scholarly journals Low frequency gravitational wave detection with ground-based atom interferometer arrays

2016 ◽  
Vol 93 (2) ◽  
Author(s):  
W. Chaibi ◽  
R. Geiger ◽  
B. Canuel ◽  
A. Bertoldi ◽  
A. Landragin ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Low Frequency ◽  
Atom Interferometer ◽  
Gravitational Wave Detection ◽  
Wave Detection

First results from the pisa seismic noise super-attenuator for low frequency gravitational wave detection

1988 ◽  
Vol 132 (5) ◽  
pp. 237-240 ◽  
Author(s):  
R. Del Fabbro ◽  
A. Di Virgilio ◽  
A. Giazotto ◽  
H. Kautzky ◽  
V. Montelatici ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Seismic Noise ◽  
Low Frequency ◽  
Gravitational Wave Detection ◽  
Wave Detection ◽  
First Results

scholarly journals A Spaceborne Multi-Arm Interferometer for VLF Gravitational Wave Detection. (The SMILE Project)

1988 ◽  
Vol 129 ◽  
pp. 321-322
Author(s):  
Allen Joel Anderson
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
Low Frequency ◽  
Deep Space ◽  
Detection Capability ◽  
Gravitational Wave Detection ◽  
Very Low Frequency ◽  
Wave Detection ◽  
Designed Experiment ◽  
Spacecraft Tracking

This project would be the next step in our ability to detect very low frequency (VLF) gravitational waves and the first committed spaceborne designed experiment. Present Deep Space spacecraft tracking experiments are severely limited in their detection capability. It is proposed to construct a spaceborne multi-arm microwave interferometer using current elements of design applicable for the detection of VLF gravitational waves. The elements are outlined with particular emphasis placed on the utilization of small inexpensive get away special (GAS) modules currently under development at JPL for launch in the 1990's.

scholarly journals Low-frequency gravitational wave detection via double optical clocks in space

2018 ◽  
Vol 35 (8) ◽  
pp. 085010 ◽  
Author(s):  
Jianfeng Su ◽  
Qiang Wang ◽  
Qinghua Wang ◽  
Philippe Jetzer
Keyword(s):  
Gravitational Wave ◽  
Low Frequency ◽  
Gravitational Wave Detection ◽  
Wave Detection

Low frequency behaviour of the Pisa seismic noise super-attenuator for gravitational wave detection

1988 ◽  
Vol 133 (9) ◽  
pp. 471-475 ◽  
Author(s):  
R. Del Fabbro ◽  
A. Di Virgilio ◽  
A. Giazotto ◽  
H. Kautzky ◽  
V. Montelatici ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Seismic Noise ◽  
Low Frequency ◽  
Gravitational Wave Detection ◽  
Wave Detection

scholarly journals Gravitational-Wave Detection Using Pulsars: Status of the Parkes Pulsar Timing Array Project

2009 ◽  
Vol 26 (2) ◽  
pp. 103-109 ◽  
Author(s):  
G. B. Hobbs ◽  
M. Bailes ◽  
N. D. R. Bhat ◽  
S. Burke-Spolaor ◽  
D. J. Champion ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
Direct Detection ◽  
Low Frequency ◽  
Current Status ◽  
Binary Black Holes ◽  
Gravitational Wave Detection ◽  
Wave Detection ◽  
Pulsar Timing ◽  
Pulsar Timing Array

AbstractThe first direct detection of gravitational waves may be made through observations of pulsars. The principal aim of pulsar timing-array projects being carried out worldwide is to detect ultra-low frequency gravitational waves (f ∼ 10−9–10−8 Hz). Such waves are expected to be caused by coalescing supermassive binary black holes in the cores of merged galaxies. It is also possible that a detectable signal could have been produced in the inflationary era or by cosmic strings. In this paper, we review the current status of the Parkes Pulsar Timing Array project (the only such project in the Southern hemisphere) and compare the pulsar timing technique with other forms of gravitational-wave detection such as ground- and space-based interferometer systems.

Three-dimensional seismic super-attenuator for low frequency gravitational wave detection

1987 ◽  
Vol 124 (4-5) ◽  
pp. 253-257 ◽  
Author(s):  
R. Del Fabbro ◽  
A. Di Virgilio ◽  
A. Giazotto ◽  
H. Kautzky ◽  
V. Montelatici ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Three Dimensional ◽  
Low Frequency ◽  
Gravitational Wave Detection ◽  
Wave Detection

THE LISA PATHFINDER MISSION

2013 ◽  
Vol 22 (01) ◽  
pp. 1341001 ◽  
Author(s):  
PAUL W. McNAMARA
Keyword(s):  
Gravitational Wave ◽  
Inertial Sensors ◽  
European Space Agency ◽  
Low Frequency ◽  
Free Fall ◽  
Flight Test ◽  
Measurement Technology ◽  
Gravitational Wave Detection ◽  
Wave Detection ◽  
Lisa Pathfinder

Laser Interferometer Space Antenna (LISA) Pathfinder (formerly known as SMART-2) is a European Space Agency mission designed to pave the way for the joint ESA/NASA LISA mission by testing in flight the critical technologies required for space borne gravitational wave detection; it will put two test masses in a near-perfect gravitational free-fall and control and measure their motion with unprecedented accuracy. This is achieved through technology comprising inertial sensors, high precision laser metrology, drag-free control and an ultra precise micro-Newton propulsion system. LISA Pathfinder (LPF) essentially mimics one arm of space-borne gravitational wave detectors by shrinking the million kilometer scale armlengths down to a few tens of centimeters, giving up the sensitivity to gravitational waves, but keeping the measurement technology. The scientific objective of the LPF mission consists then of the first in-flight test of low frequency gravitational wave detection metrology.

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