Quantum Enhanced Interferometer for Kilohertz Gravitational Wave Detection
arXiv:2007.03978
Abstract
The gravitational wave detector of higher sensitivity and greater bandwidth in kilohertz window is required for future gravitational wave astronomy and cosmology. Here we present a new type broadband high frequency laser interferometer gravitational wave detector utilizing polarization of light as signal carrier. Except for Fabry-Perot cavity arms we introduce dual power recycling to further amplify the gravitational wave signals. A novel method of weak measurement amplification is used to amplify signals for detection and to guarantee the long-term run of detector. Equipped with squeezed light, the proposed detector is shown sensitive enough within the window from 300Hz to several kHz, making it suitable for the study of high frequency gravitational wave sources. With the proposed detector added in the current detection network, we show that the ability of exploring binary neutron stars merger physics be significantly improved. The detector presented here is expected to provide an alternative way of exploring the possible ground-based gravitational wave detector for the need of future research.
arXiv commentManuscript improved and one author is added for the contribution of astronomy applications section
References in corpus (35)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- The X-ray counterpart to the gravitational wave event GW 170817
- Direct Measurement of the Quantum Wavefunction
- Colloquium: Understanding Quantum Weak Values: Basics and Applications
- Conversion of conventional gravitational-wave interferometers into QND interferometers by modifying their input and/or output optics
- A Radio Counterpart to a Neutron Star Merger
- Observation of squeezed light with 10dB quantum noise reduction
- Identifying a first-order phase transition in neutron star mergers through gravitational waves
- Measuring small longitudinal phase shifts: weak measurements or standard interferometry?
- Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
- Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
- Measuring the neutron star equation of state with gravitational wave observations
- Measuring neutron-star properties via gravitational waves from binary mergers
- Quantum Enhancement of the Zero-Area Sagnac Interferometer Topology for Gravitational Wave Detection
- Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
- Gravitational waves from neutron stars: Promises and challenges
- Towards Gravitational Wave Signals from Realistic Core Collapse Supernova Models
- The gravitational wave signal from core-collapse supernovae
- Dynamics and Gravitational Wave Signature of Collapsar Formation
- Gravitational Waves from Gravitational Collapse
- Observing and measuring the neutron-star equation-of-state in spinning binary neutron star systems
- Axion Dark Matter Search with Interferometric Gravitational Wave Detectors
- Enhancing the bandwidth of gravitational-wave detectors with unstable optomechanical filters
- Gravitational wave detectors with broadband high frequency sensitivity
- First measurements of high frequency cross-spectra from a pair of large Michelson interferometers
- First all-sky search for continuous gravitational-wave signals from unknown neutron stars in binary systems using Advanced LIGO data
- Realistic polarizing Sagnac topology with DC readout for the Einstein Telescope
- Gravitational-wave astronomy: the high-frequency window
- Effect of squeezing on parameter estimation of gravitational waves emitted by compact binary systems
- Weak value amplification and beyond the standard quantum limit in position measurements
- Gravitational Wave Detection via Weak Measurements Amplification