Results 21 to 30 of about 4,540 (191)

Doppler effect in TianQin time-delay interferometry [PDF]

open access: yesPhysical Review D, 2023
10 pages, 11 figures, revised to match the version accepted by Phys.
Lu Zheng, Shutao Yang, Xuefeng Zhang
openaire   +3 more sources

Plasma noise in TianQin time-delay interferometry [PDF]

open access: yesPhysical Review D, 2022
12 pages, 15 figures, accepted by Phys.
Yi-De Jing   +6 more
openaire   +3 more sources

Time-delay interferometry with onboard optical delays [PDF]

open access: yesPhysical Review D
Time-delay interferometry (TDI) is a data processing technique for space-based gravitational-wave detectors to create laser-noise-free equal-optical-path-length interferometers virtually on the ground. It relies on the interspacecraft signal propagation delays, which are delivered by intersatellite ranging monitors. Also, onboard signal propagation and
Jan Niklas Reinhardt   +5 more
openaire   +5 more sources

On the matrix formulation of time-delay interferometry [PDF]

open access: yes, 2021
Time-delay interferometry (TDI) is a processing step essential for the scientific exploitation of LISA, as it reduces the otherwise overwhelming laser noise in the interferometric measurements. The fundamental idea is to define new laser-noise-free observables by combining appropriately time-shifted measurements.
Bayle, Jean-Baptiste   +3 more
openaire   +3 more sources

Time delay interferometry combinations as instrument noise monitors for LISA [PDF]

open access: yesPhysical Review D, 2022
The LISA mission will likely be a signal dominated detector, such that one challenge is the separation of the different astrophysical sources, and to distinguish between them and the instrumental noise. One of the goals of LISA is to probe the early Universe by detecting stochastic GW backgrounds. As correlation with other detectors is not possible for
Martina Muratore   +3 more
openaire   +7 more sources

Time-delay interferometry for LISA with one arm dysfunctional [PDF]

open access: yesClassical and Quantum Gravity, 2010
In order to attain the requisite sensitivity for LISA - a joint space mission of the ESA and NASA- the laser frequency noise must be suppressed below the secondary noises such as the optical path noise, acceleration noise etc. By combining six appropriately time-delayed data streams containing fractional Doppler shifts - a technique called time delay ...
Dhurandhar, S. V.   +2 more
openaire   +5 more sources

Revisitation of algebraic approach for time delay interferometry [PDF]

open access: yesPhysical Review D, 2023
Time Delay Interferometry (TDI) is often utilized in the data pre-processing of space-based gravitational wave detectors, primarily for suppressing laser frequency noise. About twenty years ago, assuming armlengths remain constant over time, researchers presented comprehensive mathematical descriptions for the first-generation and modified first ...
Weisheng Huang   +3 more
openaire   +3 more sources

Time delay interferometry with minimal null frequencies [PDF]

open access: yesPhysical Review D
14 pages, 10 figures, accepted for publication in ...
Wang, Gang
openaire   +4 more sources

Split-And-Delay Unit for FEL Interferometry in the XUV Spectral Range [PDF]

open access: yesApplied Sciences, 2017
In this work we present a reflective split-and-delay unit (SDU) developed for interferometric time-resolved experiments utilizing an (extreme ultraviolet) XUV pump–XUV probe scheme with focused free-electron laser beams.
Sergey Usenko   +8 more
doaj   +2 more sources

Time-Delay Interferometry for ASTROD-GW [PDF]

open access: yes
In the detection of gravitational waves in space, the arm lengths between spacecraft are not equal due to their orbital motion. Consequently, the equal arm length Michelson interferometer used in Earth laboratories is not suitable for space. To achieve the necessary sensitivity for space gravitational wave detectors, laser frequency noise must be ...
Wang, Gang
openaire   +3 more sources

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