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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)
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).
While the underlying code is not yet public, the catalogs presented in Barausse et al 2023 are available here.
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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