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Advanced localization of massive black hole coalescences with LISA
Ryan N. Lang, Scott A. Hughes
The coalescence of massive black holes is one of the primary sources of gravitational waves (GWs) for LISA. Measurements of the GWs can localize the source on the sky to an ellipse…
The Self-Gravity of Pressure in Neutron Stars
Josiah Schwab, Scott A. Hughes, Saul Rappaport
Following an earlier analysis which examined the effect of the self-gravity of pressure on big-bang nucleosynthesis (BBN), we explore the effect of pressure's self-gravity on the s…
Localizing coalescing massive black hole binaries with gravitational waves
Ryan N. Lang, Scott A. Hughes
Massive black hole binary coalescences are prime targets for space-based gravitational wave (GW) observatories such as {\it LISA}. GW measurements can localize the position of a co…
Short GRB and binary black hole standard sirens as a probe of dark energy
Neal Dalal, Daniel E. Holz, Scott A. Hughes +1
Observations of the gravitational radiation from well-localized, inspiraling compact object binaries can measure absolute source distances with high accuracy. When coupled with an…
Using gravitational-wave standard sirens
Daniel E. Holz, Scott A. Hughes
Gravitational waves (GWs) from supermassive binary black hole (BBH) inspirals are potentially powerful standard sirens (the GW analog to standard candles) (Schutz 1986, 2002). Beca…
Golden Binary Gravitational-Wave Sources: Robust Probes of Strong-Field Gravity
Scott A. Hughes, Kristen Menou
Space-born gravitational-wave interferometers such as {\it LISA} will detect the gravitational wave (GW) signal from the inspiral, plunge and ringdown phases of massive black hole…