Sensitivity of the spherical gravitational wave detector MiniGRAIL operating at 5 K
arXiv:0705.0122 · doi:10.1103/PhysRevD.76.102005
Abstract
We present the performances and the strain sensitivity of the first spherical gravitational wave detector equipped with a capacitive transducer and read out by a low noise two-stage SQUID amplifier and operated at a temperature of 5 K. We characterized the detector performance in terms of thermal and electrical noise in the system output sygnal. We measured a peak strain sensitivity of at 2942.9 Hz. A strain sensitivity of better than has been obtained over a bandwidth of 30 Hz. We expect an improvement of more than one order of magnitude when the detector will operate at 50 mK. Our results represent the first step towards the development of an ultracryogenic omnidirectional detector sensitive to gravitational radiation in the 3kHz range.
8 pages, 5 figures, submitted to Physical Review D
References in corpus (8)
- What can we learn about GW Physics with an elastic spherical antenna?
- The TIGA technique for detecting gravitational waves with a spherical antenna
- 3-mode detection for widening the bandwidth of resonant gravitational wave detectors
- The mathematical theory of resonant transducers in a spherical gravity wave antenna
- Complete model of a spherical gravitational wave detector with capacitive transducers. Calibration and sensitivity optimization
- Comparison of advanced gravitational-wave detectors
- Solution to the inverse problem for a noisy spherical gravitational wave antenna
- Matched filter for multi-transducers resonant GW antennas
Cited by in corpus (25)
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
- Gravitational Wave Detection by Interferometry (Ground and Space)
- Detecting High-Frequency Gravitational Waves with Microwave Cavities
- Sound of Dark Matter: Searching for Light Scalars with Resonant-Mass Detectors
- Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
- Detecting single gravitons with quantum sensing
- MAGO2.0: Electromagnetic Cavities as Mechanical Bars for Gravitational Waves
- Implications of the Gravitational Wave Event GW150914
- Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
- A brief history of gravitational wave research
- Gravitational waves, dark energy and inflation
- Detection of high energy cosmic rays with the resonant gravitational wave detector NAUTILUS and EXPLORER
- Prospects for Direct Detection of Black Hole Formation in Neutron Star Mergers with Next-Generation Gravitational-Wave Detectors
- Macroscopic Dark Matter Detection with Gravitational Wave Experiments
- Detecting kHz gravitons from a neutron star merger with a multi-mode resonant mass detector
- Gravitational Waves from Preheating in Inflation with Weyl Symmetry
- Coherent detection method of gravitational wave bursts for spherical antennas
- Optical ultra-stable optical clock cavities as resonant mass gravitational wave detectors in search for new physics
- Stochastic backgrounds of gravitational waves from cosmological sources - The role of dark energy
- Vibrational excitation induced by electron beam and cosmic rays in normal and superconductive aluminum bars
- Determination of the neutron star mass-radii relation using narrow-band gravitational wave detector
- High-frequency gravitational waves from first-order phase transitions
- CUORE Opens the Door to Tonne-scale Cryogenics Experiments
- Sensitivity Characterisation of a Parametric Transducer for Gravitational Wave Detection Through Optical Spring Effect