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Divergences in gravitational-wave emission and absorption from extreme mass ratio binaries
No evidence of kinetic screening in merging binary neutron stars
Divergences in gravitational-wave emission and absorption from extreme mass ratio binaries
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Updated Binary Pulsar Constraints on Einstein-æther Theory in Light of Gravitational Wave Constraint
Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical
Updated Binary Pulsar Constraints on Einstein-æther Theory in Light of Gravitational Wave Constraint
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Latest Publications
Black holes Across Cosmic History (BACH)
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BACH is a semi-analytic model for the formation and co-evolution of galaxies and black holes, originally presented in Barausse 2012 and later updated in various publications till its most recent version (Barausse et al 2023).
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While the underlying code is not yet public, the catalogs presented in Barausse et al 2023 are available here.
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Please reference Barausse 2012 and Barausse et al 2023 if you use these catalogs.
A full list of publications can be found here:
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