Applying Bayesian methods to detect GWs and derive timing solutions for pulsar timing arrays. Zoom image.
Understanding the extraction of physical information from GW detections. Zoom image.
Building accurate signal models and designing effective search strategies. Zoom image.
Astrophysics, cosmology, and fundamental physics with low-frequency GW sources. Zoom image.
A lecture series (and soon book) to help scientists rediscover the joy of scientific computing. Zoom image.
Popularizing GW science in the scientific community and with the general public with websites, print media, and artistic performances. Zoom image.
Understanding, modeling, and improving Time Delay Interferometry (TDI), the LISA technique to cancel laser noise and measure GWs. Zoom image.
My high-fidelity open-source simulator of the LISA response to instrument noise and GWs, used worldwide to characterize the LISA performance and develop data-analysis algorithm. Zoom image.
An international collaboration (2006–2011) to demonstrate the solution to the LISA data-analysis problem. Zoom image.
Constraining the equation of state of neutron stars by GW observations. Learn more.
Simulating and characterizing GW emission by the r-mode instability. Learn more.
Investigating the philosophical foundations of spacetime theories. Learn more.
© M. Vallisneri 2014 — last modified on 2013/11/05
Tantum in modicis, quantum in maximis