Sub-pm root Hz(-1) non-reciprocal noise in the LISA backlink fiber
Sign Up to like & getrecommendations! Published in 2017 at "Classical and Quantum Gravity"
DOI: 10.1088/1361-6382/aaa276
Abstract: The future space-based gravitational wave detector Laser Interferometer Space Antenna (LISA) requires bidirectional exchange of light between its two optical benches on board of each of its three satellites. The current baseline foresees a polarization-maintaining… read more here.
Keywords: phase; sub root; root non; non reciprocal ... See more keywords
Mapping the gravitational-wave sky with LISA: a Bayesian spherical harmonic approach
Sign Up to like & getrecommendations! Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2479
Abstract: The millihertz gravitational-wave frequency band is expected to contain a rich symphony of signals with sources ranging from Galactic white dwarf binaries to extreme mass ratio inspirals. Many of these gravitational-wave signals will not be… read more here.
Keywords: spherical harmonic; gravitational wave; wave; confusion noise ... See more keywords
Background for gravitational wave signal at LISA from refractive index of solar wind plasma
Sign Up to like & getrecommendations! Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnrasl/slaa155
Abstract: A strong indication is presented that the space-based gravitational antennas, in particular the LISA concept introduced in 2017 in response to the ESA call for L3 mission concepts, are going to be sensitive to a… read more here.
Keywords: wind; plasma; lisa; solar wind ... See more keywords
Unified model for the LISA measurements and instrument simulations
Sign Up to like & getrecommendations! Published in 2022 at "Physical Review D"
DOI: 10.1103/physrevd.107.083019
Abstract: LISA is a space-based mHz gravitational-wave observatory, with a planned launch in 2034. It is expected to be the first detector of its kind, and will present unique challenges in instrumentation and data analysis. An… read more here.
Keywords: model lisa; model; lisa measurements; lisa ... See more keywords
How post-Newtonian dynamics shape the distribution of stationary binary black hole LISA sources in nearby globular clusters
Sign Up to like & getrecommendations! Published in 2019 at "Physical Review D"
DOI: 10.1103/physrevd.99.063006
Abstract: We derive the observable gravitational wave (GW) peak frequency ($f$) distribution of binary black holes (BBHs) that currently reside inside their globular clusters (GCs), with and without 2.5 Post-Newtonian (2.5PN) effects included in the dynamical… read more here.
Keywords: lisa; distribution; lisa sources; globular clusters ... See more keywords
Looking Into Mona Lisa’s Smiling Eyes: Allusion to an Illusion
Sign Up to like & getrecommendations! Published in 2022 at "Frontiers in Human Neuroscience"
DOI: 10.3389/fnhum.2022.878288
Abstract: We present results from two experiments aimed at studying the direction of Mona Lisa’s gaze and its affective expression. In experiment 1 we studied the effect of retinal image size on the perception of her… read more here.
Keywords: lisa smiling; mona lisa; group; lisa gaze ... See more keywords