papers

Publications (26)

gr-qc2015

Testing General Relativity with Present and Future Astrophysical Observations

Emanuele Berti, Enrico Barausse, Vitor Cardoso +50

One century after its formulation, Einstein's general relativity has made remarkable predictions and turned out to be compatible with all experimental tests. Most of these tests pr…

gr-qc2021

An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations

Andrew Matas, Tim Dietrich, Alessandra Buonanno +8

After the discovery of gravitational waves from binary black holes (BBHs) and binary neutron stars (BNSs) with the LIGO and Virgo detectors, neutron-star--black-holes (NSBHs) are t…

hep-th2015

Point particle motion in topologically nontrivial space-times

Andrew Matas, Daniel Müller, Glenn Starkman

It is well known that compactifying a space can break symmetries that are present in the covering space. In this paper we study the effects of such topological symmetry breaking on…

gr-qc2020

Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA

Florian Kuhnel, Andrew Matas, Glenn D. Starkman +1

A significant fraction of cosmological dark matter can be formed by very dense macroscopic objects, for example primordial black holes. Gravitational waves offer a promising way to…

gr-qc2023

pygwb: Python-based library for gravitational-wave background searches

Arianna I. Renzini, Alba Romero-Rodrguez, Colm Talbot +31

The collection of gravitational waves (GWs) that are either too weak or too numerous to be individually resolved is commonly referred to as the gravitational-wave background (GWB).…

gr-qc2023

A stochastic search for intermittent gravitational-wave backgrounds

Jessica Lawrence, Kevin Turbang, Andrew Matas +3

A likely source of a gravitational-wave background (GWB) in the frequency band of the Advanced LIGO, Virgo and KAGRA detectors is the superposition of signals from the population o…

hep-th2015

New Kinetic Terms for Massive Gravity and Multi-gravity: A No-Go in Vielbein Form

Claudia de Rham, Andrew Matas, Andrew J. Tolley

We reconsider the possibility of a class of new kinetic terms in the first order (vielbein) formulation of massive gravity and multi-gravity. We find that new degrees of freedom em…

hep-th2013

Deconstructing Dimensions and Massive Gravity

Claudia de Rham, Andrew Matas, Andrew J. Tolley

We show that the ghost-free models of massive gravity and their multi-graviton extensions follow from considering higher dimensional General Relativity in Einstein-Cartan form on a…

gr-qc2021

The Next Generation Global Gravitational Wave Observatory: The Science Book

Vicky Kalogera, B. S. Sathyaprakash, Matthew Bailes +88

The next generation of ground-based gravitational-wave detectors will observe coalescences of black holes and neutron stars throughout the cosmos, thousands of them with exceptiona…

gr-qc2020

Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches

Andrew Matas, Joseph D. Romano

Sufficient statistics are combinations of data in terms of which the likelihood function can be rewritten without loss of information. Depending on the data volume reduction, the u…

hep-th2014

Interactions of Charged Spin-2 Fields

Claudia de Rham, Andrew Matas, Nicholas Ondo +1

In light of recent progress in ghost-free theories of massive gravity and multi-gravity, we reconsider the problem of constructing a ghost-free theory of an interacting spin-2 fiel…

hep-th2012

Galileon Radiation from Binary Systems

Claudia de Rham, Andrew Matas, Andrew J. Tolley

We calculate the power emitted in scalar modes for a binary systems, including binary pulsars, with a conformal coupling to the most general Galileon effective field theory by cons…

gr-qc2017

Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background

Thomas Callister, A. Sylvia Biscoveanu, Nelson Christensen +7

The direct observation of gravitational waves with Advanced LIGO and Advanced Virgo offers novel opportunities to test general relativity in strong-field, highly dynamical regimes.…

astro-ph.HE2018

A first search for a stochastic gravitational-wave background from ultralight bosons

Leo Tsukada, Thomas Callister, Andrew Matas +1

In this work, we develop a Bayesian data analysis framework to study the SGWB from bosonic clouds using data from Advanced LIGO and Advanced Virgo, building on previous work by Bri…

astro-ph.HE2019

Cosmology and the Early Universe

B. S. Sathyaprakash, Enis Belgacem, Daniele Bertacca +15

This Astro-2020 White Paper deals with what we might learn from future gravitational wave observations about the early universe phase transitions and their energy scales, primordia…

hep-th2016

Ostrogradsky in Theories with Multiple Fields

Claudia de Rham, Andrew Matas

We review how the (absence of) Ostrogradsky instability manifests itself in theories with multiple fields. It has recently been appreciated that when multiple fields are present, t…

hep-th2014

New Kinetic Interactions for Massive Gravity?

Claudia de Rham, Andrew Matas, Andrew J. Tolley

We show that there can be no new Lorentz invariant kinetic interactions free from the Boulware-Deser ghost in four dimensions in the metric formulation of gravity, beyond the stand…

gr-qc2017

Primordial Black-Hole and Macroscopic Dark-Matter Constraints with LISA

Florian Kuhnel, Glenn D. Starkman, Katherine Freese +1

The detectability of gravitational waves originating from primordial black holes or other large macroscopic dark-matter candidates inspiraling into Sagittarius is i…

hep-th2015

Cutoff for Extensions of Massive Gravity and Bi-Gravity

Andrew Matas

Recently there has been interest in extending ghost-free massive gravity, bi-gravity, and multi-gravity by including non-standard kinetic terms and matter couplings. We first revie…

hep-th2013

Superluminality in the Bi- and Multi- Galileon

Paul de Fromont, Claudia de Rham, Lavinia Heisenberg +1

We re-explore the Bi- and Multi-Galileon models with trivial asymptotic conditions at infinity and show that propagation of superluminal fluctuations is a common and unavoidable fe…

astro-ph.CO2011

Symmetron Cosmology

Kurt Hinterbichler, Justin Khoury, Aaron Levy +1

The symmetron is a scalar field associated with the dark sector whose coupling to matter depends on the ambient matter density. The symmetron is decoupled and screened in regions o…

gr-qc2023

Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population

Deepali Agarwal, Jishnu Suresh, Vuk Mandic +2

The millisecond pulsars, old-recycled objects spinning with high frequency (kHz) sustaining the deformation from their spherical shape, may emit gravitational waves (…

gr-qc2018

Measurement and subtraction of Schumann resonances at gravitational-wave interferometers

Michael W. Coughlin, Alessio Cirone, Patrick Meyers +23

Correlated magnetic noise from Schumann resonances threatens to contaminate the observation of a stochastic gravitational-wave background in interferometric detectors. In previous…

gr-qc2021

Gravitational-wave searches in the era of Advanced LIGO and Virgo

Sarah Caudill, Shivaraj Kandhasamy, Claudia Lazzaro +3

The field of gravitational-wave astronomy has been opened up by gravitational-wave observations made with interferometric detectors. This review surveys the current state-of-the-ar…

astro-ph.IM2018

Multi-wavelength observations of cosmological phase transitions using LISA and Cosmic Explorer

Margot Fitz Axen, Sharan Banagiri, Andrew Matas +2

We reanalyze the detection possibilities for gravitational waves arising from cosmological first order phase transitions. We discuss the stochastic gravitational wave background co…

astro-ph.IM2022

Angular Resolution of the Search for Anisotropic Stochastic Gravitational-Wave Background with Terrestrial Gravitational-Wave Detectors

Erik Floden, Vuk Mandic, Andrew Matas +1

We consider an anisotropic search for the stochastic gravitational-wave (GW) background by decomposing the gravitational-wave sky into its spherical harmonics components. Previous…