LISA Symposium 2026 - Parallel 2-A @LISAcommunity

Uploaded August 2026 | Updated September 2026, 3 hours ago

(Recorded on June 22, 2026)

16th LISA Symposium Parallel Sessions
Parallel 2-A: Binaries & Multi-messenger Science

Presentations in this session:
00:01:00 - When can two nearby LISA sources look like one?
Cezar Ionescu

00:17:05 - Multimessenger Modelling of Massive Binary Black Holes: Eccentric, MAD, and Radiation GRMHD simulations
Vikram Manikantan

00:33:55 - Delensing LISA standard sirens with the CMB
Charlie Mpetha

00:48:05 - Multi-messenger Constraints on Massive Black Hole Binary Hardening Timescales and Implications for LISA
Cordell Harris

01:03:05 - Joint multi-messenger inference of double white dwarf binaries
Nina Kunert

01:17:20 - How sensitive are electromagnetic surveys to the LISA Galactic binary population?
Joheen Chakraborty

Session Chair: Tyson Littenberg

$Stochastic background of gravitational waves from turns in the landscape Stochastic background of gravitational waves from turns in the landscape Jacopo Fumagalli,Sebastien Renaux-Petel,Lukas Witkovski We have recently proposed a new model-independent mechanism for producing primordial black holes from a period of multi-ﬁeld inﬂation. The desired enhancement of primordial ﬂuctuations at short scales naturally occurs when the inﬂationary trajectory exhibits a strong turn, that is a limited period during which the trajectory strongly deviates from a geodesic in ﬁeld space. The mechanism, independently of being able to account for all or a fraction of dark matter in the form of primordial black holes, has the potential of exhibiting unique features accessible to observation through a stochastic background of gravitational waves. The peculiar features in the induced gravitational waves spectrum, such as characteristic peaks and oscillating patterns, oﬀers the possibility to link the microscopic dynamics of inﬂation with the gravitational waves energy density potentially detectable by LISA.$

Probing cosmic structures with gravitational wave lensing

LISA Symposium XIV Parallel C LISA Data Analysis 1 part 1

Status of pseudo-random noise ranging performance and optical data communication

GRMHD simulations of accretion flows onto spinning black hole binary mergers

Monte Carlo Analysis of LISA Telescope Build Process

Radiation-induced degradation of low noise quadrant photoreceivers for LISA

LISA Symposium XIV Parallel B Astrophysics with LISA 2 part 2