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Open AccessJournal ArticleDOI

Charge-induced force-noise on free-falling test masses: results from LISA Pathfinder

Michele Armano, +94 more
- 26 Apr 2017 - 
- Vol. 118, Iss: 17, pp 171101-171101
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TLDR
Electrostatic measurements made on board the European Space Agency mission LISA Pathfinder are the first made in a relevant environment for a space-based gravitational wave detector and resolve the stochastic nature of the TM charge buildup due to interplanetary cosmic rays and theTM charge-to-force coupling through stray electric fields in the sensor.
Abstract
We report on electrostatic measurements made on board the European Space Agency mission LISA Pathfinder. Detailed measurements of the charge-induced electrostatic forces exerted on free-falling test masses (TMs) inside the capacitive gravitational reference sensor are the first made in a relevant environment for a space-based gravitational wave detector. Employing a combination of charge control and electric-field compensation, we show that the level of charge-induced acceleration noise on a single TM can be maintained at a level close to 1.0  fm s-2 Hz-1/2 across the 0.1–100 mHz frequency band that is crucial to an observatory such as the Laser Interferometer Space Antenna (LISA). Using dedicated measurements that detect these effects in the differential acceleration between the two test masses, we resolve the stochastic nature of the TM charge buildup due to interplanetary cosmic rays and the TM charge-to-force coupling through stray electric fields in the sensor. All our measurements are in good agreement with predictions based on a relatively simple electrostatic model of the LISA Pathfinder instrument.

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Citations
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Journal ArticleDOI

Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μHz.

Michele Armano, +78 more
TL;DR: This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.
Journal ArticleDOI

Dynamical Boson Stars

TL;DR: This work discusses important varieties of boson stars, their dynamic properties, and some of their uses, concentrating on recent efforts.
Journal ArticleDOI

The LISA–Taiji network

TL;DR: In this article, a potential LISA-Taiji network is explored to fast and accurately localize the gravitational-wave sources, assuming a one-year overlap of the LISA and Taiji launches.
Journal ArticleDOI

Concepts and status of Chinese space gravitational wave detection projects

TL;DR: In this article, the concepts and development milestones of two Chinese space-based GW observatories, TianQin and Taiji, are introduced and discussed possible collaborations among them to improve GW source localization and characterization.
Journal ArticleDOI

Capacitive sensing of test mass motion with nanometer precision over millimeter-wide sensing gaps for space-borne gravitational reference sensors

TL;DR: In this article, the performance of the capacitive gap-sensing system of the Gravitational Reference Sensor on board the LISA Pathfinder spacecraft was reported, with a performance of up to 1mHz.
References
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Journal ArticleDOI

Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results

Michele Armano, +118 more
TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.
Journal ArticleDOI

Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy

Denis Martynov, +262 more
- 02 Jun 2016 - 
TL;DR: The first observation run of the Advanced LIGO detectors started in September 2015 and ended in January 2016 as discussed by the authors, which achieved a strain sensitivity of better than 10^(−23)/√Hz around 100 Hz.
Journal ArticleDOI

The LTP interferometer and phasemeter

TL;DR: The LISA Technology Package (LTP) is a technology demonstration mission in preparation for the LISA space-borne gravitational wave detector as mentioned in this paper, which monitors the distance between two test masses with a noise level of 10 pm Hz−1/2 between 3 mHz and 30 mHz.
Journal ArticleDOI

Gravitational sensor for LISA and its technology demonstration mission

TL;DR: In this article, the current design of the European gravitational sensor (GS) for the LISA Technology Package (LTP) is described, on board the mission SMART-2, which aims to demonstrate geodetic motion within one order of magnitude of the anticipated LISA performance.
Journal ArticleDOI

Detailed calculation of test-mass charging in the LISA mission

TL;DR: In this paper, the authors report on detailed charging simulations with the Geant4 toolkit, using comprehensive geometry and physics models, for Galactic cosmic-ray protons and helium nuclei.
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