. With this requirement, scalar…

gr-qc2015★ 27 cited

Numerical relativity simulations of thick accretion disks around tilted Kerr black holes

Vassilios Mewes, José A. Font, Filippo Galeazzi +2

In this work we present 3D numerical relativity simulations of thick accretion disks around tilted Kerr BH. We investigate the evolution of three different initial disk models with…

gr-qc2015★ 6 cited

Measuring the black hole spin direction in 3D Cartesian numerical relativity simulations

Vassilios Mewes, José A. Font, Pedro J. Montero

We show that the so-called flat-space rotational Killing vector method for measuring the Cartesian components of a black hole spin can be derived from the surface integral of Weinb…