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First search for ultralight dark matter with a space-based gravitational-wave antenna: LISA Pathfinder
DOI: 10.1103/PhysRevD.107.063015 Bibcode: 2023PhRvD.107f3015M

Miller, Andrew L.; Mendes, Luis

We present here results from the first-ever search for dark-photon dark matter that could have coupled to baryons in LISA Pathfinder, the technology demonstrator for a space-based gravitational-wave antenna. After analyzing approximately three months of data taken by LISA Pathfinder in the frequency range [2 ×10-5,5 ] Hz , corresponding…

2023 Physical Review D
LISAPathfinder 22
Charging of free-falling test masses in orbit due to cosmic rays: Results from LISA Pathfinder
DOI: 10.1103/PhysRevD.107.062007 Bibcode: 2023PhRvD.107f2007A

Mendes, L.; Russano, G.; Nofrarias, M. +72 more

A comprehensive summary of the measurements made to characterize test-mass charging due to the space environment during the LISA Pathfinder mission is presented. Measurements of the residual charge of the test mass after release by the grabbing and positioning mechanism show that the initial charge of the test masses was negative after all release…

2023 Physical Review D
INTEGRAL LISAPathfinder 12
Tilt-to-length coupling in LISA Pathfinder: A data analysis
DOI: 10.1103/PhysRevD.108.102003 Bibcode: 2023PhRvD.108j2003A

Mendes, L.; Russano, G.; Sanjuan, J. +76 more

We present a study of the tilt-to-length coupling noise during the LISA Pathfinder mission and how it depended on the system's alignment. Tilt-to-length coupling noise is the unwanted coupling of angular and lateral spacecraft or test mass motion into the primary interferometric displacement readout. It was one of the major noise sources in the LI…

2023 Physical Review D
LISAPathfinder 9
Tilt-to-length coupling in LISA Pathfinder: Analytical modeling
DOI: 10.1103/PhysRevD.108.022008 Bibcode: 2023PhRvD.108b2008H

Hartig, Marie-Sophie; Wanner, Gudrun

Tilt-to-length coupling was the limiting noise source in LISA Pathfinder between 20 and 200 mHz before subtraction in postprocessing. To prevent the adding of sensing noise to the data by the subtraction process, the success of this strategy depended on a previous direct noise reduction by test mass alignment. The exact dependency of the level of …

2023 Physical Review D
LISAPathfinder 8
Simulating the charging of isolated free-falling masses from TeV to eV energies: Detailed comparison with LISA Pathfinder results
DOI: 10.1103/PhysRevD.107.022010 Bibcode: 2023PhRvD.107b2010W

Hollington, D.; Wass, P. J.; Sumner, T. J. +1 more

A model is presented that explains the charging rate of the LISA Pathfinder test masses by the interplanetary cosmic ray environment. The model incorporates particle-tracking from TeV to eV energies using a combination of GEANT4 and a custom low-energy particle generation and tracking code. The electrostatic environment of the test mass is simulat…

2023 Physical Review D
LISAPathfinder 6
Noise effect of test mass surface roughness in spaceborne gravitational wave detectors
DOI: 10.1103/PhysRevD.108.042001 Bibcode: 2023PhRvD.108d2001Y

Wang, Shun; Yan, Hao; Miao, Haixing +2 more

The spaceborne gravitational wave detection mission has a demanding requirement for the precision of displacement sensing, which is conducted by the interaction between the laser field and test mass. However, due to the roughness of the reflecting surface of the test mass, the displacement measurement along the sensitive axis suffers a coupling er…

2023 Physical Review D
LISAPathfinder 0