#LISACommunityTalks

The #LISACommunity recently hosted a talk by Ollie Burke about a paper by Ollie Burke, Sylvain Marsat, Jonathan R. Gair, Michael L. Katz: "Mind the gap: addressing data gaps and assessing noise mismodeling in LISA", which can be found here 👉 https://arxiv.org/abs/2502.17426

Here's a summary of the paper:

"Communication outages and malfunctions for complicated space-missions are simply an inevitability. Although talented personnel will craft an instrument that runs as smoothly as possible, the space-based gravitational wave observatory LISA will be no outlier — LISA will observe gaps and gremlins in the data. These artefacts could violate a number of assumptions scientists usually place on the data prior to analysis, potentially hampering our ability to extract gravity waves from the data that are generated from collisions of the most extreme compact objects within our universe. This talk (with associated paper) details calculations, theory and computational techniques that can be used to mitigate the impact of data gaps on LISA-based gravitational wave data analysis."

#LISACommunityTalks

The #LISACommunity recently hosted a talk by David Maibach about a paper by Nils Deppe, Lavinia Heisenberg, Henri Inchauspé, Lawrence E. Kidder, David Maibach, Sizheng Ma, Jordan Moxon, Kyle C. Nelli, William Throwe, Nils L. Vu: "Echoes from Beyond: Detecting Gravitational Wave Quantum Imprints with LISA", which can be found here 👉 https://arxiv.org/abs/2411.05645

#LISACommunityTalks

The #LISACommunity recently hosted a talk by Sarah Paczkowski about a paper by Marie-Sophie Hartig, Sarah Paczkowski, Martin Hewitson, Gerhard Heinzel, Gudrun Wanner: "Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals", which can be found here 👉 https://arxiv.org/abs/2411.14191 and https://journals.aps.org/prd/abstract/10.1103/PhysRevD.111.043048

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals

The Laser Interferometer Space Antenna (LISA) will be the first space-based gravitational wave (GW) observatory. It will measure gravitational wave signals in the frequency regime from 0.1 mHz to 1 Hz. The success of these measurements will depend on the suppression of the various instrument noises. One important noise source in LISA will be tilt-to-length (TTL) coupling. Here, it is understood as the coupling of angular jitter, predominantly from the spacecraft, into the interferometric length readout. The current plan is to subtract this noise in-flight in post-processing as part of a noise minimization strategy. It is crucial to distinguish TTL coupling well from the GW signals in the same readout to ensure that the noise will be properly modeled. Furthermore, it is important that the subtraction of TTL noise will not degrade the GW signals. In the present manuscript, we show on simulated LISA data and for four different GW signal types that the GW responses have little effect on the quality of the TTL coupling fit and subtraction. Also, the GW signal characteristics were not altered by the TTL coupling subtraction.

arXiv.org

#LISACommunityTalks

The #LISACommunity recently hosted a talk by Jan Niklas Reinhardt on a paper by Jan Niklas Reinhardt, Olaf Hartwig, Gerhard Heinzel: "Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors", linked here 👉 https://arxiv.org/abs/2408.09832 and https://iopscience.iop.org/article/10.1088/1361-6382/ada2d3

Here's a summary of the paper:

"Space-based gravitational-wave detectors, such as LISA, record interferometric measurements on widely separated satellites. Their clocks are not actively synchronized. Instead, clock synchronization is performed in on-ground data processing using pseudorange measurements, which entangle the interspacecraft ranges with the relative clock desynchronizations. To achieve clock synchronization between the spacecraft, we need to isolate these clock desynchronizations by disentangling the pseudoranges. We introduce a nonstandard Kalman filter algorithm for this purpose, designed for systems where pseudorange measurements are taken in different time frames. This algorithm enables clock synchronization and light travel time estimation with sub-meter accuracy."

Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors

Space-based gravitational-wave detectors, such as LISA, record interferometric measurements on widely separated satellites. Their clocks are not synced actively. Instead, clock synchronization is performed in on-ground data processing. It relies on measurements of the so-called pseudoranges, which entangle the interspacecraft light travel times with the clock desynchronizations between emitting and receiving spacecraft. For interspacecraft clock synchronization, we need to isolate the differential clock desynchronizations, i.e., disentangle the pseudoranges. This further yields estimates for the interspacecraft light travel times, which are required as delays for the laser frequency noise suppression via time-delay interferometry. Previous studies on pseudorange disentanglement apply various simplifications in the pseudorange modeling and the data simulation. In contrast, this article derives an accurate pseudorange model in the barycentric celestial reference system, complemented by realistic state-of-the-art LISA data simulations. Concerning pseudorange disentanglement, this leads to an a priori under-determined system. We demonstrate how on-ground orbit determinations, as well as onboard transmission and on-ground reception time tags of the telemetry data, can be used to resolve this degeneracy. We introduce an algorithm for pseudorange disentanglement based on a nonstandard Kalman filter specially designed for clock synchronization in systems where pseudorange measurements are conducted in different time frames. This algorithm achieves interspacecraft clock synchronization and light travel time estimation with submeter accuracy, thus fulfilling the requirements of time-delay interferometry.

arXiv.org

#LISACommunityTalks

The #LISACommunity recently hosted a talk by Valerio De Luca on a paper by Valerio De Luca, Justin Khoury, Sam S. C. Wong: "Gravitational memory and soft theorems: the local perspective", linked here 👉 https://arxiv.org/abs/2412.01910 and https://arxiv.org/abs/2412.12273 (accepted in PRD at https://journals.aps.org/prd/accepted/76071Qd0M2118331f5b87943d34c36b167b45d9d9)

Here's a summary of the paper:

"Gravitational memory describes the lasting effect on freely falling detectors after a gravitational wave passes by, and it has been intimately connected to asymptotic symmetries and soft theorems.
In this talk, we will explore a new symmetry perspective of gravitational memory in synchronous coordinates, which are relevant for detectors like LISA.
We will show how memory ties to residual coordinate transformations, such as volume-preserving spatial rescalings, and we will derive the corresponding soft theorems for both scattering amplitudes and correlation functions. The latter are recognized as the flat-space analog of soft theorems in inflationary cosmology."

Gravitational memory and soft theorems: The local perspective

In general relativity, gravitational memory describes the lasting change in the separation and relative velocity of freely falling detectors after the passage of gravitational waves (GWs). In this paper, we elucidate the relation between Bondi-Metzner-Sachs transformations at future null infinity and the description of gravitational memory in local synchronous coordinates, commonly used in GW detectors like LISA. We show that gravitational memory corresponds to large residual diffeomorphisms in this gauge, such as volume-preserving spatial rescalings. We reproduce the associated soft theorems for scattering amplitudes. Finally, we derive novel soft theorems for equal-time (in-in) correlation functions, which are recognized as the flat space analogues of inflationary consistency relations with a soft tensor mode. These relations provide a pathway toward uncovering deeper connections between gravitational memory and cosmological correlators.

arXiv.org

#LISACommunityTalks

The #LISACommunity recently hosted a talk by Senwen Deng on a paper by Senwen Deng, Stanislav Babak, Maude Le Jeune, Sylvain Marsat, Éric Plagnol, Andrea Sartirana: "Modular global-fit pipeline for LISA data analysis", linked here 👉 https://arxiv.org/abs/2501.10277

Here's a summary of the paper:

"The #LISAMission data band is expected to be dominated by gravitational wave signals emitted by a plethora of astrophysical sources. Signals of the Galactic white dwarf Binaries are long-lived, overlapping in time and their unresolved residual forms a confusion noise. Massive Black Hole Binary signals are loud and broadband, hindering the estimation of the noise property, the knowledge of which is key to the detection and parameter estimation for the gravitational wave signals. We came up with a modular two-stage iterative pipeline prototype to disentangle the intertwined signals and to infer the parameters for the different signal sources and the noise level. We demonstrated its capability by applying it to simulated LISA dataset known as "Sangria", where we managed to recover the injected parameters at the simulation with faithfulness."

Modular global-fit pipeline for LISA data analysis

We anticipate that the data acquired by the Laser Interferometer Space Antenna (LISA) will be dominated by the gravitational wave signals from several astrophysical populations. The analysis of these data is a new challenge and is the main focus of this paper. Numerous gravitational wave signals overlap in the time and/or frequency domain, and the possible correlation between them has to be taken into account during their detection and characterization. In this work, we present a method to address the LISA data analysis challenge; it is flexible and scalable for a number of sources and across several populations. Its performance is demonstrated on the simulated data LDC2a.

arXiv.org