# Coupling of wavefront errors and pointing jitter in the LISA interferometer: misalignments of the interfering wavefronts

## TL;DR

This paper analyzes how misalignments and aberrations of wavefronts caused by spacecraft jitter affect the noise in the LISA interferometer, crucial for gravitational wave detection.

## Contribution

It provides an analytical investigation of the coupling between wavefront misalignments and aberrations, estimating their impact on heterodyne signal noise in LISA.

## Key findings

- Coupling between misalignments and aberrations significantly affects noise levels.
- Analytical estimates of noise contributions due to wavefront errors.
- Implications for spacecraft jitter control in LISA design.

## Abstract

The Laser Interferometer Space Antenna is a foreseen space-based gravitational wave detector, which aims to detect 10^20 strains in the frequency range from 0.1 mHz to 1 Hz. It is a triangular constellation of three spacecraft, with equal sides of 2,5 x 10^9 m, where every spacecraft hosts a pair of telescopes that simultaneously transmit and receive laser beams measuring the constellation arms by heterodyning the received wavefronts with local references. Due to the spacecraft and constellation jitters, the interfering (received and local) wavefronts become misaligned. We investigate analytically the coupling between misalignments and aberrations of the interfering wavefronts and estimate the relevant contribution to the noise of the heterodyne signal.