Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …

Abstract The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to
detect and study gravitational waves from space. LISA will survey the sky for Gravitational …

We use the latest constraints on the population of stellar origin binary black holes (SOBBH)
from LIGO/Virgo/KAGRA (LVK) observations, to estimate the stochastic gravitational wave …

The novel data analysis challenges posed by the Laser Interferometer Space Antenna
(LISA) arise from the overwhelmingly large number of astrophysical sources in the …

The Laser Interferometer Space Antenna (LISA) is a planned space-based observatory to
measure gravitational waves in the millihertz frequency band. This frequency band is …

Realistic models of the Galactic double white dwarf (DWD) population are crucial for testing
and quantitatively defining the science objectives of the Laser Interferometer Space Antenna …

In the next decade, the Laser Interferometer Space Antenna (LISA) will detect the
coalescence of massive black hole binaries (MBHBs) in the range [10 4, 10 8] M⊙, up to z∼ …

We develop a tool for the analysis of stochastic gravitational wave backgrounds from
cosmological first-order phase transitions with LISA: we initiate a template databank for …

Various scenarios of cosmic inflation enhance the amplitude of the stochastic gravitational
wave background (SGWB) at frequencies detectable by the LISA detector. We develop tools …