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2017

Galactic binary science with the new LISA design

Cornish, Neil, Robson, Travis

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Building on the great success of the LISA Pathfinder mission, the outlines of a new LISA mission design were laid out at the $11^{\rm th}$ International LISA Symposium in Zurich.

The revised design calls for three identical spacecraft forming an equilateral triangle with 2.5 million kilometer sides, and two laser links per side delivering full polarization sensitivity.
With the demonstrated Pathfinder performance for the disturbance reduction system, and a well studied design for the laser metrology, it is anticipated that the new mission will have a sensitivity very close to the original LISA design.
This implies that the mid-band performance, between 0.5 mHz and 3 mHz, will be limited by unresolved signals from compact binaries in our galaxy.

Galactic binary science with the new LISA design · Around

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Bender P, Brillet A, Ciufolini I, Cruise A, Cutler C, Danzmann K, Fidecaro F, Folkner W, Hough J, McNamara P, Peterseim M, Robertson D, Rodrigues M, Rüdiger A, Sandford M, Schäfer G, Schilling R, Schutz B, Speake C, Stebbins R, Sumner T, Touboul P, Vinet J, Vitale S, Ward H and Winkler W 1998 Laser interferometer space antenna for the detection and observation of gravitational waves Tech. rep. NASA mPQ 233, Second Edition URL https://lisa.gsfc.nasa.gov/Documentation/ppa2.08.pdf
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Nelemans G and Tout C A 2005 MNRAS 356
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Timpano S E, Rubbo L J and Cornish N J 2006 Phys. Rev. D
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Roelofs G H A, Nelemans G and Groot P J 2007 MNRAS 382
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Cornish N J and Littenberg T B 2007 Phys. Rev. D
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