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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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CONTACT INFORMATION
International School for Advanced Studies (SISSA)
Associate Professor-Physics
Office:
Scuola Internazionale Superiore di Studi Avanzati - Physics Department
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Office A-531 (Main building- East)
Via Bonomea, 265, 34136 Trieste TS, Italy
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barausse[at]sissa.it
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+39 040 3787 867 (office)
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